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Konstantin Batygin: Planet 9 and the Edge of Our Solar System | Lex Fridman Podcast #201 — Transcript

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  1. 0:00the following is a conversation with
  2. 0:01constantine bategan
  3. 0:03planetary astrophysicist at caltech
  4. 0:06interested in
  5. 0:07among other things the search for the
  6. 0:10distant the mysterious
  7. 0:11planet nine in the outer regions of our
  8. 0:14solar system quick mention of our
  9. 0:16sponsors
  10. 0:17squarespace literati on it and
  11. 0:20and i check them out in the description
  12. 0:22to support this podcast
  13. 0:24as a side note let me say that our
  14. 0:26little sun is orbited by
  15. 0:28not just a few planets in the planetary
  16. 0:30region but trillions of
  17. 0:32objects in the kuiper belt and the oort
  18. 0:35cloud that extends over three
  19. 0:37light years out this to me is amazing
  20. 0:40since proxima centauri
  21. 0:42the closest star to our sun is only 4.2
  22. 0:45light years away
  23. 0:46and all of it is mostly covered in
  24. 0:48darkness
  25. 0:50when i get a chance to go out swimming
  26. 0:51in the ocean far from the shore
  27. 0:53i'm sometimes overcome by the terrifying
  28. 0:56and the exciting feeling of not knowing
  29. 0:58what's there
  30. 0:59in the deep darkness that's how i feel
  31. 1:02about the edge of our solar system
  32. 1:04one day i hope humans will travel there
  33. 1:06or at the very least
  34. 1:08ai systems that carry the flame of human
  35. 1:10consciousness
  36. 1:12this is the lex friedman podcast and
  37. 1:14here's my conversation
  38. 1:15with constantine bategan
  39. 1:18what is planet nine planet nine
  40. 1:21is an object that we believe
  41. 1:25lives in the solar system beyond the
  42. 1:27orbit of neptune it orbits the sun
  43. 1:29with a period of about 10 000 years
  44. 1:33and uh is about five earth masses
  45. 1:36so that's a hypothesized object there's
  46. 1:38some evidence
  47. 1:40uh for this kind of object there's a
  48. 1:41bunch of different explanations
  49. 1:43can you give like an overview of the
  50. 1:46planets in our solar system how many are
  51. 1:49there
  52. 1:49what do we know and not know about them
  53. 1:52at a high level
  54. 1:53all right that sounds like a good plan
  55. 1:55so look the solar system
  56. 1:57basically is comprised of two parts the
  57. 2:00inner and the outer solar system
  58. 2:02the inner solar system has the planets
  59. 2:05mercury venus
  60. 2:06earth and mars now mercury is about
  61. 2:0940 percent of the orbital separation
  62. 2:13of where the earth is is closer to the
  63. 2:15sun venus
  64. 2:16about 70 percent uh then mars is about
  65. 2:21160 further away from the sun than is
  66. 2:25the earth
  67. 2:27these planets that we uh one of them
  68. 2:30we occupy right are pretty small okay
  69. 2:33they're
  70. 2:34too leading order sort of heavily
  71. 2:36overgrown asteroids
  72. 2:38if you will um and this is
  73. 2:41this becomes evident when you move out
  74. 2:44further
  75. 2:45in the solar system and encounter
  76. 2:46jupiter which is 316
  77. 2:48earth masses right 10 times the size
  78. 2:53you know and saturn is another huge one
  79. 2:5690 earth masses at about 10 times
  80. 2:59uh the separation from the sun this is
  81. 3:02the earth and then you have uranus and
  82. 3:03neptune
  83. 3:04at 20 and 30 respectively for a long
  84. 3:08time
  85. 3:09that is where the kind of massive
  86. 3:12part of the solar system ended
  87. 3:15but what we've learned in the last 30
  88. 3:17years
  89. 3:18is that beyond neptune there's this
  90. 3:21expansive field of icy debris a second
  91. 3:25icy asteroid belt in the solar system a
  92. 3:27lot of people have
  93. 3:28heard of the asteroid belt which lives
  94. 3:31be between
  95. 3:32mars and jupiter right like that's a
  96. 3:35pretty common thing that people like to
  97. 3:37imagine and draw on lunch boxes and
  98. 3:40stuff but beyond neptune
  99. 3:41there's a much more massive much more
  100. 3:44radially
  101. 3:45expansive field of debris pluto by the
  102. 3:49way
  103. 3:49it belongs to that second
  104. 3:52you know icy asteroid belt which we call
  105. 3:54the kuiper belt it's just a big
  106. 3:56object within that population of bodies
  107. 3:59oh pluto
  108. 4:00the planet pluto the the dwarf planet
  109. 4:03the former planet
  110. 4:04you know why is pluto not a planet
  111. 4:06anymore
  112. 4:07i mean it's tiny were you used to size
  113. 4:10matters when it comes to planets
  114. 4:11100 100 it's a actually a fascinating
  115. 4:15story
  116. 4:15when pluto was discovered in 1930
  117. 4:19the the reason it was discovered in the
  118. 4:21first place because astronomers at the
  119. 4:23time were looking for a seven earth mass
  120. 4:25planet
  121. 4:27somewhere beyond neptune it was
  122. 4:29hypothesized that such an object exists
  123. 4:31when they found something they
  124. 4:34interpreted that
  125. 4:35as a seven earth mass planet and
  126. 4:37immediately revised its mass downward
  127. 4:40because they couldn't resolve the object
  128. 4:42with the telescope so it looked like a
  129. 4:43just a point mass you know
  130. 4:45star rather than a physical disk they
  131. 4:48said well maybe it's not seven maybe
  132. 4:49it's one
  133. 4:50right and then so over the next um you
  134. 4:53know i guess 40 years
  135. 4:54pluto's mass kept getting revised down
  136. 4:57downwards downwards downwards until
  137. 5:00uh it was realized that's like 500 times
  138. 5:03less massive than the earth i mean like
  139. 5:06pluto's
  140. 5:07surface area is almost perfectly equal
  141. 5:11to the surface area of russia actually
  142. 5:14and you know russia is big but it's not
  143. 5:15a planet
  144. 5:17well i mean actually we can we can touch
  145. 5:19more on that that's that's another
  146. 5:21discussion
  147. 5:22uh so in some sense earlier in the
  148. 5:25century pluto represented
  149. 5:27kind of our ignorance about the edges of
  150. 5:29the solar system
  151. 5:31and perhaps planet nine is the thing
  152. 5:33that represents our ignorance
  153. 5:35about now the modern set of ignorances
  154. 5:39about the edges of our solar system
  155. 5:41that's a good way to put it by the way
  156. 5:42just
  157. 5:43imagining this belt of astero of debris
  158. 5:46at the edge of our solar system is
  159. 5:48incredible
  160. 5:50can you talk about it a little bit what
  161. 5:51is the kuiper belt and
  162. 5:53what it what is the oort cloud yeah
  163. 5:56okay so look the simple way to think
  164. 5:59about it is that if you imagine
  165. 6:01you know neptune's orbit like a circle
  166. 6:04right
  167. 6:05kind of uh maybe a factor of one and a
  168. 6:08half 1.3
  169. 6:10uh times bigger uh on a radius of
  170. 6:141.3 times bigger you've got a whole
  171. 6:16collection of icy objects most of these
  172. 6:19objects
  173. 6:20are sort of the size of austin you know
  174. 6:23maybe maybe a little bit smaller if you
  175. 6:26then
  176. 6:27zoom out right and
  177. 6:31explore the orbits of the most long
  178. 6:34period kuiper belt object these are the
  179. 6:36things that have the
  180. 6:37biggest orbits and take the longest time
  181. 6:40to go around the sun
  182. 6:43then what you find is that beyond a
  183. 6:45critical
  184. 6:47orbit size beyond a critical orbit
  185. 6:48period which is about 4 000 years
  186. 6:51you start to see weird structure like
  187. 6:54all the orbits
  188. 6:55sort of point into one direction and
  189. 6:59all the orbits are kind of tilted in the
  190. 7:01same
  191. 7:02way by about 20 degrees with respect to
  192. 7:05sun this is particularly pronounced
  193. 7:07in orbits that are not heavily affected
  194. 7:09by neptune
  195. 7:10so there you start to see this weird
  196. 7:12dichotomy where there are
  197. 7:14objects which are stable which are which
  198. 7:17neptune
  199. 7:18does not mess with gravitationally and
  200. 7:21unstable objects the unstable objects
  201. 7:23are basically all over the place
  202. 7:24because they're being you know kicked
  203. 7:26around by neptune the stable
  204. 7:29orbits show this remarkable pattern of
  205. 7:31clustering
  206. 7:33we back i guess five years ago
  207. 7:36interpreted this pattern of clustering
  208. 7:38as a gravitational one-way sign the
  209. 7:41existence of
  210. 7:42a planet in a distant planet right
  211. 7:45something that is shepherding and
  212. 7:46confining
  213. 7:48these orbits together of course
  214. 7:51right you have to have some skepticism
  215. 7:54when you're
  216. 7:54when you're talking about these things
  217. 7:56you have to ask the question of okay how
  218. 7:58statistically significant
  219. 8:00is this clustering and there are many
  220. 8:02authors that
  221. 8:03have indeed called that into question we
  222. 8:06have done
  223. 8:07our own analyses and basically just like
  224. 8:10with all statistics where
  225. 8:11you know there's kind of like you know
  226. 8:13multiple ways
  227. 8:15to uh do the exercise
  228. 8:18you can either ask the question if i
  229. 8:21have a telescope
  230. 8:22that has you know surveyed this part of
  231. 8:25the sky
  232. 8:26what are the chances that i would
  233. 8:27discover this clustering
  234. 8:30that basically tells you that you have
  235. 8:32zero confidence
  236. 8:34right like that's not that does not give
  237. 8:36you
  238. 8:37a confident answer one way or another
  239. 8:39another way to do the statistics which
  240. 8:41is what we
  241. 8:42prefer to do is to take to say we have a
  242. 8:45whole
  243. 8:46night sky of discoveries in the kuiper
  244. 8:49belt
  245. 8:50right and if we have some object over
  246. 8:53there
  247. 8:54which has right tension and declination
  248. 8:56which is a way to say it's
  249. 8:57there on the sky and it has some
  250. 9:00brightness
  251. 9:00that means somebody looked over there
  252. 9:02and discovered an object
  253. 9:04of was able to discover an object of
  254. 9:06that brightness or
  255. 9:08brighter through that analysis you can
  256. 9:10construct a whole map
  257. 9:12on the sky of kind of where all of the
  258. 9:14surveys that have ever been done
  259. 9:16have collectively looked so if you do
  260. 9:18the exercise this way
  261. 9:20the false alarm probability of
  262. 9:24the clustering on which the planet nine
  263. 9:26hypothesis is built is about 0.4
  264. 9:29wow okay so there's a million questions
  265. 9:31here one when you say bright objects
  266. 9:34why are they bright are we talking about
  267. 9:36actual objects within the kuiper belt or
  268. 9:37the stuff we see through the kupper belt
  269. 9:39this is the actual stuff we see in the
  270. 9:41kuiper belt the way
  271. 9:43you go about discovering kuiper belt
  272. 9:44objects pretty easy
  273. 9:46i mean it's easy in theory right hard in
  274. 9:49practice
  275. 9:50yeah all you do is you take snapshots of
  276. 9:53the sky
  277. 9:54right choose that direction say and take
  278. 9:56you know
  279. 9:57the high exposure snapshot then you wait
  280. 9:59a night
  281. 10:00and you do it again and then you wait
  282. 10:02another night and you do it again
  283. 10:04objects that are just random stars in
  284. 10:06the galaxy don't move
  285. 10:08on the sky whereas objects in the solar
  286. 10:10system will slowly move
  287. 10:11this is no different than if you're
  288. 10:14driving down the freeway
  289. 10:15it looks like you know trees are going
  290. 10:18by you faster than the clouds right this
  291. 10:19is parallax
  292. 10:21that's it it's just they're reflecting
  293. 10:23light off
  294. 10:24of the sun and it's going back and
  295. 10:26hitting this there's a little bit of a
  296. 10:28glimmer
  297. 10:28from the different objects that you can
  298. 10:30see based on the reflection from the sun
  299. 10:32so like
  300. 10:33there's actual light yeah it's not
  301. 10:35darkness that's right these are just
  302. 10:37big icicles basically that are just
  303. 10:39reflecting sunlight back at you
  304. 10:41it's then easy to understand why it's so
  305. 10:44hard to discover them because
  306. 10:46light has to travel to you know
  307. 10:48something like 40 times the distance
  308. 10:51um between the earth and the sun and
  309. 10:54then get reflected back was it like an
  310. 10:56hour
  311. 10:56travel or yeah that's right that's
  312. 10:58something like that because the
  313. 11:00the earth to the sun is eight minutes i
  314. 11:02believe um
  315. 11:03and so something you know yeah yeah in
  316. 11:06that
  317. 11:06in that order magnitude so that's
  318. 11:08interesting so you have to
  319. 11:10like account for all of that and then
  320. 11:12there's this huge amount of
  321. 11:14data pixels that are coming from the
  322. 11:16pictures
  323. 11:18and you have to uh integrate all that
  324. 11:20together
  325. 11:21to paint a sort of like a high estimate
  326. 11:24of the different objects
  327. 11:25can you track them can you be like
  328. 11:27that's bob like can you like
  329. 11:28yes exactly in fact uh one of them is
  330. 11:32is named joe biden i mean i'm not like
  331. 11:35this is not even a joke
  332. 11:36right is there a trump one or no no no
  333. 11:39no
  334. 11:39i don't know i haven't checked for for
  335. 11:41for that but
  336. 11:43uh like the way it works is if you
  337. 11:46discover one
  338. 11:47you right away get a license plate for
  339. 11:49it okay
  340. 11:50so like the first four numbers is the
  341. 11:53first
  342. 11:53year that this object has appeared on
  343. 11:56you know
  344. 11:57in the data set if you will and then um
  345. 12:01there's like this code that follows it
  346. 12:04which basically tells you where in the
  347. 12:06sky it is
  348. 12:07right so one of the really interesting
  349. 12:10kuiper belt objects which is very much
  350. 12:12part of the planet 9 story is called
  351. 12:15vp113
  352. 12:16because joe biden was vice president at
  353. 12:19the time
  354. 12:20you know got nicknamed biden
  355. 12:23vp113 said yeah you got nickname button
  356. 12:27beautiful
  357. 12:28what's the fingerprint for any
  358. 12:31particular
  359. 12:32object like how do you know it's the
  360. 12:33same one okay just kind of like
  361. 12:35yeah from night to night you take a
  362. 12:37picture how do you know it's the same
  363. 12:38object
  364. 12:39yeah so the way you know is it appears
  365. 12:41in almost exactly the same part of the
  366. 12:44sky except for the move but it moves but
  367. 12:46this is why actually you need at least
  368. 12:48three nights
  369. 12:49because oftentimes asteroids
  370. 12:53which are much closer to the earth like
  371. 12:55will um
  372. 12:57appear to move only
  373. 13:00slightly but then on the third night
  374. 13:02will move away so that third knight
  375. 13:04is really there to detect acceleration
  376. 13:07now
  377. 13:08the the thing that i didn't really
  378. 13:10realize until
  379. 13:12you know i started observing together
  380. 13:15with my partner in crime and all this
  381. 13:16mike brown
  382. 13:17is just the fact that for the first year
  383. 13:21when you make these detections
  384. 13:23the only thing you really know is
  385. 13:25confidence is where it is on the night
  386. 13:27sky
  387. 13:27and how far away it is okay that's it
  388. 13:30you don't know anything about the orbit
  389. 13:32because over three days the object just
  390. 13:36moves so little right the that whole
  391. 13:38motion on the sky is entirely coming
  392. 13:41from
  393. 13:41motion of the earth right so the earth
  394. 13:43is kind of the car
  395. 13:44the object is the tree and you see it
  396. 13:46moving so then
  397. 13:48to get some confident information about
  398. 13:51what its orbit looks like you have to
  399. 13:52come back
  400. 13:53a year later um and then measure it
  401. 13:56again
  402. 13:56interesting to do three nights then come
  403. 13:58back a year later and do another three
  404. 14:00nights
  405. 14:01so you get the velocity the acceleration
  406. 14:02from the three nights and then you have
  407. 14:04the
  408. 14:05maybe the additional the additional
  409. 14:07formation
  410. 14:08because an orbit is basically described
  411. 14:10by six parameters
  412. 14:11so you at least need six independent
  413. 14:13points but in reality you need
  414. 14:15many more observations to to really
  415. 14:18pin down the orbit well and from that
  416. 14:20you're able to construct for that one
  417. 14:22particular object in orbit and then
  418. 14:24there's
  419. 14:24of course like how many objects are
  420. 14:27there
  421. 14:27there's like four-ish thousand now
  422. 14:31but like the
  423. 14:34in the future that could be like
  424. 14:36millions
  425. 14:37oh sure oh sure so in fact these things
  426. 14:40are hard to predict but there's a
  427. 14:41new observatory called the vera rubin
  428. 14:44observatory which is coming online
  429. 14:47maybe next year i mean with covet these
  430. 14:49things are
  431. 14:50a little bit more uncertain but they've
  432. 14:52actually been making great progress
  433. 14:54uh with construction and so that
  434. 14:58uh telescope is gonna sort of scan the
  435. 15:01night sky
  436. 15:02uh every day automatically and it's just
  437. 15:05it's such an efficient survey that it
  438. 15:07might uh increase the census
  439. 15:10of the distant kuiper belt the things
  440. 15:12that i'm interested in
  441. 15:14by a factor of 100 i mean that would be
  442. 15:16that would be really cool
  443. 15:17and yeah that's a that's an incredible
  444. 15:20uh
  445. 15:21maybe i mean they might just find planet
  446. 15:25nine
  447. 15:26i mean that's like almost like literally
  448. 15:28pictures like visually
  449. 15:29i mean sure yeah like the first
  450. 15:31detection you make all you know is where
  451. 15:33it is in the sky and how far away it is
  452. 15:35if something is you know 500 times away
  453. 15:38from the sun
  454. 15:38as far away from the sun as is the earth
  455. 15:40you know that's planet nine that's when
  456. 15:42the story concludes
  457. 15:44and then you can study it right now you
  458. 15:46can study yeah by the way
  459. 15:47i'm going to use that as like i don't
  460. 15:49know a pickup line or a dating strategy
  461. 15:51like see the person for three days and
  462. 15:54then don't see them at all and then see
  463. 15:55them again in
  464. 15:56in a year to determine the orbit and
  465. 15:59over time
  466. 16:00you figure out if sort of uh
  467. 16:03from a cosmic perspective this this
  468. 16:05whole thing
  469. 16:07i have no dating advice to give i was
  470. 16:09good i was going to use this as a
  471. 16:11metaphor to uh to somehow
  472. 16:13uh map it on to the human condition okay
  473. 16:16you mentioned the kuiper belt what's the
  474. 16:17oor cloud
  475. 16:18if you look at the neptune orbit as uh
  476. 16:22one then the kuiper bell is like 1.3 out
  477. 16:25there
  478. 16:25and then we get farther and farther into
  479. 16:27the darkness what
  480. 16:28so okay you've got the kind of main
  481. 16:30kuiper belt was about
  482. 16:32say 1.3 1.5
  483. 16:35um then you have something called the
  484. 16:37scattered disc
  485. 16:39which is kind of an extension of the
  486. 16:40kuiper belt it's a bunch of these
  487. 16:42long very elliptical orbits that hug
  488. 16:47the orbit of neptune but come out very
  489. 16:49far so
  490. 16:50that the scattered disc
  491. 16:53with the current senses like the some of
  492. 16:56the
  493. 16:56longest orbits we know of
  494. 17:00um have a
  495. 17:03semi-major axis so half the orbit length
  496. 17:06roughly speaking of about a thousand
  497. 17:08thousand times the distance between the
  498. 17:10earth and the sun
  499. 17:11wow now if you keep moving out okay
  500. 17:15eventually once you're sort of you know
  501. 17:18ten thousand to a hundred thousand
  502. 17:21roughly that's where the oort cloud is
  503. 17:23now the oort cloud is a distinct
  504. 17:26population of
  505. 17:27icy bodies and it's distinct from the
  506. 17:29kuiper belt it's in fact it's so
  507. 17:31expansive
  508. 17:32that it ends roughly halfway between
  509. 17:36us and the next star um it's it's edge
  510. 17:39is just
  511. 17:40dictated by to what extent does the
  512. 17:43solar gravity reach
  513. 17:45solar gravity reaches that far yeah so
  514. 17:47it has to
  515. 17:49wow yeah so in fact
  516. 17:52imagining this is a little bit
  517. 17:53overwhelming so there's like a giant
  518. 17:57like vast
  519. 18:01icy rock thingy it's like a sphere
  520. 18:04it's like you know it's like it's an
  521. 18:05almost spherical structure
  522. 18:07that engulfs that encircles the sun
  523. 18:11and all the long period comets come
  524. 18:14from the oort cloud they come the way
  525. 18:17that they appear
  526. 18:18i mean for already i don't know hundreds
  527. 18:20of years
  528. 18:21we've been detecting occasionally like a
  529. 18:24comet will come in
  530. 18:26and it comes seemingly comes out of
  531. 18:28nowhere
  532. 18:29the reason these long period comets
  533. 18:31appear
  534. 18:32that very on very very long time scales
  535. 18:35right
  536. 18:36these oort cloud objects that are
  537. 18:37sitting you know 30
  538. 18:39000 times as far away from the sun as is
  539. 18:42the earth
  540. 18:43actually interact with the gravity of
  541. 18:44the galaxy the tide
  542. 18:46effectively the tide that the galaxy
  543. 18:49exerts upon them and their orbits slowly
  544. 18:51change and they elongate
  545. 18:53to the point where once they their
  546. 18:56closest approach to the sun starts to
  547. 18:59reach
  548. 19:00a critical distance where ice starts to
  549. 19:02sublimate
  550. 19:03then we discover them as comets because
  551. 19:06then the ice comes off of them
  552. 19:08they look beautiful on the night sky etc
  553. 19:10but they're all coming from
  554. 19:12you know really really far away so is
  555. 19:15there
  556. 19:15are any of them coming our way from
  557. 19:18collisions like how many collisions are
  558. 19:20there
  559. 19:20or is there a bunch of space for them to
  560. 19:22move around yeah there's zero it's
  561. 19:24completely collisionless
  562. 19:25out there the physical radii of objects
  563. 19:29are so small compared to the distance
  564. 19:31between them
  565. 19:32right it's just it is truly a
  566. 19:35collisionless
  567. 19:36uh environment i don't know there i
  568. 19:39think that probably in the age
  569. 19:42of the solar system there have literally
  570. 19:45been zero collisions in the word cloud
  571. 19:48wow when you like draw a picture of the
  572. 19:50solar
  573. 19:51system everything's really close
  574. 19:53together so that everything i guess here
  575. 19:55is
  576. 19:56spaced far apart do rogue planets
  577. 19:59like flying every once in a while and
  578. 20:00join not rogue planets but rogue objects
  579. 20:02from
  580. 20:03out there oh sure oh sure yeah join the
  581. 20:05party
  582. 20:06yeah absolutely uh we've seen a couple
  583. 20:08of them um
  584. 20:09in the last three or f or so years uh
  585. 20:12maybe four years now
  586. 20:13uh one the first one uh was
  587. 20:17the one called it's been
  588. 20:20all over the news the second one was
  589. 20:23comet borisov
  590. 20:25discovered by a guy named borisov
  591. 20:30yeah so the way you know they're coming
  592. 20:32from elsewhere is
  593. 20:33unlike solar system objects which travel
  594. 20:36on elliptical paths
  595. 20:37around the sun these guys travel on
  596. 20:40hyperbolic paths
  597. 20:41so they come in say hello and then
  598. 20:44they're gone
  599. 20:44and the fact that they exist
  600. 20:49is totally like not surprising
  601. 20:52right the neptune is con constantly
  602. 20:55ejecting
  603. 20:56kuiper belt objects into interstellar
  604. 20:59space our solar system itself
  605. 21:01is sort of leaking icy debris and
  606. 21:04injecting it so
  607. 21:06presumably every you know planetary
  608. 21:08systems around other stars do exactly
  609. 21:10the same thing
  610. 21:11let me ask you about the the millions of
  611. 21:14objects that are
  612. 21:15part of the kuiper belt and the part of
  613. 21:17the ore cloud do you think some of them
  614. 21:18have
  615. 21:19primitive life it kind of makes you sad
  616. 21:22if there's like primitive life there and
  617. 21:24they're just kind of like lonely out
  618. 21:25there in space
  619. 21:26like how many of them do you think have
  620. 21:28life like bacterial life probably a
  621. 21:30negligible amount
  622. 21:31zero you know like zero was like a plus
  623. 21:34on top
  624. 21:35uh right yeah
  625. 21:38um if so you know if you and i
  626. 21:42took a little trip to the interstellar
  627. 21:44medium i think we would develop cancer
  628. 21:47and die uh real fast right that's rough
  629. 21:50yeah it's a pretty hostile radiation
  630. 21:53environment
  631. 21:54you don't actually have to go to the
  632. 21:55interstellar medium you just have to
  633. 21:57leave the earth's magnetic field too
  634. 22:00and then you're not doing so well
  635. 22:02suddenly
  636. 22:03so you know this this idea of
  637. 22:07you know life kind of traveling between
  638. 22:10places it's not
  639. 22:12it's not entirely implausible but you
  640. 22:14you really have to
  641. 22:16twist i think a lot of parameters one of
  642. 22:18the problems we have is we don't
  643. 22:20actually know how life originates
  644. 22:22right so it's kind of a second order
  645. 22:25question of survival in the interstellar
  646. 22:28medium and how resilient it is because
  647. 22:31we we think you require
  648. 22:34water but and that's certainly the case
  649. 22:37for the earth but you know we uh
  650. 22:41we really don't know for sure that said
  651. 22:44i will argue that the question of like
  652. 22:46are there aliens out there
  653. 22:48is a very boring question because
  654. 22:51the answer is of course there are right
  655. 22:53i mean like
  656. 22:55we know that there are planets around
  657. 22:58almost every star um
  658. 23:02of course there of course there are
  659. 23:04other life forms life is not some
  660. 23:06specific thing that happened on the
  661. 23:09earth and that's it
  662. 23:10right just that's a statistical
  663. 23:12impossibility yeah um
  664. 23:14yeah but the the difficult question is
  665. 23:16before even
  666. 23:17the fact that we don't know how life
  667. 23:19originates i don't think we even know
  668. 23:21what life
  669. 23:22is like definitionally yeah like
  670. 23:24formalizing a kind of picture
  671. 23:26of in terms of the mechanism we would
  672. 23:29use
  673. 23:29to to search for life out there or even
  674. 23:32when we're on a planet
  675. 23:33to say is this life is this rock that
  676. 23:37just moved
  677. 23:38from where it was yesterday life or or
  678. 23:41maybe not even
  679. 23:41rock something else i got to tell you i
  680. 23:44want to know what life
  681. 23:45is okay and i want you to show me
  682. 23:50uh i think there's a song to basically
  683. 23:53accompany every single
  684. 23:55thing we talk about today and probably
  685. 23:57uh half of them are love songs
  686. 23:59um and somehow we'll integrate george
  687. 24:01michael into the whole thing okay
  688. 24:02so your intuition is there's life
  689. 24:04everywhere in our universe
  690. 24:07do you think there's intelligent life
  691. 24:09out there i think it's entirely
  692. 24:11plausible
  693. 24:11i mean i it's entirely plausible um
  694. 24:16i think i think there's intelligent life
  695. 24:18on earth
  696. 24:19um and so yeah taking that like say
  697. 24:23whatever this thing we got on earth
  698. 24:25whether it's dolphins or humans
  699. 24:27say that's intelligent definitely
  700. 24:29dolphins
  701. 24:30i mean have you seen the dolphins
  702. 24:34well they do some cruel stuff to each
  703. 24:36other so if cruelty
  704. 24:39is uh is the definition of intelligence
  705. 24:41that they're pretty good yeah and then
  706. 24:42humans are pretty good on that
  707. 24:44regard then there's like uh uh pigs
  708. 24:47are very intelligent i got actually a
  709. 24:49chance to hang out with pigs recently
  710. 24:51and they're um aside from the fact
  711. 24:54they're trying to
  712. 24:55eat me they're very uh
  713. 24:58they're very they love food they love
  714. 25:00food but there's an intelligence to
  715. 25:02their eyes that was kind of
  716. 25:03uh like haunts me because i also
  717. 25:06love to eat meat and then to to me the
  718. 25:09thing
  719. 25:10i later ate and i was very intelligent
  720. 25:14and uh almost charismatic with the way
  721. 25:16it was expressing its uh
  722. 25:17himself herself itself was uh was quite
  723. 25:20incredible
  724. 25:21so and all that to say is if we have
  725. 25:25intelligent life here on earth if we
  726. 25:26take dolphins pigs
  727. 25:28humans from the perspective of like
  728. 25:30planetary science
  729. 25:31how unique is earth okay so earth is not
  730. 25:35a com
  731. 25:35common outcome of the planet formation
  732. 25:38process
  733. 25:40um it's probably a
  734. 25:44something on the order of maybe a one
  735. 25:46percent effect
  736. 25:48and by earth i mean it's not just an
  737. 25:50earth mass planet
  738. 25:52okay i mean the architecture of the
  739. 25:55solar system
  740. 25:56that allows the earth to exist in in its
  741. 26:00kind of
  742. 26:00very temperate um
  743. 26:04way one thing to understand
  744. 26:07uh and this is this is pretty crucial uh
  745. 26:10right it's that the
  746. 26:11earth itself formed well after
  747. 26:14the gas disk that formed
  748. 26:18the giant planets
  749. 26:21had already dissipated you see stars
  750. 26:24start out
  751. 26:25with you know the star and then a disc
  752. 26:27of gas and dust that encircles it
  753. 26:29okay from this disk of gas and dust
  754. 26:33big planets can emerge and we have
  755. 26:37over the last uh you know two three
  756. 26:39decades discovered
  757. 26:41thousands of extra solar planets as an
  758. 26:43orbit of other studs
  759. 26:44what we see is that uh many of them
  760. 26:48are you know have these expansive
  761. 26:50hydrogen helium
  762. 26:51atmospheres the fact that the earth
  763. 26:55doesn't is deeply connected to the fact
  764. 26:58that
  765. 26:59earth took about 100 million years to
  766. 27:00form so we missed that
  767. 27:03you know train so to speak to get that
  768. 27:05hydrogen helium atmosphere
  769. 27:07that's why actually we can see the sky
  770. 27:10right that's why the
  771. 27:11sky is uh well at least in most places
  772. 27:14that's why the
  773. 27:15the atmosphere is not completely opaque
  774. 27:18um
  775. 27:20with that you know kind of thinking in
  776. 27:22mind i
  777. 27:24i would argue that we're getting the
  778. 27:26kind of emergent pictures that the earth
  779. 27:28is
  780. 27:28is not you know everywhere
  781. 27:32right we there's sort of the sci-fi view
  782. 27:34of things where we go to some other star
  783. 27:36and we just land on random planets and
  784. 27:38they're all earth-like that's totally
  785. 27:40not true
  786. 27:41but the even a low probability
  787. 27:45event even if you imagine that earth is
  788. 27:47a one in a million
  789. 27:49or one in a you know one in 10 million
  790. 27:52occurrence there are 10 to the 12 stars
  791. 27:56in the galaxy
  792. 27:58right so you just you always win by
  793. 28:01by large numbers that's right by supply
  794. 28:03they save you well
  795. 28:04you've hypothesized that our our solar
  796. 28:06system once possessed a
  797. 28:08population of short-period planets that
  798. 28:10were destroyed by the evil jupiter
  799. 28:13uh migrating through the the solar
  800. 28:17nebula can you explain
  801. 28:18if i was to say what was the kind of the
  802. 28:20key outcome of searches for extrasolar
  803. 28:22planets
  804. 28:24it is that most stars are encircled by
  805. 28:27short period planets
  806. 28:28that are you know a few earth masses
  807. 28:32right so a few times bigger than the
  808. 28:34earth um
  809. 28:35and have orbital periods that kind of
  810. 28:38range from days to
  811. 28:39to weeks now if you go in
  812. 28:43and ask the solar system what's in our
  813. 28:46region
  814. 28:47right in that region it's completely
  815. 28:49empty right
  816. 28:50it's just it's astonishingly hollow
  817. 28:53and thank you from
  818. 28:57the sun is not some you know special
  819. 28:58star that decided that it was going to
  820. 29:01form
  821. 29:02the the solar system so i think you know
  822. 29:04the natural thing to assume
  823. 29:06is is that the same processes of planet
  824. 29:09formation that occurred
  825. 29:10everywhere else also occurred in the
  826. 29:12solar system
  827. 29:14following this logic it's not
  828. 29:16implausible to imagine that the solar
  829. 29:18system once possessed
  830. 29:20a system of intra mercurian
  831. 29:24like you know compact system of
  832. 29:27of planets so then we asked ourselves
  833. 29:30would
  834. 29:30such a system survive to this day and
  835. 29:33the answer is no
  836. 29:34uh at least our calculations um suggest
  837. 29:37it's highly unlikely because of the
  838. 29:40formation of jupiter
  839. 29:41and jupiter's primordial kind of
  840. 29:43wandering through the solar system
  841. 29:44would have sent this collisional field
  842. 29:47of debris that would have pushed
  843. 29:49that system of planets onto the sun so
  844. 29:51was jupiter
  845. 29:52this primordial wandering what did what
  846. 29:55did jupiter look like
  847. 29:56like why was it wandering it didn't have
  848. 29:58the orbit it has today
  849. 30:00uh we're pretty certain that giant
  850. 30:02planets like jupiter when they form they
  851. 30:03migrate
  852. 30:04the reason they migrate is you know on a
  853. 30:08detailed level perhaps
  854. 30:09difficult to explain but you know if
  855. 30:12just in a qualitative sense
  856. 30:14they form in this fluid disk
  857. 30:18of gas and dust so it's kind of like if
  858. 30:21i
  859. 30:21plop down a raft somewhere in the ocean
  860. 30:24will it stay in where you plop it down
  861. 30:27or will it
  862. 30:28kind of get carried around it's not
  863. 30:30really a good analogy because it's not
  864. 30:32like jupiter is being
  865. 30:34affected by the currents of you know gas
  866. 30:36and dust but the way
  867. 30:38it migrates is it carves out a hole
  868. 30:41in the in the disk and then uh through
  869. 30:44by interacting with the disk
  870. 30:46gravitationally right it can change its
  871. 30:48orbit the fact that the solar system has
  872. 30:51both jupiter and saturn
  873. 30:53here complicates things a lot right
  874. 30:55because it's you have to
  875. 30:57solve the problem of the evolution of
  876. 31:00the gas disk the evolution of jupiter's
  877. 31:02orbit in the gas disk plus
  878. 31:04evolution of saturn's and their mutual
  879. 31:06interaction
  880. 31:08the common outcome of solving
  881. 31:12that problem though is pretty easy to
  882. 31:14explain
  883. 31:15jupiter forms its orbit shrinks and then
  884. 31:18once saturn forms
  885. 31:20its orbit catches up basically to the
  886. 31:22orbit of jupiter and then both come out
  887. 31:24so there's this inward outward pattern
  888. 31:26of jupiter's
  889. 31:28early motion that happens sort of within
  890. 31:29the firm within the last million years
  891. 31:32of the lifetime of the solar system's
  892. 31:35primordial disk
  893. 31:36so do while this is happening
  894. 31:40if our calculations are correct which i
  895. 31:42think they are
  896. 31:43you can destroy these in this inner
  897. 31:47system of
  898. 31:48you know few earth mass planets
  899. 31:51and then in the aftermath of all this
  900. 31:54violence
  901. 31:55you form the terrestrial planets where
  902. 31:58would they come from in that case so
  903. 32:00so jupiter clears out the space and then
  904. 32:03there's a a few terrestrial planets that
  905. 32:05come in and those coming from
  906. 32:07the from the disk somewhere like one of
  907. 32:10the larger
  908. 32:11yeah what actually happens in these
  909. 32:13calculations is you leave behind
  910. 32:15a rather mass depleted like
  911. 32:19remnant remnant disk only a couple earth
  912. 32:22masses
  913. 32:23so then from that
  914. 32:26remnant population annulus of material
  915. 32:30over 100 or about 100 million years by
  916. 32:32just collisions
  917. 32:34you grow the earth and the moon and
  918. 32:36everything else you said amulous
  919. 32:38annulus and yours annulus yeah that's a
  920. 32:40beautiful word what does that mean
  921. 32:42well it's like it's like a disc that's
  922. 32:43kind of thin it's like a
  923. 32:45yeah it's something that is you know a
  924. 32:48disc that's so thin it's almost
  925. 32:50flirting with being a ring like
  926. 32:54i was gonna say this reminds me lord of
  927. 32:55the rings so like this the word just
  928. 32:57feels like it belongs in a toll canal
  929. 32:59okay uh
  930. 33:00so that that's incredible and so that in
  931. 33:03your senses you said like one percent
  932. 33:05that's a rare
  933. 33:06the way jupiter and saturn danced and
  934. 33:10cleared out and you know cleared out the
  935. 33:13the the short period debris and then
  936. 33:17changed the gravitational landscape
  937. 33:18that's a pretty rare thing too
  938. 33:20it's rare and moreover like you don't
  939. 33:22have to go to our calculations you can
  940. 33:24just
  941. 33:25ask the night sky how many stars
  942. 33:28have jupiter and saturn analogs the
  943. 33:31answer is
  944. 33:32jupiter and saturn analogs are found
  945. 33:33around only 10
  946. 33:35of sun-mic stars so they are they
  947. 33:37themselves like you kind of have to
  948. 33:38score an a minus or better
  949. 33:40on the test to you know on the planet
  950. 33:42formation test to become
  951. 33:44a solar system analog even in that basic
  952. 33:47sense
  953. 33:48and moreover um you know low lower mass
  954. 33:51stars
  955. 33:52which are uh very numerous in the galaxy
  956. 33:56so-called m dwarfs think like zero
  957. 33:59percent
  958. 33:59of them well maybe like a negligible
  959. 34:02fraction of them have giant planets
  960. 34:04giant planets are a rare
  961. 34:08you know outcome of planet formation one
  962. 34:11of the
  963. 34:11really big problems that remain
  964. 34:13unanswered is why we don't actually
  965. 34:15understand
  966. 34:16why they're so rare how hard is it to
  967. 34:19simulate
  968. 34:20all of the things that we've been
  969. 34:21talking about each of the things we've
  970. 34:22been talking about
  971. 34:23and maybe one day all of the things
  972. 34:26we've been talking about and beyond
  973. 34:28meaning like from the initial
  974. 34:31primordial solar system you know a bunch
  975. 34:35of disks with
  976. 34:36i don't know billions trillions of
  977. 34:38objects in them
  978. 34:39like simulate that such that you
  979. 34:42eventually get a jupiter
  980. 34:44and a saturn then eventually you get the
  981. 34:46jupiter and the saturn they clear out a
  982. 34:48disc change the gravitational landscape
  983. 34:49then earth pops up
  984. 34:50like that whole thing and then be able
  985. 34:53to do that
  986. 34:54for every other system
  987. 34:57in the uh every other star in the galaxy
  988. 35:00and then
  989. 35:01be able to do that for other galaxies as
  990. 35:03well
  991. 35:05um yeah so look maybe start from the
  992. 35:07smallest simulation
  993. 35:09like what is actually being done today i
  994. 35:11mean even the smallest simulation is
  995. 35:12probably super super difficult
  996. 35:14even just like one object in the kuiper
  997. 35:16belt is probably super difficult to
  998. 35:17simulate
  999. 35:18i mean i think it's super easy i mean
  1000. 35:20like it's
  1001. 35:21it's just not that hard um but um
  1002. 35:25you know let's let's ask the most kind
  1003. 35:27of
  1004. 35:28basic problem okay so the problem of
  1005. 35:31having a star
  1006. 35:32and something in orbit of it that you
  1007. 35:35don't need a simulation for like
  1008. 35:36you can just write that down on a piece
  1009. 35:38of paper this gravity
  1010. 35:40would like yeah i guess i guess it's
  1011. 35:42important to try to
  1012. 35:44uh you know one way to simulate objects
  1013. 35:47in our solar system is to build the
  1014. 35:49universe from scratch okay
  1015. 35:51we'll get to building the universe from
  1016. 35:52scratch in a sec um but let me just kind
  1017. 35:54of go through the hierarchy of
  1018. 35:56what you know what we do two objects two
  1019. 35:59objects
  1020. 36:00analytically solvable like we can figure
  1021. 36:03it out
  1022. 36:03very easily if you just you don't i
  1023. 36:05don't think you yeah you don't need to
  1024. 36:07know calculus
  1025. 36:08uh it helps to know calculus but you
  1026. 36:10don't necessarily need to know calculus
  1027. 36:12um three objects that are
  1028. 36:14gravitationally
  1029. 36:15interacting the solution is chaotic
  1030. 36:18doesn't matter
  1031. 36:19how many simulations you do you the
  1032. 36:22answer loses meaning after
  1033. 36:23um after some time i feel like that is a
  1034. 36:26metaphor for dating as well but go on
  1035. 36:30now look yes yeah so so
  1036. 36:33the fact that you go from analytically
  1037. 36:36solvable
  1038. 36:37to unpredictable you know when you are
  1039. 36:40when your simulation goes from two up
  1040. 36:42bodies to three bodies
  1041. 36:44should immediately tell you that the
  1042. 36:47exercise
  1043. 36:48of trying to engineer a calculation
  1044. 36:51where you form this whole
  1045. 36:52entire solar system from scratch and
  1046. 36:55hope to have some predictive answer
  1047. 36:57is is a futile one right we will never
  1048. 37:02uh succeed at such a simulation just to
  1049. 37:04clarify you mean like explicitly having
  1050. 37:06a clear equation that generalizes
  1051. 37:09the the whole process enough to be able
  1052. 37:11to make a prediction what do you mean
  1053. 37:12actually like literally simulating the
  1054. 37:15objects as a hopeless pursuit
  1055. 37:16once it increases beyond three the
  1056. 37:18simulating them is not a hopeless
  1057. 37:20pursuit but the
  1058. 37:21outcome becomes a statistical one
  1059. 37:26and what's actually quite interesting is
  1060. 37:27i think we have
  1061. 37:29all the equations uh figured out
  1062. 37:32right like you know in order to really
  1063. 37:35understand this
  1064. 37:36the formation of the the solar system it
  1065. 37:38suffices to know
  1066. 37:40gravity and magneto hydrodynamics i mean
  1067. 37:44like
  1068. 37:44the combination of uh maxwell's
  1069. 37:46equations and
  1070. 37:47you know navier-stokes equations for the
  1071. 37:49fluids you need to know quantum
  1072. 37:51mechanics to understand
  1073. 37:53opacities and and so on but we have
  1074. 37:57those equations in hand it's not that we
  1075. 37:59don't
  1076. 38:00have that understanding it's that
  1077. 38:01putting it all together
  1078. 38:04is a very very difficult and b if you
  1079. 38:07were to run
  1080. 38:08the same evolution twice
  1081. 38:11changing you know the initial conditions
  1082. 38:14by
  1083. 38:15some infinitesimal amounts i'm you know
  1084. 38:18minor change in your calculation to
  1085. 38:20start with you would get the or you'd
  1086. 38:21get a different answer
  1087. 38:23this is one this is part of the reason
  1088. 38:26why planetary systems are so diverse you
  1089. 38:29don't
  1090. 38:30have like a you know very predictive
  1091. 38:32path
  1092. 38:33for you start with a disk of this mass
  1093. 38:36and
  1094. 38:37it's around this star therefore you're
  1095. 38:39going to form the solar system
  1096. 38:41right you start with this and therefore
  1097. 38:43you will conform this huge
  1098. 38:45outcome a huge set of outcomes and some
  1099. 38:47percentage of it
  1100. 38:49will resemble the solar system you
  1101. 38:50mentioned quantum mechanics and
  1102. 38:52we're talking about cosmic scale
  1103. 38:56objects you've talked about that the
  1104. 38:58evolution of astrophysical disks can be
  1105. 39:01modeled with
  1106. 39:01uh schroedinger's equation i sure did
  1107. 39:06why it's like how does quantum mechanics
  1108. 39:09uh become relevant at when you
  1109. 39:12consider the evolution of objects in the
  1110. 39:14solar system yeah
  1111. 39:16well let me take a take a step back and
  1112. 39:18just say like i remember
  1113. 39:19being you know utterly confused
  1114. 39:23by quantum mechanics when i first
  1115. 39:25learned it and
  1116. 39:27the schrodinger equation which is kind
  1117. 39:29of the parent equation
  1118. 39:30of of that whole field you know seems to
  1119. 39:33come out of nowhere
  1120. 39:34right the way that the way that i was
  1121. 39:37sort of explaining it i remember asking
  1122. 39:40you know my professor is like but where
  1123. 39:41does it come from is that like well just
  1124. 39:43just like don't worry about it and just
  1125. 39:46like calculate the
  1126. 39:47hydrogen you know energy levels right so
  1127. 39:50it's like i could do all the problems i
  1128. 39:52just did not have any intuition for
  1129. 39:55for where this parent you know super
  1130. 39:57important equation came from
  1131. 39:59now down the line i was remember i was
  1132. 40:01preparing for my own
  1133. 40:03lecture and i was trying to understand
  1134. 40:05how waves
  1135. 40:07travel in self-gravitating discs so
  1136. 40:11you know again there's a very broad
  1137. 40:15theory that's already developed but i
  1138. 40:16was looking for some simpler
  1139. 40:18way to explain it really for the
  1140. 40:20purposes of teaching class
  1141. 40:22and so i i thought okay what if i just
  1142. 40:25imagine a disc as an infinite uh
  1143. 40:29number of concentric circles right that
  1144. 40:31interact with
  1145. 40:32the with each other gravitationally
  1146. 40:36that's a problem in some sense that um
  1147. 40:39i can solve using methods from like the
  1148. 40:42late 1700s right so i can write down
  1149. 40:46hamiltonian well i can write down the
  1150. 40:48energy function basically of their
  1151. 40:49their interactions and what i
  1152. 40:54found is that when you take the
  1153. 40:56continuum limit when you
  1154. 40:58go from discrete circles that are
  1155. 41:00talking to each other gravitationally to
  1156. 41:02a
  1157. 41:02continuum disk suddenly
  1158. 41:06this gravitational interaction among
  1159. 41:08them
  1160. 41:09right the the governing equation becomes
  1161. 41:12the schrodinger equation
  1162. 41:13and i had to think about that for a
  1163. 41:15little bit did you just unify
  1164. 41:17quantum mechanics and gravity no this is
  1165. 41:20not the same thing as like
  1166. 41:22you know fusing relativity and quantum
  1167. 41:24mechanics
  1168. 41:25but it did uh it did get me thinking a
  1169. 41:28little bit
  1170. 41:29so the fact that waves in astrophysical
  1171. 41:32disks
  1172. 41:33behave just like wave functions of
  1173. 41:37of particles kind of like an interesting
  1174. 41:39analogy because for me it's easier to
  1175. 41:41imagine waves traveling through you know
  1176. 41:45astrophysical disks or really just
  1177. 41:46sheets of paper and
  1178. 41:48the reason this is that analogy exists
  1179. 41:52is because there's actually nothing
  1180. 41:54quantum about the schrodinger equation
  1181. 41:57the schrodinger equation
  1182. 41:58is just a wave equation
  1183. 42:01and all of the interpretation that comes
  1184. 42:04from it
  1185. 42:05is quantum but the equation itself
  1186. 42:08is not a quantum being so you can use it
  1187. 42:11to model
  1188. 42:12waves it's way it's not turtles it's
  1189. 42:15waves all the way down
  1190. 42:16you can pick which level you pick the
  1191. 42:18wave at and so it could be at the solar
  1192. 42:20system level that you can use right
  1193. 42:21and also it actually provides a pretty
  1194. 42:24neat calculational tool
  1195. 42:25because um it's it's difficult so we
  1196. 42:29just talked about simulations but it's
  1197. 42:30difficult to simulate
  1198. 42:32the behavior of astrophysical disks on
  1199. 42:35time scales
  1200. 42:36that are in between a few orbits
  1201. 42:40and their entire evolution so it's
  1202. 42:43over a time scale of a few orbits you
  1203. 42:45have you do a hydrodynamic you know
  1204. 42:47simulation
  1205. 42:48right you do that basically that's
  1206. 42:52something that you can do
  1207. 42:53on a modern computer on a time scale of
  1208. 42:55say a week
  1209. 42:56when it comes to their evolution over
  1210. 42:58their entire lifetime you don't hope to
  1211. 43:00resolve the orbits you just kind of
  1212. 43:02hope to understand how the system
  1213. 43:03behaves in between
  1214. 43:06right you to get access to that as it
  1215. 43:08turns out it's pretty
  1216. 43:09um it's pretty cute you can use uh you
  1217. 43:12can use the schrodinger equation to get
  1218. 43:14the answer
  1219. 43:15rapidly so it's a calculational tool
  1220. 43:17that's fascinating by the way the
  1221. 43:18astrophysical disks how what are they
  1222. 43:22how broad is this definition okay so
  1223. 43:24astrophysical disks span
  1224. 43:27a huge uh huge amount of ranges
  1225. 43:31they start maybe at the smallest scale
  1226. 43:33they start with actually kuiper belt
  1227. 43:35objects some kuiper belt objects have
  1228. 43:37rings
  1229. 43:38so that's maybe the smallest example of
  1230. 43:40an astrophysical disc
  1231. 43:42we've got this little potato shaped
  1232. 43:44asteroid
  1233. 43:45you know which is you know sort of the
  1234. 43:47size of la or something and around it
  1235. 43:50is are some rings of icy matter that
  1236. 43:54object is a small astrophysical disk
  1237. 43:56then you have
  1238. 43:57saturn the rings of saturn you have the
  1239. 44:00next set of scale you have the solar
  1240. 44:02system itself when it was forming you
  1241. 44:03have
  1242. 44:04this then you have black hole discs
  1243. 44:07you have galaxies discs are super common
  1244. 44:10in the universe
  1245. 44:12and the reason is that stuff rotates
  1246. 44:15right i mean gravity works yeah so uh
  1247. 44:17and those rings could be the material
  1248. 44:20that uh composes those rings could be
  1249. 44:24it could be gas it could be solid it
  1250. 44:26could be anything that's right so
  1251. 44:29the disc that made from which the
  1252. 44:32planets emerged was predominantly
  1253. 44:34hydrogen helium gas on the other hand
  1254. 44:36the rings of saturn
  1255. 44:38are made up of you know icicles ice
  1256. 44:41little like
  1257. 44:42ice cubes this big about a centimeter
  1258. 44:45across
  1259. 44:46that sounds refreshing so that's
  1260. 44:48incredible hydrogen helium gas
  1261. 44:50so in the beginning it was just hydrogen
  1262. 44:53and helium
  1263. 44:54around the sun how does that lead to the
  1264. 44:57first formations of solid
  1265. 44:58objects in terms of simulation okay
  1266. 45:02here's the story um so you're like have
  1267. 45:05you ever been to the desert
  1268. 45:07yes i've been to the death valley and
  1269. 45:09actually it was uh terrifying just as
  1270. 45:11total tangent i'm distracting you but i
  1271. 45:13was uh
  1272. 45:14driving through it and i was really
  1273. 45:16surprised because it was at first
  1274. 45:18hot and then as it was getting into the
  1275. 45:21evening there's this huge thunderstorm
  1276. 45:23like
  1277. 45:23it was raining and it got freezing cold
  1278. 45:25like what the hell is
  1279. 45:26it was the apocalypse yeah i had to like
  1280. 45:29just sit there
  1281. 45:30listening to bruce springsteen i
  1282. 45:31remember and just thinking i'm probably
  1283. 45:33going to die
  1284. 45:34and i was okay with it because bruce
  1285. 45:36springsteen was on the radio look
  1286. 45:38when you've got the boss you know you're
  1287. 45:40ready you're ready to meet the ball
  1288. 45:42yeah so look i mean it's a good line
  1289. 45:45so i'm sorry that's true um
  1290. 45:48yeah by the way like to continue on this
  1291. 45:50tangent i
  1292. 45:51i absolutely love the southwest for this
  1293. 45:54reason just um you know i know during
  1294. 45:57the pandemic i
  1295. 45:58drove from la to new mexico a bunch of
  1296. 46:01times
  1297. 46:02the madness the weather yeah the the the
  1298. 46:05chaos of
  1299. 46:06weather the fact that you know it'll be
  1300. 46:07blazing hot one minute and then it's
  1301. 46:09just like
  1302. 46:10we'll decide to have a little
  1303. 46:12thunderstorm maybe you'll decide
  1304. 46:14to go back momentarily to like a
  1305. 46:16thousand degrees and then go back to the
  1306. 46:17thunderstorm
  1307. 46:18it's amazing it's it's that by the way
  1308. 46:21is chaos theory in action yeah
  1309. 46:23right um but let's get back to talking
  1310. 46:25about the desert yeah
  1311. 46:27so in the desert um tumbleweeds
  1312. 46:30have a tendency to roll because the wind
  1313. 46:32rolls them
  1314. 46:33and if you're careful you'll
  1315. 46:35occasionally see this family of temple
  1316. 46:37weeds where like there's like a big one
  1317. 46:39and then there's a bunch of little ones
  1318. 46:41that that kind of hide in its
  1319. 46:43wake right and are all rolling together
  1320. 46:45and still almost looks like
  1321. 46:47you know a family of ducks crossing a
  1322. 46:49street or something
  1323. 46:50um or for example you know
  1324. 46:53if you watch tour de france right you've
  1325. 46:56got a whole bunch of cyclists and
  1326. 46:58they're like cycling
  1327. 46:59you know within 10 centimeters of each
  1328. 47:01other they're not
  1329. 47:02bffs right yeah but they're not yeah
  1330. 47:04trying to be
  1331. 47:05trying to write together they are
  1332. 47:07writing together to minimize the
  1333. 47:09collective
  1334. 47:10uh you know air resistance if you will
  1335. 47:13that uh
  1336. 47:14that they experience turns out solids in
  1337. 47:17the protoplanetary disk do
  1338. 47:19just this there's an instability
  1339. 47:23wherein solid particles right things
  1340. 47:26that are
  1341. 47:27a centimeter across will start to hide
  1342. 47:30behind one another and form these clouds
  1343. 47:33why because cumulatively that minimizes
  1344. 47:37the solid
  1345. 47:38component of the disk aerodynamic
  1346. 47:41interaction with the gas
  1347. 47:43now these clouds because they're kind of
  1348. 47:45a favorable
  1349. 47:47energetic condition for the dust to live
  1350. 47:50in
  1351. 47:50they grow grow grow grow grow until they
  1352. 47:53become so massive that they collapse
  1353. 47:54under their own weight
  1354. 47:56that's how the first building blocks of
  1355. 47:58planets form that's how the
  1356. 48:00big asteroids got there that's
  1357. 48:02incredible yeah so that
  1358. 48:04is that simulatable or is it not useful
  1359. 48:06to simulate no no that's simulatable
  1360. 48:08um and people do these types of
  1361. 48:10calculations
  1362. 48:11it's it's really cool that's actually
  1363. 48:14that's
  1364. 48:14one of the many fields of planet
  1365. 48:16formation theory that is really really
  1366. 48:18active
  1367. 48:19right now people are trying to
  1368. 48:20understand all kinds of aspects of that
  1369. 48:23process because of course
  1370. 48:24i've explained it you know like as if
  1371. 48:26there's one
  1372. 48:28thing that happens turns out it's a
  1373. 48:31it's a beautifully rich dynamic but the
  1374. 48:34but qualitatively formation of the first
  1375. 48:37building blocks
  1376. 48:38actually follows the same sequence as
  1377. 48:40formation of stars
  1378. 48:41right stars are just clouds of gas
  1379. 48:45hydrogen helium gas that sit in space
  1380. 48:49and slowly cool and at some point they
  1381. 48:53you know contract to a point where their
  1382. 48:56gravity overtakes the thermal
  1383. 48:58you know pressure support if you will
  1384. 49:00and they collapse under their own weight
  1385. 49:01and you get a little baby solar system
  1386. 49:03that's amazing so do you think one day
  1387. 49:05it will be possible to
  1388. 49:07simulate the full history
  1389. 49:10that took our solar system to what it is
  1390. 49:13today
  1391. 49:15yes and it will be useless okay
  1392. 49:18so you don't think your story many of
  1393. 49:20the ideas that you have about jupiter
  1394. 49:22clear in the space
  1395. 49:23like retelling that story in high
  1396. 49:25resolution is not that important
  1397. 49:26i actually think it's important but at
  1398. 49:28every stage
  1399. 49:30you have to you have to simul you have
  1400. 49:33to
  1401. 49:34design your experiments your your
  1402. 49:36numerical computer experiments so that
  1403. 49:39they test some specific aspect of that
  1404. 49:42evolution
  1405. 49:43um i am not a proponent of doing
  1406. 49:46huge simulations because um
  1407. 49:50even if we forget the information theory
  1408. 49:53aspect of not being able to simulate in
  1409. 49:57full detail
  1410. 49:58the universe because if you do then
  1411. 50:02you you have made an actual universe
  1412. 50:05it's not
  1413. 50:05the simulation right by simulation is in
  1414. 50:08some sense a compression
  1415. 50:09of information so therefore you must
  1416. 50:11lose detail
  1417. 50:13but that point aside if we are
  1418. 50:16able to simulate
  1419. 50:19the entire history of the solar system
  1420. 50:22in excruciating detail
  1421. 50:24i mean it'll be cool but it's not going
  1422. 50:26to be
  1423. 50:27any different from observing it
  1424. 50:31right because theoretical understanding
  1425. 50:34which is what
  1426. 50:35ultimately i'm interested in um
  1427. 50:38comes from taking complex things and
  1428. 50:41reducing them down to something
  1429. 50:43that you know some mechanism that you
  1430. 50:45can actually quantify
  1431. 50:47um that's the that's the fun part of
  1432. 50:50astrophysics
  1433. 50:51just kind of simulating things in
  1434. 50:52extreme detail
  1435. 50:54is we'll cool we'll make cool
  1436. 50:56visualizations but that doesn't get to
  1437. 50:58doesn't doesn't get you to any better
  1438. 51:01understanding than you had
  1439. 51:03before you did the simulation if you ask
  1440. 51:05very specific questions then you'll be
  1441. 51:06able to uh
  1442. 51:08create like very highly compressed
  1443. 51:12nice beautiful theories about how things
  1444. 51:14evolved and then you can use those to
  1445. 51:15then generalize to other solar systems
  1446. 51:18to other stars and other galaxies and
  1447. 51:21say something generalizable about the
  1448. 51:23entire universe
  1449. 51:24how difficult would it be to simulate
  1450. 51:28our solar system such that we would not
  1451. 51:30know the difference
  1452. 51:31meaning if we are living in a simulation
  1453. 51:35is there a nice think of it as a video
  1454. 51:38game
  1455. 51:38sure is there a nice compressible way of
  1456. 51:40doing that or
  1457. 51:42just kind of like you intuited with a
  1458. 51:43three body situation
  1459. 51:46is just a giant mess that you cannot
  1460. 51:48create a video game
  1461. 51:50that uh will seem realistic without
  1462. 51:53actually
  1463. 51:54building it so i'm you know i'm
  1464. 51:57speculating but
  1465. 51:58one of the yeah i know i know like
  1466. 52:01you have a deep understanding of this
  1467. 52:03but like for me
  1468. 52:05i'm just gonna like speculate that for
  1469. 52:08um at least in the types of simulations
  1470. 52:11that we can do
  1471. 52:12today inevitably you run into the
  1472. 52:15problem of resolution
  1473. 52:17right you're doesn't matter what you're
  1474. 52:19doing it is discrete
  1475. 52:21now um the way you would go
  1476. 52:24about asking you know if what we're
  1477. 52:26observing is that a simulation or
  1478. 52:28uh or is that you know some real
  1479. 52:31continuous
  1480. 52:32thing uh is you you zoom in right you
  1481. 52:35zoom in and try and find
  1482. 52:37the you know the grid scale if you will
  1483. 52:41um yeah i mean
  1484. 52:46it's a it's a really interesting it's a
  1485. 52:48really interesting question
  1486. 52:49and because the
  1487. 52:52solar system itself and really you know
  1488. 52:55the double pendulum is chaotic
  1489. 52:58right pendulum sitting on another
  1490. 53:00pendulum
  1491. 53:03moves unpredictably once you let them go
  1492. 53:05um
  1493. 53:06you really don't need to like inject any
  1494. 53:09randomness into a simulation for it to
  1495. 53:12to give you stochastic and unpredictable
  1496. 53:14answers
  1497. 53:15weather is a great example of this
  1498. 53:18weather has a happen of time
  1499. 53:20of you know typical weather systems have
  1500. 53:22a happen of time of a few days
  1501. 53:24and there's a fundamental reason why the
  1502. 53:27force
  1503. 53:28forecast always sucks you know two weeks
  1504. 53:30in advance
  1505. 53:31it's not that we don't know the
  1506. 53:34equations that govern
  1507. 53:37the atmosphere we know them well their
  1508. 53:39solutions are meaningless though after a
  1509. 53:41few days
  1510. 53:42the zooming in thing is very interesting
  1511. 53:45i
  1512. 53:45i think about this a lot whether
  1513. 53:48there'll be a time
  1514. 53:49soon where we would want to stay in
  1515. 53:51video game worlds
  1516. 53:53whether it's virtual reality or just
  1517. 53:54playing video games i mean i think that
  1518. 53:56time
  1519. 53:57like came in like the 90s and it's been
  1520. 54:00that time well it's not just it's not
  1521. 54:02just games i mean
  1522. 54:03it's accelerated i just recently saw
  1523. 54:06that
  1524. 54:07wow and fortnite were played 140 billion
  1525. 54:10hours
  1526. 54:11and those are just video games yeah and
  1527. 54:13that's like increasing very very quickly
  1528. 54:15especially with the people
  1529. 54:16coming up now and being born now and
  1530. 54:18become you know becoming teenagers
  1531. 54:20and so on let's have a thought
  1532. 54:22experiment where it's just you and a
  1533. 54:23video game character inside a room
  1534. 54:26where you remove the simulation they
  1535. 54:28need to simulate sort of
  1536. 54:31a lot of objects if it's just you and
  1537. 54:33that character
  1538. 54:36how far do you need to simulate in terms
  1539. 54:38of zooming in
  1540. 54:39for it to be very real to you as real as
  1541. 54:42reality
  1542. 54:43so like first of all you kind of
  1543. 54:45mentioned zooming in which is
  1544. 54:47fascinating because
  1545. 54:48we have these tools of science that
  1546. 54:50allow us to zoom in
  1547. 54:51quote unquote in all kinds of ways
  1548. 54:55uh in the world around us but our
  1549. 54:57cognitive abilities like our perception
  1550. 54:59system as humans
  1551. 55:00is very limited in terms of situations
  1552. 55:02so we might be very easily fooled
  1553. 55:04some of the video games like on the ps4
  1554. 55:08yeah like look pretty real to me yeah
  1555. 55:11right uh i think
  1556. 55:13you would really have to interrogate i
  1557. 55:15mean i think even with what we have
  1558. 55:16today
  1559. 55:17like uh i don't know ace combat seven
  1560. 55:20that's a great example
  1561. 55:22right like i mean the way that the
  1562. 55:24clouds are rendered
  1563. 55:25uh it's i mean it
  1564. 55:28looks just like when you're flying you
  1565. 55:30know on a real airplane the
  1566. 55:32the kind of transparency i think that
  1567. 55:35the
  1568. 55:35you know our perception is limited
  1569. 55:38enough already
  1570. 55:40to not be able to tell some of the uh
  1571. 55:44you know some of the differences there's
  1572. 55:46a game called uh
  1573. 55:47skyrim it's an elder scrolls role
  1574. 55:50playing game
  1575. 55:51and i just uh i played it for quite a
  1576. 55:54bit
  1577. 55:55and i think i played very different than
  1578. 55:58others like
  1579. 55:58there'll be long searches of time where
  1580. 56:00i would just walk around and look at
  1581. 56:02nature
  1582. 56:03in the game it's incredible oh sure it's
  1583. 56:06just like the graphics is like
  1584. 56:08wow i want to stay there it was better i
  1585. 56:10went hiking recently
  1586. 56:12it was like as good as hiking so look i
  1587. 56:15know what you mean
  1588. 56:16not to go on a huge video game you know
  1589. 56:18tangent but like
  1590. 56:19the the third like witcher game was
  1591. 56:23astonishingly beautiful right especially
  1592. 56:25like playing on
  1593. 56:26on a good hardware machine it's like
  1594. 56:29this is pretty
  1595. 56:31this is pretty legit that said um
  1596. 56:36you know i i don't resonate with the i
  1597. 56:38want to stay
  1598. 56:39here you know like one of the things
  1599. 56:40that i love to do
  1600. 56:43is to go to my like boxing gym
  1601. 56:46and and box with a guy right like that's
  1602. 56:49there's
  1603. 56:50there's nothing quite like that physical
  1604. 56:52you know
  1605. 56:53experience like that's fascinating that
  1606. 56:55might be
  1607. 56:56simply an artifact of the year you were
  1608. 56:59born maybe because if you're born today
  1609. 57:02it almost seems like stupid to go to a
  1610. 57:04gym yeah
  1611. 57:05like you're going to a gym to box with a
  1612. 57:07guy why not box with mike tyson when you
  1613. 57:09yourself was like in his prime when you
  1614. 57:12yourself are also an incredible boxer
  1615. 57:14in the video game world for me there
  1616. 57:17there's a multitude of reasons why i
  1617. 57:19don't want to box with mike tyson
  1618. 57:21right like no no no no you enjoy teeth
  1619. 57:24and i want to have an ear no but your
  1620. 57:26your skills
  1621. 57:27in this meat space in this physical
  1622. 57:29realm is very limited
  1623. 57:31and takes a lot of work and you're
  1624. 57:33you're uh you're a musician
  1625. 57:35uh your incredible scientist you only
  1626. 57:38have so much time in the in the day
  1627. 57:40but in the video game world you can
  1628. 57:42expand your capabilities in all kinds of
  1629. 57:44dimensions
  1630. 57:45that you can never have possibly have
  1631. 57:47time in the physical world
  1632. 57:48and so that it doesn't make sense like
  1633. 57:50to
  1634. 57:51to be existing to be working your ass
  1635. 57:54off in the physical world
  1636. 57:56when you can just be super successful uh
  1637. 57:59uh in the video game world but i still
  1638. 58:02you enjoy sucking and stuff
  1639. 58:04yeah i i really struggling to get better
  1640. 58:06i sure do
  1641. 58:07i mean i think like these days with
  1642. 58:09music music
  1643. 58:10is a great example right we just started
  1644. 58:13you know
  1645. 58:14practicing live uh with my band again
  1646. 58:17you know after
  1647. 58:18not playing for a year and uh you know
  1648. 58:21it's just it was terrible
  1649. 58:22right which is just kind of a lot of the
  1650. 58:25nuance
  1651. 58:25you know a lot of the detail is just
  1652. 58:27that detail that takes you know
  1653. 58:29years of collective practice to develop
  1654. 58:32uh
  1655. 58:32it's just lost but it was just an
  1656. 58:36incredible amount of fun
  1657. 58:37way more fun than all the like studio
  1658. 58:40you know sitting around and playing uh
  1659. 58:42that i did you know throughout the
  1660. 58:44entire year
  1661. 58:45so i think there's something there's
  1662. 58:47something intangible
  1663. 58:48or maybe maybe tangible about being uh
  1664. 58:51being in person
  1665. 58:53i i sure hope you're wrong and that
  1666. 58:56you know we that's not something that
  1667. 58:58will get lost because i think there's
  1668. 59:00like such a large part of the human
  1669. 59:02condition
  1670. 59:03is to hang out if we were doing this
  1671. 59:07interview on zoom right
  1672. 59:10i mean i'd already be i'd already be
  1673. 59:14bored out of my mind
  1674. 59:14[Laughter]
  1675. 59:16exactly i mean there's something to that
  1676. 59:18i mean i'm almost playing devil's
  1677. 59:19advocate but at the same time
  1678. 59:21you know i'm sure people talk about the
  1679. 59:23same way at the beginning of the 20th
  1680. 59:24century about horses
  1681. 59:26where they're they are much more
  1682. 59:28efficient
  1683. 59:30they're much uh easier to maintain than
  1684. 59:33cars
  1685. 59:34it doesn't make sense to have you know
  1686. 59:35all the ways that cars break down and
  1687. 59:37there's not enough infrastructure in
  1688. 59:38terms of roads for cars
  1689. 59:40it doesn't make any sense like horses
  1690. 59:42and like nature you could do the nature
  1691. 59:44like where
  1692. 59:45you know you should be living more
  1693. 59:46natural life those are real you don't
  1694. 59:48want machines in your life they're going
  1695. 59:49to pollute your mind
  1696. 59:50and the minds of young people but then
  1697. 59:52eventually just cars took over so
  1698. 59:54in that same way it just seems uh going
  1699. 59:56back to horses
  1700. 59:59just you know well you can be you can
  1701. 1:00:01play uh
  1702. 1:00:02uh uh what is it red dead
  1703. 1:00:05red dead redemption redemption and uh
  1704. 1:00:07you can ride horses in the video game
  1705. 1:00:09more
  1706. 1:00:09so let me return us back to planet nine
  1707. 1:00:12uh-huh always a good place to come back
  1708. 1:00:15to so now that we did a big
  1709. 1:00:17historical overview of our solar system
  1710. 1:00:19what is planet nine
  1711. 1:00:21okay planet nine is a hypothetical
  1712. 1:00:25object that orbits the solar system
  1713. 1:00:27right at
  1714. 1:00:28an orbital period of about 10 000 years
  1715. 1:00:32and an orbit which is slightly tilted
  1716. 1:00:36with respect to the plane of the solar
  1717. 1:00:37system
  1718. 1:00:38slightly eccentric and the object itself
  1719. 1:00:41we think is five times more massive than
  1720. 1:00:45the earth we have never seen planet nine
  1721. 1:00:48in a telescope but we have gravitational
  1722. 1:00:52evidence for it
  1723. 1:00:53and so this is where all the stuff we've
  1724. 1:00:55been talking about this clustering ideas
  1725. 1:00:57maybe you can speak to the approximate
  1726. 1:00:59location that we
  1727. 1:01:01suspect and also the question i wanted
  1728. 1:01:03to ask is uh
  1729. 1:01:05what are we supposed to be imagining
  1730. 1:01:06here because he said there's certain
  1731. 1:01:08objects in the kuiper belt that
  1732. 1:01:10are kind of have a direction to them
  1733. 1:01:12that they're all
  1734. 1:01:13like like flocking in some kind of way
  1735. 1:01:16so that's the sense that there's some
  1736. 1:01:17kind of gravitational object
  1737. 1:01:19not changing their orbit but kind of
  1738. 1:01:21confining them
  1739. 1:01:22right yeah finding like grouping their
  1740. 1:01:24orbits together
  1741. 1:01:26see what would happen if planet nine
  1742. 1:01:27were not there is these orbits that
  1743. 1:01:30roughly share
  1744. 1:01:31a common orientation they would just
  1745. 1:01:34disperse right they would just become as
  1746. 1:01:37a mutually symmetric
  1747. 1:01:38point everywhere planet nine's gravity
  1748. 1:01:42makes it such that these objects stay
  1749. 1:01:45in a state that's that's basically
  1750. 1:01:47anti-aligned with respect to the orb
  1751. 1:01:50of planet nine um and
  1752. 1:01:53and sort of hang out there and kind of
  1753. 1:01:55oscillate on time scale of about a
  1754. 1:01:57billion years
  1755. 1:01:58that's one of the lines of evidence for
  1756. 1:02:01the existence of planet nine there are
  1757. 1:02:03others that's the one that's easiest to
  1758. 1:02:05maybe visualize just because it's fun to
  1759. 1:02:07think about orbits that all point
  1760. 1:02:09into the same direction but i should
  1761. 1:02:12you know emphasize that for example the
  1762. 1:02:15existence of
  1763. 1:02:16objects again kuiper belt objects that
  1764. 1:02:19are heavily out of the plane
  1765. 1:02:20of the solar system things that are
  1766. 1:02:22tilted by say 90 degrees that's not
  1767. 1:02:25we don't expect that as an outcome
  1768. 1:02:28of planet formation indeed planet
  1769. 1:02:30formation
  1770. 1:02:31simulations have never produced such
  1771. 1:02:34objects
  1772. 1:02:35without some extrinsic gravitational
  1773. 1:02:38force
  1774. 1:02:38planet nine on the other hand generates
  1775. 1:02:40them very readily so that
  1776. 1:02:42provides kind of an alternative you know
  1777. 1:02:46population of small bodies in the solar
  1778. 1:02:48system that also get produced by planet
  1779. 1:02:509 through an
  1780. 1:02:51independent kind of gravitational effect
  1781. 1:02:54so they're kind of
  1782. 1:02:54there's basically five different things
  1783. 1:02:58that the uh that planet nine does
  1784. 1:03:01individually that are like kind of
  1785. 1:03:04maybe a one sigma effect where you would
  1786. 1:03:07say yeah okay if that's all it was
  1787. 1:03:09maybe it's not no reason to jump up and
  1788. 1:03:10down but because
  1789. 1:03:12it's it's mult it's a multitude of these
  1790. 1:03:15puzzles
  1791. 1:03:16that all are explained by one hypothesis
  1792. 1:03:19that's that's really the the magnetism
  1793. 1:03:22the attraction of the planet nine model
  1794. 1:03:25so can you just clarify so
  1795. 1:03:28most orbit most planets in the solar
  1796. 1:03:31system orbit
  1797. 1:03:33and approximately the same so it's flat
  1798. 1:03:35yeah it's like
  1799. 1:03:36one degree they the difference between
  1800. 1:03:39them is
  1801. 1:03:40about one degree so but nevertheless if
  1802. 1:03:42we looked at our solar
  1803. 1:03:44system it would look and i could see
  1804. 1:03:46every single object it would look like a
  1805. 1:03:47sphere
  1806. 1:03:48the inner part where the planets are
  1807. 1:03:51would look
  1808. 1:03:52like you know flat right the the kuiper
  1809. 1:03:55belt
  1810. 1:03:56and the asteroid belt have a larger
  1811. 1:04:00um it gets fatter and fatter yeah that's
  1812. 1:04:02kind of like becomes a sphere
  1813. 1:04:03that's right and if you look at the very
  1814. 1:04:05outside it's polluted by this
  1815. 1:04:07you know quasi-spheroidal thing
  1816. 1:04:10nobody's of course ever seen the oort
  1817. 1:04:13cloud
  1818. 1:04:14right we've only seen comments that come
  1819. 1:04:17from the oort cloud so
  1820. 1:04:18the oort cloud which is this right
  1821. 1:04:21population of distant debris
  1822. 1:04:23its existence is also inferred you could
  1823. 1:04:26say
  1824. 1:04:26alternatively there is you know there's
  1825. 1:04:30a big
  1826. 1:04:30cosmic creature that occasionally you
  1827. 1:04:32know sitting at 20 000 au and
  1828. 1:04:34occasionally throws an icy
  1829. 1:04:36rock towards the sound like that
  1830. 1:04:38spaghetti monster i think it's called
  1831. 1:04:39okay
  1832. 1:04:40i mean so it's a mystery in many ways
  1833. 1:04:44but you can kind of infer a bunch of
  1834. 1:04:45things about it
  1835. 1:04:46it's by the way both terrifying and
  1836. 1:04:48exciting that there's this
  1837. 1:04:49vast darkness all around us that's full
  1838. 1:04:51of objects that are just
  1839. 1:04:53throwing just there yeah it's actually
  1840. 1:04:55kind of astonishing right
  1841. 1:04:57that we have only
  1842. 1:05:00explored a small fraction of the solar
  1843. 1:05:03system
  1844. 1:05:04right that that really kind of baffles
  1845. 1:05:07me because
  1846. 1:05:08uh remember as a student you know
  1847. 1:05:10studying physics
  1848. 1:05:11you know you do the problem where you
  1849. 1:05:13put the earth around the sun you solve
  1850. 1:05:15that and
  1851. 1:05:16like it's one line of math and you say
  1852. 1:05:19okay well that
  1853. 1:05:20surely was figured out by newton so like
  1854. 1:05:22all the interesting stuff
  1855. 1:05:24is not in the solar system but that um
  1856. 1:05:28it's just plainly not true there are
  1857. 1:05:31there are mysteries in the solar system
  1858. 1:05:34that
  1859. 1:05:34are remarkable that we are only now
  1860. 1:05:37starting to just kind of scratch the
  1861. 1:05:39surface of
  1862. 1:05:40and some of those objects probably have
  1863. 1:05:42some information about the history of
  1864. 1:05:43our solar system
  1865. 1:05:44absolutely absolutely like a great
  1866. 1:05:46example is
  1867. 1:05:47uh you know small meteorites right small
  1868. 1:05:50meteorites
  1869. 1:05:51are melted right they have they're
  1870. 1:05:53differentiated meaning some of the
  1871. 1:05:55uh iron sinks you say
  1872. 1:05:58how can that be because they're so small
  1873. 1:06:00that they wouldn't have melted just from
  1874. 1:06:02the heat of their accretion
  1875. 1:06:04turns out the fact that the solar nebula
  1876. 1:06:07the
  1877. 1:06:07the disk that made the planets was
  1878. 1:06:09polluted by
  1879. 1:06:10aluminum 26 is in itself a remarkable
  1880. 1:06:13thing it means
  1881. 1:06:14the solar system did not form an
  1882. 1:06:16isolation it formed
  1883. 1:06:18in a giant cloud of thousands of other
  1884. 1:06:21stars that were also forming
  1885. 1:06:23some of which were undergoing you know
  1886. 1:06:26going through supernova explosions some
  1887. 1:06:28of
  1888. 1:06:28and releasing these unstable isotopes
  1889. 1:06:33that of which we now see kind of the
  1890. 1:06:35traces of
  1891. 1:06:37it's so cool do you think it's possible
  1892. 1:06:39that life from
  1893. 1:06:41other solar systems was injected and
  1894. 1:06:43that that was
  1895. 1:06:44what was uh the origin of life on earth
  1896. 1:06:47yeah defense permea idea um
  1897. 1:06:50that's seen as a low probability event
  1898. 1:06:52by people who studied the original life
  1899. 1:06:54but that's because
  1900. 1:06:55uh then they would be out of a job well
  1901. 1:06:59i don't think they'd be out of the job
  1902. 1:07:00because you just then say you have to
  1903. 1:07:01figure out how life started
  1904. 1:07:03and there but then you have to go there
  1905. 1:07:05we can study
  1906. 1:07:06life on earth much easier we could study
  1907. 1:07:08in the lab
  1908. 1:07:09much easier because we could replicate
  1909. 1:07:11conditions that are
  1910. 1:07:12from an early earth much easier
  1911. 1:07:16from a chemistry perspective from a
  1912. 1:07:17biology perspective
  1913. 1:07:19you can intuit a bunch of stuff you can
  1914. 1:07:21look at different parts of earth and
  1915. 1:07:23just
  1916. 1:07:23to an extent i mean the early earth was
  1917. 1:07:26completely
  1918. 1:07:27unlike the current earth right there was
  1919. 1:07:28no oxygen so
  1920. 1:07:30uh one of my colleagues at caltech uh
  1921. 1:07:33joe kirchnick is
  1922. 1:07:36certain right something like
  1923. 1:07:40100 certainty that life started on mars
  1924. 1:07:43and came to earth uh in on martian media
  1925. 1:07:46rights
  1926. 1:07:47um this is not a problem
  1927. 1:07:50that i like to kind of
  1928. 1:07:53think about too much like the origin of
  1929. 1:07:55life it's a fascinating problem
  1930. 1:07:57but you know it's not physics and i just
  1931. 1:08:00like
  1932. 1:08:01i just don't don't love it it's the same
  1933. 1:08:04reason you don't love
  1934. 1:08:04i thought you're a musician so music is
  1935. 1:08:07not physics either so why are you
  1936. 1:08:09showing 100
  1937. 1:08:10physics
  1938. 1:08:10[Laughter]
  1939. 1:08:13okay no no look uh in all seriousness
  1940. 1:08:15though i
  1941. 1:08:16uh there are a few things that i really
  1942. 1:08:19really enjoy
  1943. 1:08:20i genuinely enjoy physics i genuinely
  1944. 1:08:23enjoy music
  1945. 1:08:24i genuinely you know enjoy martial arts
  1946. 1:08:28and
  1947. 1:08:28i genuinely enjoy uh my family i should
  1948. 1:08:31have said that all in a reverse order or
  1949. 1:08:33something
  1950. 1:08:34but i like to focus on these things and
  1951. 1:08:37not worry too much
  1952. 1:08:38about about everything else you know
  1953. 1:08:39what i mean yes just because there is a
  1954. 1:08:41like you said earlier there's a time
  1955. 1:08:44constraint you can't
  1956. 1:08:46do it all there's many mysteries all
  1957. 1:08:48around us
  1958. 1:08:49so um and they're all beautiful in in
  1959. 1:08:52different ways
  1960. 1:08:53to me that thing i love is artificial
  1961. 1:08:55intelligence that uh
  1962. 1:08:57perhaps i love it because eventually i'm
  1963. 1:08:59trying to suck up to our future
  1964. 1:09:00overlords
  1965. 1:09:01the the question of you said there's a
  1966. 1:09:05lot of kind of
  1967. 1:09:07little pieces of evidence for this thing
  1968. 1:09:09that's planet nine
  1969. 1:09:11if we were to try to collect more
  1970. 1:09:13evidence
  1971. 1:09:14or be certain like a paper that says
  1972. 1:09:18like you drop it clear we're done
  1973. 1:09:21what what is that required does that
  1974. 1:09:23require us sending probes out
  1975. 1:09:25or do you think we can do it from
  1976. 1:09:26telescopes here on earth what are the
  1977. 1:09:28different ideas for conclusive evidence
  1978. 1:09:30for planet nine
  1979. 1:09:31the moment planet nine gets imaged from
  1980. 1:09:35a telescope on earth it's done i mean
  1981. 1:09:36it's just there
  1982. 1:09:37can you clarify because you mentioned
  1983. 1:09:39that before from an
  1984. 1:09:40image would you be able to tell yes so
  1985. 1:09:43from
  1986. 1:09:44an image the moment you see
  1987. 1:09:48something something that is reflecting
  1988. 1:09:50sunlight
  1989. 1:09:51back at you and you know that it's
  1990. 1:09:55hundreds of times as far away from
  1991. 1:09:59the sun as as the earth you're done
  1992. 1:10:02so you're thinking so basically if you
  1993. 1:10:04have a really far away thing that's big
  1994. 1:10:06yeah you know five times the size of
  1995. 1:10:08earth that means
  1996. 1:10:11uh that that's fine that is planet could
  1997. 1:10:13there be multiple objects like that i
  1998. 1:10:15guess
  1999. 1:10:16in principle yeah i mean there's no
  2000. 1:10:19there's no law of physics that uh that
  2001. 1:10:20doesn't allow you to have multiple
  2002. 1:10:22there's also no evidence at present for
  2003. 1:10:24there being multiple i wonder if
  2004. 1:10:26it's possible this is like just like
  2005. 1:10:27we're finding exoplanets
  2006. 1:10:29whether given the size of the or cloud
  2007. 1:10:32there's basically
  2008. 1:10:33it's rare and rare but they're sprinkled
  2009. 1:10:35planet nine
  2010. 1:10:37ten eleven twelve like these yeah
  2011. 1:10:40some got thirteen after that yeah i can
  2012. 1:10:43just keep counting
  2013. 1:10:45so like just something about the dynamic
  2014. 1:10:47system
  2015. 1:10:48like it becomes lower and lower
  2016. 1:10:49probability event but they gather up
  2017. 1:10:51like they they become would they become
  2018. 1:10:54larger and larger maybe
  2019. 1:10:55something like that and i wonder i
  2020. 1:10:58wonder if like discovering planet nine
  2021. 1:11:00will just like be almost like a
  2022. 1:11:02springboard it's like well what's
  2023. 1:11:04what's beyond that it's entirely
  2024. 1:11:06plausible the oort cloud itself
  2025. 1:11:08probably holds about five earth masses
  2026. 1:11:10or seven earth masses of material
  2027. 1:11:13right so it's not it's not nothing and
  2028. 1:11:17the it all ultimately comes down
  2029. 1:11:20to at what point will the observational
  2030. 1:11:25surveys
  2031. 1:11:26sample enough of the solar system to uh
  2032. 1:11:29kind of
  2033. 1:11:30reveal interesting things
  2034. 1:11:33there's a great analogy here with
  2035. 1:11:35neptune and the story of how neptune was
  2036. 1:11:37discovered
  2037. 1:11:38neptune was not discovered by looking at
  2038. 1:11:40the sky
  2039. 1:11:41right it was discovered by uh it was
  2040. 1:11:44certain mathematically
  2041. 1:11:45right so yeah the orbit of
  2042. 1:11:48uranus when uranus was found um
  2043. 1:11:52yes this was 1781. uh it's
  2044. 1:11:55the kind of tracking uh both the
  2045. 1:11:58tracking
  2046. 1:11:58of the orbit of uranus as well as the
  2047. 1:12:01reconstruction
  2048. 1:12:02of the orbit of uranus immediately
  2049. 1:12:04revealed
  2050. 1:12:05that it was not following the orbit that
  2051. 1:12:08it was supposed to
  2052. 1:12:09right the the predicted orbit deviated
  2053. 1:12:11away from where it actually was
  2054. 1:12:13so uh in the mid eighteen hundreds
  2055. 1:12:17right um a french mathematician by the
  2056. 1:12:20name of orban le verrier
  2057. 1:12:22did a beautifully sophisticated
  2058. 1:12:24calculation which said
  2059. 1:12:26if this is due to gravity of a
  2060. 1:12:30more distant planet then that planet is
  2061. 1:12:32there
  2062. 1:12:33okay and then they found it but the
  2063. 1:12:35point is the
  2064. 1:12:36understanding of where to look for
  2065. 1:12:40neptune came entirely out of celestial
  2066. 1:12:42mechanics
  2067. 1:12:43the case with planet nine is a little
  2068. 1:12:46bit different
  2069. 1:12:46because what we can do i think
  2070. 1:12:48relatively well is predict the orbit and
  2071. 1:12:50mass of planet nine we cannot tell you
  2072. 1:12:52where it is on its orbit
  2073. 1:12:54the reason is we haven't seen the kuiper
  2074. 1:12:57belt objects complete
  2075. 1:12:58in orbit their own orbit
  2076. 1:13:01even once because it takes four thousand
  2077. 1:13:03years but
  2078. 1:13:05you know i plan to live on as an ai
  2079. 1:13:07being
  2080. 1:13:08uh and you know i'll i'll be tracking
  2081. 1:13:11those
  2082. 1:13:11uh those orbits as solid takes four or
  2083. 1:13:13five thousand years i mean
  2084. 1:13:15it doesn't have to be ai it could be
  2085. 1:13:16longevity there's a lot of really
  2086. 1:13:17exciting genetic engineering research
  2087. 1:13:19so you'll just be a brain waiting for
  2088. 1:13:21the
  2089. 1:13:23for the your brain waiting for the orbit
  2090. 1:13:25to complete for the basic kuiper belt
  2091. 1:13:27objects
  2092. 1:13:27that's that's right that's like kind of
  2093. 1:13:30the worst
  2094. 1:13:31reason to want to live a long time right
  2095. 1:13:34just like can the brain like smoke a
  2096. 1:13:35cigarette
  2097. 1:13:36can you just like light one up while
  2098. 1:13:39you're waiting or
  2099. 1:13:40uh
  2100. 1:13:41[Laughter]
  2101. 1:13:43but you're making me actually realize
  2102. 1:13:45that the one way to explore
  2103. 1:13:49the the galaxy is by just sitting here
  2104. 1:13:52on earth and waiting
  2105. 1:13:54so if we can just get really good at
  2106. 1:13:55waiting it's like a more more or these
  2107. 1:13:58interstellar objects that
  2108. 1:14:00fly in you can just wait for them to
  2109. 1:14:02come to you same with the aliens you can
  2110. 1:14:03wait for them to come to you
  2111. 1:14:05if you get really good at waiting um
  2112. 1:14:08then
  2113. 1:14:09that's one way to do the exploration
  2114. 1:14:10because eventually the thing will come
  2115. 1:14:12to you maybe that's the entire
  2116. 1:14:13maybe the intelligent alien
  2117. 1:14:15civilizations
  2118. 1:14:16get much better at waiting and so they
  2119. 1:14:19all decide so
  2120. 1:14:20game theoretically to start waiting and
  2121. 1:14:21it's just a bunch of like
  2122. 1:14:23ancient intelligent civilizations of
  2123. 1:14:25aliens all throughout the universe
  2124. 1:14:27they're just sitting there waiting for
  2125. 1:14:28each other
  2126. 1:14:29look you can't just be good at waiting
  2127. 1:14:31you got to know how to chill
  2128. 1:14:32okay like like you can't just like sit
  2129. 1:14:35around and do nothing you got to be
  2130. 1:14:36you get you got to know how to chill i
  2131. 1:14:38honestly think that
  2132. 1:14:40as we progress if the aliens are
  2133. 1:14:42anything like us
  2134. 1:14:43we enjoy loving things we do
  2135. 1:14:46and it it's uh it's very possible that
  2136. 1:14:49we just figure out mechanisms
  2137. 1:14:51here on earth to enjoy our life and we
  2138. 1:14:54just stay here on our f
  2139. 1:14:55forever that exploration becomes less
  2140. 1:14:58and less of an interesting thing to do
  2141. 1:15:00and so you basically yes wait and chill
  2142. 1:15:03you get really optimally good at
  2143. 1:15:04chilling and thereby
  2144. 1:15:06exploring is not that interesting so you
  2145. 1:15:09know
  2146. 1:15:10in terms of 4 000 years would be nothing
  2147. 1:15:12for scientists we'll be chilling and
  2148. 1:15:13just
  2149. 1:15:14all kinds of scientific explorations
  2150. 1:15:16will become
  2151. 1:15:17possible because we'll just be here
  2152. 1:15:22you have a paper out recently because
  2153. 1:15:24you already mentioned some of these
  2154. 1:15:25ideas but
  2155. 1:15:26i'd love it if you could dig into it a
  2156. 1:15:27little bit yeah of course the injection
  2157. 1:15:29of inner
  2158. 1:15:30or cloud objects into the distant kuiper
  2159. 1:15:32belt by planet nine
  2160. 1:15:34what is this idea of
  2161. 1:15:38planet nine injecting objects into the
  2162. 1:15:40kuiper belt okay let me take a
  2163. 1:15:42brief step back and when we do
  2164. 1:15:45calculations of
  2165. 1:15:46planet nine we do the simulations
  2166. 1:15:49as far as our simulations are concerned
  2167. 1:15:52sort of
  2168. 1:15:52the uh neptune
  2169. 1:15:56like kind of the trans-neptunian solar
  2170. 1:15:59system
  2171. 1:16:00is entirely sourced from the inside
  2172. 1:16:03namely the kuiper belt gets scattered by
  2173. 1:16:07neptune and then planet nine does things
  2174. 1:16:09to it and aligns the orbits and
  2175. 1:16:11and so on and then we calculate what uh
  2176. 1:16:14what happens on the lifetime of the
  2177. 1:16:15solar system yada yada
  2178. 1:16:18during the pandemic one of the kind of
  2179. 1:16:20questions we asked
  2180. 1:16:21ourselves this is indeed something we
  2181. 1:16:23mike and i uh
  2182. 1:16:25mike brown whose partner in crime on
  2183. 1:16:27this and i
  2184. 1:16:29do regularly is we say how can
  2185. 1:16:33we a disprove ourselves and b
  2186. 1:16:36how can we improve our simulations like
  2187. 1:16:39what's missing
  2188. 1:16:40one idea that maybe should have been
  2189. 1:16:43obvious in retrospect is that all of our
  2190. 1:16:46simulations treated the solar system
  2191. 1:16:48as some isolated creature right but the
  2192. 1:16:50solar system did not form in isolation
  2193. 1:16:53right it formed in this cluster of stars
  2194. 1:16:55and during that phase
  2195. 1:16:57of forming together with thousands of
  2196. 1:16:59other stars
  2197. 1:17:01we believe the solar system formed this
  2198. 1:17:04almost spherical population of icy
  2199. 1:17:06debris
  2200. 1:17:08that sits maybe at a
  2201. 1:17:11few thousand times the separation
  2202. 1:17:14between
  2203. 1:17:16the earth and the sun maybe even a
  2204. 1:17:18little bit closer
  2205. 1:17:20if planet nine's not there that
  2206. 1:17:22population is completely dormant
  2207. 1:17:24and these objects just slowly orbit
  2208. 1:17:27the the sun nothing interesting had
  2209. 1:17:30happens to them ever but what we
  2210. 1:17:32realized that if planet nine is there
  2211. 1:17:35planet nine can actually grab some of
  2212. 1:17:37those objects and gravitationally
  2213. 1:17:38re-inject them
  2214. 1:17:40into the distant solar system so we
  2215. 1:17:42thought okay let's look into this
  2216. 1:17:44with numerical experiments do do our
  2217. 1:17:46simulations
  2218. 1:17:47does this process work and if it works
  2219. 1:17:50uh
  2220. 1:17:51what are its consequences so it turns
  2221. 1:17:53out indeed not only
  2222. 1:17:55does planet nine inject these distant
  2223. 1:18:00inner or cloud objects into the kuiper
  2224. 1:18:02belt
  2225. 1:18:03they follow roughly the same pathway as
  2226. 1:18:06the
  2227. 1:18:07um as the objects that are being
  2228. 1:18:09scattered out also there's this
  2229. 1:18:11kind of river two-way river of material
  2230. 1:18:14some of it is coming out from you know
  2231. 1:18:17by neptune scattering some of it is
  2232. 1:18:19moving in and if you work through the
  2233. 1:18:22numbers
  2234. 1:18:23you kind of at the end of the day that
  2235. 1:18:26it
  2236. 1:18:26it has an effect on the best fit orbit
  2237. 1:18:28for planet nine itself
  2238. 1:18:29so if you realize that the data set that
  2239. 1:18:32we're observing
  2240. 1:18:33is not entirely composed of things that
  2241. 1:18:36came out of the solar system but also
  2242. 1:18:37things that got
  2243. 1:18:38re-injected back in then turns out the
  2244. 1:18:41best fit planet nine slightly more
  2245. 1:18:42eccentric
  2246. 1:18:43that's kind of getting into the weeds
  2247. 1:18:45the the point here is that
  2248. 1:18:48uh you know the existence of planet nine
  2249. 1:18:50itself provides this
  2250. 1:18:52natural bridge that connects an
  2251. 1:18:54otherwise dormant population of icy
  2252. 1:18:56debris of the solar system
  2253. 1:18:58with things that we're starting to
  2254. 1:18:59directly observe so you can flow back so
  2255. 1:19:01it's not just the river flowing one way
  2256. 1:19:02it's
  2257. 1:19:03maybe a smaller stream go back and
  2258. 1:19:05backwash
  2259. 1:19:06you want a backwash you want to
  2260. 1:19:07incorporate that into the simulations
  2261. 1:19:09into your
  2262. 1:19:10understanding of those distant objects
  2263. 1:19:12when you're trying to make sense of the
  2264. 1:19:14various observations and so on exactly
  2265. 1:19:15that's fascinating
  2266. 1:19:17i gotta ask you some people think that
  2267. 1:19:20uh many of the observations you're
  2268. 1:19:23describing
  2269. 1:19:24could be described by a primordial black
  2270. 1:19:28hole
  2271. 1:19:29first what is the primordial black hole
  2272. 1:19:31and what do you think about this idea
  2273. 1:19:32yeah
  2274. 1:19:33so primordial black hole is a black hole
  2275. 1:19:36which is made
  2276. 1:19:37not through the usual pathway of making
  2277. 1:19:39a black hole
  2278. 1:19:41which is that you have a star which is
  2279. 1:19:44uh more massive
  2280. 1:19:45than you know 1.4 or so solar masses and
  2281. 1:19:49basically when it runs out of
  2282. 1:19:51fuel uh runs out of its nuclear fusion
  2283. 1:19:55fuel
  2284. 1:19:56it can't hold itself up anymore and just
  2285. 1:19:58the whole thing collapses on itself
  2286. 1:20:01right you create a um
  2287. 1:20:04i mean one i guess simple way to think
  2288. 1:20:07about it is you create an
  2289. 1:20:08object with zero radius that has mass
  2290. 1:20:11but zero radius
  2291. 1:20:12that singularity
  2292. 1:20:16now that's such black holes exist all
  2293. 1:20:19over the place in the galaxy there's in
  2294. 1:20:21fact
  2295. 1:20:21a really big one at the center of the
  2296. 1:20:23galaxy that's like yeah
  2297. 1:20:25that that one's always looking at you
  2298. 1:20:27when you're not looking
  2299. 1:20:28okay right and it's it's always talking
  2300. 1:20:31about you
  2301. 1:20:31and when you turn off the lights it's it
  2302. 1:20:33wakes up
  2303. 1:20:34that's right um but you know so such
  2304. 1:20:38black holes
  2305. 1:20:38are all over the place we when they
  2306. 1:20:40merge we get to see
  2307. 1:20:42you know incredible gravitational waves
  2308. 1:20:43that they emit etc etc
  2309. 1:20:45one kind of plausible scenario however
  2310. 1:20:47is that
  2311. 1:20:48when the universe was forming basically
  2312. 1:20:50during the big bang
  2313. 1:20:52you created a whole spectrum of black
  2314. 1:20:55holes
  2315. 1:20:57some with masses of five earth masses
  2316. 1:20:59some with masses of
  2317. 1:21:0110 earth masses like the entire you know
  2318. 1:21:03mass spectrum size
  2319. 1:21:05the amount some the mass of asteroids
  2320. 1:21:08now on the smaller end over the lifetime
  2321. 1:21:12of the universe
  2322. 1:21:13the small ones kind of evaporate and
  2323. 1:21:15they're not there anymore at least this
  2324. 1:21:17is what we
  2325. 1:21:18what the calculations tell us but five
  2326. 1:21:21earth masses is big enough to
  2327. 1:21:23not have evaporated so one idea is that
  2328. 1:21:27planet nine is not a planet and instead
  2329. 1:21:30it is a five
  2330. 1:21:32earth mass black hole and that's why
  2331. 1:21:35it's hard to find now
  2332. 1:21:39can we right away from our calculations
  2333. 1:21:42say
  2334. 1:21:43that's definitely true or that's not
  2335. 1:21:44true absolutely not we can't in fact our
  2336. 1:21:46calculations
  2337. 1:21:48tell you nothing other than the orbit
  2338. 1:21:52and the mass and that means the
  2339. 1:21:55black hole i mean it could be a five
  2340. 1:21:57earth mass you know
  2341. 1:21:58cup it could be a five earth mass
  2342. 1:22:01hedgehog or a black hole or
  2343. 1:22:03really anything that's five earth masses
  2344. 1:22:05will do because the gravity of a black
  2345. 1:22:07hole
  2346. 1:22:08is no different than the gravity of a
  2347. 1:22:10planet right if the sun became a black
  2348. 1:22:12hole tomorrow
  2349. 1:22:14it would be dark but or the earth would
  2350. 1:22:16keep orbiting it
  2351. 1:22:18and like this notion that oh black holes
  2352. 1:22:20suck everything in
  2353. 1:22:21it's it's not that's like a sci-fi
  2354. 1:22:24notion right it's just mass
  2355. 1:22:25what would be the difference between a
  2356. 1:22:26black hole and a planet
  2357. 1:22:29in terms of observationally uh
  2358. 1:22:32observationally the difference would be
  2359. 1:22:34that you will never find the black hole
  2360. 1:22:36right the truth is they're kind of um
  2361. 1:22:38i'm actually
  2362. 1:22:39not you know i never looked into this
  2363. 1:22:42very carefully
  2364. 1:22:43but there are some constraints that you
  2365. 1:22:46can
  2366. 1:22:47get just statistically say okay if the
  2367. 1:22:50sun
  2368. 1:22:51has a binary companion which is a five
  2369. 1:22:53earth mass black hole
  2370. 1:22:55then that means such black holes would
  2371. 1:22:58be extremely
  2372. 1:22:59common and you know you can sort of look
  2373. 1:23:01for lensing events and then you say okay
  2374. 1:23:03maybe that's not so likely
  2375. 1:23:05but you know that said i want to
  2376. 1:23:07emphasize that
  2377. 1:23:08there's a limit to what our calculations
  2378. 1:23:11uh
  2379. 1:23:11can tell you that's the orbit and the
  2380. 1:23:13mass so
  2381. 1:23:15i think there's a bunch like ed whitton
  2382. 1:23:17i think
  2383. 1:23:18wishes it's a black hole because i think
  2384. 1:23:21the one exciting things about black
  2385. 1:23:22holes
  2386. 1:23:23in our solar system is that we can go
  2387. 1:23:25there
  2388. 1:23:26and we can maybe study the singularity
  2389. 1:23:28somehow because that allows us to
  2390. 1:23:30understand some fundamental things about
  2391. 1:23:32physics
  2392. 1:23:33if um it's a planet so planet nine
  2393. 1:23:36we may not you know and we go there we
  2394. 1:23:38may not discover
  2395. 1:23:39anything profoundly new
  2396. 1:23:43the interesting thing perhaps you can
  2397. 1:23:44correct me about planet nine
  2398. 1:23:46is like the big picture of it the whole
  2399. 1:23:48big story of the kuiper belt and all
  2400. 1:23:50those kinds of things
  2401. 1:23:52it's not that planet nine would be
  2402. 1:23:54somehow fundamentally different
  2403. 1:23:56from um from i don't know neptune
  2404. 1:24:00in terms of um in terms of the kind of
  2405. 1:24:02things we can learn from it so i think
  2406. 1:24:04that
  2407. 1:24:04there's kind of a hope that it's a black
  2408. 1:24:06hole because it's an entirely new kind
  2409. 1:24:08of object maybe you can
  2410. 1:24:09uh correct me yeah i mean of course here
  2411. 1:24:13my own
  2412. 1:24:14biases creep in because i'm interested
  2413. 1:24:16you know
  2414. 1:24:17in planets around other stars and
  2415. 1:24:20i would say i would disagree that you
  2416. 1:24:23know we wouldn't find
  2417. 1:24:24things that would be truly you know
  2418. 1:24:27fundamentally new new because as it
  2419. 1:24:30turns out
  2420. 1:24:31the the galaxy is really good at making
  2421. 1:24:35five or three earth mass objects right
  2422. 1:24:38the most common type of planet that we
  2423. 1:24:42see that we you know discover orbiting
  2424. 1:24:44around other stars
  2425. 1:24:45there's a few earth masses in the solar
  2426. 1:24:48system there's no analog for that
  2427. 1:24:49right we go from one earth mass object
  2428. 1:24:51which is this one
  2429. 1:24:52and to skipping to neptune and uranus
  2430. 1:24:55which themselves are actually relatively
  2431. 1:24:57poorly understood
  2432. 1:24:59especially uranus from the interior
  2433. 1:25:01structure point of view
  2434. 1:25:03if planet nine is a planet going there
  2435. 1:25:06will give us the closest window and to
  2436. 1:25:08understanding what
  2437. 1:25:10other planets look like and um
  2438. 1:25:14i will you know i'll say this that you
  2439. 1:25:16know planets
  2440. 1:25:17kind of in terms of their complexity on
  2441. 1:25:19some logarithmic scale
  2442. 1:25:21fall somewhere between a star and an
  2443. 1:25:24insect
  2444. 1:25:25right an insect is way more complicated
  2445. 1:25:28than a star
  2446. 1:25:29right just there's all kinds of physical
  2447. 1:25:32processes and really
  2448. 1:25:34biochemical processes that occur inside
  2449. 1:25:37of an insect
  2450. 1:25:38that just make a star look like
  2451. 1:25:41you know somebody is like playing with
  2452. 1:25:43the spring or something yeah
  2453. 1:25:45right so the i i think
  2454. 1:25:48you know it would be you know arguably
  2455. 1:25:51you know more interesting to go to um
  2456. 1:25:55you know to go to planet nine if it's a
  2457. 1:25:57planet because black holes are simple
  2458. 1:25:59they're just kind of
  2459. 1:26:00they're basically macroscopic like
  2460. 1:26:03particles yeah right and so just like
  2461. 1:26:06you mentioned in terms of complexity so
  2462. 1:26:08it's possible that planet nine
  2463. 1:26:10as opposed to being like homogeneous is
  2464. 1:26:12like super
  2465. 1:26:13like heterogeneous is a bunch of cool
  2466. 1:26:15stuff going on absolutely
  2467. 1:26:16that could give us an intuition i never
  2468. 1:26:18thought about that that it's
  2469. 1:26:20basically earth number two in terms of
  2470. 1:26:22size
  2471. 1:26:24and gives us starts giving us intuition
  2472. 1:26:26that could be generalizable to
  2473. 1:26:28earth-like planets elsewhere in the
  2474. 1:26:30galaxy yeah pluto
  2475. 1:26:32is also in the sense like you know pluto
  2476. 1:26:35is a tiny tiny thing right just like
  2477. 1:26:38you would imagine there's just a tiny
  2478. 1:26:39ball of ice like who cares but the new
  2479. 1:26:41horizons
  2480. 1:26:42images of pluto reveal so much
  2481. 1:26:45remarkable structure
  2482. 1:26:46right they reveal glaciers flowing and
  2483. 1:26:49these are glaciers
  2484. 1:26:50not made out of water ice but you know
  2485. 1:26:52co ice
  2486. 1:26:53it turns out at those temperatures
  2487. 1:26:56right of like 40 or so kelvin water ice
  2488. 1:27:00looks like metal right it doesn't flow
  2489. 1:27:02at all but then
  2490. 1:27:03ice made up of carbon monoxide
  2491. 1:27:06starts to flow i mean there's just like
  2492. 1:27:08all kinds of really cool
  2493. 1:27:10uh phenomena that you otherwise just
  2494. 1:27:13wouldn't really even imagine that occur
  2495. 1:27:17so yeah i mean there's a reason why i
  2496. 1:27:19like planets
  2497. 1:27:21well let me ask you i find uh
  2498. 1:27:25as i read the idea that edwin was
  2499. 1:27:28thinking about this kind of stuff
  2500. 1:27:29fascinating so he he's a mathematical
  2501. 1:27:31physicist
  2502. 1:27:33who's uh very interested in string
  2503. 1:27:35theory won the fields
  2504. 1:27:37metal for his work in mathematics
  2505. 1:27:41so i read that he proposed a fleet of
  2506. 1:27:43probes
  2507. 1:27:44accelerated by radiation pressure that
  2508. 1:27:47could discover a planet nine primordial
  2509. 1:27:49black holes location
  2510. 1:27:52uh what do you think about this idea of
  2511. 1:27:53sending a bunch of probes out there
  2512. 1:27:56yeah look the way the the idea is a cool
  2513. 1:27:59one
  2514. 1:28:00right you go and you say
  2515. 1:28:03you know launch them basically
  2516. 1:28:05isotropically you track where they go
  2517. 1:28:07and uh if i understand the idea
  2518. 1:28:10correctly you basically measure the
  2519. 1:28:13deflection and then you say okay there
  2520. 1:28:15must be
  2521. 1:28:16something there since the the
  2522. 1:28:19probe trajectories are being altered oh
  2523. 1:28:21so the measurement
  2524. 1:28:22the basic sensory mechanism is the it's
  2525. 1:28:25not like you have sensors on the probes
  2526. 1:28:27it's more like you're
  2527. 1:28:29because you're very precisely able to
  2528. 1:28:30capture to measure the trajectory of the
  2529. 1:28:33probes you can then
  2530. 1:28:34infer the gravitational fields and i
  2531. 1:28:35think i think that's the basic idea
  2532. 1:28:38um you know back a few years ago we
  2533. 1:28:42had conversations like these with um
  2534. 1:28:45you know engineers from jpl they
  2535. 1:28:48more or less convinced me that this is
  2536. 1:28:51much more difficult than it seems
  2537. 1:28:53because
  2538. 1:28:54you don't at that level of precision
  2539. 1:28:57right
  2540. 1:28:58things like solar flares matter right
  2541. 1:29:00solar flares
  2542. 1:29:01right are completely chaotic you can't
  2543. 1:29:04predict which
  2544. 1:29:05where a solar flare will happen that
  2545. 1:29:07will drive radiation
  2546. 1:29:08pressure gradients you don't know where
  2547. 1:29:11every single asteroid is so like
  2548. 1:29:13actually doing that problem
  2549. 1:29:17i think it's possible but it's it's not
  2550. 1:29:19a trivial matter
  2551. 1:29:20right well i wonder not just about
  2552. 1:29:24planet nine i wonder if that's kind of
  2553. 1:29:26the future
  2554. 1:29:27of doing science in our solar system
  2555. 1:29:30is to just launch a huge number of
  2556. 1:29:32probes so like a
  2557. 1:29:34whole order of magnitude many orders of
  2558. 1:29:36magnitude larger
  2559. 1:29:38numbers of probes and then starting for
  2560. 1:29:40a bunch of different stuff
  2561. 1:29:42not just gravity but everything else so
  2562. 1:29:44in this regard
  2563. 1:29:45i actually think there is a huge
  2564. 1:29:47revolution that's
  2565. 1:29:49to some extent already started right the
  2566. 1:29:52standard kind of like
  2567. 1:29:53time scale for a nasa mission is that
  2568. 1:29:55you like
  2569. 1:29:56propose it and it launches i don't know
  2570. 1:29:59like
  2571. 1:29:59150 years after you propose i'm over
  2572. 1:30:02exaggerating but
  2573. 1:30:03yeah you know it's just like some huge
  2574. 1:30:05development cycle
  2575. 1:30:07yeah and it gets delayed 55 times
  2576. 1:30:11like that is not going away
  2577. 1:30:14yeah right the the really cutting edge
  2578. 1:30:17things
  2579. 1:30:18you have to do it this way because you
  2580. 1:30:19don't know what you're building so to
  2581. 1:30:21speak
  2582. 1:30:22but the cubesat kind of world
  2583. 1:30:25is starting to um you know provide an
  2584. 1:30:29avenue for like
  2585. 1:30:31you know launching something that costs
  2586. 1:30:32you know a few million dollars
  2587. 1:30:34and has a turnaround time scale of like
  2588. 1:30:37a couple years you can imagine doing
  2589. 1:30:39you know phd theses where you design the
  2590. 1:30:42mission
  2591. 1:30:43the mission goes to where you're going
  2592. 1:30:44and you do the science
  2593. 1:30:46all within a time span of five six years
  2594. 1:30:49that is has not been fully executed on
  2595. 1:30:53yet but i absolutely think that's on the
  2596. 1:30:55horizon and we're not talking
  2597. 1:30:57a decade i think we're talking like this
  2598. 1:30:59decade
  2599. 1:31:00yeah and the company is accelerating all
  2600. 1:31:02this uh
  2601. 1:31:03with uh blue origin and and uh spacex
  2602. 1:31:07there's a bunch of more cubesat oriented
  2603. 1:31:09companies that are pushing this forward
  2604. 1:31:11uh well let me ask you let me ask you on
  2605. 1:31:14that topic what do you think about
  2606. 1:31:16either one elon musk with spacex
  2607. 1:31:20uh going to mars i think he wants spacex
  2608. 1:31:22to be the first
  2609. 1:31:23to put a first human on mars and then uh
  2610. 1:31:28jeff bezos got to give him props
  2611. 1:31:32wants to be the first to fly his own
  2612. 1:31:33rocket
  2613. 1:31:35out into space so you know wasn't there
  2614. 1:31:38a guy who like
  2615. 1:31:39built his rocket out of garbage yeah
  2616. 1:31:42this was like a couple
  2617. 1:31:44years ago and somewhere in the desert he
  2618. 1:31:46launched himself
  2619. 1:31:47i'm not tracking this closely but i
  2620. 1:31:49think i am
  2621. 1:31:50familiar with folks who built their own
  2622. 1:31:52rocket to try to prove the earth is flat
  2623. 1:31:54yes that's the guy i'm talking about
  2624. 1:31:55yeah he was also like he also jumped
  2625. 1:31:57some limousine yeah
  2626. 1:31:59for truly revolutionary minds
  2627. 1:32:03uh greater men than either you or i
  2628. 1:32:07but yeah so look it's been
  2629. 1:32:10astonishing to watch how really over the
  2630. 1:32:13last like
  2631. 1:32:14decade the commercial sector
  2632. 1:32:17took over this uh you know
  2633. 1:32:20this industry that traditionally has
  2634. 1:32:23really been like
  2635. 1:32:23a you know a government thing to do um
  2636. 1:32:27motivated primarily by the the
  2637. 1:32:29competition between nations like the
  2638. 1:32:31cold war
  2639. 1:32:32sure and now it's motivated more
  2640. 1:32:35more and more by the natural forces of
  2641. 1:32:38capitalism yes
  2642. 1:32:39that's right so um okay here
  2643. 1:32:42i have i have many ideas about i think
  2644. 1:32:44on the one hand right
  2645. 1:32:45like what spacex has been able to do for
  2646. 1:32:47example phenomenal
  2647. 1:32:49um if that brings down
  2648. 1:32:53the price of spacex within that
  2649. 1:32:55turnaround time scale for space
  2650. 1:32:57exploration which i think it inevitably
  2651. 1:32:59will um that's a huge you know that's a
  2652. 1:33:03huge boost
  2653. 1:33:04to the to the human condition the same
  2654. 1:33:06time
  2655. 1:33:07right if we're talking astronomy right
  2656. 1:33:09there they're also
  2657. 1:33:11it comes at a huge cost right and the
  2658. 1:33:13starling satellites is a great example
  2659. 1:33:15of that cost right at one point uh
  2660. 1:33:18in fact i was just camping and the
  2661. 1:33:21mojave was a
  2662. 1:33:22with a friend of mine and they saw you
  2663. 1:33:24know
  2664. 1:33:25this uh the string of satellites just
  2665. 1:33:27kind of like
  2666. 1:33:28you know appear and then disappear uh
  2667. 1:33:31into nowhere so that
  2668. 1:33:33is beginning to interfere with you know
  2669. 1:33:35earth-based observations so
  2670. 1:33:37i think it's there's tremendous
  2671. 1:33:39potential there
  2672. 1:33:40it's also important to be responsible
  2673. 1:33:42about how it's executed
  2674. 1:33:44now with mars and the whole idea of you
  2675. 1:33:48know exploring mars
  2676. 1:33:50right i don't have like strong opinions
  2677. 1:33:52on whether a manned mission
  2678. 1:33:54is is required or not required
  2679. 1:33:58um but i do think you know
  2680. 1:34:02we need to focus the thing to keep in
  2681. 1:34:04mind is that
  2682. 1:34:05i i generally kind of
  2683. 1:34:08uh i'm not signed on if it will to the
  2684. 1:34:10idea that mars is some kind of a safe
  2685. 1:34:12haven that we can
  2686. 1:34:14uh you know escape to right
  2687. 1:34:17mars sucks right like living on mars if
  2688. 1:34:20you
  2689. 1:34:21if you want to live on mars like you can
  2690. 1:34:24have that experience
  2691. 1:34:25by going to the mojave desert and
  2692. 1:34:27camping and it's just like
  2693. 1:34:30it's it's just not a great well it's
  2694. 1:34:32interesting but there's something
  2695. 1:34:33captivating about that kind of mission
  2696. 1:34:35of
  2697. 1:34:35us striving out into space and by making
  2698. 1:34:39mars in some ways habitable
  2699. 1:34:43for at least like months at a time
  2700. 1:34:46i think would lead to engineering
  2701. 1:34:47breakthroughs that would make life
  2702. 1:34:49like in many ways much better on earth
  2703. 1:34:52like it would we'll come up with
  2704. 1:34:53ideas we totally don't expect yet both
  2705. 1:34:56on the robotics side
  2706. 1:34:57on the food engineering side on the
  2707. 1:35:01you know maybe like we'll switch from
  2708. 1:35:04what like there'll be huge breakthroughs
  2709. 1:35:06in insect farming as
  2710. 1:35:08as exciting as i find that idea to be
  2711. 1:35:11that in you know our in the ways we
  2712. 1:35:13consume protein maybe
  2713. 1:35:15uh it'll revolutionize we do factory
  2714. 1:35:17farming which is
  2715. 1:35:18full of cruelty and you know and torture
  2716. 1:35:21of animals will
  2717. 1:35:22revolutionize that completely because of
  2718. 1:35:24our like we don't
  2719. 1:35:25we shouldn't need to go to mars to
  2720. 1:35:27revolutionize life here on earth
  2721. 1:35:29but at the same time i shouldn't need a
  2722. 1:35:31deadline to get done
  2723. 1:35:33but i do need it and then the same way i
  2724. 1:35:35think we need
  2725. 1:35:36mars there's something about the human
  2726. 1:35:38spirit that loves that
  2727. 1:35:40longing for i i agree with that thesis
  2728. 1:35:42the going to the moon
  2729. 1:35:44right and the that whole
  2730. 1:35:47endeavor has you know
  2731. 1:35:51has captivated the imagination of so
  2732. 1:35:53many and it has uh
  2733. 1:35:55it has led to incredible kind of
  2734. 1:35:57incredible ideas really and and probably
  2735. 1:35:59in non-linear ways
  2736. 1:36:01right not like okay we went to the moon
  2737. 1:36:03therefore
  2738. 1:36:04some person here has thought of this and
  2739. 1:36:06yes in in that similar sense
  2740. 1:36:08i think you know space exploration is
  2741. 1:36:11there's something there's some real
  2742. 1:36:13magnetism about it
  2743. 1:36:15and it's on a genetic level right like
  2744. 1:36:17we have this
  2745. 1:36:18need to keep exploring right when we're
  2746. 1:36:21done
  2747. 1:36:22uh with a certain frontier we move on to
  2748. 1:36:25the next frontier all that i'm saying
  2749. 1:36:27is that i'm not moving to mars to live
  2750. 1:36:30there permanently
  2751. 1:36:31uh ever you know and i think that you
  2752. 1:36:33know i'm glad you paid
  2753. 1:36:35you you noted the kind of degradation of
  2754. 1:36:38the earth
  2755. 1:36:39right i think that is a true kind of
  2756. 1:36:42the leading order challenge of our great
  2757. 1:36:44engineering that's
  2758. 1:36:46a bunch of a bunch of engineering
  2759. 1:36:47problems i'm most interested in this
  2760. 1:36:49space because as i've read extensively
  2761. 1:36:52it's apparently very difficult to have
  2762. 1:36:54sex in space
  2763. 1:36:55and so i just want that problem to be
  2764. 1:36:57solved because i think
  2765. 1:36:58once we solve the sex and space problem
  2766. 1:37:00we'll revolutionize sex here on earth
  2767. 1:37:03thereby increasing the fun on earth and
  2768. 1:37:06um
  2769. 1:37:06the consequences of that can only be
  2770. 1:37:08good i mean you can
  2771. 1:37:10you've got a clear plan right and and it
  2772. 1:37:13sounds like uh yeah i'm submitting
  2773. 1:37:14proposals to nasa as we said that's
  2774. 1:37:16right
  2775. 1:37:18i keep getting rejected i don't know why
  2776. 1:37:20okay
  2777. 1:37:21uh you need better diagrams better
  2778. 1:37:24better pictures
  2779. 1:37:25i should have thought of that you a
  2780. 1:37:26while ago mentioned that
  2781. 1:37:28you know there's certain aspects in the
  2782. 1:37:30history of the solar system and earth
  2783. 1:37:32that resulted that it could have
  2784. 1:37:34resulted in an
  2785. 1:37:35opaque atmosphere but it didn't
  2786. 1:37:38we couldn't see the stars um
  2787. 1:37:42and uh somebody mentioned to me a little
  2788. 1:37:45bit ago
  2789. 1:37:46it's almost like a philosophical
  2790. 1:37:47question for you do you think
  2791. 1:37:51humans like human society would develop
  2792. 1:37:55as it did or at all if we couldn't see
  2793. 1:37:58the stars
  2794. 1:37:59it would be drastically different
  2795. 1:38:02just dr if it ever did develop so i
  2796. 1:38:05think some of the early developments
  2797. 1:38:08right of like fire and you know fire
  2798. 1:38:11you know first of all that atmosphere
  2799. 1:38:13would be so hot because you know if you
  2800. 1:38:15have an opaque
  2801. 1:38:16atmosphere the temperature at the bottom
  2802. 1:38:20is is huge um so we would
  2803. 1:38:23be very different beings to start with
  2804. 1:38:25we'd have it could be cloudy in certain
  2805. 1:38:27kinds of ways that you could still get
  2806. 1:38:29okay think about like uh like a
  2807. 1:38:31greenhouse right a greenhouse
  2808. 1:38:33is cloudy effectively uh but it's it's
  2809. 1:38:36super hot
  2810. 1:38:37um yeah it's hard to avoid having an
  2811. 1:38:40atmosphere if you have an
  2812. 1:38:41opaque atmosphere it's hard to right
  2813. 1:38:44venus is a great example
  2814. 1:38:45right venus is i don't remember exactly
  2815. 1:38:48how many degrees
  2816. 1:38:49and but it's hundreds in celsius right
  2817. 1:38:52it's not a hundred it's hundreds
  2818. 1:38:54uh even though it's only a little bit
  2819. 1:38:56closer to the sun that temperature
  2820. 1:38:58is entirely coming from the fact that
  2821. 1:39:00the atmosphere is thick so it's just a
  2822. 1:39:02sauna of sorts
  2823. 1:39:03yeah yeah you go there you know you feel
  2824. 1:39:06refreshed after you come back
  2825. 1:39:07you know but if you stay there i mean so
  2826. 1:39:10okay take that as an assumption
  2827. 1:39:12this is a philosophical question not a
  2828. 1:39:14biological one so you have a life that
  2829. 1:39:16develops under these
  2830. 1:39:17extremely hot conditions yeah so let's
  2831. 1:39:19see so much of
  2832. 1:39:21the early evolution of mankind
  2833. 1:39:24uh was driven by exploration yeah right
  2834. 1:39:28and the kind of interest and stars
  2835. 1:39:32originated in part as a tool
  2836. 1:39:35to guide that exploration right i mean
  2837. 1:39:38that in itself i think would be a huge
  2838. 1:39:42uh you know a huge differential in the
  2839. 1:39:44way that we
  2840. 1:39:45you know our our our evolution on this
  2841. 1:39:48planet
  2842. 1:39:48yes i mean stars is that's brilliant so
  2843. 1:39:51even in that aspect but even in further
  2844. 1:39:54aspects
  2845. 1:39:55uh astronomy just shows up in basically
  2846. 1:39:59every single development in the history
  2847. 1:40:01of science up until the 20th century
  2848. 1:40:04it shows up so i wonder without that if
  2849. 1:40:06we had we would have
  2850. 1:40:08if we would even get like calculus yeah
  2851. 1:40:10look that's a great
  2852. 1:40:12i mean that's a great point newton in
  2853. 1:40:15part developed calculus
  2854. 1:40:17because he was interested in
  2855. 1:40:19understanding
  2856. 1:40:20explaining kepler's laws right in
  2857. 1:40:22general
  2858. 1:40:23that whole mechanistic understanding of
  2859. 1:40:26the night sky
  2860. 1:40:27right replacing a religious
  2861. 1:40:29understanding where you interpret
  2862. 1:40:30you know this is you know this whatever
  2863. 1:40:33fire god
  2864. 1:40:34writing his you know uh little chariot
  2865. 1:40:37across the sky
  2866. 1:40:38as opposed to you know this is some
  2867. 1:40:41mechanistic set of laws
  2868. 1:40:42that transformed humanity and arguably
  2869. 1:40:46put us
  2870. 1:40:47on the on the course that we're on today
  2871. 1:40:49right
  2872. 1:40:50the entirety of the last 400 years and
  2873. 1:40:53the development of
  2874. 1:40:54kind of our technological world that we
  2875. 1:40:57live in today
  2876. 1:40:59was sparked by by that right
  2877. 1:41:02abandoning an effectively you know a
  2878. 1:41:05non-secular
  2879. 1:41:06view of the natural world and and kind
  2880. 1:41:09of thing okay
  2881. 1:41:11this can be understood and if it can be
  2882. 1:41:14understood it can be utilized we can
  2883. 1:41:16create our own
  2884. 1:41:17uh variants of this absolutely we would
  2885. 1:41:20be a very very different species
  2886. 1:41:22without astronomy this i think extends
  2887. 1:41:26beyond just astronomy right there there
  2888. 1:41:29are questions
  2889. 1:41:30like why do we need to spend money on
  2890. 1:41:33x right where x can be anything like
  2891. 1:41:37paleontology like right uh the mating
  2892. 1:41:40patterns of uh penguins yeah that's like
  2893. 1:41:44essential that's right um i think
  2894. 1:41:47you know there's a tremendous uh
  2895. 1:41:50underappreciation for the usefulness
  2896. 1:41:52of useless knowledge right i mean
  2897. 1:41:56uh that's brilliant i didn't come up
  2898. 1:41:58with this this was this is a little book
  2899. 1:42:00by the guy who started the institute for
  2900. 1:42:02advanced studies
  2901. 1:42:04but um you know it's
  2902. 1:42:07it's so true so much of the electronics
  2903. 1:42:10that are on this table
  2904. 1:42:11right work on maxwell's equations
  2905. 1:42:13maxwell weren't
  2906. 1:42:15wasn't sitting around in the 1800s
  2907. 1:42:17saying you know i hope one day
  2908. 1:42:19you know uh we'll make you know a couple
  2909. 1:42:22mics so
  2910. 1:42:23you know a couple uh you know a couple
  2911. 1:42:26guys can
  2912. 1:42:28have this conversation right that that
  2913. 1:42:31wasn't at no
  2914. 1:42:32at no point was that the motivation and
  2915. 1:42:34yet
  2916. 1:42:35you know it gave us the world that we
  2917. 1:42:38have today and the answer is if you
  2918. 1:42:40a purely pragmatic person if you don't
  2919. 1:42:44care at all about kind of the human
  2920. 1:42:45condition none of this
  2921. 1:42:47the answer is uh you can tax it
  2922. 1:42:50right like the useless things
  2923. 1:42:54have been have created way more capital
  2924. 1:42:58than useful things and the sad thing i
  2925. 1:43:01mean
  2926. 1:43:02first of all it's really important to
  2927. 1:43:03think about and it's
  2928. 1:43:05brilliant in the in the following
  2929. 1:43:08context
  2930. 1:43:09like neil degrasse tyson has this book
  2931. 1:43:11about the role
  2932. 1:43:12of military-based funding in the
  2933. 1:43:15development of science
  2934. 1:43:17and then so much of technological
  2935. 1:43:20breakthroughs in the 20th century
  2936. 1:43:23had to do with humans working on
  2937. 1:43:26different military things
  2938. 1:43:28and then the outcome of that had nothing
  2939. 1:43:30to do with military it had some military
  2940. 1:43:32application but
  2941. 1:43:33their impact was much much bigger than
  2942. 1:43:35the military the splitting of the atom
  2943. 1:43:38is is a kind of a canonical example of
  2944. 1:43:41this we all know the tragedy that
  2945. 1:43:43you know arises from splitting of the
  2946. 1:43:45atom and and yet you know
  2947. 1:43:47so much i mean the atom itself
  2948. 1:43:51does not care for what purpose it is
  2949. 1:43:53being split
  2950. 1:43:54so so i wonder if if we you take took
  2951. 1:43:57the same amount of funding as we used
  2952. 1:43:58for war
  2953. 1:43:59and poured it into like totally
  2954. 1:44:02seemingly
  2955. 1:44:03useless things like the mating patterns
  2956. 1:44:05of penguins
  2957. 1:44:06we would get the internet anyway i i
  2958. 1:44:08think so i think so
  2959. 1:44:10and uh you know perhaps more of the
  2960. 1:44:12internet
  2961. 1:44:13would have uh would have penguins you
  2962. 1:44:16know
  2963. 1:44:17so we're both joking but in some sense
  2964. 1:44:19like
  2965. 1:44:20i wonder it's not the the penguins
  2966. 1:44:22because penguins is more about
  2967. 1:44:24sort of biology but all useless kind of
  2968. 1:44:27tinkering and all kinds of
  2969. 1:44:29uh in all kinds of avenues
  2970. 1:44:32and also because military applications
  2971. 1:44:35are often
  2972. 1:44:36um burdened by the secrecy required
  2973. 1:44:40so it's often like so much uh
  2974. 1:44:43the openness is lacking and if we
  2975. 1:44:46learned anything from the last few
  2976. 1:44:47decades is that
  2977. 1:44:48when there's openness and science that
  2978. 1:44:51accelerates the development of science
  2979. 1:44:53that's right that's true
  2980. 1:44:55the openness of science truly
  2981. 1:44:58you know it benefits everybody the
  2982. 1:45:01notion that
  2983. 1:45:02if you know i share my science with you
  2984. 1:45:04then you're gonna catch up and like
  2985. 1:45:06know the same thing that is a
  2986. 1:45:09short-sighted viewpoint because if you
  2987. 1:45:11catch up
  2988. 1:45:12and you open you know
  2989. 1:45:15you you discover something that puts me
  2990. 1:45:17in a position to do
  2991. 1:45:19the next step right it's just so i
  2992. 1:45:22absolutely agree
  2993. 1:45:23with um with all this i mean uh
  2994. 1:45:27the kind of question of like military
  2995. 1:45:29funding versus non-military funding is
  2996. 1:45:31is obviously a complicated one but at
  2997. 1:45:34the end of the day i think we have to
  2998. 1:45:37get
  2999. 1:45:37over the notion as a society
  3000. 1:45:41that we are going to you know pay for
  3001. 1:45:44this
  3002. 1:45:45and then we will get that right that's
  3003. 1:45:48true
  3004. 1:45:48if you're buying like i don't know
  3005. 1:45:51toilet paper or something right it's
  3006. 1:45:53just not true in the intellectual
  3007. 1:45:55pursuit that's not how it works
  3008. 1:45:57and sometimes it'll fail right like
  3009. 1:46:00sometimes like
  3010. 1:46:01a huge fraction of what i do right i
  3011. 1:46:04come up with an idea
  3012. 1:46:05i think oh it's great and then i work it
  3013. 1:46:06out it's totally not great right it
  3014. 1:46:08fails immediately
  3015. 1:46:10failure is not a sign that the initial
  3016. 1:46:13pursuit
  3017. 1:46:13was worthless right failure is just part
  3018. 1:46:16of this kind of this whole exploration
  3019. 1:46:17thing and
  3020. 1:46:18we should fund more and more of this
  3021. 1:46:20exploration the variety of the
  3022. 1:46:21exploration
  3023. 1:46:22i think it was linus pauling or somebody
  3024. 1:46:25from you know that generation of
  3025. 1:46:26scientists and
  3026. 1:46:28you know a good way to have good ideas
  3027. 1:46:31is to have a lot of ideas right so
  3028. 1:46:34that's i think that's true um if you are
  3029. 1:46:38conservative in your thinking if you
  3030. 1:46:39worry about proposing something that's
  3031. 1:46:42going to fail and oh what if you know
  3032. 1:46:44like i there's no science police that's
  3033. 1:46:48going to come and arrest you for
  3034. 1:46:49proposing the wrong thing and you know
  3035. 1:46:52it's also just like why would you why
  3036. 1:46:55would you do science if you're
  3037. 1:46:57afraid of you know taking that step it'd
  3038. 1:47:01be so much better
  3039. 1:47:02to propose things that are that are
  3040. 1:47:05plausible that are interesting
  3041. 1:47:06and then for a fraction of them to be
  3042. 1:47:08wrong than to just kind of
  3043. 1:47:10you know make incremental progress all
  3044. 1:47:11your life right
  3045. 1:47:13speaking of wild ideas let me ask you
  3046. 1:47:16about
  3047. 1:47:16the thing we mentioned previously which
  3048. 1:47:18is this interstellar object a muamoa
  3049. 1:47:22could it be space junk from a distant
  3050. 1:47:25alien civilization
  3051. 1:47:27you can't immediately discount that
  3052. 1:47:30by saying absolutely it cannot
  3053. 1:47:33anything can be a space junk i mean from
  3054. 1:47:35that point of view can any of the kuiper
  3055. 1:47:37belt objects we see
  3056. 1:47:38okay you know be space beijing anything
  3057. 1:47:41on the night sky
  3058. 1:47:42can in principle be space junk and
  3059. 1:47:44kuiper belt would catch interstellar
  3060. 1:47:46objects potentially and like
  3061. 1:47:48force them into an orbit if they're like
  3062. 1:47:50small enough uh not the kuiper belt
  3063. 1:47:52itself but you can imagine like jupiter
  3064. 1:47:54family comets
  3065. 1:47:55being captured uh you know so so you can
  3066. 1:47:58actually capture things
  3067. 1:48:00it's even easier to do this very early
  3068. 1:48:03in the solar system
  3069. 1:48:04like early in the solar system's life
  3070. 1:48:05while it's still in a cluster of stars
  3071. 1:48:08um it's unavoidable that you
  3072. 1:48:11capture debris whether it be natural
  3073. 1:48:14debris or
  3074. 1:48:15unnatural debris or just debris of some
  3075. 1:48:17kind from
  3076. 1:48:18other stars that it's like a daycare
  3077. 1:48:21center
  3078. 1:48:22right like everybody passes their
  3079. 1:48:23infections on to other kids yeah
  3080. 1:48:26um you know or more and more there's
  3081. 1:48:28been a lot of discussion
  3082. 1:48:29about and there's been a lot of interest
  3083. 1:48:31in this over like is it is it
  3084. 1:48:33aliens or is it not but let's like if
  3085. 1:48:35you just kind of look at the facts
  3086. 1:48:37like what we know about it is it's kind
  3087. 1:48:39of like a weird shape
  3088. 1:48:41and it also accelerated yeah right like
  3089. 1:48:44that's the two those are those are the
  3090. 1:48:47two interesting
  3091. 1:48:48uh things about it there are
  3092. 1:48:52um there are puzzles about it and
  3093. 1:48:56perhaps the most uh daring resolution
  3094. 1:49:00to this puzzle is that it's not you know
  3095. 1:49:03aliens or it's not like a rock it's
  3096. 1:49:06actually a piece of hydrogen ice
  3097. 1:49:08so this is a friend of mine you know
  3098. 1:49:11daryl seligman greg laughlin came up
  3099. 1:49:13with this uh
  3100. 1:49:15idea where that in
  3101. 1:49:18giant molecular clouds that are just
  3102. 1:49:20clouds of hydrogen helium gas that
  3103. 1:49:22live in live throughout the galaxy
  3104. 1:49:26at their cores you can condense ice
  3105. 1:49:29to become these hydrogen you know
  3106. 1:49:32icebergs if you will and then
  3107. 1:49:34uh that explains many of the aspects of
  3108. 1:49:38uh in fact i think that explains all of
  3109. 1:49:41the
  3110. 1:49:42mystery how it becomes elongated because
  3111. 1:49:46basically the hydrogen ice sublimates
  3112. 1:49:48and kind of like a bar of soap
  3113. 1:49:50that you know slowly kind of elongates
  3114. 1:49:53as you
  3115. 1:49:53uh as you strip away the the surface
  3116. 1:49:57layers
  3117. 1:49:58uh how it was able to accelerate because
  3118. 1:50:01of a jet that is produced from
  3119. 1:50:02you know the hydrogen coming off of it
  3120. 1:50:04but you can't see it because it's
  3121. 1:50:05hydrogen gas like all of this stuff
  3122. 1:50:07uh kind of falls together nicely
  3123. 1:50:12i'm i'm intrigued by that idea truly
  3124. 1:50:14because
  3125. 1:50:15it's like if that's true that's a new
  3126. 1:50:18type of astrophysical
  3127. 1:50:20object and it would be produced by
  3128. 1:50:23what's the monster that produced
  3129. 1:50:25initially that kind of object
  3130. 1:50:27so this is giant molecular molecular
  3131. 1:50:28clouds they're everywhere
  3132. 1:50:30i mean they are the fact that they exist
  3133. 1:50:33is not are they rogue clouds or are they
  3134. 1:50:36part of like an
  3135. 1:50:36oort cloud no no they're not so clouds
  3136. 1:50:39yeah they're just floating about
  3137. 1:50:40yeah so if you go like a lot of people
  3138. 1:50:42imagine the galaxy
  3139. 1:50:44as being a you know a bunch of stars
  3140. 1:50:48right and they're just orbiting right
  3141. 1:50:50but the truth is if you fly between
  3142. 1:50:52stars you run into clouds uh they don't
  3143. 1:50:55have any large
  3144. 1:50:56object that creates orbits they're just
  3145. 1:50:58floating about just floating
  3146. 1:50:59but why are they floating together oh
  3147. 1:51:01they just flowed together for time and
  3148. 1:51:03not
  3149. 1:51:03well so these are the these eventually
  3150. 1:51:06become the nurseries of stars
  3151. 1:51:08so as they as they cool they contract
  3152. 1:51:11and uh you know then collapse into stars
  3153. 1:51:14or into
  3154. 1:51:15groups of stars but some of them they
  3155. 1:51:17the starless
  3156. 1:51:20molecular clouds according to the
  3157. 1:51:23calculations that daryl and greg
  3158. 1:51:25did can uh can create these like
  3159. 1:51:28icicles of hydrogen ice i wonder why
  3160. 1:51:31they would be flying so fast because
  3161. 1:51:34they seem to be
  3162. 1:51:34moving pretty fast
  3163. 1:51:38that's just because of the acceleration
  3164. 1:51:39due to uh due to the sun
  3165. 1:51:41if you stop i mean it's like
  3166. 1:51:44take something really far away let it go
  3167. 1:51:46and the sun is here
  3168. 1:51:48by the time it comes close to the sun
  3169. 1:51:50right it's moving pretty fast
  3170. 1:51:52so that's an attractive explanation i
  3171. 1:51:55think
  3172. 1:51:56not so much because uh it's cool but it
  3173. 1:51:58makes a clear prediction
  3174. 1:52:00right of when their rubin
  3175. 1:52:03observatory comes online next year or so
  3176. 1:52:06we will discover many many more of these
  3177. 1:52:09objects
  3178. 1:52:10right and they have um so i like i like
  3179. 1:52:14theories that are falsifiable right not
  3180. 1:52:17not just testable but falsifiable it's
  3181. 1:52:19good to have a falsifiable theory where
  3182. 1:52:21you can say that's not true
  3183. 1:52:23uh aliens is one that's
  3184. 1:52:26fundamentally difficult to say no that's
  3185. 1:52:29not aliens
  3186. 1:52:30the interesting thing to me if you look
  3187. 1:52:32at one alien civilization
  3188. 1:52:35and then we look at the things it
  3189. 1:52:36produces in terms of if we were to try
  3190. 1:52:38to detect
  3191. 1:52:39the alien civilization the
  3192. 1:52:43there's like uh say there's 10 billion
  3193. 1:52:46aliens there would probably be
  3194. 1:52:52trillions of dumb drone type things
  3195. 1:52:56produced by the aliens and then be many
  3196. 1:52:59many many
  3197. 1:53:00more orders of magnitude of junk
  3198. 1:53:04so like if you were to look for an alien
  3199. 1:53:06civilization in my mind
  3200. 1:53:07you would be looking for the junk that's
  3201. 1:53:09the more efficient thing to look for
  3202. 1:53:12so i'm not saying has any
  3203. 1:53:15characteristics of space junk but
  3204. 1:53:16it kind of opened my eyes like to the
  3205. 1:53:19idea that
  3206. 1:53:20we shouldn't necessarily be looking to
  3207. 1:53:22the queen
  3208. 1:53:23of the ant colony we should be looking
  3209. 1:53:26at i don't know
  3210. 1:53:27i don't know like the traces of alien
  3211. 1:53:30life that
  3212. 1:53:31doesn't look intelligent in any way may
  3213. 1:53:33not even look like
  3214. 1:53:34life it could be just garbage we should
  3215. 1:53:36be looking for
  3216. 1:53:37garbage just generically
  3217. 1:53:41garbage that's producible by uh
  3218. 1:53:44unnatural
  3219. 1:53:45uh forces i mean for me at least that
  3220. 1:53:48was kind of interesting because
  3221. 1:53:49if you have a successful alien
  3222. 1:53:51civilization
  3223. 1:53:52that we will be producing many more
  3224. 1:53:54orders and magnitude of junk and that'll
  3225. 1:53:56be
  3226. 1:53:56easier potentially to detect well so you
  3227. 1:53:59have to produce the junk but you have to
  3228. 1:54:00also lunch
  3229. 1:54:01launch it so this is the this is where i
  3230. 1:54:04mean
  3231. 1:54:04let's let's imagine disposal yeah but
  3232. 1:54:07let's imagine we are a successful
  3233. 1:54:10civilization that
  3234. 1:54:11you know has made it to space we clearly
  3235. 1:54:13have right um
  3236. 1:54:15and yes we're in the infancy of that
  3237. 1:54:17pursuit but
  3238. 1:54:18you know we've launched i don't know how
  3239. 1:54:20many satellites
  3240. 1:54:22um probably if you count
  3241. 1:54:25gps satellites it must be at least
  3242. 1:54:28thousands
  3243. 1:54:28it's it's certainly thousands i don't
  3244. 1:54:30know if it's over ten thousand yeah but
  3245. 1:54:31it's done that
  3246. 1:54:32but it's on that like a large order of
  3247. 1:54:33magnitude how many of the things
  3248. 1:54:36that we've launched will ever leave the
  3249. 1:54:38solar system i think two
  3250. 1:54:41two well maybe the voyager the voyager
  3251. 1:54:43one voyager two i don't know if the
  3252. 1:54:45pioneer
  3253. 1:54:46so maybe three like oh there's also a
  3254. 1:54:49tesla roadster out there
  3255. 1:54:51uh that that one it will never leave the
  3256. 1:54:53solar system it'll just
  3257. 1:54:54i think that one will eventually collide
  3258. 1:54:56with mars that can be
  3259. 1:54:58spacex's first mars destination
  3260. 1:55:01um but look so there's an energetic cost
  3261. 1:55:05to interstellar travel uh which is
  3262. 1:55:08really hard to overcome
  3263. 1:55:09and when when we think about you know
  3264. 1:55:11generically
  3265. 1:55:12what do we look for in an alien
  3266. 1:55:14civilization oftentimes we tend to
  3267. 1:55:16imagine that the
  3268. 1:55:17thing you look for is the thing that
  3269. 1:55:19we're doing right now
  3270. 1:55:21yeah right so i think that um you know
  3271. 1:55:24if i if i look at the future right i
  3272. 1:55:26mean for a while like
  3273. 1:55:28okay if aliens are are out there they
  3274. 1:55:30must be broadcasting and radio
  3275. 1:55:32right that radio um
  3276. 1:55:35you know the amount that we broadcast in
  3277. 1:55:37radio has
  3278. 1:55:38diminished tremendously in the last 50
  3279. 1:55:41years
  3280. 1:55:42but we're doing a lot more computation
  3281. 1:55:46right what are the signs of computation
  3282. 1:55:49like that's a good
  3283. 1:55:50that's an interesting question to ask
  3284. 1:55:51right
  3285. 1:55:53where i don't know i think something on
  3286. 1:55:55the order of a few percent
  3287. 1:55:56of the entire electrical grid last year
  3288. 1:56:00went
  3289. 1:56:00to mining bitcoin right uh you know well
  3290. 1:56:04yeah the there could be a lot of in the
  3291. 1:56:07future different consequences of the
  3292. 1:56:09computation which
  3293. 1:56:10i mean by unbiased but it could be
  3294. 1:56:12robotics it could be artificial
  3295. 1:56:14intelligence so we may be looking for
  3296. 1:56:18intelligent looking objects like that's
  3297. 1:56:21what i meant by probes like things that
  3298. 1:56:23move
  3299. 1:56:23in kind of artificial ways but the
  3300. 1:56:25emergence of ai is not an if
  3301. 1:56:28right it's it's happening
  3302. 1:56:31right in front of our eyes and the
  3303. 1:56:33energetic costs associated
  3304. 1:56:35with that are becoming you know a
  3305. 1:56:38tangible problem
  3306. 1:56:39so i think you know if you imagine kind
  3307. 1:56:42of extrapolating that into the future
  3308. 1:56:44right what are the you know
  3309. 1:56:48what becomes the bottleneck right the
  3310. 1:56:50bottleneck might be
  3311. 1:56:53powering you know powering the broadly
  3312. 1:56:56speaking not
  3313. 1:56:56one air but powering that entire ai
  3314. 1:56:59ecosystem
  3315. 1:57:00right so i don't know i think
  3316. 1:57:03you know space junk isn't is kind of
  3317. 1:57:07uh it's an interesting idea but it's
  3318. 1:57:09heavily influenced by like sci-fi of
  3319. 1:57:111950s where
  3320. 1:57:12by 2020 we're all like flying to the
  3321. 1:57:15moon
  3322. 1:57:16um and so we produce a lot of space junk
  3323. 1:57:19i'm not
  3324. 1:57:21sure if that's the pathway that alien
  3325. 1:57:23civilizations take
  3326. 1:57:25i've also never seen an alien
  3327. 1:57:27civilization that's that's
  3328. 1:57:28true but if your theory of chill
  3329. 1:57:33turns out to be true and then we don't
  3330. 1:57:35you know we don't necessarily
  3331. 1:57:36explore we seize the exploration phase
  3332. 1:57:39of uh
  3333. 1:57:40like alien civilizations quickly sees
  3334. 1:57:42the exploration phase of their
  3335. 1:57:45um of their efforts then uh
  3336. 1:57:48then perhaps they'll just be chilling in
  3337. 1:57:50a particular space
  3338. 1:57:52expanding slowly but then using up a lot
  3339. 1:57:55of resources and then have to have a lot
  3340. 1:57:56of garbage disposal that
  3341. 1:57:58sends stuff out and the other you know
  3342. 1:58:01the other idea was that it could be a
  3343. 1:58:03relay
  3344. 1:58:04that uh you almost have like these gps
  3345. 1:58:08like markers these
  3346. 1:58:09sent throughout which i think is kind of
  3347. 1:58:11interesting it's uh similar to this
  3348. 1:58:13probe idea
  3349. 1:58:14of sending a large number of probes out
  3350. 1:58:19to measure gravitational um
  3351. 1:58:23to to to measure basically yeah the the
  3352. 1:58:26gravitational field
  3353. 1:58:27essentially i mean a lot of people at
  3354. 1:58:29cal tech and mit are
  3355. 1:58:31trying to measure gravitational fields
  3356. 1:58:32and there's there's a lot of ideas of
  3357. 1:58:35sending
  3358. 1:58:36uh stuff out there that
  3359. 1:58:40accurately measures those gravitational
  3360. 1:58:41fields uh to
  3361. 1:58:43have a greater understanding of the
  3362. 1:58:45early universe
  3363. 1:58:46but then you might realize that
  3364. 1:58:48communication through gravitation
  3365. 1:58:50through gravity is actually much more
  3366. 1:58:52effective than than radio waves for
  3367. 1:58:54example
  3368. 1:58:55something like that and then you send
  3369. 1:58:56out
  3370. 1:58:58i mean okay if you're an alien
  3371. 1:58:59civilization that's able to
  3372. 1:59:02have gigantic masses like basically
  3373. 1:59:06we're getting there as a as a
  3374. 1:59:08civilization no we're not not even close
  3375. 1:59:10well i mean yeah okay
  3376. 1:59:14i i mean like be able to sort of uh play
  3377. 1:59:16with black holes that kind of thing so
  3378. 1:59:18we're talking about a whole nother diff
  3379. 1:59:20order of magnitude and masses then it
  3380. 1:59:23may be very effective to send signals
  3381. 1:59:25via gravitational waves
  3382. 1:59:26i actually my sense is that all of these
  3383. 1:59:29things are
  3384. 1:59:30genuinely difficult to predict you know
  3385. 1:59:33and i don't mean like to to kind of shy
  3386. 1:59:35away i just i really mean if you think
  3387. 1:59:37if you take um imagination of what the
  3388. 1:59:41future
  3389. 1:59:42looked like from you know 500 years ago
  3390. 1:59:46right it's just it is so hard to
  3391. 1:59:48conceive
  3392. 1:59:49of the impossible right so um
  3393. 1:59:52[Music]
  3394. 1:59:53it's it's almost like um you know it's
  3395. 1:59:56almost limiting to try and imagine
  3396. 1:59:58things that are an order of magnitude uh
  3397. 2:00:01you know or two orders of magnitude
  3398. 2:00:02ahead in terms of progress
  3399. 2:00:04just because you know you mentioned cars
  3400. 2:00:07before
  3401. 2:00:08you know if you were to ask people what
  3402. 2:00:10they wanted
  3403. 2:00:11in 1870 is faster buggies
  3404. 2:00:14right so um so i think the whole like
  3405. 2:00:18kind of
  3406. 2:00:19you know alien conversation inevitably
  3407. 2:00:22gets gets limited by by our entire
  3408. 2:00:26kind of collective um astrophysical lack
  3409. 2:00:29of imagination
  3410. 2:00:31so to push back a little bit i find that
  3411. 2:00:35it's really interesting to talk about
  3412. 2:00:38these wild ideas about the future
  3413. 2:00:39whether it's aliens whether it's ai
  3414. 2:00:41with brilliant people like yourself
  3415. 2:00:44who are focused on very particular tools
  3416. 2:00:47of science we have today
  3417. 2:00:48to solve very particular like rigorous
  3418. 2:00:50scientific questions
  3419. 2:00:52and it's almost like putting on this
  3420. 2:00:54wild dreamy hat like
  3421. 2:00:55some percent of the time and say like
  3422. 2:00:57what are like what would alien
  3423. 2:00:59civilizations look like what would alien
  3424. 2:01:01trash look like well what would our own
  3425. 2:01:04civilization that sends out
  3426. 2:01:06trillions of ai systems out there like
  3427. 2:01:09hal 9000
  3428. 2:01:10but 10 000 out there what would that
  3429. 2:01:12look like and you're right
  3430. 2:01:14any one prediction is probably going to
  3431. 2:01:16be horrendously wrong
  3432. 2:01:18but there's something about creating
  3433. 2:01:19these kind of wild predictions
  3434. 2:01:21that kind of opens up there's a huge
  3435. 2:01:24magnetism to it
  3436. 2:01:26right and some of some of it um
  3437. 2:01:29you know i mean some of the jules verne
  3438. 2:01:33novels did a phenomenal job predicting
  3439. 2:01:36the future
  3440. 2:01:36right uh that that actually was a great
  3441. 2:01:39example of what you're talking about
  3442. 2:01:40like allowing your imagination to
  3443. 2:01:43run free i mean i just hope
  3444. 2:01:46i just hope there there's dragons that's
  3445. 2:01:49like
  3446. 2:01:50i love dragons yeah dragons are the best
  3447. 2:01:54but see the cool thing about science
  3448. 2:01:56fiction and these kinds of conversations
  3449. 2:01:58it doesn't just predict the future i
  3450. 2:02:00think some of these things
  3451. 2:02:02will create the future pla planting the
  3452. 2:02:06idea
  3453. 2:02:07this will help the humans are amazing
  3454. 2:02:09like fake it till you make it
  3455. 2:02:12humans are really good at uh taking an
  3456. 2:02:15idea that seems impossible at the time
  3457. 2:02:18and for one any one individual human
  3458. 2:02:20that idea
  3459. 2:02:21is like a it's like planting a seed yes
  3460. 2:02:24that eventually materializes itself
  3461. 2:02:26it's weird it's weird science fiction
  3462. 2:02:28can
  3463. 2:02:29create science drive some of it it
  3464. 2:02:31drives the science i agree with you
  3465. 2:02:33and uh and i think in this regard
  3466. 2:02:37you know i i'm like a sucker for for
  3467. 2:02:40sci-fi
  3468. 2:02:41um it's it's all i listen to like now
  3469. 2:02:45when i when i run
  3470. 2:02:46and um and some of it is completely
  3471. 2:02:49implausible
  3472. 2:02:49right and it's like i don't care it's
  3473. 2:02:52it's so
  3474. 2:02:53it's uh it's both entertaining
  3475. 2:02:57and uh you know it's just like it's
  3476. 2:03:00imagination
  3477. 2:03:01you know about the black clouds book i
  3478. 2:03:03think this by fred hoyle
  3479. 2:03:05this is like this has great connections
  3480. 2:03:07with sort of a lot of the advancements
  3481. 2:03:09that are happening in nlp
  3482. 2:03:11um right now right with
  3483. 2:03:14you know transformer models and so on
  3484. 2:03:15but uh you know it's this black cloud
  3485. 2:03:17shows up
  3486. 2:03:18in in the solar system and then you know
  3487. 2:03:21people try to
  3488. 2:03:22send radio and then it learns to talk
  3489. 2:03:24back at you
  3490. 2:03:25wow you know so anyway we don't have to
  3491. 2:03:27talk at all about it but it's just
  3492. 2:03:29it's something worth checking out with
  3493. 2:03:31that on the alien front with the black
  3494. 2:03:33claw to me and
  3495. 2:03:34exactly and the llp front and also just
  3496. 2:03:37explainability of ai
  3497. 2:03:38it's fascinating just a very question
  3498. 2:03:41stephen wolfram looked at this with the
  3499. 2:03:42movie arrival
  3500. 2:03:44it's like what would be the common
  3501. 2:03:45language that we would discover
  3502. 2:03:47the the reason that's really interesting
  3503. 2:03:48to me is we have aliens
  3504. 2:03:50here on earth japanese japanese is the
  3505. 2:03:53obvious answer
  3506. 2:03:54japanese yeah that would be the common
  3507. 2:03:57maybe it would be music actually
  3508. 2:03:59that's more likely it wouldn't be a
  3509. 2:04:01language it would be art
  3510. 2:04:02that they would communicate but you know
  3511. 2:04:04i i do believe that we have
  3512. 2:04:07i'm with stephen wolfram on this a
  3513. 2:04:08little bit that to me
  3514. 2:04:11computation like programs we write that
  3515. 2:04:14you know that they're kind of
  3516. 2:04:16intelligent creatures
  3517. 2:04:17and i feel like we haven't found the
  3518. 2:04:19common language to talk with them
  3519. 2:04:21like our little creations that are
  3520. 2:04:24artificial
  3521. 2:04:26are not born with the whatever that
  3522. 2:04:28innate thing that
  3523. 2:04:29produces language with us and like
  3524. 2:04:32coming up with mechanisms for
  3525. 2:04:34communicating with them
  3526. 2:04:35uh is um is an effort that feels
  3527. 2:04:40like it will produce some incredible
  3528. 2:04:41discoveries you can even think of
  3529. 2:04:43if you think that math is discovered
  3530. 2:04:46mathematics in itself
  3531. 2:04:47is a kind of um oh yeah it's an innate
  3532. 2:04:50construction
  3533. 2:04:51of of the world we live in um i think we
  3534. 2:04:54are
  3535. 2:04:56you know a part of the way there because
  3536. 2:05:00pre-1950 right
  3537. 2:05:03computers who were human beings that
  3538. 2:05:06would carry out arithmetic
  3539. 2:05:08right and i think it was ulam um
  3540. 2:05:11who worked in los alamos at the at the
  3541. 2:05:15time like towards the end
  3542. 2:05:16of the second world war wrote something
  3543. 2:05:19about
  3544. 2:05:20how you know in the future right
  3545. 2:05:22computers will not
  3546. 2:05:23be just arithmetic tool but will be
  3547. 2:05:27truly an interactive
  3548. 2:05:29you know thing with which you could
  3549. 2:05:32do experiments right at the time the
  3550. 2:05:34notion of doing an experiment
  3551. 2:05:36not like in the lab with some beakers
  3552. 2:05:39but uh
  3553. 2:05:40an experiment on a computer designing an
  3554. 2:05:42experiment
  3555. 2:05:43a numerical experiment was
  3556. 2:05:47a new one that's like you know 70
  3557. 2:05:50of what i do is i design com you know i
  3558. 2:05:53write
  3559. 2:05:53code terrible code to be uh clear like
  3560. 2:05:57but you know i write code that creates
  3561. 2:06:00an experiment which is a which is a
  3562. 2:06:03simulation
  3563. 2:06:04so in that sense i think we're beginning
  3564. 2:06:06to interact with the computer in in a
  3565. 2:06:08way that you're
  3566. 2:06:09saying not as just a you know fancy
  3567. 2:06:12calculator not as just a
  3568. 2:06:14you know call-in request type of
  3569. 2:06:18thing but but you know something that
  3570. 2:06:19can generate uh
  3571. 2:06:21generate insights that are otherwise
  3572. 2:06:24completely unattainable right they're
  3573. 2:06:26unattainable by doing
  3574. 2:06:27analytical mathematics yeah and there's
  3575. 2:06:30uh
  3576. 2:06:30like with the alpha fold two we're now
  3577. 2:06:33trying
  3578. 2:06:33we're now starting to crack open biology
  3579. 2:06:36so being able to
  3580. 2:06:37simulate at first trivial biological
  3581. 2:06:39systems and hopefully down the line
  3582. 2:06:41complex biological systems
  3583. 2:06:42right my hope is to be able to simulate
  3584. 2:06:45psychology
  3585. 2:06:46psychological like sociological systems
  3586. 2:06:48like humans
  3587. 2:06:49i've you know um a large part of my work
  3588. 2:06:52at
  3589. 2:06:53mit was on autonomous vehicles
  3590. 2:06:56and the fascinating thing to me was
  3591. 2:06:57about pedestrians
  3592. 2:07:00human pedestrians interacting with
  3593. 2:07:01autonomous vehicles and simulating those
  3594. 2:07:03systems without murdering humans
  3595. 2:07:05would be very useful but nevertheless is
  3596. 2:07:07exceptionally difficult
  3597. 2:07:08yeah i would say so when is my mustang
  3598. 2:07:10going to drive itself
  3599. 2:07:11right i'm not even joking it looks like
  3600. 2:07:15yeah yeah i it turns out it's much
  3601. 2:07:18difficult
  3602. 2:07:19it's much more difficult than we
  3603. 2:07:20imagined yeah and and i suppose that's
  3604. 2:07:22the kind of
  3605. 2:07:24the progress of science is
  3606. 2:07:28just like you know going to mars
  3607. 2:07:31it's probably going to turn out to be
  3608. 2:07:33way more difficult to imagine
  3609. 2:07:35sending out probes to investigate planet
  3610. 2:07:37nine at the edge of our solar system
  3611. 2:07:39might turn out to be way more difficult
  3612. 2:07:40than we imagined but we do it anyway
  3613. 2:07:42yeah and we figure it out in the end
  3614. 2:07:44it's actually more of a great i mean
  3615. 2:07:45going
  3616. 2:07:46sending humans to mars is way more
  3617. 2:07:49complicated than huma sending humans to
  3618. 2:07:50the moon
  3619. 2:07:51you'd think just like naively yeah both
  3620. 2:07:54are in space
  3621. 2:07:55who cares like if you go there why don't
  3622. 2:07:57you go there
  3623. 2:07:58um you know just
  3624. 2:08:01life support is uh is an extremely
  3625. 2:08:04expensive thing yeah there's a bunch of
  3626. 2:08:06extra challenges but i disagree with you
  3627. 2:08:07i would be one of the early people to go
  3628. 2:08:09i used to think not
  3629. 2:08:10yeah i used to think i'd be one of the
  3630. 2:08:12first maybe million to go once you have
  3631. 2:08:14a little bit of a society
  3632. 2:08:15i think i'm i'm upgrading myself to the
  3633. 2:08:17first like ten thousand yeah that's
  3634. 2:08:19right
  3635. 2:08:19from the front of the cabin not
  3636. 2:08:22completely front
  3637. 2:08:23but like it would be interesting to die
  3638. 2:08:25i'm okay
  3639. 2:08:26with uh death sucks
  3640. 2:08:29but i kind of like the idea of dying on
  3641. 2:08:33mars
  3642. 2:08:34of all the places to die i gotta say in
  3643. 2:08:36this regard like
  3644. 2:08:38i don't wanna die on mars i don't no no
  3645. 2:08:40i would much rather
  3646. 2:08:42die on earth uh i mean death
  3647. 2:08:46is is fundamentally boring right like
  3648. 2:08:48death is a very boring experience
  3649. 2:08:50but i mean i've never died before so i
  3650. 2:08:52don't know from first-hand experience as
  3651. 2:08:54far as you know yeah
  3652. 2:08:55it could be a reincarnation all those
  3653. 2:08:56kinds of things so you mean uh
  3654. 2:08:59where would you die uh if you had to
  3655. 2:09:02choose oh man
  3656. 2:09:05um okay so and you know i would
  3657. 2:09:08definitely
  3658. 2:09:08you know there's a question of who i'd
  3659. 2:09:10want to die with
  3660. 2:09:12you know i'd prefer not to die alone uh
  3661. 2:09:15but like
  3662. 2:09:15you know surrounded by family would be
  3663. 2:09:18uh would be preferable where i think
  3664. 2:09:22northern new mexico and i'm not even
  3665. 2:09:24joking like this is not
  3666. 2:09:26a random place it's just like would that
  3667. 2:09:28be your favorite place on earth
  3668. 2:09:31not necessarily like favorite place on
  3669. 2:09:33earth to
  3670. 2:09:35to to reside you know indefinitely but
  3671. 2:09:38it is
  3672. 2:09:39it is one of the most beautiful places
  3673. 2:09:40i've i've ever been to
  3674. 2:09:42uh so you know there's something i don't
  3675. 2:09:46know there's something attractive about
  3676. 2:09:48about going you know returning to nature
  3677. 2:09:50in a beautiful
  3678. 2:09:52uh place let me ask you about another
  3679. 2:09:56aspect of your life
  3680. 2:09:57that is full of beauty music okay you're
  3681. 2:10:00a musician
  3682. 2:10:02uh the absurd question i have to ask
  3683. 2:10:05what is the greatest song of all time oh
  3684. 2:10:07objectively speaking
  3685. 2:10:09the greatest song of all time i suppose
  3686. 2:10:11that could change
  3687. 2:10:12moment to moment day to day but if you
  3688. 2:10:14were forced to answer for this
  3689. 2:10:16particular moment in your life that's
  3690. 2:10:18something that pops to mind
  3691. 2:10:20this could be both philosophically this
  3692. 2:10:22could be technically as a musician like
  3693. 2:10:23what you enjoy
  3694. 2:10:24maybe lyrics like for me it's lyrics is
  3695. 2:10:27very important so absolutely i would
  3696. 2:10:29probably be my choice would be lyrics
  3697. 2:10:32based
  3698. 2:10:32i don't want to answer in terms of just
  3699. 2:10:34technical uh you know
  3700. 2:10:36technical prowess i think technical
  3701. 2:10:38prowess is
  3702. 2:10:40impressive right it's just like it's
  3703. 2:10:42impressive what can be done
  3704. 2:10:44i wouldn't place that into the category
  3705. 2:10:46of the greatest music ever written
  3706. 2:10:49some the classical music uh
  3707. 2:10:52that's that's written is undeniably
  3708. 2:10:54beautiful but i don't want to
  3709. 2:10:56consider that category of music
  3710. 2:10:59either uh just because you know so if i
  3711. 2:11:02if i have to
  3712. 2:11:03limit uh the scope of this
  3713. 2:11:06philosophical discussion uh to
  3714. 2:11:10you know the kind of music that i listen
  3715. 2:11:11to you know probably what's my age again
  3716. 2:11:14by blink 182. it's just you know it's a
  3717. 2:11:17solid one
  3718. 2:11:18it's got you know
  3719. 2:11:21said nobody ever that's a good song
  3720. 2:11:24i don't know if you're joking no i i i
  3721. 2:11:27am joking it's a good one but it's it
  3722. 2:11:28was
  3723. 2:11:29yeah i mean
  3724. 2:11:35what's my age you get yeah yeah no i
  3725. 2:11:38mean
  3726. 2:11:38it would probably you know
  3727. 2:11:41songwriting-wise i think the beatles
  3728. 2:11:43came
  3729. 2:11:44pretty close to the influential to you i
  3730. 2:11:46was like the beatles
  3731. 2:11:47yeah love the beatles i love the beatles
  3732. 2:11:50uh let it be yesterday yeah
  3733. 2:11:54like straw i think strawberry feels
  3734. 2:11:55forever is is one
  3735. 2:11:57you know what what one of my favorite
  3736. 2:11:58beetle songs is it's uh
  3737. 2:12:01you know in my life right that's not
  3738. 2:12:03it's it's hard to imagine
  3739. 2:12:05how whatever 24 year old
  3740. 2:12:08wrote that it is one of the most uh
  3741. 2:12:11introspective
  3742. 2:12:12pieces of music ever you know i'm a huge
  3743. 2:12:15pink floyd fan
  3744. 2:12:17and so i think you know if you were to
  3745. 2:12:20you can sort of look at the entire dark
  3746. 2:12:22side of the moon album
  3747. 2:12:23and as you know getting pretty close up
  3748. 2:12:27there to the pinnacle of what you know
  3749. 2:12:29can be
  3750. 2:12:29created so you know time's a great song
  3751. 2:12:33yeah it's a great song just the entirety
  3752. 2:12:35of
  3753. 2:12:36just the instruments the lyrics the the
  3754. 2:12:39the feeling
  3755. 2:12:40created by a song like pink floyd
  3756. 2:12:44can create feelings the entire
  3757. 2:12:47experience i mean you have that with the
  3758. 2:12:48wall
  3759. 2:12:49of just uh transporting you into another
  3760. 2:12:52place
  3761. 2:12:53songs don't not many songs could do that
  3762. 2:12:56as as
  3763. 2:12:57well not many artists can do that as
  3764. 2:12:59well as pink floyd did
  3765. 2:13:00there are a lot of bands that you can
  3766. 2:13:02kind of say oh yeah
  3767. 2:13:04like if you take blink 182 right if you
  3768. 2:13:07have
  3769. 2:13:07no idea like if you are listening to
  3770. 2:13:10sort of that type of pop punk for the
  3771. 2:13:13first time
  3772. 2:13:14it's difficult to differentiate between
  3773. 2:13:15blink 182 and like some 41
  3774. 2:13:18and the thousand of other like
  3775. 2:13:21lesser known bands that all sounded the
  3776. 2:13:23whole they all had that sparkling
  3777. 2:13:25production
  3778. 2:13:26uh feel they all kind of sounded the
  3779. 2:13:28same
  3780. 2:13:30right when with pink floyd
  3781. 2:13:33it's hard to find another band that
  3782. 2:13:35you're like well is this one
  3783. 2:13:37pink floor like you know yeah when
  3784. 2:13:40you're listening to that
  3785. 2:13:41what you're listening to that the
  3786. 2:13:43uniqueness that that's fascinating
  3787. 2:13:45you know in the calculation of the
  3788. 2:13:47greatest
  3789. 2:13:48song in the greatest band of all time
  3790. 2:13:51you could probably
  3791. 2:13:52you probably actually quantify this like
  3792. 2:13:54scientifically is like
  3793. 2:13:56how unique uh if you play different
  3794. 2:13:59songs how well are people
  3795. 2:14:00able to recognize whether it's this band
  3796. 2:14:02or not and that you know that's
  3797. 2:14:05probably a huge component to greatness
  3798. 2:14:07like if the world would miss it if it
  3799. 2:14:09was gone
  3800. 2:14:10yes yes so but there's also the human
  3801. 2:14:14story things like i would say output
  3802. 2:14:16johnny cash's cover of hurt as one of
  3803. 2:14:19the greatest songs of all time
  3804. 2:14:21and that has less to do with the song
  3805. 2:14:24but your interaction with the
  3806. 2:14:26interaction with it but also the human
  3807. 2:14:27the full story of the human
  3808. 2:14:29so like it's not just if i just heard
  3809. 2:14:31the song it'd be like okay
  3810. 2:14:33that but if it it's the full story of it
  3811. 2:14:36also the video component for that
  3812. 2:14:38particular song
  3813. 2:14:40so like that you can't discount the full
  3814. 2:14:42experience of it
  3815. 2:14:43absolutely you know i have no confusion
  3816. 2:14:45about not
  3817. 2:14:47about being you know anywhere uh
  3818. 2:14:51you know in in that league but i just
  3819. 2:14:54like i
  3820. 2:14:54sometimes think about you know music
  3821. 2:14:56that is being
  3822. 2:14:58uh produced today feels
  3823. 2:15:02oftentimes feels like like kind of
  3824. 2:15:04clothes like clothes that you buy
  3825. 2:15:06at like h m and you wear three times
  3826. 2:15:10before they rip and you throw away so
  3827. 2:15:12like so much of it is
  3828. 2:15:15it's not bad it's just kind of
  3829. 2:15:16forgettable right
  3830. 2:15:18like the fact that we're talking about
  3831. 2:15:20pink floyd
  3832. 2:15:21in 2021 is in itself an interesting
  3833. 2:15:25uh question why are we talking about
  3834. 2:15:27pink floyd and it's there's something
  3835. 2:15:28unforgettable about them and
  3836. 2:15:30unforgettable about the the art that
  3837. 2:15:33they created
  3838. 2:15:34that could be the markets that like so
  3839. 2:15:36spotify has created this kind of
  3840. 2:15:37market where the the
  3841. 2:15:41incentives for creating music that last
  3842. 2:15:43is much lower because there's so much
  3843. 2:15:45more music right you just want something
  3844. 2:15:47that shines bright for a short amount of
  3845. 2:15:49time
  3846. 2:15:50makes a lot of money and moves on and i
  3847. 2:15:52mean the same thing you see with the
  3848. 2:15:53news and all those kinds of things we're
  3849. 2:15:54just living in a
  3850. 2:15:56shorter and shorter shorter like uh time
  3851. 2:15:59scale in terms of our attention spans
  3852. 2:16:01and that um nevertheless when we look at
  3853. 2:16:05the long arc of history of music perhaps
  3854. 2:16:06there will be some songs from today
  3855. 2:16:09that will last as much as pink floyd
  3856. 2:16:11we're just unable to see it
  3857. 2:16:13yeah just the collected works of
  3858. 2:16:14nickelback
  3859. 2:16:16exactly you know you never know you
  3860. 2:16:18never know justin bieber
  3861. 2:16:19it could have yeah he could be a
  3862. 2:16:21contender i've recently started
  3863. 2:16:22listening to justin bieber just
  3864. 2:16:23understand what people are talking about
  3865. 2:16:24and
  3866. 2:16:25you know i'll just keep my comments to
  3867. 2:16:26myself on that one it's too good to
  3868. 2:16:28explain
  3869. 2:16:29in the words we're not
  3870. 2:16:32the greatness that is the biebs uh you
  3871. 2:16:35as a musician
  3872. 2:16:37so you uh you write your own music you
  3873. 2:16:40uh play guitar
  3874. 2:16:41you sing um maybe can you
  3875. 2:16:44give an overview of the role music is
  3876. 2:16:47played in your life you're
  3877. 2:16:49one of the you're a world-class
  3878. 2:16:51scientist
  3879. 2:16:52and so it's kind of fascinating to see
  3880. 2:16:55somebody
  3881. 2:16:58in your position who's also a great
  3882. 2:17:00musician and
  3883. 2:17:01and and uh still loves playing music
  3884. 2:17:04yeah well i wouldn't call myself a great
  3885. 2:17:06musician
  3886. 2:17:06like you know one of the best of all
  3887. 2:17:08time yeah
  3888. 2:17:11that's right like we were saying offline
  3889. 2:17:13confidence is like the most essential
  3890. 2:17:15thing about that's right
  3891. 2:17:16exactly it's the confidence and kind of
  3892. 2:17:18like
  3893. 2:17:19moodiness right yeah um yeah look i mean
  3894. 2:17:22music plays an absolutely
  3895. 2:17:26essential role in in everything i do
  3896. 2:17:29because
  3897. 2:17:30i lose if i stop playing for
  3898. 2:17:33one reason or another say i'm traveling
  3899. 2:17:36i notably
  3900. 2:17:36lose creativity in every other aspect of
  3901. 2:17:39my life
  3902. 2:17:40right there's something i don't
  3903. 2:17:44view you know playing music as a
  3904. 2:17:47separate endeavor from doing science or
  3905. 2:17:49doing doing whatever it's all
  3906. 2:17:51it's all part of that same creative
  3907. 2:17:53thing
  3908. 2:17:54which is distinct from i don't know
  3909. 2:17:58uh pressing a button or like you know so
  3910. 2:18:02it's not a break from science it's
  3911. 2:18:04a part of your science it's absolutely a
  3912. 2:18:06it's a part of
  3913. 2:18:07it's it's i would say you know it's a
  3914. 2:18:10thing that enables
  3915. 2:18:12the science right the science would you
  3916. 2:18:14know
  3917. 2:18:15suck even more than it does already uh
  3918. 2:18:18without the music
  3919. 2:18:19and that means like the creating of the
  3920. 2:18:20the writing of the music or is it just
  3921. 2:18:22even playing other people's stuff is it
  3922. 2:18:24is it all of it yeah it's it's
  3923. 2:18:26definitely both
  3924. 2:18:28um yeah and also just you know
  3925. 2:18:31i love i love to play guitar i love to
  3926. 2:18:35sing you know
  3927. 2:18:36my wife tolerates my uh
  3928. 2:18:40my screeching singing you know and uh
  3929. 2:18:42even kind of likes it
  3930. 2:18:44so yeah so people should check out your
  3931. 2:18:46stuff you have a great voice so i i love
  3932. 2:18:48your stuff
  3933. 2:18:49um is there something you're you're
  3934. 2:18:51super busy
  3935. 2:18:53is there something you could say about
  3936. 2:18:55practicing
  3937. 2:18:57uh for musicians for guitar for you're
  3938. 2:18:59also in a band
  3939. 2:19:00so like that whole how you can manage
  3940. 2:19:03that is there some tricks or
  3941. 2:19:04some hacks to um being a lifelong
  3942. 2:19:08musician
  3943. 2:19:08while being like super busy so i would
  3944. 2:19:11say
  3945. 2:19:12you know the way that i optimize
  3946. 2:19:15um my life is i try to i try to do
  3947. 2:19:19you know the thing that i'm passionate
  3948. 2:19:20about in a moment
  3949. 2:19:22um and put that at the top of the
  3950. 2:19:24priority list there are moments when
  3951. 2:19:27you know you just you feel inspired to
  3952. 2:19:29play music and if you're in the middle
  3953. 2:19:31of something if you can avoid
  3954. 2:19:32if that can be put on hold just do it
  3955. 2:19:35right there are times when you
  3956. 2:19:36get inspired about something scientific
  3957. 2:19:39um
  3958. 2:19:40you know i do my best to drop
  3959. 2:19:43everything go into that you know mode of
  3960. 2:19:46that isolated mode
  3961. 2:19:48and and execute upon that so
  3962. 2:19:51it's a chaotic you know i think i have a
  3963. 2:19:54pretty chaotic lifestyle
  3964. 2:19:55where i'm always doing kind of multiple
  3965. 2:19:58things and jumping between uh
  3966. 2:20:02between what i'm doing but at the end of
  3967. 2:20:04the day
  3968. 2:20:05it's it's not like um
  3969. 2:20:08you know those those moments of
  3970. 2:20:10inspiration
  3971. 2:20:12are actually kind of rare right like
  3972. 2:20:14most of the time
  3973. 2:20:16all of us are just doing kind of uh
  3974. 2:20:19doing the stuff that get that needs to
  3975. 2:20:21get done if you
  3976. 2:20:24do the disservice to yourself of saying
  3977. 2:20:26oh i'm inspired to
  3978. 2:20:28you know do this calculation figure it
  3979. 2:20:30figure this out
  3980. 2:20:31but i've got to answer email or just
  3981. 2:20:33like do something
  3982. 2:20:34something silly um you know that is a
  3983. 2:20:38um that is nothing more than the service
  3984. 2:20:40and also
  3985. 2:20:41like i have some social media presence
  3986. 2:20:44but i i mostly stay off of you know
  3987. 2:20:48social media
  3988. 2:20:50to you know just frankly because like i
  3989. 2:20:53don't kind of
  3990. 2:20:54i don't enjoy the mental cycles that it
  3991. 2:20:56uh yeah it robs you of that
  3992. 2:20:59the yeah yeah those those precious
  3993. 2:21:01moments
  3994. 2:21:02that could be filled with inspiration in
  3995. 2:21:05your in your other pursuits
  3996. 2:21:07um but there's something to maybe you
  3997. 2:21:10and i are different this like i i try to
  3998. 2:21:12play at least 10 minutes of guitar every
  3999. 2:21:14day
  4000. 2:21:16like almost on the technical side like
  4001. 2:21:20keeping that bass uh of
  4002. 2:21:24of basic competence going and
  4003. 2:21:27i mean the same way like writers will
  4004. 2:21:29get in front of a paper no matter what
  4005. 2:21:31that kind of thing it just feels like
  4006. 2:21:34that
  4007. 2:21:35for my life has been essential to to to
  4008. 2:21:38the daily ritual of it otherwise days
  4009. 2:21:41turn into weeks weeks or into months and
  4010. 2:21:43you haven't played guitar for
  4011. 2:21:44months no no i i i understand for me
  4012. 2:21:48i think it's it's been like if we have a
  4013. 2:21:51gig coming up
  4014. 2:21:52we'll definitely yeah that's right no
  4015. 2:21:55like we
  4016. 2:21:55we will uh we will sharpen up uh
  4017. 2:21:59definitely you know especially co coming
  4018. 2:22:02up to again it's like
  4019. 2:22:03you know we're not trying to make money
  4020. 2:22:06with this this is like just
  4021. 2:22:07for the uh for that satisfaction of
  4022. 2:22:11doing something doing something well
  4023. 2:22:13right um but overall
  4024. 2:22:17i would say most i play guitar most days
  4025. 2:22:22most days and you know when i put kids
  4026. 2:22:25to sleep
  4027. 2:22:25i i play guitar you know with them and
  4028. 2:22:28we like
  4029. 2:22:29just make up random songs about you know
  4030. 2:22:33about her a cat or something you know
  4031. 2:22:35like we just
  4032. 2:22:36do kind of random stuff but you know
  4033. 2:22:39music is always involved in that process
  4034. 2:22:41yeah keeping it fun you have russian
  4035. 2:22:43roots i sure do
  4036. 2:22:45were you born in russia i was yeah when
  4037. 2:22:47did you come here
  4038. 2:22:49so i came to the us in
  4039. 2:22:53very the very end of 99 but um
  4040. 2:22:56so i was like almost 14 years old
  4041. 2:22:59but along the way we spent six years in
  4042. 2:23:02japan so like we moved
  4043. 2:23:04from russia to japan in 94
  4044. 2:23:07and then to the us in 99 so like
  4045. 2:23:10elementary school
  4046. 2:23:12all interesting school in japan so
  4047. 2:23:14elementary school in japan
  4048. 2:23:16yeah so that's interesting that do you
  4049. 2:23:19still speak russian
  4050. 2:23:20sure okay
  4051. 2:23:23okay maybe i'll uh let me ask you in
  4052. 2:23:26russian
  4053. 2:23:30um
  4054. 2:23:37[Music]
  4055. 2:23:58is
  4056. 2:24:26is
  4057. 2:24:28[Laughter]
  4058. 2:24:29so for people who don't speak russian
  4059. 2:24:31constantine was uh
  4060. 2:24:32talking about basically his first in
  4061. 2:24:361992 interaction with capitalism
  4062. 2:24:39which is pepsi and at first he
  4063. 2:24:41discovered pepsi and then he discovered
  4064. 2:24:43coke and he was confused how such
  4065. 2:24:45uh how such theft could occur
  4066. 2:24:48like an intellectual property theft and
  4067. 2:24:50remember pepsi
  4068. 2:24:52arrived to the soviet union first and
  4069. 2:24:55there's some
  4070. 2:24:56there's some complicated story which i
  4071. 2:24:58don't uh
  4072. 2:24:59quite understand the details of for a
  4073. 2:25:01while pepsi
  4074. 2:25:02like commanded submarines or something
  4075. 2:25:06yeah pepsi had like a fleet of soviet
  4076. 2:25:08submarines that
  4077. 2:25:09did they were sponsoring tanks and
  4078. 2:25:12this fascinating yeah and i and i
  4079. 2:25:14remember there's certain things that
  4080. 2:25:15trickled in like mcdonald's i remember
  4081. 2:25:17that was a big deal
  4082. 2:25:18oh yeah certainly for the west
  4083. 2:25:20absolutely so i mean we went to
  4084. 2:25:22mcdonald's
  4085. 2:25:23and we stood on i mean this is this is
  4086. 2:25:26absurd
  4087. 2:25:27right from kind of looking at it from
  4088. 2:25:29today's
  4089. 2:25:31perspective but we stood in line for
  4090. 2:25:33like six hours to get into this
  4091. 2:25:34mcdonald's
  4092. 2:25:35and i remember inside i was just like
  4093. 2:25:39a billion people and i'm just taking a
  4094. 2:25:42bite
  4095. 2:25:42out of that big mac like wow
  4096. 2:25:46what was it an incredible experience for
  4097. 2:25:48you so like
  4098. 2:25:50what is this taste of the west like uh
  4099. 2:25:52did you enjoy it
  4100. 2:25:53i enjoyed the fact that i mean this is
  4101. 2:25:57like
  4102. 2:25:57i was getting into the weeds but i
  4103. 2:25:59really enjoyed
  4104. 2:26:00the fact that the top of the bun had
  4105. 2:26:02those seeds you know like
  4106. 2:26:04and i remember how on the commercials
  4107. 2:26:06like the
  4108. 2:26:07big mac would kind of bounce i was like
  4109. 2:26:09the seeds how did they inject the seeds
  4110. 2:26:11into the bread like
  4111. 2:26:14amazing right so i think it was uh
  4112. 2:26:17artistry yeah you enjoyed the artistry
  4113. 2:26:20of the culinary
  4114. 2:26:21exactly it was the you know it was the
  4115. 2:26:23food art that kind of that is the big
  4116. 2:26:25mac
  4117. 2:26:25actually i still don't know the answer
  4118. 2:26:27to that how do they get the sesame seeds
  4119. 2:26:28on the better to not know the answer
  4120. 2:26:31you just wander at the mystery of it all
  4121. 2:26:33yeah i remember it being exceptionally
  4122. 2:26:34delicious but i
  4123. 2:26:35i'm with you i don't know you didn't
  4124. 2:26:39mention how transformative pepsi was but
  4125. 2:26:41to me basically sugar-based stuff
  4126. 2:26:44like like pepsi was uh or a coke i don't
  4127. 2:26:47remember which one we partook in but
  4128. 2:26:49that was an incredible experience yeah
  4129. 2:26:51yeah
  4130. 2:26:51yeah yeah no absolutely and uh
  4131. 2:26:54you know i think it's um
  4132. 2:26:58you know it was an important and and
  4133. 2:27:00formative uh formative period
  4134. 2:27:04i sometimes i guess rely on that a
  4135. 2:27:06little bit
  4136. 2:27:07uh you know in my daily life because uh
  4137. 2:27:10i remember like the early 90s were real
  4138. 2:27:14rough you know like my
  4139. 2:27:16parents were kind of on the on the
  4140. 2:27:19bottom
  4141. 2:27:19of the spectrum in terms of uh
  4142. 2:27:22you know in terms of financial
  4143. 2:27:25well-being so
  4144. 2:27:27um kind of like just when i
  4145. 2:27:31run into trouble not like you know
  4146. 2:27:34money trouble just any kind of trouble
  4147. 2:27:36these days it just kind of
  4148. 2:27:38is not uh particularly meaningful
  4149. 2:27:41when you compare it to that that
  4150. 2:27:43turbulent time of the
  4151. 2:27:44early 90s and the other thing is i think
  4152. 2:27:47there's there's like an advantage
  4153. 2:27:49to to being you know an immigrant which
  4154. 2:27:52is that
  4155. 2:27:53you get you go through the mental
  4156. 2:27:55exercise
  4157. 2:27:56of changing your environment completely
  4158. 2:27:59early in your life right you go
  4159. 2:28:02it's by no means you know pleasant in
  4160. 2:28:04the moment right but like going
  4161. 2:28:07into japanese elementary school right
  4162. 2:28:08like i didn't go to a
  4163. 2:28:11some like private you know
  4164. 2:28:14thing i just went to a regular like
  4165. 2:28:16japanese public elementary school and i
  4166. 2:28:18was the
  4167. 2:28:19non-japanese person in my class
  4168. 2:28:22so just like the learning japanese and
  4169. 2:28:24just kind of
  4170. 2:28:26so that's a super humbling experience in
  4171. 2:28:28many ways was when you like made fun of
  4172. 2:28:30all that kind of stuff oh
  4173. 2:28:31yeah being the outsider oh absolutely
  4174. 2:28:34but
  4175. 2:28:34you know you kind of do you kind of do
  4176. 2:28:37that
  4177. 2:28:37and then you kind of then you just
  4178. 2:28:41kind of are okay with with stuff you
  4179. 2:28:43know what i mean and so
  4180. 2:28:44like doing that again in middle school
  4181. 2:28:46in the us
  4182. 2:28:47it was arguably easy because i was like
  4183. 2:28:51yeah well i've already done this before
  4184. 2:28:53so
  4185. 2:28:54i think it kind of prepares you mentally
  4186. 2:28:56a little bit for
  4187. 2:28:57for switching up for whatever you know
  4188. 2:28:59changes that will come up for the rest
  4189. 2:29:01of
  4190. 2:29:01your life so i um i wouldn't trade
  4191. 2:29:05that that experience really for anything
  4192. 2:29:08it's a huge aspect of who i am and i'm
  4193. 2:29:11sure
  4194. 2:29:12you can relate to a lot of this yes is
  4195. 2:29:15there advice
  4196. 2:29:16from your life that you can give to
  4197. 2:29:18young people today
  4198. 2:29:20high school college you know about their
  4199. 2:29:23career
  4200. 2:29:24or maybe about life in general i'm not
  4201. 2:29:27like
  4202. 2:29:27a career coach but i like that's right
  4203. 2:29:30like i'm definitely not a life coach i
  4204. 2:29:32don't have it all figured out
  4205. 2:29:33but i think there's a um
  4206. 2:29:36there's a perpetual cycle of of
  4207. 2:29:40um you know thinking that
  4208. 2:29:43there is a um there's kind of like a
  4209. 2:29:45template for success
  4210. 2:29:48right maybe there is but i in my
  4211. 2:29:51experience i haven't seen it right um
  4212. 2:29:56you know i would say people in high
  4213. 2:29:58school
  4214. 2:29:59right so much of their focus
  4215. 2:30:02is on getting straight a's filling their
  4216. 2:30:05cv
  4217. 2:30:06with this and this and this so that it
  4218. 2:30:08looks impressive
  4219. 2:30:09right um that that is
  4220. 2:30:13not i think a good way to optimize your
  4221. 2:30:16life
  4222. 2:30:16right do the thing that fills your life
  4223. 2:30:19with passion
  4224. 2:30:20do the thing that fills your life with
  4225. 2:30:22with interest
  4226. 2:30:24and you know do that perpetually right
  4227. 2:30:28a straight a student you know
  4228. 2:30:31is really impressive but also you know
  4229. 2:30:34somewhat boring right so so i i think
  4230. 2:30:38you know injection of
  4231. 2:30:39more of that kind of um
  4232. 2:30:42interest into into the lives of young
  4233. 2:30:44people would go a long way
  4234. 2:30:46in in just both upping their level of
  4235. 2:30:49happiness
  4236. 2:30:50and then just kind of ensuring that
  4237. 2:30:53looking forward they are not suffering
  4238. 2:30:56from a
  4239. 2:30:57can you know perpetual condition of oh i
  4240. 2:30:59have to satisfy these like you know
  4241. 2:31:01check boxes
  4242. 2:31:02to to do well right because you can lose
  4243. 2:31:05yourself in that whole process for the
  4244. 2:31:06rest of your life
  4245. 2:31:07but it's nice if it's possible like max
  4246. 2:31:10tegmark was exceptionally good at this
  4247. 2:31:12at mit figure out how you can spend a
  4248. 2:31:14small
  4249. 2:31:15part of your percent of your efforts
  4250. 2:31:18that such that your cv looks really
  4251. 2:31:20impressive
  4252. 2:31:22yeah absolutely there's no like without
  4253. 2:31:25a doubt
  4254. 2:31:26like that's that's a baseline that you
  4255. 2:31:28need to have
  4256. 2:31:29um and then so like spend most of your
  4257. 2:31:33time doing like amazing things you're
  4258. 2:31:34passionate about
  4259. 2:31:35but such that it uh uh kind of like
  4260. 2:31:38planet nine produces
  4261. 2:31:40objects that uh that feed your cv
  4262. 2:31:43uh like slowly over time so getting good
  4263. 2:31:45grades in high school maybe doing
  4264. 2:31:47extracurricular activities
  4265. 2:31:48or or in terms of like you know for
  4266. 2:31:51programmers that's producing code that
  4267. 2:31:53you can show up on github
  4268. 2:31:54like leaving traces like um
  4269. 2:31:58throughout your efforts such that your
  4270. 2:32:00cv looks impressive to the rest of the
  4271. 2:32:02world
  4272. 2:32:02in fact i mean this is somewhat along
  4273. 2:32:05the lines of what i'm talking about
  4274. 2:32:07we see like getting like good grades is
  4275. 2:32:10important but
  4276. 2:32:10grades are not a tangible like product
  4277. 2:32:14like you cannot out you know show your
  4278. 2:32:17a and and have your a live a separate
  4279. 2:32:19life from you
  4280. 2:32:21code very much does right um music
  4281. 2:32:24very much takes on you know provided
  4282. 2:32:27somebody else listens to it right
  4283. 2:32:29right provide like takes on a life of
  4284. 2:32:32its own
  4285. 2:32:32that's kind of what i mean right doing
  4286. 2:32:36doing stuff that uh that can then
  4287. 2:32:40get separated from from you is is
  4288. 2:32:43exceptionally attractive right it's like
  4289. 2:32:45a it's like a fun
  4290. 2:32:47and uh and it's also very impressive to
  4291. 2:32:49others i think we're moving to a world
  4292. 2:32:51where grades mean less and less
  4293. 2:32:53like certifications mean less and less
  4294. 2:32:55if you look at
  4295. 2:32:56especially again in the computing fields
  4296. 2:32:58getting a degree
  4297. 2:32:59finishing your um currently just getting
  4298. 2:33:03finishing your degree whether it's
  4299. 2:33:04bachelor's or master's a phd
  4300. 2:33:07is less important than the things you've
  4301. 2:33:08actually put out into the world
  4302. 2:33:10right right and that's a fascinating
  4303. 2:33:12kind of that's a that's great that
  4304. 2:33:13in that sense the meritocracy is in its
  4305. 2:33:17richest most beautiful form is is
  4306. 2:33:19starting to win out
  4307. 2:33:20yeah it's weird because like you know my
  4308. 2:33:23understanding
  4309. 2:33:24and i'm not like i don't know the
  4310. 2:33:26history of science well enough to
  4311. 2:33:28to speak very confidently about this but
  4312. 2:33:30you know the
  4313. 2:33:32advisor of my advisor of my advisor
  4314. 2:33:36from undergrad uh like didn't have a phd
  4315. 2:33:39right so i think it was a more common
  4316. 2:33:41thing back in the day
  4317. 2:33:43even in uh the academic
  4318. 2:33:46sector to you know
  4319. 2:33:50not have you know faraday like faraday
  4320. 2:33:53didn't know algebra
  4321. 2:33:54when drew diagrams about you know
  4322. 2:33:57magnetic fields like
  4323. 2:33:58his faraday's law was derived entirely
  4324. 2:34:02from intuition
  4325. 2:34:03so uh it is interesting to to how
  4326. 2:34:07the world of academia has evolved into a
  4327. 2:34:10you got to do this and then get phd then
  4328. 2:34:13you have to post doc once and twice
  4329. 2:34:15and maybe thrice and then like you you
  4330. 2:34:18move on so
  4331. 2:34:19you know it does i do wonder you know if
  4332. 2:34:21we're
  4333. 2:34:23you know if there's a better i think
  4334. 2:34:25we're heading there
  4335. 2:34:26but it's a fascinating historical
  4336. 2:34:28perspective like that we might have just
  4337. 2:34:30tried this whole thing out uh for a
  4338. 2:34:32while where we put a lot more emphasis
  4339. 2:34:34on grades and certificates and
  4340. 2:34:35um degrees and all those kinds of things
  4341. 2:34:38i think the difference
  4342. 2:34:39historically is like we can actually
  4343. 2:34:42using the internet show off the
  4344. 2:34:46show off ourselves and our creations
  4345. 2:34:48better and better and more effectively
  4346. 2:34:50whether that's code or producing videos
  4347. 2:34:52or all those kinds of things that's
  4348. 2:34:54right
  4349. 2:34:54you can become a certified drone pilot
  4350. 2:34:59that's true of all the of all the things
  4351. 2:35:01you want to pick yeah for sure
  4352. 2:35:03or you could just fly make youtube
  4353. 2:35:04videos against hundreds of thousands of
  4354. 2:35:06views with your drone and
  4355. 2:35:07never getting a certificate um that's
  4356. 2:35:10probably illegal don't do it
  4357. 2:35:11what do you think is uh the meaning of
  4358. 2:35:13this whole thing so
  4359. 2:35:14you look at planets they they seem to
  4360. 2:35:18orbit stuff
  4361. 2:35:19um without without asking the why
  4362. 2:35:22question and
  4363. 2:35:23for some reason life emerged on earth
  4364. 2:35:25such that it led to big brains that
  4365. 2:35:27can ask the big why question do you
  4366. 2:35:30think there's an answer to it
  4367. 2:35:33um i'm not sure what the question is
  4368. 2:35:36like what meaning of life the meaning of
  4369. 2:35:38life um
  4370. 2:35:40it's 42. it's 42. yeah but
  4371. 2:35:43you know aside from that it's um you
  4372. 2:35:46know
  4373. 2:35:47why i think if the question you're
  4374. 2:35:50asking is like
  4375. 2:35:51why we do all this right
  4376. 2:35:55yeah um it's part of the human condition
  4377. 2:35:59right human beings are fundamentally
  4378. 2:36:04i feel like non like sort of stochastic
  4379. 2:36:08and fundamentally interested in in
  4380. 2:36:14kind of expanding our own understanding
  4381. 2:36:16of the world
  4382. 2:36:17around us and creating stuff to enable
  4383. 2:36:20that understanding
  4384. 2:36:21so we're like a stochastic
  4385. 2:36:22fundamentalist so like there's
  4386. 2:36:24just a bunch of randomness that really
  4387. 2:36:26doesn't seem like it has a good
  4388. 2:36:27explanation
  4389. 2:36:28and yet there's a kind of direction to
  4390. 2:36:31our being that we just keep wanting to
  4391. 2:36:33create and to understand
  4392. 2:36:34that's right i've met people that are
  4393. 2:36:36you know that claim to be anti-science
  4394. 2:36:39right um and yet
  4395. 2:36:42in their anti-science you know
  4396. 2:36:44discussion
  4397. 2:36:45like well like if you're so
  4398. 2:36:48you know scientific then how why don't
  4399. 2:36:51you explain to me how
  4400. 2:36:52i don't know this works and like it
  4401. 2:36:54always there's that fundamental
  4402. 2:36:57speed of curiosity and interest that is
  4403. 2:37:00common to
  4404. 2:37:01to all of us that is absolutely what
  4405. 2:37:04makes us
  4406. 2:37:06human right and and i
  4407. 2:37:09i'm in a privileged position of being
  4408. 2:37:11able to you know
  4409. 2:37:13to have that be my my job
  4410. 2:37:16right i think as uh you know as time
  4411. 2:37:20evolves forward you know when the kind
  4412. 2:37:23of
  4413. 2:37:23economy changes i mean we're already
  4414. 2:37:26starting to see
  4415. 2:37:27you know shift towards that type of you
  4416. 2:37:30know
  4417. 2:37:31creative uh you know enterprise as being
  4418. 2:37:34as emerging as taking over a bigger and
  4419. 2:37:36bigger chunk of the
  4420. 2:37:38sector it's not yet i think the dominant
  4421. 2:37:41uh portion of the economy by any account
  4422. 2:37:45but if we compare
  4423. 2:37:46this to like you know sometime when
  4424. 2:37:49the dominant thing you would do would be
  4425. 2:37:52to
  4426. 2:37:52you know go to a factory and do the same
  4427. 2:37:55exact thing
  4428. 2:37:56right i think you know there's a tide
  4429. 2:37:59there
  4430. 2:38:00and things are sort of headed in that
  4431. 2:38:02direction yeah life's becoming more and
  4432. 2:38:03more fun i can't wait
  4433. 2:38:05uh honestly what i can't wait to just
  4434. 2:38:07chill just just chill
  4435. 2:38:09terminal point of this chill and wait
  4436. 2:38:12for those kuiper belt objects to
  4437. 2:38:13complete one orbit
  4438. 2:38:14i'm gonna credit you with this idea uh i
  4439. 2:38:17do hope that
  4440. 2:38:18we definitively discover uh proof
  4441. 2:38:22that there is a planet nine out there in
  4442. 2:38:23the next few years so you can sit back
  4443. 2:38:25with a cigar a cigarette or vodka or
  4444. 2:38:28wine and
  4445. 2:38:29just uh say i told you so that's already
  4446. 2:38:32happening
  4447. 2:38:33i'm gonna do that later tonight as i
  4448. 2:38:36mentioned uh
  4449. 2:38:37confidence is essential to being a rock
  4450. 2:38:39star i really appreciate you uh
  4451. 2:38:42explaining so many fascinating things to
  4452. 2:38:44me today i really appreciate the work
  4453. 2:38:46that you do out there
  4454. 2:38:47and um i really appreciate you talking
  4455. 2:38:50with me today
  4456. 2:38:50thank you pleasure thanks for having me
  4457. 2:38:52on thanks for listening to this
  4458. 2:38:54conversation with constantine
  4459. 2:38:56botegan and thank you to squarespace
  4460. 2:38:59literati
  4461. 2:39:00onit and and i check them out in the
  4462. 2:39:03description
  4463. 2:39:04to support this podcast and now let me
  4464. 2:39:06leave you with some words from douglas
  4465. 2:39:08adams
  4466. 2:39:08in the hitchhiker's guide to the galaxy
  4467. 2:39:12far out in the uncharted backwaters of
  4468. 2:39:14the
  4469. 2:39:15unfashionable end of the western spiral
  4470. 2:39:18arm
  4471. 2:39:18of the galaxy lies a small unregarded
  4472. 2:39:22yellow sun
  4473. 2:39:23orbiting this at a distance of roughly
  4474. 2:39:2692 million miles
  4475. 2:39:28is an utterly insignificant little blue
  4476. 2:39:30green planet
  4477. 2:39:31whose ape descendant life forms are so
  4478. 2:39:34amazingly primitive
  4479. 2:39:36that they still think digital watches
  4480. 2:39:38are a pretty neat
  4481. 2:39:40idea thank you for listening and hope to
  4482. 2:39:43see you
  4483. 2:39:43next time
  4484. 2:39:53you

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