1 00:00:05,349 --> 00:00:03,030 there's a planet in our galaxy that 2 00:00:07,510 --> 00:00:05,359 scientists are really excited about in 3 00:00:10,070 --> 00:00:07,520 fact it's the closest earth-sized planet 4 00:00:12,310 --> 00:00:10,080 outside our solar system it's probably 5 00:00:14,629 --> 00:00:12,320 rocky and could have liquid water 6 00:00:16,710 --> 00:00:14,639 flowing on its surface an essential 7 00:00:19,189 --> 00:00:16,720 ingredient for life 8 00:00:21,269 --> 00:00:19,199 there's only one problem 9 00:00:27,429 --> 00:00:21,279 we can't actually see it and it's 10 00:00:32,950 --> 00:00:29,910 to get to proxima centauri b it would 11 00:00:35,430 --> 00:00:32,960 take a spacecraft over 75 000 years to 12 00:00:37,590 --> 00:00:35,440 travel there with today's technology 13 00:00:39,910 --> 00:00:37,600 even powerful ground-based telescopes 14 00:00:41,590 --> 00:00:39,920 can't see the planet in any detail 15 00:00:43,350 --> 00:00:41,600 mostly because it's being drowned out by 16 00:00:45,270 --> 00:00:43,360 the light of its star 17 00:00:47,270 --> 00:00:45,280 this raises the question 18 00:00:49,520 --> 00:00:47,280 how do we investigate a planet that you 19 00:00:54,069 --> 00:00:49,530 can't see and you can't get to 20 00:00:57,990 --> 00:00:55,910 this supercomputer is tasked with 21 00:01:00,709 --> 00:00:58,000 running sophisticated climate models to 22 00:01:03,510 --> 00:01:00,719 predict earth's future climate it's loud 23 00:01:06,630 --> 00:01:03,520 you can feel air rushing by you can feel 24 00:01:08,149 --> 00:01:06,640 a hum in the room it feels powerful it's 25 00:01:09,109 --> 00:01:08,159 one of the most powerful supercomputers 26 00:01:11,270 --> 00:01:09,119 in the world 27 00:01:12,789 --> 00:01:11,280 and now it might be scientists only hope 28 00:01:14,870 --> 00:01:12,799 for discovering whether any of these 29 00:01:17,830 --> 00:01:14,880 newly discovered planets could possibly 30 00:01:22,070 --> 00:01:20,230 last year a team at nasa goddard 31 00:01:25,510 --> 00:01:22,080 institute for space studies in new york 32 00:01:27,350 --> 00:01:25,520 city decided to investigate further 33 00:01:29,510 --> 00:01:27,360 what happens when you take a possibly 34 00:01:31,990 --> 00:01:29,520 rocky planet situated in its solar 35 00:01:34,310 --> 00:01:32,000 system's habitable zone and simulate 36 00:01:36,310 --> 00:01:34,320 hypothetical climates based on the only 37 00:01:37,270 --> 00:01:36,320 planet we know of with life 38 00:01:39,510 --> 00:01:37,280 earth 39 00:01:41,670 --> 00:01:39,520 we only know basic details about proxima 40 00:01:44,069 --> 00:01:41,680 centauri b its size 41 00:01:46,710 --> 00:01:44,079 mass distance from its star and the type 42 00:01:49,030 --> 00:01:46,720 of star it orbits and that's it 43 00:01:50,310 --> 00:01:49,040 right out of the gate proxima b has some 44 00:01:52,789 --> 00:01:50,320 problems 45 00:01:57,510 --> 00:01:52,799 it's 20 times closer to its star proxima 46 00:02:01,109 --> 00:01:58,789 this means that it's likely 47 00:02:03,109 --> 00:02:01,119 gravitationally locked to it just like 48 00:02:05,190 --> 00:02:03,119 the moon is gravitationally locked to 49 00:02:08,070 --> 00:02:05,200 the earth 50 00:02:11,110 --> 00:02:08,080 as a result one side of proxima b always 51 00:02:12,949 --> 00:02:11,120 faces its sun's intense radiation while 52 00:02:14,790 --> 00:02:12,959 the other freezes in the darkness of 53 00:02:16,949 --> 00:02:14,800 space 54 00:02:19,589 --> 00:02:16,959 but slap on a hypothetical atmosphere on 55 00:02:25,370 --> 00:02:19,599 the planet and fill it with an ocean and 56 00:02:25,380 --> 00:02:32,550 [Music] 57 00:02:32,560 --> 00:02:38,550 here's where this gets interesting 58 00:02:42,309 --> 00:02:39,990 we're looking at the side of proxima 59 00:02:44,630 --> 00:02:42,319 centauri b that's facing its star so 60 00:02:46,869 --> 00:02:44,640 it's the warmer side 61 00:02:48,949 --> 00:02:46,879 in the simulation the modelers gave the 62 00:02:50,790 --> 00:02:48,959 planet a global ocean 63 00:02:52,790 --> 00:02:50,800 the ocean circulates heat around the 64 00:02:55,270 --> 00:02:52,800 planet through ocean currents that are 65 00:02:57,670 --> 00:02:55,280 produced by the planet's rotation just 66 00:02:59,670 --> 00:02:57,680 as we see on earth 67 00:03:01,509 --> 00:02:59,680 the ocean current actually carries warm 68 00:03:05,030 --> 00:03:01,519 water to the side of the planet without 69 00:03:06,869 --> 00:03:05,040 starlight and up towards the poles 70 00:03:09,190 --> 00:03:06,879 this creates a characteristic pattern of 71 00:03:12,149 --> 00:03:09,200 ice-covered ocean similar to our own 72 00:03:14,149 --> 00:03:12,159 north pole versus ice-free ocean 73 00:03:17,270 --> 00:03:14,159 a pattern we would see on any rotating 74 00:03:19,750 --> 00:03:17,280 ocean-covered planet 75 00:03:21,750 --> 00:03:19,760 in this simulation modelers use earth's 76 00:03:23,509 --> 00:03:21,760 continents as a stand-in to predict what 77 00:03:25,350 --> 00:03:23,519 would happen if most of the land was on 78 00:03:27,110 --> 00:03:25,360 the side of the planet facing away from 79 00:03:29,270 --> 00:03:27,120 its star 80 00:03:31,190 --> 00:03:29,280 how much land might be covered in ice 81 00:03:35,280 --> 00:03:31,200 and how might ocean currents interact 82 00:03:37,430 --> 00:03:35,290 with land masses when transferring heat 83 00:03:39,670 --> 00:03:37,440 [Music] 84 00:03:41,589 --> 00:03:39,680 conversely if most of the continents 85 00:03:43,350 --> 00:03:41,599 face the warmth of its star 86 00:03:45,910 --> 00:03:43,360 how much incoming radiation would 87 00:03:47,270 --> 00:03:45,920 actually be absorbed by the ocean and 88 00:03:51,509 --> 00:03:47,280 how could this affect the planet's 89 00:03:54,229 --> 00:03:53,190 so those are some of the tricks we play 90 00:03:56,949 --> 00:03:54,239 we give it different kinds of 91 00:03:58,550 --> 00:03:56,959 atmospheres and see how the planet 92 00:04:00,070 --> 00:03:58,560 responds the climate response to that 93 00:04:01,670 --> 00:04:00,080 because we really want the planet to be 94 00:04:03,110 --> 00:04:01,680 in in what we call the habitable zone 95 00:04:08,470 --> 00:04:03,120 where it would have liquid water on its 96 00:04:11,990 --> 00:04:10,550 scientists are finding these exoplanets 97 00:04:14,789 --> 00:04:12,000 could actually have ingredients to 98 00:04:16,870 --> 00:04:14,799 support life under a range of surprising 99 00:04:18,710 --> 00:04:16,880 conditions compared to earth 100 00:04:20,789 --> 00:04:18,720 is it possible that our notions of what 101 00:04:21,990 --> 00:04:20,799 make a planet suitable for life are too 102 00:04:23,990 --> 00:04:22,000 limiting 103 00:04:25,590 --> 00:04:24,000 had alien civilizations pointed their 104 00:04:27,830 --> 00:04:25,600 telescopes towards earth billions of 105 00:04:29,749 --> 00:04:27,840 years ago expecting to find a blue 106 00:04:31,749 --> 00:04:29,759 planet swimming in oxygen they would 107 00:04:33,749 --> 00:04:31,759 have found a much different world we 108 00:04:35,110 --> 00:04:33,759 definitely look at earth through time we 109 00:04:37,350 --> 00:04:35,120 might try different topographies 110 00:04:39,030 --> 00:04:37,360 different land sea masks for example 111 00:04:40,469 --> 00:04:39,040 you know the topography we have today on 112 00:04:42,550 --> 00:04:40,479 earth is not the topography earth had 113 00:04:44,310 --> 00:04:42,560 250 million years ago 114 00:04:46,710 --> 00:04:44,320 with money and time both limited 115 00:04:48,469 --> 00:04:46,720 resources scientists are looking for the 116 00:04:49,990 --> 00:04:48,479 most promising planets to point their 117 00:04:52,629 --> 00:04:50,000 observatories at 118 00:04:54,629 --> 00:04:52,639 proxima centauri b may offer a blueprint