1 00:00:00,000 --> 00:00:02,583 (serene music) 2 00:00:05,813 --> 00:00:08,359 - Welcome to another episode of E.Z. Science, 3 00:00:08,359 --> 00:00:11,230 I'm Ellen Stofan, the John and Adrienne Mars 4 00:00:11,230 --> 00:00:13,160 Director of the Smithsonian's National 5 00:00:13,160 --> 00:00:16,170 Air and Space museum, or Dr. E. 6 00:00:16,170 --> 00:00:17,600 - And I'm Thomas Zurbuchen, the associate 7 00:00:17,600 --> 00:00:19,800 administrator for science at NASA, 8 00:00:19,800 --> 00:00:21,670 also referred to as Dr. Z. 9 00:00:21,670 --> 00:00:23,881 - We're here today to talk about a subject that's 10 00:00:23,881 --> 00:00:26,264 pretty near and dear to my heart, 11 00:00:26,264 --> 00:00:29,067 and that's the Hubble Space Telescope. 12 00:00:29,067 --> 00:00:32,812 You can see behind us, the structural dynamic test vehicle 13 00:00:32,812 --> 00:00:35,120 of Hubble and off to the side here, 14 00:00:35,120 --> 00:00:37,780 at the National Air and Space Museum, we have some 15 00:00:37,780 --> 00:00:40,350 of the instruments that were actually brought back 16 00:00:40,350 --> 00:00:42,350 from Hubble, the ones that weren't working so well, 17 00:00:42,350 --> 00:00:44,790 they had to put new instruments up on board, 18 00:00:44,790 --> 00:00:47,480 so if you haven't been here before, come and see this 19 00:00:47,480 --> 00:00:49,250 amazing history of Hubble. 20 00:00:49,250 --> 00:00:51,750 - To me this is one of the real highlights in the museum, 21 00:00:51,750 --> 00:00:54,840 and kind of every time I'm here I'm standing I'm in awe. 22 00:00:54,840 --> 00:00:58,512 So first of all, this mission is what I would consider 23 00:00:58,512 --> 00:01:01,580 the most important discovery machine we've ever done. 24 00:01:01,580 --> 00:01:04,720 If you look at that mission, last year alone, there 25 00:01:04,720 --> 00:01:08,130 are close to a thousand new publications written, 26 00:01:08,130 --> 00:01:10,510 it's not just a science mission, it's a science mission 27 00:01:10,510 --> 00:01:13,730 enabled by human exaperations, by astronauts. 28 00:01:13,730 --> 00:01:15,260 - [Dr. E] The fact that the astronauts were able 29 00:01:15,260 --> 00:01:17,990 to go up in shuttle and replace the instruments, 30 00:01:17,990 --> 00:01:20,432 constantly putting better, more advanced instrumentation 31 00:01:20,432 --> 00:01:24,210 on board, has really allowed Hubble over its twenty-nine 32 00:01:24,210 --> 00:01:28,300 years to completely change our view of the universe. 33 00:01:28,300 --> 00:01:31,800 - So there's a story that was out there about a planet 34 00:01:31,800 --> 00:01:34,770 called 'K2-18B' 35 00:01:34,770 --> 00:01:36,260 and here's a question regard with 36 00:01:36,260 --> 00:01:38,707 the hashtag 'E.Z. Science', and it said 37 00:01:38,707 --> 00:01:42,319 "Hubble just found water vapor on an exoplanet, 38 00:01:42,319 --> 00:01:46,953 in a habitable zone, what does that mean for other planets?" 39 00:01:46,953 --> 00:01:50,470 - So recently some scientists actually discovered water 40 00:01:50,470 --> 00:01:52,880 vapor in the atmosphere of this planet. 41 00:01:52,880 --> 00:01:57,170 We now have over four thousand planets around other stars 42 00:01:57,170 --> 00:02:00,073 that have been detected, a lot of them are very large, 43 00:02:00,073 --> 00:02:03,106 so we're not really thinking about those as sort of 44 00:02:03,106 --> 00:02:06,542 Earth 2.0. a place where we could go to look for life. 45 00:02:06,542 --> 00:02:09,400 But the intriguing thing is, we're pretty sure water 46 00:02:09,400 --> 00:02:12,020 is critical to life, life here on Earth evolved 47 00:02:12,020 --> 00:02:14,620 in the ocean so when we go out and look at planets 48 00:02:14,620 --> 00:02:17,490 around other stars, we're looking for that blue planet, 49 00:02:17,490 --> 00:02:20,671 that ocean planet like the Earth, so the fact that we found 50 00:02:20,671 --> 00:02:25,470 water vapor, was exciting but unfortunately not sufficient 51 00:02:25,470 --> 00:02:28,460 because habitability is a complicated thing. 52 00:02:28,460 --> 00:02:31,693 - Yeah, so found water here, a water vapor but, 53 00:02:31,693 --> 00:02:35,050 there's many questions we have about for example: 54 00:02:35,050 --> 00:02:39,200 Do these planets magnetic protections layers like our Earth? 55 00:02:39,200 --> 00:02:42,637 Is the surface actually solid, or would you just sink in? 56 00:02:42,637 --> 00:02:45,710 Like if something is a gaseous type of planet, there's 57 00:02:45,710 --> 00:02:47,860 many, many questions so we're just at the 58 00:02:47,860 --> 00:02:50,090 beginning of that journey. 59 00:02:50,090 --> 00:02:52,101 - That's right and when you look at our own solar system, 60 00:02:52,101 --> 00:02:55,182 obviously the earth is habitable, it's been habitable 61 00:02:55,182 --> 00:02:57,839 for hundred of millions of years, and yet if you look 62 00:02:57,839 --> 00:03:01,870 at Venus or Mars, Mars was habitable for a very small 63 00:03:01,870 --> 00:03:04,600 portion of its history and a lot of us feel strongly 64 00:03:04,600 --> 00:03:06,533 that there could be evidence of past life on Mars. 65 00:03:06,533 --> 00:03:10,910 Venus was maybe habitable for a very short time in its 66 00:03:10,910 --> 00:03:13,591 history and as early in Earth's history, this planet 67 00:03:13,591 --> 00:03:16,550 was not habitable and as our solar system evolves, 68 00:03:16,550 --> 00:03:20,000 Earth will become no longer habitable so you have to 69 00:03:20,000 --> 00:03:23,540 think of habitability as not just a condition but 70 00:03:23,540 --> 00:03:27,112 actually a phase that a planet could potentially go through. 71 00:03:27,112 --> 00:03:29,710 - What we have done with the exoplanets is we've, 72 00:03:29,710 --> 00:03:31,970 using Kepler, looked at one part of the 73 00:03:31,970 --> 00:03:34,330 sky and just stared at it. 74 00:03:34,330 --> 00:03:37,499 And from that we managed to do a tally of exoplanets, 75 00:03:37,499 --> 00:03:40,175 so we know that for every star at least, there's one 76 00:03:40,175 --> 00:03:43,566 exoplanet out there, most of those exoplanets 77 00:03:43,566 --> 00:03:45,800 live in systems just like we do. 78 00:03:45,800 --> 00:03:49,170 There's other planets in our solar system, 79 00:03:49,170 --> 00:03:53,300 what we're now doing with TESS is we're looking at 80 00:03:53,300 --> 00:03:57,153 the entire sky, to really find the closest such things 81 00:03:57,153 --> 00:03:59,835 to investigate and like you said, 82 00:03:59,835 --> 00:04:03,040 there's very little we know about this. 83 00:04:03,040 --> 00:04:06,720 It's very critical to be able to follow up with 84 00:04:06,720 --> 00:04:10,290 telescopes like this one, the Hubble Space Telescope 85 00:04:10,290 --> 00:04:12,144 but also James Webb that's coming out in 86 00:04:12,144 --> 00:04:14,490 just a couple of years out there. 87 00:04:14,490 --> 00:04:16,963 - We're incredibly excited about the James Webb telescope 88 00:04:16,963 --> 00:04:20,550 because if you think of TESS, Kepler, Hubble, 89 00:04:20,550 --> 00:04:23,170 finding these exoplanets and getting a little bit 90 00:04:23,170 --> 00:04:25,480 of information, James Webb is really gonna be 91 00:04:25,480 --> 00:04:27,679 able to takes us to the next level. 92 00:04:27,679 --> 00:04:30,033 - What's really amazing about Webb, is when 93 00:04:30,033 --> 00:04:32,991 Webb was conceived early on, exoplanets 94 00:04:32,991 --> 00:04:35,300 were kind of a side story. 95 00:04:35,300 --> 00:04:38,120 Right now, it's one of the key stories because 96 00:04:38,120 --> 00:04:40,077 we discovered this abundance of exoplanets 97 00:04:40,077 --> 00:04:43,183 and we have an abundance of questions, many, many 98 00:04:43,183 --> 00:04:46,400 questions that we didn't know how to ask before. 99 00:04:46,400 --> 00:04:48,510 - So what the Webb telescope can do, is it can look at 100 00:04:48,510 --> 00:04:50,452 much higher resolution of the atmospheres of some of 101 00:04:50,452 --> 00:04:52,384 these planets around other stars. 102 00:04:52,384 --> 00:04:55,188 Not just looking for water vapor, but also gasses like 103 00:04:55,188 --> 00:04:59,710 carbon dioxide, methane and it's these combinations 104 00:04:59,710 --> 00:05:01,640 of gasses that we're looking for. 105 00:05:01,640 --> 00:05:05,600 The presence of water vapor isn't sufficient for life, 106 00:05:05,600 --> 00:05:08,232 but if you see a mixture of gasses and especially if those 107 00:05:08,232 --> 00:05:11,940 gasses seem to be out of equilibrium, or there's something 108 00:05:11,940 --> 00:05:14,710 causing an imbalance in the gasses, chemically and the 109 00:05:14,710 --> 00:05:17,480 atmosphere, that starts to make us think, 110 00:05:17,480 --> 00:05:20,280 not only could that planet be habitable, 111 00:05:20,280 --> 00:05:22,890 but is it actually inhabited. 112 00:05:22,890 --> 00:05:25,580 When I started out as a planetary scientist, you know, 113 00:05:25,580 --> 00:05:28,130 there were nine planets and then because of the 114 00:05:28,130 --> 00:05:30,214 declassification of Pluto we went down to eight, 115 00:05:30,214 --> 00:05:34,150 but for kids who are students now, by the time they're 116 00:05:34,150 --> 00:05:36,410 ready to become planetary scientists, which of course 117 00:05:36,410 --> 00:05:38,010 they're all gonna do, they are gonna be 118 00:05:38,010 --> 00:05:40,870 thousands of planets for them to study. 119 00:05:40,870 --> 00:05:42,720 And we got another questions on E.Z. 120 00:05:42,720 --> 00:05:45,523 Science it's asking about TESS, 121 00:05:45,523 --> 00:05:48,930 "What is the transiting exo-planet survey satellite? 122 00:05:48,930 --> 00:05:50,425 How does that actually work?" 123 00:05:50,425 --> 00:05:53,270 - What the TESS mission is doing, it's looking in a large 124 00:05:53,270 --> 00:05:57,426 part of the sky and it's staring at it and as it's staring, 125 00:05:57,426 --> 00:06:00,980 it's looking at the stability of light, so every 126 00:06:00,980 --> 00:06:04,000 once in a while, one of those exoplanets is 127 00:06:04,000 --> 00:06:07,640 going right in front of the star that it's around, 128 00:06:07,640 --> 00:06:10,280 and when it does so it every so faintly, 129 00:06:10,280 --> 00:06:13,858 reduces the light of that star, creating 130 00:06:13,858 --> 00:06:16,790 a transient feature and so that's what 131 00:06:16,790 --> 00:06:20,590 we're observing for all those stars, in that part of the sky 132 00:06:20,590 --> 00:06:22,077 that TESS is looking at. 133 00:06:22,077 --> 00:06:26,650 - And we can then use, how the light has dimmed 134 00:06:26,650 --> 00:06:29,290 to say what's the size of that planet, 135 00:06:29,290 --> 00:06:31,274 what kind of orbit it's in, which really helps us then 136 00:06:31,274 --> 00:06:33,858 start to nail down which of these planets are more like 137 00:06:33,858 --> 00:06:36,500 Earth, which ones are more like Jupiter, we're just 138 00:06:36,500 --> 00:06:38,500 about out of time, I'm sorry to say, thank you 139 00:06:38,500 --> 00:06:40,656 for joining us for another episode of E.Z. Science. 140 00:06:40,656 --> 00:06:42,982 - And please keep sending those questions, 141 00:06:42,982 --> 00:06:46,100 with hashtag 'E.Z. Science' so we can answer them