0:00:00.960,0:00:04.072 I'm here to tell you[br]about the real search for alien life. 0:00:04.675,0:00:07.906 Not little green humanoids[br]arriving in shiny UFOs, 0:00:07.930,0:00:09.654 although that would be nice. 0:00:09.678,0:00:12.955 But it's the search for planets[br]orbiting stars far away. 0:00:13.924,0:00:15.759 Every star in our sky is a sun. 0:00:15.783,0:00:17.164 And if our sun has planets -- 0:00:17.188,0:00:19.685 Mercury, Venus, Earth, Mars, etc., 0:00:19.709,0:00:22.145 surely those other stars[br]should have planets also, 0:00:22.169,0:00:23.431 and they do. 0:00:23.455,0:00:24.867 And in the last two decades, 0:00:24.891,0:00:27.788 astronomers have found[br]thousands of exoplanets. 0:00:28.502,0:00:31.313 Our night sky is literally[br]teeming with exoplanets. 0:00:31.337,0:00:32.889 We know, statistically speaking, 0:00:32.913,0:00:35.406 that every star has at least one planet. 0:00:35.984,0:00:37.961 And in the search for planets, 0:00:37.985,0:00:40.751 and in the future,[br]planets that might be like Earth, 0:00:40.775,0:00:42.144 we're able to help address 0:00:42.168,0:00:45.017 some of the most amazing[br]and mysterious questions 0:00:45.041,0:00:47.612 that have faced humankind for centuries. 0:00:47.636,0:00:48.882 Why are we here? 0:00:49.215,0:00:50.889 Why does our universe exist? 0:00:51.476,0:00:53.523 How did Earth form and evolve? 0:00:53.912,0:00:56.896 How and why did life originate[br]and populate our planet? 0:00:57.665,0:01:00.720 The second question[br]that we often think about is: 0:01:00.744,0:01:02.030 Are we alone? 0:01:02.911,0:01:04.299 Is there life out there? 0:01:05.109,0:01:06.601 Who is out there? 0:01:07.783,0:01:10.789 You know, this question has been around[br]for thousands of years, 0:01:10.813,0:01:13.230 since at least the time[br]of the Greek philosophers. 0:01:13.254,0:01:15.801 But I'm here to tell you[br]just how close we're getting 0:01:15.825,0:01:18.706 to finding out the answer[br]to this question. 0:01:18.730,0:01:22.945 It's the first time in human history[br]that this really is within reach for us. 0:01:23.294,0:01:26.273 Now when I think about the possibilities[br]for life out there, 0:01:26.297,0:01:30.384 I think of the fact that our sun[br]is but one of many stars. 0:01:30.825,0:01:32.703 This is a photograph of a real galaxy, 0:01:32.727,0:01:35.173 we think our Milky Way[br]looks like this galaxy. 0:01:35.197,0:01:36.836 It's a collection of bound stars. 0:01:36.860,0:01:41.247 But our Milky Way is one[br]of hundreds of billions of stars 0:01:41.271,0:01:45.595 and our galaxy is one of upwards[br]of hundreds of billions of galaxies. 0:01:46.707,0:01:49.474 Knowing that small planets[br]are very common, 0:01:49.498,0:01:50.772 you can just do the math. 0:01:51.424,0:01:55.425 And there are just so many stars[br]and so many planets out there, 0:01:55.449,0:01:58.139 that surely, there must be life[br]somewhere out there. 0:01:59.060,0:02:02.480 Well, the biologists get furious[br]with me for saying that, 0:02:02.504,0:02:05.948 because we have absolutely no evidence[br]for life beyond Earth, yet. 0:02:06.977,0:02:11.770 Well, if we were able to look[br]at our galaxy from the outside 0:02:11.794,0:02:14.002 and zoom in to where our sun is, 0:02:14.026,0:02:15.586 we see a real map of the stars. 0:02:16.046,0:02:19.069 And the highlighted stars[br]are those with known exoplanets. 0:02:19.745,0:02:21.934 This is really just[br]the tip of the iceberg. 0:02:22.642,0:02:26.284 Here, this animation is zooming in[br]onto our solar system. 0:02:26.872,0:02:28.357 And you'll see here the planets 0:02:28.381,0:02:31.214 as well as some spacecraft[br]that are also orbiting our sun. 0:02:32.968,0:02:36.332 Now if we can imagine going[br]to the west coast of North America, 0:02:36.356,0:02:38.482 and looking out at the night sky, 0:02:38.506,0:02:40.784 here's what we'd see on a spring night. 0:02:40.808,0:02:42.818 And you can see[br]the constellations overlaid 0:02:42.842,0:02:45.111 and again, so many stars with planets. 0:02:45.135,0:02:49.329 There's a special patch of the sky[br]where we have thousands of planets. 0:02:49.353,0:02:53.043 This is where the Kepler Space Telescope[br]focused for many years. 0:02:53.576,0:02:58.250 Let's zoom in and look[br]at one of the favorite exoplanets. 0:02:58.863,0:03:02.124 This star is called Kepler-186f. 0:03:02.529,0:03:04.727 It's a system of about five planets. 0:03:04.751,0:03:08.576 And by the way, most of these exoplanets,[br]we don't know too much about. 0:03:08.600,0:03:11.583 We know their size, and their orbit[br]and things like that. 0:03:11.607,0:03:15.569 But there's a very special planet[br]here called Kepler-186f. 0:03:15.593,0:03:19.697 This planet is in a zone[br]that is not too far from the star, 0:03:19.721,0:03:22.980 so that the temperature[br]may be just right for life. 0:03:23.004,0:03:26.035 Here, the artist's conception[br]is just zooming in 0:03:26.059,0:03:28.329 and showing you what that planet[br]might be like. 0:03:31.074,0:03:36.676 So, many people have this[br]romantic notion of astronomers 0:03:36.700,0:03:40.256 going to the telescope[br]on a lonely mountaintop 0:03:40.280,0:03:43.829 and looking at the spectacular night sky[br]through a big telescope. 0:03:43.853,0:03:47.225 But actually, we just work[br]on our computers like everyone else, 0:03:47.249,0:03:51.074 and we get our data by email[br]or downloading from a database. 0:03:51.098,0:03:53.621 So instead of coming here to tell you 0:03:53.645,0:03:56.776 about the somewhat tedious nature[br]of the data and data analysis 0:03:56.800,0:03:58.866 and the complex computer models we make, 0:03:58.890,0:04:01.088 I have a different way[br]to try to explain to you 0:04:01.112,0:04:03.757 some of the things[br]that we're thinking about exoplanets. 0:04:03.781,0:04:04.947 Here's a travel poster: 0:04:04.971,0:04:07.291 "Kepler-186f: 0:04:07.315,0:04:10.029 Where the grass is always redder[br]on the other side." 0:04:10.053,0:04:13.783 That's because Kepler-186f[br]orbits a red star, 0:04:13.807,0:04:16.499 and we're just speculating[br]that perhaps the plants there, 0:04:16.523,0:04:19.141 if there is vegetation[br]that does photosynthesis, 0:04:19.165,0:04:21.108 it has different pigments and looks red. 0:04:22.137,0:04:26.495 "Enjoy the gravity on HD 40307g, 0:04:26.519,0:04:27.978 a Super-Earth." 0:04:28.002,0:04:30.159 This planet is more massive than Earth 0:04:30.183,0:04:31.905 and has a higher surface gravity. 0:04:32.333,0:04:35.230 "Relax on Kepler-16b, 0:04:35.254,0:04:37.150 where your shadow always has company." 0:04:37.174,0:04:39.134 (Laughter) 0:04:39.158,0:04:43.340 We know of a dozen planets[br]that orbit two stars, 0:04:43.364,0:04:45.483 and there's likely many more out there. 0:04:45.507,0:04:47.468 If we could visit one of those planets, 0:04:47.492,0:04:49.379 you literally would see two sunsets 0:04:49.403,0:04:50.658 and have two shadows. 0:04:51.484,0:04:53.901 So actually, science fiction[br]got some things right. 0:04:53.925,0:04:55.134 Tatooine from Star Wars. 0:04:56.047,0:04:58.342 And I have a couple of other[br]favorite exoplanets 0:04:58.366,0:04:59.563 to tell you about. 0:04:59.587,0:05:01.119 This one is Kepler-10b, 0:05:01.143,0:05:03.126 it's a hot, hot planet. 0:05:03.642,0:05:06.577 It orbits over 50 times closer to its star 0:05:06.601,0:05:08.768 than the Earth does to our sun. 0:05:08.792,0:05:10.372 And actually, it's so hot, 0:05:10.396,0:05:13.029 we can't visit any[br]of these planets, but if we could, 0:05:13.053,0:05:15.027 we would melt long before we got there. 0:05:15.051,0:05:17.380 We think the surface[br]is hot enough to melt rock 0:05:17.404,0:05:18.830 and has liquid lava lakes. 0:05:19.457,0:05:21.041 Gliese 1214b. 0:05:21.065,0:05:23.164 This planet, we know the mass and the size 0:05:23.188,0:05:24.776 and it has a fairly low density. 0:05:24.800,0:05:25.998 It's somewhat warm. 0:05:26.053,0:05:28.737 We actually don't know[br]really anything about this planet, 0:05:28.761,0:05:31.266 but one possibility[br]is that it's a water world, 0:05:31.290,0:05:34.797 like a scaled-up version[br]of one of Jupiter's icy moons 0:05:34.821,0:05:37.304 that might be 50 percent water by mass. 0:05:37.328,0:05:40.289 And in this case, it would have[br]a thick steam atmosphere 0:05:40.313,0:05:42.169 overlaying an ocean, 0:05:42.193,0:05:43.703 not of liquid water, 0:05:43.727,0:05:46.732 but of an exotic form[br]of water, a superfluid -- 0:05:46.756,0:05:48.746 not quite a gas, not quite a liquid. 0:05:48.770,0:05:50.370 And under that wouldn't be rock, 0:05:50.394,0:05:51.990 but a form of high-pressure ice, 0:05:52.014,0:05:53.290 like ice IX. 0:05:54.593,0:05:56.768 So out of all these planets out there, 0:05:56.792,0:06:00.006 and the variety[br]is just simply astonishing, 0:06:00.030,0:06:05.160 we mostly want to find the planets[br]that are Goldilocks planets, we call them. 0:06:05.184,0:06:07.101 Not too big, not too small, 0:06:07.125,0:06:08.972 not too hot, not too cold -- 0:06:08.996,0:06:10.345 but just right for life. 0:06:10.658,0:06:12.776 But to do that,[br]we'd have to be able to look 0:06:12.800,0:06:14.134 at the planet's atmosphere, 0:06:14.158,0:06:16.954 because the atmosphere[br]acts like a blanket trapping heat -- 0:06:16.978,0:06:18.314 the greenhouse effect. 0:06:18.338,0:06:21.158 We have to be able to asses[br]the greenhouse gases 0:06:21.182,0:06:22.332 on other planets. 0:06:23.169,0:06:25.288 Well, science fiction[br]got some things wrong. 0:06:25.796,0:06:27.186 The Star Trek Enterprise 0:06:27.210,0:06:30.837 had to travel vast distances[br]at incredible speeds 0:06:30.861,0:06:32.590 to orbit other planets 0:06:32.614,0:06:36.590 so that First Officer Spock[br]could analyze the atmosphere 0:06:36.614,0:06:38.575 to see if the planet was habitable 0:06:38.599,0:06:40.272 or if there were lifeforms there. 0:06:40.745,0:06:43.235 Well, we don't need[br]to travel at warp speeds 0:06:43.259,0:06:45.388 to see other planet atmospheres, 0:06:45.412,0:06:48.196 although I don't want to dissuade[br]any budding engineers 0:06:48.220,0:06:50.143 from figuring out how to do that. 0:06:50.167,0:06:52.459 We actually can and do study[br]planet atmospheres 0:06:52.483,0:06:54.096 from here, from Earth orbit. 0:06:54.120,0:06:57.297 This is a picture, a photograph[br]of the Hubble Space Telescope 0:06:57.321,0:07:00.071 taken by the shuttle Atlantis[br]as it was departing 0:07:00.095,0:07:02.334 after the last[br]human space flight to Hubble. 0:07:02.358,0:07:04.244 They installed a new camera, actually, 0:07:04.268,0:07:06.413 that we use for exoplanet atmospheres. 0:07:06.437,0:07:11.342 And so far, we've been able to study[br]dozens of exoplanet atmospheres, 0:07:11.366,0:07:13.490 about six of them in great detail. 0:07:13.514,0:07:15.686 But those are not[br]small planets like Earth. 0:07:15.710,0:07:18.104 They're big, hot planets[br]that are easy to see. 0:07:18.128,0:07:19.366 We're not ready, 0:07:19.390,0:07:23.765 we don't have the right technology yet[br]to study small exoplanets. 0:07:24.106,0:07:25.264 But nevertheless, 0:07:25.288,0:07:29.185 I wanted to try to explain to you[br]how we study exoplanet atmospheres. 0:07:29.652,0:07:31.874 I want you to imagine,[br]for a moment, a rainbow. 0:07:32.532,0:07:35.278 And if we could look[br]at this rainbow closely, 0:07:35.302,0:07:37.969 we would see that some[br]dark lines are missing. 0:07:39.127,0:07:40.548 And here's our sun, 0:07:40.572,0:07:42.339 the white light of our sun split up, 0:07:42.363,0:07:44.649 not by raindrops, but by a spectrograph. 0:07:44.673,0:07:47.124 And you can see[br]all these dark, vertical lines. 0:07:47.148,0:07:48.702 Some are narrow, some are wide, 0:07:48.726,0:07:50.407 some are shaded at the edges. 0:07:50.431,0:07:54.035 And this is how astronomers[br]have studied objects in the heavens, 0:07:54.059,0:07:55.554 literally, for over a century. 0:07:55.578,0:07:58.004 So here, each different atom and molecule 0:07:58.028,0:07:59.553 has a special set of lines, 0:07:59.577,0:08:01.133 a fingerprint, if you will. 0:08:01.157,0:08:03.894 And that's how we study[br]exoplanet atmospheres. 0:08:03.918,0:08:06.278 And I'll just never forget[br]when I started working 0:08:06.302,0:08:08.158 on exoplanet atmospheres 20 years ago, 0:08:08.182,0:08:09.367 how many people told me, 0:08:09.391,0:08:10.600 "This will never happen, 0:08:10.624,0:08:13.414 we'll never be able to study them.[br]Why are you bothering?" 0:08:13.438,0:08:17.112 And that's why I'm pleased to tell you[br]about all the atmospheres studied now, 0:08:17.136,0:08:18.985 and this is really a field of its own. 0:08:19.009,0:08:21.531 So when it comes to[br]other planets, other earths, 0:08:21.555,0:08:23.632 in the future when we can observe them, 0:08:23.656,0:08:25.715 what kind of gases would be looking for? 0:08:26.144,0:08:29.319 Well, you know, our own Earth[br]has oxygen in the atmosphere 0:08:29.343,0:08:30.802 to 20 percent by volume. 0:08:31.445,0:08:32.714 That's a lot of oxygen. 0:08:33.457,0:08:36.202 But without plants[br]and photosynthetic life, 0:08:36.226,0:08:37.636 there would be no oxygen, 0:08:37.660,0:08:39.501 virtually no oxygen in our atmosphere. 0:08:40.116,0:08:42.039 So oxygen is here because of life. 0:08:42.063,0:08:46.170 And our goal then is to look for gases[br]in other planet atmospheres, 0:08:46.194,0:08:48.231 gases that don't belong, 0:08:48.255,0:08:50.638 that we might be able[br]to attribute to life. 0:08:50.662,0:08:52.743 But which molecules should we search for? 0:08:52.767,0:08:55.430 I actually told you[br]how diverse exoplanets are. 0:08:55.454,0:08:57.451 We expect that to continue in the future 0:08:57.475,0:08:58.776 when we find other earths. 0:08:58.800,0:09:01.372 And that's one of the main things[br]I'm working on now, 0:09:01.396,0:09:02.689 I have a theory about this. 0:09:02.713,0:09:05.001 It reminds me that nearly every day, 0:09:05.025,0:09:07.677 I receive an email or emails 0:09:07.701,0:09:11.328 from someone with a crazy theory[br]about physics of gravity 0:09:11.352,0:09:13.184 or cosmology or some such. 0:09:13.208,0:09:16.541 So, please don't email me[br]one of your crazy theories. 0:09:16.565,0:09:17.779 (Laughter) 0:09:17.803,0:09:19.981 Well, I had my own crazy theory. 0:09:20.005,0:09:21.989 But, who does the MIT professor go to? 0:09:22.703,0:09:26.914 Well, I emailed a Nobel Laureate[br]in physiology and medicine 0:09:26.938,0:09:28.911 and he said, "Sure, come and talk to me." 0:09:28.935,0:09:30.934 So I brought my two biochemistry friends 0:09:30.958,0:09:33.310 and we went to talk to him[br]about our crazy theory. 0:09:33.334,0:09:36.775 And that theory was that life[br]produces all small molecules, 0:09:36.799,0:09:38.473 so many molecules. 0:09:38.497,0:09:41.392 Like, everything I could think of,[br]but not being a chemist. 0:09:41.416,0:09:42.599 Think about it: 0:09:42.623,0:09:44.653 carbon dioxide, carbon monoxide, 0:09:44.677,0:09:46.536 molecular hydrogen, molecular nitrogen, 0:09:46.560,0:09:47.926 methane, methyl chloride -- 0:09:47.950,0:09:49.111 so many gases. 0:09:49.135,0:09:51.070 They also exist for other reasons, 0:09:51.094,0:09:52.946 but just life even produces ozone. 0:09:52.970,0:09:54.728 So we go to talk to him about this, 0:09:54.752,0:09:56.894 and immediately, he shot down the theory. 0:09:57.226,0:09:59.493 He found an example that didn't exist. 0:09:59.948,0:10:01.729 So, we went back to the drawing board 0:10:01.753,0:10:05.181 and we think we have found something[br]very interesting in another field. 0:10:05.205,0:10:06.625 But back to exoplanets, 0:10:06.649,0:10:09.928 the point is that life produces[br]so many different types of gases, 0:10:09.952,0:10:12.164 literally thousands of gases. 0:10:12.188,0:10:14.855 And so what we're doing now[br]is just trying to figure out 0:10:14.879,0:10:16.468 on which types of exoplanets, 0:10:16.492,0:10:19.712 which gases could be attributed to life. 0:10:22.182,0:10:24.230 And so when it comes time[br]when we find gases 0:10:24.254,0:10:25.605 in exoplanet atmospheres 0:10:25.629,0:10:27.725 that we won't know[br]if they're being produced 0:10:27.749,0:10:30.779 by intelligent aliens or by trees, 0:10:30.803,0:10:32.013 or a swamp, 0:10:32.037,0:10:34.898 or even just by simple,[br]single-celled microbial life. 0:10:35.541,0:10:37.091 So working on the models 0:10:37.115,0:10:38.766 and thinking about biochemistry, 0:10:38.790,0:10:39.987 it's all well and good. 0:10:40.011,0:10:42.896 But a really big challenge[br]ahead of us is how. 0:10:42.920,0:10:45.082 How are we going to find these planets? 0:10:45.106,0:10:47.170 They're actually many ways[br]to find planets, 0:10:47.194,0:10:48.829 several different ways. 0:10:48.853,0:10:52.712 But the one that I'm most focused on[br]is how can we open a gateway 0:10:52.736,0:10:53.973 so that in the future, 0:10:53.997,0:10:55.846 we can find hundreds of earths. 0:10:55.870,0:10:58.203 We have a real shot[br]at finding signs of life. 0:10:58.227,0:11:01.353 And actually, I just finished[br]leading a two-year project 0:11:01.377,0:11:03.465 in this very special phase 0:11:03.489,0:11:06.143 of a concept we call the starshade. 0:11:06.167,0:11:09.120 And the starshade[br]is a very specially shaped screen 0:11:09.144,0:11:11.011 and the goal is to fly that starshade 0:11:11.035,0:11:14.129 so it blocks out the light of a star 0:11:14.153,0:11:17.092 so that a telescope[br]can see the planets directly. 0:11:17.116,0:11:19.509 Here, you can see myself[br]and two team members 0:11:19.533,0:11:21.722 holding up one small part[br]of the starshade. 0:11:21.746,0:11:23.326 It's shaped like a giant flower, 0:11:23.350,0:11:25.833 and this is one of the prototype petals. 0:11:26.907,0:11:31.368 The concept is that a starshade[br]and telescope could launch together, 0:11:31.392,0:11:33.986 with the petals unfurling[br]from the stowed position. 0:11:34.896,0:11:36.952 The central truss would expand, 0:11:36.976,0:11:40.068 with the petals snapping into place. 0:11:40.092,0:11:42.322 Now, this has to be made very precisely, 0:11:42.346,0:11:43.934 literally, the petals to microns 0:11:43.958,0:11:46.673 and they have to deploy to millimeters. 0:11:46.697,0:11:48.752 And this whole structure would have to fly 0:11:48.776,0:11:52.135 tens of thousands of kilometers[br]away from the telescope. 0:11:52.159,0:11:54.301 It's about tens of meters in diameter. 0:11:54.785,0:11:59.738 And the goal is to block out[br]the starlight to incredible precision 0:11:59.762,0:12:02.500 so that we'd be able to see[br]the planets directly. 0:12:03.333,0:12:05.562 And it has to be a very special shape, 0:12:05.586,0:12:07.475 because of the physics of defraction. 0:12:07.499,0:12:09.718 Now this is a real project[br]that we worked on, 0:12:09.742,0:12:12.210 literally, you would not believe how hard. 0:12:12.234,0:12:14.896 Just so you believe[br]it's not just in movie format, 0:12:14.920,0:12:16.556 here's a real photograph 0:12:16.580,0:12:21.571 of a second-generation[br]starshade deployment test bed in the lab. 0:12:21.595,0:12:23.674 And in this case,[br]I just wanted you to know 0:12:23.698,0:12:26.188 that that central truss[br]has heritage left over 0:12:26.212,0:12:28.126 from large radio deployables in space. 0:12:29.372,0:12:31.028 So after all of that hard work 0:12:31.052,0:12:34.845 where we try to think of all the crazy[br]gases that might be out there, 0:12:34.869,0:12:37.797 and we build the very[br]complicated space telescopes 0:12:37.821,0:12:39.048 that might be out there, 0:12:39.072,0:12:40.368 what are we going to find? 0:12:40.725,0:12:42.483 Well, in the best case, 0:12:42.507,0:12:45.304 we will find an image[br]of another exo-Earth. 0:12:46.328,0:12:48.587 Here is Earth as a pale blue dot. 0:12:48.611,0:12:51.170 And this is actually[br]a real photograph of Earth 0:12:51.194,0:12:53.064 taken by the Voyager 1 spacecraft, 0:12:53.088,0:12:54.706 four billion miles away. 0:12:55.159,0:12:58.397 And that red light is just scattered light[br]in the camera optics. 0:12:59.315,0:13:01.711 But what's so awesome to consider 0:13:01.735,0:13:04.784 is that if there are intelligent aliens 0:13:04.808,0:13:08.762 orbiting on a planet[br]around a star near to us 0:13:08.786,0:13:10.831 and they build complicated[br]space telescopes 0:13:10.855,0:13:12.782 of the kind that we're trying to build, 0:13:12.806,0:13:15.306 all they'll see is this pale blue dot, 0:13:15.330,0:13:16.615 a pinprick of light. 0:13:17.456,0:13:20.522 And so sometimes, when I pause to think 0:13:20.546,0:13:24.799 about my professional struggle[br]and huge ambition, 0:13:24.823,0:13:26.816 it's hard to think about that 0:13:26.840,0:13:29.259 in contrast to the vastness[br]of the universe. 0:13:30.120,0:13:34.246 But nonetheless, I am devoting[br]the rest of my life 0:13:34.270,0:13:35.620 to finding another Earth. 0:13:36.296,0:13:38.511 And I can guarantee 0:13:38.535,0:13:40.918 that in the next generation[br]of space telescopes, 0:13:40.942,0:13:42.482 and the second generation, 0:13:42.506,0:13:47.912 we will have the capability[br]to find and identity other earths. 0:13:47.936,0:13:50.610 And the capability[br]to split up the starlight 0:13:50.634,0:13:52.187 so that we can look for gases 0:13:52.211,0:13:55.697 and assess the greenhouse gases[br]in the atmosphere, 0:13:55.721,0:13:57.319 estimate the surface temperature, 0:13:57.343,0:13:59.101 and look for signs of life. 0:13:59.736,0:14:01.157 But there's more. 0:14:01.181,0:14:04.545 In this case of searching[br]for other planets like Earth, 0:14:04.569,0:14:07.164 we are making a new kind of map 0:14:07.188,0:14:10.448 of the nearby stars[br]and of the planets orbiting them, 0:14:10.472,0:14:14.243 including stars that actually might be[br]inhabitable by humans. 0:14:14.915,0:14:17.296 And so I envision that our descendants, 0:14:17.320,0:14:19.125 hundreds of years from now, 0:14:19.149,0:14:22.176 will embark on an interstellar[br]journey to other worlds. 0:14:23.059,0:14:25.971 And they will look back at all of us 0:14:25.995,0:14:29.003 as the generation who first found[br]the Earth-like worlds. 0:14:29.822,0:14:30.973 Thank you. 0:14:30.997,0:14:37.508 (Applause) 0:14:37.532,0:14:39.632 June Cohen: And I give you,[br]for a question, 0:14:39.656,0:14:41.384 Rosetta Mission manager Fred Jansen. 0:14:41.817,0:14:43.848 Fred Jansen: You mentioned halfway through 0:14:43.872,0:14:47.659 that the technology[br]to actually look at the spectrum 0:14:47.683,0:14:50.312 of an exoplanet like Earth[br]is not there yet. 0:14:50.336,0:14:52.223 When do you expect this will be there, 0:14:52.247,0:14:53.515 and what's needed? 0:14:53.539,0:14:58.154 Actually, what we expect is what we call[br]our next-generation Hubble telescope. 0:14:58.531,0:15:00.872 And this is called the James Webb[br]Space Telescope, 0:15:00.896,0:15:02.599 and that will launch in 2018, 0:15:02.623,0:15:04.445 and that's what we're going to do, 0:15:04.469,0:15:06.733 we're going to look[br]at a special kind of planet 0:15:06.757,0:15:08.213 called transient exoplanets, 0:15:08.237,0:15:11.338 and that will be our first shot[br]at studying small planets 0:15:11.362,0:15:14.660 for gases that might indicate[br]the planet is habitable. 0:15:15.477,0:15:18.286 JC: I'm going to ask you[br]one follow-up question, too, Sara, 0:15:18.310,0:15:19.516 as the generalist. 0:15:19.540,0:15:22.633 So I am really struck[br]by the notion in your career 0:15:22.657,0:15:24.056 of the opposition you faced, 0:15:24.080,0:15:26.224 that when you began thinking[br]about exoplanets, 0:15:26.248,0:15:28.914 there was extreme skepticism[br]in the scientific community 0:15:28.938,0:15:30.089 that they existed, 0:15:30.113,0:15:31.382 and you proved them wrong. 0:15:31.406,0:15:33.119 What did it take to take that on? 0:15:33.143,0:15:35.213 SS: Well, the thing is that as scientists, 0:15:35.237,0:15:37.195 we're supposed to be skeptical, 0:15:37.219,0:15:40.267 because our job to make sure[br]that what the other person is saying 0:15:40.291,0:15:41.630 actually makes sense or not. 0:15:41.654,0:15:44.211 But being a scientist, 0:15:44.235,0:15:46.655 I think you've seen it from this session, 0:15:46.679,0:15:48.361 it's like being an explorer. 0:15:48.385,0:15:50.374 You have this immense curiosity, 0:15:50.398,0:15:51.697 this stubbornness, 0:15:51.721,0:15:54.103 this sort of resolute will[br]that you will go forward 0:15:54.127,0:15:56.158 no matter what other people say. 0:15:56.182,0:15:57.858 JC: I love that. Thank you, Sara. 0:15:57.882,0:16:00.877 (Applause)