0:00:00.943,0:00:02.364 I'm really glad to be here. 0:00:03.015,0:00:04.703 I'm glad you're here, 0:00:04.727,0:00:06.560 because that would be a little weird. 0:00:07.460,0:00:09.565 I'm glad we're all here. 0:00:10.303,0:00:13.156 And by "here," I don't mean here. 0:00:14.831,0:00:15.981 Or here. 0:00:16.728,0:00:17.880 But here. 0:00:17.904,0:00:19.054 I mean Earth. 0:00:19.627,0:00:23.570 And by "we," I don't mean[br]those of us in this auditorium, 0:00:23.594,0:00:25.064 but life, 0:00:25.088,0:00:26.537 all life on Earth -- 0:00:26.561,0:00:31.943 (Laughter) 0:00:32.280,0:00:34.271 from complex to single-celled, 0:00:34.295,0:00:36.619 from mold to mushrooms 0:00:36.643,0:00:38.021 to flying bears. 0:00:38.045,0:00:39.411 (Laughter) 0:00:41.736,0:00:43.245 The interesting thing is, 0:00:43.269,0:00:46.300 Earth is the only place[br]we know of that has life -- 0:00:46.324,0:00:48.201 8.7 million species. 0:00:48.660,0:00:49.914 We've looked other places, 0:00:49.938,0:00:52.035 maybe not as hard[br]as we should or we could, 0:00:52.059,0:00:53.986 but we've looked and haven't found any; 0:00:54.010,0:00:56.286 Earth is the only place[br]we know of with life. 0:00:57.318,0:00:58.592 Is Earth special? 0:00:59.591,0:01:02.045 This is a question I've wanted[br]to know the answer to 0:01:02.069,0:01:03.323 since I was a small child, 0:01:03.347,0:01:05.379 and I suspect 80 percent[br]of this auditorium 0:01:05.403,0:01:08.411 has thought the same thing[br]and also wanted to know the answer. 0:01:08.879,0:01:11.046 To understand whether[br]there are any planets -- 0:01:11.070,0:01:13.348 out there in our solar system or beyond -- 0:01:13.372,0:01:14.830 that can support life, 0:01:14.854,0:01:18.051 the first step is to understand[br]what life here requires. 0:01:18.575,0:01:22.138 It turns out, of all of those[br]8.7 million species, 0:01:22.162,0:01:24.360 life only needs three things. 0:01:25.032,0:01:27.884 On one side, all life[br]on Earth needs energy. 0:01:27.908,0:01:31.393 Complex life like us derives[br]our energy from the sun, 0:01:31.417,0:01:33.518 but life deep underground[br]can get its energy 0:01:33.542,0:01:35.264 from things like chemical reactions. 0:01:35.288,0:01:37.439 There are a number[br]of different energy sources 0:01:37.463,0:01:38.706 available on all planets. 0:01:39.400,0:01:40.556 On the other side, 0:01:40.580,0:01:43.285 all life needs food or nourishment. 0:01:43.741,0:01:48.215 And this seems like a tall order,[br]especially if you want a succulent tomato. 0:01:48.239,0:01:49.955 (Laughter) 0:01:49.979,0:01:53.045 However, all life on Earth[br]derives its nourishment 0:01:53.069,0:01:55.099 from only six chemical elements, 0:01:55.123,0:01:58.127 and these elements can be found[br]on any planetary body 0:01:58.151,0:01:59.487 in our solar system. 0:02:00.537,0:02:03.764 So that leaves the thing[br]in the middle as the tall pole, 0:02:03.788,0:02:05.742 the thing that's hardest to achieve. 0:02:05.766,0:02:07.658 Not moose, but water. 0:02:07.682,0:02:10.463 (Laughter) 0:02:11.285,0:02:13.079 Although moose would be pretty cool. 0:02:13.103,0:02:14.261 (Laughter) 0:02:14.285,0:02:19.820 And not frozen water, and not water[br]in a gaseous state, but liquid water. 0:02:20.748,0:02:23.201 This is what life needs[br]to survive, all life. 0:02:23.680,0:02:27.016 And many solar system bodies[br]don't have liquid water, 0:02:27.040,0:02:28.676 and so we don't look there. 0:02:28.700,0:02:31.693 Other solar system bodies[br]might have abundant liquid water, 0:02:31.717,0:02:33.052 even more than Earth, 0:02:33.076,0:02:35.526 but it's trapped beneath an icy shell, 0:02:35.550,0:02:37.811 and so it's hard to access,[br]it's hard to get to, 0:02:37.835,0:02:40.554 it's hard to even find out[br]if there's any life there. 0:02:41.475,0:02:44.470 So that leaves a few bodies[br]that we should think about. 0:02:44.494,0:02:46.923 So let's make the problem[br]simpler for ourselves. 0:02:46.947,0:02:50.288 Let's think only about liquid water[br]on the surface of a planet. 0:02:50.312,0:02:53.268 There are only three bodies[br]to think about in our solar system, 0:02:53.292,0:02:55.874 with regard to liquid water[br]on the surface of a planet, 0:02:55.898,0:03:00.724 and in order of distance from the sun,[br]it's: Venus, Earth and Mars. 0:03:01.265,0:03:04.637 You want to have an atmosphere[br]for water to be liquid. 0:03:04.661,0:03:07.039 You have to be very careful[br]with that atmosphere. 0:03:07.063,0:03:10.475 You can't have too much atmosphere,[br]too thick or too warm an atmosphere, 0:03:10.499,0:03:13.404 because then you end up[br]too hot like Venus, 0:03:13.428,0:03:15.165 and you can't have liquid water. 0:03:15.189,0:03:19.142 But if you have too little atmosphere[br]and it's too thin and too cold, 0:03:19.166,0:03:21.190 you end up like Mars, too cold. 0:03:21.865,0:03:24.340 So Venus is too hot, Mars is too cold, 0:03:24.364,0:03:25.528 and Earth is just right. 0:03:25.552,0:03:29.027 You can look at these images behind me[br]and you can see automatically 0:03:29.051,0:03:31.648 where life can survive[br]in our solar system. 0:03:32.296,0:03:33.896 It's a Goldilocks-type problem, 0:03:33.920,0:03:36.410 and it's so simple[br]that a child could understand it. 0:03:37.452,0:03:38.632 However, 0:03:39.450,0:03:42.378 I'd like to remind you of two things 0:03:42.402,0:03:45.356 from the Goldilocks story[br]that we may not think about so often, 0:03:45.380,0:03:47.476 but that I think are really relevant here. 0:03:48.056,0:03:49.206 Number one: 0:03:50.311,0:03:53.103 if Mama Bear's bowl is too cold 0:03:53.833,0:03:55.841 when Goldilocks walks into the room, 0:03:56.642,0:03:58.785 does that mean it's always been too cold? 0:03:59.825,0:04:03.093 Or could it have been just right[br]at some other time? 0:04:03.650,0:04:07.331 When Goldilocks walks into the room[br]determines the answer 0:04:07.355,0:04:08.687 that we get in the story. 0:04:09.114,0:04:10.844 And the same is true with planets. 0:04:10.868,0:04:12.894 They're not static things. They change. 0:04:12.918,0:04:14.660 They vary. They evolve. 0:04:14.684,0:04:16.727 And atmospheres do the same. 0:04:16.751,0:04:18.453 So let me give you an example. 0:04:18.477,0:04:20.479 Here's one of my favorite[br]pictures of Mars. 0:04:20.503,0:04:23.634 It's not the highest resolution image,[br]it's not the sexiest image, 0:04:23.658,0:04:25.161 it's not the most recent image, 0:04:25.185,0:04:28.679 but it's an image that shows riverbeds[br]cut into the surface of the planet; 0:04:29.320,0:04:31.904 riverbeds carved by flowing, liquid water; 0:04:33.515,0:04:38.401 riverbeds that take hundreds or thousands[br]or tens of thousands of years to form. 0:04:38.425,0:04:40.043 This can't happen on Mars today. 0:04:40.067,0:04:42.548 The atmosphere of Mars today[br]is too thin and too cold 0:04:42.572,0:04:44.713 for water to be stable as a liquid. 0:04:44.737,0:04:49.085 This one image tells you[br]that the atmosphere of Mars changed 0:04:49.109,0:04:51.141 and it changed in big ways. 0:04:51.714,0:04:56.523 And it changed from a state[br]that we would define as habitable, 0:04:56.547,0:05:00.137 because the three requirements[br]for life were present long ago. 0:05:01.049,0:05:03.117 Where did that atmosphere go 0:05:03.141,0:05:05.961 that allowed water[br]to be liquid at the surface? 0:05:05.985,0:05:09.332 Well, one idea is it escaped[br]away to space. 0:05:09.356,0:05:12.023 Atmospheric particles[br]got enough energy to break free 0:05:12.047,0:05:13.700 from the gravity of the planet, 0:05:13.724,0:05:16.413 escaping away to space, never to return. 0:05:16.437,0:05:19.125 And this happens with all bodies[br]with atmospheres. 0:05:19.149,0:05:20.321 Comets have tails 0:05:20.345,0:05:23.602 that are incredibly visible reminders[br]of atmospheric escape. 0:05:23.626,0:05:27.035 But Venus also has an atmosphere[br]that escapes with time, 0:05:27.059,0:05:28.719 and Mars and Earth as well. 0:05:28.743,0:05:31.711 It's just a matter of degree[br]and a matter of scale. 0:05:32.092,0:05:34.768 So we'd like to figure out[br]how much escaped over time 0:05:34.792,0:05:36.908 so we can explain this transition. 0:05:36.932,0:05:39.543 How do atmospheres[br]get their energy for escape? 0:05:39.567,0:05:41.698 How do particles get[br]enough energy to escape? 0:05:41.722,0:05:44.907 There are two ways, if we're going[br]to reduce things a little bit. 0:05:44.931,0:05:46.082 Number one, sunlight. 0:05:46.106,0:05:49.518 Light emitted from the sun can be absorbed[br]by atmospheric particles 0:05:49.542,0:05:51.256 and warm the particles. 0:05:51.280,0:05:53.388 Yes, I'm dancing, but they -- 0:05:53.412,0:05:54.883 (Laughter) 0:05:55.693,0:05:57.605 Oh my God, not even at my wedding. 0:05:57.629,0:05:59.121 (Laughter) 0:05:59.145,0:06:02.148 They get enough energy[br]to escape and break free 0:06:02.172,0:06:04.672 from the gravity of the planet[br]just by warming. 0:06:04.696,0:06:07.858 A second way they can get energy[br]is from the solar wind. 0:06:07.882,0:06:12.908 These are particles, mass, material,[br]spit out from the surface of the sun, 0:06:12.932,0:06:15.336 and they go screaming[br]through the solar system 0:06:15.360,0:06:17.145 at 400 kilometers per second, 0:06:17.169,0:06:19.763 sometimes faster during solar storms, 0:06:19.787,0:06:22.509 and they go hurtling[br]through interplanetary space 0:06:22.533,0:06:24.979 towards planets and their atmospheres, 0:06:25.003,0:06:26.628 and they may provide energy 0:06:26.652,0:06:28.780 for atmospheric particles[br]to escape as well. 0:06:29.182,0:06:31.151 This is something that I'm interested in, 0:06:31.175,0:06:32.888 because it relates to habitability. 0:06:33.378,0:06:36.510 I mentioned that there were two things[br]about the Goldilocks story 0:06:36.534,0:06:39.518 that I wanted to bring to your attention[br]and remind you about, 0:06:39.542,0:06:41.781 and the second one[br]is a little bit more subtle. 0:06:41.805,0:06:44.593 If Papa Bear's bowl is too hot, 0:06:46.180,0:06:49.414 and Mama Bear's bowl is too cold, 0:06:51.057,0:06:54.168 shouldn't Baby Bear's bowl be even colder 0:06:55.081,0:06:56.877 if we're following the trend? 0:06:58.195,0:07:00.507 This thing that you've accepted[br]your entire life, 0:07:00.531,0:07:03.601 when you think about it a little bit more,[br]may not be so simple. 0:07:04.513,0:07:08.541 And of course, distance of a planet[br]from the sun determines its temperature. 0:07:08.565,0:07:10.831 This has to play into habitability. 0:07:10.855,0:07:13.785 But maybe there are other things[br]we should be thinking about. 0:07:13.809,0:07:15.425 Maybe it's the bowls themselves 0:07:15.449,0:07:18.505 that are also helping to determine[br]the outcome in the story, 0:07:18.529,0:07:19.829 what is just right. 0:07:20.765,0:07:23.630 I could talk to you about a lot[br]of different characteristics 0:07:23.654,0:07:24.805 of these three planets 0:07:24.829,0:07:26.398 that may influence habitability, 0:07:26.422,0:07:29.016 but for selfish reasons related[br]to my own research 0:07:29.040,0:07:32.628 and the fact that I'm standing up here[br]holding the clicker and you're not -- 0:07:32.652,0:07:33.658 (Laughter) 0:07:33.682,0:07:35.791 I would like to talk[br]for just a minute or two 0:07:35.815,0:07:37.112 about magnetic fields. 0:07:37.715,0:07:40.247 Earth has one; Venus and Mars do not. 0:07:40.825,0:07:43.948 Magnetic fields are generated[br]in the deep interior of a planet 0:07:43.972,0:07:47.689 by electrically conducting[br]churning fluid material 0:07:47.713,0:07:50.618 that creates this big old magnetic field[br]that surrounds Earth. 0:07:50.642,0:07:53.038 If you have a compass,[br]you know which way north is. 0:07:53.062,0:07:54.556 Venus and Mars don't have that. 0:07:54.580,0:07:56.494 If you have a compass on Venus and Mars, 0:07:56.518,0:07:57.914 congratulations, you're lost. 0:07:57.938,0:07:59.841 (Laughter) 0:07:59.865,0:08:01.905 Does this influence habitability? 0:08:03.175,0:08:04.477 Well, how might it? 0:08:05.024,0:08:07.628 Many scientists think[br]that a magnetic field of a planet 0:08:07.652,0:08:10.047 serves as a shield for the atmosphere, 0:08:10.071,0:08:13.426 reflecting solar wind particles[br]around the planet 0:08:13.450,0:08:15.265 in a bit of a force field-type effect 0:08:15.289,0:08:17.989 having to do with electric charge[br]and those particles. 0:08:18.362,0:08:21.989 I like to think of it instead[br]as a salad bar sneeze guard for planets. 0:08:22.013,0:08:24.292 (Laughter) 0:08:24.962,0:08:28.343 And yes, my colleagues[br]who watch this later will realize 0:08:28.367,0:08:30.911 this is the first time in the history[br]of our community 0:08:30.935,0:08:33.214 that the solar wind has been[br]equated with mucus. 0:08:33.238,0:08:34.888 (Laughter) 0:08:36.978,0:08:40.453 OK, so the effect, then, is that Earth[br]may have been protected 0:08:40.477,0:08:41.646 for billions of years, 0:08:41.670,0:08:43.520 because we've had a magnetic field. 0:08:43.544,0:08:45.723 Atmosphere hasn't been able to escape. 0:08:45.747,0:08:47.854 Mars, on the other hand,[br]has been unprotected 0:08:47.878,0:08:49.720 because of its lack of magnetic field, 0:08:49.744,0:08:51.696 and over billions of years, 0:08:51.720,0:08:53.900 maybe enough atmosphere[br]has been stripped away 0:08:53.924,0:08:56.517 to account for a transition[br]from a habitable planet 0:08:56.541,0:08:58.207 to the planet that we see today. 0:08:59.059,0:09:02.048 Other scientists think[br]that magnetic fields 0:09:02.072,0:09:04.235 may act more like the sails on a ship, 0:09:04.958,0:09:09.995 enabling the planet to interact[br]with more energy from the solar wind 0:09:10.019,0:09:13.291 than the planet would have been able[br]to interact with by itself. 0:09:13.315,0:09:15.806 The sails may gather energy[br]from the solar wind. 0:09:15.830,0:09:18.496 The magnetic field may gather[br]energy from the solar wind 0:09:18.520,0:09:21.764 that allows even more[br]atmospheric escape to happen. 0:09:21.788,0:09:24.042 That's an idea that has to be tested, 0:09:24.066,0:09:25.951 but the effect and how it works 0:09:25.975,0:09:27.126 seems apparent. 0:09:27.150,0:09:28.301 That's because we know 0:09:28.325,0:09:31.400 energy from the solar wind[br]is being deposited into our atmosphere 0:09:31.424,0:09:32.575 here on Earth. 0:09:32.599,0:09:35.004 That energy is conducted[br]along magnetic field lines 0:09:35.028,0:09:36.376 down into the polar regions, 0:09:36.400,0:09:38.536 resulting in incredibly beautiful aurora. 0:09:38.560,0:09:41.216 If you've ever experienced them,[br]it's magnificent. 0:09:41.240,0:09:43.246 We know the energy is getting in. 0:09:43.270,0:09:46.303 We're trying to measure[br]how many particles are getting out, 0:09:46.327,0:09:49.365 and if the magnetic field[br]is influencing this in any way. 0:09:50.722,0:09:53.102 So I've posed a problem for you here, 0:09:53.126,0:09:54.672 but I don't have a solution yet. 0:09:54.696,0:09:55.972 We don't have a solution. 0:09:56.702,0:09:59.059 But we're working on it.[br]How are we working on it? 0:09:59.083,0:10:01.381 Well, we've sent spacecraft[br]to all three planets. 0:10:01.405,0:10:02.881 Some of them are orbiting now, 0:10:02.905,0:10:05.977 including the MAVEN spacecraft[br]which is currently orbiting Mars, 0:10:06.001,0:10:09.533 which I'm involved with[br]and which is led here, 0:10:09.557,0:10:11.366 out of the University of Colorado. 0:10:11.390,0:10:13.672 It's designed to measure[br]atmospheric escape. 0:10:14.022,0:10:16.496 We have similar measurements[br]from Venus and Earth. 0:10:16.953,0:10:18.618 Once we have all our measurements, 0:10:18.642,0:10:21.517 we can combine all these together[br]and we can understand 0:10:21.541,0:10:24.958 how all three planets interact[br]with their space environment, 0:10:24.982,0:10:26.144 with the surroundings. 0:10:26.168,0:10:29.690 And we can decide whether magnetic fields[br]are important for habitability 0:10:29.714,0:10:30.872 or not. 0:10:30.896,0:10:33.161 Once we have that answer,[br]why should you care? 0:10:33.185,0:10:34.485 I mean, I care deeply ... 0:10:36.128,0:10:38.134 And financially as well, but deeply. 0:10:38.158,0:10:40.000 (Laughter) 0:10:40.763,0:10:42.681 First of all, an answer to this question 0:10:42.705,0:10:44.808 will teach us more[br]about these three planets, 0:10:44.832,0:10:45.992 Venus, Earth and Mars, 0:10:46.016,0:10:48.927 not only about how they interact[br]with their environment today, 0:10:48.951,0:10:50.878 but how they were billions of years ago, 0:10:50.902,0:10:52.964 whether they were habitable[br]long ago or not. 0:10:52.988,0:10:54.632 It will teach us about atmospheres 0:10:54.656,0:10:56.651 that surround us and that are close. 0:10:57.127,0:10:59.311 But moreover, what we learn[br]from these planets 0:10:59.335,0:11:01.356 can be applied to atmospheres everywhere, 0:11:02.485,0:11:05.398 including planets that we're now[br]observing around other stars. 0:11:05.422,0:11:07.177 For example, the Kepler spacecraft, 0:11:07.201,0:11:10.409 which is built and controlled[br]here in Boulder, 0:11:10.433,0:11:13.718 has been observing[br]a postage stamp-sized region of the sky 0:11:13.742,0:11:14.989 for a couple years now, 0:11:15.013,0:11:17.241 and it's found thousands of planets -- 0:11:17.265,0:11:20.178 in one postage stamp-sized[br]region of the sky 0:11:20.202,0:11:24.291 that we don't think is any different[br]from any other part of the sky. 0:11:24.815,0:11:26.625 We've gone, in 20 years, 0:11:26.649,0:11:30.686 from knowing of zero planets[br]outside of our solar system, 0:11:30.710,0:11:32.463 to now having so many, 0:11:32.487,0:11:35.626 that we don't know[br]which ones to investigate first. 0:11:37.269,0:11:38.729 Any lever will help. 0:11:40.539,0:11:44.123 In fact, based on observations[br]that Kepler's taken 0:11:44.147,0:11:46.276 and other similar observations, 0:11:46.300,0:11:47.469 we now believe that, 0:11:47.493,0:11:52.192 of the 200 billion stars[br]in the Milky Way galaxy alone, 0:11:52.786,0:11:57.390 on average, every star[br]has at least one planet. 0:11:58.819,0:12:00.322 In addition to that, 0:12:00.346,0:12:06.047 estimates suggest there are somewhere[br]between 40 billion and 100 billion 0:12:06.071,0:12:09.403 of those planets[br]that we would define as habitable 0:12:11.139,0:12:12.551 in just our galaxy. 0:12:14.590,0:12:16.627 We have the observations of those planets, 0:12:16.651,0:12:19.135 but we just don't know[br]which ones are habitable yet. 0:12:19.159,0:12:22.765 It's a little bit like[br]being trapped on a red spot -- 0:12:22.789,0:12:23.960 (Laughter) 0:12:23.984,0:12:25.216 on a stage 0:12:26.178,0:12:29.740 and knowing that there are[br]other worlds out there 0:12:31.042,0:12:33.818 and desperately wanting to know[br]more about them, 0:12:35.174,0:12:39.108 wanting to interrogate them and find out[br]if maybe just one or two of them 0:12:39.132,0:12:40.742 are a little bit like you. 0:12:42.244,0:12:44.803 You can't do that.[br]You can't go there, not yet. 0:12:44.827,0:12:48.820 And so you have to use the tools[br]that you've developed around you 0:12:48.844,0:12:50.139 for Venus, Earth and Mars, 0:12:50.163,0:12:52.976 and you have to apply them[br]to these other situations, 0:12:53.000,0:12:57.696 and hope that you're making[br]reasonable inferences from the data, 0:12:57.720,0:13:00.838 and that you're going to be able[br]to determine the best candidates 0:13:00.862,0:13:03.261 for habitable planets[br]and those that are not. 0:13:04.139,0:13:06.854 In the end, and for now, at least, 0:13:06.878,0:13:09.665 this is our red spot, right here. 0:13:10.376,0:13:13.712 This is the only planet[br]that we know of that's habitable, 0:13:13.736,0:13:16.927 although very soon we may[br]come to know of more. 0:13:16.951,0:13:19.687 But for now, this is[br]the only habitable planet, 0:13:19.711,0:13:21.013 and this is our red spot. 0:13:21.976,0:13:23.396 I'm really glad we're here. 0:13:24.507,0:13:25.682 Thanks. 0:13:25.706,0:13:28.793 (Applause)