1 00:00:00,200 --> 00:00:04,560 Speaker 1: Now here's a highlight from Coast to coast am on iHeartRadio. 2 00:00:04,800 --> 00:00:07,240 Speaker 1: While you just heard from Michael Warner. And now his 3 00:00:07,360 --> 00:00:11,560 Speaker 1: colleague joins us, Peter Eisenhardt. He's a senior research scientist 4 00:00:11,640 --> 00:00:16,000 Speaker 1: at the Jet Propulsion Laboratory. He received NASA's Exceptional Scientific 5 00:00:16,000 --> 00:00:19,840 Speaker 1: Achievement Medal for his work on the Spitzer space telescope 6 00:00:19,880 --> 00:00:21,599 Speaker 1: as well. Peter, it's an honor to have you on 7 00:00:21,640 --> 00:00:24,759 Speaker 1: the program. Thank you, George. I'm glad to be here. 8 00:00:24,960 --> 00:00:27,400 Speaker 1: And you two started off. I bet as a kid 9 00:00:27,520 --> 00:00:31,560 Speaker 1: loving space, didn't you. I did. I actually was born 10 00:00:32,400 --> 00:00:35,200 Speaker 1: a couple of weeks before the Sputnik launch in nineteen 11 00:00:35,240 --> 00:00:37,280 Speaker 1: fifty seven. Uh. Oh, you know it was sort of 12 00:00:38,000 --> 00:00:42,400 Speaker 1: program to be interested in space. I guess from from childhood. 13 00:00:43,200 --> 00:00:45,519 Speaker 1: I just always knew I wanted to explore the universe, 14 00:00:45,560 --> 00:00:47,560 Speaker 1: and it just seemed like, you know, what else is 15 00:00:47,600 --> 00:00:50,080 Speaker 1: there to do. There's a little kid during spot Nick 16 00:00:50,159 --> 00:00:55,400 Speaker 1: and I remember though, everybody panicking, my parents panicking, everybody panicking. 17 00:00:55,640 --> 00:00:59,360 Speaker 1: This thing was only the size of a basketball, wasn't it. Yeah. 18 00:00:59,400 --> 00:01:02,560 Speaker 1: I think it's it's a lot heavier than in basketball, um, 19 00:01:02,600 --> 00:01:05,440 Speaker 1: and a little bit bigger. But um, but yeah, it's 20 00:01:05,480 --> 00:01:07,640 Speaker 1: it's it's not that big, and I guess there was 21 00:01:07,680 --> 00:01:10,319 Speaker 1: a lot of fear about what else would the Russians 22 00:01:10,319 --> 00:01:12,759 Speaker 1: be able to do us and uh. And of course 23 00:01:12,800 --> 00:01:16,640 Speaker 1: this led to the rapid growth of NASA and the 24 00:01:16,680 --> 00:01:19,760 Speaker 1: space program, and I was caught up in that, as 25 00:01:19,800 --> 00:01:22,360 Speaker 1: I think most people in the country were, And in 26 00:01:22,440 --> 00:01:25,440 Speaker 1: the end it turned into an exciting time for the 27 00:01:25,480 --> 00:01:28,600 Speaker 1: whole world when Neil Armstrong finally touched down just fifty 28 00:01:28,640 --> 00:01:31,080 Speaker 1: years ago. How did you make your way to JPL. 29 00:01:32,000 --> 00:01:36,320 Speaker 1: I came to JPL from from Ames Research Center in 30 00:01:36,600 --> 00:01:39,720 Speaker 1: the Bay Area. UM I was working on Spitzer there 31 00:01:39,800 --> 00:01:42,840 Speaker 1: with with Mike Corner, who heard from earlier. And I 32 00:01:42,840 --> 00:01:44,560 Speaker 1: guess Mike's going to be back a little bit later. 33 00:01:46,720 --> 00:01:50,360 Speaker 1: Being interested in astronomy as a kid, I studied it 34 00:01:50,440 --> 00:01:55,600 Speaker 1: in college, and after after doing my undergraduate work in 35 00:01:55,720 --> 00:02:00,520 Speaker 1: Philadelphia and a year off in England, um I went 36 00:02:00,560 --> 00:02:03,120 Speaker 1: to graduate school in Arizona, where the skies are really 37 00:02:03,160 --> 00:02:06,880 Speaker 1: clear and big telescopes work well. And then I went 38 00:02:06,920 --> 00:02:10,760 Speaker 1: to work on Spitzer with Mike at AIMS in nineteen 39 00:02:10,800 --> 00:02:14,480 Speaker 1: eighty seven. And then a few years later NASA decided 40 00:02:14,560 --> 00:02:18,880 Speaker 1: that Spitzer, which was then called CERTIFA would be better 41 00:02:18,919 --> 00:02:22,560 Speaker 1: built by JPL than than by AIMS, And so Mike 42 00:02:22,639 --> 00:02:25,440 Speaker 1: and I came down here in nineteen ninety with it, 43 00:02:25,480 --> 00:02:28,240 Speaker 1: and then we've been there ever since. That's fantastic. Now 44 00:02:28,280 --> 00:02:30,840 Speaker 1: today I'm told that you were last night. You were 45 00:02:30,880 --> 00:02:34,120 Speaker 1: at the Polymar Mountain area looking through its two hundred 46 00:02:34,120 --> 00:02:37,280 Speaker 1: inch telescope. That's right. Yeah, it was up till about 47 00:02:37,320 --> 00:02:40,040 Speaker 1: six am this morning. So if I'm not off a bit, 48 00:02:40,120 --> 00:02:43,280 Speaker 1: please excuse me. Well, what were you looking at? I 49 00:02:43,360 --> 00:02:50,639 Speaker 1: was studying infrared stars basically, so stars shine because of 50 00:02:50,680 --> 00:02:54,160 Speaker 1: the heat that is being generated in their course by 51 00:02:54,240 --> 00:02:57,079 Speaker 1: by nuclear fusionists, like our fusion bombs going off all 52 00:02:57,080 --> 00:03:00,639 Speaker 1: the time in the middle stars. But if you make 53 00:03:00,680 --> 00:03:04,120 Speaker 1: a star that's less and less massive, less than say, 54 00:03:04,160 --> 00:03:07,760 Speaker 1: eight percent of the mass of the Sun, those fusion 55 00:03:07,880 --> 00:03:13,160 Speaker 1: reactions can't really get going. And so a puny star 56 00:03:13,240 --> 00:03:15,160 Speaker 1: like that eight percent or less of the mass of 57 00:03:15,200 --> 00:03:18,520 Speaker 1: the Sun will shine for a while invisible light just 58 00:03:18,639 --> 00:03:21,200 Speaker 1: from the heat of its collapse. But then there's no 59 00:03:21,200 --> 00:03:25,160 Speaker 1: no fusion to replace that that light that's radiating outward, 60 00:03:25,240 --> 00:03:28,280 Speaker 1: and so it will cool off, and as it cools off, 61 00:03:28,600 --> 00:03:31,600 Speaker 1: um less and less visible light comes out um and 62 00:03:31,880 --> 00:03:34,880 Speaker 1: and it's really only detectable and infrared light. And so 63 00:03:35,240 --> 00:03:40,160 Speaker 1: what I was looking at was candidates were very very 64 00:03:40,160 --> 00:03:45,560 Speaker 1: small failed stars, basically maybe one percent of the mass 65 00:03:45,560 --> 00:03:47,440 Speaker 1: of the Sun or maybe even a half a percent 66 00:03:47,480 --> 00:03:49,920 Speaker 1: of the mass of the Sun, where you could only 67 00:03:49,960 --> 00:03:53,080 Speaker 1: pick them up in infrared light. UM. So these are 68 00:03:53,160 --> 00:03:56,040 Speaker 1: these are called brown dwarfs, And we were doing infrared 69 00:03:56,040 --> 00:04:00,240 Speaker 1: measurements from the ground with the Palmar telescope and and 70 00:04:00,360 --> 00:04:04,280 Speaker 1: trying to measure those brown dworst to see how far 71 00:04:04,320 --> 00:04:07,040 Speaker 1: away they were and how hot they were. What would 72 00:04:07,080 --> 00:04:11,000 Speaker 1: you say is the most exciting thing that Spitzer has 73 00:04:11,040 --> 00:04:15,320 Speaker 1: found for us? Well, I think there's probably no contest 74 00:04:15,920 --> 00:04:20,920 Speaker 1: with the trappist one system that Michael mentioned earlier. Just 75 00:04:20,960 --> 00:04:26,000 Speaker 1: an amazing system of planets around another star. Seven planets 76 00:04:26,839 --> 00:04:30,960 Speaker 1: earth sized, and several of them at the distance from 77 00:04:31,000 --> 00:04:34,599 Speaker 1: their star where where liquid water is possible on their surface, 78 00:04:34,640 --> 00:04:38,960 Speaker 1: so habitable planets only forty light years away from Earth. 79 00:04:39,040 --> 00:04:41,839 Speaker 1: That's that's pretty exciting, And in fact, the New York 80 00:04:41,839 --> 00:04:45,680 Speaker 1: Times had that on their front page. So that's I think, 81 00:04:45,680 --> 00:04:49,400 Speaker 1: without question number one. But but for me, I'm I'm 82 00:04:49,480 --> 00:04:53,240 Speaker 1: more into the distant universe and so I get quite 83 00:04:53,240 --> 00:04:57,600 Speaker 1: excited about the the very distant stuff. And you were 84 00:04:57,640 --> 00:05:00,680 Speaker 1: asking Michael about that how far away could be? And 85 00:05:00,760 --> 00:05:04,719 Speaker 1: so there's there's a galaxy that Spitzer has studied that 86 00:05:04,920 --> 00:05:08,960 Speaker 1: is it's ninety seven percent of the way back to 87 00:05:09,040 --> 00:05:12,000 Speaker 1: the Big Bang. It's way way far back. And so 88 00:05:12,520 --> 00:05:15,560 Speaker 1: it's just amazing to me that we can pick up 89 00:05:15,680 --> 00:05:17,760 Speaker 1: light from that early in the history of the universe 90 00:05:17,800 --> 00:05:20,200 Speaker 1: and see what was going on that that far back 91 00:05:20,360 --> 00:05:23,200 Speaker 1: in the history. When when we talked Peter about the universe, 92 00:05:23,279 --> 00:05:26,599 Speaker 1: our universe being thirteen and a half billion years old, 93 00:05:27,320 --> 00:05:34,200 Speaker 1: why isn't it twenty billion years old? Well, the why 94 00:05:34,480 --> 00:05:39,800 Speaker 1: is a tough question. I guess I don't have a 95 00:05:39,839 --> 00:05:42,520 Speaker 1: strong opinion or an informed answer for you on that. 96 00:05:42,640 --> 00:05:45,479 Speaker 1: I'm more interested in seeing the way things are than 97 00:05:45,560 --> 00:05:48,000 Speaker 1: in saying why they would have to be that way. 98 00:05:48,120 --> 00:05:50,920 Speaker 1: So there was a time not so many years ago 99 00:05:51,640 --> 00:05:55,039 Speaker 1: when astronomers thought the universe was about twenty billion years old. 100 00:05:55,760 --> 00:05:58,680 Speaker 1: And that's just from measuring the rate of expansion and 101 00:05:58,720 --> 00:06:01,720 Speaker 1: then going back words saying well, when when was all 102 00:06:01,760 --> 00:06:04,200 Speaker 1: of that stuff together in the same place and the 103 00:06:04,320 --> 00:06:07,280 Speaker 1: rate of expansion that we thought we was correct at 104 00:06:07,279 --> 00:06:09,920 Speaker 1: that time worked out to everything being in the same 105 00:06:09,960 --> 00:06:12,560 Speaker 1: place twenty billion years ago, but we've now measured that 106 00:06:12,760 --> 00:06:17,080 Speaker 1: much much more accurately, and so the answer today, to 107 00:06:17,320 --> 00:06:21,320 Speaker 1: within about a percent of accuracy, is about thirteen point 108 00:06:21,360 --> 00:06:24,279 Speaker 1: seven to thirteen point eight billion years. Isn't it amazing? Though? 109 00:06:24,400 --> 00:06:27,000 Speaker 1: To try to think how it all started? I mean, 110 00:06:27,760 --> 00:06:31,160 Speaker 1: things just don't happen. I mean, there's reason, and there's 111 00:06:31,240 --> 00:06:36,800 Speaker 1: there's organization, there's there's order to these things, and it's 112 00:06:36,880 --> 00:06:40,880 Speaker 1: just mind boggling, isn't it. It certainly is mind boggling. 113 00:06:40,920 --> 00:06:44,159 Speaker 1: And you know, it's easy for those of us who 114 00:06:44,720 --> 00:06:49,120 Speaker 1: work with these vast distances and times to kind of 115 00:06:49,160 --> 00:06:55,640 Speaker 1: forget how incredible the subject is the universe is. I mean, 116 00:06:55,720 --> 00:07:00,479 Speaker 1: life is certainly amazing as well. I would argue that 117 00:07:02,680 --> 00:07:06,880 Speaker 1: if if there were not life and the universe didn't exist, 118 00:07:06,960 --> 00:07:10,520 Speaker 1: we wouldn't be asking the question, so that that's not 119 00:07:10,880 --> 00:07:14,360 Speaker 1: not really a good answer. Um. I certainly don't rule 120 00:07:14,400 --> 00:07:16,400 Speaker 1: out the existence of God. I think that's up for 121 00:07:16,440 --> 00:07:21,720 Speaker 1: everybody to decide for themselves. But it's regardless of where 122 00:07:21,720 --> 00:07:25,640 Speaker 1: there there's some omniscient being out there who's making it 123 00:07:25,640 --> 00:07:29,840 Speaker 1: all happen, regardless of the why it is still an 124 00:07:29,840 --> 00:07:32,720 Speaker 1: amazing universe. And that's what excites me is how how 125 00:07:32,760 --> 00:07:35,240 Speaker 1: amazing the universe? Well, but but even if there's a 126 00:07:35,400 --> 00:07:40,000 Speaker 1: being like God that made this happen, how did God 127 00:07:40,080 --> 00:07:44,119 Speaker 1: start exactly right? So you know, we have a quote 128 00:07:44,120 --> 00:07:48,119 Speaker 1: in our book. Um uh it's it's called some people 129 00:07:48,240 --> 00:07:51,160 Speaker 1: I think have have heard of a song called Turtles 130 00:07:51,200 --> 00:07:55,440 Speaker 1: all the way Down. So you know, there's a little 131 00:07:55,520 --> 00:07:59,200 Speaker 1: quote that starts at chapter about galaxy clusters, which is 132 00:07:59,200 --> 00:08:03,120 Speaker 1: is a area astronomy I particularly work on, and and 133 00:08:03,600 --> 00:08:08,200 Speaker 1: it starts off by saying, well, this little old lady 134 00:08:08,200 --> 00:08:11,760 Speaker 1: says to William James, who had just given a lecture 135 00:08:11,800 --> 00:08:16,560 Speaker 1: on astronomy, says, your theory that the universe is u 136 00:08:17,600 --> 00:08:21,280 Speaker 1: is thirteen point seven billion years old and that the 137 00:08:21,320 --> 00:08:23,840 Speaker 1: Sun is on the outskirts of a galaxy is very interesting, 138 00:08:23,920 --> 00:08:27,200 Speaker 1: mister James. But I have a better theory. And he asks, well, 139 00:08:27,240 --> 00:08:30,600 Speaker 1: what's that? He says, Well, we are on the back 140 00:08:30,640 --> 00:08:34,560 Speaker 1: of a turtle, and oh, well, that's very interesting, but 141 00:08:34,600 --> 00:08:37,760 Speaker 1: what does this turtle stand on. Well, that turtle stands 142 00:08:37,800 --> 00:08:42,760 Speaker 1: on a larger turtle, and that's very interesting. But what 143 00:08:42,840 --> 00:08:47,319 Speaker 1: does this larger turtle Another question. Yeah, well a way 144 00:08:47,360 --> 00:08:50,000 Speaker 1: ahead of you, mister James. It's turtles all the way down, 145 00:08:50,120 --> 00:08:54,760 Speaker 1: so so you know it either way. Uh, it's really 146 00:08:54,760 --> 00:08:57,680 Speaker 1: a philosophical problem. Either way, it's it's hard to answer. 147 00:08:57,720 --> 00:08:59,600 Speaker 1: You know, if there's a beginning, what was there before 148 00:08:59,640 --> 00:09:02,560 Speaker 1: the beginning? Or if the universe is endless? You know, 149 00:09:02,600 --> 00:09:05,320 Speaker 1: how can that be? And you know, I think our 150 00:09:05,360 --> 00:09:11,080 Speaker 1: minds aren't quite capable of wrapping around all this. We 151 00:09:11,120 --> 00:09:16,040 Speaker 1: can speculate, but we are coming up with new discoveries 152 00:09:16,080 --> 00:09:20,160 Speaker 1: all the time, and we are learning more and more 153 00:09:20,880 --> 00:09:23,720 Speaker 1: that we never would have expected, and sometimes we're realizing 154 00:09:23,720 --> 00:09:26,120 Speaker 1: that we're not even asking the right question. I would say, Peter, 155 00:09:26,240 --> 00:09:29,680 Speaker 1: what will technology do for us that we don't even 156 00:09:30,240 --> 00:09:33,520 Speaker 1: know exists today? I mean, how far will we gain 157 00:09:33,679 --> 00:09:37,040 Speaker 1: knowledge beyond where we are today, Let's say fifty years 158 00:09:37,080 --> 00:09:43,280 Speaker 1: from now. Well, that's that's another great question, George. Fifty 159 00:09:43,320 --> 00:09:47,720 Speaker 1: years from now, I would expect that we will know 160 00:09:48,400 --> 00:09:51,920 Speaker 1: about life beyond the Earth. I think it's very likely 161 00:09:51,960 --> 00:09:55,120 Speaker 1: we will know that, and that will be probably as 162 00:09:55,120 --> 00:09:58,520 Speaker 1: exciting as any discovery ever made, to know that we 163 00:09:58,559 --> 00:10:03,760 Speaker 1: aren't alone. That's that's my prediction. You can ask me 164 00:10:03,800 --> 00:10:06,200 Speaker 1: again of course, with this program, we already believe they've 165 00:10:06,200 --> 00:10:09,960 Speaker 1: been here. But you know what, scientifically, I'd like to 166 00:10:10,000 --> 00:10:16,120 Speaker 1: find out for sure. Yeah, life is life is surprising, 167 00:10:16,200 --> 00:10:18,400 Speaker 1: and you know, we're still discovering new forms of life 168 00:10:18,480 --> 00:10:21,280 Speaker 1: right here on Earth. Life is going to surprise us 169 00:10:21,320 --> 00:10:27,600 Speaker 1: beyond the Earth, too. But our technology is advancing so greatly, 170 00:10:28,520 --> 00:10:31,160 Speaker 1: and people really want to know. They really want to know, 171 00:10:31,320 --> 00:10:35,720 Speaker 1: not just not just from a faked photograph or something 172 00:10:35,760 --> 00:10:37,800 Speaker 1: like that. They want to know for sure, is there 173 00:10:37,920 --> 00:10:41,240 Speaker 1: life outside the Earth? And and I think we know, 174 00:10:41,320 --> 00:10:44,360 Speaker 1: partly because the Spitzer, that it's very very likely. We 175 00:10:44,440 --> 00:10:48,360 Speaker 1: know that there are chemicals that are similar to those 176 00:10:48,440 --> 00:10:51,800 Speaker 1: in our own solar system and other solar systems. We 177 00:10:51,840 --> 00:10:54,400 Speaker 1: know that the structure of those other solar systems is 178 00:10:54,440 --> 00:10:57,560 Speaker 1: not that different from from ours. In some cases. We 179 00:10:57,600 --> 00:11:00,560 Speaker 1: know that there are planets where water can this around 180 00:11:00,880 --> 00:11:04,360 Speaker 1: other stars. Um, it won't be too long before I 181 00:11:04,400 --> 00:11:09,679 Speaker 1: think we're detecting liquid water around stars, around planets, on planets, 182 00:11:09,720 --> 00:11:12,640 Speaker 1: around other stars. So you know, this is this is 183 00:11:12,679 --> 00:11:16,160 Speaker 1: something that taxpayers want to know. Is this something NASA 184 00:11:16,320 --> 00:11:19,360 Speaker 1: is working on, is something astronomers are working on. And 185 00:11:20,200 --> 00:11:22,560 Speaker 1: I think the way we're going we're going to have 186 00:11:22,600 --> 00:11:25,400 Speaker 1: the answer before very long. And I think Peter, that 187 00:11:25,520 --> 00:11:30,000 Speaker 1: the primordial soup which made up us is probably the 188 00:11:30,120 --> 00:11:34,319 Speaker 1: same throughout the universe. I think the similarities are endless 189 00:11:34,360 --> 00:11:38,080 Speaker 1: out there, where other planets may have the same elements. 190 00:11:38,240 --> 00:11:40,840 Speaker 1: I don't think there's going to be anything specifically different. 191 00:11:41,080 --> 00:11:43,960 Speaker 1: I think it's all the same. What do you think? Yes, 192 00:11:44,040 --> 00:11:46,800 Speaker 1: I agree with you, George. There's there's actually good evidence 193 00:11:46,960 --> 00:11:49,440 Speaker 1: for that. One of the things that we've learned from 194 00:11:49,480 --> 00:11:52,440 Speaker 1: the from the spectra that Spitzer has taken is that 195 00:11:52,520 --> 00:11:58,520 Speaker 1: there is, oh, I'm not very glamorous molecule UM, which 196 00:11:58,600 --> 00:12:01,480 Speaker 1: is a lot like the foot you get from a barbecue. 197 00:12:01,960 --> 00:12:05,800 Speaker 1: And and there's lots of those soot particles UM in 198 00:12:06,000 --> 00:12:10,040 Speaker 1: other galaxies uh and, including in galaxies that are billions 199 00:12:10,040 --> 00:12:13,720 Speaker 1: of light years away. Uh and And so we know 200 00:12:13,800 --> 00:12:20,720 Speaker 1: the chemistry is similar in galaxies far far away early 201 00:12:20,760 --> 00:12:23,920 Speaker 1: in the history of the universe. UM. So you know, 202 00:12:24,000 --> 00:12:27,960 Speaker 1: the chemistry is there, and the planets are there, the 203 00:12:28,000 --> 00:12:30,800 Speaker 1: stars are there, and and so life is probably there too. 204 00:12:31,160 --> 00:12:34,400 Speaker 1: Listen to more Coast to Coast AM every weeknight at 205 00:12:34,440 --> 00:12:37,000 Speaker 1: one a m Eastern and go to Coast to Coast 206 00:12:37,040 --> 00:12:38,480 Speaker 1: am dot com for more