1 00:00:00,200 --> 00:00:03,480 Speaker 1: Now here's a highlight from Coast to Coast AM on 2 00:00:03,600 --> 00:00:06,920 Speaker 1: iHeartRadio and welcome back to Coast to Coast George nor 3 00:00:07,160 --> 00:00:10,040 Speaker 1: with you, Don Lincoln with Us the Scientist. Several of 4 00:00:10,080 --> 00:00:14,240 Speaker 1: his books include The Large Hadron Collider, Understanding the Universe, 5 00:00:14,360 --> 00:00:17,600 Speaker 1: Alien Universe as well. His website is linked up at 6 00:00:17,600 --> 00:00:20,160 Speaker 1: Coast to Coast AM dot com. He's also on Facebook 7 00:00:20,480 --> 00:00:23,160 Speaker 1: and he also has a YouTube channel as well. We'll 8 00:00:23,160 --> 00:00:25,120 Speaker 1: tell you how you can get to that and watch that, 9 00:00:25,400 --> 00:00:27,680 Speaker 1: you know, Don, you were saying that life is complex. 10 00:00:27,760 --> 00:00:31,320 Speaker 1: There's no question about it. But it is baffling how 11 00:00:31,680 --> 00:00:35,239 Speaker 1: a universe could create life the way we know it 12 00:00:35,400 --> 00:00:39,200 Speaker 1: right now, me talking to you people living dying. It's 13 00:00:39,320 --> 00:00:44,680 Speaker 1: it's amazing, isn't it. Well, it certainly is, um you know, 14 00:00:44,720 --> 00:00:51,360 Speaker 1: but there's sort of levels of fascinating fascination. Life, you know, 15 00:00:51,720 --> 00:00:56,040 Speaker 1: is biochemistry, but it all is predicated on even deeper laws, 16 00:00:56,120 --> 00:01:01,360 Speaker 1: like you know, the the chemistry of the carbon and 17 00:01:01,440 --> 00:01:04,679 Speaker 1: oxygen still forth that make up us. It's tied to 18 00:01:04,920 --> 00:01:08,480 Speaker 1: the properties of the particles that make up the atoms, 19 00:01:08,600 --> 00:01:12,000 Speaker 1: which is the stuff that that I study. The deeper laws, 20 00:01:12,520 --> 00:01:14,800 Speaker 1: the ones that that you know make the universe come 21 00:01:14,840 --> 00:01:18,080 Speaker 1: to people. Once that you have those laws, then it's 22 00:01:18,120 --> 00:01:22,319 Speaker 1: sort of inevitable that you will get complex chemistry. Now, 23 00:01:22,360 --> 00:01:25,479 Speaker 1: whether that complex chemistry turns into life, well that's an 24 00:01:25,480 --> 00:01:28,920 Speaker 1: open question. After all, when you look out, um, you know, 25 00:01:29,000 --> 00:01:31,959 Speaker 1: here on Earth, there's it seems that life was formed 26 00:01:32,880 --> 00:01:35,400 Speaker 1: at one time. I mean it, I suppose it could 27 00:01:35,400 --> 00:01:37,840 Speaker 1: have started and stopped a few times. But the last 28 00:01:37,840 --> 00:01:40,759 Speaker 1: time I get started pretty good it it took off. 29 00:01:41,319 --> 00:01:46,800 Speaker 1: So um, you know, I admit that it's a completely 30 00:01:46,840 --> 00:01:50,360 Speaker 1: fascinating question of how that came to be, But the 31 00:01:50,560 --> 00:01:53,960 Speaker 1: idea of chemistry is not so striking. It's you know, 32 00:01:54,240 --> 00:01:58,640 Speaker 1: but whether or not the form of life chemistry is inevitable, 33 00:01:59,200 --> 00:02:00,680 Speaker 1: you know, we're going to have to find life on 34 00:02:00,720 --> 00:02:03,880 Speaker 1: another planet before before we know that this is really 35 00:02:04,080 --> 00:02:07,600 Speaker 1: a common thing or not. Well, absolutely, But would it 36 00:02:07,640 --> 00:02:12,160 Speaker 1: not be very unusual, especially with the billions of stars 37 00:02:12,200 --> 00:02:14,680 Speaker 1: we have in the universe and the millions of planets 38 00:02:14,680 --> 00:02:17,200 Speaker 1: that we have, and many of them goldilock like us, 39 00:02:17,760 --> 00:02:20,240 Speaker 1: that we would be the only ones in this vast 40 00:02:20,360 --> 00:02:25,760 Speaker 1: universe to be here. Well, we can't generalize, I mean, 41 00:02:26,000 --> 00:02:30,040 Speaker 1: scientifically speaking, it's difficult to generalize on you know, a 42 00:02:30,120 --> 00:02:32,560 Speaker 1: single example, and all we have is is what we 43 00:02:32,639 --> 00:02:35,480 Speaker 1: see here. But I would grant you that that I 44 00:02:35,520 --> 00:02:39,440 Speaker 1: think what you said is true, and there's actually, you know, 45 00:02:39,720 --> 00:02:43,960 Speaker 1: some evidence here on Earth that makes me that supports that. 46 00:02:45,120 --> 00:02:47,040 Speaker 1: You know, we know sort of how the Earth was 47 00:02:47,080 --> 00:02:51,240 Speaker 1: formed by planetesimals, you know, crashing into one another and 48 00:02:51,240 --> 00:02:53,960 Speaker 1: heating up, and eventually you had the Earth, but it 49 00:02:54,040 --> 00:02:57,480 Speaker 1: was just this molten ball of rock. However, as soon 50 00:02:57,520 --> 00:03:01,280 Speaker 1: as the Earth cooled and water started to form, we 51 00:03:01,360 --> 00:03:05,600 Speaker 1: find that life formed here on Earth really very quickly 52 00:03:05,720 --> 00:03:10,079 Speaker 1: after the Earth cooled enough to sustain liquid water. And 53 00:03:10,120 --> 00:03:15,280 Speaker 1: so that's not a definitive answer, but the fact that 54 00:03:15,320 --> 00:03:17,160 Speaker 1: it didn't take a long time. It's not like the 55 00:03:17,200 --> 00:03:20,320 Speaker 1: Earth cooled and there was water and it took billions 56 00:03:20,320 --> 00:03:23,800 Speaker 1: and billions of years and then life formed. It's almost 57 00:03:23,880 --> 00:03:27,080 Speaker 1: immediately after it got cooled that life forms. So that 58 00:03:27,200 --> 00:03:29,320 Speaker 1: suggests to me that when you do look at all 59 00:03:29,320 --> 00:03:33,720 Speaker 1: those other planets that you talked about, that it's almost 60 00:03:34,360 --> 00:03:36,200 Speaker 1: I would say, this is no an opinion, it's not 61 00:03:36,240 --> 00:03:39,680 Speaker 1: a scientific fact, but I think it's almost inevitable that 62 00:03:39,800 --> 00:03:43,360 Speaker 1: life is incredibly common throughout the cosmos. What the hecked 63 00:03:43,480 --> 00:03:48,480 Speaker 1: on are black holes? What are those things? Black holes 64 00:03:48,560 --> 00:03:52,960 Speaker 1: are just crazy. What black holes are typically are the 65 00:03:53,200 --> 00:03:57,000 Speaker 1: burnt out hult husks of stars that once exploded, so 66 00:03:57,040 --> 00:04:00,840 Speaker 1: they were ginormous stars, much larger than ours. They burn 67 00:04:00,960 --> 00:04:05,040 Speaker 1: through their fuel, They they gave up, they died, and 68 00:04:05,280 --> 00:04:09,560 Speaker 1: when in doing so, they collapsed. They collapsed and the 69 00:04:09,840 --> 00:04:14,960 Speaker 1: outer levels of the stars. Does every star do that, 70 00:04:15,040 --> 00:04:17,760 Speaker 1: by the way, No, all the stars that are actually 71 00:04:17,800 --> 00:04:21,320 Speaker 1: pretty heavy, so you know, more than a I don't know, 72 00:04:21,360 --> 00:04:24,440 Speaker 1: eight times the side the mass of our star, for instance, 73 00:04:24,440 --> 00:04:27,840 Speaker 1: our star will not be a black hole will end up. 74 00:04:27,839 --> 00:04:29,920 Speaker 1: What it'll do is it'll burn through all its fuel. 75 00:04:30,320 --> 00:04:33,240 Speaker 1: It will do some pretty amazing gyrations before it dies. 76 00:04:33,279 --> 00:04:35,479 Speaker 1: I mean, it will puff up until what's called a 77 00:04:35,560 --> 00:04:39,040 Speaker 1: red giant. That giant the size of that red giant 78 00:04:39,080 --> 00:04:42,960 Speaker 1: star will almost certainly encompass the orbit of the Earth, 79 00:04:43,000 --> 00:04:45,440 Speaker 1: so the Earth will melt. But then when all of 80 00:04:45,520 --> 00:04:49,040 Speaker 1: the fuel is used up, what will happen is the 81 00:04:50,000 --> 00:04:54,760 Speaker 1: heat will will turn off. The mass of the star 82 00:04:54,880 --> 00:04:58,640 Speaker 1: will collapse down into what's called a white dwarf, so 83 00:04:58,680 --> 00:05:02,159 Speaker 1: it'll be a very small star, like a hot glowing 84 00:05:02,200 --> 00:05:05,360 Speaker 1: number that just sort of slowly dies out over hundreds 85 00:05:05,400 --> 00:05:07,960 Speaker 1: of billions of years. But getting back to your question 86 00:05:08,000 --> 00:05:10,720 Speaker 1: of the black hole, So in a star that is 87 00:05:10,880 --> 00:05:14,640 Speaker 1: enormous and it explodes and it drives a lot of 88 00:05:14,720 --> 00:05:18,920 Speaker 1: the mask down into a very very small volume. It 89 00:05:18,960 --> 00:05:22,360 Speaker 1: gets to be so small, with so much mass packed 90 00:05:22,400 --> 00:05:25,800 Speaker 1: into it, that the gravity becomes so strong that not 91 00:05:25,920 --> 00:05:28,680 Speaker 1: even light can escape. So that's why it's called a 92 00:05:28,680 --> 00:05:33,719 Speaker 1: black hole. Black Holes, they're very, very bizarre some people. 93 00:05:34,279 --> 00:05:36,240 Speaker 1: You know, if you listen to people, they'll say that 94 00:05:36,720 --> 00:05:40,560 Speaker 1: the black hole has a zero size, and that's probably 95 00:05:40,600 --> 00:05:43,680 Speaker 1: not true, but it is that it is incredibly small, 96 00:05:44,240 --> 00:05:46,680 Speaker 1: and so you can't get to the center of a 97 00:05:46,680 --> 00:05:51,960 Speaker 1: black hole because, if you know, the gravity changes as 98 00:05:52,000 --> 00:05:54,600 Speaker 1: a function of distance from the center, So at the 99 00:05:54,600 --> 00:05:58,799 Speaker 1: center gravity is ridiculous. But even at some distances where 100 00:05:59,120 --> 00:06:02,599 Speaker 1: you know it's not huge, it's a kilometer or something 101 00:06:02,640 --> 00:06:05,479 Speaker 1: like that, that's where the gravity is so big that 102 00:06:05,880 --> 00:06:08,560 Speaker 1: light can escape from it. Would it rip you apart 103 00:06:08,720 --> 00:06:11,520 Speaker 1: if you were going into it with a spacecraft, if 104 00:06:11,680 --> 00:06:15,440 Speaker 1: you were to fall. So that's actually interesting and it's 105 00:06:15,480 --> 00:06:18,560 Speaker 1: absolutely counterintuitive because there are two kinds of black holes 106 00:06:18,920 --> 00:06:21,920 Speaker 1: of which we're familiar. One is the black hole, which 107 00:06:21,960 --> 00:06:24,440 Speaker 1: is the death of a star. And the other is 108 00:06:24,480 --> 00:06:27,440 Speaker 1: a super huge black hole at the center of galaxies 109 00:06:27,480 --> 00:06:30,320 Speaker 1: which have masses of millions of which we've got in 110 00:06:30,320 --> 00:06:33,120 Speaker 1: the Milky Way, don't, which we do in all galaxies 111 00:06:33,240 --> 00:06:35,520 Speaker 1: seem to have that. So if you were to fall 112 00:06:35,560 --> 00:06:41,000 Speaker 1: into the a star size, a stellar size black hole, 113 00:06:41,480 --> 00:06:43,919 Speaker 1: as you were to fall into it, what would happen 114 00:06:44,080 --> 00:06:46,960 Speaker 1: is the gravity on your feet would be so much stronger, 115 00:06:47,040 --> 00:06:49,039 Speaker 1: say than the gravity on your head if you're falling 116 00:06:49,080 --> 00:06:53,320 Speaker 1: feet first, that the gravity would pull you apart. It's 117 00:06:53,320 --> 00:06:56,919 Speaker 1: called spaghetification, which is kind of a neat name for 118 00:06:56,960 --> 00:07:00,560 Speaker 1: what would undoubtedly be a painful and grizzly death. Now, 119 00:07:01,040 --> 00:07:03,239 Speaker 1: if you were to fall into one of these super 120 00:07:03,279 --> 00:07:08,400 Speaker 1: massive black holes, and it's very counterintuitive, but in that case, 121 00:07:08,560 --> 00:07:11,200 Speaker 1: you would not get pulled apart. And the reason there 122 00:07:11,800 --> 00:07:15,240 Speaker 1: is while the gravity is very strong, the gravity difference 123 00:07:15,400 --> 00:07:17,400 Speaker 1: from your feet and your head is not very much, 124 00:07:17,680 --> 00:07:19,440 Speaker 1: and so you would just fall into the black hole 125 00:07:19,480 --> 00:07:21,440 Speaker 1: and you would not get pulled apart. But what would 126 00:07:21,480 --> 00:07:23,600 Speaker 1: you see? What would you see don as you're being 127 00:07:23,640 --> 00:07:28,160 Speaker 1: pulled into it. Well, if you were to look towards 128 00:07:28,200 --> 00:07:30,600 Speaker 1: the black hole, you would see the matter that was 129 00:07:30,640 --> 00:07:32,600 Speaker 1: falling in ahead of you, and you would see it 130 00:07:32,640 --> 00:07:35,240 Speaker 1: being very red. And if you turn to look at 131 00:07:35,280 --> 00:07:40,160 Speaker 1: the outside universe, the universe you know that you're leaving behind, 132 00:07:40,760 --> 00:07:42,880 Speaker 1: you would see all of the stars, but they'd all 133 00:07:42,960 --> 00:07:46,360 Speaker 1: be very much bluer than they were. And that's because 134 00:07:47,200 --> 00:07:52,640 Speaker 1: as light falls into a black hole, it it essentially 135 00:07:52,640 --> 00:07:55,040 Speaker 1: picks up energy as it goes into the black hole, 136 00:07:55,080 --> 00:07:58,400 Speaker 1: and it gets bluer and bluer because blue light has 137 00:07:58,440 --> 00:08:03,120 Speaker 1: more energy than um. You know, then ordinarily, well, I'm 138 00:08:03,120 --> 00:08:05,440 Speaker 1: thinking of a black hole almost as if you're looking 139 00:08:05,600 --> 00:08:09,160 Speaker 1: at a water going down a drain, how it swirls. 140 00:08:09,800 --> 00:08:14,280 Speaker 1: Would that be the same kind of thing? Um, You know, 141 00:08:14,480 --> 00:08:19,800 Speaker 1: all analogies suffer from from some you know, weaknesses. But 142 00:08:19,880 --> 00:08:23,480 Speaker 1: there's some truth to that, now, not all. I mean, 143 00:08:23,800 --> 00:08:26,680 Speaker 1: in principal, black holes don't have to rotate, so that 144 00:08:26,760 --> 00:08:30,640 Speaker 1: the swirling analogy is really a very accurate one for 145 00:08:30,720 --> 00:08:33,600 Speaker 1: a black hole that's rotating. But of course many do 146 00:08:33,760 --> 00:08:36,760 Speaker 1: because if the star that made the black hole was rotating, 147 00:08:36,800 --> 00:08:40,400 Speaker 1: then the black hole itself will rotate. But it's not necessary. 148 00:08:40,440 --> 00:08:43,040 Speaker 1: They don't have to rotate, so you could, you know, 149 00:08:43,040 --> 00:08:45,920 Speaker 1: occasionally you could have water go down a drain and 150 00:08:46,000 --> 00:08:50,079 Speaker 1: that's not swirling in a little vortex. So you know, yeah, 151 00:08:50,160 --> 00:08:53,320 Speaker 1: your analogy isn't too too bad. Not bad for a 152 00:08:53,360 --> 00:08:58,800 Speaker 1: non scientist, huh, not even bad for a scientist. Now, 153 00:08:59,360 --> 00:09:02,240 Speaker 1: does the black hole come to an end? And by 154 00:09:02,280 --> 00:09:05,439 Speaker 1: that I mean, can you, in theory reach the end 155 00:09:05,480 --> 00:09:10,040 Speaker 1: of it and like bounce into a wall or something. Well, 156 00:09:11,559 --> 00:09:14,520 Speaker 1: that's a good question and it's not one that I 157 00:09:14,559 --> 00:09:18,960 Speaker 1: can answer definitively. So I'd like to distinguish between two 158 00:09:19,160 --> 00:09:22,120 Speaker 1: sort of different ways of thinking. There's what you know 159 00:09:22,200 --> 00:09:24,520 Speaker 1: from data, what you know from measurements, what you know 160 00:09:24,600 --> 00:09:27,719 Speaker 1: from looking and seeing, and then there's what you know 161 00:09:28,320 --> 00:09:32,560 Speaker 1: from taking your theory your mathematics and finding out what 162 00:09:32,760 --> 00:09:36,640 Speaker 1: the mathematics tells you. So what the mathematics tells you 163 00:09:36,760 --> 00:09:39,920 Speaker 1: is you fall into a black hole. It's there's no 164 00:09:40,040 --> 00:09:43,080 Speaker 1: bounce or anything. What happens is everything gets smaller and 165 00:09:43,120 --> 00:09:48,400 Speaker 1: smaller and smaller until you get to you at the 166 00:09:48,400 --> 00:09:51,280 Speaker 1: simplest mathematics, you get down to literal zero size. So 167 00:09:51,320 --> 00:09:53,760 Speaker 1: you get down to the very very center and everything 168 00:09:53,880 --> 00:09:57,199 Speaker 1: is crushed to zero size. Now we think that's probably wrong, 169 00:09:57,400 --> 00:09:59,719 Speaker 1: but we also think that it's not so wrong. So 170 00:09:59,840 --> 00:10:02,200 Speaker 1: the so we get to between a very small that's 171 00:10:02,240 --> 00:10:07,000 Speaker 1: the theoretical prediction, and that's, you know, our best understanding. 172 00:10:07,640 --> 00:10:10,840 Speaker 1: But from the from someone like me who's an experimentalist 173 00:10:10,840 --> 00:10:15,560 Speaker 1: who bases my conclusions on what we're able to see 174 00:10:15,600 --> 00:10:19,280 Speaker 1: and measure, we actually can't answer that question because there 175 00:10:19,480 --> 00:10:23,079 Speaker 1: is this thing called the event horizon, and the event 176 00:10:23,120 --> 00:10:29,240 Speaker 1: horizon is a sphere around the black hole where where 177 00:10:29,280 --> 00:10:32,480 Speaker 1: the gravity is so strong that light can escape. So 178 00:10:33,000 --> 00:10:35,920 Speaker 1: if you're on the outside watching something fall into the 179 00:10:35,960 --> 00:10:40,280 Speaker 1: black hole, you can't see inside the event horizon because 180 00:10:40,559 --> 00:10:42,600 Speaker 1: the gravity is so strong, light can't get back to you, 181 00:10:42,640 --> 00:10:47,120 Speaker 1: so you don't We don't literally know from from observation 182 00:10:47,320 --> 00:10:50,120 Speaker 1: what actually is going to happen inside there. So you 183 00:10:50,120 --> 00:10:52,079 Speaker 1: have to be careful when you talk about black holes, 184 00:10:52,360 --> 00:10:56,000 Speaker 1: what you see versus what you predict from your mathematics. 185 00:10:56,840 --> 00:11:00,720 Speaker 1: That's fascinating it truly is it Is it possible that 186 00:11:00,840 --> 00:11:07,199 Speaker 1: black holes connect you to another universe a multiverse? Yeah? Well, 187 00:11:07,240 --> 00:11:10,600 Speaker 1: as I said, you know, since we can't look inside, 188 00:11:10,640 --> 00:11:14,360 Speaker 1: there's some room for some speculation. That doesn't seem to 189 00:11:14,440 --> 00:11:17,760 Speaker 1: be the case. We don't think that black holes will 190 00:11:17,800 --> 00:11:21,800 Speaker 1: connect to two different universes. There is some mathematics that 191 00:11:21,920 --> 00:11:24,680 Speaker 1: says that two black holes can connect to one another. 192 00:11:25,160 --> 00:11:28,160 Speaker 1: So you could have a black hole, say here near 193 00:11:28,200 --> 00:11:32,680 Speaker 1: the Earth hypothetically, and another one halfway across the galaxy, 194 00:11:33,080 --> 00:11:36,040 Speaker 1: and those two black holes could connect to each other 195 00:11:36,559 --> 00:11:40,439 Speaker 1: in what's called a wormhole, which is very hypothetical and 196 00:11:41,120 --> 00:11:43,960 Speaker 1: maybe not something one should believe. But if it's true, 197 00:11:44,400 --> 00:11:48,200 Speaker 1: then it could be that this wormhole is like a 198 00:11:48,240 --> 00:11:51,600 Speaker 1: doorway between these two black holes, so that even though 199 00:11:51,600 --> 00:11:53,480 Speaker 1: if you were to go through normal space it might 200 00:11:53,559 --> 00:11:55,920 Speaker 1: take you tens of thousands of years to travel from 201 00:11:55,960 --> 00:11:58,679 Speaker 1: one to the other, going through the wormholes, you could 202 00:11:59,480 --> 00:12:01,959 Speaker 1: it's like a step from one side to the other. Now, 203 00:12:02,000 --> 00:12:05,720 Speaker 1: there's some downsides to that. If what I just told 204 00:12:05,720 --> 00:12:08,800 Speaker 1: you about wormholes is one of those mathematical predictions, and 205 00:12:08,960 --> 00:12:12,120 Speaker 1: one of the weirdnesses of the mathematical predictions is it 206 00:12:12,120 --> 00:12:15,240 Speaker 1: can only happen if there's a kind of energy called 207 00:12:15,320 --> 00:12:17,800 Speaker 1: negative energy, which is no one's ever seen before. It 208 00:12:17,840 --> 00:12:20,640 Speaker 1: may not exist, So this just may be some math 209 00:12:20,760 --> 00:12:24,200 Speaker 1: thing that isn't true. So that's the first thing. And 210 00:12:24,240 --> 00:12:26,719 Speaker 1: the second thing is, like we said, just a moment ago, 211 00:12:26,720 --> 00:12:29,600 Speaker 1: when you fall into a black hole, you get ripped apart. 212 00:12:29,880 --> 00:12:32,520 Speaker 1: So it may be that those two black holes connect 213 00:12:32,559 --> 00:12:34,360 Speaker 1: one another, but if they do, you're still going to 214 00:12:34,400 --> 00:12:37,960 Speaker 1: get ripped apart falling into one. And you know, so 215 00:12:38,040 --> 00:12:40,520 Speaker 1: it doesn't really work like it does in science fiction. 216 00:12:40,720 --> 00:12:43,760 Speaker 1: With everything you've worked on, don and will work on, 217 00:12:44,240 --> 00:12:49,199 Speaker 1: what's that one question that you would love answered? You know, 218 00:12:50,000 --> 00:12:54,599 Speaker 1: the questions that I ask? And I mean Albert Einstein 219 00:12:54,760 --> 00:12:57,080 Speaker 1: was once asked sort of what he wanted to know, 220 00:12:57,400 --> 00:12:59,600 Speaker 1: and what he said is, you know, I'm not interested 221 00:12:59,640 --> 00:13:03,400 Speaker 1: in the you know, the the light that comes off 222 00:13:03,440 --> 00:13:05,360 Speaker 1: from this or that element. He doesn't want to know 223 00:13:05,400 --> 00:13:07,560 Speaker 1: some of the details of the chemistry of a certain 224 00:13:08,080 --> 00:13:12,640 Speaker 1: specific material. What he wants to know is God's thoughts. 225 00:13:12,679 --> 00:13:15,200 Speaker 1: The rest are just details. Now, he did not believe 226 00:13:15,240 --> 00:13:19,080 Speaker 1: in a literal God, but it's a lovely metaphor. And 227 00:13:19,520 --> 00:13:22,920 Speaker 1: basically what he wanted to know was the answer to everything. 228 00:13:23,160 --> 00:13:25,960 Speaker 1: How does it all hang together? Why? Or things the 229 00:13:25,960 --> 00:13:29,920 Speaker 1: way they are? And he thought about that his entire life, 230 00:13:29,920 --> 00:13:32,640 Speaker 1: and he died not knowing. But this is the sort 231 00:13:32,679 --> 00:13:34,480 Speaker 1: of question that I'd like to know the answer. I mean, 232 00:13:34,520 --> 00:13:37,280 Speaker 1: I really would like to know how come we are? 233 00:13:37,480 --> 00:13:39,720 Speaker 1: How we are. I mean, it didn't seem it doesn't 234 00:13:39,720 --> 00:13:41,760 Speaker 1: seem like it has to be that way. There's got 235 00:13:41,760 --> 00:13:44,040 Speaker 1: to be a reason. And you know, we're not going 236 00:13:44,080 --> 00:13:47,160 Speaker 1: to figure this out in my lifetime or or you know, 237 00:13:47,240 --> 00:13:50,080 Speaker 1: my great great grandchildren's lifetime. It's a it's a journey 238 00:13:50,080 --> 00:13:53,680 Speaker 1: of millennia. But you know, I'm hoping to find a 239 00:13:53,720 --> 00:13:56,960 Speaker 1: little peace on that journey. Well, I think so. I 240 00:13:57,000 --> 00:14:02,080 Speaker 1: think we'll get to that point indeed. And it's just 241 00:14:02,200 --> 00:14:07,480 Speaker 1: fascinating what science is doing, this technology helping us get 242 00:14:07,520 --> 00:14:11,160 Speaker 1: to that or is it just still brainpower? No, I 243 00:14:11,200 --> 00:14:15,000 Speaker 1: mean it has to be technology, because you know, brainpower 244 00:14:15,160 --> 00:14:18,080 Speaker 1: is amazing. But the fact of the matter is that 245 00:14:18,160 --> 00:14:21,360 Speaker 1: the human mind is enormously inventive. They can think of 246 00:14:21,400 --> 00:14:25,520 Speaker 1: all sorts of possible ideas, possible answers to the questions 247 00:14:25,560 --> 00:14:28,840 Speaker 1: that plague us. But you know, just like you can 248 00:14:28,920 --> 00:14:31,520 Speaker 1: go to a library and you go to the science 249 00:14:31,560 --> 00:14:34,600 Speaker 1: fiction section, there are all sorts of need ideas that 250 00:14:34,680 --> 00:14:38,440 Speaker 1: people have played with and explored that aren't actually true. 251 00:14:38,440 --> 00:14:42,280 Speaker 1: They're just really cool ideas. So it's only through having 252 00:14:42,360 --> 00:14:45,640 Speaker 1: those need ideas and having technology where you can test 253 00:14:45,720 --> 00:14:49,320 Speaker 1: all the interesting hypotheses and you find the one that 254 00:14:49,360 --> 00:14:53,040 Speaker 1: the universe happens to be so no, this technology is 255 00:14:53,040 --> 00:14:57,760 Speaker 1: crucial in pursuing these timeless questions. Listen to more Coast 256 00:14:57,760 --> 00:15:01,320 Speaker 1: to Coast AM every weeknight at one am Eastern, and 257 00:15:01,600 --> 00:15:04,479 Speaker 1: go to Coast to Coast am dot com for more