1 00:00:00,200 --> 00:00:03,440 Speaker 1: Now here's a highlight from Coast to Coast AM on 2 00:00:03,600 --> 00:00:06,720 Speaker 1: iHeart Radio and welcome back to Coast to Coast George 3 00:00:06,760 --> 00:00:09,520 Speaker 1: Nori with you, Marcus Charming with us as we will 4 00:00:09,560 --> 00:00:12,520 Speaker 1: be talking about all things space. What is it about 5 00:00:12,520 --> 00:00:17,120 Speaker 1: the universe that excites you, Marcus? I suppose the most 6 00:00:17,160 --> 00:00:22,239 Speaker 1: exciting thing for me at the moment is that we 7 00:00:22,280 --> 00:00:25,080 Speaker 1: can only see two and a half percent of it. Okay, 8 00:00:25,120 --> 00:00:27,680 Speaker 1: so we've now discovered, incredibly, after three hundred and fifty 9 00:00:27,720 --> 00:00:33,080 Speaker 1: years or so, that the visible stuff, the start and galaxies, 10 00:00:33,120 --> 00:00:38,400 Speaker 1: the planets, and the accounts for five percent of the universe, 11 00:00:38,440 --> 00:00:40,440 Speaker 1: five percent of the matter at the universe, and only 12 00:00:40,520 --> 00:00:42,600 Speaker 1: half of that five percent two and a half percent, 13 00:00:42,680 --> 00:00:45,080 Speaker 1: if we actually seen with our telescopes the rest of it. 14 00:00:45,159 --> 00:00:47,720 Speaker 1: We think it might be invisible gas between the galaxies, 15 00:00:48,120 --> 00:00:51,240 Speaker 1: it's only five percent, and it turns out that there 16 00:00:51,360 --> 00:00:56,640 Speaker 1: is about twenty five percent is what we call dark matter. Okay. 17 00:00:56,120 --> 00:00:58,960 Speaker 1: We know it's out there because we can see it 18 00:00:59,120 --> 00:01:00,960 Speaker 1: pulling on the visible stuff. So we see all the 19 00:01:01,000 --> 00:01:03,880 Speaker 1: visible stuff and moving in ways we would not expect. 20 00:01:04,319 --> 00:01:06,440 Speaker 1: So we say, this stuff that's got gravity, but we 21 00:01:06,760 --> 00:01:10,480 Speaker 1: literally can't see it. And about seventy percent is what 22 00:01:10,520 --> 00:01:12,760 Speaker 1: we call dark energy, and that was only discovered in 23 00:01:12,840 --> 00:01:15,320 Speaker 1: nineteen ninety eight. Can you believe it? The major mass 24 00:01:15,319 --> 00:01:18,679 Speaker 1: component of the universe we didn't know about until nineteen 25 00:01:18,760 --> 00:01:22,520 Speaker 1: ninety eight, which is like twenty two years ago. And 26 00:01:23,040 --> 00:01:26,679 Speaker 1: we've got really very little idea what dark energy and 27 00:01:26,760 --> 00:01:29,640 Speaker 1: dark matter are, so really we're in this weird position. 28 00:01:29,680 --> 00:01:32,640 Speaker 1: Imagine if Darwin was going to come up with his 29 00:01:32,720 --> 00:01:36,160 Speaker 1: theory evolution and he only knew about frogs and snakes, 30 00:01:36,680 --> 00:01:38,560 Speaker 1: but he didn't know about insects, and he didn't know 31 00:01:38,600 --> 00:01:41,480 Speaker 1: about fish or most of the things in the animal kingdom. 32 00:01:41,520 --> 00:01:43,920 Speaker 1: I mean, what kind of theory would he have concocted? 33 00:01:44,480 --> 00:01:49,520 Speaker 1: They of cosmology, and we only know it's based on 34 00:01:49,960 --> 00:01:51,960 Speaker 1: that the two a half or the fire descent that 35 00:01:52,000 --> 00:01:53,920 Speaker 1: we can see. So I think that's pretty amazing that 36 00:01:53,960 --> 00:01:57,000 Speaker 1: most of the universe is invisible. So if anyone think 37 00:01:57,040 --> 00:01:59,480 Speaker 1: out there any kids who want to go into France 38 00:01:59,720 --> 00:02:02,279 Speaker 1: and I think it's all sewn up and there's nothing 39 00:02:02,320 --> 00:02:05,480 Speaker 1: more to don't We don't actually know what most of 40 00:02:05,480 --> 00:02:07,320 Speaker 1: the universe is made of. So I find that very 41 00:02:07,400 --> 00:02:10,520 Speaker 1: very exciting. And when you say it's invisible, but it's there. 42 00:02:11,000 --> 00:02:13,600 Speaker 1: Does that mean in theory, if you launched a rocket 43 00:02:13,639 --> 00:02:19,120 Speaker 1: toward it, could you crash into it? You couldn't crash 44 00:02:19,200 --> 00:02:22,639 Speaker 1: into it because one of the one of its characteristic 45 00:02:22,760 --> 00:02:25,560 Speaker 1: is that it doesn't give out a light Okay, So 46 00:02:25,840 --> 00:02:29,079 Speaker 1: what we mean is it doesn't interact with light, and 47 00:02:29,360 --> 00:02:33,000 Speaker 1: light is a product of what we call the electromagnetic force, 48 00:02:33,040 --> 00:02:35,359 Speaker 1: So it doesn't interact with the electromagnetic force. So the 49 00:02:35,400 --> 00:02:40,600 Speaker 1: electromaetic agnetic force is responsible for kind of the repulsion. 50 00:02:40,720 --> 00:02:42,440 Speaker 1: So the reason that if you try it, I don't know, 51 00:02:42,480 --> 00:02:47,080 Speaker 1: if you'll put your hand on the cabinet vehicle or 52 00:02:46,760 --> 00:02:49,440 Speaker 1: on a desk, you can feel that your fingers don't 53 00:02:49,480 --> 00:02:53,280 Speaker 1: go through that desk is because there's a repulsion, an 54 00:02:53,280 --> 00:02:56,519 Speaker 1: electric repulsion between the electrons and the atoms in your 55 00:02:56,520 --> 00:02:59,520 Speaker 1: fingers and the electrons in the atoms in your in 56 00:02:59,560 --> 00:03:03,359 Speaker 1: the tabe. Okay, Now, dark matter doesn't feel that. It 57 00:03:03,440 --> 00:03:07,720 Speaker 1: doesn't don't experience that. So literally you would fry straight 58 00:03:07,800 --> 00:03:11,040 Speaker 1: through the dark matter as if it wasn't there, you know, 59 00:03:11,120 --> 00:03:14,000 Speaker 1: So you would crash into it at all, you know. 60 00:03:14,440 --> 00:03:17,320 Speaker 1: So I mean, so the dark matter, as far as 61 00:03:17,360 --> 00:03:19,600 Speaker 1: we know, the dark matter is in the you know, 62 00:03:19,800 --> 00:03:22,760 Speaker 1: it's in the studio where you're actually, you know, talking 63 00:03:22,760 --> 00:03:24,440 Speaker 1: to me from, it's in the room where I'm talking 64 00:03:24,440 --> 00:03:27,680 Speaker 1: to you from. It's it is everywhere, but it doesn't 65 00:03:27,720 --> 00:03:30,520 Speaker 1: interact with normal matter, so it doesn't bump into normal 66 00:03:30,800 --> 00:03:33,280 Speaker 1: matter in any way. And that's why we can't we 67 00:03:33,360 --> 00:03:36,200 Speaker 1: can't detect that. That's strange. How do we know what's 68 00:03:36,240 --> 00:03:40,880 Speaker 1: there simply because we well, if you say, I'll go 69 00:03:40,960 --> 00:03:45,000 Speaker 1: back to my book The Magicians, because the first magician 70 00:03:45,320 --> 00:03:48,160 Speaker 1: was a guy called Urban the Verier, and he deduced 71 00:03:48,360 --> 00:03:51,040 Speaker 1: that there had to be another planet because there was 72 00:03:51,080 --> 00:03:53,840 Speaker 1: a planet Uranus or Uranus however you'd like to pronounce it, 73 00:03:54,040 --> 00:03:56,400 Speaker 1: and it wasn't orbiting the Sun in the right way. 74 00:03:56,760 --> 00:04:00,480 Speaker 1: It was weird. It's allbit. So he passed. But there 75 00:04:00,480 --> 00:04:04,520 Speaker 1: had to exist another planet further out whose gravity was 76 00:04:05,040 --> 00:04:08,600 Speaker 1: pulling on on Neptune and perturbing its orbit, and it 77 00:04:09,600 --> 00:04:12,760 Speaker 1: predicted exist as a Neptune. Well, dark matter is simply 78 00:04:12,840 --> 00:04:16,719 Speaker 1: the Neptune of today. You know, we see things moving. 79 00:04:16,800 --> 00:04:20,719 Speaker 1: So for instance, we see fars orbiting around the cause 80 00:04:20,760 --> 00:04:23,960 Speaker 1: of their galaxies and they're meeting too fast. By rights, 81 00:04:24,200 --> 00:04:27,480 Speaker 1: they should be flying off into intermactic space. So what 82 00:04:27,520 --> 00:04:31,960 Speaker 1: we infer is that there's more matter whose extra gravity 83 00:04:32,040 --> 00:04:34,800 Speaker 1: is gripping onto them. So it's rather likely it is 84 00:04:34,839 --> 00:04:37,239 Speaker 1: just like Neptune. You know, it's because things are moving. 85 00:04:37,720 --> 00:04:41,080 Speaker 1: We see things moving in a way that we cannot 86 00:04:41,120 --> 00:04:45,680 Speaker 1: explain from the visible far than gravity and a starting 87 00:04:45,680 --> 00:04:49,320 Speaker 1: galaxies and air gravity. We infer that this stuff is around, 88 00:04:49,520 --> 00:04:52,680 Speaker 1: so as that there's about six six times as much 89 00:04:52,800 --> 00:04:57,279 Speaker 1: dark matter as there is ordinary don't you figure what 90 00:04:57,279 --> 00:04:59,520 Speaker 1: it is? There's an Obel prize waiting for you in 91 00:04:59,560 --> 00:05:02,080 Speaker 1: stock Fo. You got that right. Could Could there be 92 00:05:02,200 --> 00:05:05,800 Speaker 1: life out there on the dark matter? That is a 93 00:05:05,880 --> 00:05:10,400 Speaker 1: fantastic question because I I one of the one of 94 00:05:09,480 --> 00:05:13,240 Speaker 1: the default position of physicists is they think the dark 95 00:05:13,279 --> 00:05:18,279 Speaker 1: matter might be made of some subatomic pascal we haven't found, okay, 96 00:05:18,279 --> 00:05:20,840 Speaker 1: so they think it's an amorphous, you know, it's just 97 00:05:21,400 --> 00:05:24,480 Speaker 1: all all made of just one thing. But the one 98 00:05:24,600 --> 00:05:26,680 Speaker 1: the thing that we know about augury matter is it's 99 00:05:26,720 --> 00:05:29,720 Speaker 1: not made of one thing. It's made of ninety two 100 00:05:29,880 --> 00:05:32,640 Speaker 1: different elements, all the way from hydrogen to you know, 101 00:05:32,800 --> 00:05:37,360 Speaker 1: uranium naturally occurring and it and it the pieces come 102 00:05:37,400 --> 00:05:41,120 Speaker 1: together to make molecules, to make life, to make planets. 103 00:05:41,160 --> 00:05:43,000 Speaker 1: So what we One thing we know of that augury 104 00:05:43,080 --> 00:05:49,159 Speaker 1: matter is it clumps into complex organization. So who knows. 105 00:05:49,240 --> 00:05:51,760 Speaker 1: The dark matter could similarly be made of lots of 106 00:05:51,760 --> 00:05:55,200 Speaker 1: different particles which clump together, as you just said, to 107 00:05:55,320 --> 00:06:00,400 Speaker 1: make maybe dark stars, dark planets, dark life. You know, 108 00:06:00,720 --> 00:06:04,760 Speaker 1: could that be the answer to why we have after 109 00:06:04,760 --> 00:06:09,120 Speaker 1: searching since well for fifty years, searching for signals from extraterrestrials, 110 00:06:09,160 --> 00:06:11,240 Speaker 1: we've never found them. Could it be that all the 111 00:06:11,279 --> 00:06:15,200 Speaker 1: activity is in the dark matter? You know, there's all 112 00:06:15,240 --> 00:06:17,240 Speaker 1: this activity going on all around us and we can't 113 00:06:17,279 --> 00:06:21,520 Speaker 1: see it. Who knows? I mean, but in theory, could 114 00:06:21,600 --> 00:06:26,320 Speaker 1: planets collide? Could a planet that we see collide with 115 00:06:26,400 --> 00:06:30,839 Speaker 1: a planet that is in the dark matter stage? It 116 00:06:30,960 --> 00:06:35,560 Speaker 1: certainly could. But the yeah, that's a good question. That's 117 00:06:35,560 --> 00:06:41,120 Speaker 1: a good question if one of the problems with at 118 00:06:41,120 --> 00:06:44,640 Speaker 1: the moment, one of the problems is that why did 119 00:06:44,720 --> 00:06:47,720 Speaker 1: why do planets form? You know, why does spider stars form? 120 00:06:47,760 --> 00:06:52,160 Speaker 1: You know? Why does material shrink perform from gas clouds 121 00:06:52,279 --> 00:06:56,480 Speaker 1: per form stars and planets? Right? Okay, throughout the entire universe. 122 00:06:56,560 --> 00:06:59,680 Speaker 1: I mean, it's uniform. I'm just going to make a comparative. 123 00:07:00,080 --> 00:07:03,359 Speaker 1: Your wide, dart matter may not trump. The reason it 124 00:07:03,400 --> 00:07:05,240 Speaker 1: can do that is because, well, first of all, if 125 00:07:05,279 --> 00:07:08,119 Speaker 1: you have a big cloud of gas in space, it's warm, 126 00:07:08,720 --> 00:07:13,280 Speaker 1: and the warmth of the gas pushes outwards against gravity, right, 127 00:07:13,360 --> 00:07:15,880 Speaker 1: so that the thing can't collapse because gravity is trying 128 00:07:15,880 --> 00:07:19,760 Speaker 1: to squeeze it, but the hot gas inside is pushing outwards. Okay, 129 00:07:19,760 --> 00:07:22,200 Speaker 1: So the only way it's going to collapse is if 130 00:07:22,280 --> 00:07:26,400 Speaker 1: it loses that internal heat. Now, normal matter, what actually 131 00:07:26,480 --> 00:07:30,120 Speaker 1: happens is it radiates. It radiates what we call microwaves, 132 00:07:31,040 --> 00:07:33,160 Speaker 1: which is a kind of light that we can't see. 133 00:07:33,160 --> 00:07:37,080 Speaker 1: And that's right, or heat escapes from the crowd. So 134 00:07:37,240 --> 00:07:42,680 Speaker 1: because normal normal matter radiate, the interior of gas clouds 135 00:07:42,760 --> 00:07:45,040 Speaker 1: is robbed of heat. So gravity and there can then 136 00:07:45,080 --> 00:07:49,320 Speaker 1: crush it. Now, dart matter does not interact with light. 137 00:07:49,480 --> 00:07:52,280 Speaker 1: It does not produce what we call electromega radiation, so 138 00:07:52,360 --> 00:07:56,080 Speaker 1: it has no way of removing its internal heat. So 139 00:07:56,120 --> 00:07:59,680 Speaker 1: as far as you can tell, it can't shrink or 140 00:08:00,400 --> 00:08:04,560 Speaker 1: in the same way as ordinary matter. So when we 141 00:08:04,640 --> 00:08:07,520 Speaker 1: when we infer its existence. So for instance, if you 142 00:08:07,520 --> 00:08:10,520 Speaker 1: think about Milky Way, I don't feel that everyone's got 143 00:08:10,520 --> 00:08:11,960 Speaker 1: a picture of our galaxy, but it's kind of like 144 00:08:12,040 --> 00:08:15,000 Speaker 1: a like a whirlpool of stars, you know, a flat 145 00:08:15,000 --> 00:08:18,920 Speaker 1: whirlpool of stars. We believe that the dark matter is 146 00:08:18,920 --> 00:08:24,880 Speaker 1: actually a spherical cloud in which the Milky Way is embedded. 147 00:08:25,320 --> 00:08:29,640 Speaker 1: Because although the orbity matter could claps, could shrink down 148 00:08:29,680 --> 00:08:34,480 Speaker 1: to form this flat spiral, the dark matter couldn't because 149 00:08:35,080 --> 00:08:37,079 Speaker 1: it couldn't get rid of its heat. And if you 150 00:08:37,160 --> 00:08:39,280 Speaker 1: can't get it can't get rid of its heat, gravity 151 00:08:39,320 --> 00:08:42,040 Speaker 1: can't crash it. Now, so that that kind of contradicts 152 00:08:42,040 --> 00:08:46,719 Speaker 1: the thing that I just told you about about how 153 00:08:46,760 --> 00:08:49,680 Speaker 1: we could have dark stars and planet. But of course 154 00:08:49,720 --> 00:08:52,520 Speaker 1: it's quite possible that there was another type of light, 155 00:08:52,720 --> 00:08:55,400 Speaker 1: dark light, you know, there was another interaction other than 156 00:08:55,440 --> 00:08:58,440 Speaker 1: the electric magnetic interaction, maybe dark light, and that dark 157 00:08:58,440 --> 00:09:01,040 Speaker 1: matter could collapse because of that reason. That would that reason. 158 00:09:01,480 --> 00:09:05,120 Speaker 1: But but but we think that that, yeah, So that's 159 00:09:05,160 --> 00:09:10,559 Speaker 1: why would would would so if it were possible to 160 00:09:11,080 --> 00:09:14,320 Speaker 1: have a dark matter planet and it did collide with 161 00:09:14,360 --> 00:09:19,439 Speaker 1: the Earth, I think we would feel it. You would think, so, question, 162 00:09:20,040 --> 00:09:22,120 Speaker 1: you would think, So, let's talk about the Big Bang 163 00:09:22,160 --> 00:09:26,440 Speaker 1: for a moment. Marcus, My gosh, how could something create 164 00:09:26,480 --> 00:09:30,600 Speaker 1: itself from nothing? I still don't understand that nobody knows 165 00:09:32,000 --> 00:09:35,920 Speaker 1: will will we ever get the answer? Hard to hard 166 00:09:36,000 --> 00:09:39,880 Speaker 1: to tell, um. I mean, what's what we can do 167 00:09:40,120 --> 00:09:43,040 Speaker 1: is which is incredible. I mean, you know, remember that 168 00:09:43,080 --> 00:09:46,880 Speaker 1: we are an ape that arose on an African plane 169 00:09:46,960 --> 00:09:50,120 Speaker 1: three million years ago with a brain, a three pound brain, 170 00:09:50,280 --> 00:09:53,120 Speaker 1: you know, made mostly of jelly and water. And yet 171 00:09:53,160 --> 00:09:56,200 Speaker 1: with our telescopes we've seen to the edge of the 172 00:09:56,200 --> 00:10:01,000 Speaker 1: observable universe. We can u we can see what the 173 00:10:01,080 --> 00:10:04,839 Speaker 1: universe has made of about two trillion galaxies. There's two 174 00:10:04,920 --> 00:10:08,959 Speaker 1: million million galaxies like our own. And we have an idea. 175 00:10:08,920 --> 00:10:11,760 Speaker 1: We also have an idea that because all the galaxies 176 00:10:11,760 --> 00:10:13,480 Speaker 1: are flying apart from each other, they must have been 177 00:10:13,480 --> 00:10:16,120 Speaker 1: closer in the past. And if we run that kind 178 00:10:16,160 --> 00:10:18,959 Speaker 1: of movie of the universe's expansion backwards and like a 179 00:10:19,040 --> 00:10:22,200 Speaker 1: movie in reverse, we come to this time thirteen point 180 00:10:22,280 --> 00:10:24,959 Speaker 1: eighteen billion years ago when everything was compressed into a 181 00:10:25,000 --> 00:10:28,160 Speaker 1: smaller region, the big Banks. So we know that's correct, 182 00:10:28,520 --> 00:10:33,560 Speaker 1: we know it's correct. But as for you know, you 183 00:10:33,679 --> 00:10:37,520 Speaker 1: always come back to this fundamental question, how did something 184 00:10:38,240 --> 00:10:43,440 Speaker 1: come from nothing? I know it, and you've got crazy thinking. Yeah, 185 00:10:43,520 --> 00:10:46,040 Speaker 1: the answer is that we don't really know that but 186 00:10:46,080 --> 00:10:48,640 Speaker 1: I would tell you that in the in the modern picture, 187 00:10:49,360 --> 00:10:53,840 Speaker 1: which is we bolted onto other ideas, onto the big bank. Okay, 188 00:10:53,840 --> 00:10:56,640 Speaker 1: so the big Bang model now has a few other 189 00:10:56,679 --> 00:10:59,240 Speaker 1: things bolted on. It had dark matter bolted on, it 190 00:10:59,360 --> 00:11:02,000 Speaker 1: had darker that you bolted on, and another thing it 191 00:11:02,040 --> 00:11:05,559 Speaker 1: has bolted on is what we call inflation. And in 192 00:11:05,600 --> 00:11:09,080 Speaker 1: this picture, the Big Bang is not a one off, 193 00:11:09,559 --> 00:11:12,400 Speaker 1: so it's not the only big bang. So these these 194 00:11:12,400 --> 00:11:16,520 Speaker 1: big bangs are going off all across this huge universe 195 00:11:16,640 --> 00:11:21,720 Speaker 1: rather like firecrackers, you know, randomly, So we are just one, 196 00:11:21,880 --> 00:11:24,079 Speaker 1: you know, we are just in the vicinity of one 197 00:11:24,120 --> 00:11:27,240 Speaker 1: of these these big bangs. Religious people Marcus will say 198 00:11:27,320 --> 00:11:30,000 Speaker 1: God did it and leave it at that. Well, the 199 00:11:30,040 --> 00:11:32,800 Speaker 1: problem with that, the problem is adding inflation is you 200 00:11:32,880 --> 00:11:36,880 Speaker 1: just push back the problem because you say, well, yes, 201 00:11:36,880 --> 00:11:39,319 Speaker 1: there was something before the Big Bang, because there was 202 00:11:39,360 --> 00:11:42,240 Speaker 1: what we call this inflationary vacuum, and when it decayed, 203 00:11:42,360 --> 00:11:46,880 Speaker 1: randomly is expanding, and it decayed, those decays were big 204 00:11:46,880 --> 00:11:51,040 Speaker 1: Bang universes. But it turns out that inflation itself had 205 00:11:51,080 --> 00:11:53,559 Speaker 1: to have a beginning. So although you've said, well, okay, 206 00:11:53,559 --> 00:11:55,920 Speaker 1: there was something before the Big Bang, you know, there 207 00:11:55,960 --> 00:11:58,320 Speaker 1: was what we call inflation, and there are other big banks. 208 00:11:58,559 --> 00:12:01,120 Speaker 1: You still get to the point that inflation had to 209 00:12:01,160 --> 00:12:03,640 Speaker 1: begin as well. Well, I don't know, I mean the 210 00:12:03,640 --> 00:12:07,360 Speaker 1: problem is it. I mean again, that isn't really I mean, 211 00:12:07,400 --> 00:12:09,120 Speaker 1: you can believe that God creates it if you like, 212 00:12:09,760 --> 00:12:14,160 Speaker 1: but obviously that's not the preserve of science because of 213 00:12:14,440 --> 00:12:18,200 Speaker 1: one of the characteristics of science is that you put 214 00:12:18,320 --> 00:12:21,360 Speaker 1: very little in and you get a lot out. So, 215 00:12:21,440 --> 00:12:23,240 Speaker 1: for instance, you have a law of gravity, which you 216 00:12:23,240 --> 00:12:25,320 Speaker 1: can write in the back of the stamp, and that 217 00:12:25,440 --> 00:12:29,600 Speaker 1: explains tons of stuff, explains how how planets are formed 218 00:12:29,640 --> 00:12:33,959 Speaker 1: and stars. It how the orbit stars, how stars orbit 219 00:12:34,000 --> 00:12:36,360 Speaker 1: in downaces. Tons of stuff comes out from a tiny, 220 00:12:36,520 --> 00:12:40,160 Speaker 1: tiny little thing, so you get a lot out. You 221 00:12:40,200 --> 00:12:43,000 Speaker 1: put very little in. With the God explanation, you have 222 00:12:43,040 --> 00:12:45,440 Speaker 1: to put a lot in to get a lot out. 223 00:12:45,480 --> 00:12:48,680 Speaker 1: In fact, God has to be more complicated than your universe. 224 00:12:48,679 --> 00:12:51,440 Speaker 1: So it's kind of the obverse of science. So you 225 00:12:51,440 --> 00:12:54,240 Speaker 1: can believe that, but I mean, it isn't really the 226 00:12:53,720 --> 00:12:58,240 Speaker 1: preserve of science, you know, because science doesn't work that way. 227 00:12:58,400 --> 00:13:02,080 Speaker 1: When we get a scientific explanation, and I hope we 228 00:13:02,080 --> 00:13:05,800 Speaker 1: will get a science at exclamation because because basically I mean, 229 00:13:06,280 --> 00:13:09,280 Speaker 1: let's go back to Newton. Newton was an incredibly religious man, 230 00:13:09,920 --> 00:13:13,199 Speaker 1: and the reason he did science was he because because 231 00:13:13,200 --> 00:13:15,960 Speaker 1: he believed he was getting an insight into the mind 232 00:13:16,000 --> 00:13:18,880 Speaker 1: of God. That's what drove him, because he wanted to 233 00:13:18,920 --> 00:13:24,079 Speaker 1: know how God had put the universe together, so he 234 00:13:24,440 --> 00:13:27,920 Speaker 1: didn't see any conflict whatsoever. You know, he thought, I'll 235 00:13:27,920 --> 00:13:29,439 Speaker 1: figure out how, you know, I want to figure out 236 00:13:29,480 --> 00:13:32,559 Speaker 1: how God did this, so you know, that's one way 237 00:13:32,559 --> 00:13:35,040 Speaker 1: of thinking about it. Listen to more Coast to Coast 238 00:13:35,080 --> 00:13:38,760 Speaker 1: AM every weeknight at one am Eastern and go to 239 00:13:38,840 --> 00:13:40,880 Speaker 1: Coast to Coast am dot com for more