1 00:00:00,240 --> 00:00:04,640 Speaker 1: Now here's a highlight from Coast to Coast AM on iHeartRadio. 2 00:00:05,040 --> 00:00:07,640 Speaker 2: Man, Welcome back to Coast to Coast, George Nori with you. 3 00:00:07,760 --> 00:00:11,039 Speaker 2: Marcus choundback with us. An award winning writer and broadcaster. 4 00:00:11,240 --> 00:00:15,760 Speaker 2: He's based in London, England, formerly a radio astronomer at 5 00:00:15,800 --> 00:00:20,040 Speaker 2: the California Institute of Technology in Pasadena. He's the author 6 00:00:20,079 --> 00:00:23,200 Speaker 2: of a number of popular science books, including The Magicians, 7 00:00:23,239 --> 00:00:26,799 Speaker 2: The Ascent of Gravity, Quantum Theory, Cannot Hurt You, We 8 00:00:26,920 --> 00:00:30,480 Speaker 2: need to talk to Kelvin, and Solar System for iPad now. 9 00:00:30,520 --> 00:00:33,280 Speaker 2: His latest book we're talking about tonight is called The 10 00:00:33,360 --> 00:00:35,920 Speaker 2: One Thing You Need to Know. Marcus, Welcome back to 11 00:00:35,960 --> 00:00:36,479 Speaker 2: the program. 12 00:00:36,520 --> 00:00:37,080 Speaker 1: How have you been? 13 00:00:38,080 --> 00:00:38,199 Speaker 2: Hi? 14 00:00:38,440 --> 00:00:40,880 Speaker 3: Thanks George, It's great to be on the program. Thanks 15 00:00:40,960 --> 00:00:44,200 Speaker 3: inviting me. I'm well, how are you? I mean? Unhappy 16 00:00:44,240 --> 00:00:45,080 Speaker 3: Independence Day? 17 00:00:45,479 --> 00:00:48,880 Speaker 2: Thank you very much. Thanks. Calming down in France right now? Boy, 18 00:00:48,920 --> 00:00:49,560 Speaker 2: what a mess? 19 00:00:49,640 --> 00:00:53,280 Speaker 3: Huh wow. It's very difficult to know. I don't know 20 00:00:53,280 --> 00:00:56,240 Speaker 3: how much you get on your news in the US. 21 00:00:56,400 --> 00:00:59,400 Speaker 3: It's covered a bit in Britain, but I think things 22 00:00:59,400 --> 00:01:02,920 Speaker 3: are coming. My sister actually lives in Nant, which is 23 00:01:02,960 --> 00:01:05,640 Speaker 3: in France, so I think they had a bit of 24 00:01:05,680 --> 00:01:07,560 Speaker 3: trouble there, but she lives in a main new kind 25 00:01:07,600 --> 00:01:11,039 Speaker 3: of rural country area, so hopefully it is quieting down. 26 00:01:11,200 --> 00:01:14,000 Speaker 2: Yeah, tragic story. Anyways, You've got your new book that 27 00:01:14,160 --> 00:01:15,360 Speaker 2: just came out, right. 28 00:01:16,160 --> 00:01:18,720 Speaker 3: Yeah, it's published in the US today, So that's really 29 00:01:19,040 --> 00:01:19,920 Speaker 3: exciting for me. 30 00:01:21,120 --> 00:01:23,479 Speaker 2: The one thing you need to know tell me about that. 31 00:01:23,360 --> 00:01:28,760 Speaker 3: Title, right, Well, basically it's about the one thing you 32 00:01:28,800 --> 00:01:31,280 Speaker 3: need to know to understand a particular topic. So I've 33 00:01:31,280 --> 00:01:37,400 Speaker 3: picked twenty one topics, things like relativity, the Big Bang, 34 00:01:38,680 --> 00:01:41,600 Speaker 3: plate tectonics, you know, evolution, all this kind of stuff, 35 00:01:41,640 --> 00:01:43,839 Speaker 3: and I've tried to think of what is the one 36 00:01:43,880 --> 00:01:47,840 Speaker 3: thing you need to know from which everything else follows logically. 37 00:01:47,920 --> 00:01:50,840 Speaker 3: So it's kind of a way of trying to make 38 00:01:50,880 --> 00:01:54,280 Speaker 3: a lot of really complicated science and what. 39 00:01:54,480 --> 00:01:56,120 Speaker 2: Is that one thing we need to know. 40 00:01:57,960 --> 00:02:01,240 Speaker 3: Well, for each topic, there's a different thing. So if 41 00:02:01,280 --> 00:02:03,600 Speaker 3: I were to tell you about, for instance, relativity, I'm 42 00:02:03,640 --> 00:02:05,880 Speaker 3: side to relativity. The one thing that you need to 43 00:02:05,960 --> 00:02:09,280 Speaker 3: know is that that light is uncatchable. You know, it's 44 00:02:09,320 --> 00:02:11,800 Speaker 3: impossible to catch up a light beam. This was something 45 00:02:11,840 --> 00:02:14,000 Speaker 3: that was realized by Einstein when he was just sixteen. 46 00:02:14,560 --> 00:02:18,080 Speaker 3: He was imagining what it would be like to travel 47 00:02:18,080 --> 00:02:21,560 Speaker 3: alongside the light, alongside the light beam, and he realized 48 00:02:21,560 --> 00:02:25,040 Speaker 3: that you would see something impossible. So he concluded that 49 00:02:25,120 --> 00:02:27,720 Speaker 3: you could never catch up a light beam. And all 50 00:02:27,800 --> 00:02:30,720 Speaker 3: of the stuff of relativity or that or the madness 51 00:02:30,720 --> 00:02:34,880 Speaker 3: of relative relativity follows from that sentence. You know, if 52 00:02:34,880 --> 00:02:37,640 Speaker 3: you were to someone must move past you traveling near 53 00:02:37,639 --> 00:02:40,720 Speaker 3: the light, you would see their times slow down, and 54 00:02:40,760 --> 00:02:43,240 Speaker 3: you would see them shrink in the direction of motion. 55 00:02:43,440 --> 00:02:45,280 Speaker 3: So they would have looked like they were walking through 56 00:02:45,320 --> 00:02:51,680 Speaker 3: treacle or walking in slow motion, and they would drink 57 00:02:51,720 --> 00:02:53,720 Speaker 3: like a pancake in the direction of motion. And we 58 00:02:53,760 --> 00:02:57,400 Speaker 3: see this all the time when we accelerate particles, for instance, 59 00:02:57,440 --> 00:03:00,480 Speaker 3: in particle accelerators like the large hadron collide. We see 60 00:03:00,480 --> 00:03:03,280 Speaker 3: these effects of relativity. But they all stem from this 61 00:03:03,440 --> 00:03:07,520 Speaker 3: simple idea that you cannot catch up light. So it 62 00:03:07,639 --> 00:03:10,840 Speaker 3: plays the role of the cosmic speed limit. So I 63 00:03:10,919 --> 00:03:12,880 Speaker 3: take things like this and I just you know, I 64 00:03:13,000 --> 00:03:15,800 Speaker 3: take the sentence that you need, and then I kind 65 00:03:15,800 --> 00:03:19,560 Speaker 3: of deduce from that all the consequences. 66 00:03:19,960 --> 00:03:22,560 Speaker 2: You've got twenty one great chapters in this book will 67 00:03:22,600 --> 00:03:25,200 Speaker 2: digest some of them, and maybe by the end of 68 00:03:25,240 --> 00:03:28,760 Speaker 2: this interview over the next couple hours, Marcus, you'll help 69 00:03:28,800 --> 00:03:32,000 Speaker 2: us learn about the Big Bang, which I still don't understand. 70 00:03:33,320 --> 00:03:36,640 Speaker 3: Yeah, well nobody does really, Let's face, that's good to 71 00:03:36,720 --> 00:03:40,640 Speaker 3: hear that. Well, we don't know. We know a lot, 72 00:03:41,080 --> 00:03:43,920 Speaker 3: you know. So we can see that the universe is expanding, 73 00:03:44,280 --> 00:03:47,080 Speaker 3: and we can kind of imagine it the expansion running 74 00:03:47,120 --> 00:03:49,320 Speaker 3: backwards like a movie in reverse. And you know, we 75 00:03:49,400 --> 00:03:52,360 Speaker 3: come to this point about fourteen billion years ago when 76 00:03:52,400 --> 00:03:56,360 Speaker 3: everything was concentrated into a single location, which we call 77 00:03:56,440 --> 00:03:59,320 Speaker 3: a Big Bang, and we see all around us the 78 00:03:59,360 --> 00:04:03,080 Speaker 3: heat of to glow with the Big Bang. So incredibly, 79 00:04:04,080 --> 00:04:06,960 Speaker 3: the whole universe is growing with the afterglow of the 80 00:04:07,000 --> 00:04:11,200 Speaker 3: Big Bang fireball. About ninety nine point nine percent of 81 00:04:11,240 --> 00:04:13,920 Speaker 3: all the light in the universe is the afterglow of 82 00:04:13,960 --> 00:04:17,120 Speaker 3: the Big Bang, and only point one percent, that's one 83 00:04:17,120 --> 00:04:19,880 Speaker 3: thousandth of the light in the universe is coming from 84 00:04:19,920 --> 00:04:22,400 Speaker 3: stars and galaxies. But of course it's not light that 85 00:04:22,440 --> 00:04:25,279 Speaker 3: we can see with our with the naked eye, which 86 00:04:25,279 --> 00:04:27,760 Speaker 3: is why we didn't spot it until two guys at 87 00:04:27,760 --> 00:04:32,400 Speaker 3: Bell Lads in nineteen sixty five. So the evidence that 88 00:04:33,080 --> 00:04:35,120 Speaker 3: the universe began in a hot, dense phase and a 89 00:04:35,160 --> 00:04:38,080 Speaker 3: big bang of exploded outwards and the galaxy is like 90 00:04:38,160 --> 00:04:41,640 Speaker 3: a milky way of kind of coalesced from congealed from 91 00:04:41,720 --> 00:04:45,240 Speaker 3: the cooling debris. That's kind of beyond doubt. But of 92 00:04:45,240 --> 00:04:48,919 Speaker 3: course the questions you're you're wondering about are what was 93 00:04:48,960 --> 00:04:51,479 Speaker 3: the Big Bang? You know, what drove the Big Bang? 94 00:04:52,000 --> 00:04:54,359 Speaker 3: What happened before the Big Bang? You don't know the 95 00:04:54,400 --> 00:04:55,640 Speaker 3: answers to those questions? 96 00:04:55,680 --> 00:04:58,000 Speaker 2: Will we ever right? Will we ever get the answers? 97 00:04:58,040 --> 00:05:01,480 Speaker 3: Marcus got I really hope, I really hope. So, I mean, 98 00:05:01,680 --> 00:05:04,240 Speaker 3: I think we're in an amazing position at the moment. 99 00:05:05,200 --> 00:05:08,400 Speaker 3: I think previous generations would would have killed to have 100 00:05:08,480 --> 00:05:10,280 Speaker 3: the kind of information we've got, you know, I mean 101 00:05:10,360 --> 00:05:12,920 Speaker 3: James Webb Space Telescope, And that's as James Webb's Space 102 00:05:12,960 --> 00:05:17,159 Speaker 3: Telescope was launched Christmas twenty twenty one, and it's looking 103 00:05:17,240 --> 00:05:19,720 Speaker 3: back to very very close to the Big Bang, and 104 00:05:20,000 --> 00:05:23,520 Speaker 3: it's already surprising us with its discoveries. You know, so 105 00:05:23,560 --> 00:05:27,479 Speaker 3: we we we can look at how the galaxies began 106 00:05:27,640 --> 00:05:31,159 Speaker 3: to can jeel out of the cooling stuff of the 107 00:05:31,200 --> 00:05:34,159 Speaker 3: debris of the Big Bang, and we can kind of 108 00:05:34,240 --> 00:05:36,840 Speaker 3: learn more and more about this this Big Bang picture 109 00:05:37,360 --> 00:05:41,279 Speaker 3: so yeah, I think I think we I mean, the 110 00:05:41,320 --> 00:05:43,840 Speaker 3: incredible thing is that we have a good chance of 111 00:05:43,880 --> 00:05:47,640 Speaker 3: asking answering these ultimate questions, you know, like what happened 112 00:05:47,680 --> 00:05:50,000 Speaker 3: before the Big Bang? What is space? What is time? 113 00:05:50,040 --> 00:05:52,240 Speaker 3: All these really really big questions. We have a good 114 00:05:52,320 --> 00:05:56,000 Speaker 3: chance of answering them, maybe in the next couple of decades, 115 00:05:56,120 --> 00:05:58,359 Speaker 3: you know. So that's an amazing position to be in 116 00:05:58,400 --> 00:06:01,400 Speaker 3: the history of science because it's there's so many these 117 00:06:01,400 --> 00:06:04,880 Speaker 3: incredible space experiments that are up there. You know. James 118 00:06:04,880 --> 00:06:09,080 Speaker 3: Webb Euclid was launched, i think this week, and it's 119 00:06:09,720 --> 00:06:12,640 Speaker 3: trying to probe dark matter and dark energy. These are 120 00:06:13,000 --> 00:06:17,760 Speaker 3: the two biggest mysteries in the whole of astronomy are 121 00:06:17,640 --> 00:06:20,719 Speaker 3: the universe is filled with this dark matter stuff that 122 00:06:20,760 --> 00:06:23,840 Speaker 3: doesn't give out any light, and dark energy, which doesn't 123 00:06:23,880 --> 00:06:26,279 Speaker 3: give out any light and is speeding up the expansion 124 00:06:26,320 --> 00:06:28,920 Speaker 3: of the universe. So that there's another chance that we'll 125 00:06:29,000 --> 00:06:30,760 Speaker 3: well had, maybe in the next few years, to figure 126 00:06:30,760 --> 00:06:32,920 Speaker 3: out what they are. So yeah, I think there is hope. 127 00:06:32,960 --> 00:06:33,720 Speaker 3: There's hope. 128 00:06:34,560 --> 00:06:37,080 Speaker 2: Who are you structuring and going after with the book? 129 00:06:37,120 --> 00:06:38,600 Speaker 2: The one thing you need to know, who do you 130 00:06:38,640 --> 00:06:39,240 Speaker 2: want to read? 131 00:06:40,120 --> 00:06:42,320 Speaker 3: Who do I want to read it. I kind of 132 00:06:42,400 --> 00:06:46,120 Speaker 3: aim it all on my wife's she's a nurse in Britain, 133 00:06:46,200 --> 00:06:49,440 Speaker 3: you know, and she doesn't have any science background, so 134 00:06:49,640 --> 00:06:51,800 Speaker 3: I kind of I kind of aim it at her. Really, 135 00:06:51,880 --> 00:06:54,360 Speaker 3: you know, I was very lucky, as you pointed out, 136 00:06:54,440 --> 00:06:56,840 Speaker 3: to go to caw Tech, and I was taught by 137 00:06:56,839 --> 00:07:00,359 Speaker 3: a lot of really interesting people, I reach of women. 138 00:07:01,400 --> 00:07:05,599 Speaker 3: But I want to communicate the kind of things I 139 00:07:05,680 --> 00:07:08,719 Speaker 3: learned to everyone, you know, because I think when people 140 00:07:09,080 --> 00:07:13,760 Speaker 3: understand how amazing science is, they realize, you know, that 141 00:07:14,280 --> 00:07:18,240 Speaker 3: it's a fascinating topic. And maybe at school, you know, 142 00:07:18,480 --> 00:07:22,160 Speaker 3: they learned the whole and boring science, but actually it's 143 00:07:22,240 --> 00:07:24,880 Speaker 3: really you know, when you tell them about what we know, 144 00:07:25,720 --> 00:07:28,640 Speaker 3: it really fires their imagination. So my aim is really 145 00:07:28,720 --> 00:07:34,120 Speaker 3: to communicate some of this stuff that I learned to everybody, really, anybody, 146 00:07:34,200 --> 00:07:36,200 Speaker 3: even if you have no science background whatsoever. 147 00:07:37,640 --> 00:07:42,640 Speaker 2: Back in the eighteen fifty four, there was a scientists 148 00:07:42,680 --> 00:07:44,920 Speaker 2: that not a lot of people knew about. Unie's Foot. 149 00:07:45,360 --> 00:07:46,360 Speaker 2: Tell us about her. 150 00:07:46,920 --> 00:07:51,000 Speaker 3: That's right. So she was an American scientist called Unice Foot, 151 00:07:51,120 --> 00:07:55,600 Speaker 3: and she's pretty much nobody knows her name, but she 152 00:07:55,760 --> 00:07:58,960 Speaker 3: did an incredibly important experiment and it's such an simple 153 00:07:59,040 --> 00:08:01,840 Speaker 3: experiment that any one could do it in high school, 154 00:08:01,880 --> 00:08:05,720 Speaker 3: you know. So what she actually did was she got 155 00:08:07,240 --> 00:08:10,679 Speaker 3: some glass tubes and she filled them with different gases. 156 00:08:10,680 --> 00:08:13,239 Speaker 3: She filled one with oxygen, she filled one with water vapor, 157 00:08:13,600 --> 00:08:17,160 Speaker 3: another one with carbon dioxide, nitrogen, all these kind of things. 158 00:08:17,520 --> 00:08:22,160 Speaker 3: And she's start thermometers in these sealed glass tubes and 159 00:08:22,200 --> 00:08:25,160 Speaker 3: she put them in the sun, and to her amazement, 160 00:08:26,040 --> 00:08:29,080 Speaker 3: the tube that contained carbon dioxide and the tubes that 161 00:08:29,120 --> 00:08:33,719 Speaker 3: contained water vapor in there, the temperature rose dramatically. So 162 00:08:33,800 --> 00:08:36,520 Speaker 3: she realized she was the first person to realize that 163 00:08:36,640 --> 00:08:39,720 Speaker 3: these gases, I mean, carbon dioxide is a made there's 164 00:08:39,720 --> 00:08:41,560 Speaker 3: hardly any of it in the in the atmosphere. I 165 00:08:41,559 --> 00:08:43,600 Speaker 3: mean it's I don't know, it's a fraction, a very 166 00:08:43,640 --> 00:08:47,320 Speaker 3: small fraction of one percent of the atmosphere of cambraxer. 167 00:08:47,440 --> 00:08:51,360 Speaker 3: So this gas that appears to have no be to 168 00:08:51,400 --> 00:08:56,080 Speaker 3: be really unusual and really there's not much of it, 169 00:08:56,480 --> 00:08:59,600 Speaker 3: was having this tremendous effect. So she made the she 170 00:08:59,720 --> 00:09:02,720 Speaker 3: spentated in eighteen fifty four that changes in the amount 171 00:09:02,720 --> 00:09:06,760 Speaker 3: of carbon dioxide might be connected with changes in the climate. 172 00:09:06,880 --> 00:09:10,880 Speaker 3: So she was the first person in history to recognize 173 00:09:10,880 --> 00:09:13,640 Speaker 3: what we now call the greenouse effect. And now an 174 00:09:13,679 --> 00:09:17,320 Speaker 3: Irish physinessist three years later called John Tyndall made the 175 00:09:17,360 --> 00:09:20,840 Speaker 3: same discovery. And in all the history books we remember 176 00:09:21,559 --> 00:09:24,400 Speaker 3: John Tyndall, and Unice Foot has kind of been written 177 00:09:24,440 --> 00:09:26,679 Speaker 3: out of history. So we need to remember Unie Foot, 178 00:09:26,720 --> 00:09:31,560 Speaker 3: the American scientist who basically discovered the greenouse effect. 179 00:09:31,720 --> 00:09:34,400 Speaker 2: Yeah, Unis is not mentioned in many high school books 180 00:09:34,400 --> 00:09:35,040 Speaker 2: on science. 181 00:09:36,040 --> 00:09:38,920 Speaker 3: No that she should be. But this is really common 182 00:09:39,160 --> 00:09:43,440 Speaker 3: that you get these women who make these enormous contributions 183 00:09:43,960 --> 00:09:46,720 Speaker 3: and are completely forgotten. I mean, my favorite is the 184 00:09:46,800 --> 00:09:51,600 Speaker 3: Celia Paine and she was English, but she went from 185 00:09:51,720 --> 00:09:55,640 Speaker 3: Cambridge to Harvard in the nineteen twenties and they didn't 186 00:09:55,760 --> 00:09:58,000 Speaker 3: I mean, I think she was paid on equipment expenses 187 00:09:58,040 --> 00:10:02,240 Speaker 3: something like that. And she actually discovered that the Sun 188 00:10:02,640 --> 00:10:06,560 Speaker 3: was made of ninety eight percent hydrogen and the helium. Now, 189 00:10:06,600 --> 00:10:10,160 Speaker 3: these are two gases which are almost nonexistent on the 190 00:10:10,200 --> 00:10:13,360 Speaker 3: Earth basically because they're very light, so they float off 191 00:10:13,400 --> 00:10:17,320 Speaker 3: into space. So Ever, since Greek times, people have thought 192 00:10:17,360 --> 00:10:19,840 Speaker 3: that sun was made of iron, you know, because it 193 00:10:19,840 --> 00:10:22,640 Speaker 3: looks like it looks like a ball of glowing iron. 194 00:10:22,720 --> 00:10:26,400 Speaker 3: It glows orange, glows in a golden color, and so 195 00:10:26,520 --> 00:10:29,319 Speaker 3: until then people have thought it that had. Her supervisor 196 00:10:29,440 --> 00:10:31,560 Speaker 3: was called Henry Norris Russell was one of the great 197 00:10:31,600 --> 00:10:36,360 Speaker 3: American astronomers. He told her in her PhD thesis to 198 00:10:36,440 --> 00:10:40,360 Speaker 3: actually write that her result was almost certainly wrong. But 199 00:10:40,480 --> 00:10:43,440 Speaker 3: ten years later, when it was discovered that she was right, 200 00:10:43,720 --> 00:10:45,640 Speaker 3: he mentioned her on about one hundred and page one 201 00:10:45,720 --> 00:10:48,080 Speaker 3: hundred and fifty of a paper that he wrote, and 202 00:10:48,120 --> 00:10:51,000 Speaker 3: he got the credit. But part of the Celia Pain 203 00:10:51,160 --> 00:10:55,960 Speaker 3: basically discovered the major component of the whole universe because 204 00:10:56,080 --> 00:10:59,560 Speaker 3: most of the universe that we see is hydrogen and helium. 205 00:10:59,600 --> 00:11:02,559 Speaker 3: I mean, all the elements that we're made of calcium 206 00:11:02,600 --> 00:11:05,640 Speaker 3: and oxydshire and oh and all the things that are 207 00:11:05,640 --> 00:11:07,920 Speaker 3: in our body are am I in a contaminant at 208 00:11:07,960 --> 00:11:10,880 Speaker 3: the universe. So she was the person who basically discovered 209 00:11:11,120 --> 00:11:12,320 Speaker 3: what the universe was made of. 210 00:11:13,000 --> 00:11:16,240 Speaker 2: Marcus, when I was young in school, very very young, 211 00:11:16,320 --> 00:11:19,000 Speaker 2: our teacher said that the son's going to burn out 212 00:11:19,040 --> 00:11:22,680 Speaker 2: folks in the four and a half billion years, there'll 213 00:11:22,720 --> 00:11:27,280 Speaker 2: be nothing anymore. And I would go home really upset. 214 00:11:27,679 --> 00:11:29,839 Speaker 2: I talked to my dad and my mother, and I 215 00:11:29,880 --> 00:11:33,640 Speaker 2: would say, the son's going to burn out. We're all 216 00:11:33,679 --> 00:11:37,880 Speaker 2: going to be gone. And I didn't comprehend what four 217 00:11:37,920 --> 00:11:40,000 Speaker 2: point five billion years from now was. 218 00:11:41,080 --> 00:11:43,559 Speaker 3: And we've got plenty of time. We can sleep tonight. 219 00:11:43,400 --> 00:11:46,840 Speaker 2: We can, we can. But I don't know why the 220 00:11:46,920 --> 00:11:50,160 Speaker 2: teacher didn't explain that part of it to us, Like 221 00:11:50,280 --> 00:11:53,160 Speaker 2: four point five billion years, folks is a long time. 222 00:11:53,280 --> 00:11:54,920 Speaker 2: We're just kids. 223 00:11:55,559 --> 00:11:57,720 Speaker 3: Well maybe they should have done. I mean, the interesting 224 00:11:57,720 --> 00:12:01,440 Speaker 3: thing is that when people started thinking of this in 225 00:12:01,480 --> 00:12:05,079 Speaker 3: the nineteenth century, they obviously thought the lump of the 226 00:12:06,120 --> 00:12:08,400 Speaker 3: sun is a lump of coal, because in the nineteenth 227 00:12:08,400 --> 00:12:11,640 Speaker 3: century it was an age which was driven by steam, 228 00:12:12,040 --> 00:12:14,120 Speaker 3: so they thought it was a lump of coal. And 229 00:12:14,160 --> 00:12:15,640 Speaker 3: they were able to look at a lump of coal 230 00:12:15,679 --> 00:12:17,400 Speaker 3: in the grate, you know, and they could see how 231 00:12:17,520 --> 00:12:20,400 Speaker 3: long it took before it burnt out, and they could 232 00:12:20,400 --> 00:12:23,840 Speaker 3: extrapolate to something the size of the sun. And the 233 00:12:23,920 --> 00:12:27,240 Speaker 3: calculation showed that, in fact, it was only five thousand 234 00:12:27,360 --> 00:12:31,120 Speaker 3: years that the sun would burn before it burnt out, 235 00:12:32,080 --> 00:12:34,200 Speaker 3: which was not enough for anybody, you know, It wasn't 236 00:12:34,200 --> 00:12:36,679 Speaker 3: really enough even with every guy called Bishop Usher, who 237 00:12:36,720 --> 00:12:39,679 Speaker 3: was an Irish bishop who calculated from the Bible that 238 00:12:39,720 --> 00:12:42,560 Speaker 3: the Earth was created on. I think it was twenty 239 00:12:42,559 --> 00:12:45,360 Speaker 3: third of October four thousand and four BC, So it 240 00:12:45,400 --> 00:12:49,640 Speaker 3: wasn't even enough for him, and certainly not for geologists. 241 00:12:49,640 --> 00:12:51,480 Speaker 3: You know, we know that mountains rise up out of 242 00:12:51,520 --> 00:12:53,960 Speaker 3: the sea, and for the biologists because we know that 243 00:12:55,440 --> 00:13:00,760 Speaker 3: organisms have diverged from a common ancestor, but that process 244 00:13:00,800 --> 00:13:03,600 Speaker 3: takes a long time. But it's this thicker you're talking 245 00:13:03,600 --> 00:13:08,160 Speaker 3: about comes from analysis of meteorites, you know, the builder's 246 00:13:08,280 --> 00:13:11,440 Speaker 3: ravel left over after the formation of Sosis, and we 247 00:13:11,480 --> 00:13:14,360 Speaker 3: can date them, and you're actually right. We find out 248 00:13:14,440 --> 00:13:16,640 Speaker 3: what the Earth is about four point five billion years, 249 00:13:16,640 --> 00:13:18,000 Speaker 3: which seems a long time, doesn't it. 250 00:13:18,000 --> 00:13:18,480 Speaker 1: It doesn't, it. 251 00:13:18,559 --> 00:13:22,640 Speaker 2: Does, Marcus. What does this mean in terms of a 252 00:13:22,679 --> 00:13:26,240 Speaker 2: divine creator? When you think of all the different things, 253 00:13:26,320 --> 00:13:29,880 Speaker 2: just just by reading your book, we talk about gravity, electricity, 254 00:13:30,080 --> 00:13:33,880 Speaker 2: all these incredible things. There seems to be so much 255 00:13:34,200 --> 00:13:37,240 Speaker 2: order in the universe to make all these things happen. 256 00:13:37,720 --> 00:13:40,560 Speaker 2: Where does the divine creator come in on this? Do 257 00:13:40,640 --> 00:13:41,840 Speaker 2: you think about that much? 258 00:13:41,880 --> 00:13:45,959 Speaker 3: A matter of choice? Really? Where you can I mean 259 00:13:45,960 --> 00:13:49,240 Speaker 3: some of the great physessests in history, like Isaac were 260 00:13:49,320 --> 00:13:52,760 Speaker 3: very religious. They believed that in figuring out how the 261 00:13:52,880 --> 00:13:56,920 Speaker 3: universe was working, they were actually laying bare the mind 262 00:13:56,960 --> 00:14:00,839 Speaker 3: of God. So actually incredibly Newton is one probably the 263 00:14:00,920 --> 00:14:05,640 Speaker 3: greatest scientist in history, but most of his work was 264 00:14:05,679 --> 00:14:10,840 Speaker 3: analysis of the Bible, alchemy, and hardly any of his 265 00:14:10,960 --> 00:14:13,480 Speaker 3: work was actually science. But he thought these were all 266 00:14:14,120 --> 00:14:18,960 Speaker 3: ways of appreciating God. So he would he, you know, 267 00:14:19,360 --> 00:14:22,640 Speaker 3: the lord of gravity. He imagined that God had imposed 268 00:14:22,640 --> 00:14:25,080 Speaker 3: the law of gravity. So you see this throughout history. 269 00:14:25,360 --> 00:14:27,760 Speaker 3: So you have scientists who don't believe and scientists who do. 270 00:14:27,840 --> 00:14:29,880 Speaker 3: But it doesn't really make much difference, you know, because 271 00:14:30,680 --> 00:14:34,840 Speaker 3: either you believe the universe is this fantastically incredible beautiful 272 00:14:36,400 --> 00:14:40,520 Speaker 3: thing or you think it's a fantastically incredibly beautiful thing 273 00:14:40,560 --> 00:14:42,600 Speaker 3: that God made, it doesn't really make a lot of 274 00:14:42,600 --> 00:14:45,840 Speaker 3: difference really. So but what we actually see is that 275 00:14:45,920 --> 00:14:51,040 Speaker 3: laws of physics that we've actually discovered do actually produce 276 00:14:51,080 --> 00:14:53,440 Speaker 3: the universe that we that we see around us. So, 277 00:14:53,520 --> 00:14:56,440 Speaker 3: for instance, we kind of know what's what the universe 278 00:14:56,560 --> 00:14:59,120 Speaker 3: was like very early on in a big band, because 279 00:14:59,120 --> 00:15:00,840 Speaker 3: we can see the art to go with the big Bank, 280 00:15:00,920 --> 00:15:02,680 Speaker 3: so we could we know what the universe was like 281 00:15:04,160 --> 00:15:06,720 Speaker 3: within within a few hundred thousand years of the Big Bank. 282 00:15:07,280 --> 00:15:10,600 Speaker 3: We can run in our computers forward the history of 283 00:15:10,600 --> 00:15:12,640 Speaker 3: the universe using the laws of gravity, you know, the 284 00:15:12,720 --> 00:15:15,000 Speaker 3: law of gravity in the laws that we see, and 285 00:15:15,040 --> 00:15:17,160 Speaker 3: it gives us the universe which is very similar to 286 00:15:17,160 --> 00:15:19,520 Speaker 3: the one that puts around us, you know, with galaxies, 287 00:15:19,560 --> 00:15:22,800 Speaker 3: the size of the Milky Way, and all the properties 288 00:15:22,840 --> 00:15:26,080 Speaker 3: of the universe. So it doesn't appear to be any 289 00:15:26,120 --> 00:15:30,400 Speaker 3: divine hand is actually needed. So that's why I say 290 00:15:30,440 --> 00:15:33,760 Speaker 3: it's a matter of choice, really, And some some physicists 291 00:15:33,800 --> 00:15:37,360 Speaker 3: are or scientists are religious, and others are not. I mean, 292 00:15:37,400 --> 00:15:40,040 Speaker 3: Eiseen used to make loads of statements that use the 293 00:15:40,040 --> 00:15:43,160 Speaker 3: word God. He wasn't religious himself, but he used to 294 00:15:43,200 --> 00:15:45,080 Speaker 3: say things like God does not play dice with the 295 00:15:45,200 --> 00:15:49,400 Speaker 3: universe and all that kind of stuff. But that's that's 296 00:15:49,400 --> 00:15:53,000 Speaker 3: so that's really as I say, that's that's you can 297 00:15:53,120 --> 00:15:57,240 Speaker 3: or you can't. It depends on your your own belief really. 298 00:15:57,320 --> 00:16:01,240 Speaker 2: Sure do you think gravity is the glue that keeps 299 00:16:01,280 --> 00:16:02,120 Speaker 2: everything together? 300 00:16:03,960 --> 00:16:04,120 Speaker 1: Well? 301 00:16:04,160 --> 00:16:08,120 Speaker 3: Gravity is that is the glue that keeps large things together. 302 00:16:08,200 --> 00:16:11,400 Speaker 3: Because gravity, and this is one of the absolute mysteries 303 00:16:11,400 --> 00:16:16,680 Speaker 3: of science, is one followed by forty zero strong weaker 304 00:16:17,280 --> 00:16:20,200 Speaker 3: than the forced the electric force. That's holding together the 305 00:16:20,240 --> 00:16:24,480 Speaker 3: atoms in your body. So that's ten thousand, billion, billion, 306 00:16:25,000 --> 00:16:30,640 Speaker 3: billion billion times weaker. Okay, So that's a real mystery 307 00:16:30,720 --> 00:16:35,000 Speaker 3: why the electric force is so much stronger. But it 308 00:16:35,040 --> 00:16:38,080 Speaker 3: turns out that the electric force comes in two types, 309 00:16:38,200 --> 00:16:41,600 Speaker 3: So it says a repulsive type and an attractive type, 310 00:16:41,800 --> 00:16:45,840 Speaker 3: and in your body, those two forces completely cancel out. 311 00:16:46,160 --> 00:16:49,720 Speaker 3: But gravity only comes in one form. It's only attractive. 312 00:16:50,280 --> 00:16:53,840 Speaker 3: So the more material you get, the more gravity you get. 313 00:16:53,880 --> 00:16:57,320 Speaker 3: So when you get to a certain size a certain 314 00:16:57,320 --> 00:17:01,600 Speaker 3: amount of material, gravity begins to dominate. And in our 315 00:17:01,640 --> 00:17:04,920 Speaker 3: solar system, that size is an object about three or 316 00:17:04,960 --> 00:17:08,960 Speaker 3: four hundred kilometers across. Okay, So when you get beyond that, 317 00:17:09,440 --> 00:17:12,920 Speaker 3: gravity is so strong it can gather everything, crash everything 318 00:17:12,960 --> 00:17:18,240 Speaker 3: into a sphere. When you have less material and that 319 00:17:18,359 --> 00:17:21,080 Speaker 3: it can't. So when you look out across the Solar system, 320 00:17:21,280 --> 00:17:23,679 Speaker 3: everything that's less than three or four hundred kilometers across 321 00:17:23,760 --> 00:17:27,239 Speaker 3: is like a potato potato shaped, and everything that's more 322 00:17:27,280 --> 00:17:31,040 Speaker 3: than three or four hundred klometers across is a sphere. 323 00:17:31,520 --> 00:17:34,040 Speaker 3: And that's because that's the scale of which gravity begins 324 00:17:34,040 --> 00:17:37,119 Speaker 3: to dominate. So after that scale, it dominates everything. So 325 00:17:37,200 --> 00:17:40,520 Speaker 3: it dominates planets, It dominates stars, it dominates the galaxy, 326 00:17:40,520 --> 00:17:44,320 Speaker 3: and it dominates the universe. So in a way, it 327 00:17:44,400 --> 00:17:47,919 Speaker 3: controls everything that matters to us. But of course it 328 00:17:47,960 --> 00:17:51,679 Speaker 3: doesn't control the physics in your body, because that's the 329 00:17:51,720 --> 00:17:55,440 Speaker 3: electric force. But so yeah, yeah, it is the dominant 330 00:17:55,480 --> 00:17:59,040 Speaker 3: force because it only comes in one form and it 331 00:17:59,160 --> 00:18:01,760 Speaker 3: only gets strong the more matter. The more matter you have, 332 00:18:02,280 --> 00:18:03,359 Speaker 3: the more gravity you have. 333 00:18:04,000 --> 00:18:07,280 Speaker 1: Listen to more Coast to Coast AM every weeknight at 334 00:18:07,280 --> 00:18:10,159 Speaker 1: one a m. 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