1 00:00:07,360 --> 00:00:11,120 Speaker 1: Hey, Daniel, what's the most distant object you've ever seen? 2 00:00:12,200 --> 00:00:15,080 Speaker 2: You know, the Andromeda galaxy is pretty far away. It's 3 00:00:15,080 --> 00:00:18,320 Speaker 2: like millions of light years. How about you, what's the 4 00:00:18,320 --> 00:00:19,919 Speaker 2: most distant thing you've ever seen? 5 00:00:21,160 --> 00:00:23,920 Speaker 1: When I am sleepy, it is my couch. 6 00:00:24,040 --> 00:00:25,720 Speaker 2: Your couch is far away. 7 00:00:26,200 --> 00:00:27,319 Speaker 1: Yeah, it's so fun. 8 00:00:30,280 --> 00:00:50,280 Speaker 3: W want mom. 9 00:00:50,440 --> 00:00:50,640 Speaker 4: Hi. 10 00:00:50,720 --> 00:00:53,360 Speaker 2: I'm Daniel. I'm a particle physicist and a professor at 11 00:00:53,479 --> 00:00:56,560 Speaker 2: UC Irvine, and I like to couch all my puns. 12 00:00:57,080 --> 00:01:01,800 Speaker 1: Hi. I am Katie Golden. I a podcast on animals, 13 00:01:02,200 --> 00:01:10,400 Speaker 1: and I am cushion for a never mind. I I 14 00:01:10,440 --> 00:01:14,440 Speaker 1: thought if I just said cushion that a pun would 15 00:01:14,520 --> 00:01:17,440 Speaker 1: come to me, and it didn't. It just made me 16 00:01:17,480 --> 00:01:18,280 Speaker 1: want to take a nap. 17 00:01:18,480 --> 00:01:19,800 Speaker 2: You were pushing for a pun, Cushion. 18 00:01:20,120 --> 00:01:22,000 Speaker 1: I thought I was going to be bruising for a 19 00:01:22,040 --> 00:01:25,520 Speaker 1: cruise in, but I was cushion for a pushing. I 20 00:01:25,560 --> 00:01:27,120 Speaker 1: guess a defenestration. 21 00:01:28,280 --> 00:01:31,680 Speaker 2: Sounds like you're set up for some punishment anyway. Welcome 22 00:01:31,760 --> 00:01:34,679 Speaker 2: to the podcast. Daniel and Jorge explain the universe in 23 00:01:34,760 --> 00:01:37,160 Speaker 2: which we try not to punish you. We try to 24 00:01:37,520 --> 00:01:40,680 Speaker 2: enrapture you. We try to share with you the joy 25 00:01:40,720 --> 00:01:43,920 Speaker 2: of understanding the nature of the universe, or when we 26 00:01:44,000 --> 00:01:47,640 Speaker 2: are mystified by the puzzles, the curiosity, the open questions 27 00:01:47,920 --> 00:01:50,640 Speaker 2: about the nature of this cosmos we find ourselves in, 28 00:01:50,960 --> 00:01:53,600 Speaker 2: we seek to understand it, we seek to explain all 29 00:01:53,640 --> 00:01:54,400 Speaker 2: of it to you. 30 00:01:54,600 --> 00:01:56,520 Speaker 3: On the podcast, Daniel. 31 00:01:56,200 --> 00:01:59,120 Speaker 1: Is this the one coming out on the summer solstice? 32 00:02:00,360 --> 00:02:03,440 Speaker 1: Just the quickest side before we get into our listener question. 33 00:02:03,560 --> 00:02:11,000 Speaker 1: I just visited in near Dublin, Bruno Boyne, these funeral mounds, 34 00:02:12,080 --> 00:02:15,880 Speaker 1: and it was so interesting because these very very ancient 35 00:02:15,960 --> 00:02:21,760 Speaker 1: people created these funeral mounds which had an internal structure 36 00:02:21,880 --> 00:02:24,320 Speaker 1: that they're large mounds like you could actually you can 37 00:02:24,360 --> 00:02:27,519 Speaker 1: go inside it. They can do ceremonies inside, and they 38 00:02:27,720 --> 00:02:32,720 Speaker 1: constructed it such that like during the solstice, the summer solstice, 39 00:02:32,840 --> 00:02:35,880 Speaker 1: on the longest day of the year, it illuminates this 40 00:02:36,240 --> 00:02:40,760 Speaker 1: entire inner chamber. And I just love that. So long 41 00:02:40,840 --> 00:02:45,440 Speaker 1: ago we were already thinking about physics, figuring out the universe, 42 00:02:45,520 --> 00:02:48,600 Speaker 1: and like trying to think about how light works and 43 00:02:49,240 --> 00:02:52,279 Speaker 1: use it for our interesting little Richard. 44 00:02:52,160 --> 00:02:54,600 Speaker 2: Yeah, exactly. I don't think that's a digression at all. 45 00:02:54,919 --> 00:02:57,359 Speaker 2: That's exactly what we're talking about today. People have been 46 00:02:57,400 --> 00:02:59,960 Speaker 2: asking questions about how the universe works, trying to make 47 00:03:00,160 --> 00:03:03,240 Speaker 2: connections with the cosmos. For as long as people have 48 00:03:03,280 --> 00:03:05,120 Speaker 2: been asking questions, all you have to do is look 49 00:03:05,200 --> 00:03:06,960 Speaker 2: up at the night sky and wonder, how does that 50 00:03:07,000 --> 00:03:09,160 Speaker 2: all work? Why does it seem so regular? Why are 51 00:03:09,160 --> 00:03:11,880 Speaker 2: their patterns? And then patterns within those patterns, what do 52 00:03:11,960 --> 00:03:15,120 Speaker 2: they reveal about the nature of the universe. Because one 53 00:03:15,120 --> 00:03:17,520 Speaker 2: of my favorite things about the universe is that it 54 00:03:17,560 --> 00:03:20,000 Speaker 2: does seem to follow laws, and we can figure those 55 00:03:20,080 --> 00:03:22,640 Speaker 2: laws out if we pay attention to those patterns and 56 00:03:22,760 --> 00:03:25,320 Speaker 2: try to draw dotted lines between them. And as you say, 57 00:03:25,480 --> 00:03:27,880 Speaker 2: people have been doing that for a long long time. 58 00:03:28,160 --> 00:03:31,600 Speaker 2: We sometimes dismiss our ancient history as like prescience and 59 00:03:31,720 --> 00:03:33,679 Speaker 2: only take things seriously if it's been figured out in 60 00:03:33,680 --> 00:03:36,280 Speaker 2: the last few hundred years. But you know, the development 61 00:03:36,280 --> 00:03:39,240 Speaker 2: of science is much more gradual than is often described 62 00:03:39,240 --> 00:03:42,240 Speaker 2: in history textbooks. People a long long time ago. We're 63 00:03:42,240 --> 00:03:45,520 Speaker 2: thinking methodically and trying to understand the universe, and that's 64 00:03:45,520 --> 00:03:47,760 Speaker 2: what people are still doing. And one of my favorite 65 00:03:47,760 --> 00:03:50,240 Speaker 2: things is trying to think deeply about the nature of 66 00:03:50,400 --> 00:03:53,480 Speaker 2: time and the universe. How far back in space can 67 00:03:53,480 --> 00:03:55,640 Speaker 2: we see, what do we see, and what do we 68 00:03:55,760 --> 00:03:58,880 Speaker 2: learn about how big and how strange the universe is 69 00:03:59,240 --> 00:04:02,520 Speaker 2: as we look into space. And so on today's episode, 70 00:04:02,520 --> 00:04:04,160 Speaker 2: we're going to be doing exactly that. We're going to 71 00:04:04,200 --> 00:04:07,240 Speaker 2: be answering a question a listener asked us about the 72 00:04:07,320 --> 00:04:10,840 Speaker 2: nature of deep time. So today on the podcast, we'll 73 00:04:10,880 --> 00:04:20,440 Speaker 2: be answering listener questions. Summer Solstice Edition. We're so happy 74 00:04:20,560 --> 00:04:22,520 Speaker 2: to be back and be back in your ear with 75 00:04:22,560 --> 00:04:27,120 Speaker 2: this special episode to celebrate the summer Solstice. Happy Solstice, everybody. 76 00:04:26,760 --> 00:04:33,680 Speaker 1: Happy Solstice. Enjoy your roasted pine combs and your chicken 77 00:04:33,760 --> 00:04:36,520 Speaker 1: feather damp and you're huge bonfires. 78 00:04:36,560 --> 00:04:38,320 Speaker 2: I hope you stay up late in the night, stare 79 00:04:38,360 --> 00:04:40,760 Speaker 2: at the stars, wonder about the nature of the universe, 80 00:04:41,040 --> 00:04:43,480 Speaker 2: and then write to me with your questions about it 81 00:04:43,880 --> 00:04:47,000 Speaker 2: questions at Danielanjorge dot com. Don't be shy, send me 82 00:04:47,040 --> 00:04:50,800 Speaker 2: your questions. You will get an answer. And on today's show, 83 00:04:50,800 --> 00:04:54,359 Speaker 2: we're answering a question from Nick in Florida, who's wondering 84 00:04:54,400 --> 00:04:57,080 Speaker 2: about the very oldest things we see in the sky. 85 00:04:57,720 --> 00:04:58,919 Speaker 2: Here is Nick's question. 86 00:04:59,400 --> 00:05:03,920 Speaker 4: Hey Daniel, this is Nick from Jacksonville, Florida. I came 87 00:05:03,960 --> 00:05:06,479 Speaker 4: across an article this morning that taught me something new 88 00:05:06,480 --> 00:05:10,520 Speaker 4: and amazing about the universe. Apparently, beyond the distance of 89 00:05:10,560 --> 00:05:14,880 Speaker 4: approximately fifteen billion light years, objects we see with telescopes 90 00:05:15,000 --> 00:05:19,320 Speaker 4: start becoming larger again instead of smaller. My question is 91 00:05:19,720 --> 00:05:21,719 Speaker 4: how close are we to being able to see this 92 00:05:21,880 --> 00:05:25,400 Speaker 4: far and what will be the implications for cosmology once 93 00:05:25,400 --> 00:05:27,919 Speaker 4: we get there? Thanks and love the show. 94 00:05:28,600 --> 00:05:32,960 Speaker 1: So this is really interesting. I have never actually heard this, 95 00:05:33,160 --> 00:05:37,080 Speaker 1: that objects that you see beyond a certain distance start 96 00:05:37,160 --> 00:05:42,120 Speaker 1: to appear larger, and I also don't understand how we 97 00:05:42,160 --> 00:05:44,359 Speaker 1: can see this far in the first place. 98 00:05:45,360 --> 00:05:48,320 Speaker 2: Yeah, it's really fascinating. It's one of my favorite facts 99 00:05:48,320 --> 00:05:51,360 Speaker 2: about the universe. It really shows us that the universe 100 00:05:51,440 --> 00:05:53,960 Speaker 2: is expanding and that we have a pretty good grasp 101 00:05:54,279 --> 00:05:56,560 Speaker 2: on how that works, or at least what's been happening, 102 00:05:56,880 --> 00:05:59,880 Speaker 2: which is already kind of astounding. The fact that wall 103 00:06:00,040 --> 00:06:02,360 Speaker 2: we've been trapped on this tiny little rock in one 104 00:06:02,440 --> 00:06:05,320 Speaker 2: corner of the universe, we can measure things that tell 105 00:06:05,400 --> 00:06:08,279 Speaker 2: us about the universe on the grandest scale. You know, 106 00:06:08,320 --> 00:06:11,800 Speaker 2: what's happening over billions and billions of light years, and 107 00:06:12,000 --> 00:06:15,039 Speaker 2: what's been going on over the last few billion years. 108 00:06:15,279 --> 00:06:18,680 Speaker 2: It's really incredible what we are able to piece together 109 00:06:18,920 --> 00:06:21,279 Speaker 2: from just the few photons that happen to land on 110 00:06:21,440 --> 00:06:22,000 Speaker 2: our rock. 111 00:06:22,520 --> 00:06:25,400 Speaker 1: That is wild. I mean, it's also just kind of 112 00:06:25,480 --> 00:06:28,520 Speaker 1: weird that in a way we can time travel, but 113 00:06:28,720 --> 00:06:32,520 Speaker 1: just with our eyes and some fancy shaped glass. 114 00:06:33,120 --> 00:06:36,320 Speaker 2: Yeah, it is really amazing. So there's a few different 115 00:06:36,360 --> 00:06:39,360 Speaker 2: things going on here that all come together to make 116 00:06:39,360 --> 00:06:42,120 Speaker 2: this really weird effect that if you can get them 117 00:06:42,160 --> 00:06:44,640 Speaker 2: all working together in your mind, show you how beautiful 118 00:06:44,640 --> 00:06:47,520 Speaker 2: our explanation is. So let's take them one at a time. 119 00:06:48,080 --> 00:06:50,400 Speaker 2: One concept is the one you just measured that looking 120 00:06:50,520 --> 00:06:53,719 Speaker 2: up into the sky is basically time travel, and that's 121 00:06:53,760 --> 00:06:56,520 Speaker 2: because the speed of light is not instantaneous. You know, 122 00:06:56,600 --> 00:06:59,679 Speaker 2: something happens in Andromeda, you don't see it right away. 123 00:07:00,080 --> 00:07:03,400 Speaker 2: It takes time for light to go from Andromeda to 124 00:07:03,640 --> 00:07:06,080 Speaker 2: our eyeballs. And so when we look up at the 125 00:07:06,160 --> 00:07:08,760 Speaker 2: night sky and we see Andromeda, we're not seeing what's 126 00:07:08,800 --> 00:07:12,200 Speaker 2: happening in Andromeda right now. We're seeing what's happening in 127 00:07:12,240 --> 00:07:16,360 Speaker 2: Andromeda when that light left Andromeda. And because Andromeda is 128 00:07:16,520 --> 00:07:20,840 Speaker 2: several million light years away, it means we're seeing photons 129 00:07:20,840 --> 00:07:24,920 Speaker 2: that left Andromeda several million years ago. Andromeda is not 130 00:07:24,960 --> 00:07:27,920 Speaker 2: even in the same place it was when emitted that light, 131 00:07:28,440 --> 00:07:31,440 Speaker 2: and so what we're seeing really is ancient history. And 132 00:07:31,520 --> 00:07:34,520 Speaker 2: the further we look out into the universe, the deeper 133 00:07:34,600 --> 00:07:38,040 Speaker 2: back in time. We are seeing like things are happening 134 00:07:38,040 --> 00:07:40,640 Speaker 2: out there in the deep universe right now, but we 135 00:07:40,720 --> 00:07:43,679 Speaker 2: won't see them for millions or billions of years, depending 136 00:07:43,720 --> 00:07:45,960 Speaker 2: on how far away they are. So as we look 137 00:07:46,000 --> 00:07:48,440 Speaker 2: out into the universe, we are really seeing further and 138 00:07:48,480 --> 00:07:51,040 Speaker 2: back in time just because of this simple basic physics 139 00:07:51,120 --> 00:07:53,720 Speaker 2: fact that light takes time to get to us. 140 00:07:54,000 --> 00:07:58,840 Speaker 1: So you're saying that if Andromeda has a newspaper that 141 00:07:59,040 --> 00:08:01,800 Speaker 1: is really huge that we can see with a telescope, 142 00:08:02,240 --> 00:08:05,440 Speaker 1: by the time that light reaches us, we're looking at 143 00:08:05,440 --> 00:08:07,760 Speaker 1: a pretty old headline. It is out of date. 144 00:08:08,000 --> 00:08:12,440 Speaker 2: Yeah, exactly. And conversely, it means that if Andromeda has 145 00:08:12,520 --> 00:08:16,600 Speaker 2: aliens that point their telescope at us, they're seeing millions 146 00:08:16,600 --> 00:08:19,360 Speaker 2: of years ago. They would see the Earth as it 147 00:08:19,640 --> 00:08:21,960 Speaker 2: was millions of years ago. They wouldn't even know that 148 00:08:22,000 --> 00:08:25,960 Speaker 2: there was an intelligent technological civilization on our planet for 149 00:08:26,120 --> 00:08:29,600 Speaker 2: millions of years, because that's only the very briefest part 150 00:08:29,720 --> 00:08:34,439 Speaker 2: of our history. And so somewhere out there are photons 151 00:08:34,720 --> 00:08:37,000 Speaker 2: from like when the Earth had dinosaurs on it, or 152 00:08:37,040 --> 00:08:39,920 Speaker 2: even further away, there are photons from the Earth when 153 00:08:39,920 --> 00:08:42,600 Speaker 2: it was like just a ball of magma. All those 154 00:08:42,600 --> 00:08:45,480 Speaker 2: photons are still out there in the universe. Somebody could 155 00:08:45,520 --> 00:08:48,040 Speaker 2: be picking them up where they're alien eyeballs and seeing 156 00:08:48,080 --> 00:08:49,800 Speaker 2: the ancient history of our planet. 157 00:08:50,080 --> 00:08:53,119 Speaker 1: I like to imagine that the reason aliens don't contact 158 00:08:53,200 --> 00:08:56,360 Speaker 1: us is they caught us when we had the weird 159 00:08:56,480 --> 00:09:03,640 Speaker 1: Anomalocaris that came marine explosion, giant disgusting shrimp looking thing, 160 00:09:03,679 --> 00:09:06,839 Speaker 1: and they're like, no, thank you, I'm not gonna get 161 00:09:06,840 --> 00:09:07,800 Speaker 1: in touch with that planet. 162 00:09:07,800 --> 00:09:08,520 Speaker 2: It's too icky. 163 00:09:08,920 --> 00:09:09,120 Speaker 3: Nah. 164 00:09:10,400 --> 00:09:12,720 Speaker 1: Yes, don't like shellfish seafood. 165 00:09:12,960 --> 00:09:15,880 Speaker 2: So that's one concept, right, Things in the sky are 166 00:09:15,960 --> 00:09:18,440 Speaker 2: old news. Right, We're not seeing the universe as it 167 00:09:18,520 --> 00:09:20,960 Speaker 2: is now. We're seeing the universe as it was. And 168 00:09:21,000 --> 00:09:23,640 Speaker 2: on one hand, that's frustrating because it means like we're 169 00:09:23,679 --> 00:09:27,000 Speaker 2: missing out on the latest, greatest news. On the other hand, 170 00:09:27,200 --> 00:09:30,320 Speaker 2: it's a huge gift. It means we can see back 171 00:09:30,400 --> 00:09:32,840 Speaker 2: in time and like on Earth, you want to know 172 00:09:33,160 --> 00:09:35,160 Speaker 2: what happened during the Roman Era or what happened a 173 00:09:35,160 --> 00:09:37,480 Speaker 2: million years ago, you got to look for clues that 174 00:09:37,559 --> 00:09:39,320 Speaker 2: happened to be here and be left over. Most of 175 00:09:39,320 --> 00:09:42,400 Speaker 2: that stuff is destroyed or buried, but in the history 176 00:09:42,440 --> 00:09:44,400 Speaker 2: of the universe, you just look into the sky. It's 177 00:09:44,440 --> 00:09:47,559 Speaker 2: all still there. It's just arriving right now, fresh as 178 00:09:47,600 --> 00:09:49,880 Speaker 2: the day was emitted. So you want to know what 179 00:09:49,920 --> 00:09:52,080 Speaker 2: happened in the universe a million years ago, or a 180 00:09:52,120 --> 00:09:54,640 Speaker 2: billion years ago or ten billion years ago, you just 181 00:09:54,679 --> 00:09:58,440 Speaker 2: build bigger telescopes to capture more distant, fainter photons, and 182 00:09:58,480 --> 00:10:01,040 Speaker 2: you can see it. It's all still they're in the sky. 183 00:10:01,480 --> 00:10:04,280 Speaker 1: So the further back in time we want to go 184 00:10:04,480 --> 00:10:08,680 Speaker 1: in understanding our universe, the further way look exactly. 185 00:10:09,040 --> 00:10:11,679 Speaker 2: So you have to imagine these shells, like in a 186 00:10:11,760 --> 00:10:13,840 Speaker 2: shell that's very close to the Earth, we're seeing the 187 00:10:13,880 --> 00:10:16,440 Speaker 2: more recent past. We can't see the distant past in 188 00:10:16,480 --> 00:10:19,480 Speaker 2: a close by shell, but we can't see the ancient 189 00:10:19,520 --> 00:10:22,480 Speaker 2: past in a more distant shell. So we can't just 190 00:10:22,520 --> 00:10:24,200 Speaker 2: like dial the knob and say I want to see 191 00:10:24,200 --> 00:10:27,400 Speaker 2: what happened over here at that time. We can only 192 00:10:27,440 --> 00:10:31,800 Speaker 2: see a certain time for every certain location because photons 193 00:10:31,840 --> 00:10:34,520 Speaker 2: are just now arriving from that location based on how 194 00:10:34,559 --> 00:10:37,240 Speaker 2: far away they are, all right, So that's one concept. 195 00:10:37,600 --> 00:10:40,480 Speaker 2: The other concept is how big things look in the sky. 196 00:10:41,200 --> 00:10:43,640 Speaker 2: And so to understand this first, let's just imagine the 197 00:10:43,720 --> 00:10:46,960 Speaker 2: universe is not expanding. Imagine that you have galaxies and 198 00:10:47,000 --> 00:10:50,120 Speaker 2: they're just hanging in space and nothing is moving. Everything 199 00:10:50,160 --> 00:10:54,000 Speaker 2: is just hanging there. There's no relative velocity. Then you 200 00:10:54,000 --> 00:10:58,320 Speaker 2: would expect things that are further away look smaller, right, because, 201 00:10:58,360 --> 00:11:00,840 Speaker 2: for example, if you have some galaxy and it's right 202 00:11:00,920 --> 00:11:04,240 Speaker 2: up in your eyeball, then photons from one side of 203 00:11:04,240 --> 00:11:05,880 Speaker 2: the galaxy and photons from the other side of the 204 00:11:05,920 --> 00:11:09,160 Speaker 2: galaxy are gonna come from very very different angles. Now 205 00:11:09,200 --> 00:11:12,840 Speaker 2: you move that galaxy further away in the sky, photons 206 00:11:12,840 --> 00:11:15,679 Speaker 2: from two different edges of the galaxy are now getting 207 00:11:15,679 --> 00:11:18,080 Speaker 2: closer and closer together, so they just seem smaller in 208 00:11:18,120 --> 00:11:20,640 Speaker 2: the sky. This is no magic. It's just like you 209 00:11:20,679 --> 00:11:23,079 Speaker 2: hold your finger close to your eyeball, looks big. You 210 00:11:23,120 --> 00:11:25,360 Speaker 2: push it further away, it looks smaller. 211 00:11:25,480 --> 00:11:28,200 Speaker 1: Right, It's just perspective, I see, Yes, So I have 212 00:11:28,400 --> 00:11:31,959 Speaker 1: been told that people from far away are not tiny people. 213 00:11:32,040 --> 00:11:35,640 Speaker 1: They are just far away. So all right, that makes 214 00:11:35,679 --> 00:11:36,319 Speaker 1: perfect sense. 215 00:11:36,400 --> 00:11:39,280 Speaker 2: Yeah, exactly, And we have an intuition for this exactly 216 00:11:39,320 --> 00:11:41,440 Speaker 2: the way you describe you don't think that people who 217 00:11:41,480 --> 00:11:43,400 Speaker 2: are standing next to you are giants and people who 218 00:11:43,400 --> 00:11:46,840 Speaker 2: are far away are midgets. You know this, and you 219 00:11:47,160 --> 00:11:49,640 Speaker 2: invert it in your mind. When you see people, you 220 00:11:49,679 --> 00:11:52,160 Speaker 2: can tell how far away they are, and so you 221 00:11:52,679 --> 00:11:55,880 Speaker 2: estimate their actual size because you've taken that into account. Right, 222 00:11:55,920 --> 00:11:58,720 Speaker 2: You have this intuition for things looking small far away 223 00:11:58,760 --> 00:12:01,160 Speaker 2: and things looking big close up, and you'll count for 224 00:12:01,200 --> 00:12:04,079 Speaker 2: this naturally. So if the universe was like that and 225 00:12:04,120 --> 00:12:06,640 Speaker 2: nothing was moving, then it would just look like that. 226 00:12:06,679 --> 00:12:10,160 Speaker 2: Things that are further away would look smaller. But there's 227 00:12:10,240 --> 00:12:12,600 Speaker 2: one more effect you have to throw into the mix, 228 00:12:13,160 --> 00:12:16,600 Speaker 2: and that's the expansion of the universe. Things are not 229 00:12:16,800 --> 00:12:20,440 Speaker 2: just hanging in space. There's a relative velocity there. Space 230 00:12:20,520 --> 00:12:23,960 Speaker 2: is expanding between galaxies, or another way to think about 231 00:12:23,960 --> 00:12:26,840 Speaker 2: that is galaxies are running away from us and from 232 00:12:26,880 --> 00:12:29,800 Speaker 2: each other, so everything is getting further and further away. 233 00:12:30,600 --> 00:12:33,199 Speaker 2: And what that means is that the light we're seeing 234 00:12:33,200 --> 00:12:36,600 Speaker 2: from those galaxies is not from where they are now, 235 00:12:36,960 --> 00:12:40,400 Speaker 2: it's from where they were when they emitted that light. 236 00:12:40,760 --> 00:12:43,959 Speaker 2: Oo okay, right, So, for example, imagine something on the 237 00:12:44,080 --> 00:12:46,800 Speaker 2: very distant edge of the universe. We talk about how 238 00:12:46,840 --> 00:12:50,040 Speaker 2: something could be forty five billion light years away, the 239 00:12:50,160 --> 00:12:53,839 Speaker 2: furthest things in our observable universe, all right, But when 240 00:12:53,840 --> 00:12:55,840 Speaker 2: we talk about that, we mean that's how far away 241 00:12:55,840 --> 00:12:59,559 Speaker 2: it is now, not how far away it was when 242 00:12:59,559 --> 00:13:02,120 Speaker 2: it admitted the light that's now coming to us, that's 243 00:13:02,160 --> 00:13:05,560 Speaker 2: now arriving on Earth. It was much much closer when 244 00:13:05,559 --> 00:13:08,480 Speaker 2: it emitted that light. What's happened in the intervening period 245 00:13:08,800 --> 00:13:11,760 Speaker 2: as that photon has flown through space towards us is 246 00:13:11,800 --> 00:13:14,760 Speaker 2: the universe has expanded and it's gotten further and further away. 247 00:13:15,000 --> 00:13:17,640 Speaker 1: Okay, So if I try to think about this on 248 00:13:17,720 --> 00:13:21,480 Speaker 1: human scale, you have various people standing out in a field, 249 00:13:22,240 --> 00:13:24,680 Speaker 1: and it's a very big field. So I need a 250 00:13:24,679 --> 00:13:29,880 Speaker 1: telescope for me to see people, and it's a telescope 251 00:13:29,920 --> 00:13:33,079 Speaker 1: with a slight delay, or a camera, let's say a camera. 252 00:13:33,120 --> 00:13:35,880 Speaker 1: It's got a delay in it, so I will only 253 00:13:35,960 --> 00:13:39,360 Speaker 1: see them after a while. So like, I could be 254 00:13:39,920 --> 00:13:43,280 Speaker 1: looking at these people who are further away, but then 255 00:13:43,320 --> 00:13:45,600 Speaker 1: the people who are closer to me, let's say they 256 00:13:45,640 --> 00:13:49,720 Speaker 1: are running away from me at a faster rate, so 257 00:13:49,800 --> 00:13:53,800 Speaker 1: they might with my delayed camera, look further away by 258 00:13:53,840 --> 00:13:56,680 Speaker 1: the time I get my snapshot than the ones who 259 00:13:56,720 --> 00:13:59,920 Speaker 1: were actually further away from me, but they look bigger 260 00:14:00,120 --> 00:14:02,880 Speaker 1: because they were not running away from me as fast 261 00:14:02,880 --> 00:14:03,319 Speaker 1: as the other. 262 00:14:03,480 --> 00:14:06,680 Speaker 2: Yeah, exactly, you have old information, and so you're taking 263 00:14:06,720 --> 00:14:08,880 Speaker 2: these snapshots and you're seeing people where they were when 264 00:14:08,920 --> 00:14:10,600 Speaker 2: the picture was taken. But if the picture takes a 265 00:14:10,600 --> 00:14:12,600 Speaker 2: while to get to you, by the time it does, 266 00:14:12,679 --> 00:14:16,679 Speaker 2: they could be much further away, right. And that's important 267 00:14:16,679 --> 00:14:19,640 Speaker 2: to think about because that affects how big they look 268 00:14:19,760 --> 00:14:22,480 Speaker 2: in the sky because when we talk about things that 269 00:14:22,520 --> 00:14:26,080 Speaker 2: are really really far away, we're seeing them remember as 270 00:14:26,120 --> 00:14:28,640 Speaker 2: they were when they emitted those photons, and if they 271 00:14:28,640 --> 00:14:31,520 Speaker 2: were much closer when they emitted those photons, they took 272 00:14:31,600 --> 00:14:34,800 Speaker 2: up more space in the sky because they were closer. 273 00:14:35,200 --> 00:14:38,400 Speaker 2: So those photons have been flying towards us those millions 274 00:14:38,480 --> 00:14:41,080 Speaker 2: or billions of years, but they started pretty close by, right, 275 00:14:41,280 --> 00:14:44,080 Speaker 2: So they started further apart because the thing was closer 276 00:14:44,080 --> 00:14:47,000 Speaker 2: to us. So there are two effects happening here. One 277 00:14:47,080 --> 00:14:49,680 Speaker 2: is things that are further away look smaller, right, But 278 00:14:49,720 --> 00:14:52,640 Speaker 2: the other effect is this expansion effect that some of 279 00:14:52,640 --> 00:14:55,520 Speaker 2: those things that are now really really far away were 280 00:14:55,720 --> 00:14:59,480 Speaker 2: closer when they emitted the photons. So these two competing 281 00:14:59,520 --> 00:15:02,360 Speaker 2: effects there. And so what that means is that if 282 00:15:02,400 --> 00:15:06,120 Speaker 2: we look at nearby stuff, mostly the first effect dominates 283 00:15:06,400 --> 00:15:09,000 Speaker 2: that things that are further away look smaller. So as 284 00:15:09,000 --> 00:15:11,760 Speaker 2: you look out into the night sky, stuff that's further 285 00:15:11,800 --> 00:15:14,760 Speaker 2: away looks smaller and smaller and smaller. But then there's 286 00:15:14,800 --> 00:15:18,280 Speaker 2: a point from about ten billion years ago when the 287 00:15:18,320 --> 00:15:21,360 Speaker 2: other effects starts to dominate. When we're seeing stuff that 288 00:15:21,480 --> 00:15:24,520 Speaker 2: was much closer when it admitted that light. Stuff looks 289 00:15:24,640 --> 00:15:27,360 Speaker 2: smaller and smaller and smaller as it gets further away 290 00:15:27,720 --> 00:15:30,600 Speaker 2: until about ten billion years into the past, and then 291 00:15:30,640 --> 00:15:34,000 Speaker 2: stuff starts to look bigger and bigger. So the oldest 292 00:15:34,000 --> 00:15:37,040 Speaker 2: stuff actually looks bigger in the night sky than some 293 00:15:37,200 --> 00:15:39,560 Speaker 2: of the closer stuff, some of the more recent stuff, 294 00:15:39,800 --> 00:15:42,120 Speaker 2: because you have these two effects that are competing with 295 00:15:42,200 --> 00:15:42,760 Speaker 2: each other. 296 00:15:42,760 --> 00:15:46,680 Speaker 1: Because we're basically seeing like an after image of something 297 00:15:46,840 --> 00:15:51,480 Speaker 1: that was going Yeah, it's actually not further from us. 298 00:15:51,520 --> 00:15:54,840 Speaker 1: I mean that the actual star is that was there, 299 00:15:54,960 --> 00:15:58,880 Speaker 1: but those photons that after image are finally hitting us, 300 00:15:58,960 --> 00:16:01,320 Speaker 1: representing where in the sky. 301 00:16:01,560 --> 00:16:03,320 Speaker 2: When we talk about the universe, we talk about where 302 00:16:03,360 --> 00:16:05,080 Speaker 2: things are now, that's where we put them in our 303 00:16:05,120 --> 00:16:07,800 Speaker 2: mental maps, but we don't think about where they were 304 00:16:08,040 --> 00:16:10,960 Speaker 2: when they emitted that light. And so if you just 305 00:16:11,040 --> 00:16:12,960 Speaker 2: line things up based on where they were when they 306 00:16:13,000 --> 00:16:15,800 Speaker 2: emitted that light, then yes, closer things would look bigger, 307 00:16:15,840 --> 00:16:18,560 Speaker 2: and further things would look more distant. But because the 308 00:16:18,600 --> 00:16:21,400 Speaker 2: expansion of the universe, not all the photons that are 309 00:16:21,480 --> 00:16:25,080 Speaker 2: arriving here are perfectly lined up with where things are now, 310 00:16:25,720 --> 00:16:27,840 Speaker 2: So things that are more distant now can actually look 311 00:16:27,880 --> 00:16:31,960 Speaker 2: closer than things that actually are closer still, so there's 312 00:16:32,000 --> 00:16:35,920 Speaker 2: this amazing effect in cosmology. And so Nick is asking 313 00:16:35,960 --> 00:16:39,920 Speaker 2: about this effect, and he's wondering, can we see this yet? 314 00:16:39,920 --> 00:16:42,040 Speaker 2: Can we see far enough out into the universe to 315 00:16:42,080 --> 00:16:45,000 Speaker 2: see this turnover where the really distant stuff starts to 316 00:16:45,000 --> 00:16:47,760 Speaker 2: get larger and larger again, and what does that mean 317 00:16:47,800 --> 00:16:51,720 Speaker 2: for cosmology? And the answer Nick is that yes, we 318 00:16:51,840 --> 00:16:55,000 Speaker 2: already can see that. We can see much further than 319 00:16:55,080 --> 00:16:57,920 Speaker 2: ten billion years into our history. We can see all 320 00:16:57,960 --> 00:17:01,000 Speaker 2: the way back to almost fourteen billion in years. So 321 00:17:01,040 --> 00:17:03,880 Speaker 2: we have observed this. This is not like a theoretical 322 00:17:03,920 --> 00:17:06,480 Speaker 2: concept that people are wondering about and going ooh, maybe 323 00:17:06,560 --> 00:17:09,400 Speaker 2: in the future sometime. This is something we see. We've 324 00:17:09,520 --> 00:17:13,200 Speaker 2: measured this, and this really nicely confirms our whole model 325 00:17:13,280 --> 00:17:16,440 Speaker 2: for how the universe is expanding and how that expansion 326 00:17:16,560 --> 00:17:20,600 Speaker 2: is accelerating. It's all encoded in the distances and the 327 00:17:20,640 --> 00:17:22,560 Speaker 2: intensity of stuff in the sky. 328 00:17:22,960 --> 00:17:25,200 Speaker 1: Did anyone come up with a theory that this might 329 00:17:25,240 --> 00:17:28,120 Speaker 1: be the case before we actually observed it, or did 330 00:17:28,119 --> 00:17:31,399 Speaker 1: we observe it and then come up with the theory 331 00:17:31,440 --> 00:17:32,000 Speaker 1: behind it. 332 00:17:32,119 --> 00:17:34,879 Speaker 2: Oh, yeah, great question. It al sort came together at 333 00:17:34,920 --> 00:17:37,960 Speaker 2: the same moment when we realized that the universe's expansion 334 00:17:38,160 --> 00:17:40,879 Speaker 2: was accelerating. We didn't even know that until we had 335 00:17:40,880 --> 00:17:43,800 Speaker 2: a solid way for measuring how far away things were 336 00:17:43,920 --> 00:17:46,560 Speaker 2: when they are really distant. We only figured that out 337 00:17:46,560 --> 00:17:49,200 Speaker 2: when we were able to calibrate type one A supernova 338 00:17:49,600 --> 00:17:52,240 Speaker 2: around the turn of the century, like twenty five years ago, 339 00:17:52,640 --> 00:17:54,879 Speaker 2: and that's what told us that the expansion of the 340 00:17:54,960 --> 00:17:58,280 Speaker 2: universe was different from what we expected. It's actually accelerating, 341 00:17:58,640 --> 00:18:00,840 Speaker 2: and that changed the whole picture. At the same time, 342 00:18:00,960 --> 00:18:03,520 Speaker 2: gave us a way to measure the distances to these 343 00:18:03,520 --> 00:18:07,120 Speaker 2: big things and showed us that distant objects are actually 344 00:18:07,280 --> 00:18:11,399 Speaker 2: larger than some nearer objects in our sky. And so 345 00:18:11,440 --> 00:18:13,240 Speaker 2: it all sort of came together about the same time 346 00:18:13,280 --> 00:18:15,960 Speaker 2: when we had this revolution in our understanding about the 347 00:18:16,000 --> 00:18:19,280 Speaker 2: expansion history of the universe. It's really nice confirmation of 348 00:18:19,320 --> 00:18:19,960 Speaker 2: that idea. 349 00:18:20,200 --> 00:18:23,919 Speaker 1: That's incredible. I mean, that must be so special as 350 00:18:24,000 --> 00:18:29,240 Speaker 1: a scientist to actually see these things that fit into 351 00:18:30,080 --> 00:18:32,119 Speaker 1: all of this theory and all all of these things 352 00:18:32,119 --> 00:18:34,480 Speaker 1: that you're discovering of like, oh yeah, there is visual 353 00:18:34,520 --> 00:18:36,280 Speaker 1: confirmation of this stuff at ward. 354 00:18:36,359 --> 00:18:38,440 Speaker 2: It's amazing that we can look up the night sky 355 00:18:38,520 --> 00:18:41,119 Speaker 2: and we can piece the story together from again, just 356 00:18:41,200 --> 00:18:44,400 Speaker 2: these photons and the patterns within them. And for thousands 357 00:18:44,400 --> 00:18:47,360 Speaker 2: of years, our ancestors desperately wanted to do that. They 358 00:18:47,440 --> 00:18:49,400 Speaker 2: looked up at the stars and wondered what they meant, 359 00:18:49,400 --> 00:18:52,520 Speaker 2: and found patterns, but never really had an understanding anywhere 360 00:18:52,520 --> 00:18:55,439 Speaker 2: close to what we have until very very recently. So 361 00:18:55,600 --> 00:19:00,680 Speaker 2: many people lived in such deep ignorance. Unfortunately, real blessed 362 00:19:00,800 --> 00:19:02,800 Speaker 2: to live in an era when we know anything about 363 00:19:02,840 --> 00:19:05,160 Speaker 2: the universe. But you know, I wonder about the deep 364 00:19:05,200 --> 00:19:08,080 Speaker 2: future when people will know so much more about how 365 00:19:08,119 --> 00:19:10,199 Speaker 2: the universe works, and wonder what it was like to 366 00:19:10,240 --> 00:19:11,879 Speaker 2: be as ignorant as we are today. 367 00:19:12,400 --> 00:19:14,920 Speaker 1: Uh, blissful is what I would say. 368 00:19:15,760 --> 00:19:17,480 Speaker 2: All right, If you're listening to this podcast in the 369 00:19:17,560 --> 00:19:19,720 Speaker 2: year three thousand know that we were dumb, but we 370 00:19:19,760 --> 00:19:20,320 Speaker 2: were happy. 371 00:19:20,560 --> 00:19:24,000 Speaker 1: We were dumb and happy. Take that future us all right. 372 00:19:24,040 --> 00:19:26,040 Speaker 2: Thanks very much to Nick for your question, and thanks 373 00:19:26,040 --> 00:19:28,760 Speaker 2: to everybody who wonders about how the universe works and 374 00:19:28,840 --> 00:19:30,840 Speaker 2: wants to figure it out. Please don't be shy to 375 00:19:30,840 --> 00:19:34,119 Speaker 2: write to me to questions at Danielandhorgheay dot com. You'll 376 00:19:34,119 --> 00:19:37,080 Speaker 2: always hear back. Happy Summer solsis everybody, and you'll hear 377 00:19:37,119 --> 00:19:44,640 Speaker 2: from us again soon. For more science and curiosity, come 378 00:19:44,680 --> 00:19:47,480 Speaker 2: find us on social media, where we answer questions and 379 00:19:47,640 --> 00:19:51,800 Speaker 2: post videos. We're on Twitter, This org, Instant, and now TikTok. 380 00:19:52,520 --> 00:19:55,320 Speaker 2: Thanks for listening, and remember that Daniel and Jorge Explain 381 00:19:55,400 --> 00:19:59,320 Speaker 2: the Universe is a production of Iheartwriting. For more podcasts 382 00:19:59,400 --> 00:20:03,360 Speaker 2: from my Heart Radio, visit the iHeartRadio app, Apple Podcasts, 383 00:20:03,480 --> 00:20:05,800 Speaker 2: or wherever you listen to your favorite shows.