WEBVTT - What is a black hole eclipse?

0:00:08.440 --> 0:00:12.399
<v Speaker 1>Hey or hey, are you a fan of Pokemon cards? Yeah,

0:00:12.400 --> 0:00:14.000
<v Speaker 1>a little bit. My son used to play them. My

0:00:14.040 --> 0:00:17.439
<v Speaker 1>son also, though I think he mostly collected and traded them.

0:00:17.480 --> 0:00:20.680
<v Speaker 1>I don't think he ever actually played with them. M Yeah,

0:00:20.680 --> 0:00:22.279
<v Speaker 1>I think that happens a lot, although I did play

0:00:22.360 --> 0:00:24.640
<v Speaker 1>with him for a few times. It's a pretty interesting game.

0:00:24.680 --> 0:00:26.080
<v Speaker 1>And do you have any of those cards with like

0:00:26.239 --> 0:00:29.040
<v Speaker 1>super awesome powers? Yeah? They have pretty good names, like

0:00:29.240 --> 0:00:32.959
<v Speaker 1>flame body. My personal favorite is the card that can

0:00:32.960 --> 0:00:37.120
<v Speaker 1>do a black hole eclipse. Although that sounds kind of

0:00:37.159 --> 0:00:39.959
<v Speaker 1>like a random combination of words from physics that they

0:00:40.000 --> 0:00:42.640
<v Speaker 1>just kind of put together. I think that's the same

0:00:42.640 --> 0:00:46.000
<v Speaker 1>way that physicist name things though. Ah, so you admitted

0:00:46.560 --> 0:00:49.720
<v Speaker 1>it's all random. We just type the words into an

0:00:49.720 --> 0:00:52.320
<v Speaker 1>online random number generator and that's where we go with.

0:00:53.200 --> 0:00:55.800
<v Speaker 1>They have a bunch of physicists working for Pokemon, just

0:00:55.840 --> 0:00:57.680
<v Speaker 1>in case that the whole physics scurity doesn't work out.

0:00:57.720 --> 0:01:00.880
<v Speaker 1>Do you have a promising career working for That's always

0:01:00.880 --> 0:01:18.600
<v Speaker 1>been my backup plane. Hi am Poor Hamming, cartoonist and

0:01:18.600 --> 0:01:21.840
<v Speaker 1>the co author of Frequently Asked Questions about the Universe. Hi.

0:01:22.000 --> 0:01:24.720
<v Speaker 1>I'm Daniel. I'm a particle physicist and a professor at

0:01:24.800 --> 0:01:27.600
<v Speaker 1>UC Irvine, and I probably have hundreds of dollars worth

0:01:27.600 --> 0:01:30.520
<v Speaker 1>of Pokemon cards somewhere in the closets of my home.

0:01:31.200 --> 0:01:33.679
<v Speaker 1>Are they wrapped an individual plastic though, to keep him

0:01:33.680 --> 0:01:36.640
<v Speaker 1>in mint condition? Otherwise I'm not sure they're worth that much.

0:01:38.840 --> 0:01:41.839
<v Speaker 1>They have definitely been prepared as an investment in the future.

0:01:42.080 --> 0:01:44.840
<v Speaker 1>That's how you plan to pay for your son's college education.

0:01:44.959 --> 0:01:46.680
<v Speaker 1>I think that's how my son plans to pay for

0:01:46.720 --> 0:01:49.240
<v Speaker 1>his retirement. Yeah. Wow, if it's worth that much, maybe

0:01:49.240 --> 0:01:51.880
<v Speaker 1>they should conveniently disappear from your closet. Only if I

0:01:51.880 --> 0:01:53.960
<v Speaker 1>could find them in my son's closet. I think that's

0:01:54.000 --> 0:01:57.720
<v Speaker 1>part of his security plan. Yes, it's such a mess,

0:01:57.760 --> 0:02:00.080
<v Speaker 1>it's like a black hole in itself, but anyway is

0:02:00.080 --> 0:02:02.840
<v Speaker 1>Welcome to our podcast Daniel and Jorge Explain the Universe,

0:02:02.880 --> 0:02:05.640
<v Speaker 1>a production of I Heart Radio in which we try

0:02:05.680 --> 0:02:08.800
<v Speaker 1>to clean up a mess that is this universe and

0:02:08.919 --> 0:02:12.040
<v Speaker 1>all of its crazy, confusing glory. We dig right into

0:02:12.120 --> 0:02:15.000
<v Speaker 1>everything that doesn't make sense, everything that should make sense,

0:02:15.040 --> 0:02:18.000
<v Speaker 1>and things that might never make sense. We talked about

0:02:18.000 --> 0:02:21.040
<v Speaker 1>the biggest questions at the heart of philosophical inquiries about

0:02:21.040 --> 0:02:24.240
<v Speaker 1>the nature of our universe, and we talk about practical

0:02:24.280 --> 0:02:27.400
<v Speaker 1>stuff like how things around you actually work. We dive

0:02:27.440 --> 0:02:30.000
<v Speaker 1>into all of these questions and try to explain to

0:02:30.040 --> 0:02:33.680
<v Speaker 1>you what scientists do and do not know about them

0:02:33.720 --> 0:02:36.560
<v Speaker 1>because it is a pretty fun universe full of interesting

0:02:36.639 --> 0:02:39.600
<v Speaker 1>and amazing characters, not all of them with superpowers like

0:02:39.639 --> 0:02:42.880
<v Speaker 1>Pokemon characters, but there are a lot of interesting objects

0:02:42.919 --> 0:02:46.680
<v Speaker 1>out there in the universe with the seemingly superpowerful powers.

0:02:46.880 --> 0:02:49.000
<v Speaker 1>And it is our belief, or at least our hope,

0:02:49.080 --> 0:02:52.320
<v Speaker 1>that the universe does make sense, that it's following some

0:02:52.360 --> 0:02:54.560
<v Speaker 1>set of rules, and that if we dig into it

0:02:54.639 --> 0:02:56.919
<v Speaker 1>hard enough, if we use our brains, if we come

0:02:57.000 --> 0:02:59.720
<v Speaker 1>up with a clever set of experiments, we can figure

0:02:59.720 --> 0:03:01.720
<v Speaker 1>out what those rules are. That in the end, there

0:03:01.800 --> 0:03:04.320
<v Speaker 1>isn't magic in the universe, but that everything can be

0:03:04.400 --> 0:03:07.800
<v Speaker 1>explained with science. I'm not sure the same can be

0:03:07.840 --> 0:03:10.880
<v Speaker 1>said about Pokemon powers. What are you saying that Pokemon

0:03:11.080 --> 0:03:15.160
<v Speaker 1>aren't physically accurate there? How do you know, Daniel, I'm

0:03:15.200 --> 0:03:17.440
<v Speaker 1>not sure we have to suspend disbelief. But I did

0:03:17.520 --> 0:03:20.120
<v Speaker 1>do a bit of research into what the black hole

0:03:20.200 --> 0:03:23.600
<v Speaker 1>eclipse move is for the Pokemon character, and here's the

0:03:23.639 --> 0:03:27.880
<v Speaker 1>official description. The user gathers dark energy with its Z

0:03:28.120 --> 0:03:33.600
<v Speaker 1>power and forms a black hole that sucks the opponent up. Interesting.

0:03:33.680 --> 0:03:35.839
<v Speaker 1>That seems like a bit of a dangerous weapon there,

0:03:35.840 --> 0:03:38.680
<v Speaker 1>because once you start the black hole, I guess, can

0:03:38.720 --> 0:03:40.880
<v Speaker 1>you turn it off? Or is there a Z switch

0:03:40.960 --> 0:03:44.360
<v Speaker 1>for it? It depends on what your Z power can do.

0:03:44.800 --> 0:03:47.400
<v Speaker 1>If you can tap into dark energy and expand or

0:03:47.440 --> 0:03:50.360
<v Speaker 1>contract space, then hey, you have got a lot of options. Well,

0:03:50.360 --> 0:03:52.800
<v Speaker 1>there is the idea that maybe there are unknown forces

0:03:52.800 --> 0:03:55.400
<v Speaker 1>in the universe we haven't discovered. Maybe the Z force

0:03:55.520 --> 0:03:57.520
<v Speaker 1>is one of them. And if I discovered an unknown

0:03:57.560 --> 0:03:59.640
<v Speaker 1>force and called it the Z force, would you be

0:03:59.640 --> 0:04:03.080
<v Speaker 1>impress with my naming? I guess I mean to try

0:04:03.120 --> 0:04:05.160
<v Speaker 1>out any of the other letters in the alphabet first.

0:04:05.240 --> 0:04:07.440
<v Speaker 1>The Z force makes me think it's related to the

0:04:07.560 --> 0:04:10.680
<v Speaker 1>Z boson, which we know is a very feeble boson.

0:04:10.760 --> 0:04:14.320
<v Speaker 1>It carries the weak force, probably not capable of making

0:04:14.400 --> 0:04:17.840
<v Speaker 1>black holes. So there is technically a Z force in

0:04:17.880 --> 0:04:20.880
<v Speaker 1>the universe right now, like the force made by a

0:04:21.000 --> 0:04:24.600
<v Speaker 1>Z boson is technically a Z force. Yeah, that's right,

0:04:24.640 --> 0:04:26.360
<v Speaker 1>though I'm not sure you can use it to gather

0:04:26.440 --> 0:04:29.520
<v Speaker 1>any dark energy and throw your opponent into a black hole.

0:04:29.640 --> 0:04:32.039
<v Speaker 1>But hey, best to luck to you. How do you know, Daniel,

0:04:32.520 --> 0:04:34.560
<v Speaker 1>have you tried? I haven't tried, but I'm going to

0:04:34.640 --> 0:04:38.080
<v Speaker 1>write a grand proposal to the Pokemon Science Foundation to

0:04:38.120 --> 0:04:40.360
<v Speaker 1>see if I can get some funds to try it out. Yeah,

0:04:40.360 --> 0:04:42.400
<v Speaker 1>the PSF, they fund a lot of work out here.

0:04:42.640 --> 0:04:45.000
<v Speaker 1>But technically, in a multiverse, isn't it possible that there

0:04:45.040 --> 0:04:48.160
<v Speaker 1>are Pokemon characters out there? I mean, if you say

0:04:48.200 --> 0:04:50.840
<v Speaker 1>in a multiverse, isn't it possible that I suppose almost

0:04:50.839 --> 0:04:54.200
<v Speaker 1>anything is possible because in some theories of the multiverse

0:04:54.279 --> 0:04:57.719
<v Speaker 1>there are universes with other laws of physics, which basically

0:04:57.760 --> 0:05:01.600
<v Speaker 1>allows almost anything to happen. Oh, there you go, It's official.

0:05:01.640 --> 0:05:06.120
<v Speaker 1>Here in the podcast, Daniel thinks Pokemon are real. They

0:05:06.160 --> 0:05:09.240
<v Speaker 1>are a really good investment in my son's feature and

0:05:09.279 --> 0:05:12.440
<v Speaker 1>a real possibility. But it is interesting. How did you

0:05:12.520 --> 0:05:17.039
<v Speaker 1>end up googling Pokemon powers online? What's going on there? Daniel? No,

0:05:17.160 --> 0:05:20.520
<v Speaker 1>I was googling black hole eclipse, of course, in preparation

0:05:20.600 --> 0:05:23.520
<v Speaker 1>for today's episode. And the top hit was not black

0:05:23.560 --> 0:05:26.920
<v Speaker 1>holes or eclipses or anything scientific. The top like ten

0:05:27.040 --> 0:05:29.479
<v Speaker 1>hits were all about Pokemon. I think that tells you

0:05:29.480 --> 0:05:32.599
<v Speaker 1>a little bit about the priority of the Internet. But

0:05:32.680 --> 0:05:34.200
<v Speaker 1>it is interesting. What do you think is going on

0:05:34.240 --> 0:05:37.799
<v Speaker 1>inside the head of those Pokemon creators, artists and writers

0:05:37.839 --> 0:05:39.440
<v Speaker 1>when they come up with these things, Right, because they

0:05:39.760 --> 0:05:41.800
<v Speaker 1>used to work dark energy, they must know a little

0:05:41.839 --> 0:05:44.440
<v Speaker 1>bit of something about physics. Well, you know, I think

0:05:44.480 --> 0:05:47.680
<v Speaker 1>as they make more and more Pokemon characters, that have

0:05:47.720 --> 0:05:49.920
<v Speaker 1>to be more and more powerful or as my son

0:05:49.960 --> 0:05:53.160
<v Speaker 1>would say, totally opie, and so they want to come

0:05:53.200 --> 0:05:55.720
<v Speaker 1>up with something really dramatics and they're really crazy. And

0:05:55.760 --> 0:05:57.719
<v Speaker 1>I guess black holes are on the top of the

0:05:57.760 --> 0:06:00.920
<v Speaker 1>list of like aspirational powers to whether you can make

0:06:00.960 --> 0:06:03.520
<v Speaker 1>a black hole using dark energy. You know, we don't

0:06:03.520 --> 0:06:05.920
<v Speaker 1>really know what dark energy is at all. We just

0:06:06.000 --> 0:06:09.960
<v Speaker 1>know that it's accelerating the expansion of space and separating

0:06:09.960 --> 0:06:12.200
<v Speaker 1>the black holes from each other. So if anything, it's

0:06:12.279 --> 0:06:14.680
<v Speaker 1>keeping black holes from getting bigger. Well, I guess my

0:06:14.760 --> 0:06:17.920
<v Speaker 1>question is what kind of energy car does that attack us?

0:06:18.040 --> 0:06:21.320
<v Speaker 1>Dark energy cars? Is there such a thing? If there

0:06:21.360 --> 0:06:24.680
<v Speaker 1>isn't such a thing, then there should be Pokemon Science Foundation,

0:06:24.839 --> 0:06:27.800
<v Speaker 1>please fund that. There should be a science type Pokemon.

0:06:28.279 --> 0:06:31.159
<v Speaker 1>You know, there's like a water type, fire type. There

0:06:31.160 --> 0:06:33.520
<v Speaker 1>should be like a physics type. We have exhausted my

0:06:33.600 --> 0:06:35.960
<v Speaker 1>knowledge of Pokemon. Now I have nothing else to contribute

0:06:35.960 --> 0:06:39.279
<v Speaker 1>to this conversation. I went a little opie on you

0:06:40.080 --> 0:06:42.960
<v Speaker 1>all overpowered you. But it is an interesting name to

0:06:42.960 --> 0:06:45.040
<v Speaker 1>give a power to a fictional character. But it kind

0:06:45.040 --> 0:06:48.240
<v Speaker 1>of makes you think, is it actually possible for something

0:06:48.480 --> 0:06:50.880
<v Speaker 1>like that to happen? And we know that crazy things

0:06:50.880 --> 0:06:53.800
<v Speaker 1>happen out there in the universe. We are constantly surprised

0:06:53.800 --> 0:06:56.800
<v Speaker 1>by what's going on in the hearts of other galaxies

0:06:56.839 --> 0:06:59.719
<v Speaker 1>and even in between galaxies, and so you should never

0:07:00.040 --> 0:07:02.120
<v Speaker 1>say never, and so do they. On the podcast, we'll

0:07:02.160 --> 0:07:10.760
<v Speaker 1>be asking the question can a black hole be eclipsed?

0:07:11.120 --> 0:07:13.120
<v Speaker 1>And can you use it to suck up your enemies?

0:07:13.880 --> 0:07:17.680
<v Speaker 1>Is the question that a lot of kids are probably asking,

0:07:17.760 --> 0:07:20.360
<v Speaker 1>and maybe some physicists. Please, if you do have the

0:07:20.480 --> 0:07:23.600
<v Speaker 1>z power to manipulate dark energy to create black holes,

0:07:23.880 --> 0:07:25.960
<v Speaker 1>don't do it. You might win the battle and then

0:07:26.120 --> 0:07:28.800
<v Speaker 1>destroy the planet. Although they'll give you a Nobel prize, though,

0:07:28.800 --> 0:07:31.360
<v Speaker 1>wouldn't they in the five minutes between the creation of

0:07:31.400 --> 0:07:33.400
<v Speaker 1>your black hole and the destruction of the Earth. I'm

0:07:33.400 --> 0:07:36.560
<v Speaker 1>not sure the Swedish Academy acts that fast. I don't know.

0:07:36.640 --> 0:07:39.520
<v Speaker 1>I've seen you talk, Daniel, you will sacrifice anything for science.

0:07:39.680 --> 0:07:41.480
<v Speaker 1>If you have such a Z power, create a black

0:07:41.520 --> 0:07:44.000
<v Speaker 1>hole out in the depths of space where we can

0:07:44.040 --> 0:07:46.200
<v Speaker 1>study it. Please. I guess if you have that kind

0:07:46.200 --> 0:07:48.600
<v Speaker 1>of power, you can afford to go out into space. Right.

0:07:48.640 --> 0:07:50.640
<v Speaker 1>Maybe you also have the ex power and the why power?

0:07:50.840 --> 0:07:53.640
<v Speaker 1>Right right? Although I thought the why power was physicist

0:07:53.680 --> 0:07:56.240
<v Speaker 1>superpower or is that the philosophers? It's the four year

0:07:56.240 --> 0:08:01.280
<v Speaker 1>olds power? Why? Why? Why? Why? Yes, it's an interminable

0:08:01.320 --> 0:08:03.880
<v Speaker 1>source of energy. But it is an interesting question, and

0:08:03.920 --> 0:08:06.320
<v Speaker 1>as usual, we were wondering how many people out there

0:08:06.360 --> 0:08:09.040
<v Speaker 1>had thought about this question whether a black hole can

0:08:09.080 --> 0:08:12.280
<v Speaker 1>be eclipsed. So thanks very much to everybody who volunteers

0:08:12.320 --> 0:08:15.480
<v Speaker 1>to answer these questions in advance. Were very grateful to you,

0:08:15.520 --> 0:08:17.760
<v Speaker 1>and we hope that you enjoy hearing your voice on

0:08:17.800 --> 0:08:20.160
<v Speaker 1>the podcast. If any of you out there would like

0:08:20.200 --> 0:08:22.720
<v Speaker 1>to participate, please don't be shy. Right to me two

0:08:22.800 --> 0:08:25.680
<v Speaker 1>questions at Daniel and Jorne dot com. So think about

0:08:25.720 --> 0:08:28.120
<v Speaker 1>it for a second. Do you think a black hole

0:08:28.160 --> 0:08:31.280
<v Speaker 1>can be eclipsed? Here's what people had to say. Assuming

0:08:31.280 --> 0:08:37.560
<v Speaker 1>the definition of eclipse is for one body to obscure

0:08:37.600 --> 0:08:42.120
<v Speaker 1>another body from a given a vantage point. Um sure,

0:08:42.200 --> 0:08:44.280
<v Speaker 1>I don't see why a black hole could not be

0:08:44.320 --> 0:08:48.880
<v Speaker 1>eclipsed by another celestial body. I thought that might be

0:08:48.920 --> 0:08:51.720
<v Speaker 1>how we discovered them or something. I guess a black

0:08:51.760 --> 0:08:54.760
<v Speaker 1>hole can be eclipsed. I mean normally in eclipse is

0:08:54.800 --> 0:08:58.800
<v Speaker 1>when the light from something is blocked by something else

0:08:58.800 --> 0:09:01.800
<v Speaker 1>in space. So as a black hole doesn't have any

0:09:01.880 --> 0:09:04.000
<v Speaker 1>light emitting from it, I wouldn't have thought it could

0:09:04.040 --> 0:09:06.839
<v Speaker 1>be eclipsed as such. But I guess if you get

0:09:06.880 --> 0:09:09.439
<v Speaker 1>something massive enough in front of it, in between us

0:09:09.520 --> 0:09:12.840
<v Speaker 1>and it, then it would be eclipsed. I don't see

0:09:12.880 --> 0:09:17.800
<v Speaker 1>why not. As long as something subjectively larger than them

0:09:17.880 --> 0:09:22.439
<v Speaker 1>is between them and the observer, it would eclipse. The

0:09:22.480 --> 0:09:25.480
<v Speaker 1>black hole might have to be subjectively larger than the

0:09:25.600 --> 0:09:29.000
<v Speaker 1>disc around it to really have a shot at it. Well,

0:09:29.040 --> 0:09:31.520
<v Speaker 1>the concept of eclipse, the way I understand it, is

0:09:31.559 --> 0:09:37.720
<v Speaker 1>that light from a star as blocked from Earth's view

0:09:37.840 --> 0:09:43.480
<v Speaker 1>by an intervening body. Certain's black holes do not emit light.

0:09:44.200 --> 0:09:47.880
<v Speaker 1>I don't think they can be eclipsed. I don't think

0:09:47.960 --> 0:09:52.199
<v Speaker 1>so because I believe when black holes mass passes before

0:09:52.200 --> 0:09:55.280
<v Speaker 1>a gravity you see lensing effects. And I don't know

0:09:55.960 --> 0:09:58.679
<v Speaker 1>I've ever heard of one being eclipsed before. Yes, I

0:09:58.760 --> 0:10:00.679
<v Speaker 1>think they can do if they're is a planet or

0:10:00.760 --> 0:10:04.360
<v Speaker 1>star closer to us in the right alignment with the

0:10:06.120 --> 0:10:08.800
<v Speaker 1>black hole. Yes, I think they can be eclipsed. Yes,

0:10:08.880 --> 0:10:11.160
<v Speaker 1>I think it can in the sense that is coming

0:10:11.200 --> 0:10:14.280
<v Speaker 1>in front of something else. Um. But like instead of

0:10:14.320 --> 0:10:17.040
<v Speaker 1>blocking the light like the moon we block the Sun's light,

0:10:17.800 --> 0:10:20.120
<v Speaker 1>I think it would just absorb the light of whatever

0:10:20.400 --> 0:10:23.600
<v Speaker 1>is behind it. But um, it could also have this

0:10:24.240 --> 0:10:27.920
<v Speaker 1>gravitational lensing effect where the light of the objects that

0:10:27.920 --> 0:10:31.400
<v Speaker 1>aren't directly behind it kind of get curved um due

0:10:31.440 --> 0:10:34.240
<v Speaker 1>to the black hole, and we perceive it um in

0:10:34.280 --> 0:10:36.920
<v Speaker 1>that way. So that's kind of the black hole version

0:10:36.920 --> 0:10:40.880
<v Speaker 1>of an eclipse. Yes, they can be eclips Let's say

0:10:41.000 --> 0:10:43.240
<v Speaker 1>instead of our son, it will be a black hole

0:10:44.440 --> 0:10:49.280
<v Speaker 1>like we heard at a podcast Danielle and Horhan. We

0:10:49.360 --> 0:10:51.520
<v Speaker 1>would need to be at a safe distance from it,

0:10:51.920 --> 0:10:56.040
<v Speaker 1>and we can safely go around it. And if we

0:10:56.120 --> 0:10:59.800
<v Speaker 1>have the moon that would be between us and the

0:11:00.040 --> 0:11:03.040
<v Speaker 1>that hole. I don't see why not the more collectives

0:11:03.120 --> 0:11:07.080
<v Speaker 1>the site of the black hole. All right, A wide

0:11:07.160 --> 0:11:10.000
<v Speaker 1>range of answers here. Somebody said, why not always a

0:11:10.040 --> 0:11:12.600
<v Speaker 1>good answer? Am I talking about physics of the universe.

0:11:13.160 --> 0:11:17.760
<v Speaker 1>Why not, there's the multiverse, Doctor Strange says, anything can

0:11:17.800 --> 0:11:19.520
<v Speaker 1>happen in the multiverse. Or do you think they were

0:11:19.520 --> 0:11:21.760
<v Speaker 1>taking it as a proposal, like, hey, should we make

0:11:21.800 --> 0:11:24.880
<v Speaker 1>a black hole eclipse? Why not? Let's go right now.

0:11:25.200 --> 0:11:26.839
<v Speaker 1>I'm up for it. I guess it made me think,

0:11:27.040 --> 0:11:29.240
<v Speaker 1>what do you mean by eclipse, like in terms of

0:11:29.280 --> 0:11:34.000
<v Speaker 1>attention or in terms of blocking its light? But it's

0:11:34.000 --> 0:11:36.360
<v Speaker 1>a black hole. Yeah, it's a good question. And I

0:11:36.440 --> 0:11:39.680
<v Speaker 1>noticed that there was like two different interpretations of eclipse there,

0:11:39.800 --> 0:11:43.520
<v Speaker 1>one the black hole being eclipsed like something blocking light

0:11:43.600 --> 0:11:46.600
<v Speaker 1>from a black hole, and the other the black hole

0:11:46.720 --> 0:11:50.000
<v Speaker 1>doing the eclipsing, like passing in front of something else

0:11:50.080 --> 0:11:54.040
<v Speaker 1>that makes light. So there's sort of two possibilities there. Interesting,

0:11:54.200 --> 0:11:56.079
<v Speaker 1>and I guess we're going to argue about which one

0:11:56.160 --> 0:11:58.719
<v Speaker 1>is more correct. For the next hour, we're going to

0:11:58.800 --> 0:12:01.080
<v Speaker 1>talk about both possibility. At least. Of course, we're gonna

0:12:01.080 --> 0:12:03.640
<v Speaker 1>do the quantum superposition. We're gonna do the forwards and

0:12:03.720 --> 0:12:06.840
<v Speaker 1>the backwards. All right, Well, let's start with the basics here, Daniel,

0:12:06.880 --> 0:12:08.600
<v Speaker 1>What is a black hole? First of all, so we

0:12:08.640 --> 0:12:11.280
<v Speaker 1>don't really know what a black hole is in the

0:12:11.360 --> 0:12:15.120
<v Speaker 1>actual universe, and we don't actually even really know if

0:12:15.200 --> 0:12:19.160
<v Speaker 1>black holes exist. As described by the theory, we have

0:12:19.280 --> 0:12:23.040
<v Speaker 1>this concept in general relativity that if you get enough

0:12:23.120 --> 0:12:27.760
<v Speaker 1>stuff together, it's gravity will overcome any sort of internal strength,

0:12:28.080 --> 0:12:31.480
<v Speaker 1>any power of the material to resist being compressed. The

0:12:31.520 --> 0:12:33.880
<v Speaker 1>gravity will eventually get so strong that it will just

0:12:33.920 --> 0:12:36.559
<v Speaker 1>squeeze it down further and further and further, and as

0:12:36.559 --> 0:12:38.920
<v Speaker 1>it gets denser and denser, and the gravity gets stronger

0:12:38.960 --> 0:12:41.840
<v Speaker 1>and stronger, and you get this crazy runaway effect, and

0:12:42.040 --> 0:12:46.559
<v Speaker 1>where gravity essentially becomes infinitely strong in a tiny little dot,

0:12:46.760 --> 0:12:49.800
<v Speaker 1>this singularity at the point in space where you have

0:12:50.160 --> 0:12:54.360
<v Speaker 1>not infinite mass but infinite density, because gravity is compressed

0:12:54.440 --> 0:12:57.600
<v Speaker 1>some blob of stuff down to a very very small distance,

0:12:57.760 --> 0:13:00.320
<v Speaker 1>and because it's compressed it so far and means that

0:13:00.360 --> 0:13:02.160
<v Speaker 1>you can get pretty close to a lot of mass,

0:13:02.240 --> 0:13:05.280
<v Speaker 1>which means the gravity even nearby it would be very strong,

0:13:05.520 --> 0:13:08.440
<v Speaker 1>so strong that we think that it curves space so

0:13:08.520 --> 0:13:11.520
<v Speaker 1>much that light cannot even escape it. So if these

0:13:11.520 --> 0:13:14.000
<v Speaker 1>things are real, if they're out there in the universe,

0:13:14.040 --> 0:13:16.720
<v Speaker 1>then whatever falls into this black hole you will never

0:13:16.800 --> 0:13:20.280
<v Speaker 1>see again because light from it cannot escape. Would you

0:13:20.320 --> 0:13:23.440
<v Speaker 1>say it's an actual hole in space, Daniel. And you know,

0:13:23.480 --> 0:13:25.160
<v Speaker 1>if you define a hole is something that you can

0:13:25.240 --> 0:13:28.120
<v Speaker 1>fall into, then it's technically it is. That's why it's

0:13:28.120 --> 0:13:30.560
<v Speaker 1>called a whole. Right, if you accept the general relativity

0:13:30.600 --> 0:13:32.640
<v Speaker 1>view of it, it's kind of a hole because it

0:13:32.679 --> 0:13:35.720
<v Speaker 1>makes a portion of space that's cut off from the

0:13:35.760 --> 0:13:39.040
<v Speaker 1>rest of the universe. It's like a little sub universe,

0:13:39.080 --> 0:13:41.600
<v Speaker 1>and once you enter that sub universe, you really are

0:13:41.679 --> 0:13:43.800
<v Speaker 1>cut off from the rest of it. I mean inside

0:13:43.800 --> 0:13:46.040
<v Speaker 1>the black hole, you can still see the rest of

0:13:46.040 --> 0:13:48.120
<v Speaker 1>the universe. Light from the rest of the universe can

0:13:48.160 --> 0:13:50.280
<v Speaker 1>still reach you, so you can see out from it,

0:13:50.440 --> 0:13:53.760
<v Speaker 1>but nobody can see into it, right, So in that sense,

0:13:53.840 --> 0:13:56.800
<v Speaker 1>it's a hole in space, right, Although that's assuming your

0:13:56.800 --> 0:13:58.800
<v Speaker 1>eyeball is still in one piece when you're inside of

0:13:58.800 --> 0:14:01.920
<v Speaker 1>a black hole, right, Yeah, precisely, assuming that you survive

0:14:02.040 --> 0:14:04.520
<v Speaker 1>long enough to look out into the black hole. And

0:14:04.559 --> 0:14:06.920
<v Speaker 1>black holes can come in all sorts of sizes. You

0:14:06.960 --> 0:14:09.040
<v Speaker 1>can make a black hole in theory out of a

0:14:09.080 --> 0:14:11.800
<v Speaker 1>pretty small amount of mass as long as you squeeze

0:14:11.840 --> 0:14:14.680
<v Speaker 1>it down to a small enough radius. You can also

0:14:14.720 --> 0:14:17.720
<v Speaker 1>make black holes out of enormous masses. Some of the

0:14:17.760 --> 0:14:19.880
<v Speaker 1>things out there that we think are black holes probably

0:14:19.920 --> 0:14:23.800
<v Speaker 1>have millions or billion times the mass of our sun.

0:14:24.000 --> 0:14:26.440
<v Speaker 1>Those black holes are really really big, and if you

0:14:26.520 --> 0:14:30.040
<v Speaker 1>fall into one of those, the gravity at the outskirts

0:14:30.080 --> 0:14:33.000
<v Speaker 1>of the black hole is not actually that strong. I mean,

0:14:33.000 --> 0:14:35.200
<v Speaker 1>it's strong enough to suck up light, but it's not

0:14:35.280 --> 0:14:38.040
<v Speaker 1>so strong to like tear you apart to spaghettify you.

0:14:38.360 --> 0:14:41.000
<v Speaker 1>So you might be able to survive the very first

0:14:41.080 --> 0:14:44.360
<v Speaker 1>few moments of falling into a really really big black hole,

0:14:44.680 --> 0:14:47.000
<v Speaker 1>and then you can take it selfie, although you can

0:14:47.080 --> 0:14:49.720
<v Speaker 1>never send that selfie to anyone. Hey, selfies are just

0:14:49.800 --> 0:14:54.240
<v Speaker 1>for yourself, right, that's why they're called selfie. Ironically, that

0:14:54.360 --> 0:14:57.920
<v Speaker 1>is the opposite purpose of a selfie. They should be

0:14:57.920 --> 0:15:00.320
<v Speaker 1>called that everyone else's. But it is interesting what you

0:15:00.320 --> 0:15:02.760
<v Speaker 1>said about the black holes having a size, because it's

0:15:02.760 --> 0:15:04.440
<v Speaker 1>it's kind of into it's like a hole in space,

0:15:04.480 --> 0:15:07.280
<v Speaker 1>but it does have volume, right, Like, it does occupy

0:15:07.720 --> 0:15:11.120
<v Speaker 1>three dimensional space. In fact, it's a sphere in space, right,

0:15:11.360 --> 0:15:13.560
<v Speaker 1>I mean, it's just kind of distort space, but it

0:15:13.640 --> 0:15:16.760
<v Speaker 1>does sort of occupy a certain you know, length, width

0:15:16.800 --> 0:15:19.480
<v Speaker 1>and in height. Yeah, if you say black hole, you're

0:15:19.480 --> 0:15:22.080
<v Speaker 1>probably imagining like a circle on the ground a two

0:15:22.120 --> 0:15:25.200
<v Speaker 1>dimensional object that things can fall into and disappear, like

0:15:25.320 --> 0:15:27.960
<v Speaker 1>in cartoon shows. But as you say, they are three

0:15:27.960 --> 0:15:32.000
<v Speaker 1>dimensional objects. So the simplest black hole, one that isn't spinning,

0:15:32.000 --> 0:15:34.520
<v Speaker 1>would be a perfect sphere, and you can fall into

0:15:34.560 --> 0:15:37.440
<v Speaker 1>it from any direction. If you're looking at a perfect

0:15:37.480 --> 0:15:40.280
<v Speaker 1>sphere that's perfectly black, it's always just gonna look like

0:15:40.320 --> 0:15:42.760
<v Speaker 1>a circle to you because there's no texture to it,

0:15:42.840 --> 0:15:45.520
<v Speaker 1>so you can't sort of like tell how much curvature

0:15:45.560 --> 0:15:47.880
<v Speaker 1>it has. But actually, if you look at a black hole,

0:15:47.920 --> 0:15:50.960
<v Speaker 1>you don't even really just see a black sphere. It

0:15:51.000 --> 0:15:54.320
<v Speaker 1>looks even bigger than it actually is because the paths

0:15:54.360 --> 0:15:56.840
<v Speaker 1>of light around the black hole are really really weird.

0:15:56.920 --> 0:15:58.720
<v Speaker 1>Like if somebody was very close to the edge of

0:15:58.720 --> 0:16:00.720
<v Speaker 1>the black hole on the back side of it and

0:16:00.760 --> 0:16:03.080
<v Speaker 1>turned on a flashlight, you could see it from the

0:16:03.120 --> 0:16:05.360
<v Speaker 1>other side of the black hole because the light from

0:16:05.360 --> 0:16:08.400
<v Speaker 1>that flashlight would curve around the black hole, bent by

0:16:08.400 --> 0:16:11.880
<v Speaker 1>its incredible gravity to your eyeballs. So if you're near

0:16:11.920 --> 0:16:13.920
<v Speaker 1>a black hole, if you're just looking at it, you

0:16:13.960 --> 0:16:17.320
<v Speaker 1>can actually see the entire surface of the black hole

0:16:17.640 --> 0:16:19.240
<v Speaker 1>right in front of you. You can see the front

0:16:19.520 --> 0:16:22.640
<v Speaker 1>and the back right though it just looks black, right, Yeah,

0:16:22.640 --> 0:16:25.160
<v Speaker 1>it just looks like a bigger black circle than it

0:16:25.240 --> 0:16:27.840
<v Speaker 1>actually is. It's like puffed up, yeah, like puffed up

0:16:27.880 --> 0:16:30.760
<v Speaker 1>because in the vicinity of a black hole, space is curved,

0:16:30.760 --> 0:16:33.480
<v Speaker 1>and when space is curved, you can't trust your eyes

0:16:33.520 --> 0:16:36.080
<v Speaker 1>to be just showing you what he's there. You're seeing

0:16:36.200 --> 0:16:38.360
<v Speaker 1>now an image of what is there, and then image

0:16:38.360 --> 0:16:40.280
<v Speaker 1>can be distorted, just like if you're in a fun

0:16:40.320 --> 0:16:43.160
<v Speaker 1>house mirror and it's not flat and what you're seeing

0:16:43.320 --> 0:16:46.400
<v Speaker 1>isn't reality the same as true. Near a black hole,

0:16:46.720 --> 0:16:49.240
<v Speaker 1>light doesn't travel in straight lines anymore, and so what

0:16:49.360 --> 0:16:52.320
<v Speaker 1>you see is an image is generated by the physical

0:16:52.360 --> 0:16:54.960
<v Speaker 1>stuff that's there, but it's not a fully faithful image

0:16:55.120 --> 0:16:57.360
<v Speaker 1>of what's actually out there. It's a little bit mind

0:16:57.400 --> 0:16:59.720
<v Speaker 1>bending because a black hole is sort of like a sphere.

0:17:00.000 --> 0:17:02.080
<v Speaker 1>It sort of has the surface, but it's not really

0:17:02.080 --> 0:17:04.520
<v Speaker 1>a surface because it's not solid. It's just kind of

0:17:04.520 --> 0:17:06.080
<v Speaker 1>like the edge of the hole. So it's like a

0:17:06.119 --> 0:17:08.480
<v Speaker 1>three dimensional edge of a hole is the surface of

0:17:08.480 --> 0:17:10.640
<v Speaker 1>a black hole. Yeah, And what you call the edge

0:17:10.640 --> 0:17:13.159
<v Speaker 1>of a black hole is a little bit arbitrary. We

0:17:13.320 --> 0:17:16.920
<v Speaker 1>usually use the location of the event horizon, the point

0:17:16.920 --> 0:17:19.960
<v Speaker 1>past which light and particles and nothing can escape, and

0:17:20.160 --> 0:17:22.160
<v Speaker 1>to mark the edge of the black hole. But there's

0:17:22.200 --> 0:17:25.000
<v Speaker 1>nothing there at the edge. It's sort of like a

0:17:25.040 --> 0:17:28.199
<v Speaker 1>calculation we do to say where it is, and you

0:17:28.200 --> 0:17:31.879
<v Speaker 1>can't actually even tell where the event horizon is until

0:17:31.920 --> 0:17:34.359
<v Speaker 1>the end of the universe. The definition of the event

0:17:34.359 --> 0:17:38.639
<v Speaker 1>horizon is any particle past this point never escapes. But

0:17:38.680 --> 0:17:41.280
<v Speaker 1>it's not always easy to tell exactly what can escape

0:17:41.320 --> 0:17:44.359
<v Speaker 1>and what can't, and so you can't actually know in

0:17:44.440 --> 0:17:46.840
<v Speaker 1>any moment where the event horizon is. You have to

0:17:46.880 --> 0:17:48.720
<v Speaker 1>sort of like wait to the end of time and

0:17:48.720 --> 0:17:51.399
<v Speaker 1>then say, particles that got closer than this, none of

0:17:51.440 --> 0:17:54.640
<v Speaker 1>them escaped. So here was the event horizon, right, because

0:17:54.680 --> 0:17:57.359
<v Speaker 1>we actually like fall into the hole that sort of

0:17:57.440 --> 0:18:00.600
<v Speaker 1>almost sort of never happens, right, because time gets distorted

0:18:00.640 --> 0:18:02.800
<v Speaker 1>around the black hole that it basically as you said,

0:18:02.840 --> 0:18:06.080
<v Speaker 1>happens never. Yeah. And also there's just like nothing there

0:18:06.119 --> 0:18:08.080
<v Speaker 1>at the event horizon. It's not like a surface you

0:18:08.160 --> 0:18:10.400
<v Speaker 1>land on. It's just a point of no return. It's

0:18:10.400 --> 0:18:12.240
<v Speaker 1>like if you got into your car and you drove

0:18:12.280 --> 0:18:14.200
<v Speaker 1>too far away from a gas station so that you

0:18:14.240 --> 0:18:16.359
<v Speaker 1>didn't have enough gas to get to the next gas station.

0:18:16.480 --> 0:18:18.800
<v Speaker 1>Nothing would happen at that moment when you had gone

0:18:18.800 --> 0:18:21.120
<v Speaker 1>too far. You would only realize it later, like, oops,

0:18:21.440 --> 0:18:24.120
<v Speaker 1>we forgot to get gas and now we're stranded. The

0:18:24.160 --> 0:18:26.760
<v Speaker 1>moment when you crossed that threshold where you now too

0:18:26.800 --> 0:18:28.600
<v Speaker 1>far away from the nearest gas station you don't have

0:18:28.680 --> 0:18:31.720
<v Speaker 1>enough fuel to get one, no warning light necessarily goes off.

0:18:31.760 --> 0:18:33.439
<v Speaker 1>And the same is true for the event horizon. It

0:18:33.480 --> 0:18:36.520
<v Speaker 1>just feels like the rest of space. You pass through it,

0:18:36.600 --> 0:18:40.199
<v Speaker 1>and unbeknownst to you, you are now wrapped inside the

0:18:40.200 --> 0:18:43.359
<v Speaker 1>black hole. Right, Although you know, if you're flying that

0:18:43.400 --> 0:18:45.439
<v Speaker 1>close to a black hole, you can't claim not to

0:18:45.440 --> 0:18:47.480
<v Speaker 1>have seen it because it's going to look pretty big

0:18:47.520 --> 0:18:50.400
<v Speaker 1>to flying close to a black hole. Right. Oh yeah,

0:18:50.400 --> 0:18:53.080
<v Speaker 1>it's definitely irresponsible space flight in the same way like

0:18:53.240 --> 0:18:55.240
<v Speaker 1>you should know if you're about to run out of gas,

0:18:55.240 --> 0:18:57.000
<v Speaker 1>and somebody should be paying attention to it, or at

0:18:57.040 --> 0:18:59.720
<v Speaker 1>least there should be a warning alarm on your space ship.

0:19:00.760 --> 0:19:05.080
<v Speaker 1>Black hole ahead, turn right, use your Z powers now.

0:19:05.280 --> 0:19:07.560
<v Speaker 1>But as you said, it doesn't occupy space because it

0:19:07.640 --> 0:19:10.800
<v Speaker 1>is an object. It doesn't have less solid surface, and

0:19:10.840 --> 0:19:13.800
<v Speaker 1>it's also like moving around in space, right, black holes

0:19:13.840 --> 0:19:16.720
<v Speaker 1>can move around in space. Even though their holes in space,

0:19:17.000 --> 0:19:20.240
<v Speaker 1>they can move around in space. It's like a moving hole. Yeah,

0:19:20.320 --> 0:19:22.360
<v Speaker 1>well they are a thing, right, They are made out

0:19:22.400 --> 0:19:25.160
<v Speaker 1>of mass, and so like everything else, they have a location,

0:19:25.200 --> 0:19:27.159
<v Speaker 1>and then they can have a velocity. But you know,

0:19:27.200 --> 0:19:29.439
<v Speaker 1>the velocity of the black hole is relative, just like

0:19:29.520 --> 0:19:32.120
<v Speaker 1>everything else. If you are moving towards a black hole,

0:19:32.160 --> 0:19:34.840
<v Speaker 1>you could also say the black hole is moving towards you.

0:19:35.320 --> 0:19:37.960
<v Speaker 1>There is no difference in the physics of the universe

0:19:38.119 --> 0:19:41.280
<v Speaker 1>in those two pictures, and so black holes, like everything else,

0:19:41.320 --> 0:19:44.040
<v Speaker 1>can have location and velocity. Yeah, there could be one

0:19:44.080 --> 0:19:47.879
<v Speaker 1>moving towards us right now, right almost definitely, because we

0:19:47.920 --> 0:19:50.240
<v Speaker 1>know that there's a supermassive black hole at the heart

0:19:50.240 --> 0:19:52.840
<v Speaker 1>of the Andromeda Galaxy which is coming for us. Right

0:19:52.880 --> 0:19:55.320
<v Speaker 1>The Andromeda Galaxy is going to collide with the Milky

0:19:55.320 --> 0:19:57.359
<v Speaker 1>Way in a few billion years, and so the black

0:19:57.400 --> 0:20:00.639
<v Speaker 1>holes at the heart of each galaxy are moving towards

0:20:00.680 --> 0:20:03.920
<v Speaker 1>the other galaxy. So, yeah, black holes are headed our way.

0:20:04.040 --> 0:20:07.479
<v Speaker 1>Better get working on that Z force, Daniel. We're counting

0:20:07.480 --> 0:20:09.720
<v Speaker 1>on you. I only have the P force, the physics force.

0:20:09.800 --> 0:20:11.600
<v Speaker 1>Other people have to work on the Z force, or

0:20:11.600 --> 0:20:13.600
<v Speaker 1>it could be the W force. For whites and there

0:20:13.640 --> 0:20:16.320
<v Speaker 1>you go. I guess the the Andromeda black hole. That's

0:20:16.320 --> 0:20:18.399
<v Speaker 1>something we don't want to catch alther if you find

0:20:18.640 --> 0:20:21.000
<v Speaker 1>a good container for it. I guess, yeah, maybe you do.

0:20:21.119 --> 0:20:23.119
<v Speaker 1>All right, well, let's talk about whether or not a

0:20:23.200 --> 0:20:26.840
<v Speaker 1>black hole can be involved in an eclipse, whether it

0:20:26.880 --> 0:20:29.679
<v Speaker 1>can eclipse other things, or whether you can eclipse a

0:20:29.800 --> 0:20:45.679
<v Speaker 1>black hole. But first let's take a quick break. All right,

0:20:45.760 --> 0:20:49.520
<v Speaker 1>we're talking about the physics of Pokemon, right, that's the

0:20:49.560 --> 0:20:53.160
<v Speaker 1>title of the episode. That's right, Pokemon characters use physics

0:20:53.160 --> 0:20:54.800
<v Speaker 1>on each other. I feel like that would be a

0:20:54.800 --> 0:20:57.439
<v Speaker 1>pretty viral title to put on this episode. What do

0:20:57.480 --> 0:20:59.760
<v Speaker 1>you think, physics of Pokemon? It might be viral. It

0:20:59.760 --> 0:21:02.040
<v Speaker 1>would also be totally misleading, but I guess that's how

0:21:02.040 --> 0:21:04.440
<v Speaker 1>everything goes viral. But we could do a whole episode

0:21:04.440 --> 0:21:06.360
<v Speaker 1>on this, right, just pick a bunch of Pokemon cars

0:21:06.400 --> 0:21:08.920
<v Speaker 1>and we'll break down the physics of their superpowers. Yeah,

0:21:09.000 --> 0:21:11.280
<v Speaker 1>le's good like this. Yeah that's totally made up. Yeah

0:21:11.359 --> 0:21:14.760
<v Speaker 1>that doesn't where Yeah that's ridiculous, But could it happened?

0:21:15.320 --> 0:21:17.439
<v Speaker 1>Aren't there books about the physics of Star Trek and

0:21:17.480 --> 0:21:20.879
<v Speaker 1>Star Wars in a multiverse where Pokemon is real, But

0:21:20.920 --> 0:21:23.400
<v Speaker 1>we are talking about the powers of one specific Pokemon.

0:21:23.480 --> 0:21:25.920
<v Speaker 1>Which Pokemon has this power? Daniel did, did you look

0:21:26.000 --> 0:21:28.720
<v Speaker 1>up the name? Well, according to my research, it says

0:21:28.760 --> 0:21:33.280
<v Speaker 1>any non mega evolved non primal Pokemon can use black

0:21:33.280 --> 0:21:36.960
<v Speaker 1>hole eclipse if it knows a damaging dark type move

0:21:37.359 --> 0:21:41.119
<v Speaker 1>and holds darkinium z and if it's trainer where's a

0:21:41.200 --> 0:21:44.600
<v Speaker 1>z ring? So if that made sense to you, please

0:21:44.640 --> 0:21:48.440
<v Speaker 1>explain it to me. Well, that's a lot of preconditions there,

0:21:48.560 --> 0:21:51.800
<v Speaker 1>so any Pokemon that checks those boxes can use it. Yeah,

0:21:51.840 --> 0:21:55.200
<v Speaker 1>apparently any non mega evolved non primal Pokemon. I don't

0:21:55.200 --> 0:21:56.560
<v Speaker 1>know if there's a lot of them or just one.

0:21:58.119 --> 0:22:00.600
<v Speaker 1>We we should you should have interviewed an expert. But anyways,

0:22:00.600 --> 0:22:03.000
<v Speaker 1>we're asking the question of whether or not you can

0:22:03.040 --> 0:22:06.280
<v Speaker 1>actually eclipse a black hole or I guess involved a

0:22:06.320 --> 0:22:08.560
<v Speaker 1>black hole in an eclipse. And you said, Daniels, there's

0:22:08.560 --> 0:22:11.840
<v Speaker 1>two possibilities here. You can either eclipse a black hole

0:22:12.280 --> 0:22:15.439
<v Speaker 1>or have the black hole eclipse something else. And so

0:22:15.480 --> 0:22:18.000
<v Speaker 1>I guess, first of all, Daniel, what's the legal definition

0:22:18.040 --> 0:22:20.919
<v Speaker 1>of an eclipse? So an eclipse is a fun astronomical

0:22:20.960 --> 0:22:24.160
<v Speaker 1>situation where two things fall along the same line, your

0:22:24.320 --> 0:22:27.359
<v Speaker 1>line of sight. So you're looking out into the universe

0:22:27.640 --> 0:22:30.119
<v Speaker 1>and you can imagine a line between your eyeball and

0:22:30.280 --> 0:22:34.320
<v Speaker 1>some object. If something else passes along that line, then

0:22:34.359 --> 0:22:37.000
<v Speaker 1>it has eclipsed whatever you were looking at. So if

0:22:37.000 --> 0:22:40.119
<v Speaker 1>you're looking at the Sun not recommended, and the Moon

0:22:40.440 --> 0:22:43.719
<v Speaker 1>passes in front of it, then that's a solar eclipse. Right.

0:22:43.760 --> 0:22:47.399
<v Speaker 1>The moon is eclipsing the Sun because it's passing along

0:22:47.440 --> 0:22:51.360
<v Speaker 1>the line between your eyeball and the Sun. Interesting, so

0:22:51.400 --> 0:22:53.320
<v Speaker 1>if a technically, if I put my thumb in front

0:22:53.320 --> 0:22:55.760
<v Speaker 1>of me and block out the Sun, I'm creating a

0:22:55.800 --> 0:22:59.600
<v Speaker 1>solar eclipse. That's what you're saying. Yeah, I mean your

0:22:59.640 --> 0:23:02.400
<v Speaker 1>thumb is not an astronomical object. Have you seen my sun?

0:23:03.640 --> 0:23:06.200
<v Speaker 1>It's pretty stiller. It's been a while, So assuming you've

0:23:06.280 --> 0:23:09.200
<v Speaker 1>upgraded it with your Z powers, than maybe or his

0:23:09.440 --> 0:23:12.200
<v Speaker 1>them can perform in eclipse. One of my favorite things

0:23:12.200 --> 0:23:15.720
<v Speaker 1>though about solar eclipses is that they're possible. Right, Like,

0:23:15.800 --> 0:23:19.400
<v Speaker 1>the moon can block the Sun in the sky, which

0:23:19.400 --> 0:23:21.560
<v Speaker 1>requires not just that the Moon goes in front of

0:23:21.560 --> 0:23:24.080
<v Speaker 1>the Sun, but that the Moon is the same size

0:23:24.200 --> 0:23:26.680
<v Speaker 1>or bigger than the Sun in the sky. The amazing

0:23:26.720 --> 0:23:29.199
<v Speaker 1>thing is that the Moon and the Sun are just

0:23:29.359 --> 0:23:31.680
<v Speaker 1>about the same size in our sky, like they can

0:23:31.760 --> 0:23:36.720
<v Speaker 1>eclipse each other just about, which is a total cosmic coincidence.

0:23:37.000 --> 0:23:38.639
<v Speaker 1>The Moon could have been bigger, or it could have

0:23:38.680 --> 0:23:41.000
<v Speaker 1>been further, or it could have been closer. They don't

0:23:41.040 --> 0:23:43.320
<v Speaker 1>have to be the same apparent size in the sky,

0:23:43.600 --> 0:23:46.400
<v Speaker 1>and yet they are. Yeah, that's a pretty wild coincidence.

0:23:46.400 --> 0:23:48.400
<v Speaker 1>Although it is also a function of where we are

0:23:48.520 --> 0:23:51.040
<v Speaker 1>right now, right, because eventually the Moon is going to

0:23:51.119 --> 0:23:53.640
<v Speaker 1>move further away from Earth and so it will look

0:23:53.680 --> 0:23:56.520
<v Speaker 1>smaller than the Sun. Yeah, exactly, it gets smaller and

0:23:56.560 --> 0:23:59.920
<v Speaker 1>smaller every year, and before like it maybe increased or

0:24:00.119 --> 0:24:02.440
<v Speaker 1>times or millions of years ago, the moon looked bigger

0:24:02.480 --> 0:24:04.679
<v Speaker 1>than the Sun during a solar eclipse. Yeah, And the

0:24:04.720 --> 0:24:08.000
<v Speaker 1>Sun is also growing in size as it gets older, right,

0:24:08.320 --> 0:24:11.359
<v Speaker 1>and pushing out more of its layers further and further.

0:24:11.560 --> 0:24:13.399
<v Speaker 1>So the Sun is getting bigger and the Moon is

0:24:13.440 --> 0:24:17.000
<v Speaker 1>getting smaller. And it's a really valuable lesson about coincidences.

0:24:17.040 --> 0:24:19.240
<v Speaker 1>You know, sometimes we see coincidences out there in the

0:24:19.320 --> 0:24:21.760
<v Speaker 1>universe and we go, oh, there must be an explanation

0:24:21.840 --> 0:24:25.600
<v Speaker 1>for that, and can't be by chance, But sometimes it is, right.

0:24:25.600 --> 0:24:27.800
<v Speaker 1>We don't think there's a reason that the Moon and

0:24:27.840 --> 0:24:29.960
<v Speaker 1>the Sun happened to appear to be the same size

0:24:29.960 --> 0:24:33.640
<v Speaker 1>in our sky, but it seems like a huge coincidence.

0:24:34.000 --> 0:24:36.760
<v Speaker 1>But sometimes they just happen. Yeah, And I guess the

0:24:36.800 --> 0:24:40.080
<v Speaker 1>coincidence is that they're almost the same size and from

0:24:40.080 --> 0:24:41.800
<v Speaker 1>our point of view and the sky. But it's sort

0:24:41.840 --> 0:24:43.920
<v Speaker 1>of not a coincidence that it just happens to fly

0:24:44.080 --> 0:24:46.560
<v Speaker 1>in front of the Sun, right, because the Moon is,

0:24:46.720 --> 0:24:49.160
<v Speaker 1>you know, spinning around Earth all the time, and we're

0:24:49.200 --> 0:24:51.960
<v Speaker 1>spinning around the Sun all the time, and so technically

0:24:52.040 --> 0:24:55.840
<v Speaker 1>the Moon kind of sits everywhere at any point in

0:24:55.880 --> 0:24:58.439
<v Speaker 1>the sky at some point eventually, right, So it's not

0:24:58.480 --> 0:25:00.440
<v Speaker 1>a coincidence that it just happens to line front of

0:25:00.440 --> 0:25:02.399
<v Speaker 1>the Sun, that's right. And most of the things in

0:25:02.400 --> 0:25:04.760
<v Speaker 1>the Solar System are in the same plane, and so

0:25:04.800 --> 0:25:07.400
<v Speaker 1>it's possible for them to line up. If the Moon,

0:25:07.440 --> 0:25:10.159
<v Speaker 1>for example, was orbiting the Earth outside the plane of

0:25:10.240 --> 0:25:12.560
<v Speaker 1>the Earth's orbit, it would be much harder for it

0:25:12.600 --> 0:25:14.879
<v Speaker 1>to eclipse the Sun. But because it moves around in

0:25:14.920 --> 0:25:17.919
<v Speaker 1>the same plane than it gets itself between the Earth

0:25:18.040 --> 0:25:20.040
<v Speaker 1>and the Sun, and of course it doesn't eclipse the

0:25:20.240 --> 0:25:23.040
<v Speaker 1>entire Earth. The Moon casts a shadow on the Earth,

0:25:23.080 --> 0:25:25.920
<v Speaker 1>and that shadow moves across the surface of the Earth.

0:25:26.200 --> 0:25:29.240
<v Speaker 1>When you're in that shadow, then you can see the eclipse.

0:25:29.560 --> 0:25:31.119
<v Speaker 1>And at the same time, there are people who are

0:25:31.160 --> 0:25:33.080
<v Speaker 1>not in that shadow who can still see the Sun

0:25:33.160 --> 0:25:35.439
<v Speaker 1>sort of around the side of the moon because they

0:25:35.480 --> 0:25:37.400
<v Speaker 1>have a different angle. I saw the total eclips back

0:25:37.400 --> 0:25:40.640
<v Speaker 1>in two thousand eighteen. Was it? It was pretty awesome event. Yeah,

0:25:40.640 --> 0:25:42.600
<v Speaker 1>And there's another one coming up in a in a

0:25:42.680 --> 0:25:44.800
<v Speaker 1>year or two. Right. There are a bunch of eclipses

0:25:45.080 --> 0:25:47.080
<v Speaker 1>all around the world the next few years, and if

0:25:47.119 --> 0:25:49.959
<v Speaker 1>you have the opportunity to see them, I totally encourage you.

0:25:50.359 --> 0:25:53.800
<v Speaker 1>Even though it has no deep astronomical significance, is just

0:25:53.800 --> 0:25:56.000
<v Speaker 1>sort of like a cool event. It makes you feel

0:25:56.040 --> 0:25:58.639
<v Speaker 1>connected to people who have seen these things since prehistoric

0:25:58.720 --> 0:26:01.479
<v Speaker 1>times and looked up and wondered, like, WHOA, something is

0:26:01.520 --> 0:26:04.720
<v Speaker 1>different about the sky today. I wonder what that means. Yeah,

0:26:04.760 --> 0:26:06.680
<v Speaker 1>just like I feel connected to my thumb whenever I

0:26:06.720 --> 0:26:09.760
<v Speaker 1>put it in front of the sun. Are there times

0:26:09.760 --> 0:26:12.000
<v Speaker 1>you don't feel connected to your thumb. That's what we

0:26:12.000 --> 0:26:16.040
<v Speaker 1>should worry about. Sometimes I feel like the thumb is

0:26:17.960 --> 0:26:20.439
<v Speaker 1>like we're not connecting into a deep level. You know,

0:26:20.760 --> 0:26:22.159
<v Speaker 1>you and your thumb needs to go to therapy. It

0:26:22.200 --> 0:26:24.280
<v Speaker 1>sounds like work out these issues. Yeah, yeah, do you

0:26:24.280 --> 0:26:27.359
<v Speaker 1>know anyone Maybe there's a good podcast for that. Maybe

0:26:27.400 --> 0:26:30.360
<v Speaker 1>I can point you to one I could point off

0:26:30.359 --> 0:26:33.320
<v Speaker 1>with my index finger isn't talking to me either, so

0:26:33.680 --> 0:26:35.879
<v Speaker 1>there's always a surprise in the podcast. This is the

0:26:35.960 --> 0:26:38.600
<v Speaker 1>direction I never would have guessed. Yeah, but it's interesting.

0:26:39.080 --> 0:26:41.600
<v Speaker 1>So what do you call a solar eclipse? Is when

0:26:41.680 --> 0:26:44.520
<v Speaker 1>something blocks your view of it? Right, Like, you can

0:26:44.560 --> 0:26:48.120
<v Speaker 1>also have a moon eclipse, right, the lunar eclipse, Yeah,

0:26:48.160 --> 0:26:51.000
<v Speaker 1>that's right. That's when the Earth gets between the Sun

0:26:51.119 --> 0:26:54.200
<v Speaker 1>and the Moon, and so the Moon is then blocked

0:26:54.280 --> 0:26:56.800
<v Speaker 1>from the Sun by the Earth, and so you can

0:26:56.840 --> 0:26:59.119
<v Speaker 1>still see the Moon, but it's sort of like shaded.

0:26:59.200 --> 0:27:01.920
<v Speaker 1>It turns a funny color because it's no longer getting

0:27:01.920 --> 0:27:05.040
<v Speaker 1>as much direct sunlight because it's in the Earth's shadow.

0:27:05.160 --> 0:27:07.800
<v Speaker 1>So basically, eclipses are like when somebody gets into somebody

0:27:07.800 --> 0:27:10.880
<v Speaker 1>else's shadow, right, or I guess technically a lunar eclipse

0:27:11.000 --> 0:27:13.000
<v Speaker 1>is like an earth eclipse if you were standing on

0:27:13.040 --> 0:27:14.880
<v Speaker 1>the moon. Yeah, although if you were in the moon

0:27:14.880 --> 0:27:17.240
<v Speaker 1>you would probably call that is solar eclipse, right, because

0:27:17.240 --> 0:27:20.760
<v Speaker 1>the Sun would be getting eclipsed. Are you saying it's

0:27:20.760 --> 0:27:24.280
<v Speaker 1>all relative, Daniel, It's all relative and the names are

0:27:24.320 --> 0:27:28.200
<v Speaker 1>not consistent. That's exactly the lesson of the podcast, all right.

0:27:28.240 --> 0:27:30.040
<v Speaker 1>And so it's interesting that you can you can block

0:27:30.080 --> 0:27:32.760
<v Speaker 1>out the light from the Sun, but that applies also

0:27:32.800 --> 0:27:35.480
<v Speaker 1>to any star, right, Like, you can have eclipses out

0:27:35.480 --> 0:27:37.680
<v Speaker 1>there in space with any star, not just our sun.

0:27:37.800 --> 0:27:40.920
<v Speaker 1>That's right. Stars out there have their own planets, and

0:27:40.920 --> 0:27:44.080
<v Speaker 1>those planets have moons, and so on those planets there

0:27:44.119 --> 0:27:47.919
<v Speaker 1>are eclipses happening. Those planets. Moons are blocking that Sun's

0:27:48.000 --> 0:27:50.879
<v Speaker 1>light and creating shadows which crawl along the surface of

0:27:50.960 --> 0:27:54.520
<v Speaker 1>those planets around other stars, and maybe aliens are looking

0:27:54.560 --> 0:27:58.080
<v Speaker 1>up at those and being impressed by the astronomical display.

0:27:58.440 --> 0:28:01.639
<v Speaker 1>But we can actually see those eclipses as well, because

0:28:01.680 --> 0:28:05.640
<v Speaker 1>sometimes those planets pass in front of their star, blocking

0:28:05.720 --> 0:28:08.359
<v Speaker 1>a little bit of the light from that star. So

0:28:08.400 --> 0:28:11.680
<v Speaker 1>instead of making a line from your eyeball to our sun, now,

0:28:11.720 --> 0:28:14.960
<v Speaker 1>imagine a line from your eyeball to some star far

0:28:15.119 --> 0:28:18.240
<v Speaker 1>far away, millions or billions of miles away, and a

0:28:18.240 --> 0:28:21.520
<v Speaker 1>planet can pass along that line. Now, because you're so

0:28:21.600 --> 0:28:25.040
<v Speaker 1>far away. The planet can't hope to block the entire star,

0:28:25.560 --> 0:28:27.760
<v Speaker 1>but what it can do is dim it a tiny

0:28:28.000 --> 0:28:31.040
<v Speaker 1>little bit. And that's actually one way that we discover

0:28:31.200 --> 0:28:34.400
<v Speaker 1>planets around other stars. We see them making these sort

0:28:34.400 --> 0:28:38.800
<v Speaker 1>of many or partial eclipses of their star. Yeah, it's

0:28:38.840 --> 0:28:42.120
<v Speaker 1>one way we can detect a planet and other stars.

0:28:42.160 --> 0:28:44.040
<v Speaker 1>And in fact, you sort of look for its stars

0:28:44.080 --> 0:28:47.520
<v Speaker 1>that twinkle a little bit periodically, right with a constant beat,

0:28:47.640 --> 0:28:49.400
<v Speaker 1>and that kind of tells you, hey, maybe it has

0:28:49.400 --> 0:28:52.400
<v Speaker 1>a planet swinging around it. Yeah. You study the brightness

0:28:52.400 --> 0:28:54.520
<v Speaker 1>of the star and you notice a dimming and it

0:28:54.600 --> 0:28:57.400
<v Speaker 1>dims periodically. So it dims for like a few days,

0:28:57.400 --> 0:28:59.200
<v Speaker 1>and then it gets bright again for a fixed amount

0:28:59.200 --> 0:29:02.160
<v Speaker 1>of days, and then dims again, and it happens periodically,

0:29:02.360 --> 0:29:04.360
<v Speaker 1>and that's how you can tell that something is going

0:29:04.400 --> 0:29:07.080
<v Speaker 1>in front of it and blocking it, because otherwise stars

0:29:07.120 --> 0:29:10.480
<v Speaker 1>can just twinkle and dust clouds can interfere with your observation.

0:29:10.600 --> 0:29:12.880
<v Speaker 1>But if it's something regular, then you know that it's

0:29:12.880 --> 0:29:16.160
<v Speaker 1>probably something orbiting near the star that's moving around it.

0:29:16.240 --> 0:29:19.440
<v Speaker 1>And so it's a really powerful way to discover these

0:29:19.480 --> 0:29:22.960
<v Speaker 1>other planets and also to measure their size because the

0:29:23.000 --> 0:29:25.920
<v Speaker 1>more dimming you get the bigger the planet is, and

0:29:25.960 --> 0:29:29.440
<v Speaker 1>these are always tiny little eclipses. You need really sensitive

0:29:29.480 --> 0:29:32.480
<v Speaker 1>telescopes to even notice that these things are dimming. You

0:29:32.480 --> 0:29:34.600
<v Speaker 1>could never see this with a naked eye, right, And

0:29:34.640 --> 0:29:36.920
<v Speaker 1>so if you see a star out there dimming and

0:29:37.000 --> 0:29:39.960
<v Speaker 1>being eclipse regularly, it might be a planet in its orbit.

0:29:40.200 --> 0:29:42.360
<v Speaker 1>But it's kind of interesting also to think about that.

0:29:42.640 --> 0:29:45.080
<v Speaker 1>You know, there are probably eclips is happening all the

0:29:45.120 --> 0:29:47.160
<v Speaker 1>time with all the stars out there, right, Like maybe

0:29:47.160 --> 0:29:50.120
<v Speaker 1>even asteroid flies near us, or it gets in our

0:29:50.160 --> 0:29:53.480
<v Speaker 1>way between us and another star. Technically that's an eclipse too. Yeah,

0:29:53.520 --> 0:29:56.080
<v Speaker 1>that's probably true, And there are eclips is happening that

0:29:56.160 --> 0:29:59.560
<v Speaker 1>we can't see, right this technique of seeing these planets

0:29:59.560 --> 0:30:01.800
<v Speaker 1>and we're lo eyes on the planet lining up with

0:30:01.880 --> 0:30:04.320
<v Speaker 1>our line of sight to that star. There are plenty

0:30:04.360 --> 0:30:06.600
<v Speaker 1>of planets out there around stars that are just not

0:30:06.720 --> 0:30:09.280
<v Speaker 1>aligned with us. Like we talked about how in our

0:30:09.360 --> 0:30:11.480
<v Speaker 1>Solar system, the Moon and the Earth and the Sun

0:30:11.520 --> 0:30:13.920
<v Speaker 1>of mostly aligned in the disc of the Solar system.

0:30:13.960 --> 0:30:16.000
<v Speaker 1>But the disc of our Solar system is not the

0:30:16.080 --> 0:30:18.800
<v Speaker 1>same as the disc of other solar systems. Those are

0:30:18.800 --> 0:30:21.240
<v Speaker 1>mostly random. I mean every solar system has its own

0:30:21.280 --> 0:30:24.480
<v Speaker 1>disc and the planets mostly follow that disc, but the

0:30:24.600 --> 0:30:28.040
<v Speaker 1>arrangement of our disc relative to other Solar System discs

0:30:28.240 --> 0:30:31.040
<v Speaker 1>is kind of random, which means that most stars, when

0:30:31.080 --> 0:30:33.440
<v Speaker 1>their planets passes in front of them, don't cause an

0:30:33.440 --> 0:30:36.280
<v Speaker 1>eclipse that we can see. All right, Well, we're talking

0:30:36.280 --> 0:30:38.640
<v Speaker 1>about whether or not you can involve a black hole

0:30:38.800 --> 0:30:41.840
<v Speaker 1>in an eclipse, and so Daniel, can can you eclipse

0:30:41.880 --> 0:30:44.800
<v Speaker 1>a black hole? Or can a black hole eclipse something else? Yeah,

0:30:44.800 --> 0:30:47.320
<v Speaker 1>it's a really fun question. Let's first talk about whether

0:30:47.360 --> 0:30:49.800
<v Speaker 1>you can eclipse a black hole. And the very question

0:30:49.920 --> 0:30:53.280
<v Speaker 1>is like, well, could you see a black hole anyway? Right? Like, technically,

0:30:53.280 --> 0:30:55.200
<v Speaker 1>what does it mean to see a black hole? Like,

0:30:55.240 --> 0:30:57.360
<v Speaker 1>even if there was nothing between you and the black hole,

0:30:57.440 --> 0:31:00.040
<v Speaker 1>are you actually seeing a hole? Like the whole it

0:31:00.160 --> 0:31:02.920
<v Speaker 1>was the absence of something, right, Exactly. A shadow can't

0:31:03.080 --> 0:31:05.680
<v Speaker 1>cast a shadow, right in the case of an eclipse

0:31:05.680 --> 0:31:08.240
<v Speaker 1>on the Earth, the moon is casting a shadow on

0:31:08.360 --> 0:31:11.400
<v Speaker 1>the Earth. But a black hole doesn't give off anything

0:31:11.600 --> 0:31:15.440
<v Speaker 1>to create a shadow. And so technically a pure classical

0:31:15.720 --> 0:31:19.080
<v Speaker 1>general relativity black hole is completely black. You saw it

0:31:19.120 --> 0:31:21.200
<v Speaker 1>out in the middle of space, you would not see

0:31:21.200 --> 0:31:23.760
<v Speaker 1>it doesn't give off any light. The only way you

0:31:23.760 --> 0:31:25.600
<v Speaker 1>could see it is if it was in front of

0:31:25.640 --> 0:31:28.200
<v Speaker 1>something else that was bright. It was like passing in

0:31:28.240 --> 0:31:30.960
<v Speaker 1>front of a star and eclipsing it. So a classical

0:31:31.000 --> 0:31:34.600
<v Speaker 1>black hole doesn't give off any light. Something could technically

0:31:34.640 --> 0:31:37.720
<v Speaker 1>block your view of the black hole, right, Like if

0:31:37.720 --> 0:31:41.240
<v Speaker 1>a planet happened to fly between you and the black hole,

0:31:41.560 --> 0:31:44.080
<v Speaker 1>you wouldn't see the black hole anymore? Would you call

0:31:44.120 --> 0:31:46.960
<v Speaker 1>that an eclipse? That sounds like a legal decision? Mean

0:31:47.040 --> 0:31:49.600
<v Speaker 1>the black hole not giving off any light than is

0:31:49.600 --> 0:31:52.600
<v Speaker 1>it being eclipsed? Right, And let's say behind the black

0:31:52.600 --> 0:31:55.800
<v Speaker 1>hole isn't like a galaxy or something bright or a

0:31:55.840 --> 0:31:58.200
<v Speaker 1>cloud of a bright cloud of gas or something, so

0:31:58.280 --> 0:32:00.600
<v Speaker 1>you can actually without the planet blocking, you would see

0:32:00.600 --> 0:32:02.880
<v Speaker 1>the black hole. But now there's a planet between you

0:32:02.920 --> 0:32:05.960
<v Speaker 1>and the black hole, so you don't see the black hole.

0:32:06.160 --> 0:32:08.160
<v Speaker 1>And technically it would sort of look like an eclipse, right,

0:32:08.160 --> 0:32:10.440
<v Speaker 1>It would be like a black circle getting blocked by

0:32:10.480 --> 0:32:14.640
<v Speaker 1>something maybe brighter. Yeah, that's technically possible. But we do

0:32:14.720 --> 0:32:17.320
<v Speaker 1>think that black holes do give off a little bit

0:32:17.320 --> 0:32:20.440
<v Speaker 1>of radiation in some cases, and the black holes create

0:32:20.640 --> 0:32:23.400
<v Speaker 1>an environment that gives off a lot of radiation, a

0:32:23.480 --> 0:32:25.600
<v Speaker 1>lot of light. So if you move away from just

0:32:25.680 --> 0:32:30.520
<v Speaker 1>like the classical general relativity pure black sphere and talk

0:32:30.560 --> 0:32:32.760
<v Speaker 1>about like the quantum version of it, or if you

0:32:32.800 --> 0:32:35.040
<v Speaker 1>talk about the stuff around the black hole, in the

0:32:35.160 --> 0:32:38.800
<v Speaker 1>environment created by the black hole, then that could be eclipsed, right,

0:32:38.840 --> 0:32:41.440
<v Speaker 1>because what stuff falls into the black hole, it tends

0:32:41.480 --> 0:32:44.080
<v Speaker 1>to get sped up so fast that it actually burns up.

0:32:44.120 --> 0:32:46.400
<v Speaker 1>And then that's right right. So things when they come

0:32:46.480 --> 0:32:48.400
<v Speaker 1>near the black hole, they don't always fall right in.

0:32:48.480 --> 0:32:50.120
<v Speaker 1>I mean, if your head is straight for the black hole,

0:32:50.280 --> 0:32:52.280
<v Speaker 1>you're going into the black hole. But if you sort

0:32:52.280 --> 0:32:54.760
<v Speaker 1>of go near the black hole, then you get bent

0:32:54.920 --> 0:32:57.040
<v Speaker 1>towards it and you sort of spin around it for

0:32:57.080 --> 0:33:00.120
<v Speaker 1>a long time before falling in. And so that's all

0:33:00.160 --> 0:33:03.120
<v Speaker 1>the accretion disc. It's like stuff that's on deck to

0:33:03.240 --> 0:33:05.680
<v Speaker 1>be sucked into the black hole. And while you're in

0:33:05.680 --> 0:33:07.720
<v Speaker 1>the accretion disk, the black hole is still working you.

0:33:08.000 --> 0:33:10.240
<v Speaker 1>It's got these tidal forces. It's pulling on the part

0:33:10.320 --> 0:33:12.760
<v Speaker 1>that's closer to you harder than the part that's further

0:33:12.840 --> 0:33:16.000
<v Speaker 1>from you, because gravity is stronger for closer things, and

0:33:16.040 --> 0:33:18.520
<v Speaker 1>so big clouds of gas and dust that are about

0:33:18.600 --> 0:33:20.400
<v Speaker 1>to fall into the black hole have a lot of

0:33:20.440 --> 0:33:23.400
<v Speaker 1>internal friction because of the black holes tidal forces, so

0:33:23.440 --> 0:33:26.600
<v Speaker 1>they get heated up incredibly hot and admit a lot

0:33:26.680 --> 0:33:30.520
<v Speaker 1>of radiation, and some stuff almost falls into the black hole,

0:33:30.680 --> 0:33:33.680
<v Speaker 1>but the strong magnetic fields like guided around the black

0:33:33.720 --> 0:33:35.600
<v Speaker 1>hole and it gets spun out at the top of

0:33:35.640 --> 0:33:38.880
<v Speaker 1>the black hole, making these enormous jets of radiation. So

0:33:39.000 --> 0:33:42.640
<v Speaker 1>black holes, even though themselves past the event horizon are black,

0:33:43.040 --> 0:33:45.400
<v Speaker 1>the stuff around them could actually be very, very bright.

0:33:45.480 --> 0:33:48.120
<v Speaker 1>These things quasars are some of the brightest things in

0:33:48.160 --> 0:33:51.280
<v Speaker 1>the universe. Yeah, we've had episodes about that. Now. It's

0:33:51.360 --> 0:33:53.440
<v Speaker 1>kind of ironic, right that some of the brightest things

0:33:53.440 --> 0:33:56.600
<v Speaker 1>in the universe actually come from black holes. Yeah, because

0:33:56.640 --> 0:33:59.440
<v Speaker 1>they are the source of a lot of gravitational energy,

0:33:59.720 --> 0:34:02.200
<v Speaker 1>so they can speed stuff up, they can focus stuff,

0:34:02.200 --> 0:34:05.480
<v Speaker 1>they can shoot stuff in another direction, even though you know,

0:34:05.520 --> 0:34:07.800
<v Speaker 1>if they actually ate that stuff up, you would never

0:34:07.840 --> 0:34:09.960
<v Speaker 1>see it. But when they're not actually eating stuff, they're

0:34:10.000 --> 0:34:14.320
<v Speaker 1>also powering the acceleration of other stuff nearby, which creates

0:34:14.360 --> 0:34:18.239
<v Speaker 1>fantastical light shows. And those light shows can be eclipsed

0:34:18.680 --> 0:34:21.520
<v Speaker 1>right right, although, as you said earlier, not every black

0:34:21.560 --> 0:34:24.040
<v Speaker 1>hole has these light shows, right, Like, there's a whole

0:34:24.120 --> 0:34:25.960
<v Speaker 1>range of black holes. There are maybe black holes who

0:34:25.960 --> 0:34:28.680
<v Speaker 1>are sitting all by themselves somewhere with nothing around it

0:34:28.719 --> 0:34:30.520
<v Speaker 1>to feed it to make it bright. And there are

0:34:30.560 --> 0:34:33.440
<v Speaker 1>black holes with huge clouds of stuff that is constantly

0:34:33.440 --> 0:34:35.840
<v Speaker 1>falling into the black holes. Yeah, there's a broad diversity

0:34:35.840 --> 0:34:38.879
<v Speaker 1>of black holes. The ones with big accretion disks are

0:34:38.880 --> 0:34:41.040
<v Speaker 1>the ones that are easier for us to see because

0:34:41.080 --> 0:34:44.000
<v Speaker 1>you can see the accretion disk right. Otherwise, it's very

0:34:44.000 --> 0:34:46.480
<v Speaker 1>difficult to spot a black hole. You have to see

0:34:46.480 --> 0:34:48.440
<v Speaker 1>it passing in front of something else. You have to

0:34:48.440 --> 0:34:51.480
<v Speaker 1>see it eclipsing something in order to spot it. Mostly

0:34:51.520 --> 0:34:54.279
<v Speaker 1>the way that we've identified black holes is from their

0:34:54.280 --> 0:34:57.840
<v Speaker 1>accretion disk or from like the motion of stuff near them,

0:34:57.880 --> 0:35:00.400
<v Speaker 1>indicating that there must be something very very heavy but

0:35:00.480 --> 0:35:02.680
<v Speaker 1>not right there. Well, I think I see what you're saying. Like,

0:35:02.719 --> 0:35:05.560
<v Speaker 1>if you define an eclipse as when you're blocking the

0:35:05.719 --> 0:35:08.560
<v Speaker 1>light that's coming from something else, then you sort of

0:35:08.600 --> 0:35:11.799
<v Speaker 1>need the situation where the black hole is giving off

0:35:11.880 --> 0:35:15.160
<v Speaker 1>light from its incretion disk to have a black hole eclipse. Yeah,

0:35:15.239 --> 0:35:17.440
<v Speaker 1>Otherwise you're just having a shadow of a shadow. And

0:35:17.440 --> 0:35:19.600
<v Speaker 1>I don't even know what that is, but probably exists

0:35:19.600 --> 0:35:22.319
<v Speaker 1>in the Pokemon universe. A shadow of a shadow is

0:35:22.360 --> 0:35:25.360
<v Speaker 1>a it's a double shadow, it's a shadow squared. But

0:35:25.400 --> 0:35:28.480
<v Speaker 1>I guess you could thankically block the shadow of a shadow, right,

0:35:28.480 --> 0:35:31.880
<v Speaker 1>like you could blog looking at the shadow. Yeah, I suppose.

0:35:31.920 --> 0:35:33.400
<v Speaker 1>I mean, if you stand in a shadow, do you

0:35:33.440 --> 0:35:35.719
<v Speaker 1>still have your own shadow? I don't know. That's a

0:35:35.760 --> 0:35:39.319
<v Speaker 1>philosophical question. That's like the sound of one hand clapping. Well,

0:35:39.360 --> 0:35:41.080
<v Speaker 1>I guess you need like a third source of light

0:35:41.160 --> 0:35:43.239
<v Speaker 1>or something, right, right, Yeah, and then you can also

0:35:43.239 --> 0:35:46.080
<v Speaker 1>it's a complicated shadows, but you're saying there's a situation

0:35:46.080 --> 0:35:48.080
<v Speaker 1>in which a black hole could have an increation disk

0:35:48.160 --> 0:35:50.360
<v Speaker 1>around it, which would make it bright, in which case

0:35:50.640 --> 0:35:52.880
<v Speaker 1>something could float between you and it and block your

0:35:52.960 --> 0:35:55.200
<v Speaker 1>view of this light source exactly, And that would be

0:35:55.239 --> 0:35:58.520
<v Speaker 1>a really powerful way to see interesting things really really

0:35:58.560 --> 0:36:02.319
<v Speaker 1>far away. Because black holes are very very bright when

0:36:02.320 --> 0:36:04.800
<v Speaker 1>we see them. We can see them in very very distant,

0:36:04.880 --> 0:36:08.560
<v Speaker 1>very ancient galaxies. So the very powerful probe of what's

0:36:08.600 --> 0:36:10.759
<v Speaker 1>out there in the universe. There's sort of like these

0:36:10.800 --> 0:36:13.560
<v Speaker 1>pencil rays of light that shine out into the universe.

0:36:13.640 --> 0:36:15.719
<v Speaker 1>We can use them to measure like the density of

0:36:15.760 --> 0:36:18.800
<v Speaker 1>stuff along that ray. We once talked about the cosmic

0:36:18.880 --> 0:36:21.359
<v Speaker 1>web and how we use these pencil rays of light

0:36:21.400 --> 0:36:24.839
<v Speaker 1>from quasars to like illuminate the universe and tell like

0:36:25.120 --> 0:36:27.560
<v Speaker 1>where the dark matter is and where these filaments of

0:36:27.600 --> 0:36:31.600
<v Speaker 1>gas between the galaxies are super interesting. And when something

0:36:31.640 --> 0:36:34.759
<v Speaker 1>else happens to pass in front of that pencil ray

0:36:34.800 --> 0:36:36.600
<v Speaker 1>of light in a way that we can see it,

0:36:36.719 --> 0:36:38.839
<v Speaker 1>then we can use that to identify something. We can

0:36:38.920 --> 0:36:41.200
<v Speaker 1>use that to see something that otherwise would have been

0:36:41.239 --> 0:36:44.319
<v Speaker 1>invisible to us. So we can use these eclipses as

0:36:44.360 --> 0:36:47.319
<v Speaker 1>ways to find stuff really really far away. Wait wait

0:36:47.320 --> 0:36:49.520
<v Speaker 1>you mean, what what does this stuff do well? For example,

0:36:49.800 --> 0:36:53.040
<v Speaker 1>the technique we talked about for finding planets around other

0:36:53.120 --> 0:36:56.880
<v Speaker 1>stars that mostly only works in our galaxy because the

0:36:56.920 --> 0:36:58.920
<v Speaker 1>stars have to be close enough for us to like

0:36:59.080 --> 0:37:02.799
<v Speaker 1>resolve a single star and measure its brightness very effectively.

0:37:03.239 --> 0:37:06.400
<v Speaker 1>So it's very difficult to see exoplanets in other galaxies

0:37:06.440 --> 0:37:09.720
<v Speaker 1>because remember, our galaxies like a hundred thousand light years across.

0:37:09.800 --> 0:37:13.560
<v Speaker 1>Other galaxies are like millions of light years away, So

0:37:13.600 --> 0:37:16.320
<v Speaker 1>we can't really use that technique to find planets around

0:37:16.360 --> 0:37:20.239
<v Speaker 1>stars in other galaxies. But scientists have recently used this

0:37:20.320 --> 0:37:23.799
<v Speaker 1>to find planets passing in front of black holes in

0:37:23.920 --> 0:37:27.920
<v Speaker 1>other galaxies because black holes are such intense sources of

0:37:27.960 --> 0:37:31.560
<v Speaker 1>this kind of radiation whoa, because they act like a

0:37:31.640 --> 0:37:35.120
<v Speaker 1>beacon within that other galaxy. But is this a planet

0:37:35.160 --> 0:37:38.040
<v Speaker 1>that is part of the black hole system or is

0:37:38.080 --> 0:37:40.680
<v Speaker 1>this like a random planet floating around another star that

0:37:40.760 --> 0:37:44.880
<v Speaker 1>just happens to ones fly in front of the black hole.

0:37:45.120 --> 0:37:47.560
<v Speaker 1>We don't know, and in the case of a recent observation,

0:37:47.680 --> 0:37:50.360
<v Speaker 1>the theories that it might be a planet orbiting black

0:37:50.360 --> 0:37:54.279
<v Speaker 1>hole with a period of about seventy years, which means

0:37:54.280 --> 0:37:57.239
<v Speaker 1>that we wouldn't know for another seventy years because we'd

0:37:57.280 --> 0:37:59.400
<v Speaker 1>have to wait that long to see the next eclipse.

0:37:59.600 --> 0:38:02.319
<v Speaker 1>If it is in fact orbiting that black hole, it's

0:38:02.360 --> 0:38:05.439
<v Speaker 1>just like a random transit, some blob passing in front

0:38:05.440 --> 0:38:07.880
<v Speaker 1>of the black hole. Then it won't happen again. But

0:38:07.920 --> 0:38:10.400
<v Speaker 1>they actually did see this. They looked out with the

0:38:10.480 --> 0:38:14.080
<v Speaker 1>Chandra X ray telescope at a galaxy called the Whirlpool

0:38:14.160 --> 0:38:17.359
<v Speaker 1>galaxy and they saw this kind of eclipse, meaning that

0:38:17.400 --> 0:38:20.120
<v Speaker 1>we're looking at this galaxy that's far away, and we

0:38:20.239 --> 0:38:23.320
<v Speaker 1>think that the light coming from it is a black hole.

0:38:23.440 --> 0:38:25.680
<v Speaker 1>That's right. We can zoom in on one part of

0:38:25.680 --> 0:38:28.399
<v Speaker 1>that galaxy, and they think that there's a binary system there.

0:38:28.400 --> 0:38:31.120
<v Speaker 1>They have like a normal like star and around it

0:38:31.200 --> 0:38:34.160
<v Speaker 1>is orbiting a black hole, and the black holes probably

0:38:34.200 --> 0:38:37.479
<v Speaker 1>from some other star which collapsed and left a black hole.

0:38:37.920 --> 0:38:41.240
<v Speaker 1>So the origin is probably some binary star system. Two

0:38:41.239 --> 0:38:44.000
<v Speaker 1>stars orbiting each other, and that's a little bit surprisingly

0:38:44.040 --> 0:38:46.839
<v Speaker 1>not uncommon, because stars tend to form near each other.

0:38:46.920 --> 0:38:48.880
<v Speaker 1>One of them becomes a black hole. They have this

0:38:48.960 --> 0:38:51.920
<v Speaker 1>binary system where the black hole is now like sucking

0:38:52.000 --> 0:38:54.960
<v Speaker 1>material from the other star and it generates a very

0:38:55.040 --> 0:38:58.600
<v Speaker 1>bright accretion disk. And so from that black hole you

0:38:58.640 --> 0:39:01.800
<v Speaker 1>now have this invariant hence source of radiation, and the

0:39:01.880 --> 0:39:04.880
<v Speaker 1>telescope consume in on that and see the radiation from

0:39:04.920 --> 0:39:07.560
<v Speaker 1>the accretion disc of this black hole as it eats

0:39:07.600 --> 0:39:11.239
<v Speaker 1>its sibling. Wait, the black hole is orbiting the Sun.

0:39:11.400 --> 0:39:14.080
<v Speaker 1>I guess it. It's it's a smaller mass than the Sun. Well,

0:39:14.080 --> 0:39:17.120
<v Speaker 1>the sort of orbiting each other, right, the two both

0:39:17.200 --> 0:39:20.359
<v Speaker 1>came from stars, and the black hole doesn't have all

0:39:20.440 --> 0:39:23.200
<v Speaker 1>the mass of the original star came from Probably these

0:39:23.239 --> 0:39:27.120
<v Speaker 1>two stars started out similar mass, and so more accurately

0:39:27.160 --> 0:39:29.719
<v Speaker 1>you would say they orbit each other m And then

0:39:29.760 --> 0:39:32.279
<v Speaker 1>on top of that they think that maybe there's a

0:39:32.280 --> 0:39:35.360
<v Speaker 1>planet orbiting around the black hole that's orbiting around the

0:39:35.360 --> 0:39:39.200
<v Speaker 1>Sun exactly, because the black hole is actually quite small,

0:39:39.239 --> 0:39:42.239
<v Speaker 1>it's very compact, and so when this planet passes in

0:39:42.280 --> 0:39:44.960
<v Speaker 1>front of the black hole, it actually eclipses a good

0:39:45.000 --> 0:39:47.759
<v Speaker 1>fraction of it. We would think about a planet transitting

0:39:47.800 --> 0:39:49.680
<v Speaker 1>in front of a star in our galaxy, it's a

0:39:49.680 --> 0:39:52.840
<v Speaker 1>tiny little dip in front of that star. But here,

0:39:53.080 --> 0:39:56.040
<v Speaker 1>because the accretion disc in the black hole are very compact,

0:39:56.120 --> 0:39:59.880
<v Speaker 1>every compressed by gravity, this planet actually blocked most of

0:40:00.040 --> 0:40:03.120
<v Speaker 1>the light from the secretion disc as it passed forward.

0:40:03.480 --> 0:40:05.839
<v Speaker 1>So you can look at like the brightness of this

0:40:05.920 --> 0:40:08.719
<v Speaker 1>black hole over time, and they see this huge dip

0:40:08.880 --> 0:40:12.080
<v Speaker 1>as something apparently eclipsed it. It clips the black hole,

0:40:12.239 --> 0:40:15.160
<v Speaker 1>lips the black hole. Yeah, but they only saw this once,

0:40:15.520 --> 0:40:18.120
<v Speaker 1>or have they seen this periodically. They've only seen it

0:40:18.160 --> 0:40:20.560
<v Speaker 1>once and now have a model for this system and

0:40:20.600 --> 0:40:22.120
<v Speaker 1>how far aware this plant would have to be and

0:40:22.120 --> 0:40:24.200
<v Speaker 1>how big it is, and in that model it takes

0:40:24.200 --> 0:40:27.000
<v Speaker 1>about seventy years to orbit this system. But of course

0:40:27.000 --> 0:40:29.840
<v Speaker 1>they're not making the grad student wait seventy years to graduate,

0:40:29.880 --> 0:40:32.360
<v Speaker 1>although it could have also been like an asteroid passing

0:40:32.360 --> 0:40:34.399
<v Speaker 1>in front of the Chindra telescope or something that could

0:40:34.440 --> 0:40:36.920
<v Speaker 1>have caused this dip. Right, Yeah, there's a lot of possibilities.

0:40:36.960 --> 0:40:38.960
<v Speaker 1>We don't see this thing very directly. We only just

0:40:39.000 --> 0:40:41.680
<v Speaker 1>see a dip in this black hole, which we otherwise

0:40:41.719 --> 0:40:45.239
<v Speaker 1>can't explain, which means something probably passed in front of

0:40:45.239 --> 0:40:48.720
<v Speaker 1>it to block our view. And one hypothesis is a planet,

0:40:49.040 --> 0:40:51.560
<v Speaker 1>but we can't tell very precisely. Right, it could have

0:40:51.560 --> 0:40:55.279
<v Speaker 1>been somebody's thumb. Maybe did you put your thumb on

0:40:55.360 --> 0:40:59.080
<v Speaker 1>Chindre that day? Is that what happened? I don't know.

0:40:59.160 --> 0:41:01.600
<v Speaker 1>My son doesn't tell me everything it does. That's the

0:41:01.640 --> 0:41:04.800
<v Speaker 1>whole problem. But if it's true, then it's really interesting

0:41:04.840 --> 0:41:07.880
<v Speaker 1>because it's the first time we've discovered a planet in

0:41:07.960 --> 0:41:14.320
<v Speaker 1>a far away galaxy using this transit technique. Interesting. That's amazing,

0:41:14.440 --> 0:41:16.400
<v Speaker 1>and it would be amazing to be on that planet.

0:41:16.400 --> 0:41:18.640
<v Speaker 1>Can you imagine living on that planet and having like

0:41:18.760 --> 0:41:21.919
<v Speaker 1>not just a sun but a black hole also kind

0:41:21.960 --> 0:41:25.319
<v Speaker 1>of like sunrising and sunsetting every day and seeing the

0:41:25.320 --> 0:41:28.400
<v Speaker 1>black hole eat your sun. Right, That sun gets dimmer

0:41:28.440 --> 0:41:30.960
<v Speaker 1>and dimmer every year as the black hole pulls the

0:41:31.000 --> 0:41:33.720
<v Speaker 1>material out of it. Wow, that'd be a pretty amazing

0:41:33.840 --> 0:41:36.200
<v Speaker 1>view when you look up from that planet. I wonder

0:41:36.200 --> 0:41:39.600
<v Speaker 1>if that's where Pokemon out from, that's where they get

0:41:39.600 --> 0:41:44.440
<v Speaker 1>their Z power from the view. It's so amazing. Alright, Well,

0:41:44.480 --> 0:41:47.279
<v Speaker 1>we've seen a black hole get eclipse, and there are

0:41:47.280 --> 0:41:50.480
<v Speaker 1>other examples of that, and there's also the reverse situation

0:41:50.520 --> 0:41:53.719
<v Speaker 1>of whether or not a black hole can eclip something else.

0:41:53.760 --> 0:41:56.000
<v Speaker 1>So let's get into those. But first let's take another

0:41:56.120 --> 0:42:11.560
<v Speaker 1>quick break. All right, we're talking about black hole eclipses,

0:42:11.640 --> 0:42:14.040
<v Speaker 1>whether or not you can eclipse a black hole or

0:42:14.080 --> 0:42:16.640
<v Speaker 1>whether a black hole can eclip something else. And it

0:42:16.640 --> 0:42:18.879
<v Speaker 1>turns out that yes, you can eclipse a black hole.

0:42:18.920 --> 0:42:20.919
<v Speaker 1>We've seen it. We have data from a black hole

0:42:20.920 --> 0:42:23.520
<v Speaker 1>being eclipse out there in another galaxy. That's right. Even

0:42:23.520 --> 0:42:26.200
<v Speaker 1>though black holes are super powerful in the real world

0:42:26.239 --> 0:42:29.279
<v Speaker 1>and in Pokemon, you can just stand in front of

0:42:29.280 --> 0:42:31.640
<v Speaker 1>them and block their light. Yeah, it's pretty amazing. We

0:42:31.680 --> 0:42:33.960
<v Speaker 1>have data from that. And you said there's another example

0:42:34.000 --> 0:42:36.560
<v Speaker 1>of a black hole eclipse that we've seen. That's right.

0:42:36.560 --> 0:42:40.040
<v Speaker 1>There's a really cool galaxy about sixty million light years away.

0:42:40.120 --> 0:42:44.399
<v Speaker 1>It goes by the exciting name of n GC, and

0:42:44.560 --> 0:42:48.040
<v Speaker 1>it's exciting because it has a very active galactic nucleus.

0:42:48.480 --> 0:42:50.839
<v Speaker 1>This is what astronomers say when they mean that there's

0:42:50.880 --> 0:42:53.000
<v Speaker 1>a big black hole at the heart of it, and

0:42:53.040 --> 0:42:55.640
<v Speaker 1>it's very powerful and it's shooting a lot of stuff out.

0:42:55.719 --> 0:42:58.080
<v Speaker 1>So if you imagine a galaxy is like a big

0:42:58.160 --> 0:43:01.839
<v Speaker 1>flat disc of stuff, maybe with arms trailing behind it.

0:43:02.160 --> 0:43:05.560
<v Speaker 1>Now add to that huge jets of stuff shooting up

0:43:05.600 --> 0:43:08.360
<v Speaker 1>and down sort of from the middle of that disk.

0:43:08.480 --> 0:43:10.600
<v Speaker 1>So the galaxy is no longer just like flat. It

0:43:10.600 --> 0:43:13.200
<v Speaker 1>now has like an axle around which it's spinning. And

0:43:13.239 --> 0:43:16.399
<v Speaker 1>so we've seen this galaxy and and has something eclipses. Yeah,

0:43:16.400 --> 0:43:19.200
<v Speaker 1>astronomers were really curious about what was going on in

0:43:19.280 --> 0:43:21.000
<v Speaker 1>the heart of that galaxy, and they wanted to know

0:43:21.080 --> 0:43:22.960
<v Speaker 1>how big was the black hole and how big was

0:43:22.960 --> 0:43:25.400
<v Speaker 1>the active part of it, this sort of like really

0:43:25.440 --> 0:43:28.400
<v Speaker 1>intense part of the center of the galaxy. How big

0:43:28.520 --> 0:43:31.000
<v Speaker 1>is that accretion disk. Problem is that the galaxy is

0:43:31.040 --> 0:43:34.080
<v Speaker 1>so far away that it's really hard to measure that.

0:43:34.160 --> 0:43:37.120
<v Speaker 1>Like we've taken pictures of black holes and their acreation disks,

0:43:37.239 --> 0:43:39.600
<v Speaker 1>but it's very very difficult, and for this galaxy, it's

0:43:39.640 --> 0:43:41.640
<v Speaker 1>too far away for us to even use the event

0:43:41.680 --> 0:43:44.520
<v Speaker 1>horizon telescope. So they were trying to figure out how

0:43:44.560 --> 0:43:47.480
<v Speaker 1>big this thing was. And then they got lucky. They

0:43:47.480 --> 0:43:50.680
<v Speaker 1>got lucky because a big cloud of gas, when they

0:43:50.680 --> 0:43:53.600
<v Speaker 1>already knew and they had studied before, passed in front

0:43:53.640 --> 0:43:56.360
<v Speaker 1>of the black hole and eclipsed it. Because they knew

0:43:56.520 --> 0:43:59.400
<v Speaker 1>how big this cloud was and how fast it was going,

0:43:59.680 --> 0:44:02.640
<v Speaker 1>they were able to use that to measure the size

0:44:02.800 --> 0:44:06.600
<v Speaker 1>of the black hole accretion disc itself. Wait, what so

0:44:06.680 --> 0:44:09.000
<v Speaker 1>there was a black hole in another galaxy far waing

0:44:09.840 --> 0:44:13.160
<v Speaker 1>and a gas cloud within that galaxy pass in front

0:44:13.160 --> 0:44:15.920
<v Speaker 1>of it, or between us and that other galaxy. The

0:44:15.920 --> 0:44:18.600
<v Speaker 1>gas cloud is part of that other galaxy. You know, Oh,

0:44:18.680 --> 0:44:20.279
<v Speaker 1>I see? And how do we know how big that

0:44:20.320 --> 0:44:22.600
<v Speaker 1>gas cloud was? Because it's so far away. It's so

0:44:22.640 --> 0:44:24.480
<v Speaker 1>far away, but it's really big. And so they were

0:44:24.520 --> 0:44:26.680
<v Speaker 1>able to measure the size of this gas cloud. It's

0:44:26.800 --> 0:44:29.440
<v Speaker 1>much bigger than the black hole, but it's big enough

0:44:29.480 --> 0:44:32.239
<v Speaker 1>to see with the telescopes. It's big enough to see. You.

0:44:32.400 --> 0:44:34.680
<v Speaker 1>We can see other galaxies and we can see individual

0:44:34.760 --> 0:44:37.600
<v Speaker 1>components of it. We can't always resolve things as small

0:44:37.640 --> 0:44:41.000
<v Speaker 1>as stars, but big gas clouds we can resolve. And

0:44:41.080 --> 0:44:44.120
<v Speaker 1>so the cloud eclipse the black hole in the middle

0:44:44.239 --> 0:44:46.880
<v Speaker 1>or the quasar in in the middle, like it blocked

0:44:46.880 --> 0:44:48.720
<v Speaker 1>it completely or it just made it kind of fuzzy

0:44:48.760 --> 0:44:50.960
<v Speaker 1>for a while. It blocked it almost completely. I mean,

0:44:51.080 --> 0:44:53.880
<v Speaker 1>some light can get through it at some wavelengths. But

0:44:54.040 --> 0:44:57.320
<v Speaker 1>you can see definitely the dramatic dimming of this black

0:44:57.320 --> 0:45:00.840
<v Speaker 1>hole because this cloud passes in front of the accretion disk,

0:45:01.239 --> 0:45:03.240
<v Speaker 1>and so as it passes in front of one side

0:45:03.239 --> 0:45:05.319
<v Speaker 1>of the acreation disc, it starts to dim. And then

0:45:05.360 --> 0:45:07.840
<v Speaker 1>if it's totally blocking the disk, then you get the

0:45:07.880 --> 0:45:10.480
<v Speaker 1>minimum brightness. And then as it starts to reveal the

0:45:10.480 --> 0:45:13.200
<v Speaker 1>accretion disc again, the light comes back up. And so

0:45:13.680 --> 0:45:16.000
<v Speaker 1>from the size of the gas cloud and the speed

0:45:16.040 --> 0:45:18.240
<v Speaker 1>and with the gas cloud was moving, you can figure

0:45:18.239 --> 0:45:20.680
<v Speaker 1>out the size of the accretion disk, which is what

0:45:20.760 --> 0:45:24.160
<v Speaker 1>the astronomers are really curious to know. Interesting, So these

0:45:24.160 --> 0:45:27.799
<v Speaker 1>are recorded instances of black hole eclipses, Like you could

0:45:27.840 --> 0:45:31.839
<v Speaker 1>be the astronomer that saw a black hole eclip. Yeah, exactly.

0:45:32.120 --> 0:45:35.359
<v Speaker 1>And these are lucky coincidences, right, just like the Sun

0:45:35.400 --> 0:45:37.680
<v Speaker 1>and the moon lining up. In the case that these

0:45:37.719 --> 0:45:39.640
<v Speaker 1>things line up in the sky, we can use that

0:45:39.680 --> 0:45:42.799
<v Speaker 1>to learn something about these systems. We're always taking an

0:45:42.800 --> 0:45:45.799
<v Speaker 1>advantage of what's going on in the universe. Astronomers never

0:45:45.800 --> 0:45:48.400
<v Speaker 1>get to like build experiments and say what happens if

0:45:48.400 --> 0:45:50.800
<v Speaker 1>I crash these two things together, or if I pass

0:45:50.880 --> 0:45:52.719
<v Speaker 1>this in front of the other thing. They have to

0:45:52.760 --> 0:45:55.320
<v Speaker 1>just be clever in other ways of saying, well, I

0:45:55.360 --> 0:45:57.799
<v Speaker 1>didn't get to design this situation, but what can I

0:45:57.880 --> 0:46:01.120
<v Speaker 1>do to learn about the universe? Frum it anyway, And

0:46:01.120 --> 0:46:03.640
<v Speaker 1>so I love seeing astronomers be clever this way and

0:46:03.680 --> 0:46:06.160
<v Speaker 1>figure out, like how to use the lucky lining up

0:46:06.160 --> 0:46:08.719
<v Speaker 1>of these two objects to learn something about them. And

0:46:08.800 --> 0:46:10.960
<v Speaker 1>in this case, I used the gas cloud to learn

0:46:11.080 --> 0:46:12.880
<v Speaker 1>about the size of this black hole. What did they

0:46:12.920 --> 0:46:15.160
<v Speaker 1>learn about it? So they learned the size not just

0:46:15.200 --> 0:46:17.520
<v Speaker 1>to the black hole, but also the disc around it, right,

0:46:17.520 --> 0:46:19.880
<v Speaker 1>because it's the disc around it, the accretion disc that

0:46:19.960 --> 0:46:22.400
<v Speaker 1>really is generating that radiation. So they learned that this

0:46:22.400 --> 0:46:25.919
<v Speaker 1>disc is about seven a U wide, where a us

0:46:25.960 --> 0:46:28.040
<v Speaker 1>the distance from the Earth to the Sun. And so

0:46:28.080 --> 0:46:30.239
<v Speaker 1>if you put this thing in our solar system and

0:46:30.239 --> 0:46:34.040
<v Speaker 1>you extend out past the Earth's orbit and out past Mars,

0:46:34.600 --> 0:46:36.520
<v Speaker 1>so this thing is really pretty big. Wait, we can

0:46:36.600 --> 0:46:39.120
<v Speaker 1>measure the size of the cloud before, but we couldn't

0:46:39.120 --> 0:46:40.960
<v Speaker 1>measure the size of the black hole. Yeah, and the

0:46:40.960 --> 0:46:42.960
<v Speaker 1>cloud is bigger than the black hole, so we were

0:46:42.960 --> 0:46:45.360
<v Speaker 1>able to resolve it all right. Well, the final question

0:46:45.480 --> 0:46:48.839
<v Speaker 1>is whether a black hole could eclipse something else. Like

0:46:49.239 --> 0:46:51.400
<v Speaker 1>if there's a star or a sun out there and

0:46:51.440 --> 0:46:54.400
<v Speaker 1>a black hole pass in between it and us, would

0:46:54.400 --> 0:46:57.680
<v Speaker 1>it create an eclipse? That would be pretty dramatic, wouldn't it.

0:46:57.719 --> 0:47:00.920
<v Speaker 1>That would be pretty dramatic, But it's almost impossible. If

0:47:00.920 --> 0:47:03.240
<v Speaker 1>somebody standing on the other side of a black hole

0:47:03.320 --> 0:47:06.040
<v Speaker 1>and like turning on and off a flashlight, then a

0:47:06.080 --> 0:47:09.240
<v Speaker 1>lot of those photons would get to you anyway. Remember

0:47:09.280 --> 0:47:11.960
<v Speaker 1>that space around the black hole is really really curved,

0:47:12.000 --> 0:47:15.319
<v Speaker 1>so light doesn't always travel in straight lines. So light

0:47:15.400 --> 0:47:17.960
<v Speaker 1>that comes out from their flashlight that wouldn't otherwise get

0:47:17.960 --> 0:47:20.680
<v Speaker 1>to your eye gets bent by the black hole towards

0:47:20.719 --> 0:47:23.279
<v Speaker 1>your eye. So the black hole would eat some of

0:47:23.280 --> 0:47:26.560
<v Speaker 1>the photons from the flashlight, but other photons that were

0:47:26.560 --> 0:47:29.360
<v Speaker 1>going in other directions would get bent towards your eyeball,

0:47:29.600 --> 0:47:32.080
<v Speaker 1>so you would still see it. Right, Like if a

0:47:32.120 --> 0:47:34.680
<v Speaker 1>black hole just happened to fly into our solar system

0:47:34.719 --> 0:47:37.320
<v Speaker 1>and get between us and the Sun, it wouldn't totally

0:47:37.360 --> 0:47:41.000
<v Speaker 1>block the Sun. It would only block some of it. Yeah, Like,

0:47:41.040 --> 0:47:42.759
<v Speaker 1>if somebody stood on the other side of a black

0:47:42.760 --> 0:47:45.560
<v Speaker 1>hole with a laser of single photons, they could shoot

0:47:45.560 --> 0:47:47.440
<v Speaker 1>them at the black hole and you would eat them

0:47:47.480 --> 0:47:49.359
<v Speaker 1>and you wouldn't see it. But if their source has

0:47:49.400 --> 0:47:51.359
<v Speaker 1>any sort of width to it, if the photons come

0:47:51.400 --> 0:47:53.439
<v Speaker 1>out at any sort of angle, then some of those

0:47:53.480 --> 0:47:56.279
<v Speaker 1>are going to get bent around the black hole and

0:47:56.360 --> 0:47:59.360
<v Speaker 1>towards your eye. We see the same thing happening actually

0:47:59.360 --> 0:48:02.800
<v Speaker 1>already with the moon the Desiginstein's famous proof of general

0:48:02.800 --> 0:48:06.240
<v Speaker 1>relativity that space is curved by mass, because he showed

0:48:06.520 --> 0:48:09.000
<v Speaker 1>that photons from the Sun don't always get blocked by

0:48:09.040 --> 0:48:12.120
<v Speaker 1>the Moon. The Moon bends them around itself a tiny

0:48:12.239 --> 0:48:15.040
<v Speaker 1>little bit. The Moon is lensing the light from the

0:48:15.080 --> 0:48:17.040
<v Speaker 1>Sun a little bit, and a black hole would be

0:48:17.040 --> 0:48:21.160
<v Speaker 1>a very very powerful gravitational lens. So it's almost impossible

0:48:21.200 --> 0:48:24.160
<v Speaker 1>to hide behind a black hole, right, you're saying, like,

0:48:24.200 --> 0:48:26.480
<v Speaker 1>because the Moon is almost the same size as the

0:48:26.520 --> 0:48:29.759
<v Speaker 1>Sun and the sky, it doesn't totally block the Sun

0:48:29.800 --> 0:48:32.080
<v Speaker 1>because some of the light kind of flows around the

0:48:32.080 --> 0:48:34.399
<v Speaker 1>Moon and gets to us anyway. But if the Moon

0:48:34.520 --> 0:48:37.359
<v Speaker 1>was bigger, right, and the sky might like ten times

0:48:37.400 --> 0:48:41.360
<v Speaker 1>bigger than the Sun. It would almost totally blocked the Sun, right, Yeah, exactly.

0:48:41.600 --> 0:48:44.160
<v Speaker 1>Although the Moon was more massive than it would be

0:48:44.160 --> 0:48:46.960
<v Speaker 1>more effective at bending some of the Sun's light towards us.

0:48:47.120 --> 0:48:49.200
<v Speaker 1>And so there's two different effects going on there. And

0:48:49.239 --> 0:48:52.080
<v Speaker 1>so something is very small, like a black hole and

0:48:52.320 --> 0:48:55.080
<v Speaker 1>very very dense, it's going to be excellent at gathering

0:48:55.239 --> 0:48:57.840
<v Speaker 1>light that otherwise wouldn't have gone to you and sending

0:48:57.840 --> 0:49:00.200
<v Speaker 1>it your direction. So what would we see if a

0:49:00.200 --> 0:49:02.759
<v Speaker 1>black hole stood between us and our son. We would

0:49:02.760 --> 0:49:06.399
<v Speaker 1>see like a black circle with a bright ring around it, right,

0:49:06.440 --> 0:49:10.000
<v Speaker 1>and then that ring would sort of merge with the

0:49:10.040 --> 0:49:13.480
<v Speaker 1>Sun and kind of distort the light around it, and

0:49:13.480 --> 0:49:16.879
<v Speaker 1>then they would block the Sun, and then it would

0:49:16.920 --> 0:49:20.080
<v Speaker 1>keep going. Yeah exactly. It would look really weird and awesome.

0:49:20.160 --> 0:49:22.719
<v Speaker 1>It reminds me actually of a great science fiction book

0:49:22.719 --> 0:49:25.839
<v Speaker 1>I read, Paraheli In by Greg Egan. He talks about

0:49:25.840 --> 0:49:28.240
<v Speaker 1>what happens when a black hole enters our solar system,

0:49:28.360 --> 0:49:30.399
<v Speaker 1>and it's not something you should look forward to because

0:49:30.440 --> 0:49:33.640
<v Speaker 1>it would disrupt everything in the solar system even before

0:49:33.800 --> 0:49:36.480
<v Speaker 1>it made an impressive distortion of the Sun's light. Would

0:49:36.520 --> 0:49:38.719
<v Speaker 1>be bad news, but let's say it was a really

0:49:38.760 --> 0:49:41.520
<v Speaker 1>big black hole. It would totally eclipse our sun, right,

0:49:41.680 --> 0:49:43.440
<v Speaker 1>or we we still see all of the light from

0:49:43.440 --> 0:49:45.960
<v Speaker 1>the sun. We wouldn't, right, We would only see some

0:49:46.000 --> 0:49:47.960
<v Speaker 1>of the light from the sun get bent around the

0:49:48.000 --> 0:49:50.760
<v Speaker 1>black hole, but mostly it would be blocked. We wouldn't

0:49:50.800 --> 0:49:53.239
<v Speaker 1>see all of the light from the sun because photons

0:49:53.280 --> 0:49:56.000
<v Speaker 1>shot directly towards the center of the black hole would

0:49:56.040 --> 0:49:58.719
<v Speaker 1>still fall into the black hole, but photons shot in

0:49:58.840 --> 0:50:01.839
<v Speaker 1>other directions would get bent around it. To us, well,

0:50:01.880 --> 0:50:04.520
<v Speaker 1>there would be a range, right, wouldn't there be a range? Like,

0:50:04.560 --> 0:50:06.680
<v Speaker 1>It's not just the ones directly to the center of

0:50:06.719 --> 0:50:08.799
<v Speaker 1>the black hole and the ones a little bit off

0:50:08.840 --> 0:50:11.520
<v Speaker 1>to the side also get sucked into the black hole. Yeah,

0:50:11.520 --> 0:50:13.480
<v Speaker 1>the bigger the black hole, or the closer you are

0:50:13.560 --> 0:50:15.920
<v Speaker 1>to it, the sort of the wider range of photons

0:50:16.000 --> 0:50:18.360
<v Speaker 1>that do fall into the black hole. But also the

0:50:18.400 --> 0:50:20.880
<v Speaker 1>more powerful the black hole, the more it's able to

0:50:20.960 --> 0:50:24.279
<v Speaker 1>bend other photons around it so that you can see it.

0:50:24.440 --> 0:50:26.840
<v Speaker 1>And have we seen an example of this, I guess

0:50:27.600 --> 0:50:30.360
<v Speaker 1>we kind of have, right, I mean, we've taken pictures

0:50:30.360 --> 0:50:33.360
<v Speaker 1>of black holes, right, we have pictures of black holes,

0:50:33.400 --> 0:50:36.239
<v Speaker 1>and presumably there are stars behind the black hole that

0:50:36.280 --> 0:50:39.919
<v Speaker 1>we're not seeing because they're getting blocked by this black hole.

0:50:40.080 --> 0:50:42.240
<v Speaker 1>I don't know that we've seen that directly. We've discovered

0:50:42.239 --> 0:50:45.160
<v Speaker 1>smaller black holes because of their gravitational effects on the

0:50:45.200 --> 0:50:48.480
<v Speaker 1>nearby stars. Like if you see a star and it's

0:50:48.560 --> 0:50:50.319
<v Speaker 1>moving in such a way that you can tell it's

0:50:50.400 --> 0:50:53.200
<v Speaker 1>orbiting something, but you don't see the thing there, then

0:50:53.200 --> 0:50:56.000
<v Speaker 1>you deduce that there's probably a black hole there, even

0:50:56.040 --> 0:50:57.480
<v Speaker 1>if you don't see it. I don't know if we've

0:50:57.480 --> 0:51:00.560
<v Speaker 1>seen direct lensing of background stuff from a tellar mass

0:51:00.560 --> 0:51:02.440
<v Speaker 1>black hole. Well, I guess if we have a picture

0:51:02.440 --> 0:51:05.399
<v Speaker 1>of a black hole, technically it was blocking something behind it, right,

0:51:06.280 --> 0:51:09.439
<v Speaker 1>assuming there was something behind it, then yeah, it's getting blocked. Yeah, well,

0:51:09.440 --> 0:51:12.439
<v Speaker 1>technically there that has to be something behind it, doesn't there.

0:51:12.840 --> 0:51:14.839
<v Speaker 1>I mean, it's not like they're it's totally empty space

0:51:14.880 --> 0:51:17.600
<v Speaker 1>behind it, right, Yeah, there's always background galaxies no matter

0:51:17.600 --> 0:51:19.160
<v Speaker 1>how far you look. All right, Well, I think your

0:51:19.200 --> 0:51:22.360
<v Speaker 1>point is that it's complicated, right, because black holes bend

0:51:22.400 --> 0:51:25.680
<v Speaker 1>space so much that it and they act like lenses

0:51:25.719 --> 0:51:27.719
<v Speaker 1>out there in space that it's it's kind of a

0:51:27.760 --> 0:51:31.120
<v Speaker 1>complicated situation to have a black hole block something else. Yeah,

0:51:31.160 --> 0:51:34.160
<v Speaker 1>black holes are great at bending light and eating photons,

0:51:34.239 --> 0:51:36.960
<v Speaker 1>but they're also great at showing you what's behind them. Yeah,

0:51:36.960 --> 0:51:39.800
<v Speaker 1>but definitely, for sure, we've seen things block black holes

0:51:40.120 --> 0:51:42.399
<v Speaker 1>from our view. It's just that the situation is more

0:51:42.440 --> 0:51:46.320
<v Speaker 1>complicated for a black hole blocking our view of something else. Yeah, exactly.

0:51:46.440 --> 0:51:48.720
<v Speaker 1>All right, Well, I think the main lesson is Pokemon

0:51:48.880 --> 0:51:52.319
<v Speaker 1>is right. I think that's what you're seeing, right, that's right.

0:51:52.360 --> 0:51:54.359
<v Speaker 1>You don't need a physics degree. You just invest your

0:51:54.360 --> 0:51:57.640
<v Speaker 1>college savings in Pokemon. That's right. Just catch them all

0:51:57.680 --> 0:52:01.799
<v Speaker 1>and you can't retired to that tropical island or at

0:52:01.880 --> 0:52:03.879
<v Speaker 1>least pay for your son's college. It kind of caused

0:52:03.880 --> 0:52:06.920
<v Speaker 1>the same these days, does cause the same. Maybe you'll

0:52:06.920 --> 0:52:09.279
<v Speaker 1>get a PhD in Pokemon. I think there are pro

0:52:09.840 --> 0:52:13.600
<v Speaker 1>hard people getting their PhDs on the cultural impact of Pokemon.

0:52:13.640 --> 0:52:16.320
<v Speaker 1>I'm sure you can get a PhD on anything, exactly.

0:52:16.360 --> 0:52:18.960
<v Speaker 1>Everybody can get a PhD. Al right, Well, I guess

0:52:19.000 --> 0:52:21.200
<v Speaker 1>the next time you look out into the night sky

0:52:21.360 --> 0:52:23.960
<v Speaker 1>or even the daytime sky, imagine that there are black

0:52:24.000 --> 0:52:27.239
<v Speaker 1>holes out there being eclipse and also eclipsing our view

0:52:27.239 --> 0:52:29.719
<v Speaker 1>of the universe. Because the universe is full of all

0:52:29.760 --> 0:52:32.799
<v Speaker 1>these amazing objects and be impressed by how astronomers are

0:52:32.800 --> 0:52:36.120
<v Speaker 1>taking an advantage of coincidences and happenstands out there in

0:52:36.160 --> 0:52:39.560
<v Speaker 1>the universe to teach us lessons, to reveal the nature

0:52:39.600 --> 0:52:42.120
<v Speaker 1>of the mysteries of our cosmos. That's right. The main

0:52:42.200 --> 0:52:44.600
<v Speaker 1>lesson here is don't put your thumb down on physics.

0:52:45.040 --> 0:52:47.480
<v Speaker 1>Give it those thumbs up. Yeah, two thumbs up to astronomy.

0:52:47.719 --> 0:52:49.799
<v Speaker 1>All right. We hope you enjoyed that. Thanks for joining us,

0:52:50.480 --> 0:53:00.480
<v Speaker 1>See you next time. Thanks for listening, and remember that

0:53:00.600 --> 0:53:03.360
<v Speaker 1>Daniel and Jorge explained. The Universe is a production of

0:53:03.440 --> 0:53:06.800
<v Speaker 1>I Heart Radio. For more podcast from my Heart Radio,

0:53:06.960 --> 0:53:10.520
<v Speaker 1>visit the I Heart Radio app, Apple Podcasts, or wherever

0:53:10.640 --> 0:53:14.080
<v Speaker 1>you listen to your favorite shows. Ye