StarTalk Radio - Cosmic Queries: Telescopes

Episode Date: March 28, 2013

In this Cosmic Queries episode, Neil deGrasse Tyson answers fan questions about radio and microwave telescopes, from the Hubble to the VLA to the James Webb Space Telescope. Subscribe to SiriusXM Podc...asts+ on Apple Podcasts to listen to new episodes ad-free and a whole week early.

Transcript
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Starting point is 00:00:00 Welcome to StarTalk, your place in the universe where science and pop culture collide. StarTalk begins right now. I'm your host, Neil deGrasse Tyson, your personal astrophysicist. And this is StarTalk. Colin Jost. Colin, welcome to StarTalk Radio. It's great to be here, Neil. So you wrote for Saturday Night Live some years ago. Do you still? Yeah, I've been there seven years now.
Starting point is 00:00:39 So you're still there. Yeah, I'm still there. I'm one of the supervising writers there now. And it's been great. Yeah, it's been a good run. Excellent. Excellent. And I did a little bit of homework on you. So you were a comedian dude in college as well. Yeah, I worked for this magazine called The Harvard Lampoon.
Starting point is 00:00:54 This magazine called. This magazine called. Where, you know, Conan O'Brien and people started out. And so I did that basically way more than I did any of my classes, including my astronomy class. So you flunked out of school is what you're telling me here. All the great ones flunked out. I got through. I got through.
Starting point is 00:01:11 I didn't Matt Damon it and just leave early. Oh, gotcha, gotcha, gotcha. So we're in the cosmic queries part, and we just came off an entire hour on telescopes. hour on telescopes. And so we called from the internet all ways that our listeners reach us by telephone, by Facebook, by tweets. And so I haven't seen any of these questions, but you've been reviewing them and just- Fire away? Bring it on. I'm ready for you. This is great. So this first one's from Facebook. It's from a guy named Dominic Irizarry.
Starting point is 00:02:05 This is great. So this first one is from Facebook. It's from a guy named Dominic Irizarry. And he wants to know, aside from the Arecibo Observatory and the VLA in New Mexico, are there any other large-scale operation radio telescopes in use today? And if so, what are we looking for or the scientists using them looking for aside from SETI data, which I don't even know what SETI is. Yes, you do know what SETI is. Okay, so SETI, the Search for Extraterrestrial Intelligence. Oh, yes. Okay, gotcha. That's just the acronym. Of course I knew that. Yes, of course. You would just, of course. I was slow playing it. So just to get people on the same page, the Arecibo Telescope is a single-dish radio telescope embedded in a natural crater near... I've been there. I've seen it. It's pretty awesome. In the island of Puerto Rico
Starting point is 00:02:21 and it's an awesome... It's otherworldly, actually. Nothing in the area looks like it, and you think it just landed from space. That telescope had sort of a cameo appearance in the film Contact. That's where Jodie Foster and Matthew McConaughey established their love interest in each other. As each sentence gets uttered, they get an inch closer to each other and then cut to the next scene. They're undercovers together in bed.
Starting point is 00:02:50 So that's what happens when you're hanging out at telescope. Always. Always. And the VLA, the Very Large Array Telescope, that's a set of much smaller radio telescope dishes that are on tracks. radio telescope dishes that are on tracks. And so this array can be expanded to be 14 miles across, or it can be compressed. And depending on the size, depending on the extent of these dishes on those tracks will determine what your resolution is of what it is you're looking at.
Starting point is 00:03:19 And do those combine kind of Voltron style? They brilliantly combine in an awesome feat of hardware and software. The signals from all those dishes combine to make a single image of what you're looking at. And the farther apart they are, the more resolution you have for what it is you're looking at. You might say, well, why not always view things with a far apart configuration? The problem is it's not as sensitive when the dishes are far apart. When they're close together, you can hear, you can see dim radio signals. When they're far apart, you need a bright signal, but you can get very good detail about what's going on.
Starting point is 00:03:55 So those remain two of a few leading radio telescopes in the world. The one that's getting all the recent attention, however, is one called ALMA, the Atacama, which for the Atacama Desert, Large Array. Okay. Did I get all my, I got Large Millimeter Array. ALMA, A-L-M-A, Atacama Large Millimeter Array. So millimeter is a wavelength of light just short of what we typically call radio waves. Millimeter light is microwaves.
Starting point is 00:04:28 Gotcha. And so microwaves are, if you remember what a wavelength would look like, you draw a crest and a trough. So the distance between two consecutive crests, that's the wavelength. Right. Microwaves have anywhere between a millimeter and a centimeter, typically. And beyond a centimeter, you go up to meters and things, that's radio waves. That's how we've divided the kingdom there.
Starting point is 00:04:55 But in fact, it transitions smoothly from one to the other. But if you Google Alma, you'll find an extensive discussion of what it is we're targeting with this brand newly, freshly opened array. Where is that? Which desert? That's in Chile. That's the Atacama Desert. In fact, it's high altitude. And I think that the Atacama Desert has the record for the lowest rainfall of any place in the world, like an inch a decade or so. I'm not going to dispute it now. It's very low.
Starting point is 00:05:18 I don't know the exact number, but you don't want to live there. Gotcha. you don't want to live there. Gotcha. And that's important because water in the atmosphere interferes with microwaves we're trying to get from the universe. And so you want to go to the driest possible place you can. And the Atacama Desert is just such a place. By the way, the fact that water interferes with microwaves, we exploit on the other end
Starting point is 00:05:41 of this and make microwave ovens. Water is a major food additive, of course. So there you have something you want to eat. You want to heat it up. It has water in it. You put it in a microwave cavity. You beam powerful microwaves across it. That water absorbs the microwaves and it heats the food.
Starting point is 00:06:00 See, I never knew. I just thought it was, you know, just that spinning plate. It just moved so fast that it just started bursting into flames. I think three out of five people surveyed still say they use the word nuke it. Yeah, they think it's something nuclear. And it's so not nuclear. It's ordinary microwaves. And that's why the holes, if you look at the screen, by the way, microwaves pass through glass.
Starting point is 00:06:24 And all microwave ovens have a glass door. So what prevents them from coming out? Look on the other side of the glass door. You'll see a mesh, a screen mesh. So that prevents it? Check the size of those holes, all right? If they are larger than, you know, you don't want the hole to be larger than the size of the wavelength of the microwave. Otherwise, it will pass right on through.
Starting point is 00:06:46 So there's no way of getting – if it's – they can't sneak in somehow, huh? If they hit at the right moment. No, any more than visible light can sneak through the wall of a room. Right. It's just not transparent to microwaves. A mesh that you could otherwise see through using visible light with much smaller wavelength. Wow. Microwaves can't make it through.
Starting point is 00:07:08 That's great. Yeah. So we've got smart people figuring smart engineers. You're listening to StarTalk. Stay tuned for another segment. Welcome back to StarTalk. Here's more of this week's episode. Well, so we're in the cosmic queries part of our telescope show. And we left off talking about microwaves and how they don't come out of your microwave oven
Starting point is 00:07:45 because you ask, where in the universe might you find microwaves? And in fact, they're everywhere coming to us from the depths of space. But they also come from regions of the galaxy where stars are being born. So they help us map gas clouds, sort of the birth sack of
Starting point is 00:08:01 stellar nurseries. And so microwaves are – You mean are they almost like in the way there's a Big Bang? The Big Bang may start over again in different areas? Yeah. So the Big Bang births all the matter and energy in the universe. But now what do you show for me lately? Right.
Starting point is 00:08:15 So the matter and energy, we have gas clouds that condense and form galaxies and condense and form stars and planets and people. So in there, different bands of light, including microwaves, probe different parts of the universe. And for the longest while, we thought it was just visible light, you know, red, orange, yellow, green, blue, violet. And then we realized, oh, there's ultraviolet and X-rays and gamma rays and radio waves. The universe is trying to talk to us in more ways than our eyes can see, thus the birth of this whole suite of telescopes. And so you asked where you're going to get microwaves. So I was talking about ALMA, the Atacama Large Microwave Array. In everyday life, microwaves are what is used for your cell phone communication.
Starting point is 00:09:00 Most communications – Microwaves, I didn't know that. They're microwaves, exactly. And the walkie-talkies are all microwaves. If you had sensitivity to microwaves with your eyes, you can tune it, let's say. If you tune them to microwaves and look around, first you'd be able to see through walls because why else would your cell phone work inside of a room unless the microwaves can see through the walls. Or getting through. Can get through, exactly.
Starting point is 00:09:22 So is that where x-ray – you know, there's X-ray vision, but should we be working on microwave vision? Microwave vision is just as good as X-ray. In fact, it's better. It's better. We got to talk after this. We'll talk. Yeah, some prototypes going.
Starting point is 00:09:35 And so microwaves, if you tune into that and went by those cell phone towers, they'd be ablaze with light. They'd be the brightest things on the horizon. You wouldn't even see the streetlights. You'd be seeing the microwave towers. And you'd see people walking on the phone as they go down the street.
Starting point is 00:09:52 The whole – the phone would be aglow. Now, is there danger to that? Do we know? There are people who would claim there is, but there is no reliable evidence to say so. Are you concerned at all or not? No, not in the least. Oh, great. Yeah. Good. In fact, I sleep with all my cell phones, you concerned at all or not? No, not in the least. Oh, great. Yeah.
Starting point is 00:10:05 Good. Then I'm set. In fact, I sleep with all my cell phones, you know, all around me. I know. I end up doing it. Not by choice always. I've been on a couple of conversations with people who would have thought they were going to continue, but then I was asleep. What did that night cost on your credit card?
Starting point is 00:10:27 Yeah, or in my personal account life. So you got other questions that came in? Yes. Here's one from Facebook. It's from Tim Gearan Jr. And he says, if you were on a livable planet near Deneb, I don't know. Deneb is one of the stars that traced the constellation Cygnus the Swan. Oh, okay.
Starting point is 00:10:46 There you go. If you were on a livable planet near Deneb with a telescope looking toward Earth, would our sun be in a constellation? Can we, with our computer technology, visualize what the night sky would look like from that planet? Totally. Oh, my gosh. Yeah, we've got three-dimensional coordinates of all the stars in the neighborhood out to several thousand light years. And so, oh, yeah, you can transpose what the night sky would look like on any of the – by the way, it wouldn't have to be a livable planet. Right. It could be from any – yeah. Just from any point in space. Apparently, he wants to move.
Starting point is 00:11:22 Yeah, I guess. But he wants to know the view first. The view. Was he creating a real estate brochure? Exactly, yeah. He's not looking at ones that don't have photos. So the nighttime view. So I don't have off the top of my head what this part of the night sky would look like. Yeah.
Starting point is 00:11:36 But what matters is not what the constellation looks like because they never really look like what they're supposed to anyway. There's like three out of the 88 that sort of resemble what they're purported to be. To be, yeah, exactly. For example, do you know the constellation Apis? A-P-U-S. You ever hear of it? No, no, I don't know. It's a bird of paradise.
Starting point is 00:11:58 It's got four stars in it. It's like somebody is smoking something to call these five stars a bird of paradise. I'm not going there. So you know what we did when we rebuilt the Hayden Planetarium? I had a fit of, I don't know, a fit of irresponsibility. I thought to myself, you know what I want to do? I want to sneak into the Star Ball and update all the constellations to stuff that matters to us today. You know, put in this guy, the Prius, you know, the cell phone, the laptop.
Starting point is 00:12:31 It's like two dots are a Prius. Yeah. I mean, he's just, why not? Or just make them box, line. Actually, there are, there's a constellation called Triangulum, which is just a triangle. We got you already. They got real there. They got so real as to be boring, right?
Starting point is 00:12:47 So what's fun about the constellations of the ancients is that they're embedded within their mythologies and what mattered in their everyday lives. So it's a window to the past. And back then, very few people were literate. So it was a way – it was kind of the library books of the day. You'd go out with people. You'd say, oh, here's Perseus and he saved Andromeda. So it was a way – it was kind of the library books of the day. You'd go out with people. You'd say, oh, here's Perseus and he saved Andromeda. You know, all the stories.
Starting point is 00:13:11 It's quite a bit of storytelling. So I'm thinking today it's time to update the constellations. Yeah. I think of the ice cream cone. There are some that have V shapes and I like ice cream. And I have Conus Major, Conus Minor. You know, we could do that. Like a one scoop, two scoop.
Starting point is 00:13:25 Exactly. A two scoop constellation, yeah. So who knows what they'll look like but they'd be subject not so much to what they literally look like
Starting point is 00:13:33 but what the cultural imperative is for those who are. It's like, yeah, it's like cloud gazing where you're just, it's reflecting your own
Starting point is 00:13:39 personality as much as we see. It's very Rorschach. Yes. This next question I'm very curious about too is it comes from Facebook from Brandon Fitzpatrick and he asked, can amateur astronomers It's very Rorschach. Yeah, excellent question. And the big ones, no. The big ones are all for professional use. And even so, they're quite expensive. I mean, they're tens of thousands of dollars a night to run them. Even for universities to rent them? Yeah, yeah. Universities that own them, you're paying for the physical plant, the maintenance, there are engineers there at all times, there's the food services. You're living nocturnally on the mountaintop and there's an entire support store. Somebody built the road to get to the mountaintop. So it costs money. And so even if they could afford it, it's not available to them unless they applied competitively
Starting point is 00:14:37 for time. And there's something called the TAC, the Telescope Allocation Committee. Every telescope has it. And usually quarterly or semi-annually, you apply for time. I want to use that telescope with this filter and that detector to observe this object for that long for this reason. That's all in your proposal. And so all the proposals get put on a table and the telescope allocation committee reviews them, figures out how much total time is requested. Can it be wedged into the total time available? If not, they come at you and say, we're going to cut you in half.
Starting point is 00:15:12 We're not going to give you time at all. We like this one better than that one. We think this will be more fertile as a research path. And so this gets done in every time period. Some people get telescope time and others don't. And is it a little bit bidding too, like money or is it? No, no, no, no, no. It's all based on the scientific. It's always scientific.
Starting point is 00:15:30 So you can't be like, I want to check out this girl. You know, that would not work. That's less convincing. And as far as I know, no one has bought their way onto it. Because plus, if you buy because your research isn't good, we know it. We'll know you're not, you can't hide if you're not good. Right. Right?
Starting point is 00:15:48 And so this is the self-checking that goes on in science as an enterprise. Right? You can't – there's a limit to how long you can try to pull the wool over someone's eyes because you're incompetent. Because it's ultimately still science. Well, still, we will so reveal this fact. It cannot hide. So the Hubble, what we talk about is what is the award rate of your applied time. Depending on how competitive one cycle is versus another, as many as two-thirds of all proposals won't get awarded time.
Starting point is 00:16:23 Wow. And so then you try again and try to come up with a better idea. And that's how that goes. Now, there are other telescopes that are not on the frontier but still exist and still have time available to them. Most of the big observatories have some telescopes where they give access to amateur astronomers. And so what you do is call the main office of the various observatories.
Starting point is 00:16:45 You're listening to StarTalk Radio. Stay tuned. More up next. Welcome back. Here's more of StarTalk. So we are in the cosmic queries part of StarTalk Radio for the show on telescopes. And Colin, you're just pulling these off the internet, off of Twitter. I haven't seen any of these questions in advance.
Starting point is 00:17:19 What do you have for me? Yeah, we were just talking about the Hubble telescope. And Brandon Fitzpatrick continues. He had another question about the Hubble, which is, is it possible to build a telescope on Earth that's just as good as the Hubble? So in what ways do telescope operators account for atmospheric distortion? And he wants to know, is that going to be – when is that going to be retired? And are there going to be plans for replacing it? Yeah, first of all, that's an awesome question.
Starting point is 00:17:43 But there are several parts to that. Let me back up for a minute. It turns out data from the Hubble telescope, once it's obtained by the people who request it, they get to study it and analyze it in all the ways they had intended. Then the data gets posted and it essentially becomes public at that point. So while you can't apply, typically apply as an amateur to command the Hubble telescope, you can actually apply to mine the preexisting data. Maybe there's a question you could ask of those something called the International Virtual Observatory, where all the data from all the telescopes would be in one place. And you'd say, observe this part of the sky in these wavelength bands. And you'd go into the data and you'd send a worm through and would find all the images taken in all the various wavelength bands you cared about and would find them in the repositories of data that hadn't been looked at for years possibly. And it would bring it back to you and you would have the chance to discover something that no one even thought to ask.
Starting point is 00:18:55 And so it's called data mining. That's what it's called as a procedure. Now, in terms of Hubble, we have telescopes far more powerful than Hubble. Hubble is only 94 inches in diameter. Only, it's big. It's 94 inches in diameter. The Keck telescope, there's a pair of them in Hawaii. Those are 10 meters across.
Starting point is 00:19:15 What's that in inches? That would be 400 inches. 80 million. I'm bad at estimating. 400 inches versus 80 million. I'm bad at this. I'm bad at estimating. 400 inches versus 94 inches. So the Keck telescope can see much, much dimmer things in the universe. The bigger your telescope is, the dimmer you can observe. Right.
Starting point is 00:19:35 The advantage of Hubble being above the atmosphere is that the atmosphere renders the sharpness of images fuzzy. And so you go above this fuzz layer and then you see the universe as the universe intended to be viewed. Over the years, however, we've invoked special technology borrowed from the military that allows us to compensate for the fuzzing effects of the atmosphere. And it's called adaptive optics. Wow. It will deform the shape of the mirror in real time with what it reads is going on in the turbulent layers of the atmosphere and exactly compensates for it in a remarkable feat of engineering and software so that you can get very close to the sharpness of the images that Hubble would have gotten.
Starting point is 00:20:22 Like a contact lens or something. Yeah. That's constantly updating. Constantly updating. Constantly updating. It's an awesome bit of hardware that we now have called adaptive optics. And so now is that making telescopes like the ones in Hawaii getting to that level? It has greatly improved the usability of telescopes or given them a new lease on life. There are objects that were just too fuzzy to do any work with them.
Starting point is 00:20:46 Even though your telescope was big enough to detect them, you were detecting just something that was fuzzy. Now we can detect them and we have sufficient detail. So you know more about it. Exactly. Interesting. This next question is from DeRay Pringle, Mr. Pringle, who had a great one. Just the same guy from –
Starting point is 00:21:03 Same guy, but he's multi – he's got a lot of topics on his mind. DeRay Pringle, is he related? I don't know. Well, we'll see. He asks, do you think the James Webb telescope will end up getting cut due to budget shortfalls? Yeah, not if I have anything to do with it. I'm kicking some congressional butt. Let's hope then this is the real Pringle.
Starting point is 00:21:25 This is the Pringle family in there. He's willing to chip in. Can I use that joke? Chip in. Very good. Very good. Thank you. I'm professional.
Starting point is 00:21:34 Thank you. Keep your distance from my professional glow. So the question surely arose because the budget, there were cost overruns on the James Webb Telescope. I mean by a factor of four even. And there was great worry that Congress would just get fed up with this and cut the budget. And my response here is the James Webb Telescope, which is going to – it's going to – it's not going to just go in orbit around the Earth. It's going to go a million miles on the other side of the moon and we're going to park it there, far away from Earth, far away from any contamination. And it's going to observe galaxies being born in the early universe.
Starting point is 00:22:11 It's a telescope unlike any other and required extraordinary engineering innovations to make it happen. Let it not be the highway system you're building or anything else you've done a million times before. Why be surprised that if you encounter a cost overrun on something you have never even attempted that's going to advance human understanding of the universe? You're listening to StarTalk. Stay tuned for another segment. Welcome back to StarTalk. Here's more of this week's episode. So, you got questions. More on telescopes. Yes.
Starting point is 00:23:03 I had a question, too, because, you know, obviously Curiosity is now on Mars. Curiosity the rover, yes. That's the rover, yes. And I'm wondering what – is there any sort of opportunity there to establish – to build either a telescope or is there any sort of telescoping technology they're sending over with that? Does that aid us in any way? No, not really. From that vantage point. Yeah, no. I mean, Mars is a little farther out away from the sun.
Starting point is 00:23:26 Right. But it's not so much closer to the rest of the universe that that gives us any kind of telescopic advantage. It's so no. And plus, you might ask, would we use a telescope to see our way just on Mars? That's not necessary when you have a rover. You can just – the rover got lazy when, hey, I'm just pulling out the telescopes on this one. I think I'm just going to sit here.
Starting point is 00:23:50 You're just going to sit. No, get off your duff. I did travel all the way here from Earth. Give me a second. Give me a second. So, yeah, we just send it there, and it's got tools to actually dig into the rocks and analyze the chemical composition of them.
Starting point is 00:24:05 So that's something a telescope can't do. So, yeah, when you're there – Maybe just do it in person. Forget – yeah, just do it in person with your own damn rock. Yeah. And so, yeah, yeah. Why watch pornography when you can have a girlfriend, right? I mean that's basically –
Starting point is 00:24:19 Oh, that would be the corollary to that theorem. Yes. I'm trying to take it – put it in real layman's terms. Exactly. All right. So this next question is, it comes from Google Plus from Paul Stewart, and he's wondering, we keep producing larger and larger telescopes. Is there any limit on
Starting point is 00:24:36 how large they can be? No. In fact, we are taking it to we are, we that's what we're doing. So check out, hear what we're doing. So check out – Well said. Here's what we're about to do. We're about to say, okay, the bigger the telescope, the more light it can collect.
Starting point is 00:24:51 All right? It's like a bucket and you're trying to collect rain. The person with the bigger bucket collects more rain than the person with the little bucket because we're passive receivers of light that comes from the universe. We can't hurry the light along. We can't go grab it before it gets here. We sit here and wait for it to reach us. Big telescopes gather more light and see dimmer things. Not only that, the wider the telescope, the more precise, the sharper the resolution will
Starting point is 00:25:20 be for what it is it's observing. Why is that? Is it just because you're getting more information? You have a much – your angle of the – so the way it works is the wider your – the diameter of your detector. So by the way, it doesn't have to be one solid detector such as the VLA. You can be spread out. Then you have to be clever about how you combine them. So the wider is that field of view, the smaller is the angle that you can accurately observe on that object.
Starting point is 00:25:54 And the smaller that angle is, the better is your resolution. That's all. So, for example, if you're not wearing your glasses, but you should, and you take a look at a lawn, it'll just look like a green carpet. Put on your glasses, you see blades of grass. If you had even better resolution, you'd see insects crawling within it. And then you could see the cells. And then you could see. So you can imagine having much better vision than even perfect human vision.
Starting point is 00:26:20 And you'd see right on down to the threads in the fibers of the grass. So this is the challenge of big telescopes. You want a big telescope to accomplish this. The frontier of this is we're going to float telescopes in space and have a baseline that's wider than the diameter of the Earth. Well, chew on that. You're listening to StarTalk Radio. Stay tuned.
Starting point is 00:26:47 More up next. Welcome back. Here's more of StarTalk. So we were talking about telescopes and we were talking about the size of telescopes and how that affects it. Size matters. Size matters for telescopes. Yeah, it does matter. Bigger is better.
Starting point is 00:27:16 What about material-wise, like what it's created from? Oh, perfect. Here's the problem. There's a limit to how big you can make a telescope on Earth because it's subject to gravity, the 1G force of gravity. Structurally, that's why the largest radio telescope in the world is sitting in a crater that cradles it. The size of that telescope is so large you could not hold it up and steer it. In fact, it's an unsteerable telescope. You have to wait for stuff to drift into its field of view.
Starting point is 00:27:46 This is the Arecibo Radio Telescope in Puerto Rico. You have to wait for stuff to drift into its field of view just to observe it. Is it because the material is so heavy? No, it's that the, well, not that the material itself is heavy, but the size of the structure is so unwieldy, given the gravitational forces that operate, that you just, we have no knowledge of materials that could sustain it. So, what we learned is, forget Earth's surface.
Starting point is 00:28:10 Go into orbit where you have zero G. Right. And when you have zero G, the structural integrity of your materials is no longer relevant. Not at least with regard to the stress of weight. Because it still matters in terms of temperature fluctuations and things because it gets hot and cold as it goes in and out of earth's shadow but other than that you can make structures that are otherwise unstable in fact the hubble telescope if brought to earth would be unusable as a telescope because it is not structurally stable under its own weight
Starting point is 00:28:41 wow so and not only that uh in terms of the detectors and the material that focuses the light, for regular light, you'd use glass. It's very reflective. It's a familiar surface that you put a silver coating on and it reflects. Radio waves, you don't need glass. You can just use wire mesh. The size of the hole in your surface just has to be smaller than the wavelength of light that you're trying to reflect. Interesting.
Starting point is 00:29:07 So that's all. Now, was the Hubble built and finished in space? Was it structurally unsanitary? Oh, no, no, sorry. Or it was just unusable. It was unusable. Gotcha. But it wouldn't have, like, fallen apart.
Starting point is 00:29:17 That's a steerable telescope. I thought it was like a couch that you have to build in the room or something. Yeah. that you have to build in the room or something. Yeah. So when it was opened up and the solar panels were exposed, then you have a zero-g telescope. The space station itself is structurally unstable. I don't know.
Starting point is 00:29:35 That's the thing of the size of a football field with booms hanging out and solar panels and pieces screwed in together. There's no way that could sustain itself in any kind of force of gravity at all. That's a nice, yeah, that's a freeing thing. This question is from Facebook, from Watson McKeel. And the question is, could there ever be such a thing as a gravity telescope, a device that could measure not the effects of gravity but gravity itself, or dark matter or dark energy telescope?
Starting point is 00:30:05 And what would the universe look like through one of those devices? Okay. So it's an interesting question just to see the gravity field. Right now, we only know gravity by its influence on the movement of other objects, right? So in a sense, all the telescopes and the software and the detectors that have been brought to bear to discover exoplanets, in a way, those were gravity telescopes. We were observing the response of the host star to the tugging upon it of the planet in orbit around it. So we're observing the effects of gravity through the light emitted by the host star. Is this almost asking, is there a way to show the negative space?
Starting point is 00:30:50 Yeah, I don't know. We have no way. No, I don't know any way to show that. But we do have what are called, there's the Laser Interferometric Gravity Wave Observatory, abbreviated LIGO. gravity wave observatory, abbreviated LIGO. And that's a telescope that's to observe – that's a telescope to observe – that's a telescope to observe ripples in the fabric of space and time that come our way. And this is predicted by Einstein. Einstein said there should be something called gravity waves.
Starting point is 00:31:21 He's ahead of everything. Way. Maybe he came from the future into the past and showed up looking pretty cool. And then it was like, oh, yeah, I know. This is – Trivial. I guess, yeah, maybe the bears are going to win in 85. Maybe.
Starting point is 00:31:31 I don't know. Maybe. The bears. So what you have there is if two black holes collide, that's an awesome disturbance in the fabric of space-time. And that ripple moves through space and it comes across the telescope. The telescope can then measure it. The birth of the universe itself has a gravitational signature. These gravity wave telescopes would be brought to bear to observe them.
Starting point is 00:31:55 But otherwise, just to see gravity sitting there in empty space, I don't know of any way to do that. And what about observing dark energy or dark matter? Oh, well, again, we're observing the effects of dark energy and dark matter. And that's the effect of when you see the universe expanding. Exactly. Thanks for listening to StarTalk Radio. I hope you enjoyed this episode. Many thanks to our comedian, our guest, our experts, and I've been your host, Neil deGrasse Tyson.
Starting point is 00:32:23 Until next time, I bid you to keep looking up.

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