#434: Gravity, Energy, and Hidden Galaxies: Listener Queries Unpacked
Space Nuts: Exploring the CosmosJuly 14, 2024
434
00:24:0122.05 MB

#434: Gravity, Energy, and Hidden Galaxies: Listener Queries Unpacked

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Space Nuts Q&A: Gravity Without Mass, Energy and Gravity, and Early GalaxiesJoin Andrew Dunkley and Professor Fred Watson in this engaging Q&A episode of Space Nuts, where they tackle intriguing questions from our listeners about gravity, energy, and the movement of galaxies.
Episode Highlights:
  • Gravity Without Mass? Steve from New Zealand asks if gravity can exist without mass. Fred dives into the complexities of this question, exploring the relationship between energy and mass, and whether this could offer an alternative explanation for dark matter.
  • - Energy and Gravity: Gus from Issaquah, Washington, ponders whether energy creates gravity and if a gravitational field itself generates energy and mass. Fred discusses the potential implications and the concept of gravitational energy.
  • - Early Galaxies Moving Towards Us: Nick from Auckland, New Zealand, wonders if early galaxies could be moving towards us, currently out of reach. Fred explains the mechanics of galaxy movements and the Doppler effect, shedding light on whether such galaxies could be hidden from view.
  • Don't forget to send us your questions via our website... [spacenuts.io].
  • Support Space Nuts and join us on this interstellar journey by visiting our website support page. Your contributions help us continue our mission to explore the wonders of the universe.Clear skies and boundless exploration await on Space Nuts, where we make the cosmos your backyard.
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[00:00:00] Hi there, this is Space Nuts Q&A. My name is Andrew Dunkley. Great to have you company. Coming up on this episode, we'll answer questions from Steve, Gus and Nick. Steve and Gus are sort

[00:00:10] of focused on the same thing, gravity. Steve wants to know if it can exist without mass. And Gus is talking about gravity and energy and what's the relationship. And Nick is asking about galaxy movements and are any moving towards us that we can't see yet?

[00:00:29] Well, we don't know. We can't see them yet. But we'll see if we can tackle all of that on this episode of Space Nuts. 15 seconds, guidance is internal. 10, 9, ignition sequence start. Space Nuts. 5, 4, 3, 2, 1. 1, 2, 3, 4, 5, 5, 4, 3, 2, 1. Space Nuts. Astronauts report it feels good. Here he is again, Professor Fred Watson. Hello, Fred.

[00:00:56] Hello, Andrew. Hello. How are you doing now? I'm doing the same as I was before. How about you? Well, I'm still doing the same as I was before. Yes, that's right. And I hope to be doing the same again very soon. Yes, indeed. Yes.

[00:01:15] Shall we just sort of muck in and get these questions sorted out? I think it was like a couple of weeks ago, we had gravity questions coming in thick and fast. No, black hole questions. But today it's gravity questions. It is. And our first one comes from Steve.

[00:01:36] Hi guys. My name is Steve. I'm from New Zealand. I really enjoy your show. Recently, you've read an article implying that gravity could be possible without mass. And I'm wondering if that would be another alternative explanation to dark matter and to Monde.

[00:02:08] You haven't, it makes it very clear anyway. All right. Steve, thanks for the question. Gravity without mass. Well, I doubt that we can turn to the Catholic Church because they do have mass. But... Terrible. It's an interesting question though.

[00:02:30] It is. And so my reading on this, excuse me, is yes, that's correct. So actually, there's a nice thread about this on Reddit, if anybody looks at that website. I do. I love Reddit.

[00:02:50] Yeah. I do remember one of my sons was an absolute Reddit fiend at one time. He was very much a Reddit fan. Now, so that's how I was aware of it. But I haven't been a great user of Reddit.

[00:03:08] But the bottom line, excuse me, is, and this is the way it's phrased in this particular conversation. If you increase the temperature of an object, and they take a planet in this case, and in fact, I might just read it because this kind of is quite interesting.

[00:03:32] And take your Neptune, take your Neptunian planet, something the size of Neptune, raise the temperature by 300 degrees Kelvin instantly. Now, the mass of Neptune is about 10 to 26 kilograms. And if we roughly assume all its hydrogen corresponds to about 6 times 10 to 52 particles of hydrogen,

[00:03:55] it's the thermal energy is roughly given by an equation there equals nkT, which leads to an increase in thermal energy of da da da, and it's a large number of joules. Actually, it's a small number of joules. It's k times 6 times 10 to the minus 52 times 300 joules.

[00:04:20] But which if you then convert that, so what this is saying is you warm up a planet, you get an increase in the thermal energy of that planet, you can then use E equals mc squared to convert that thermal energy into mass.

[00:04:37] And in this case, it comes out to be something like 3 times 10 to 15 kilograms, which is a lot, but is not very much in comparison with a planet. But that does mean that adding energy to something will increase its gravitational mass.

[00:04:57] Now, Steve's sort of, you know, next step in the argument from that is whether that could be misleading us in the idea of dark matter and things of that sort. And I can't really get my head around how that would work.

[00:05:18] He mentioned MAM as well, Modified Newtonian Dynamics. Because my understanding is that everybody who looks at these particular problems, what is dark matter? What is dark energy? They take into account everything. I've read some of the papers on this.

[00:05:37] And so things like, you know, gravitational influence of pure energy, and in this case, we're talking about heat energy, that is likely to be something that would be already in the equations. So I don't think it's the answer, but it's a really interesting

[00:05:58] suggestion and an interesting thing to think about. So thank you very much, Steve. Yeah, indeed. Just made me wonder, are we increasing Earth's gravity because we're heating the planet up? Yep, that's probably right.

[00:06:15] I mean, the example that I just read out was about 300 degrees Kelvin, an instant increase in that. We're talking about one or two degrees Kelvin, but which makes a big difference to the Earth's atmosphere, but probably not that much difference to its gravitational potential.

[00:06:36] Okay, so the answer is yes, gravity can exist without mass, but it's probably not a major factor. Is that fair enough? Yes, that is right. I've just been dragging through my memory, Andrew, something else that's sort of vaguely related to this.

[00:06:57] Which is the, we haven't used this name, but we did talk about it a while ago, the Kugelblitz. Do you know what a Kugelblitz is? Look, I've heard this before. No, remind me. Yeah, so it basically is a black hole made of light.

[00:07:18] It's, and Wikipedia says, it's a concentration of heat, light or radiation so intense that its energy forms an event horizon and becomes self-trapped. In other words, if enough radiation is aimed into a region of space,

[00:07:30] the concentration of energy can warp space-time so much that it creates a black hole. It's a black hole, it has a black hole whose original mass energy was in the form of radiant energy rather than matter.

[00:07:44] Now, there is a paper that was published in 2024 that concludes that a phenomenon like this cannot occur in any realistic scenario within our universe. So Kugelblitzes are a theoretical entity that are thought not to occur in nature. But it is a similar thing, isn't it?

[00:08:08] So it basically, it's a black hole made of energy. Yeah, wow. That's really interesting. I'll tell you something else that does exist is a Kugelschreiber. So I've got one of those. Have you? Yeah, there it is. It's a pen. German for pen. Hold it up. Ah, okay. Kugelschreiber.

[00:08:29] A Kugelschreiber. Yes. Do you know what the German is for pencil? I probably did once but I don't know. No, that's not the... Bleistift. Bleistift. All right, there you go. It's probably...

[00:08:45] I did languages at high school and I was very good at them and I should have probably pursued that somewhere along the line but German stuck with me. Some of the references I still remember today. Someone's going to correct me now because I've probably buggered up the pronunciation.

[00:09:01] Anyway. That's all right. I'm just showing off now. No, it's a side of your character that I was unaware of, Andrew. I am curiously, I never joined Lerman at school. I never learned German at school.

[00:09:19] But when I was 14, I went on a school exchange to Germany, which was barbless because I wasn't studying German. But that was my first overseas visit, of course, from the United Kingdom. And so I've spent however many years it is, 60 odd years since then trying to learn German.

[00:09:43] And yeah. Yeah. I'm so jealous of students in countries like the United States and the UK and Europe because they get to do excursions to other countries. In Australia, we got to do excursions to Sydney and Canberra. I mean, come on. That was it. Yeah.

[00:10:04] That was as good as it got for us. Yeah. These days, they get to go to New Zealand once in a while. But yeah, we're so far from everywhere. It's just not easy. Although my son did get to do a couple of weeks in Japan through high school.

[00:10:18] There you go. There are a few options these days. This is Space Nuts. Andrew Dunkley here with Professor Fred Watson. Let's take a little break from the show to tell you about our sponsor, Incogni.

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[00:13:40] But peace of mind is probably, yeah, something that we all need in this world of data thieves. So check it out today. incogni.com slash SpaceNuts. Now back to the show. Two, one. SpaceNuts. We better keep moving. Thank you, Steve. Let's get a question from Gus.

[00:14:06] Hello, Professor Fred and Andrew. This is Gus Iverson from Issaquah, Washington. I sent in a question for you guys previously. You thought I was in Western Australia. Yes. I've been thinking about gravity today and it came to my mind that if energy and mass

[00:14:29] are equivalent, then essentially shouldn't energy also create gravity at some level? I'm not sure if this is a related question or an extension or a separate question though. Additionally, if a body of any size is generating or has mass and it is generating a gravitational

[00:14:59] field, does not that field itself have energy and mass? And would that field not create additional gravity by its simple existence? So if that's the case, or even kind of the case, my question is, where does the energy

[00:15:24] and mass go if, or I have no idea where to go with this. Thank you. I love the show and appreciate being able to ask questions. Thank you, Gus. That sounded very much like something from Catch-22. Was it apples or tomatoes? I don't know.

[00:15:47] But yeah, it sounded a bit like that. Gravity plus energy, body plus mass plus gravity equals energy. But then does that add mass, which adds to gravity? I think that's what he was trying to say. Yeah, that's right.

[00:16:04] The whole thing gets completely out of hand because everything's got gravity. So the first part of what Gus was saying is what we've just been talking about. If you have energy and mass. And gravitation, you probably have to be careful with the words. Gravitation is a potential.

[00:16:30] An object in a gravitational field has potential energy. So it does have energy. But I kind of need to take this one and notice. Actually, he did give me notice, Andrew, but I didn't have time to really look further into it.

[00:16:45] But I think there's a stumbling block somewhere in that argument, which is probably that gravitational energy isn't energy that's convertible to mass. But I need to get my thoughts clearer on that, which they are at the moment.

[00:17:02] So Gus, thank you for a very tricky question, which I might think a little bit more about. And perhaps we will revisit it in a future episode of SpaceNuts Q&A. I put a homework marker next to it. Yeah, that's what I'm just doing that. I'm doing it.

[00:17:24] You're doing it in your Kugelschreiber. I'm using a red Kugelschreiber. Okay. I don't know what the German word for red is though. Oh, I could probably do it on Translate. It's wort. Wort. R-O-T. Ah, there you are. There you are. I don't have to look it up.

[00:17:42] You don't. So Gus, we don't know. Maybe, possibly, could be, don't know. There's the answer. Don't yet know. I like that. Let's get to the final question. We'll get back to you, Gus, at some stage in Western Australia, or it could be the United States.

[00:18:06] Now we've got a question from... just by coincidence from New Zealand again. Hi team, amazing podcast. Which one are you talking about now? I have been listening since your early days and have always looked forward to new uploads. My question is around the discovery of early galaxies

[00:18:25] from the James Webb Space Telescope. Is it possible for earlier galaxies to be traveling towards us that are currently out of reach, filling with potentially nothing... filling where potentially nothing was in view before? If possible, would the light be compressed? How would the instruments deal with that?

[00:18:47] Hope that makes sense. Cheers, Nick from Auckland, New Zealand. I... My brain just went, well, I suppose it's possible, but how do we prove it until it happens? Yes, so a couple of things in here. Thanks, Nick. Great question. The last bit about light being compressed.

[00:19:06] And in a way, that's quite a nice way of putting it. So anything that comes toward you that's emitting light, its light will be blue shifted. In other words, its wavelength will get shorter. And that's saying it's compressed. It's pretty well... That's pretty well what happens.

[00:19:25] It's like the good old ambulance siren or fire engine siren or whatever it is coming towards you, which compresses the sound waves. And the result is an increase in pitch, which corresponds to a shortening of wavelength. So that's standard physics. We can detect by the Doppler shift,

[00:19:46] anything coming towards us, by the fact that its light is shifted towards the blue end of the spectrum. But the first bit of the question about galaxies, earlier galaxies traveling towards us, we... When we think about galaxies, we have two different velocities involved.

[00:20:13] One is the velocity of a galaxy as it's carried along by the expansion of the universe. And that is what we measure as a redshift. The expansion of the universe is carrying galaxies away from us. And so their light is being redshifted.

[00:20:31] And by the time you get to these really early galaxies, where you're looking back almost the whole age of the universe, the redshift is very considerable. It's a factor of 13 or 14, something like that. We give it a name Z. The redshift is about 14.

[00:20:47] So I beg your pardon, no, that's not true. That's me confusing the age with the redshift. Forget that bit. But the number is quite high. The redshifts are probably five or six or something like that. But it's still a high level of the light being stretched out

[00:21:04] by the expansion of the universe. So that's one velocity. But galaxies can have a superimposed on that, a velocity which we call the peculiar motion, its own velocity caused by local eddies in space or whatever that might move a galaxy towards us.

[00:21:24] It's the gravitational field that it's exposed to. Very much like the analog is always a river carrying you along. And if you're in a rowboat, you can move relative to the river, but the river's always carrying you along. That's exactly what's happening with the Hubble flow,

[00:21:39] the expansion of the universe. And these peculiar motions are superimposed on that, but they're much, much less than the motion those distances or look back times. It's much, much less than the expansion flow of the universe. No, there won't be anything hidden from us that's coming towards us.

[00:21:59] I don't think it's an interesting suggestion, but everything's moving away from us at this very high velocity at those distances. Of course, Nick, if you want to check with us in a million years or so, we might have an alternative answer. Well, that's true.

[00:22:15] Put that in your diary and I'll mark it with an asterisk knowing that it's homework for a million years time. Yes, it's good. And I'm really disappointed that the people who make diaries haven't gone ahead that far yet. Thanks, Nick. Probably not, I think is the answer.

[00:22:39] Thanks for the question. Thanks to everyone who sent in questions. Keep them coming. You can do that via our website, spacenutspodcast.com, spacenuts.io, which has two options, the AMA tab at the top where you can send us text and audio or the send us your questions button

[00:22:55] on the right-hand side of our home screens. Don't forget to tell us who you are and where you're from, and you can probably upload your audio questions on any device as long as you've got a microphone. And mobile phones are perfect for this,

[00:23:08] but a lot of people have home computers with mics built in, et cetera, et cetera, et cetera. Always happy to hear from you. Fred, thanks so much. We're done with another episode. Jeez, we're racking them up. We are racking them up. Good to talk to you, Andrew.

[00:23:22] We'll speak again soon. Indeed, we will. Professor Fred Watson, astronomer at large, and thanks to Hugh in the studio for collating... Not much, but we thank him anyway. And from me, Andrew Dunkley, thanks to your company. See you on the very next episode of Space Nuts. Bye-bye.

[00:23:52] This has been another quality podcast production from tights.com