Dec. 20, 2024

Space Station Smells, Sombrero Galaxy & Dark Energy Dilemmas: #479

Space Station Smells, Sombrero Galaxy & Dark Energy Dilemmas: #479

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Space Nuts Episode: Stink in Space, Sombrero...

This episode is brought to you with the support of Incogni...the best way to cleanup your privacy online and remain that way. To get our special 60% off offer, visit www.incogni.com/spacenuts

Space Nuts Episode: Stink in Space, Sombrero Galaxy, and Dark Energy Revelations #479
Join Andrew Dunkley and Professor Fred Watson as they explore the latest cosmic events in this entertaining episode of Space Nuts. From a mysterious odour aboard the International Space Station to stunning images of the Sombrero Galaxy and groundbreaking theories on dark energy, this episode is packed with stellar insights and astronomical wonders.
Episode Highlights:
- International Space Station's Stinky Situation: Discover the unexpected odour that caused astronauts to temporarily seal off a recently docked Russian supply ship. Explore the potential causes and the measures taken to ensure the crew's safety.
- Sombrero Galaxy's New Look: Marvel at the breathtaking mid-infrared images of the Sombrero Galaxy captured by the James Webb Space Telescope. Learn about the intricate details revealed in the galaxy's dusty rings and the presence of polycyclic aromatic hydrocarbons.
- Dark Energy's New Twist: Delve into the latest research suggesting that dark energy might not be constant, challenging our understanding of the universe's expansion. Consider the implications of this potential paradigm shift in cosmology.
For more Space Nuts, including our continually updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, X, YouTube, Tumblr, Instagram, and TikTok. We love engaging with our community, so be sure to drop us a review, message or comment on your favourite platform.
For more Space and Astronomy News Podcasts, visit our HQ at www.bitesz.com.
Become a supporter of this podcast for extended commercial-free episodes and more. Visit our Support page for options: spacenutspodcast.com/about
Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.
For our special NordVPN deal, visit www.bitesz.com/nordvpn
00:00 - Andrew Dunkley hosts Space Nuts, where we talk astronomy and space science
01:08 - Professor Fred Watson will be doing archival episodes over the Christmas New Year period
03:02 - Bad smell coming from Russian spacecraft docking with International Space Station
09:01 - Arthur Dent. What a name. Only Douglas Adams could think up a name like that
09:24 - Andrew Dunkley says odour on International Space Station could be anything
11:09 - Incogni is a way of cleaning up your online presence
13:17 - James Webb telescope has taken a marvellous mid infrared image of galaxy
18:32 - The James Webb Space Telescope is seeking 78,000 hours of observing time
24:54 - Andrew Dunkley and Fred Watson discuss the accelerating expansion of the universe
32:25 - Fred Watson: This could indicate new physics that we don't yet understand
✍️ Episode References
Space.com
[https://www.space.com](https://www.space.com)
Phys.org
[https://www.phys.org](https://www.phys.org)
Incogni
[https://www.incogni.com/spacenuts](https://www.incogni.com/spacenuts)
Bytes.com
[https://www.bytes.com](https://www.bytes.com)


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WEBVTT

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Hi there, Thanks for joining us on Space Nuts, where

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we talk astronomy and space science. My name is Andrew Dunkley.

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Coming up on this episode. It is a real stinker,

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and we'll tell you why. Also some also some you're

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not supposed to make any noise yet, Fred.

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And also it's the end of the year, so we'll

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do whatever we like.

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The Sombrero Galaxy a new image or two, and it

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is stunning, to say the least, and possible new data

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about dark energy that might just tip everything upside down.

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We'll talk about all of that on this episode of Space.

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Nut fifteen in Channel ten nine Ignition Space Nuts or

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three two one Space Notes.

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I bought it, Neils good.

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It's very hard to keep Fred quiet when he's excited.

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Hello, Fred, I do apologize for speaking out of sherp.

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I keep forgetting you know.

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I'm not here yet, not here until I introduce you

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Professor Fred Watts, an astronomer at large.

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Thank you.

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That'll be that'll do yet.

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Nice Nice to see you, Nice to see you. It's

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our second to last episode of the year.

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Officially, we will be.

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Doing some archival episodes over the Christmas New Year period,

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probably some that people haven't heard in a very long time.

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It's it's I don't know whether it's a good or

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a bad thing that we've been going long enough to

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have archives.

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That's the past, that's the bart that stun speeding. It's

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fair enough.

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So yeah, but they're really good episodes. And what we're

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going to do just to keep them a bit fresher

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is tag them with a little bit of astronomical news

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as it happens over the Christmas New Year period. I'm

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leaving that up to Hugh in the studio. We finally

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found him a job.

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But yes, that's that's well.

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You see, there is a job there because if you've

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got if you've got an archive, you've got to have

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an archivist, Yes, somebody who you know, who looks after

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the archive. And I'm not going to give anything away

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here but money. And I have a really good friend

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who is the archivist to a former prime minister and

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she is still very very busy with things that concerned

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you know, his prime ministership and ongoing stuff.

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It's really about that.

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Yeah.

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Yeah, gosh, over my forty years in radio, I got

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to meet a lot of people with really fascinating jobs.

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I remember doing an interview with a fellow from Dubbo

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who was a tennis coach and he was a point

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he was appointed. You don't think about this thing, this

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sort of thing happening in Dubbo, but he was appointed

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to be the Davis Cup coach for India. Well, it

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was really fascinating. Yeah, you just never know what's going

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to pop up, never know it's correct.

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Now, we have.

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Some stories to tell in this second last episode of

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the year, and the first one's a real stinker involving

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the International Space Station, or at least a transport spacecraft

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that's arrived there. Recently, we talked about that weird sound

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coming from the Boeing star Liner, which ended up meaning

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it was they thought it was feedback, but there's been

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a few other theories. Now it's a rather stinky situation,

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quite literally for it.

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Yes, it is.

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So.

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This is a supply ship, a Russian supply ship. It's

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a Progress ninety spacecraft which docked with the International Space

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Station on the twenty third of November, just a few

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days ago as we're speaking now. And they it's a routine,

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completely routine process. You know, the supply ship arrives, you

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the hatches do the airlocks stuff, and.

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You take all thet all the peckets of M and

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m's and get on with everything.

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Yeah, that's right, and all the you know, the coffee

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supplies and all the rest of it. Probably, yes, that's right. Anyway,

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notwithstanding all that, they opened the door but immediately have

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to shut it again because there's such a bad smell

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coming from it.

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Wow, and uh.

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It's it's actually we might be we might be jumping

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to conclusions here. It's been described as an unexpected odor.

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And in fact, somebody, I think one of the comments

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was it smells a bit like a spray. And I

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assume by that I mean, you know, like an air

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freshener or something like that.

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So it might not be a bad smell, right, we're

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just assuming that because.

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Yeah, well that's why they don't only have baked beans

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on the Internet space track.

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Sure, that's right.

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The truth about being right, what was that blazing saddles

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the Yeah, so they shut the door straight away. And

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I should explain that the spacecraft, the the International Space

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Station is divided into sector excuse me, sectors. You know,

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it was made by joining together lots of modules, some

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of which were Russian, some of which were NASA and

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the Russian spacecraft dock with the Russian side of the

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of the International Space Station. So they the cosmonauts, Ross

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Cosmos scientists and well the cosmonauts, they're all flying. They

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they shut the shut the door immediately. Apparently they also

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saw what are described as small droplets, but I don't

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know whether they were droplets in the air or droplets

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in you know, the surfaces. But anyway, at the moment

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as we speak this, the door is shut and they

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are apparently and I'm quotingspace dot com here, the crew

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is not in danger and efforts to open the spacecraft

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are ongoing. That NASA stressed, but.

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There is.

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There is, you know, it's it's not when you've got

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an environment like that. All the air that these people

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are breathing is contained in the space station. It's not

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a question of opening the windows to let.

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I was about to say, they just should have just

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opened a window, open a window fresh and get some

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fresh nothing in there.

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Well, yes, so, but so what you have to do

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is something a little bit more serious. And again quoting

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from space dot com, very nice article on this. After

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Russian cosmonauts closed the hatch, air scrubbers and contaminant sensors

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on the International Space Station monitored the station's atmosphere and

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flight to Control has said their air quality was at

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normal level, so it hasn't sort the spread a bad

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smell throughout the whole of the of the spacecraft. Yeah, yes,

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that's right, Yeah, it is. It is a bit complex

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because there's there's doors and valves everywhere, and something I

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didn't know. Apparently the hatch that separates the Russian side

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from the U. S side is quite often closed at

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the moment, and that's people.

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Yeah, I was going to say, people will automatically, automatically

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assume that's got something to do with the war in Ukraine.

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But it's not nothing to do with that at all.

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Nothing at all. It's because the Russian side's leaking. There's

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an air leak. Again, everybody's stressing it's not a danger

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to anybody on board, but there is disagreement between NASA

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and Ross Cosmos as to what this leak is caused

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by and how you fix it and whether there is

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a longer term risk. You know, if if you've got

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a leak, you kind of worry that some something's fractured

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or something like that, and that it might catastrophically give

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way and suddenly you've got a big hole in the spacecraft.

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Yeah, apparently that leak's been going for.

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Like five years. That five years, I know, Oh goodness, Yeah,

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that was surprised at that too. Clearly, the the International

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Space Station is an aging piece of recruitment, and obviously

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you know it's it's the shining example of modern technology.

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But I'm always reminded of what was it that the

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I forgot what the name of the construction fleet was

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in the Hitchhiker's Guide to the Galaxy.

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Oh, theog Voggs.

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That's right, it is the Vogon Constructive Fleet. And when

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they when the heroes got inside one of the spacecraft,

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it was just full of old mattresses, l dingy, and

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so that it makes you think of that sort of thing.

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Was Arthur Arthur Dent, wasn't it then?

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After d Yes, that's right, and forward prefect.

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Yes, Oh gosh, I remember some trash.

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Oh no, that's that's worth remembering that it is.

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And and my favorite slaty bad Fast.

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Yeah slightly bart fast. Yeah, what a name. Only Douglas

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Adams could think of the name.

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He was avazing, wasn't he amazing, we're off the track.

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We're talking about the old mattresses on the ISS.

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Well, I mean we were talking not very long ago

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Andrew about people just parking things on places where there's

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a bit of velcrow that they can do something on,

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and you know, stuff that you wouldn't expect because uh,

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there was that study of done of the archaeology of

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the International Space Station and people photographing bits of the

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space station just to provide a record of how what

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life is like on the International Space.

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And they put all these still porage systems up for

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certain uses and found that people were using them for

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completely different reasons.

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For other things.

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That's right, Yeah, it's quite interesting. So they don't know

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what the stink is. They don't know. What I understand

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about this supply chip is that they take all the

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goods out and then they fill a thing with rubbish

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and then they burn it up on re entry.

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I'll get rid of the rubbish.

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So that's you know, if you yeah, if you can't

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get into it without a space tom, Yeah, it's not

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very nice. Yeah, we'll worry. Look forward to hearing what

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the cause was if they have a work it out,

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and if we can we'll bring it to spacelu's listeners.

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Yes, indeed, not something you really need going into Christmas. Yeah,

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could could be anything, could could be anything. Hopefully it's

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not a bad smell. We haven't determined, you know, what

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the caliber of the odor is, but yeah, hopefully nothing

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nasty or noxious.

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Or any like that.

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You can read that story at space dot com. This

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is Space Nuts with Andrew Dunkley and Professor Fred Watson.

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Let's take a break from the show to tell you

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00:13:08.759 --> 00:13:17.919
slash space nuts. Now back to the show Space Nuts Now, Fred,

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we head out a little way from our own galaxy

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to a wonderful place called the Sombrero galaxy M one

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O four to be official, and James Webb has just

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taken a marvelous mid infrared image of it that has

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got a lot of people very excited.

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It does, yeah, and it's you know, this is the

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thing about the web telescope. It just blows you away

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with everything new that comes from it, because we're seeing

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familiar objects in the completely new lights in for red

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lights to be exact. So just to paint the picture,

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you said, m one O four and is Messier of

240
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French astronomer of the eighteenth i think late eighteenth century

241
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who was interested in comets and he could see all

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these other fuzzy patches in the sky, so he just

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numbered them and we and these are mostly galaxies. He

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didn't know that's what they were, but that's what we find.

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So M one O four normally known as the Sombrero

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galaxy because that's what it looks like. It's got a

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prominent dusty ring around it and a very bright and

248
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very extended core so that the central region, you know,

249
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looks like the top of a hat, and the and

250
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the outer ring looks like the rim of the hat,

251
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but with the MIRI view, and MIRI is the midim

252
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for red instrument on the James West Telescope. The core

253
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which is made of stars, that extended core the sort

254
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of bowl of the hat, if I can put it

255
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that way, it vanishes completely and we see the ring

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itself in glorious detail. This is I think they're actually

257
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two rings, because there's a ring very near the center

258
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of the galaxy also, but this outer ring which is

259
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very very dusty, and that's why it shows up so

260
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well in mid in forread remember mid in for read light,

261
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the dusties opaque, and you can actually see the dust

262
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directly near In forred, the light penetrates the dust. So

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what is excited people is detail in this ring that

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has never been seen before. And it's the scientists, and

265
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some of them are a number among my friends who

266
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look at this kind of thing, dusty regions in galaxies.

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They are excited to see that it's very clumpy on

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a scale of detail that, as I said, hasn't been

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seen before. And when you look at the image, you

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can see that this ring is made up of myriads

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of tiny clumps of dust. Now, the spectroscopy instrument or

272
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part of Mary. The infrared detector has provided evidence of

273
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polycyclic aromatic hydrocarbons.

274
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Wow, that's that's a coincidence, because I believe that's what

275
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they're smelling on it extra space.

276
00:16:17.360 --> 00:16:20.159
It might be, Yeah, it might be. It depends how

277
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aromatic they are. They might be a bit un aromatic.

278
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The might it is.

279
00:16:25.200 --> 00:16:31.720
But polycyclic aromatic hydrocarbons a class of organic molecules carbon containing,

280
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and you know the sort of thing that we think

281
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of as as going into young solar systems that they

282
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demonstrate that there's probably star forming regions embedded in the

283
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disc of the of the galaxy Sombrero is it's a

284
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it's not a you know, one of these galaxies that's

285
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rapidly forming forming stars. It's it's what you might call

286
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a quiescent galaxy. It is forming stars, but it's at

287
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a slow rate. It's about half the rate that our

288
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own galaxy is forming stars, which is roughly two stars

289
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per year.

290
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Roughly. I think, I think I know why.

291
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I think I know why the sombrero is slightly dipped.

292
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So I think this galaxy is having a siesta.

293
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There you go.

294
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That would be the official scientific reason.

295
00:17:28.119 --> 00:17:30.759
That probably would be look.

296
00:17:30.799 --> 00:17:31.240
I like that.

297
00:17:31.359 --> 00:17:36.240
I like that terminology. The siesta time of the Sombrero galaxy.

298
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Lovely good bit.

299
00:17:37.799 --> 00:17:41.480
And indeed it is slightly dipped in the sky, so

300
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it does have a black hole, supermassive black hole something

301
00:17:47.240 --> 00:17:49.720
like nine billion solar masses, much much bigger than the

302
00:17:49.720 --> 00:17:53.240
black hole at the center of our own galaxy. And

303
00:17:53.319 --> 00:17:57.680
it is active. So it's what we call an agn

304
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an active galactic nucleus, which is something that is you know,

305
00:18:02.039 --> 00:18:06.799
it's having a polite and well behaved meal of material

306
00:18:06.880 --> 00:18:11.039
that's falling into it from its surroundings, rather than a

307
00:18:11.160 --> 00:18:15.440
quasar which is absolutely gobbling everything up and radiating energy

308
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at a great rate because of that.

309
00:18:17.759 --> 00:18:21.759
So, yes, I think they described this one as docile,

310
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if that.

311
00:18:22.799 --> 00:18:24.680
Can be a yeah, I think that's probably the word

312
00:18:24.720 --> 00:18:29.759
I was looking for. Andrew, Yeah, Doso, Yes, it's low

313
00:18:29.839 --> 00:18:34.720
luminosity active galactic nucleus. Sombrero has always been interesting though,

314
00:18:34.799 --> 00:18:38.240
and this goes back to beautiful images of the Sombrero

315
00:18:38.279 --> 00:18:40.680
that were made by my colleague David Maelin back in

316
00:18:40.720 --> 00:18:43.680
the nineteen eighties, the first time we saw these galaxies

317
00:18:43.720 --> 00:18:48.119
in color, along with many other nebulae. He was the

318
00:18:48.160 --> 00:18:52.519
person who put true color into astronomical imaging by using

319
00:18:52.519 --> 00:18:55.799
a three color photographic technique. His image of the Sombrero

320
00:18:55.960 --> 00:18:59.799
is perhaps one of the iconic images of the galaxy.

321
00:19:00.359 --> 00:19:03.400
But what it did show was that the Sombrero is

322
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very rich in globular clusters, these sort of more or

323
00:19:08.000 --> 00:19:13.039
less spherical clusters of hundreds of thousands of stars. There

324
00:19:13.039 --> 00:19:17.799
are about two thousand of them surrounding the Sombrero galaxy.

325
00:19:17.839 --> 00:19:20.960
We have less than two hundred. I think this about

326
00:19:20.960 --> 00:19:23.599
one hundred and sixty if I remember rightly, globular clusters

327
00:19:24.319 --> 00:19:26.799
in the outskirts of our own galaxy. But the Sombrero

328
00:19:26.960 --> 00:19:30.640
is much much richard. And of course it's near enough.

329
00:19:30.640 --> 00:19:34.680
It's thirty million light years away. That's pretty well on

330
00:19:34.720 --> 00:19:40.480
our doorstep, which is where gets such good images of it.

331
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It's near enough that we can study those globular clusters

332
00:19:43.799 --> 00:19:46.920
in detail. And globular clusters are one of the they're

333
00:19:46.960 --> 00:19:51.680
one of the puzzling things in our understanding of the universe.

334
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Are they the nuclei of galaxies that have been stripped

335
00:19:56.960 --> 00:20:01.480
of their outer stars by interactions with other galaxies, or

336
00:20:01.640 --> 00:20:05.240
where they formed like that as globular clusters in the

337
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earliest history of the universe. There was quite a under

338
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discussion on that topic.

339
00:20:08.599 --> 00:20:09.359
Actually our.

340
00:20:12.200 --> 00:20:16.000
Fiftieth anniversary symposium for the End of Australian Telescope, it

341
00:20:16.039 --> 00:20:19.720
was an interesting session on globular clusters what we can

342
00:20:19.799 --> 00:20:20.599
learn from them.

343
00:20:21.039 --> 00:20:24.680
Judy and I've got a lot of experience with globular clusters.

344
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Every Tuesday we baby sit the grandchildren.

345
00:20:28.920 --> 00:20:30.400
A lot of globby for clusters.

346
00:20:31.559 --> 00:20:34.039
I bet there are. Yeah, you've got two thousands of

347
00:20:34.039 --> 00:20:35.480
them though, then you're in real trouble.

348
00:20:35.839 --> 00:20:36.839
Oh I think they managed that.

349
00:20:37.799 --> 00:20:42.400
Yeah, yeah, So look, there's just more to come. It's

350
00:20:42.400 --> 00:20:47.720
a reminder of how prolific the James Web Telescope is.

351
00:20:48.400 --> 00:20:51.839
Its fourth year of science. Operations will start in the

352
00:20:51.839 --> 00:20:53.279
middle of next year, next July.

353
00:20:53.359 --> 00:20:53.640
Wow.

354
00:20:54.279 --> 00:20:59.160
They've already had a record breaking number of proposals for

355
00:21:00.119 --> 00:21:06.319
time on that during that fourth period. The deadline for

356
00:21:07.400 --> 00:21:13.359
submissions for observations was fifteenth of October. And you know

357
00:21:13.519 --> 00:21:20.279
it's an over subscribed instrument. The request I love this

358
00:21:20.640 --> 00:21:24.200
request for seventy eight thousand hours of observing time, which

359
00:21:24.240 --> 00:21:27.759
is nine times more than there is available. That's what

360
00:21:27.799 --> 00:21:29.839
we call an over subscription rate. We used to get

361
00:21:30.119 --> 00:21:33.519
over subscription rates of two or three and sometimes four

362
00:21:33.559 --> 00:21:36.119
on the Anglo Australian Telescope. People want, you know, for

363
00:21:36.200 --> 00:21:38.240
every one night on it, the four people wanted to

364
00:21:38.319 --> 00:21:42.079
use it. But nine to one is quite extraordinary, and

365
00:21:42.319 --> 00:21:44.720
it speaks of just the excellence of the data that

366
00:21:44.759 --> 00:21:46.480
are coming from the Jamesweg Telescope.

367
00:21:46.839 --> 00:21:48.240
I suppose that means fre it.

368
00:21:48.319 --> 00:21:53.519
If they've got a record number of proposals put to

369
00:21:53.599 --> 00:21:56.599
them for time on the James web Space telescope, they're

370
00:21:56.640 --> 00:21:59.440
going to have to sit down and pick hand pick

371
00:21:59.720 --> 00:22:01.720
who gets to use it and who gets to miss out.

372
00:22:02.440 --> 00:22:04.759
Yes, that's the job of time allocation committees.

373
00:22:04.759 --> 00:22:05.799
That's exactly what they do.

374
00:22:06.519 --> 00:22:08.680
And I think every telescope in the world has got

375
00:22:09.519 --> 00:22:12.799
committees like that that go through them, and they're usually

376
00:22:14.079 --> 00:22:20.319
extremely ethical. They give time based only on scientific excellence.

377
00:22:21.279 --> 00:22:24.920
So the applications throughout the world again I would think

378
00:22:24.920 --> 00:22:27.079
this is true. They're anonymized, so you don't know who

379
00:22:27.079 --> 00:22:30.000
they've come from. They're sort of gender free, so you

380
00:22:30.000 --> 00:22:33.359
don't know you know what the gender of the applicant is.

381
00:22:33.400 --> 00:22:36.200
It's to avoid any kind of bias of any sort,

382
00:22:37.079 --> 00:22:43.079
and it's a fairly stringent proge process. I do remember

383
00:22:43.119 --> 00:22:46.440
talking to one of my colleagues who was sat on

384
00:22:46.440 --> 00:22:48.640
one of these time allocation committees actually for the Angle

385
00:22:48.640 --> 00:22:51.400
of Australian Telescope over quite a long period, and he

386
00:22:51.759 --> 00:22:55.559
mentioned the occasional death threats that he got from you know,

387
00:22:56.880 --> 00:23:01.079
who hadn't been given their time. Yeah. Yeah, people life

388
00:23:01.079 --> 00:23:03.319
and soul into it. There weren't death threats, So it's

389
00:23:03.400 --> 00:23:08.720
just you know, uh, fairly fairly. How can I put

390
00:23:08.720 --> 00:23:10.319
its robust criticism?

391
00:23:10.440 --> 00:23:13.519
That's sort of yeah, well that's a nice win putting

392
00:23:13.519 --> 00:23:14.200
it robust.

393
00:23:14.440 --> 00:23:16.119
He interpreted them as death threats.

394
00:23:18.119 --> 00:23:19.640
Wow, that's extraordinary.

395
00:23:19.839 --> 00:23:22.319
Yes, I wouldn't have thought that of the of the

396
00:23:22.599 --> 00:23:24.200
astronomical community for it.

397
00:23:24.400 --> 00:23:24.839
You wouldn't.

398
00:23:25.319 --> 00:23:27.359
But if you've you know, if you've submitted the same

399
00:23:27.400 --> 00:23:29.960
application maybe three years in a row, and you've put

400
00:23:29.960 --> 00:23:32.079
your life and soul into it, and you've got students

401
00:23:32.079 --> 00:23:35.759
who's whose future depends on getting the observing time and

402
00:23:35.799 --> 00:23:38.960
you don't get it, you would feel naturally very frustrated.

403
00:23:39.319 --> 00:23:43.039
Oh yeah, that makes that makes perfect sense. But I

404
00:23:43.039 --> 00:23:45.880
think when we were first talking about James Web we

405
00:23:45.960 --> 00:23:49.839
did talk about how that process worked and how how

406
00:23:49.880 --> 00:23:51.480
they were going to do it to make sure that

407
00:23:51.519 --> 00:23:54.880
it was all, you know, above board, level playing field,

408
00:23:54.960 --> 00:24:00.480
no bias, and yeah, but if you want look at

409
00:24:00.519 --> 00:24:04.240
the pictures of the Sombrero Galaxy as taken by the

410
00:24:04.319 --> 00:24:05.880
James web Space telescope.

411
00:24:06.319 --> 00:24:08.799
Not surprisingly, it's at fizz dot org.

412
00:24:09.240 --> 00:24:11.400
I'm starting to feel sorry for Hubble because.

413
00:24:11.160 --> 00:24:13.400
Whenever there's a new James Webb image, they go and

414
00:24:13.440 --> 00:24:18.559
this is what Hubble took. I just don't think that's fair.

415
00:24:19.519 --> 00:24:22.880
No, but it's you know, and of course the Hubbles

416
00:24:22.880 --> 00:24:25.559
are two point three meters telescope. James Webb is a

417
00:24:25.599 --> 00:24:28.559
six point five meter telescope. He astronomy sizes everything.

418
00:24:29.480 --> 00:24:32.920
Yes, well, very true. But Hubble's still doing a great job.

419
00:24:33.160 --> 00:24:35.200
But feel sorry for Hubbling, you know it is.

420
00:24:35.519 --> 00:24:38.559
It's doing doing a fine job and still producing good science.

421
00:24:38.799 --> 00:24:41.000
I'm sorry I was slightly distracted there. I'm trying to

422
00:24:41.039 --> 00:24:43.720
pick the key to the James Webb telescope which has

423
00:24:43.720 --> 00:24:45.759
fallen on the floor and I can't actually pick.

424
00:24:45.599 --> 00:24:45.920
It up.

425
00:24:48.200 --> 00:24:49.960
Fair enough fizz dot org.

426
00:24:50.000 --> 00:24:51.640
If you want to check out that story about the

427
00:24:51.680 --> 00:24:54.599
Sombrero Galaxy and what we're learning about it.

428
00:24:54.960 --> 00:24:58.799
This is Space Nuts with Andrew Dunkley and Professor Fred Watson.

429
00:25:01.359 --> 00:25:02.440
Okay, we've taken all.

430
00:25:04.279 --> 00:25:10.359
Space nuts. Finally, Fred a story that has been published

431
00:25:10.599 --> 00:25:14.240
only in the last few days our time, but this

432
00:25:14.279 --> 00:25:16.799
one will be talked about for a long time because

433
00:25:17.880 --> 00:25:22.799
again they're suggesting that this one could rewrite what we

434
00:25:22.839 --> 00:25:28.400
know about the cosmos. This all centers around dark energy

435
00:25:29.400 --> 00:25:32.960
and we might have to explain what that is again

436
00:25:33.039 --> 00:25:37.480
because it's so poorly named. But now they're starting to

437
00:25:37.680 --> 00:25:43.319
think that dark energy might be a finite thing based

438
00:25:43.319 --> 00:25:44.240
on this new data.

439
00:25:46.079 --> 00:25:51.880
Yes, it's a very difficult thing to measure. Is the

440
00:25:52.200 --> 00:25:54.880
accelerated expansion of the universe, which is why we didn't

441
00:25:54.920 --> 00:25:58.599
know about it until nineteen ninety eight. Two groups of scientists,

442
00:25:58.680 --> 00:26:03.160
one in the USA and one in Australia actually worked

443
00:26:03.160 --> 00:26:06.960
out that the expansion of the universe is accelerating. So

444
00:26:07.759 --> 00:26:10.079
a lot of thoughts has gone into it since then.

445
00:26:10.880 --> 00:26:20.319
That's twenty six years ago. And the simplest interpretation is

446
00:26:20.359 --> 00:26:25.599
that dark energy is constant. That means that the acceleration

447
00:26:25.720 --> 00:26:30.880
of the universe is something that does not change over

448
00:26:30.960 --> 00:26:34.319
time except by the fact that a space gets bigger,

449
00:26:35.559 --> 00:26:39.400
the energy content of space gets bigger, and so you've

450
00:26:39.440 --> 00:26:43.519
got an increased push to accelerate the expansion of the universe.

451
00:26:44.319 --> 00:26:53.000
So there's been a fairly consistent view which has apparently

452
00:26:53.079 --> 00:27:00.839
been supported by observations that this dark energy is constant. However,

453
00:27:01.960 --> 00:27:08.920
some work that's been done on basically a telescope in Arizona.

454
00:27:08.960 --> 00:27:13.920
Actually it's the Male telescope, which has a camera on

455
00:27:13.960 --> 00:27:15.079
it which has been.

456
00:27:15.039 --> 00:27:15.640
Used to.

457
00:27:17.240 --> 00:27:21.119
Basically study distant galaxies in great detail and look at

458
00:27:21.119 --> 00:27:23.839
a huge number of them. It's a very very elegant

459
00:27:23.960 --> 00:27:30.799
sort of camera. They are now thinking that the dark

460
00:27:30.920 --> 00:27:38.519
energy is not quite constant. And it's basically that issue

461
00:27:38.559 --> 00:27:42.839
that is concerning those of us in the astronomy community

462
00:27:42.839 --> 00:27:45.240
who are interested in the future of the universe as

463
00:27:45.240 --> 00:27:48.240
well as it's past. What it means is so and

464
00:27:48.279 --> 00:27:53.119
I should you know, I shouldst mentioned that this involves

465
00:27:53.119 --> 00:27:56.000
a very large number of scientists. It's a huge collaboration.

466
00:27:56.119 --> 00:27:58.599
Some of my colleagues here in Australia, the members of

467
00:27:58.640 --> 00:28:02.680
this collaboration. There are ninehundred scientists all over the world

468
00:28:02.759 --> 00:28:09.720
studying these data. Now it's a re analysis that we've

469
00:28:10.200 --> 00:28:12.960
seen coming out within the last few days. This is

470
00:28:12.960 --> 00:28:17.400
why this is in the headlines again. It was the

471
00:28:17.400 --> 00:28:20.599
original data were published earlier in the year, but the

472
00:28:20.680 --> 00:28:26.160
new analysis has sort of confirmed it that there is

473
00:28:26.200 --> 00:28:32.359
something going on that we don't understand that change.

474
00:28:32.480 --> 00:28:35.319
That's a big change.

475
00:28:34.960 --> 00:28:38.960
So the way it works, it's an instrument called DESI,

476
00:28:39.400 --> 00:28:43.960
the Dark Energy Spectroscopic Instrument, which is on the Male Telescope,

477
00:28:44.720 --> 00:28:48.920
and that's very similar to the to d F instrument

478
00:28:48.960 --> 00:28:51.319
that we have on the d Australian Telescope, which did

479
00:28:51.319 --> 00:28:53.440
this sort of thing back in the early two thousands.

480
00:28:53.440 --> 00:28:56.279
But now the technology has improved to the extent that

481
00:28:56.319 --> 00:28:59.279
you can look at many many more objects simultaneously. To

482
00:28:59.440 --> 00:29:03.359
DF looked at at four hundred and now you've got

483
00:29:03.400 --> 00:29:05.799
many many more than that and seeing them in more

484
00:29:05.839 --> 00:29:11.759
detail spectroscopically and with sensitive detectors that you let you

485
00:29:11.839 --> 00:29:15.960
look back in time up to about eleven billion years

486
00:29:16.279 --> 00:29:19.720
before the present time. So what you're doing there is

487
00:29:19.839 --> 00:29:24.400
you are basically you're mapping the universe. This is where

488
00:29:24.400 --> 00:29:27.400
it gets a little bit counterintuitive the way you detect

489
00:29:27.480 --> 00:29:31.160
dark energies to map the universe, to map where galaxies lie,

490
00:29:31.240 --> 00:29:35.200
because it's all about the way galaxies cluster. That gives

491
00:29:35.200 --> 00:29:37.799
you the geometry of the universe, and that then gives

492
00:29:37.839 --> 00:29:44.440
you what its expansion rate is doing. So they've looked

493
00:29:44.440 --> 00:29:51.200
at these galaxies over eleven billion years and basically it

494
00:29:51.319 --> 00:29:57.519
reveals that, yes, if dark energy was a constant force,

495
00:29:58.319 --> 00:30:02.000
and Jordie's getting excited because somebody's about to come home.

496
00:30:04.240 --> 00:30:08.599
If dark energy was a constant force, that map would

497
00:30:09.720 --> 00:30:14.920
would not make sense. And what they are interpreting this

498
00:30:15.039 --> 00:30:19.160
mapping as telling us that the energy is weakening and

499
00:30:19.440 --> 00:30:24.640
that it's you've got an acceleration that is itself slowing down,

500
00:30:24.839 --> 00:30:28.359
even though the expansion of the universe is still accelerating,

501
00:30:28.680 --> 00:30:32.759
but the acceleration is slowing down because dark energy is

502
00:30:32.839 --> 00:30:36.640
reducing and that means it's quite different from what we

503
00:30:36.759 --> 00:30:40.519
thought it was, or that we're barking up the wrong

504
00:30:40.599 --> 00:30:44.519
tree completely, that it's not an energy of space, that

505
00:30:44.599 --> 00:30:46.759
there is something totally different going on.

506
00:30:47.400 --> 00:30:53.119
This could turn a whole understanding of the cosmological model

507
00:30:53.200 --> 00:30:57.680
upside down. They're basically, oh, Jeordie's upset by that.

508
00:30:58.400 --> 00:31:00.359
No, you've hit the nail on the head there. I

509
00:31:00.400 --> 00:31:04.119
think the joy I think that's that's agreed, that's agreement.

510
00:31:04.240 --> 00:31:08.960
Is that Jodey if O, my goodness, say, I'm really sorry.

511
00:31:10.160 --> 00:31:12.920
This is what he does is he gets very enthusiastic

512
00:31:13.079 --> 00:31:15.440
hang hagos ad.

513
00:31:18.599 --> 00:31:22.880
Oh gosh, that is so funny. Do you reckon.

514
00:31:24.880 --> 00:31:24.960
It?

515
00:31:25.079 --> 00:31:26.319
Can't even find him.

516
00:31:26.640 --> 00:31:30.480
Oh boy, we've just got to the key, the key

517
00:31:30.559 --> 00:31:40.839
moment of the story. Yeah, oh gosh, I'm going to

518
00:31:40.880 --> 00:31:43.880
put an asterisk on that so that I can find

519
00:31:43.920 --> 00:31:47.480
it later. I hope you're listening here. That's that's worth

520
00:31:47.480 --> 00:31:53.240
bottling that one. They can't hear me because Fred used

521
00:31:53.279 --> 00:31:56.079
his Headphanes, I keep telling you this part of the

522
00:31:56.119 --> 00:31:59.680
story without him, But honestly, it's it's it's mind blowing.

523
00:32:00.039 --> 00:32:03.960
It's mind blowing. Needs an expert touch, which I can't

524
00:32:04.160 --> 00:32:06.160
give you. Here he cams with here gams.

525
00:32:08.200 --> 00:32:11.559
Sorry about that, so we might have got that bit

526
00:32:11.680 --> 00:32:12.960
able to do apologize.

527
00:32:13.319 --> 00:32:16.119
Oh no, that's all right. He'll probably lave it in.

528
00:32:18.000 --> 00:32:20.839
It just goes mad. Apparently there's another dog around.

529
00:32:20.559 --> 00:32:23.359
Which, oh, well, that'll do it. That'll do it.

530
00:32:23.200 --> 00:32:23.440
Do it.

531
00:32:25.319 --> 00:32:27.880
So we were talking about what this means for our

532
00:32:28.000 --> 00:32:31.920
understanding of the standing cosmological model.

533
00:32:32.400 --> 00:32:34.720
We were and it obviously means that dogs are going

534
00:32:34.759 --> 00:32:37.000
to bark louder and longer than they ever have done

535
00:32:37.039 --> 00:32:41.519
before because it's such an astonishing result. Yeah, So what

536
00:32:41.559 --> 00:32:46.839
it means is it's it's going to be an ongoing story.

537
00:32:47.039 --> 00:32:48.720
We will hear more about.

538
00:32:48.559 --> 00:32:54.559
This over the next few months probably, and hopefully we

539
00:32:54.640 --> 00:32:57.799
will have some sort of what you might call a

540
00:32:57.839 --> 00:33:03.880
consensus coming up something that that that will you know,

541
00:33:03.960 --> 00:33:08.400
allow the theory theoretical astronomers who build models of all

542
00:33:08.440 --> 00:33:11.359
this stuff to try and get their heads around what

543
00:33:11.440 --> 00:33:15.920
might be happening with this current reduction of the acceleration

544
00:33:16.079 --> 00:33:16.839
rate of a time.

545
00:33:17.559 --> 00:33:17.960
Mm hmm.

546
00:33:18.720 --> 00:33:21.960
Well, yeah, it's it's one of the big mysteries, and

547
00:33:22.519 --> 00:33:25.240
it's something that we get asked about quite often for

548
00:33:25.319 --> 00:33:28.920
Q and A episodes, and it's something that keeps coming up,

549
00:33:28.960 --> 00:33:33.440
and they keep testing Einstein's theory of general relativity to

550
00:33:33.440 --> 00:33:38.240
see if they can break it. You know, there is

551
00:33:38.319 --> 00:33:41.960
so much at stake in terms of this kind of

552
00:33:42.720 --> 00:33:47.799
data and studying dark energy and you know, finding out

553
00:33:47.839 --> 00:33:49.519
what it is and what it's doing and why it's

554
00:33:49.559 --> 00:33:52.240
there and how it works, all of which we don't

555
00:33:52.279 --> 00:33:53.119
really understand.

556
00:33:53.759 --> 00:33:56.079
No, I mean, you've hit the nail on the head

557
00:33:56.079 --> 00:33:59.559
and drew in the sense that this could be an

558
00:33:59.599 --> 00:34:03.000
indicat of new physics that we don't understand. Going on

559
00:34:03.039 --> 00:34:06.319
in the universe, and that's where things get really exciting,

560
00:34:06.359 --> 00:34:08.960
because we rewrite the textbooks on levels of that sort

561
00:34:09.000 --> 00:34:09.239
of thing.

562
00:34:09.920 --> 00:34:13.880
Yes, and that leads to dogs and cats living together

563
00:34:13.960 --> 00:34:24.119
and all sorts of terrible things. Maybe not, but yeah.

564
00:34:21.320 --> 00:34:23.159
Yeah indeed, but yeah.

565
00:34:23.199 --> 00:34:28.440
It's a fascinating story, very much worth reading, and I'm

566
00:34:28.480 --> 00:34:32.400
sure it will spawn multiple questions for us to deal

567
00:34:32.480 --> 00:34:36.280
with in the next a series of episodes in twenty

568
00:34:36.320 --> 00:34:40.880
twenty five. You can read that story in fizz dot org.

569
00:34:41.039 --> 00:34:43.760
The dark energy pushing a universe apart may not be

570
00:34:43.920 --> 00:34:47.039
what it seems scientists say. That's the title of the piece.

571
00:34:48.239 --> 00:34:51.519
We are just about done, Fred, thank you so much.

572
00:34:52.320 --> 00:34:57.119
Ah, pleasure as always, and we'll speak again soon, I hope.

573
00:34:57.039 --> 00:35:01.360
Yes, very soon, probably for our finalpisode of the year.

574
00:35:01.480 --> 00:35:05.199
Thanks Fred, Professor Fred Watson, Astronomer at Large, and thanks

575
00:35:05.199 --> 00:35:07.960
to Hugh in the studio who couldn't be with us

576
00:35:07.960 --> 00:35:10.760
because he was dealing with a dark matter bomb bomb.

577
00:35:11.079 --> 00:35:13.199
And from me from me Andrew Dunkley.

578
00:35:13.559 --> 00:35:15.239
By the way, don't forget to visit our website and

579
00:35:15.280 --> 00:35:19.840
our social media platforms and leave reviews on your podcasting

580
00:35:19.880 --> 00:35:23.119
platforms if you If you do don't mind. Reviews are

581
00:35:23.159 --> 00:35:26.320
always very helpful to spread the word. But for now,

582
00:35:26.480 --> 00:35:28.280
thank you and we'll see you again on the next

583
00:35:28.320 --> 00:35:30.199
episode of Space Nuts.

584
00:35:30.320 --> 00:35:35.360
Bye bye Nuts. You'll be listening to the Space Nuts podcast.

585
00:35:36.400 --> 00:35:42.480
Available at Apple Podcasts, Spotify, iHeartRadio, or your favorite podcast player.

586
00:35:42.639 --> 00:35:45.920
You can also stream on demand at bides dot com.

587
00:35:45.960 --> 00:35:51.239
This has been another quality podcast production from nights dot com.
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