March 6, 2025

Lunar Landings, Asteroid Adventures & Andromeda Mysteries: #501

Lunar Landings, Asteroid Adventures & Andromeda Mysteries: #501

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Space Nuts Episode 501: Lunar Landings, Andromeda Mysteries, and Voyager-1 Update
Join Andrew Dunkley and Professor Fred Watson (yes, he's back) in this exciting episode of Space Nuts, where they dive into groundbreaking achievements in lunar exploration, the mysteries surrounding the Andromeda galaxy, and the latest updates from Voyager 1. This episode is packed with fascinating insights and updates that will keep you engaged and curious about the cosmos.
Episode Highlights:
- Blue Ghost Lunar Lander: The episode kicks off with the successful landing of the Blue Ghost lunar lander by Firefly Aerospace. Andrew and Fred discuss the significance of this commercial mission, how it differs from past government-funded endeavors, and what it means for future lunar exploration.
- Odin Asteroid Probe Troubles: The duo then shifts focus to the Odin asteroid probe, which has encountered some challenges en route to its target. They explore the implications of its current state and what this means for the future of asteroid mining and exploration missions.
- Andromeda Galaxy's Dwarf Galaxies: Andrew and Fred delve into the latest research on Andromeda, discussing how its dwarf galaxies are behaving unusually. They explore the potential gravitational influences at play and the surprising findings from Hubble observations that challenge existing theories about galaxy formation.
- Voyager 1's Communication Update: The episode wraps up with an update on Voyager 1, the most distant human-made object, which has resumed sending intelligible signals back to Earth after overcoming some technical difficulties. Andrew and Fred reflect on the incredible journey of Voyager 1 and its ongoing contributions to our understanding of the universe.
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 Music Music, Tumblr, Instagram, and TikTok. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.
If you'd like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit 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.
00:00 - Introduction and lunar lander success
02:15 - Discussion on the Blue Ghost lunar lander
10:30 - Updates on the Odin asteroid probe
18:00 - Insights into Andromeda's dwarf galaxies
26:45 - Voyager 1's communication update
30:00 - Closing thoughts and listener engagement
✍️ Episode References
Blue Ghost Lunar Lander Mission Details
https://www.firefly.com/blueghost
Odin Asteroid Mission Overview
https://www.astro.com/odin
Andromeda Galaxy Research Findings

 

 

WEBVTT

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Andrew Dunkley: Hello again. Thanks for joining us. This is

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Space Nuts. My name is Andrew Dunkley. Thanks

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for joining us. Coming up on this episode, we

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are going to be looking at a rather amazing

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achievement involving a. An

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organization who have landed on the moon. And

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you're saying, yeah, it's been done. Not like

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this, it hasn't. On top of that, we've got

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a mission that's going past the moon that

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is in a little bit of trouble as well. We'll

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also focus our attention on the Andromeda

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galaxy. And we've had some questions recently

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about Andromeda. Well, uh, you be interested

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to know that it has been

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suffering from interference and it wasn't us.

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It wasn't. We didn't do it. And Voyager

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1 back in the news again. That's all coming

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up on this episode of space nuts.

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Voice Over Guy: 15 seconds. Guidance is internal.

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10, 9. Ignition

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sequence start. Space nuts. 5, 4, 3,

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2. 1. 2, 3, 4, 5, 5, 4,

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3, 2, 1. Space nuts. Astronauts

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report it feels good.

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Andrew Dunkley: And he's back in the big chair after a month

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away. It's Professor Fred Watson, Astronomer

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at large. Hello, Fred.

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Professor Fred Watson: Hello, Andrew. Good to be back. Uh, so

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the politicians always say, good to be with

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you.

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Andrew Dunkley: Yes, they do, don't they?

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Professor Fred Watson: Good to be with you.

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Andrew Dunkley: I'm sure they sit there with, um, with

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consultants and committees. The right way to

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say hello.

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Professor Fred Watson: Yes, that's right. And the answer

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is. Good to be with you.

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Andrew Dunkley: Good to be with you.

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Um, now, we talked on the last

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episode or two, um, when you

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popped in on us, um, about your trip

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north. One thing I wondered

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is, while you were there to look at the

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aurora borealis and the like,

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um, on an astronomy tour, did you actually

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get to see, uh, the planetary

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alignment? Or couldn't you view it from that

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far north?

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Professor Fred Watson: Uh, we could, but, uh,

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you're right, it's a good question because

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the ecliptic, which is where all the planets

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lie, uh, just like the equator, the

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celestial equator is very low down at the

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latitudes we were at. The furthest north we

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got was to north cape, which is 71 degrees

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latitude. Um, a lot of the time we're in

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Greenland. Iceland's a little bit further

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south. It's only the top, really. The north

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coast of Iceland, that's within the Arctic

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Circle. But we're also, well, in the Arctic

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Circle in Sweden and Norway. North Cape, of

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course, is in Norway. Uh, so, yes, your view

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of the sky is different. Um,

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what? Always. And I remember being struck by

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this in my very, very first visit

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to the Arctic, which was back in 2012 when we

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led our first expedition up there.

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Uh, and I was struck by the fact that I

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could see stars which

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from our latitude in. And I'm

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still thinking of the northern hemisphere

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from the latitude of the United Kingdom, were

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only visible in the summertime and we were

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there in the middle of winter. So you can

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see, um, at least two stars of something

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called the summer triangle. The summer

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triangle is Vega, Altair, and

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the brightest star in Cygnus, which is,

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um, Deneb. Deneb. Vega

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and Altair. Vega and Deneb were very,

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very visible, uh, in

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midwinter, uh, near the north pole

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because the pole of the sky

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is tilted upwards so you can see things that

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from kind of middle latitudes you'd only see

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in summer. Uh, so what it meant was. Yes,

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your question is well made. Uh, we certainly

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saw Venus, Jupiter and Mars very

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clearly, probably Saturn, although it was

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quite near the horizon then. And I don't

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think we got a glimpse of Mercury. So that

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parade of planets that really, uh, occupied

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the media, uh, for us in the southern

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hemisphere, it was actually best back in

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January.

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Andrew Dunkley: Yeah.

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Professor Fred Watson: Uh, it's, uh, it's only in the north that

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it's been a hot topic within the last few

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days.

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Andrew Dunkley: The reason I ask is it's been in the news

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again because they said that, uh, well,

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the popular press is saying, oh, you know,

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the big alignment first time. Yeah, last time

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we'll see it in 60 years, blah, blah. Um,

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Jonti has a particular problem with the way

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the media.

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Professor Fred Watson: Yeah.

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Andrew Dunkley: Spews this kind of information out and,

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you know, don't let the truth get in the way

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of good story type of attitude.

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Professor Fred Watson: That's right.

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Andrew Dunkley: Um, but it was,

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uh, apparently it was the whole set

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at the end of February because Mercury was

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part of the deal then.

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Professor Fred Watson: From the Northern hemisphere.

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Andrew Dunkley: Yeah. Well, there you go. And um,

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Yeah, I was just wondering if you got a

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chance to spot it.

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Professor Fred Watson: But, uh, no, didn't see Mercury.

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Andrew Dunkley: No, I didn't see any of it much.

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Professor Fred Watson: Okay.

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Andrew Dunkley: I did go out and look, but where I am in

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town, it's. It's a really bad position and

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I'd have to, uh, go out and find a hill and

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as you know, there are not that many of them

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around here.

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Professor Fred Watson: No, no. You're a bit, uh, a bit low on hills

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up there. You need somebody to come and build

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one for you.

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Andrew Dunkley: Yeah, yeah. Or just cut all the trees

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down and.

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Professor Fred Watson: Oh, is that too. But that's not a good idea.

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Andrew Dunkley: No, not really.

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Professor Fred Watson: No.

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Andrew Dunkley: Okay.

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All right. Uh, let's get onto Our first

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official story and this one is very

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exciting and again getting a lot of

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press and that's been the successful landing

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of the Blue Ghost Lunar

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lander on the moon. Uh, this

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is a lot different to what we were

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witnessing in the 60s and 70s and a

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few of the more recent missions because they

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were um, publicly

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funded and um, government gazetted and all

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that jazz. This is a completely different

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kettle of.

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Professor Fred Watson: Fish indeed because it

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is a commercial spaceflight, it's a

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commercial company, uh, with the lovely name

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of Firefly Aerospace. Uh, their Blue

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Ghost lander is named after a rare species

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of Firefly, uh, which is found in the

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Appalachian area of the United States.

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I uh, love the name of the mission. It's not

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Apollo or Artemis or anything. It's called

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Ghost Riders in the Sky.

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Andrew Dunkley: I love it.

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Professor Fred Watson: Uh, and we did see, uh, earlier in the week

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before the spacecraft landed successfully,

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which it did on uh, March 2, uh,

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Eastern Standard Time, Sunday

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at the weekend. The weekend just gone. Uh, we

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did see some images during the week from the

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navigation cameras which uh, showed the Earth

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and the moon as uh, the lander flew

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by. But the reason why this lander is going

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to the moon or has gone to the moon is that

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it's part of uh, something you and I have

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Talked about, Andrew. NASA's Commercial Lunar

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Payload Services program,

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CLPS Commercial Commercial Lunar

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Payload, uh, which basically is NASA

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contracting to private companies,

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uh, for payloads to go to the

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lunar surface, uh, either experiments

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or um, you know, I suppose they, they're

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all experiments or at least uh, things that

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test the technology, uh, uh,

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basically to check things out before the

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Artemis mission really gets underway with

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a lunar landing. We hope that

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Artemis will see humans walking on the

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moon. 2027 I

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think is the current date. Uh, but

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that could change because all sorts of things

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are happening, uh, inside NASA, which we

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really didn't expect. Um, anyway, uh,

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the Launch was on the 15th of January, so

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it's taken a little while to get there.

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It uh,

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um, the spacecraft rode into orbit on a

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Falcon 9, a SpaceX Falcon 9, uh,

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and essentially uh, having gone into

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lunar orbit, uh, earlier in February,

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13th of February, it was

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descended or sent, um, a

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command to descend to the lunar

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surface on the 1st of March and successfully

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touched down on the 2nd. So really great

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stuff. Fantastic news that a, uh,

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commercial spaceflight has landed

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successfully on the moon.

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Andrew Dunkley: Yes, it is marvelous and

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um, it's a very short mission though, isn't

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it? They're not going to be doing much for

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long from what I understand.

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Professor Fred Watson: I think that's Right. I think the, the, you

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know, the essential part was just

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demonstrating that they can get there.

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Andrew Dunkley: Yeah.

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Professor Fred Watson: Uh, which they've now done very

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successfully. Um, it's, uh,

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it's. I think it's, uh,

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as you said, it's a short mission. Uh, I

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think it's one of these things that will only

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last for a lunar day. I need to check that.

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But it's that sort of time.

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Uh, it's easy to find some really nice

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pictures of, uh, what

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the sky would look like for Blue

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Ghost. Uh, there's a very nice picture on

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X of a gentleman by the name of

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Buzz Aldrin watching the landing. Yes.

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Andrew Dunkley: Yeah. He sent them a message of

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congratulations.

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Professor Fred Watson: Yes. Yeah. Uh, which is great. And, you

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know, who better to send a

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congratulations to a, um, like

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that than Buzz Aldrin, the second man to walk

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on the moon.

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Andrew Dunkley: Absolutely. Yes. And I, uh, think I've

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mentioned before I've had the great pleasure

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of meeting and interviewing him in my radio

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career. So that was one of the big highlights

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for me.

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Professor Fred Watson: Uh, and one of the highlights for me was

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having dinner with him.

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Andrew Dunkley: Oh, uh, that's even better. Yeah.

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Professor Fred Watson: Yeah, it was really interesting. We'll talk

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about that some of the time. It was a very

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interesting meeting, but it was very

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stimulating. This is probably a decade ago.

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Yeah, yeah.

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Andrew Dunkley: Great.

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Professor Fred Watson: Great company, as you know.

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Andrew Dunkley: Yeah.

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I, I notice, uh, in one of the stories, I

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think it's in sky and telescope,

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uh.org they they refer to

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the, uh, descent orbit insertion

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as nine minutes of terror.

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Professor Fred Watson: Yes.

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Andrew Dunkley: But we've talked about these terrifying

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landings on other worlds, particularly

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Mars. I wouldn't have thought that it would

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be as big a deal on the moon, given that

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this, you know, no atmosphere of.

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Professor Fred Watson: You're right. Yeah. And you're

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absolutely right because, um, you know, if

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you're landing on Mars, a lot of the, uh,

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trajectory is dictated not just by, uh,

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orbital mechanics, which is how things work

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in space, but dictated by the vagaries of

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the atmosphere. If you've got slightly higher

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pressure than you expected, you've got more

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braking force, and suddenly, uh, your

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spacecraft is heading for a different part of

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the surface at a higher speed than you would

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want or lower speed or whatever. Um, and

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you're right that, um, in the case of the

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Moon, it's all about orbital mechanics, which

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are very, very predictable. But you can

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imagine, you know, you've got to fire those

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thrusters at just the right moment to break

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it so that when it lands on the moon, it

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doesn't land too hard and smash up on the

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rocks or basically bounce off and then

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smash up. You've got to get things just

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right. So nine minutes of terror. I can

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sympathize with that. I think I'd feel like

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that too.

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Andrew Dunkley: Well, when you're talking about breaking from

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3,800 miles an hour to 90 miles an

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hour. Yes, that, that would be,

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that would be terrifying if, um, you know,

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you push the wrong button.

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And I think I had to smile when I read

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the story because they, they said successful,

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uh, landing and upright.

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So I think, I think they were

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sort of saying, well, you know, even if it

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lands on its side, that's a success. But it's

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even better that it's standing.

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Professor Fred Watson: It was last year, wasn't it, that one of the

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spacecraft did land on its side? That's

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right.

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Andrew Dunkley: I think it was the Indian mission.

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Professor Fred Watson: Was it, Was it Indian or Japanese? I can't

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remember. Um, but yeah. So it was landed in

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such a way that the solar panels weren't

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seeing the sun.

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Andrew Dunkley: Yes, that's right.

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Professor Fred Watson: So, yes, it's very important to have it the

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right way up.

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Andrew Dunkley: Yeah. Anyway, we wish them well. It'll be a

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quick visit and it

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paves the way for Artemis too. We still don't

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know when that's going to happen. Seems to be

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getting pushed back time and time again. But

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they will get there eventually.

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Professor Fred Watson: I'm sure they will.

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Andrew Dunkley: One will hope.

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Generic: Roger, you're allowed to start here also

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space nuts.

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Andrew Dunkley: Now, while we're talking about these kinds

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of, uh, commercial missions, there's another

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one that's in the news. This is a private

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mission, uh, that was heading out past

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the moon to the Odin asteroid, the

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um, private Odin asteroid probe.

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All was looking nominal

324
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until recently. Things seem to have gone

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awry somewhat.

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Professor Fred Watson: Yes, the uh, the comment

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that perhaps highlights the situation comes

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from, uh, uh, somebody by the name of

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Matthew Gialish, I think it is, who is the co

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founder and CEO of AstroDailyPod Forge, which

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is the, um, the organization that

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is operating the Odin

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spacecraft. Uh, what he said

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on Friday, uh, the 28th of February

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was we don't fully understand the state of

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the vehicle. Uh, it's

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thought still though, to be in a mode that

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means it's not being fried by the light of

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the sun. It's in an attitude

340
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in regard to the sun

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that will not have

342
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parts of it being unduly heated, although,

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uh, we believe that it is tumbling.

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Um, and uh, you know, uh, this is

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not a good thing for a spacecraft, um,

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uh, to experience.

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That's one of two alternatives which I think

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are still valid, Andrew. One is that the

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spacecraft is tumbling, uh, which is not

350
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nice, uh, or the other is that everything's

351
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fine, but there are issues with the telemetry

352
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back on Earth, their ground receivers not

353
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being properly configured or whatever. So

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they're still basically worrying about

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what's. What's going on. We should check that

356
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story again, perhaps next week.

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Andrew Dunkley: What's the goal of the mission? They're going

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to visit an asteroid. But what do they want

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to do with it?

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Professor Fred Watson: Basically check it out, uh, to

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send imagery, uh, of,

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uh, an asteroid which rejoices in the name of

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2022 OB5. Uh,

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and, um, it's a

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possible first step

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in basically

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recovering resources from a space

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object. In other words, asteroid mining. Wow.

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So if this mission was successful, and

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we're not sure that that's the case at the

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moment, um, this mission is

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basically designed to focus,

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uh, the cameras, uh, on

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that asteroid 2022 OB5,

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in order to get a

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survey of the surface, see what's there, take

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lots of images, use, um, the filters in the

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cameras to get some idea of the surface

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texture and things of that sort, which you

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can do, particularly in the infrared wave

381
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band. But that's a precursor, uh, to a second

382
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mission. This mission's called odin. The

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second mission is called Vestri, which will

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aim to land on the asteroid. So that's

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perhaps the more ambitious one that we

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will be looking at down the track. Assuming

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that Odin, uh, pulls it off or Space

388
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Forge pulls it off, as far as odin's

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concerned.

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Andrew Dunkley: Yeah, uh, well, fingers crossed. Um,

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I think this quote from Matt Gillick,

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uh, who you quoted earlier, says it

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all. I think we all know the hope is fading

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as we continue the mission.

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Professor Fred Watson: Yeah, um, I mean, it's what

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we've always said. Space is hard.

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Andrew Dunkley: It's tough out there. Yeah, yeah, it's, uh,

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it's a difficult gig. But they keep on

399
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trying. And, uh, you know, not all missions

400
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are absolute failures. Even when they don't

401
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go well, there's something to learn, and

402
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there's always something to learn.

403
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Professor Fred Watson: That's right.

404
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Andrew Dunkley: It's better next time. Yes, indeed.

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And you, uh, can read about that story if you

406
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like@spare.com. this is

407
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Space Nets with Andrew Dunkley and Professor

408
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Fred Watson.

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Okay, we checked all four systems and team

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with a Go Space Net.

411
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Okay, Fred, let's, uh, head towards

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Andromeda. Or is it heading towards us?

413
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Either way, uh, we. We've

414
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had a few questions recently with Jonti about

415
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Andromeda, and he was, um. Yeah, uh, he had a

416
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lot to say about it. Uh, and one of the

417
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questions we got recently was is the

418
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Milky Way already affecting

419
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Andromeda? And you know, to

420
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a certain degree, not a massive amount. The

421
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answer is yes, according to Jonti. Uh,

422
00:16:39.130 --> 00:16:42.062
but uh, we don't have to do that because it's

423
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now been discovered that Andromeda's um,

424
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being picked on by some little

425
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cousins nearby. It's already

426
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getting ah, a bit of a dust up, so to

427
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speak.

428
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Professor Fred Watson: It may. Yeah. So this may be the

429
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results of something bigger, something

430
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that we probably need to know about as well.

431
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Um, the bottom

432
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line here is you're quite right. Uh,

433
00:17:08.420 --> 00:17:11.292
the Andromeda galaxy, we can see, we see

434
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it in the constellation of Andromeda,

435
00:17:13.068 --> 00:17:15.948
obviously, uh, at a distance of about 2 1/2

436
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million light years, uh, like the

437
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Earth. Sorry, let me

438
00:17:21.588 --> 00:17:24.200
rephrase that. Like the Milky Way,

439
00:17:24.900 --> 00:17:27.804
our own galaxy, um, it's surrounded

440
00:17:27.852 --> 00:17:30.092
by a uh, swarm of dwarf

441
00:17:30.156 --> 00:17:32.732
galaxies. In fact about

442
00:17:32.916 --> 00:17:35.200
three or four dozen of them altogether.

443
00:17:35.470 --> 00:17:37.830
Um, it's uh, it is,

444
00:17:37.870 --> 00:17:40.762
uh, those dwarf galaxies, we call

445
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them satellite galaxies because they are

446
00:17:42.466 --> 00:17:45.258
satellites of Andromeda, uh, have

447
00:17:45.314 --> 00:17:48.234
been analyzed to death, uh, in a,

448
00:17:48.322 --> 00:17:51.082
in you know, some new research that's been

449
00:17:51.106 --> 00:17:53.299
carried out using the Hubble Space TeleScope

450
00:17:53.416 --> 00:17:56.250
still, after 35 years, still doing

451
00:17:56.290 --> 00:17:59.258
a very, very fine job in giving us

452
00:17:59.394 --> 00:18:02.272
spectra and images of distant objects.

453
00:18:02.336 --> 00:18:05.216
So uh, the researchers have used the Hubble,

454
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uh, essentially to map the motion

455
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of these dwarf galaxies, which is an

456
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extraordinary thing to be able to do, um,

457
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and look at their

458
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position in three dimensions around the

459
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uh, Andromeda galaxy. Uh,

460
00:18:20.960 --> 00:18:23.320
and it's comparing uh,

461
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what they found with what we know from

462
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the dwarf galaxies that orbit our own. And

463
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it's is probably a similar sort of number.

464
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It's about two dozen, I think, satellite uh,

465
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galaxies that we have. The biggest two are

466
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the Large and Small Magellanic Clouds. Uh,

467
00:18:38.860 --> 00:18:41.320
so you take all that, um,

468
00:18:41.760 --> 00:18:43.716
uh, you build a map of where these galaxies

469
00:18:43.748 --> 00:18:45.972
are around Andromeda and you find that

470
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they're in quite different orientations

471
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from what we find in our own

472
00:18:51.580 --> 00:18:54.452
galaxy. Um, uh, one

473
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of the comments, uh, in

474
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this story, uh, and this is uh, coming

475
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from uh, some of the researchers in fact, uh,

476
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Daniel Weiss of the University of

477
00:19:05.446 --> 00:19:08.260
California at Berkeley, uh,

478
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has basically pointed out

479
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that something significant has happened to

480
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Andromeda to change the

481
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distribution of the satellite galaxies.

482
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Um, because half of them, uh,

483
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rather than sort of swarming around, uh,

484
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like you know, moths around a flame, half

485
00:19:28.390 --> 00:19:31.090
of these galaxies are actually in a plane.

486
00:19:31.300 --> 00:19:33.470
Uh, you know, they're

487
00:19:33.630 --> 00:19:36.414
basically in, in one plane. Of

488
00:19:36.502 --> 00:19:39.294
the space around, uh, around Andromeda, and

489
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they're all going in the same direction. And

490
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that is, uh, as, um, as

491
00:19:44.326 --> 00:19:46.770
Daniel Weiss says, that is weird.

492
00:19:47.060 --> 00:19:49.766
Um, he says it was actually a total

493
00:19:49.838 --> 00:19:51.702
surprise to find the satellites in that

494
00:19:51.726 --> 00:19:53.446
configuration. And we still don't fully

495
00:19:53.478 --> 00:19:56.210
understand why they appear that way.

496
00:19:56.750 --> 00:19:59.330
Another colleague, uh, says,

497
00:19:59.690 --> 00:20:01.782
um, this uh, is Alessandro

498
00:20:01.846 --> 00:20:04.838
Savino, says it is clear,

499
00:20:04.974 --> 00:20:07.734
it's a clear indication of how small galaxy

500
00:20:07.782 --> 00:20:10.742
growth is disturbed by the influence of

501
00:20:10.766 --> 00:20:13.290
a massive galaxy like Andromeda.

502
00:20:13.510 --> 00:20:16.446
Um, and I think the, the bottom

503
00:20:16.478 --> 00:20:19.410
line here is that they've got much, um,

504
00:20:20.134 --> 00:20:22.910
younger, uh, stars in them.

505
00:20:22.950 --> 00:20:25.758
These dwarf galaxies, uh, form

506
00:20:25.814 --> 00:20:28.334
their stars very early on in the history of

507
00:20:28.342 --> 00:20:29.918
the Andromeda galaxy, which probably goes

508
00:20:29.934 --> 00:20:32.862
back 12 or 13 billion years, um, and

509
00:20:32.886 --> 00:20:35.870
then kept on. And uh, the

510
00:20:35.990 --> 00:20:38.650
idea is that the,

511
00:20:39.430 --> 00:20:42.280
the perhaps. And they say that they

512
00:20:42.320 --> 00:20:44.200
really don't know what's happening, but

513
00:20:44.240 --> 00:20:46.664
perhaps there was a collision between

514
00:20:46.752 --> 00:20:49.740
Andromeda and another galaxy,

515
00:20:49.870 --> 00:20:52.408
uh, some billions of years ago, which

516
00:20:52.464 --> 00:20:55.048
caused this peculiarity

517
00:20:55.224 --> 00:20:58.024
of the, uh, of the, of the dwarf galaxies

518
00:20:58.072 --> 00:21:00.920
surrounding Andromeda. Everything about it is

519
00:21:00.960 --> 00:21:03.832
weird, including my, um, my account of it.

520
00:21:03.856 --> 00:21:04.420
Andrew Dunkley: Just

521
00:21:06.210 --> 00:21:08.832
uh. So they're saying it's weird. They say

522
00:21:08.856 --> 00:21:11.152
they don't really know what happened, but it

523
00:21:11.176 --> 00:21:14.144
would have to be some kind of gravitational

524
00:21:14.272 --> 00:21:16.096
effect or interference, wouldn't it?

525
00:21:16.168 --> 00:21:18.224
Professor Fred Watson: Yeah, I think you're absolutely right. And I

526
00:21:18.232 --> 00:21:20.272
think that's probably what they're looking

527
00:21:20.296 --> 00:21:22.192
at, you know, as they try to understand how

528
00:21:22.216 --> 00:21:24.688
you can end up with a, uh, with a set

529
00:21:24.744 --> 00:21:27.680
of, uh, something like 15 or

530
00:21:27.720 --> 00:21:30.304
20 dwarf galaxies, all of which lie in a

531
00:21:30.312 --> 00:21:31.952
single plane that flies in the face of

532
00:21:31.976 --> 00:21:33.936
everything we understand about dwarf galaxy

533
00:21:33.968 --> 00:21:36.702
formation, um, and certainly

534
00:21:36.766 --> 00:21:38.542
is very different from what we find in our

535
00:21:38.566 --> 00:21:40.046
own Milky Way galaxy.

536
00:21:40.158 --> 00:21:42.238
Andrew Dunkley: And from what I can tell, they've tried to

537
00:21:42.294 --> 00:21:44.558
figure this out using computer simulations

538
00:21:44.574 --> 00:21:45.918
and it didn't work.

539
00:21:46.054 --> 00:21:48.942
Professor Fred Watson: Yeah, yeah, yeah. So there you go.

540
00:21:48.966 --> 00:21:51.502
And uh, that's just basically telling you

541
00:21:51.526 --> 00:21:54.062
that you need to put something else into the

542
00:21:54.086 --> 00:21:55.998
simulation and maybe it is a collision with

543
00:21:56.054 --> 00:21:58.398
another large galaxy, something else that's

544
00:21:58.414 --> 00:22:00.770
not in there already, to try and, uh,

545
00:22:00.770 --> 00:22:03.370
replicate what we see in the real world.

546
00:22:03.490 --> 00:22:05.514
Andrew Dunkley: So could that mean that if there was a

547
00:22:05.522 --> 00:22:07.882
collision with another large galaxy, that the

548
00:22:07.906 --> 00:22:09.530
result is Andromeda?

549
00:22:09.690 --> 00:22:12.170
Professor Fred Watson: Yes, that's. I think what you'd have to agree

550
00:22:12.210 --> 00:22:14.370
with that. Um,

551
00:22:15.490 --> 00:22:18.202
it, it's not been a, I mean the

552
00:22:18.226 --> 00:22:20.538
collision between Andromeda and the Milky

553
00:22:20.554 --> 00:22:22.602
Way, when it happens in three and a half

554
00:22:22.626 --> 00:22:24.762
billion years or whenever it says in the

555
00:22:24.786 --> 00:22:27.596
diary that that's going to happen. Uh, it's,

556
00:22:27.708 --> 00:22:30.524
that changes the shape of both of them.

557
00:22:30.600 --> 00:22:33.292
Uh, it basically you get a collision. All the

558
00:22:33.396 --> 00:22:36.140
shockwaves, gravitational shock waves,

559
00:22:36.300 --> 00:22:38.732
cause formation of

560
00:22:38.756 --> 00:22:40.720
supernovae. Basically, uh,

561
00:22:41.388 --> 00:22:44.284
form really big stars which last only a

562
00:22:44.292 --> 00:22:46.652
short time, then explode as supernovae. That

563
00:22:46.676 --> 00:22:49.196
uses up all the gas, uh, in the

564
00:22:49.268 --> 00:22:51.960
galaxies and you end up with what we call

565
00:22:52.560 --> 00:22:54.888
Milkomeda, the Milky Way

566
00:22:54.944 --> 00:22:57.180
Andromeda combination, which looks more like

567
00:22:57.180 --> 00:22:59.064
uh, what we call an elliptical galaxy. A

568
00:22:59.072 --> 00:23:01.960
galaxy with no, um, no gas, no

569
00:23:02.000 --> 00:23:04.904
star formation. Uh, and Andromeda

570
00:23:04.952 --> 00:23:07.816
now is not like that at all. It's a actively

571
00:23:07.848 --> 00:23:10.072
star forming galaxy. So the suggestion is

572
00:23:10.096 --> 00:23:12.392
that maybe it was a smaller object that

573
00:23:12.416 --> 00:23:14.424
caused this disruption to the satellite

574
00:23:14.472 --> 00:23:15.192
galaxies.

575
00:23:15.336 --> 00:23:18.072
Andrew Dunkley: It's. Is it classified as a spiral

576
00:23:18.136 --> 00:23:18.866
galaxy?

577
00:23:19.008 --> 00:23:21.598
Professor Fred Watson: Yes, it's a, it's a spiral definitely.

578
00:23:21.694 --> 00:23:24.622
Andrew Dunkley: Okay. Um, and so is ours. But when they

579
00:23:24.646 --> 00:23:26.494
get together they're just going to be boring.

580
00:23:26.622 --> 00:23:28.302
Professor Fred Watson: Yeah, they will, they'll be shaped like a

581
00:23:28.326 --> 00:23:30.974
football, uh, with no spiral arms.

582
00:23:31.102 --> 00:23:32.942
Nothing happening, nothing to see here.

583
00:23:33.046 --> 00:23:35.230
Andrew Dunkley: Yeah. Ah, it's a bit sad really.

584
00:23:35.270 --> 00:23:37.342
Professor Fred Watson: I mean because they're both pretty smart

585
00:23:37.406 --> 00:23:38.330
looking now.

586
00:23:39.190 --> 00:23:41.750
Andrew Dunkley: What a pity. Oh well, um,

587
00:23:42.150 --> 00:23:44.702
you know, we can't stop it. We'll just have

588
00:23:44.726 --> 00:23:47.122
to put up with it when the time comes. How

589
00:23:47.146 --> 00:23:48.770
long? Three and a half billion.

590
00:23:48.890 --> 00:23:50.882
Professor Fred Watson: Yeah, yeah, it's um, something to look

591
00:23:50.906 --> 00:23:52.754
forward to, you know, with trepidation

592
00:23:52.802 --> 00:23:53.170
perhaps.

593
00:23:53.250 --> 00:23:56.114
Andrew Dunkley: Yes, eventually. All right, uh, that story

594
00:23:56.202 --> 00:23:58.642
is uh, uh, at Cosmos

595
00:23:58.706 --> 00:24:01.602
magazine dot com if you'd like to read up on

596
00:24:01.626 --> 00:24:02.430
that one.

597
00:24:04.970 --> 00:24:07.602
Generic: Three, two, one.

598
00:24:07.786 --> 00:24:09.270
Space nuts.

599
00:24:09.610 --> 00:24:12.108
Andrew Dunkley: Uh, Fred, let's uh, go and visit an old

600
00:24:12.164 --> 00:24:14.316
friend, uh, someone who we thought had

601
00:24:14.388 --> 00:24:16.572
stopped writing to us. We don't know what we

602
00:24:16.596 --> 00:24:19.420
did wrong, but they have reached out to say

603
00:24:19.460 --> 00:24:21.836
hello. I'm still here. I'm alive again.

604
00:24:21.988 --> 00:24:23.324
Voyager 1.

605
00:24:23.492 --> 00:24:25.870
Professor Fred Watson: Yeah, that's right, uh,

606
00:24:25.870 --> 00:24:28.476
20. I looked it up the other day.

607
00:24:28.548 --> 00:24:29.926
25,

608
00:24:30.233 --> 00:24:32.924
is that right? Yeah, no, 20.

609
00:24:33.012 --> 00:24:35.560
About 27 billion kilometers away.

610
00:24:36.500 --> 00:24:39.308
And the most distant human made

611
00:24:39.364 --> 00:24:42.076
object. I uh, think it's

612
00:24:42.108 --> 00:24:45.084
got uh, 22.5

613
00:24:45.252 --> 00:24:47.852
light hours of travel time for the

614
00:24:47.876 --> 00:24:50.180
commands. Um,

615
00:24:50.260 --> 00:24:53.228
so the. What the.

616
00:24:53.364 --> 00:24:56.120
Basically the story goes back in fact to

617
00:24:56.460 --> 00:24:59.340
uh, the 20. I uh, think.

618
00:24:59.380 --> 00:25:00.908
I can't remember what date it was, but it's

619
00:25:00.924 --> 00:25:03.500
back in November 2023. So it's

620
00:25:03.500 --> 00:25:06.130
um, you know, well over a year ago,

621
00:25:06.460 --> 00:25:09.446
uh, that um, the transmission started

622
00:25:09.518 --> 00:25:11.814
coming through in a gobbledygook

623
00:25:11.862 --> 00:25:14.290
format. Uh, and

624
00:25:14.590 --> 00:25:16.930
there was, I think an issue

625
00:25:17.230 --> 00:25:19.558
with one of the memory

626
00:25:19.654 --> 00:25:22.130
chips. Um, and

627
00:25:22.750 --> 00:25:25.510
you know, there was work done on

628
00:25:25.630 --> 00:25:28.598
trying to fix that, uh, which

629
00:25:28.734 --> 00:25:31.490
basically I think took Five months or so.

630
00:25:31.740 --> 00:25:34.502
Uh, and then, uh, was

631
00:25:34.526 --> 00:25:37.250
it in April 2024,

632
00:25:37.760 --> 00:25:40.214
uh there was uh, a

633
00:25:40.302 --> 00:25:42.854
successful uh, receipt

634
00:25:42.982 --> 00:25:45.010
of data,

635
00:25:45.480 --> 00:25:48.130
um, and that the

636
00:25:48.750 --> 00:25:50.822
machine was sending back things that you

637
00:25:50.846 --> 00:25:52.070
could actually read rather than just

638
00:25:52.110 --> 00:25:54.854
gobbledygook. So that was back in

639
00:25:54.942 --> 00:25:56.930
April 2024.

640
00:25:57.950 --> 00:26:00.614
But I think there's been another loss

641
00:26:00.702 --> 00:26:03.118
since then. Uh, and

642
00:26:03.254 --> 00:26:05.970
the you know, the um,

643
00:26:05.970 --> 00:26:08.890
difficulties that Voyager 1 has are

644
00:26:08.890 --> 00:26:11.420
uh, to some extent ongoing. Um,

645
00:26:11.750 --> 00:26:14.478
but uh, there is, you know, it's good news

646
00:26:14.534 --> 00:26:17.454
that uh, uh, at least we are

647
00:26:17.542 --> 00:26:19.758
still in some sort of communication with

648
00:26:19.814 --> 00:26:22.654
Voyager 1 and hopefully there's

649
00:26:22.702 --> 00:26:25.130
still potential for intelligible uh,

650
00:26:25.822 --> 00:26:28.590
signals to come back. The, the really

651
00:26:28.630 --> 00:26:30.718
interesting thing I guess is the, the power

652
00:26:30.774 --> 00:26:33.394
supply which is the radioisotope thermoele

653
00:26:33.502 --> 00:26:36.154
generator, which is now delivering a tiny

654
00:26:36.202 --> 00:26:38.314
fraction of what it delivered right at the

655
00:26:38.322 --> 00:26:40.922
beginning of the mission in the late 1970s.

656
00:26:41.066 --> 00:26:43.786
And so we've got uh, an issue

657
00:26:43.858 --> 00:26:46.506
there. And what NASA has done is switched off

658
00:26:46.658 --> 00:26:49.482
various instruments progressively so

659
00:26:49.506 --> 00:26:51.562
that things like the magnetometers that we

660
00:26:51.586 --> 00:26:53.290
call the magnetic field and things like that,

661
00:26:53.330 --> 00:26:55.674
I think they are now switched off so that

662
00:26:55.682 --> 00:26:58.234
you're saving power just for

663
00:26:58.402 --> 00:27:00.314
pointing the antenna, which is done by the

664
00:27:00.322 --> 00:27:03.082
spacecraft's thrusters and essentially

665
00:27:03.146 --> 00:27:05.318
sending signals backwards and forwards.

666
00:27:05.514 --> 00:27:07.998
Andrew Dunkley: Yeah, it's uh, it's quite remarkable though

667
00:27:08.054 --> 00:27:10.958
after all these decades that

668
00:27:11.014 --> 00:27:13.342
it's still going, we still communicate with

669
00:27:13.366 --> 00:27:15.930
it, we can still send it information.

670
00:27:16.230 --> 00:27:16.942
Professor Fred Watson: Yes.

671
00:27:17.086 --> 00:27:19.886
Andrew Dunkley: And um, of course Voyager 2 is

672
00:27:19.958 --> 00:27:22.238
still out there and still going strong,

673
00:27:22.294 --> 00:27:25.246
although it too has had some issues. Although

674
00:27:25.358 --> 00:27:28.270
I think um, the most

675
00:27:28.310 --> 00:27:30.724
recent big issue with Voyager 2 was July

676
00:27:30.848 --> 00:27:33.604
2023 when a series of commands was sent

677
00:27:33.742 --> 00:27:35.880
to the spacecraft, causing its

678
00:27:35.920 --> 00:27:38.792
antenna to point away from Earth. I think

679
00:27:38.816 --> 00:27:39.848
we did talk about that.

680
00:27:39.904 --> 00:27:41.240
Professor Fred Watson: We did talk about it. That's right.

681
00:27:41.280 --> 00:27:43.432
Andrew Dunkley: And it stopped the uh, spacecraft from

682
00:27:43.456 --> 00:27:46.040
receiving commands or sending data back to

683
00:27:46.160 --> 00:27:48.760
Earth. And I

684
00:27:48.880 --> 00:27:51.544
think they managed to somehow

685
00:27:51.592 --> 00:27:54.504
circumvent that. Um, I,

686
00:27:54.592 --> 00:27:57.336
I, I believe it involved the Canberra deep

687
00:27:57.368 --> 00:27:59.032
space complex.

688
00:27:59.096 --> 00:28:01.072
Professor Fred Watson: Yeah, I was just going to mention that. In

689
00:28:01.096 --> 00:28:03.376
fact it must have done because that Canberra

690
00:28:03.408 --> 00:28:06.128
deep space complex, uh, the Tidbin

691
00:28:06.144 --> 00:28:09.120
Billa dish, as we call it in the trade, uh,

692
00:28:09.120 --> 00:28:12.020
is uh, the only uh, antenna um,

693
00:28:12.368 --> 00:28:14.480
on Earth that can actually communicate with

694
00:28:14.520 --> 00:28:17.056
Voyager 2. And that's because Voyager

695
00:28:17.088 --> 00:28:19.184
2's at a latitude, if I remember rightly.

696
00:28:19.232 --> 00:28:22.112
It's about 66 degrees below

697
00:28:22.216 --> 00:28:24.704
the equator in terms of the direction it's

698
00:28:24.752 --> 00:28:27.632
going out to, which makes it invisible to

699
00:28:27.656 --> 00:28:30.544
the other two, uh, stations in the Deep

700
00:28:30.592 --> 00:28:33.276
Space, uh, network, which are in Madrid and

701
00:28:33.290 --> 00:28:36.172
uh, Goldstone in California. So, uh, yes,

702
00:28:36.236 --> 00:28:38.956
only, uh, only Tidbinbilla can see Voyager

703
00:28:38.988 --> 00:28:39.420
2.

704
00:28:39.540 --> 00:28:41.740
Andrew Dunkley: Yeah, and that's how they saved it. They

705
00:28:41.780 --> 00:28:43.468
picked up a very faint signal.

706
00:28:43.564 --> 00:28:44.108
Professor Fred Watson: That's right.

707
00:28:44.164 --> 00:28:46.924
Andrew Dunkley: NASA was able to transmit some corrective

708
00:28:46.972 --> 00:28:49.500
data like, uh, to

709
00:28:49.540 --> 00:28:52.300
Voyager 2 and got it back online, which

710
00:28:52.340 --> 00:28:55.116
was very good news. Uh, and Voyager

711
00:28:55.148 --> 00:28:57.020
1's now back with us. So they're both still

712
00:28:57.060 --> 00:28:59.462
going. They're both still talking to us. We

713
00:28:59.486 --> 00:28:59.766
did.

714
00:28:59.838 --> 00:29:00.502
Professor Fred Watson: Extraordinary.

715
00:29:00.566 --> 00:29:02.102
Andrew Dunkley: Yeah. We thought we'd offended both of them,

716
00:29:02.126 --> 00:29:04.838
but no, it's. It's all good. I mean, they've

717
00:29:04.854 --> 00:29:07.270
been alone for so long. I can understand them

718
00:29:07.310 --> 00:29:08.278
being a bit grumpy.

719
00:29:08.374 --> 00:29:11.270
Professor Fred Watson: Yeah. They might

720
00:29:11.310 --> 00:29:13.718
like their own company though. M. They've

721
00:29:13.734 --> 00:29:15.318
both got music to listen to, so.

722
00:29:15.374 --> 00:29:16.854
Andrew Dunkley: Going different ways, aren't they?

723
00:29:16.942 --> 00:29:19.158
Professor Fred Watson: Yes, they are. That's the thing. Uh, Voyager

724
00:29:19.174 --> 00:29:21.190
2 is heading much more to the south than

725
00:29:21.230 --> 00:29:22.038
Voyager 1 is.

726
00:29:22.094 --> 00:29:24.130
Andrew Dunkley: Yeah. M. It's such

727
00:29:24.520 --> 00:29:27.520
amazing. An amazing story for

728
00:29:27.560 --> 00:29:30.288
both of them, too. I mean, how

729
00:29:30.344 --> 00:29:32.528
far past end of mission have they survived?

730
00:29:32.624 --> 00:29:34.768
That's extraordinary.

731
00:29:34.864 --> 00:29:37.728
Professor Fred Watson: Yeah. Decades. It is, it is. It's

732
00:29:37.744 --> 00:29:40.192
fantastic. And they, you know, eventually

733
00:29:40.256 --> 00:29:42.610
their batteries will run out. Those, uh,

734
00:29:42.610 --> 00:29:44.624
radioisotope thermal thermoelectric

735
00:29:44.672 --> 00:29:47.216
generators will fizzle out so that they can't

736
00:29:47.248 --> 00:29:49.872
even send power to the, uh, to the

737
00:29:49.896 --> 00:29:52.550
transmitters. But the spacecraft will keep on

738
00:29:52.590 --> 00:29:54.050
going because they are

739
00:29:55.470 --> 00:29:57.462
orbital mechanics. Maybe for billions of

740
00:29:57.486 --> 00:29:58.694
years. We just don't know.

741
00:29:58.782 --> 00:30:01.126
Andrew Dunkley: Yes. Until someone catches them in a Venus

742
00:30:01.158 --> 00:30:04.086
fly trap on some other planet and it's

743
00:30:04.118 --> 00:30:05.670
all over Red Rover. Who knows?

744
00:30:05.750 --> 00:30:06.310
Professor Fred Watson: Who knows?

745
00:30:06.390 --> 00:30:09.254
Andrew Dunkley: Yeah, Great, uh, story about Voyager 1. You

746
00:30:09.262 --> 00:30:11.734
can, um, find that online. There's quite a

747
00:30:11.742 --> 00:30:13.654
few news stories about it.

748
00:30:13.822 --> 00:30:16.422
Professor Fred Watson: Can I just, um, add one comment?

749
00:30:16.526 --> 00:30:19.090
So, the Canberra deep space communication

750
00:30:19.170 --> 00:30:21.890
complex is 60 years old this

751
00:30:21.930 --> 00:30:22.514
month.

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00:30:22.682 --> 00:30:23.218
Andrew Dunkley: Wow.

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00:30:23.314 --> 00:30:24.754
Professor Fred Watson: There you go. I should have, should have

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00:30:24.762 --> 00:30:27.410
remembered that. You did, yeah.

755
00:30:27.570 --> 00:30:29.682
Should have remembered it earlier. 60 years

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00:30:29.706 --> 00:30:30.610
old this month.

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00:30:30.730 --> 00:30:33.470
Andrew Dunkley: Yes. It took you 60 years to remember that?

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00:30:35.610 --> 00:30:38.386
All right, um, we are just about

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00:30:38.458 --> 00:30:40.178
done. Thanks, uh, for your company. Thank

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00:30:40.194 --> 00:30:42.290
you, Fred, as always. We'll wrap it up and

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00:30:42.330 --> 00:30:44.022
we'll catch you on the next episode.

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00:30:44.146 --> 00:30:46.910
Professor Fred Watson: That sounds wonderful. I'll look

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00:30:46.950 --> 00:30:47.726
forward to it.

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00:30:47.798 --> 00:30:49.406
Andrew Dunkley: All right, we'll see you then. Professor Fred

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00:30:49.438 --> 00:30:51.742
Watson, Astronomer at large. Don't forget to

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00:30:51.766 --> 00:30:53.614
visit us, uh, on our website. In the

767
00:30:53.622 --> 00:30:54.414
meantime, you can do

768
00:30:54.422 --> 00:30:57.118
that@spacenutspodcast.com or spacenuts

769
00:30:57.214 --> 00:30:59.838
IO all sorts of things to see and do and

770
00:30:59.894 --> 00:31:02.750
buy there. Um, more

771
00:31:02.790 --> 00:31:04.286
mainly Fred's books. But you know, there's

772
00:31:04.318 --> 00:31:06.750
other stuff as well. Some of it's even

773
00:31:06.790 --> 00:31:09.070
interesting. Oh, sorry. Um,

774
00:31:09.510 --> 00:31:11.630
some of it's not. And I think I wrote those

775
00:31:11.670 --> 00:31:14.478
books. Never mind. Ah, and thanks, uh, to

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00:31:14.534 --> 00:31:16.890
Huw in the studio, who couldn't be with us

777
00:31:16.930 --> 00:31:19.090
today because he was, um,

778
00:31:19.570 --> 00:31:22.474
stirring the pot around Andromeda, causing

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00:31:22.522 --> 00:31:25.290
all sorts of mayhem. Typical of you.

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00:31:25.410 --> 00:31:27.002
And from me, Andrew Dunkley, thanks for your

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00:31:27.026 --> 00:31:28.586
company. Catch you on the very next episode

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00:31:28.618 --> 00:31:30.670
of Space Nuts. Bye. Bye.

783
00:31:31.490 --> 00:31:33.706
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00:31:33.738 --> 00:31:36.730
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