March 5, 2026

Artemis Updates, The Brain Nebula & Mapping the Galactic Center

Artemis Updates, The Brain Nebula & Mapping the Galactic Center

Artemis Updates, the Brian Nebula, and Galactic Mapping In this enlightening episode of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson dive into the latest developments in space exploration and celestial phenomena. From the shifting...

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Artemis Updates, the Brian Nebula, and Galactic Mapping
In this enlightening episode of Space Nuts, hosts Andrew Dunkley and Professor Fred Watson dive into the latest developments in space exploration and celestial phenomena. From the shifting timelines of the Artemis program to the fascinating discoveries made by the James Webb Space Telescope, this episode is packed with cosmic insights and intriguing discussions.
Episode Highlights:
Artemis Program Updates: Andrew and Fred discuss the recent delays in the Artemis 2 mission, which is now expected to launch no earlier than April. They also explore the implications of the newly inserted Artemis 3 mission, which will focus on testing spacecraft capabilities in Earth orbit before the lunar landing.
The Brian in Space: The hosts delve into the discovery of the PMR1 nebula, also known as the Exposed Cranium Nebula. They discuss its unusual appearance and the significance of the James Webb Space Telescope's observations that reveal this nebula's intricate structure, reminiscent of a brain.
Mapping the Galactic Center: Andrew and Fred highlight a groundbreaking survey of the center of our galaxy, revealing the complex dynamics and chemical compositions within this turbulent region. They discuss the technologies used in this research and what it means for our understanding of the Milky Way.

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Stay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.

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WEBVTT

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Hi there, thanks for joining us again. This is Space Nuts.

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My name is Andrew Dunkley. It's great to have your company.

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We're going to talk about a lot of things today,

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and one of them is the Artemis program. Now, we

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did talk about it very recently because things had changed.

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The Artemis to launch was set back, and it looks

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like they're actually going to take the artemist to rocket

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back to the assembly building now and they're not anticipating

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an Artemis to launch to send humans around the Moon

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and back until at least April. But that's not what

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we're going to talk about. We'll explain that shortly. We're

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going to look at the new Ukrainium nebula. This one

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sounds quite unbelievable a brain in space could be and

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the center of our galaxy has been mapped in detail.

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What's it look like? We will tell you on this

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episode of Space.

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Nuts fifteen, Channel ten nine ignition sign Space Nuts NY

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or three.

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Two Space Nuts as when I reported Bill's good. Joining

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us once again is Professor Fred Watson, Astronomer at Large.

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Hi Fred, Hello Andrew. Good to see you back from

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your sod.

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Yes, yes, I won't dwell on it too much. I'm

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sure people have seen the photos on Facebook if they

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cared to look on my page. I didn't put them

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on the space nuts page. But yeah, we went to

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Borneo for a couple of weeks and we saw some

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amazing wildlife, orangutang sun bears, proboscous monkeys, civets. You know,

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you know about the civet They eat the coffee berry

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and pooh out the bean and then they collect the

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beans and turn them into coffee. Yeah, we saw some

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of those. Didn't try to coffee. What else? Macaque monkeys.

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I even managed data in holes at a rather nice

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resort golf course, and I've paid the price for that

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because it was a pretty ordinary game. But I enjoyed

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the course beautiful, although the greens in are better than

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that there, you go much better. It's how Superintendent was

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very pleased to hear when I saw him the other day.

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But yeah, incredible country.

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I think.

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I don't know if you can see the map behind me,

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Fred say that, I tell you, yes, that is the

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map of the Sandikan Death March. In World War Two,

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Australian and English military personnel that had been captured by

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the Japanese were sent to Borneo to build an airport,

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and when it looked like the war was lost to Japan,

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they were ordered to kill all prisoners and they force

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marched one eight hundred Australians from Sandakan to a place

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called Ranao in northern Borneo. Of those, eighteen hundred six survived.

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It's a terrible tragedy. It's Australia's worst atrocity in terms

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of war, and not many people know about it. They

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know all about Gallipoli, they know all about some of

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the major battles of World War One and World War Two,

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the Rats of to Brook. It all goes down in folklore,

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but it is is one of the probably one of

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the most forgotten elements of Australian military history really, and

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I would encourage people to go and read about it.

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I knew about it.

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But it's not well publicized. And I think it's a

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tragedy that we tend to put this stuff at the

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back of our minds and should never be forgotten what

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happened over there. So we've basically on the tour followed

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the route of the death March, not intentionally. It was

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just the way the road went, but went to the

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memorials and read all the names, one hundreds and hundreds

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of names. The British suffered similarly, there were six hundred

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British that were captured and basically left to die. It

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was just just horrible. For itd horrible, but the wildlife

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and the rainforests and the rivers and the people magnificent.

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Highly recommend borneo, highly recommend it. Now, you were up

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late last night, weren't you.

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I was, Yeah, there was because of the total eclipse

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of the Moon, which I know you didn't get to

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see because you had eight eighths cloud. I know that

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because of the angle. Australian telescope not very far away

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from you got no observations last night of any can

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But in Sydney we've had cloudy weather for weeks, but

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the clouds, the clouds broke and so we saw the

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eclipse and that was Geordie. Of course that just chimed

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in there. But we actually have Geordie's sister staying with

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us for a whole one. So yeah, this is going

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to probably for the next few weeks. We'll have the

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terrible duo, the more or less identical ones a little

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bit fatter than the other. I won't mention which is which,

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but yeah, and so they yes, she arrived, Rosy arrived today.

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But yeah, that's nothing to do with the clips. We

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did see the blood moon. It was a total eclipse

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of the moon, so that the Earth, the moon was

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well immersed in the shadow of the Earth. We had

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about an hour of totality and during that time the

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clouds came and went a bit, but we got a

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really good view of that blood moon phenomenon caused by

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scattering of lights from the atmosphere, scattering of sunlight. Yes,

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so it was good, but it was, as you've just said,

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of late night and I'm just catching up.

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Yeah enough, it's quite a spectacle of blood moon. I'm

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sorry I missed it, but it can't help the weather,

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which reminds me we also had to deal with flooding

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at the end of the monsoon while we were overseas,

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and that it was fun driving through floodwaters. They wouldn't

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let you do that in Australia, but we weren't in Australia,

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were we. So yeah, we should get down to it, Fred,

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There's a lot to talk about, and our first subject

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is yet again the Artemis missions. And I mentioned at

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the beginning that Artemis two has been put back in

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the shed and probably won't launch those astronauts until at

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least April. But we are now talking about Artemis three. Now,

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this was the mission that was slated for initially twenty

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twenty seven, then push back to probably twenty twenty eight

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to put people on the Moon. There's been several changes.

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It looks like they won't be doing that, and they

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might not be using SpaceX the way things are shaping up.

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That's right. So this was an announcement last week at

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the time we're recording, and you're quite right. What has

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happened is that there's in a major update to the

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Artemis program with an extra mission slotted in. So Artemis three,

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exactly as you've said, was originally going to be the

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lunar landing mission sometime after twenty twenty seven. But what

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they have, what NASA has done, is inserted another mission,

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which is now Artemis three, which will not land on

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the Moon. It will be a spacecraft that will simply

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go into Earth orbit, and what it will do is

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essentially replicate in a sense what Apollo nine did after

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the Apollo eight mission. It's to check that you can

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rendezvous with the equipment, you can do the necessary steps

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that need to be taken in space which have not

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yet been tried and tested. Because Artemis two will simply

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involve the Orion capsule containing the four astronauts, what that

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will do is it will accelerate up to the eleven

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kilometers per second needing to get to the Moon, go

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around the Moon, and then come back again without any

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of the kind of technical details involved with first of all,

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refueling spacecraft in space, that's one of the things that's

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part of the Artemist program, but also doing the rendezvous

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and turning spacecraft around and things of that sort. It's

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a bit like in the Apollo missions where you had

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to turn the turn the lunar module around to dock

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with the with the crew module, with the basically the

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crew capsule. So all of that is now being slotted

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into Apollo. Sorry, Becky. Artemis three, with the landing itself,

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actually forecasts for Artemis four, and one of the reasons

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for this is the fact that there is still a

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lot of work to do on the landing vehicle. Now.

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Back in the day some years ago, NASA contracted both

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SpaceX and Blue Origin. The two companies led by the

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two billionaires Elon Musk and Jeff Bezos. Those two companies

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were tasked with developing a crew lander vehicle to land

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on the Moon. The favored version was Elon Musk's Starship

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the top end of a starship which would which was

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originally going to be the Artemis three Lander. Now the

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lander landing has been pushed back to Artemis four, but

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the gate is now still open for the Bezos company

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to further develop its own lunar landing module, which has

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been under test for quite a while and is so

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in a sense, is a competitor to SpaceX. So the

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two programs are running side by side, and NASA will

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eventually have to make a choice as to which one

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they go with. If I may, there's a very nice

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quote from NASA NASA Associated Administrator, a very senior person

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in NASA, who says, we are looking back to the

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wisdom of the folks that designed Apollo. The entire sequence

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of Artemis flights needs to represent a step by step

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build up of capability, with each step bringing us closer

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to our ability to perform the landing missions. Each step

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needs to be big enough to make progress but not

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so big that we take unnecessary risk given previous learnings. Therefore,

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we want to fly the landing missions in as close

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to the same Earth are sent configuration as possible, which

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means using an upper stage and pad system as close

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to the Block one configuration as possible. That's the basic,

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the basic space launch system configuration. So we will see

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what happens. You're right that Artemis two, the the stack

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is currently back in the vehicle assembly building for checks

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on the upper stage, that's the second stage that will

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actually push the spacecraft into a lunar trajectory. There were

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issues with the helium mechanism for that upper stage, you

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might remember we did talk about that before. That's now

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being fixed and we have a date no sooner than

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April the sixth for a launch of Artemis two, so

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we'll look out for that. But yes, a major change

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in the in the Artemist strategy, which makes a lot

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of sense.

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Yeah, I think it does, and copying a successful series

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like the Apollo missions, notwithstanding what happened to Apollo third

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in but that wasn't that was unforeseen.

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It was just a quirk really.

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And everyone got time. But yeah, what I find interesting

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is those Apollo missions went back to back to back

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to back to back really fast. They seem to be

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much more inflated in their in their mission dates, don't they.

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They do, and that's partly because the technology is now

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far more complex, because these missions are not just to

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achieve boots on the ground. It's all about setting up science,

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you know, a kind of almost permanent presence on the Moon.

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The ultimate schedule, again, this came out of the recent

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press releases and press conferences. The ultimate schedule is one

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Artemis mission per year once we have started, once the

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first lunar landing has taken place, there'll be one a year. Now.

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That is much slower than the Apollo cadence. They were

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one every few months I think. So Apollo eleven was July,

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Pollo twelve was was November, when Apollo thirteen was. But

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you get that, you know that the intervals were a

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few months rather than a few years. I guess another

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reason for not just not just the scientific reasons for

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making it a spacing of one year, but that each

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of these is a very expensive venture. I've seen a

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figure quoted a four billion dollars per launch for an

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Artimist mission, which is high watering. That's right.

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Yeah, did they hit you up for a loan for it?

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I think yeah, I could probably muster a few dollars. Though.

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It's funny when you talk about the advances in technology

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because I'm holding my mobile phone in my hand right now.

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It's got a hell of a lot more computer power

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than the computer on Apollo eleven.

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Sadly, it's also invisible because of your background. No, no, yeah,

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it just disappears what it looks like. You know what

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it looks like. That's right, Yeah, but you're absolutely right. Yes,

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it's quite amazing.

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Not many people probably realize they're packing a lot more

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power than the Apollo missions carried. So yeah, it's all

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in your pocket. If you'd like to read about the

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latest in regard to the Artemis missions, you can do

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that at the Universe today dot com website. But Nasau

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I'll have it on their website and many others as well.

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Is a Space Nuts with Andrew Dunkley and Professor Fred Watson.

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That's a that's agreement is that if the goodness this

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is what he does is he gets very enthusiastic.

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Nuts. Oh drives me in mud. Honestly, it drives me mud.

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I love it. I really do.

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To our next story this this could be the title

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of a science fiction novel, The Brain in space. We're

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talking about a very strange nebula that looks like a

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brain inside a clear sphere, and this is the consequence

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of a star that's kind of shed its out of

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layers and created this quite bizarre looking nebula called PMR one.

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Indeed, that's right. I very much like the headline from

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space dot Com covering this story, which is James Webspace

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telescope performs brain surgery or mysterious exposed cranium nebula, which

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I think sums it up pretty well. That's a good one. Yeah,

240
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it's great. So it's basically a highly evolved star, by

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which I mean a star that's getting near the end

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of its life. It's thrown off some of the layers

243
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of its outer envelope. And what we've seen from the

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James web is images which are taken in the near

245
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infrared and in the mid infrared, and so we get

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two quite different views of this thing that does look

247
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for all the world like an X ray inside somebody's head.

248
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You can see the outline of the skull and a

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lot of funny stuff going on inside.

250
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It really does look that way, doesn't it Like somebody

251
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does put a brain in a goldfish ball and check

252
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that up in the air.

253
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Yes, that's right, with a few stars in the backgroom.

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It's a little bit close to home for me actually,

255
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because the object's technical formal name is PMR one, and

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it was discovered originally by astronomers using the telescope, one

257
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of the telescopes. I was astronomer in charge of the

258
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one point to me to UK Schmidt telescope back in

259
00:16:56.519 --> 00:17:00.440
the late nineteen nineties, and three of my close leagues

260
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were involved with this program, Quentin Parker, David Morgan, and

261
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Ken Russell. And their names are Parker, Morgan, and Russell.

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And that is why this is called PMR one. It

263
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was the first object that was discovered under a program

264
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actually really masterminded by Quentin Parker, an old friend who's

265
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now a professor in the University of Hong Kong. He

266
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had a mission to photograph the sky because back in

267
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those days we were still using photography on the Schmid

268
00:17:30.920 --> 00:17:34.720
telescope using what we call a narrow band filter that

269
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just picked out the light of excited hydrogen, something called

270
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an H one filter or an H alpha filter, and

271
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so the telescope used this filter to survey the night

272
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sky and many interesting objects were revealed, of which the

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first one in the particular program that he collaborated with

274
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David Morgan and Ken Russell was concerned PMR one. That's

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the object we're talking about now. Now we never saw

276
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it with the Schmidt telescope. That was just a flaint,

277
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faint glowing blob. But with the James Webb we see

278
00:18:11.839 --> 00:18:16.720
this extraordinarily detailed, this detailed image. So that the history

279
00:18:16.799 --> 00:18:18.920
is that it was discovered in the late nineteen nineties

280
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on the Schmidt telescope, the Spitzer Space Telescope, which was

281
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a kind of fore runner of the James Web telescopes

282
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and Infrared Telescope and NASA Infrared Observatory when they looked

283
00:18:28.920 --> 00:18:32.680
at PMR one. That was when this curious appearance led

284
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to its unofficial name of the exposed cranium nebula. But

285
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the James Webb was taking that a step further with

286
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these latest observations, which are really quite remarkable, and you

287
00:18:43.160 --> 00:18:46.839
do get a very strong impression of the three dimensional

288
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view of this ball of not so much a ball

289
00:18:51.920 --> 00:18:55.519
it's a kind of elongated almost like a you know,

290
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an oval football elongated sphere of gas with a whole

291
00:19:02.200 --> 00:19:06.200
lot of stuff going on inside it. And what we've

292
00:19:06.240 --> 00:19:12.799
got is an ancient star which is casting off its

293
00:19:12.000 --> 00:19:18.440
outer layers. There is a class of stars called wolf

294
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Rea stars, named after two astronomers I think Drs wolf

295
00:19:25.359 --> 00:19:28.880
and Reya. I think that's right thinking back, and they

296
00:19:28.920 --> 00:19:31.880
are really ancient stars, massive stars that are getting near

297
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the end of their lives, and basically they have winds

298
00:19:35.440 --> 00:19:40.079
of radiation which are blowing away their outer envelopes and

299
00:19:40.599 --> 00:19:44.279
form this nebula, and eventually they may turn into a

300
00:19:44.319 --> 00:19:51.000
supernova and exploding star. So we understand though from the

301
00:19:51.039 --> 00:19:54.039
research that's been carried out with this, that whether it

302
00:19:54.119 --> 00:19:57.160
is a wolf raya star in the middle of PMR one,

303
00:19:57.480 --> 00:20:00.599
or something else, we don't know. The that's going to

304
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be absolutely at the very center of that brain like

305
00:20:04.160 --> 00:20:06.960
nebula inside the exposed cranium.

306
00:20:07.799 --> 00:20:12.640
Yeah, I'm gathering that seeing something like this is very unusual.

307
00:20:13.519 --> 00:20:18.759
It doesn't look like the kind of nebulaly normally see photographed.

308
00:20:19.200 --> 00:20:23.680
It's got uniformity for a start, and it's and you

309
00:20:23.720 --> 00:20:29.240
can see the explosive effect radiating out, it just happens

310
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to look like a brain.

311
00:20:32.079 --> 00:20:38.240
Yes, that's right, So I mean that hydrogen alpha survey

312
00:20:38.279 --> 00:20:42.000
that I mentioned that Quentin Parker and colleagues were engaged in.

313
00:20:42.319 --> 00:20:44.880
I'm pretty sure I took some of the photographs for

314
00:20:45.000 --> 00:20:47.359
it as well back in the day, because I was

315
00:20:47.400 --> 00:20:50.000
still a working astronomer then when I was an astronomy

316
00:20:50.160 --> 00:20:54.000
in charge. I think that one of the main things

317
00:20:54.039 --> 00:20:58.640
that that program did was reveal a very large number

318
00:20:58.799 --> 00:21:02.440
of silicle planetary nebula. So a planetary nebula is a

319
00:21:02.440 --> 00:21:06.960
cloud of gas that's got usually has circular symmetry, which

320
00:21:07.000 --> 00:21:08.960
is why it looks like a planet. And it was

321
00:21:08.960 --> 00:21:11.599
William Hershall who gave it that gave them the name

322
00:21:11.599 --> 00:21:15.279
a planetary nebula. The most famous ones are the Ring

323
00:21:15.319 --> 00:21:18.359
nebula in the northern hemisphere and the Helix nebula down

324
00:21:18.400 --> 00:21:22.119
in the south. But this thing might might be might

325
00:21:22.200 --> 00:21:24.359
actually in the end turn out to be a planetary nebula,

326
00:21:24.400 --> 00:21:28.440
which is an old star that's cast off its out

327
00:21:28.440 --> 00:21:31.799
a lairs and the central core of the star has

328
00:21:31.799 --> 00:21:34.839
turned into what we call a white dwarf, something about

329
00:21:34.920 --> 00:21:40.279
the size of the Earth, but with very high mass

330
00:21:41.680 --> 00:21:45.440
massive a star, and those are white dwarfs are very

331
00:21:45.440 --> 00:21:48.839
hot and they're what excite the glowing the gas into

332
00:21:49.200 --> 00:21:52.640
into glowing. But it's not clear whether this object is

333
00:21:52.640 --> 00:21:54.720
actually a white dwarf or one of these al free

334
00:21:54.839 --> 00:21:56.359
stars that I was just talking about.

335
00:21:56.480 --> 00:21:59.519
Yeah, yeah, I think we've probably got a bit of

336
00:21:59.599 --> 00:22:03.440
a Dolier effect here because we've just got it and gone,

337
00:22:03.559 --> 00:22:04.519
that's a brain.

338
00:22:04.880 --> 00:22:08.240
It's a brain. Yeah, that's right, Yeah, definitely. Yeah.

339
00:22:08.279 --> 00:22:11.680
When we were out on the river in Borneo, what

340
00:22:11.799 --> 00:22:15.160
they told us was it's chock full of saltwater crocodiles,

341
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because every time we saw a log, Yes, that's the

342
00:22:19.039 --> 00:22:19.359
thing you.

343
00:22:19.400 --> 00:22:22.720
Thought it was, Oh, it's a crocodile. Yeah.

344
00:22:22.920 --> 00:22:26.680
Yeah, I think when we saw that forty meter crocodile

345
00:22:26.960 --> 00:22:29.079
surging down the river, we were all panicking a bit

346
00:22:29.200 --> 00:22:31.759
turned out to be a tree.

347
00:22:32.680 --> 00:22:35.319
Well the brunches gave it away, did they, Yes.

348
00:22:35.079 --> 00:22:37.880
Well, no, I didn't have any was that's what really made.

349
00:22:37.680 --> 00:22:39.519
It weird like a crocodile?

350
00:22:39.640 --> 00:22:42.359
Yeah, Well, because we had all that monsoon rain while

351
00:22:42.359 --> 00:22:44.720
we were there, and the river was flooded. And this

352
00:22:44.839 --> 00:22:47.359
is a river five hundred and sixty kilometers long and

353
00:22:47.400 --> 00:22:50.200
about where we were two or three hundred meters wide.

354
00:22:50.240 --> 00:22:53.599
It was massive and the water was flowing very fast.

355
00:22:53.599 --> 00:22:57.359
It was quite scary actually, but yeah, it is. It is, Yeah,

356
00:22:57.400 --> 00:23:00.119
one of those weird effects. We try to humanize every

357
00:23:00.119 --> 00:23:04.400
thing we see in You look at something and think crocodile. No, actually, no,

358
00:23:04.480 --> 00:23:07.599
that's a log And here here we are looking at

359
00:23:07.640 --> 00:23:12.279
a brain in space, which is a some kind of nebula.

360
00:23:12.400 --> 00:23:15.359
Trying to figure out what kind and how it all happened.

361
00:23:15.400 --> 00:23:19.279
But you can read about that at theaweb dot org

362
00:23:19.759 --> 00:23:22.240
website if you want to check it out. Amazing images

363
00:23:22.279 --> 00:23:25.279
they are too. This is Space Nuts with Andrew Dunkley

364
00:23:25.319 --> 00:23:26.440
and Fred Watson.

365
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About step Bartolom mount Up. I'm all crowd preman space nuts.

366
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In the past spread we've had questions from the audience

367
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about the center of our galaxy and it's not easy

368
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to answer because we can't see it. It's all shrouded

369
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in dust. Although you and I have discussed what it

370
00:23:55.119 --> 00:23:57.839
would be like on Earth if there was no dust,

371
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and the light would be so much different for us,

372
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So things could have turned out a different way had

373
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that not been there. But yes, it's shrouded, but there

374
00:24:08.279 --> 00:24:13.319
are ways to look, and they've just published a finding,

375
00:24:13.920 --> 00:24:16.960
thanks to a couple of the great telescopes on Earth,

376
00:24:17.440 --> 00:24:20.000
of what the center of our galaxy is like. They've

377
00:24:20.039 --> 00:24:24.079
mapped a massive section of it in significant detail.

378
00:24:25.799 --> 00:24:29.960
That is correct. And I might just preface this discussion

379
00:24:30.000 --> 00:24:35.519
by noting that in terms of personnel there is a

380
00:24:35.559 --> 00:24:38.799
close connection with what we've just been talking about the

381
00:24:38.920 --> 00:24:42.160
UK Schmidt Telescope, because one of my former colleagues at

382
00:24:42.160 --> 00:24:47.319
the UK Schmidt Telescope, doctor Andy Longmore, I worked with

383
00:24:47.400 --> 00:24:51.319
him at the Royal Observatory Edinburgh. He's still based in Edinburgh,

384
00:24:51.359 --> 00:24:54.720
but he and his wife Marie were actually visiting us

385
00:24:54.799 --> 00:24:57.359
here in Australia at the beginning of this year, so

386
00:24:57.400 --> 00:25:00.400
I went up to Newcastle to see them. And it's

387
00:25:00.480 --> 00:25:04.000
their son that is the lead author on the paper

388
00:25:04.079 --> 00:25:07.720
that has just mapped the center of the galaxy, which

389
00:25:07.759 --> 00:25:10.440
is very nice. It's a lovely connection. So Steve Longmore

390
00:25:10.599 --> 00:25:14.920
their son, like father, like son. He's turned into an

391
00:25:14.920 --> 00:25:19.680
astronomer and very capable because he has led this major

392
00:25:19.880 --> 00:25:27.279
survey which is called ACES. ACES is an acronym for

393
00:25:27.640 --> 00:25:33.680
Alma CMZ Exploration Survey and the CMZ, if I remember rightly,

394
00:25:33.759 --> 00:25:38.160
is the central something zone, central molecular zone of the

395
00:25:39.359 --> 00:25:45.480
galaxy where molecules lurk around around the black hole at

396
00:25:45.480 --> 00:25:48.839
the center of the galaxy. So these observations have been

397
00:25:48.880 --> 00:25:52.640
principally done by as you said, it's been done by

398
00:25:52.640 --> 00:25:55.319
some of the great telescopes. One of them is ALMA.

399
00:25:55.440 --> 00:26:01.759
ALMA itself the Attakama large millimeter submillimeter array that has

400
00:26:02.279 --> 00:26:07.200
basically formed images of the whole of the region around

401
00:26:07.440 --> 00:26:10.680
the center of our galaxy, and it's a very very

402
00:26:10.720 --> 00:26:14.440
detailed image. It's a mosaic basically that's been built up.

403
00:26:14.799 --> 00:26:17.559
The great thing about ALMA is that you can tune

404
00:26:17.599 --> 00:26:21.920
it in to various chemical molecules, all of which emit

405
00:26:22.039 --> 00:26:26.720
their radio frequencies at different wavelengths, so it's like having

406
00:26:26.720 --> 00:26:30.720
a radio spectrum of every point in the center of

407
00:26:30.720 --> 00:26:33.119
our galaxy, which means that you can build up images

408
00:26:33.200 --> 00:26:41.319
showing how these molecules behave around the center of the galaxy.

409
00:26:41.400 --> 00:26:46.759
So it really is an extraordinary piece of work with

410
00:26:47.480 --> 00:26:52.880
a lot of detail, a great deal of information about

411
00:26:52.920 --> 00:26:57.680
both the turbulence and the chemistry that's taking place around

412
00:26:57.720 --> 00:27:01.960
the center of our galaxy. There's a very extensive article

413
00:27:02.000 --> 00:27:06.480
about it on the brighter side of science, on brighter

414
00:27:06.480 --> 00:27:10.680
side of news. It's got some great images and a

415
00:27:10.759 --> 00:27:14.119
lot of details about what has been found. I'm looking

416
00:27:14.160 --> 00:27:16.640
for a quote which came from one of the scientists

417
00:27:17.799 --> 00:27:26.079
which really describes very cogently what they've done. In fact,

418
00:27:26.160 --> 00:27:31.039
Andy sorry, Steve Longmore himself is saying the CMZ or CMZ,

419
00:27:31.160 --> 00:27:35.119
we would call it americanizing it because that's arta karma.

420
00:27:35.200 --> 00:27:38.279
Large millimeter array has got a strong US contingent as

421
00:27:38.319 --> 00:27:42.079
well as other international users. The CMZ hosts some of

422
00:27:42.119 --> 00:27:45.839
the most massive styles known in our galaxy. Many of

423
00:27:45.839 --> 00:27:48.119
these styles live fast and die young, and the end

424
00:27:48.119 --> 00:27:50.480
in super and ova explosions and in some cases what

425
00:27:50.519 --> 00:27:56.240
we call hypernova, very very intense supernova. Let me just

426
00:27:56.400 --> 00:27:59.200
find some other words that I was looking for, because

427
00:28:02.160 --> 00:28:06.799
the extraordinary thing is just how turbulent this region is

428
00:28:07.640 --> 00:28:12.319
the fact that we've got packed into that region around

429
00:28:12.359 --> 00:28:15.160
the center of our galaxy. We've got the turbulence of

430
00:28:15.640 --> 00:28:19.680
gas moving under the gravitational influence of a black hole.

431
00:28:19.720 --> 00:28:21.920
You've got the gravity of the black hole. You've got

432
00:28:21.960 --> 00:28:26.359
intense magnetic fields, you've got outflows from these giant stars,

433
00:28:26.599 --> 00:28:29.400
and all of this is coming together to make a

434
00:28:29.519 --> 00:28:34.119
very complex region of space, which basically is what has

435
00:28:34.160 --> 00:28:37.799
been revealed by this new image. It is quite extraordinary.

436
00:28:38.039 --> 00:28:40.880
It is rather and I'm just reading some of the

437
00:28:40.960 --> 00:28:45.799
data and you know the description they've given lists of

438
00:28:45.880 --> 00:28:49.759
radius of six point one pass six with an expansion

439
00:28:49.799 --> 00:28:53.880
velocity of twenty one killed meat. It's a second. Like

440
00:28:53.920 --> 00:28:55.799
you said, it's a pretty busy neighborhood.

441
00:28:56.440 --> 00:29:00.759
Yes, about six hundred and fifty years across, so really

442
00:29:00.880 --> 00:29:03.720
quite a large a large area. And you're right, it's

443
00:29:03.720 --> 00:29:07.319
actually that the other telescope that was involved. Sorry I

444
00:29:07.359 --> 00:29:11.319
didn't mention that is the European Southern Observatory's Vista telescope,

445
00:29:11.359 --> 00:29:14.119
which is one that is also at Sera Paranell near

446
00:29:14.160 --> 00:29:18.559
the VLT. Vista was a telescope built actually by the

447
00:29:18.599 --> 00:29:22.359
Brits and used by them as there buy into the

448
00:29:22.440 --> 00:29:24.039
European Southern Observatory.

449
00:29:25.480 --> 00:29:28.640
It's a really great article. I like the way they've

450
00:29:28.640 --> 00:29:32.440
got those different images of the various chemical makeups of

451
00:29:33.559 --> 00:29:36.200
and they've overlapped them all to create one image. But

452
00:29:36.839 --> 00:29:40.200
you can you can look at it from several viewpoints

453
00:29:40.279 --> 00:29:43.799
really and it helps you to understand what's going on

454
00:29:43.839 --> 00:29:46.279
in there, which we've been trying to figure out for

455
00:29:46.319 --> 00:29:47.039
a long time for it.

456
00:29:47.640 --> 00:29:51.480
Yeah, that's right. I mean, you know, again happing back

457
00:29:51.519 --> 00:29:55.000
to my time in the Royal Observation in Edinburgh, my

458
00:29:55.200 --> 00:29:58.319
work was actually on my research was about stars in

459
00:29:58.359 --> 00:30:02.839
the galactic sense region, and we couldn't see the galactic

460
00:30:02.920 --> 00:30:05.359
centers because it's hidden from us by dust. And a

461
00:30:05.400 --> 00:30:09.359
lot of these stars were visible through thick layers of

462
00:30:09.440 --> 00:30:13.359
dust that's all penetrated of course with infrared telescopes and

463
00:30:13.400 --> 00:30:18.079
that's why, and by millimeter wave telescopes too, that's why

464
00:30:18.079 --> 00:30:22.319
you can reveal all these fairly complex molecules that have

465
00:30:22.359 --> 00:30:27.640
been that have been found, so really quite a remarkable

466
00:30:27.759 --> 00:30:31.079
is exactly as you've said. It's a great article. Gives

467
00:30:31.079 --> 00:30:33.119
you a good idea of just what's going on in

468
00:30:33.160 --> 00:30:34.359
the center of our galaxy.

469
00:30:34.799 --> 00:30:37.279
Somebody's going to ask, so I'll ask on their behalf,

470
00:30:37.319 --> 00:30:39.240
why couldn't James Webb have done this?

471
00:30:41.440 --> 00:30:44.599
So a lot of it's to do with field of view,

472
00:30:45.240 --> 00:30:47.759
the fact that you've got a huge area here. You

473
00:30:47.839 --> 00:30:50.839
need the coverage of what we would call a survey telescope,

474
00:30:50.880 --> 00:30:54.039
which the James Webb isn't it homes in on fine

475
00:30:54.079 --> 00:30:57.200
points of detail. And the other thing is that James

476
00:30:57.200 --> 00:31:02.599
Webb would give you a different set of of chemical

477
00:31:02.680 --> 00:31:07.359
constituents because you're looking at different wavebands. So these are

478
00:31:08.240 --> 00:31:14.240
the ACES projects, the one I just mentioned which uses

479
00:31:14.279 --> 00:31:19.160
Alma as its main instrument, that's looking in the millimeter

480
00:31:19.400 --> 00:31:23.559
similarly to wave region, and so you see that sensitive

481
00:31:23.599 --> 00:31:26.480
to different molecules from what you get in the infrared.

482
00:31:27.000 --> 00:31:30.920
So it is it's really it's a really neat piece

483
00:31:30.920 --> 00:31:33.160
of work that's been done by the right telescope by

484
00:31:33.160 --> 00:31:34.920
the look of it, and the right group of people

485
00:31:35.119 --> 00:31:35.599
in Breed.

486
00:31:35.839 --> 00:31:38.599
Yes, fantastic. If you want to read all about it,

487
00:31:38.599 --> 00:31:42.119
you can do so by finding the paper. Just do

488
00:31:42.160 --> 00:31:45.319
a search for ACES overview paper, or you can read

489
00:31:45.440 --> 00:31:51.480
the fabulous article at the Brighter Side dot News. We're

490
00:31:51.680 --> 00:31:53.480
just about done, Fred, Thank you very much.

491
00:31:54.200 --> 00:31:56.960
It's a pleasure that went extremely quickly, Andrew.

492
00:31:57.000 --> 00:32:00.839
It hasn't been lately. Maybe we finally get more efficient.

493
00:32:01.599 --> 00:32:05.000
No, no, no, all the other not efficient.

494
00:32:05.799 --> 00:32:08.319
I think it's because Jordie didn't actually play up too much.

495
00:32:08.440 --> 00:32:13.640
So that's right, because his sisters are holding him down. Yeah, cheez,

496
00:32:14.319 --> 00:32:17.680
sisters do that. Thanks. Fred, will catch it very very soon.

497
00:32:18.119 --> 00:32:18.759
Sounds great.

498
00:32:18.799 --> 00:32:21.880
Thanks Andre, Professor Fred Wat's an astronomer at large. I

499
00:32:21.880 --> 00:32:25.160
don't forget to visit us online while you're listening to

500
00:32:25.160 --> 00:32:28.319
the podcast, maybe Space nuts podcast dot com or space

501
00:32:28.400 --> 00:32:31.839
Nuts dot io and have a look around, visit the shop,

502
00:32:32.240 --> 00:32:37.759
maybe become a supporter, leave a review on your platform.

503
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Wherever you listen to us, and don't forget. You can

504
00:32:40.599 --> 00:32:44.559
send us notes and information and questions on the Ask

505
00:32:44.680 --> 00:32:48.119
Me Anything tab at the top AMA And thanks to

506
00:32:48.160 --> 00:32:51.000
Hugh in the studio. Now Hugh couldn't be with us

507
00:32:51.039 --> 00:32:55.119
today Apparently he heard about this, this mapping of the

508
00:32:55.160 --> 00:32:57.319
center of the galaxy and put the coordinates in his

509
00:32:57.839 --> 00:33:02.160
car GPS and he hasn't been said since. And from

510
00:33:02.160 --> 00:33:04.119
me Andrew Duncle, thanks for your company. We'll see you

511
00:33:04.160 --> 00:33:08.039
on the next episode of Space Nuts. Bye bye. You'll

512
00:33:08.079 --> 00:33:16.039
be listening to the Space Nuts podcast available at Apple Podcasts, Spotify, iHeartRadio,

513
00:33:16.400 --> 00:33:19.440
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demand at bites dot com. This has been another quality

515
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podcast production from Nights dot com.