The Starless Galaxy That Shouldn’t Exist - But Does | Space Nuts: Astronomy Insights & Cosmic...
Space News TodaySeptember 03, 202600:38:2835.23 MB

The Starless Galaxy That Shouldn’t Exist - But Does | Space Nuts: Astronomy Insights & Cosmic...

Space Nuts: Spanish Eclipse, Nancy Grace Roman Launch, Cloud Nine, and Venus's Mysterious Clouds

Andrew Dunkley and Professor Fred Watson cover four big astronomy stories in this episode, from Fred’s trip to view a sunset eclipse in Spain to the launch of the Nancy Grace Roman Space Telescope. They also unpack a starless dwarf galaxy called Cloud Nine and a new way of thinking about the strange dark material in Venus’s clouds.

Guests and speakers

Andrew Dunkley - Host, frames the news, asks listener questions, and guides the discussion.

Professor Fred Watson - Astronomer at large, explains the eclipse, the Roman telescope, Cloud Nine, and Venus’s clouds.

Key topics

In this episode, Fred recounts the Spanish eclipse expedition

The eclipse was only 9 degrees above the western horizon at totality, making the viewing conditions unusually challenging.

He and Marnie led a 16-person tour through France, Spain, and Switzerland before settling near Santander in northern Spain.

They staked out a viewing site 2 kilometers from the hotel, set up a gazebo, and had to tie it down to a car to keep it from blowing away.

The weather looked threatening, but a hole opened in the cloud just before totality, giving them a clear view of the corona.

Fred described the yellowish corona, pink hydrogen clouds, and the crowd of around 2,000 people.

We discuss the Nancy Grace Roman Space Telescope launch

Andrew watched the launch live after being nudged by his own brain at the right moment.

Fred noted the launch was flawless, with 27 Merlin motors firing.

The telescope is headed for the L2 Lagrange point, about 1.5 million kilometers away.

Roman is a 2.4-meter Hubble-class telescope but with 100 times the field of view.

Its wide-angle infrared design should enable major surveys of dark matter, dark energy, and exoplanets via its coronagraph.

Fred explains why Cloud Nine matters

Cloud Nine is described as a starless dwarf galaxy about 14 million light years away.

It lies near Messier 94 and was studied using the Gran Telescopio Canarias and its Hypercam instrument.

The deep exposure was 2.36 hours, yet the team found no convincing stellar population.

Fred says theory suggests the gas may be too hot to cool and collapse into stars because of the ultraviolet background radiation after reionization.

He says Cloud Nine may be the first strong example of a galaxy predicted by standard cosmology but never before clearly identified.

Venus’s clouds are still puzzling astronomers

Fred explains that Venus appears yellowish because we see the top of its cloud layer, especially in visible light.

In ultraviolet, Venus shows dramatic global cloud patterns caused by an as-yet unidentified absorber.

The new study uses radiative transfer modeling to constrain what the unknown absorber could be.

The team compares Venus’s cloud droplets to cigarette smoke, tiny particles that look light-colored when dispersed but could become dark sludge in bulk.

The result suggests the absorber must be very efficient, very concentrated, or both, but it is not being claimed as evidence of life.




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Episode link: https://play.headliner.app/episode/35083231?utm_source=youtube

Kind: captions Language: en
00:00:00 --> 00:00:02 Hi there. Thanks for joining us. This is

00:00:02 --> 00:00:04 Space Nuts. My name is Andrew Dunley,

00:00:04 --> 00:00:06 your host. And it is good to have your

00:00:06 --> 00:00:09 company as always. Uh coming up on this

00:00:09 --> 00:00:12 episode. Uh we're going to revisit the

00:00:12 --> 00:00:14 Spanish eclipse because the man of the

00:00:14 --> 00:00:16 moment, the man who went there and

00:00:16 --> 00:00:17 pointed it out to everyone and said

00:00:17 --> 00:00:19 that's what an eclipse looks like, he

00:00:19 --> 00:00:21 couldn't join us. But Fred Watson will

00:00:21 --> 00:00:24 talk about it. Uh we'll also be uh

00:00:24 --> 00:00:28 discussing the Nancy um Roman uh uh

00:00:28 --> 00:00:30 observatory launch which I watched

00:00:30 --> 00:00:32 online the other the other night which

00:00:32 --> 00:00:35 was spectacular. Uh and there's a

00:00:35 --> 00:00:37 there's a galaxy that they're looking at

00:00:37 --> 00:00:40 with um a bit of a frown and a scratch

00:00:40 --> 00:00:42 of the neck because uh it does not

00:00:42 --> 00:00:45 appear to have many stars. Uh it's not

00:00:45 --> 00:00:48 emitting starlight. How could that be?

00:00:48 --> 00:00:50 And we'll finish up with the mystery

00:00:50 --> 00:00:53 clouds of Venus. That's all coming up on

00:00:53 --> 00:00:55 this episode of Space Nuts.

00:00:55 --> 00:01:00 >> 15 seconds. Guidance is internal. 10 9g

00:01:00 --> 00:01:02 Ignition sequence start.

00:01:02 --> 00:01:03 >> Space nuts.

00:01:03 --> 00:01:08 >> 5 4 3 2 1 2 3 4 5 5 4 3 2 1

00:01:08 --> 00:01:09 >> Space Nuts.

00:01:09 --> 00:01:12 >> Astronauts report. It feels good.

00:01:12 --> 00:01:14 and he's back after traveling halfway

00:01:14 --> 00:01:16 around the world and returning and then

00:01:16 --> 00:01:19 getting his leg um amputated. Well, not

00:01:19 --> 00:01:21 quite, but uh he got it rebuilt. $6

00:01:22 --> 00:01:24 million. It was I think the price of

00:01:24 --> 00:01:26 that. Uh it's Professor Fred Watson,

00:01:26 --> 00:01:28 astronomer at large. Hello, Fred.

00:01:28 --> 00:01:30 >> Hi, Andrew. Thank you for that great

00:01:30 --> 00:01:34 intro. Yes, $6 million. Um and my health

00:01:34 --> 00:01:36 fund provided $42.50. So,

00:01:36 --> 00:01:38 >> yes, that's usually how it goes in

00:01:38 --> 00:01:40 Australia. Um, that's the going rate. No

00:01:40 --> 00:01:41 matter what it cost you to go and see a

00:01:42 --> 00:01:43 doctor, you get 40 bucks back.

00:01:43 --> 00:01:47 >> Yeah, it's a great system. Um, yeah.

00:01:47 --> 00:01:49 Anyway, we won't go there. That's

00:01:49 --> 00:01:50 politics.

00:01:50 --> 00:01:52 >> Yeah, that's right. But as you alluded,

00:01:52 --> 00:01:55 uh, I have indeed received a new knee.

00:01:55 --> 00:01:59 So, I had a my second T TKR, total knee

00:01:59 --> 00:02:00 replacement.

00:02:00 --> 00:02:00 >> Wow.

00:02:00 --> 00:02:02 >> Um, which is, uh, it was a week ago.

00:02:02 --> 00:02:05 Yesterday was the surgery. So, I'm still

00:02:05 --> 00:02:07 on painkillers, so will not make any

00:02:07 --> 00:02:09 sense whatsoever. Um, I might go to

00:02:09 --> 00:02:10 sleep halfway through the show. That's

00:02:10 --> 00:02:13 been one of the symptoms.

00:02:14 --> 00:02:16 >> Well, between you falling asleep and me

00:02:16 --> 00:02:18 sneezing, it should be an interesting

00:02:18 --> 00:02:20 show. Hay fever is running right here at

00:02:20 --> 00:02:21 the moment,

00:02:21 --> 00:02:25 >> and I I cannot control it. Um, I know

00:02:25 --> 00:02:27 there's medications out there, but I'm

00:02:27 --> 00:02:29 some I'm not allowed to take anymore

00:02:29 --> 00:02:30 because of my eyes.

00:02:30 --> 00:02:32 >> So, it's made it more complicated. So,

00:02:32 --> 00:02:36 um, I'm I'm I'm well armed. Look, I've

00:02:36 --> 00:02:38 got Oh, yes. the mandatory box of

00:02:38 --> 00:02:41 tissues within arms length. So hopefully

00:02:41 --> 00:02:43 we'll get through it, Fred. And um I'm

00:02:43 --> 00:02:44 glad the knee operation went well.

00:02:44 --> 00:02:46 You're the second person in a week that

00:02:46 --> 00:02:48 I've met who's had a total knee

00:02:48 --> 00:02:51 replacement. A friend of mine um

00:02:51 --> 00:02:53 >> literally stepped into a hole that he

00:02:53 --> 00:02:54 didn't know was there because it was

00:02:54 --> 00:02:57 full of grass and buckled his knee and

00:02:57 --> 00:02:58 the damage was too severe and they had

00:02:58 --> 00:03:01 to do a a knee replacement. Bit of a

00:03:01 --> 00:03:02 shocker that one.

00:03:02 --> 00:03:03 >> Yes.

00:03:03 --> 00:03:06 >> But um he's still on crutches.

00:03:06 --> 00:03:08 >> Okay. Well, I've parked my crutches,

00:03:08 --> 00:03:10 although I did resort to one in the

00:03:10 --> 00:03:12 middle of the night uh when I had to get

00:03:12 --> 00:03:14 up. Uh I thought I'm just going to use

00:03:14 --> 00:03:16 the crotch that came this time. But

00:03:16 --> 00:03:20 yeah, um it doesn't take long. But um

00:03:20 --> 00:03:23 you know, your colleague uh uh there, he

00:03:23 --> 00:03:25 had much more than just a knee

00:03:25 --> 00:03:27 replacement with that accident damage.

00:03:27 --> 00:03:30 Mine was just a quick one out, one in.

00:03:30 --> 00:03:32 Uh and so I think it's a lot more

00:03:32 --> 00:03:34 predictable and probably a lot easier

00:03:34 --> 00:03:37 for me to recover. Um, I'm sorry he's

00:03:37 --> 00:03:39 still on crutches and hope he I wish him

00:03:39 --> 00:03:41 well. We used to speak on the radio a

00:03:41 --> 00:03:42 long time ago.

00:03:42 --> 00:03:45 >> That's right. One of my old radio mates.

00:03:45 --> 00:03:47 >> Uh, Fred, let's talk about the Spanish

00:03:47 --> 00:03:49 Eclipse. I saw a lot of pictures and

00:03:49 --> 00:03:51 footage online. People getting very

00:03:51 --> 00:03:53 artistic with their photography at

00:03:53 --> 00:03:56 times. Uh, these things have become very

00:03:56 --> 00:03:57 popular.

00:03:57 --> 00:04:00 >> And, uh, from what I could tell, it was

00:04:00 --> 00:04:01 it was a little bit different because it

00:04:01 --> 00:04:04 wasn't sort of up there. It was over

00:04:04 --> 00:04:06 there. Is that how it went? It was more

00:04:06 --> 00:04:08 on the horizon than than you'd normally

00:04:08 --> 00:04:09 expect.

00:04:09 --> 00:04:11 >> That's right. It was um and that was

00:04:11 --> 00:04:14 always the issue for us uh because at

00:04:14 --> 00:04:18 the time of totality it was only 9°

00:04:18 --> 00:04:20 above the western horizon and that's

00:04:20 --> 00:04:25 very low down. Um but we figured that we

00:04:25 --> 00:04:28 would take that risk. Uh the story

00:04:28 --> 00:04:31 actually goes back a long way. So so we

00:04:31 --> 00:04:34 were leading a tour group. We had uh uh

00:04:34 --> 00:04:37 16 16 of us through France and Spain and

00:04:37 --> 00:04:38 Switzerland. We went to Large Hadron

00:04:38 --> 00:04:40 Collider. We went to two observatories

00:04:40 --> 00:04:43 in France uh or Puvance and Pipidi, both

00:04:43 --> 00:04:45 of which were sensational. We really

00:04:45 --> 00:04:47 enjoyed those visits and wound up at um

00:04:47 --> 00:04:51 Santandere in northern Spain. Uh we we

00:04:51 --> 00:04:54 got there I think three days before the

00:04:54 --> 00:04:57 eclipse. Um, and the first thing Mani

00:04:57 --> 00:05:01 and I did was to basically stake out

00:05:01 --> 00:05:03 where we were going to watch it from.

00:05:03 --> 00:05:05 Uh, because, um, in those resorts in

00:05:05 --> 00:05:08 northern Spain on the coast, uh, they're

00:05:08 --> 00:05:10 all built facing eastwards because they

00:05:10 --> 00:05:12 get the morning sun and often there is

00:05:12 --> 00:05:16 high ground behind them and and so we um

00:05:16 --> 00:05:18 found a spot about 2 kilometers from our

00:05:18 --> 00:05:20 hotel. We had a couple of vehicles so we

00:05:20 --> 00:05:24 could manipulate everything. Um Manne um

00:05:24 --> 00:05:28 bought a gazebo uh which we erected on

00:05:28 --> 00:05:30 our chosen spot. There was nobody there

00:05:30 --> 00:05:33 at that time, but we knew it was going

00:05:33 --> 00:05:36 to fill up. Uh so we had this gazebo. Um

00:05:36 --> 00:05:38 we the first night I said, "This is

00:05:38 --> 00:05:40 going to blow away if we just leave it

00:05:40 --> 00:05:43 here." So So we parked one of our

00:05:43 --> 00:05:45 vehicles under the gazebo and tied the

00:05:45 --> 00:05:48 gazebo down onto the roof of the car.

00:05:48 --> 00:05:50 Still there the next day. Yeah.

00:05:50 --> 00:05:52 >> And so the next day, but the gazebo was

00:05:52 --> 00:05:56 That's right. So, yeah, it turned into

00:05:56 --> 00:05:58 quite a big event. There were there were

00:05:58 --> 00:06:00 very big crowds there. We'd obviously

00:06:00 --> 00:06:03 chosen exactly the right spot. Um, lots

00:06:03 --> 00:06:05 of people. An ice cream van was there

00:06:05 --> 00:06:07 that turned up on day two.

00:06:07 --> 00:06:08 >> Oh, wow.

00:06:08 --> 00:06:11 >> Day tminus one. Um, a whole lot of cops

00:06:11 --> 00:06:14 came on horseback and in vehicles and in

00:06:14 --> 00:06:15 helicopters. They were obviously all

00:06:15 --> 00:06:18 taken completely by surprise by this

00:06:18 --> 00:06:21 event. What's going on up there? Um but

00:06:21 --> 00:06:23 yes on the afternoon so it was an

00:06:23 --> 00:06:26 evening eclipse the afternoon uh the sky

00:06:26 --> 00:06:29 was completely clear but uh towards the

00:06:29 --> 00:06:31 end of the afternoon this bank of cloud

00:06:31 --> 00:06:34 appeared in the west uh and you could

00:06:34 --> 00:06:36 see that it was sort of spreading

00:06:36 --> 00:06:38 upwards as it approached.

00:06:38 --> 00:06:40 >> So the sun was effectively setting into

00:06:40 --> 00:06:42 that. The partial phase started at half

00:06:42 --> 00:06:45 7. We got I spotted that with the

00:06:45 --> 00:06:47 binoculars. It was a magical moment when

00:06:47 --> 00:06:49 I first saw the mountains of the moon

00:06:49 --> 00:06:51 just encroaching into the sun's disc.

00:06:51 --> 00:06:53 This was with binoculars with filters.

00:06:53 --> 00:06:56 Uh and then we, you know, eclipses are

00:06:56 --> 00:06:58 an amazing spectacle. You've got this

00:06:58 --> 00:07:00 buildup over an hour or so as the moon's

00:07:00 --> 00:07:03 disc gradually covers the sun and then

00:07:03 --> 00:07:05 that time of perfection when it's when

00:07:05 --> 00:07:07 the two are exactly aligned. So what

00:07:07 --> 00:07:08 happened? We all got steadily more and

00:07:08 --> 00:07:10 more depressed as the sun was sinking

00:07:10 --> 00:07:13 into this bank of cloud. But about 2

00:07:13 --> 00:07:16 minutes before totality, a hole opened

00:07:16 --> 00:07:19 up uh right where the sun was. And when

00:07:19 --> 00:07:21 the total eclipse happened, we got a

00:07:21 --> 00:07:23 perfect view of the corona. It was just

00:07:23 --> 00:07:26 magical. It was clear. Um so we could

00:07:26 --> 00:07:28 see the outer atmosphere of the sun. The

00:07:28 --> 00:07:30 corona looked slightly yellowish and

00:07:30 --> 00:07:32 that's because the sun was so low.

00:07:32 --> 00:07:34 Normally pure white

00:07:34 --> 00:07:36 >> and pink clouds of hydrogen which were

00:07:36 --> 00:07:38 bigger than I've seen before. They were

00:07:38 --> 00:07:40 spectacular. Lots of cheers from the

00:07:40 --> 00:07:42 crowd. There were about 2 people

00:07:42 --> 00:07:45 there by then. Uh we in our little tent,

00:07:45 --> 00:07:46 there were 20 of us, too, cuz two

00:07:46 --> 00:07:48 members of my UK family or four members

00:07:48 --> 00:07:51 came out to watch. So, a good time was

00:07:51 --> 00:07:52 had by all.

00:07:52 --> 00:07:55 >> Uh and we were delighted to to get a

00:07:55 --> 00:07:57 great eclipse and I think everybody was

00:07:57 --> 00:08:00 very happy. And I spent the next

00:08:00 --> 00:08:01 >> I was going to say, isn't it twice in a

00:08:01 --> 00:08:03 row that you've been to an eclipse that

00:08:03 --> 00:08:04 was cloudy and it cleared up at the last

00:08:04 --> 00:08:05 second?

00:08:05 --> 00:08:07 >> Cleared up. That's right. Um not nearly

00:08:07 --> 00:08:09 twice in a It was the one before last, I

00:08:09 --> 00:08:09 think. Was

00:08:09 --> 00:08:10 >> Oh, yeah.

00:08:10 --> 00:08:13 >> Uh, no. Was it the last one? Yes, it was

00:08:13 --> 00:08:15 the last one. It was in Texas. That's

00:08:15 --> 00:08:15 right.

00:08:15 --> 00:08:18 >> Uh, and it was cloudy. Uh, and then the

00:08:18 --> 00:08:20 holes appeared and

00:08:20 --> 00:08:22 >> we we saw the eclipse. So,

00:08:22 --> 00:08:24 >> yeah, some somebody's looking after us.

00:08:24 --> 00:08:26 I don't know who is looking after us. It

00:08:26 --> 00:08:27 was great.

00:08:27 --> 00:08:29 >> Um, yeah. And that sort of wrapped up

00:08:29 --> 00:08:31 the tour. Then we had a couple of days.

00:08:31 --> 00:08:33 Uh, we had I won't bore you with the

00:08:33 --> 00:08:35 details. We had a nightmare journey

00:08:35 --> 00:08:36 home.

00:08:36 --> 00:08:39 >> Oh. which involved rebooking flights uh

00:08:39 --> 00:08:41 two hours before they left through to

00:08:41 --> 00:08:44 Sim from Barcelona. But anyway, that's

00:08:44 --> 00:08:45 another story.

00:08:45 --> 00:08:46 >> Travelers tales, you've got plenty of

00:08:46 --> 00:08:47 them as well.

00:08:47 --> 00:08:51 >> Yeah. Yeah. Yeah. Um I I guess the

00:08:51 --> 00:08:53 difference with that eclipse in Spain

00:08:53 --> 00:08:56 was it was happening at sunset. And

00:08:56 --> 00:08:57 normally when you watch one of these

00:08:57 --> 00:09:01 eclipses, it turns day into night and

00:09:01 --> 00:09:03 then it comes back to day again. But at

00:09:03 --> 00:09:05 sunset, I guess you sort of missed out

00:09:05 --> 00:09:07 on that kind of effect to a certain

00:09:07 --> 00:09:08 degree.

00:09:08 --> 00:09:09 >> Yeah, to a excuse me, to a certain

00:09:09 --> 00:09:11 extent because it but it got dark very

00:09:11 --> 00:09:14 quickly as it does. It's only

00:09:14 --> 00:09:16 >> when the something like 80 or 90% of the

00:09:16 --> 00:09:18 sun's disc is covered. That's the only

00:09:18 --> 00:09:20 time when you notice the that things are

00:09:20 --> 00:09:23 dimming. Um I think birds did go to

00:09:23 --> 00:09:24 sleep. We didn't really take much

00:09:24 --> 00:09:27 notice. It was um 1 minute and 3 seconds

00:09:27 --> 00:09:29 was the time of totality that we had.

00:09:29 --> 00:09:32 >> Yeah. Uh um but yes, it did get light

00:09:32 --> 00:09:34 again. Uh light enough for us to take

00:09:34 --> 00:09:36 lots of photographs of each other and

00:09:36 --> 00:09:38 all the rest of it. Uh we demolished the

00:09:38 --> 00:09:41 gazebo, gave it to a guy, a French guy

00:09:41 --> 00:09:43 who thought it was the bees knees. He he

00:09:43 --> 00:09:46 had a camper van next door. We also gave

00:09:46 --> 00:09:48 him the inflatable fridge that we

00:09:48 --> 00:09:49 bought.

00:09:49 --> 00:09:49 >> Oh my goodness.

00:09:49 --> 00:09:51 >> Did you know there was such a thing?

00:09:51 --> 00:09:52 >> I've never heard of it.

00:09:52 --> 00:09:54 >> My wife does. Uh, we had an inflatable

00:09:54 --> 00:09:56 fridge and we gave him some chairs as

00:09:56 --> 00:09:58 well because we couldn't take all this

00:09:58 --> 00:09:59 stuff back to Australia.

00:09:59 --> 00:10:00 >> Of course.

00:10:00 --> 00:10:01 >> Yeah.

00:10:01 --> 00:10:02 >> Fantastic.

00:10:02 --> 00:10:06 >> Yeah. Well, you know, I'm all set for do

00:10:06 --> 00:10:07 2028.

00:10:07 --> 00:10:10 >> Yeah. 2028. That's right. So,

00:10:10 --> 00:10:11 >> less than two years now.

00:10:12 --> 00:10:12 >> Not far.

00:10:12 --> 00:10:14 >> We just been sitting on this one for 20

00:10:14 --> 00:10:16 years when we first found out about it.

00:10:16 --> 00:10:18 But, uh, yeah, looking forward to that.

00:10:18 --> 00:10:20 In fact, uh I think that year um there's

00:10:20 --> 00:10:23 going to be three or four eclipses in

00:10:23 --> 00:10:25 our part of the world or over those next

00:10:25 --> 00:10:25 couple years.

00:10:25 --> 00:10:27 >> Each of the next few years, yeah, I

00:10:27 --> 00:10:31 think till 20 30 something. I can't

00:10:31 --> 00:10:33 remember what it 38.

00:10:33 --> 00:10:35 >> Yeah, I don't know. There there are

00:10:35 --> 00:10:36 another three. That's right.

00:10:36 --> 00:10:37 >> Yeah.

00:10:37 --> 00:10:39 >> Okay. Um well, that sounds like fun.

00:10:39 --> 00:10:40 Let's talk about something else

00:10:40 --> 00:10:42 extraordinary. Uh the other night I was

00:10:42 --> 00:10:45 sitting uh in my lounge just about to

00:10:45 --> 00:10:46 pop off to sleep and my brain said, "You

00:10:46 --> 00:10:48 know, they should be launching the Nancy

00:10:48 --> 00:10:51 Roman Telescope sometime soon, Andrew."

00:10:51 --> 00:10:52 So I thought, "Oh yeah, yeah."

00:10:52 --> 00:10:55 >> So I grabbed my iPad and I logged on and

00:10:55 --> 00:10:57 and sure enough, the countdown was 5

00:10:57 --> 00:10:59 minutes from launch. And I thought,

00:10:59 --> 00:11:02 >> "Isn't the brain an amazing thing?"

00:11:02 --> 00:11:02 >> Yeah.

00:11:02 --> 00:11:05 >> That it that it reminded me of that 5

00:11:05 --> 00:11:07 minutes before the launch. And and and I

00:11:07 --> 00:11:10 I was oblivious to it at that moment.

00:11:10 --> 00:11:12 So, I watched the whole thing. It was

00:11:12 --> 00:11:15 fantastic. Yeah, I I watched the replay

00:11:15 --> 00:11:18 the next day. I wasn't um switched on as

00:11:18 --> 00:11:19 you were. I was probably asleep actually

00:11:19 --> 00:11:23 with them with the with the painkillers.

00:11:23 --> 00:11:25 But yes, I did I did um realize that it

00:11:25 --> 00:11:27 was taking place then. Uh and yeah,

00:11:27 --> 00:11:29 flawless launch. It looked fantastic.

00:11:29 --> 00:11:30 >> It was, wasn't it?

00:11:30 --> 00:11:33 >> All 27 of those Merlin motors firing

00:11:33 --> 00:11:35 away there. M

00:11:35 --> 00:11:39 and it's now makes the 1 million is it

00:11:39 --> 00:11:42 kilometers or miles journey to

00:11:42 --> 00:11:44 >> uh yes a million miles a million and a

00:11:44 --> 00:11:46 half kilometers uh and I think it's well

00:11:46 --> 00:11:49 on the way this is to the the L2 point

00:11:49 --> 00:11:51 that point on the far side of the earth

00:11:51 --> 00:11:53 from the sun where there's this stable

00:11:53 --> 00:11:56 stable gravitational thing which we call

00:11:56 --> 00:11:58 a lrangee point um several spacecraft

00:11:58 --> 00:12:01 there already including the James Web

00:12:01 --> 00:12:03 and Gia the that European fantastic

00:12:03 --> 00:12:05 European project that's there. Few other

00:12:05 --> 00:12:06 ones

00:12:06 --> 00:12:07 >> they'll be running out of room up there.

00:12:07 --> 00:12:09 They'll have to put in traffic lights.

00:12:09 --> 00:12:11 >> So it's interesting. Um you kind of

00:12:11 --> 00:12:12 think of that. Oh, if this is a stable

00:12:12 --> 00:12:14 point, they must always be trying to get

00:12:14 --> 00:12:16 to the same point. But actually what

00:12:16 --> 00:12:18 they are, they're all in orbit around a

00:12:18 --> 00:12:19 stable point.

00:12:19 --> 00:12:21 >> So you're in orbit around nothing. Um

00:12:21 --> 00:12:24 but the gravitational forces work to

00:12:24 --> 00:12:25 sort of keep you keep you in orbit

00:12:25 --> 00:12:31 there. Um yep. So it's um yes. So so I I

00:12:31 --> 00:12:33 don't know. I haven't really looked at

00:12:33 --> 00:12:36 the commissioning schedule for the Nancy

00:12:36 --> 00:12:39 Grace Roman. Uh but um it's probably

00:12:39 --> 00:12:41 already started because they don't waste

00:12:41 --> 00:12:43 much time with these things to you know

00:12:43 --> 00:12:45 get as much data as they can just in

00:12:45 --> 00:12:47 case something catastrophic goes wrong

00:12:47 --> 00:12:50 early on. Um what we've got here is a

00:12:50 --> 00:12:54 Hubble class telescope um same sort of

00:12:54 --> 00:12:58 size as the Hubble uh 2.4 4 meters with

00:12:58 --> 00:13:01 uh the big difference that even though

00:13:01 --> 00:13:04 it's got the fine detail, the resolving

00:13:04 --> 00:13:06 power of the Hubble, it's got a 100

00:13:06 --> 00:13:09 times the field of view of the Hubble,

00:13:09 --> 00:13:12 >> which means it sees 100 times more sky.

00:13:12 --> 00:13:14 And so, you know, the Pubble's always

00:13:14 --> 00:13:17 been giving us these what you might call

00:13:17 --> 00:13:19 pinhole images, just almost looking

00:13:20 --> 00:13:22 through a straw at the sky. Uh the Nancy

00:13:22 --> 00:13:24 Grace Roman is a wide angle telescope.

00:13:24 --> 00:13:27 It's also infrared. Uh so it um it is

00:13:27 --> 00:13:30 actually seeing redder than red light.

00:13:30 --> 00:13:33 And we've got high hopes for what it

00:13:33 --> 00:13:35 might achieve with the huge galaxy

00:13:35 --> 00:13:38 surveys which hopefully will show light

00:13:38 --> 00:13:40 on would shed light on dark matter and

00:13:40 --> 00:13:45 dark energy. And um also it's got a very

00:13:45 --> 00:13:48 sophisticated coronagraph on board. And

00:13:48 --> 00:13:50 a coronagraph is a thing that blocks out

00:13:50 --> 00:13:52 the light of a star so you can look for

00:13:52 --> 00:13:55 other objects nearby. until we should

00:13:55 --> 00:13:58 start seeing images of exoplanets coming

00:13:58 --> 00:14:00 from the anti-grace Roman as well. So,

00:14:00 --> 00:14:02 it is lots to talk about down the track,

00:14:02 --> 00:14:03 Andrew.

00:14:03 --> 00:14:05 >> Yeah, very exciting. When do they expect

00:14:05 --> 00:14:08 it to actually be ready to roll? It it's

00:14:08 --> 00:14:10 a bit of a process, isn't it?

00:14:10 --> 00:14:11 >> It is. That's right. I'm not sure what

00:14:11 --> 00:14:14 the schedule is, as I was saying, but um

00:14:14 --> 00:14:16 we'll keep um we'll keep Space Not

00:14:16 --> 00:14:17 listeners posted. At the moment, the

00:14:17 --> 00:14:19 news is all good. And

00:14:19 --> 00:14:23 >> yeah, it is. It is. Uh in fact um I'm

00:14:23 --> 00:14:25 just looking.

00:14:25 --> 00:14:28 Yeah, first observations maybe early

00:14:28 --> 00:14:30 next year sometime. They haven't got

00:14:30 --> 00:14:33 >> exactly I had it in mind. It was 2027.

00:14:33 --> 00:14:33 >> Yeah.

00:14:33 --> 00:14:36 >> Um and I mean I I remember because we

00:14:36 --> 00:14:39 lived it in real time the commissioning

00:14:39 --> 00:14:42 for the Hubble telescope back in 1990. I

00:14:42 --> 00:14:43 was an astronomer at the UK Schmidt

00:14:44 --> 00:14:46 telescope then and we were getting

00:14:46 --> 00:14:48 direct reports from NASA actually about

00:14:48 --> 00:14:51 the commissioning before the interweb.

00:14:51 --> 00:14:55 Um and we very quickly realized that

00:14:55 --> 00:14:57 something was wrong uh because we got um

00:14:57 --> 00:14:59 reports of the image diameter as they

00:14:59 --> 00:15:01 went through focus

00:15:01 --> 00:15:03 >> and the image diameter never got small.

00:15:03 --> 00:15:05 So it was quite obvious very early on

00:15:05 --> 00:15:07 that um there was a problem with the

00:15:07 --> 00:15:09 Hubble and of course took them three

00:15:09 --> 00:15:12 years to build a a little device to

00:15:12 --> 00:15:15 correct for that and um uh then it was

00:15:15 --> 00:15:18 flown on a space shuttle mission and the

00:15:18 --> 00:15:19 rest is history.

00:15:19 --> 00:15:21 >> Yeah. A pufu valve I think it was they

00:15:21 --> 00:15:24 needed to put on it. Yeah. But um anyway

00:15:24 --> 00:15:27 >> did have a name costbar was it something

00:15:27 --> 00:15:27 like that.

00:15:27 --> 00:15:30 >> Something like that. Um it was lucky

00:15:30 --> 00:15:32 that it was close enough to get to. Um,

00:15:32 --> 00:15:33 >> yes, that's right.

00:15:33 --> 00:15:35 >> Can't do that with the L2.

00:15:35 --> 00:15:39 >> You can't. That's exactly right. Um,

00:15:39 --> 00:15:41 >> yes, things have moved on a bit since

00:15:41 --> 00:15:42 then. They have.

00:15:42 --> 00:15:44 >> Uh, exciting times and we will watch

00:15:44 --> 00:15:47 with interest and of course uh when they

00:15:47 --> 00:15:49 um achieve first light and we start to

00:15:49 --> 00:15:51 see some other images, we will share

00:15:51 --> 00:15:53 them with you here on Space Nuts. And

00:15:53 --> 00:15:56 you are listening to the latest edition

00:15:56 --> 00:15:58 with Andrew Dunley and Professor Fred

00:15:58 --> 00:15:59 Watson.

00:15:59 --> 00:16:01 Think

00:16:01 --> 00:16:03 we need to do a little more all weather

00:16:03 --> 00:16:04 testing.

00:16:04 --> 00:16:05 >> Amen.

00:16:05 --> 00:16:07 >> Space nets.

00:16:07 --> 00:16:09 >> Okay, Fred, let's talk about this

00:16:09 --> 00:16:12 strange galaxy. Um, some are saying it's

00:16:12 --> 00:16:15 a failed galaxy. Uh, it's been described

00:16:15 --> 00:16:17 as a starless galaxy and it's got a

00:16:17 --> 00:16:19 name. It's called Cloud9. What is this

00:16:19 --> 00:16:21 thing?

00:16:21 --> 00:16:26 Uh it's um yes it's a not a mystery

00:16:26 --> 00:16:28 galaxy in the sense that people have

00:16:28 --> 00:16:30 speculated

00:16:30 --> 00:16:33 that there may be galaxies without stars

00:16:33 --> 00:16:36 and you know we tend to think of

00:16:36 --> 00:16:39 galaxies as being made of stars because

00:16:39 --> 00:16:42 ours is Milky Way is a gigantic spiral

00:16:42 --> 00:16:45 of stars and gas and dust.

00:16:45 --> 00:16:46 Very beautiful if we could see it from

00:16:46 --> 00:16:49 the outside which sadly we we never can.

00:16:49 --> 00:16:54 Uh but um it has always been speculated

00:16:54 --> 00:16:56 that there may be

00:16:56 --> 00:17:00 uh galaxies which contain clouds of

00:17:00 --> 00:17:03 hydrogen, the raw material of stars,

00:17:03 --> 00:17:07 which basically is too hot for the

00:17:08 --> 00:17:10 clouds to collapse into individual

00:17:10 --> 00:17:11 stars. I think I've got the logic the

00:17:11 --> 00:17:12 right way there.

00:17:12 --> 00:17:16 >> Yeah. Um, so you've got the raw material

00:17:16 --> 00:17:20 of stars, but um, it doesn't form a

00:17:20 --> 00:17:25 stellar population. Um, and maybe um,

00:17:25 --> 00:17:27 it's because there's, you know, as I

00:17:27 --> 00:17:30 said, the gas is too hot. So this

00:17:30 --> 00:17:33 particular object, Cloud9, it's not very

00:17:34 --> 00:17:37 far away. Uh, it is about 14 million

00:17:37 --> 00:17:40 light years away. Uh, which puts it

00:17:40 --> 00:17:42 really on our galactic doorstep. Uh it's

00:17:42 --> 00:17:45 not far from uh a spiral galaxy called

00:17:45 --> 00:17:50 Messier 94 uh which is a lovely spiral

00:17:50 --> 00:17:51 uh if I remember rightly in the northern

00:17:51 --> 00:17:54 hemisphere sky. Uh well it must be

00:17:54 --> 00:17:55 because it's being observed by a

00:17:55 --> 00:17:57 telescope that um I never really had

00:17:57 --> 00:18:00 anything to do with but I knew its site

00:18:00 --> 00:18:01 well because it was built on a place

00:18:01 --> 00:18:03 where I used to observe a lot. Uh this

00:18:03 --> 00:18:07 is the Grand Telescopio Canaras uh which

00:18:07 --> 00:18:10 is the big Canarian telescope. It's

00:18:10 --> 00:18:11 actually the biggest optical telescope

00:18:11 --> 00:18:13 in the world. It has a 10 m mirror.

00:18:13 --> 00:18:17 >> Um, and it's located

00:18:17 --> 00:18:19 in La Palma in the Canary Islands and I

00:18:19 --> 00:18:21 used to observe there on a telescope

00:18:21 --> 00:18:23 called the William Roshaw telescope. So

00:18:23 --> 00:18:25 uh GTC as it's called Grand Telescopio

00:18:26 --> 00:18:30 Canarius has a a camera um uh called

00:18:30 --> 00:18:34 Hyper Cam uh which is the one that I

00:18:34 --> 00:18:37 think has really given us this research

00:18:37 --> 00:18:40 on Cloud9 because the uh the colleagues

00:18:40 --> 00:18:44 who observed uh this object what they

00:18:44 --> 00:18:46 did was they used that big telescope

00:18:46 --> 00:18:49 with its um wide-angle camera uh in

00:18:49 --> 00:18:53 order to get very very deep images and

00:18:53 --> 00:18:55 by deep images we mean ones that

00:18:55 --> 00:18:58 penetrate to really faint levels. Uh

00:18:58 --> 00:19:02 they got 2 hours of integration uh

00:19:02 --> 00:19:06 which is quite quite a long time. Uh and

00:19:06 --> 00:19:09 didn't see any stars. I think they they

00:19:09 --> 00:19:12 think they might have seen a small

00:19:12 --> 00:19:16 number of stars but not uh a what we

00:19:16 --> 00:19:21 expect in a galaxy. Um so the uh one of

00:19:21 --> 00:19:25 the authors of this paper um basically

00:19:25 --> 00:19:27 in offering an explanation of as to how

00:19:27 --> 00:19:31 you could have a galaxy with no stars uh

00:19:31 --> 00:19:32 I'll quote the leading theoretical

00:19:32 --> 00:19:35 explanation involves the ultraviolet

00:19:35 --> 00:19:37 background radiation that permeates the

00:19:37 --> 00:19:39 universe. Uh after the epoch of

00:19:40 --> 00:19:41 reionization

00:19:41 --> 00:19:43 uh that's right at the beginning this

00:19:43 --> 00:19:45 radiation field heats the gas in low

00:19:45 --> 00:19:48 mass dark matter halos to temperatures

00:19:48 --> 00:19:50 high enough that the gas cannot cool

00:19:50 --> 00:19:52 efficiency and collapse to form stars. I

00:19:52 --> 00:19:53 think that might be what I said earlier

00:19:53 --> 00:19:56 which is good. And so um when they do

00:19:56 --> 00:19:58 simulations

00:19:58 --> 00:20:01 um of uh you know the basically what

00:20:01 --> 00:20:03 this galaxy how it might have evolved

00:20:03 --> 00:20:05 sure enough it remains starless. They

00:20:05 --> 00:20:09 don't have any stars. So this looks like

00:20:09 --> 00:20:12 uh look like looks like a the first real

00:20:12 --> 00:20:15 example of something that people have

00:20:15 --> 00:20:18 thought must exist. Um and again quoting

00:20:18 --> 00:20:22 from it's Dr. Trujill Trujillo who I

00:20:22 --> 00:20:23 think I might have worked with in La

00:20:23 --> 00:20:27 Palma many many years ago uh says cloud9

00:20:28 --> 00:20:30 has a halo mass consistent with this

00:20:30 --> 00:20:32 regime. In this picture, starless

00:20:32 --> 00:20:36 galaxies are not exotic anomalies, but a

00:20:36 --> 00:20:38 natural and abundant prediction of

00:20:38 --> 00:20:40 standard cosmological models. The

00:20:40 --> 00:20:43 challenge has simply been finding them.

00:20:43 --> 00:20:45 So, um maybe it's not such an unusual

00:20:45 --> 00:20:49 thing after all. Uh but, uh something

00:20:49 --> 00:20:52 that has been predicted, but yes, the

00:20:52 --> 00:20:54 first I think the first one that we can

00:20:54 --> 00:20:58 really be sure uh is a starless galaxy.

00:20:58 --> 00:21:01 >> Yeah, very very unusual. Um, I'd suppose

00:21:01 --> 00:21:05 the description failed galaxy would be

00:21:05 --> 00:21:06 probably accurate given the

00:21:06 --> 00:21:07 circumstances.

00:21:08 --> 00:21:10 >> Yes, if you if you think of a normal

00:21:10 --> 00:21:12 galaxy as being populated by stars, it

00:21:12 --> 00:21:15 is. Um, but you you can see that there's

00:21:15 --> 00:21:17 good reason for it to fail. If the if

00:21:17 --> 00:21:19 the temperature of the background gas

00:21:19 --> 00:21:21 and the dark matter that's in it are too

00:21:21 --> 00:21:24 high for stars to form

00:21:24 --> 00:21:27 >> um and you might consider it a success

00:21:27 --> 00:21:30 because it's a purely gaseous galaxy.

00:21:30 --> 00:21:33 Yeah. Yeah. Uh I suppose one day it

00:21:33 --> 00:21:36 might merge with another galaxy and then

00:21:36 --> 00:21:39 you know all hell would break loose.

00:21:39 --> 00:21:40 >> That No, you're right. That's a good

00:21:40 --> 00:21:43 point because it's not that far from M94

00:21:43 --> 00:21:46 which is a big galaxy. Uh this is a it

00:21:46 --> 00:21:48 counts as a dwarf galaxy. I didn't

00:21:48 --> 00:21:50 really make that clear. And of course

00:21:50 --> 00:21:53 our our own galaxy has dwarf galaxies in

00:21:53 --> 00:21:55 orbit around it most of which contain

00:21:55 --> 00:21:59 stars. Uh and so and the fate of those

00:21:59 --> 00:22:00 dwarf galaxies is basically to become

00:22:00 --> 00:22:03 part of the of the bigger galaxy. So it

00:22:04 --> 00:22:06 may be that cloud 9 eventually does that

00:22:06 --> 00:22:09 and maybe the conditions will change so

00:22:09 --> 00:22:12 that the the gas becomes um uh cool

00:22:12 --> 00:22:15 enough or or otherwise relaxed enough uh

00:22:15 --> 00:22:18 in order to start form stars.

00:22:18 --> 00:22:20 >> Okay, if you want to read all about the

00:22:20 --> 00:22:22 starless galaxy cloud9 uh there's a

00:22:22 --> 00:22:26 great article on space.com.

00:22:26 --> 00:22:30 Um Fred, we got a live viewer who has it

00:22:30 --> 00:22:33 was from do actually. Hi Lynette. Um,

00:22:33 --> 00:22:36 she says, "Uh, hello from do. How long

00:22:36 --> 00:22:39 did you stay?" I assume she means Spain.

00:22:39 --> 00:22:40 Um,

00:22:40 --> 00:22:42 >> our earlier conversation.

00:22:42 --> 00:22:45 >> Yes, we were in Spain for, uh, roughly a

00:22:45 --> 00:22:47 week. Actually, uh, I didn't tell you,

00:22:47 --> 00:22:51 but I I got, um, I got

00:22:51 --> 00:22:54 thieved from by a pickpocket.

00:22:54 --> 00:22:55 >> Oh,

00:22:55 --> 00:22:58 >> yeah. Um, but very very common thing

00:22:58 --> 00:23:01 over there. It was in Bilbo and

00:23:01 --> 00:23:02 >> Oh, we went there.

00:23:02 --> 00:23:03 >> Lovely place.

00:23:03 --> 00:23:05 >> Yeah. Did you get your binoculars nicked

00:23:05 --> 00:23:06 as well?

00:23:06 --> 00:23:12 >> No. No. I I'm very very um

00:23:12 --> 00:23:14 look, we'll use the word anal about

00:23:14 --> 00:23:16 holding on to my stuff quite literally.

00:23:16 --> 00:23:16 Yep.

00:23:16 --> 00:23:18 >> I put stuff in my pockets and I'll shove

00:23:18 --> 00:23:20 my hands in my pockets and I will not

00:23:20 --> 00:23:21 take them out.

00:23:21 --> 00:23:22 >> Yeah.

00:23:22 --> 00:23:24 >> I must look weird.

00:23:24 --> 00:23:25 >> Well, you look weird anyway, Andrew. But

00:23:25 --> 00:23:28 that's, you know, not not good. Not bad

00:23:28 --> 00:23:30 news anyway. Uh but but no, you're

00:23:30 --> 00:23:34 right. Um so I'm like that too. But um I

00:23:34 --> 00:23:39 I had a a sort of manbag. Um and um I

00:23:39 --> 00:23:41 was walking back from the Guggenheim

00:23:42 --> 00:23:43 exhibition which you probably went to

00:23:43 --> 00:23:45 see as well in Bel

00:23:45 --> 00:23:46 >> to our hotel

00:23:46 --> 00:23:50 >> and I thought I noticed a bit of a

00:23:50 --> 00:23:52 disturbance behind me. I had headphones

00:23:52 --> 00:23:54 on um noise cancelling headphones cuz I

00:23:54 --> 00:23:55 was walking.

00:23:55 --> 00:23:58 >> Yeah. Um, and when I got into the hotel,

00:23:58 --> 00:24:01 I looked in my manb bag and the zip was

00:24:01 --> 00:24:04 open and I know I'd shut it up and my

00:24:04 --> 00:24:06 binoculars were missing.

00:24:06 --> 00:24:08 >> So, man said, "Go outside and have a

00:24:08 --> 00:24:10 look. They might have thrown them away."

00:24:10 --> 00:24:13 So, went outside.

00:24:13 --> 00:24:15 Here's four policemen bailing up these

00:24:15 --> 00:24:18 two guys.

00:24:18 --> 00:24:18 >> Got them.

00:24:18 --> 00:24:19 >> And they've been they've been following

00:24:20 --> 00:24:21 them because they'd created some sort of

00:24:22 --> 00:24:25 problems in a bar. Um, and I approached

00:24:25 --> 00:24:29 one of the policemen and said, "Um,

00:24:29 --> 00:24:30 I've lost a pair of binoculars." And he

00:24:30 --> 00:24:31 just said, "Yeah, we've got your

00:24:31 --> 00:24:32 binoculars."

00:24:32 --> 00:24:33 >> Wow.

00:24:33 --> 00:24:35 >> So, I got them back.

00:24:35 --> 00:24:37 >> Fantastic.

00:24:38 --> 00:24:40 >> It Yeah. These guys had tried to throw

00:24:40 --> 00:24:42 them away when they saw the police were

00:24:42 --> 00:24:45 on them and the cops had seen it. The

00:24:45 --> 00:24:46 cop who

00:24:46 --> 00:24:48 >> dealt with me spoke great English. He

00:24:48 --> 00:24:51 was an absolute gentleman. It was uh

00:24:51 --> 00:24:53 such a good experience that man insisted

00:24:53 --> 00:24:55 on taking our photographs together and

00:24:55 --> 00:24:57 things like that afterwards.

00:24:57 --> 00:24:58 >> Well, you got very lucky, Fred. Very

00:24:58 --> 00:24:59 lucky.

00:24:59 --> 00:25:01 >> Very, very lucky indeed. Yeah,

00:25:01 --> 00:25:03 absolutely lucky. I couldn't believe it.

00:25:03 --> 00:25:05 And actually those

00:25:05 --> 00:25:06 >> uh you know, I can go on about

00:25:06 --> 00:25:09 binoculars add infinitum having written

00:25:09 --> 00:25:10 the first book in English on the history

00:25:10 --> 00:25:13 of binoculars. Uh but they were a

00:25:13 --> 00:25:15 special pair as well, quite new. They're

00:25:15 --> 00:25:18 new to me. They're um basically they

00:25:18 --> 00:25:21 were made in the 60s or sorry the the '

00:25:21 --> 00:25:23 70s but they're very very good ones and

00:25:23 --> 00:25:25 um a lot of money.

00:25:25 --> 00:25:28 >> So Starchild says um we got a few live

00:25:28 --> 00:25:30 uh viewers at the moment and Starchild

00:25:30 --> 00:25:32 says quite a few thieves in the Milky

00:25:32 --> 00:25:34 Way.

00:25:34 --> 00:25:35 >> Yes, that's right.

00:25:35 --> 00:25:39 >> Yeah. Um and there was another question.

00:25:39 --> 00:25:42 Uh oh, good says good to see you two

00:25:42 --> 00:25:43 together again. Moose says how much did

00:25:44 --> 00:25:47 I miss? Uh about that much.

00:25:47 --> 00:25:49 I think we're a bit past halfway, Moose.

00:25:49 --> 00:25:53 And um another question. Um how many

00:25:53 --> 00:25:55 light years across is a dwarf galaxy? I

00:25:55 --> 00:25:57 guess they're all different sizes. They

00:25:57 --> 00:26:00 are, but it's a good question. I mean um

00:26:00 --> 00:26:02 so think of our galaxy, which is kind of

00:26:02 --> 00:26:06 100 lighty years across. Um and

00:26:06 --> 00:26:09 that's typical of a of a major spiral

00:26:09 --> 00:26:13 galaxy. A dwarf galaxy would probably be

00:26:13 --> 00:26:16 less than a tenth of that. Um 10

00:26:16 --> 00:26:18 light years, that sort of size, you

00:26:18 --> 00:26:21 know, just on on on average, that kind

00:26:21 --> 00:26:23 of that kind of size.

00:26:23 --> 00:26:25 >> Okay, thanks for the question. It

00:26:25 --> 00:26:27 doesn't happen like this very often, but

00:26:27 --> 00:26:28 today

00:26:28 --> 00:26:30 we've got an active audience. That's

00:26:30 --> 00:26:32 good.

00:26:32 --> 00:26:34 >> Yeah. All right. Uh you're listening to

00:26:34 --> 00:26:36 Space Nuts, by the way, uh with Andrew

00:26:36 --> 00:26:40 Dunley and Professor Fred Watson.

00:26:40 --> 00:26:43 Okay, we checked all four systems and

00:26:43 --> 00:26:44 >> space nets.

00:26:44 --> 00:26:47 >> Our final topic, Fred, takes us to

00:26:47 --> 00:26:50 Venus. Sunny Venus. Oh, yes. What a

00:26:50 --> 00:26:52 place. Go outside, take a deep breath,

00:26:52 --> 00:26:55 drop dead. Um, but there's some news

00:26:55 --> 00:26:57 about Venus, which involves its clouds

00:26:57 --> 00:26:59 again. Now, the last time this was big

00:26:59 --> 00:27:01 news was when they thought they might

00:27:01 --> 00:27:03 have found um signs of life in the

00:27:03 --> 00:27:05 clouds. That's still under a lot of

00:27:05 --> 00:27:08 speculation and debate. But what's the

00:27:08 --> 00:27:10 latest with these clouds? The these

00:27:10 --> 00:27:11 aren't the the ones we were talking

00:27:12 --> 00:27:13 about last time. These these are a

00:27:13 --> 00:27:15 little bit different again. Yes, they

00:27:16 --> 00:27:17 are. Yeah. So, I think that was sulfur

00:27:17 --> 00:27:19 was it sulfur dioxide? I can't remember

00:27:19 --> 00:27:22 the um the detection which uh which

00:27:22 --> 00:27:24 people got excited because it might been

00:27:24 --> 00:27:26 living organisms in the upper atmosphere

00:27:26 --> 00:27:28 of Venus, but I think that's gone away

00:27:28 --> 00:27:31 now. Um, it's great to talk about Venus,

00:27:31 --> 00:27:33 especially just now because you would

00:27:33 --> 00:27:35 know, Andrew, it's absolutely lighting

00:27:35 --> 00:27:37 up the evening sky, uh, over there in

00:27:38 --> 00:27:39 the west. It is very bright, very high

00:27:40 --> 00:27:41 in the sky.

00:27:41 --> 00:27:43 >> Beautiful object. And when we look at

00:27:43 --> 00:27:47 it, it's kind of got a yellowish color.

00:27:47 --> 00:27:49 Uh, which is because we're seeing

00:27:49 --> 00:27:51 reflections from the top of its cloud

00:27:51 --> 00:27:56 layer. Um but uh it's been known for a

00:27:56 --> 00:27:59 long time that if you photograph Venus

00:28:00 --> 00:28:04 in with ultraviolet light you you see

00:28:04 --> 00:28:08 patterns really dramatic patterns and I

00:28:08 --> 00:28:09 I haven't got one in front of me now but

00:28:09 --> 00:28:11 I do remember photographs of this that

00:28:11 --> 00:28:13 these are sort of globalized patterns

00:28:14 --> 00:28:17 that actually move uh with the the

00:28:17 --> 00:28:20 clouds of Venus. And as we know, I think

00:28:20 --> 00:28:23 most space notes uh listeners and

00:28:23 --> 00:28:25 viewers would know that we don't

00:28:25 --> 00:28:26 actually see the surface of Venus

00:28:26 --> 00:28:29 directly. We can with radar uh certain

00:28:29 --> 00:28:31 infrared observations that let you

00:28:31 --> 00:28:32 penetrate to the surface, but basically

00:28:32 --> 00:28:35 all we see uh and certainly in

00:28:35 --> 00:28:37 ultraviolet is the upper parts of the of

00:28:37 --> 00:28:40 the cloud belts, cloud layers.

00:28:40 --> 00:28:43 >> So the markings themselves uh are a

00:28:43 --> 00:28:47 puzzle. And um this is where it sort of

00:28:47 --> 00:28:49 gets interesting, although it's not one

00:28:49 --> 00:28:50 of these stories that's got a neat and

00:28:50 --> 00:28:53 tidy answer, I'm afraid. Um there's

00:28:53 --> 00:28:56 there's a chemical that is thought to be

00:28:56 --> 00:28:59 in Venus's upper atmosphere,

00:28:59 --> 00:29:02 which is called the unknown absorber.

00:29:02 --> 00:29:06 Uh and because uh it absorbs light uh in

00:29:06 --> 00:29:08 the ultraviolet, and you get dark

00:29:08 --> 00:29:12 patches from from this this stuff. Um, I

00:29:12 --> 00:29:14 was talking to somebody about this the

00:29:14 --> 00:29:15 other day and they said it sounds like a

00:29:15 --> 00:29:18 superhero, the unknown absorber. Uh,

00:29:18 --> 00:29:20 which, uh, I think probably would work

00:29:20 --> 00:29:22 well. Yeah.

00:29:22 --> 00:29:25 >> His superhero name would be the sponge.

00:29:25 --> 00:29:28 >> The sponge. That's right.

00:29:28 --> 00:29:33 So what's happened is that um a team an

00:29:33 --> 00:29:35 international team actually of basically

00:29:35 --> 00:29:38 astrobiologists people who are looking

00:29:38 --> 00:29:42 at uh the origin of life in the universe

00:29:42 --> 00:29:44 and what we need for life to form and

00:29:44 --> 00:29:46 all of those other good things not

00:29:46 --> 00:29:47 necessarily trying to find life but

00:29:47 --> 00:29:49 trying to understand life. um what

00:29:50 --> 00:29:53 they've done uh they've essentially this

00:29:53 --> 00:29:56 this research team I think they've done

00:29:56 --> 00:29:59 very cluey kind of modeling

00:29:59 --> 00:30:03 um of the droplets within the clouds of

00:30:03 --> 00:30:08 Venus to try and not identify what this

00:30:08 --> 00:30:12 unknown absorber is but sort of um place

00:30:12 --> 00:30:15 limits on its properties you know it

00:30:15 --> 00:30:18 does this but it doesn't do that uh and

00:30:18 --> 00:30:19 it does this to to this extent, but it

00:30:19 --> 00:30:22 doesn't do that to this extent. So, it's

00:30:22 --> 00:30:25 uh it's all about trying to model what

00:30:25 --> 00:30:28 cloud droplets would look like to

00:30:28 --> 00:30:30 actually reproduce what we see when we

00:30:30 --> 00:30:35 observe the planet. Um so,

00:30:35 --> 00:30:39 uh one of the authors of the paper

00:30:39 --> 00:30:43 basically poses a question. Uh, if we

00:30:43 --> 00:30:46 were to collect Venus's cloud droplets,

00:30:46 --> 00:30:48 and I'm paraphrasing here, into a

00:30:48 --> 00:30:52 bucket, how would the reformed bulk

00:30:52 --> 00:30:53 liquid appear?

00:30:53 --> 00:30:55 >> Uh, the scientist actually said a

00:30:55 --> 00:30:58 spectrometric cuette, but a bucket's as

00:30:58 --> 00:31:01 good an analogy for that as you need. If

00:31:01 --> 00:31:02 you could collect the droplets, what

00:31:02 --> 00:31:08 would it look like? Um and that is the

00:31:08 --> 00:31:11 sort of key to the modeling that's been

00:31:11 --> 00:31:15 done. Um they there's a comment um I

00:31:15 --> 00:31:17 think it might come from the original

00:31:17 --> 00:31:20 paper but um fsdoc.org has got a very

00:31:20 --> 00:31:23 nice article on this uh and I think it

00:31:23 --> 00:31:26 may even come from their press release.

00:31:26 --> 00:31:30 Uh but basically it's um likening the

00:31:30 --> 00:31:33 droplets in the clouds of Venus to

00:31:33 --> 00:31:37 cigarette smoke. Uh because um cigarette

00:31:37 --> 00:31:40 smoke is tiny particles, tar tiny tarry

00:31:40 --> 00:31:42 particles

00:31:42 --> 00:31:45 um which look sort of white or bluish

00:31:45 --> 00:31:47 because of the scattering of light.

00:31:47 --> 00:31:49 Because these things are so small they

00:31:49 --> 00:31:51 scatter light very effectively. But if

00:31:51 --> 00:31:53 you collected it into a flask, you got

00:31:53 --> 00:31:57 this horrible sludge uh t- like sludge.

00:31:57 --> 00:31:59 Of course, that is what ends up in your

00:31:59 --> 00:32:01 lungs if you're a smoker.

00:32:01 --> 00:32:05 >> Um yeah. So what they're suggesting is

00:32:05 --> 00:32:08 that there's a similar phenomenon

00:32:08 --> 00:32:10 happening in Venus's clouds. Uh because

00:32:10 --> 00:32:13 the particle size of the droplets in

00:32:13 --> 00:32:15 Venus's upper atmosphere are comparable

00:32:15 --> 00:32:18 to the particle size of cigarette smokes

00:32:18 --> 00:32:21 smoke. So even though um you know even

00:32:21 --> 00:32:24 though the clouds with the with visible

00:32:24 --> 00:32:27 light look that sort of yellowish color

00:32:28 --> 00:32:31 that we've mentioned already, the actual

00:32:31 --> 00:32:34 droplets themselves could be really

00:32:34 --> 00:32:36 really dark and it's only because they

00:32:36 --> 00:32:37 scatter the light in a certain way that

00:32:37 --> 00:32:40 they look that they look yellowish.

00:32:40 --> 00:32:44 Um so this basically this uh research is

00:32:44 --> 00:32:46 asking that question. What h what would

00:32:46 --> 00:32:48 happen if you could collect a cloud of

00:32:48 --> 00:32:50 material from the atmosphere of Venus

00:32:50 --> 00:32:52 and put it into a

00:32:52 --> 00:32:57 basically you know a a flask or a or a

00:32:57 --> 00:33:00 beaker or something like that. Um and

00:33:00 --> 00:33:03 that's where this analysis has gone and

00:33:03 --> 00:33:06 they've used something it's words that

00:33:06 --> 00:33:08 used to strike terror into me when I was

00:33:08 --> 00:33:10 a student in astronomy Andrew and I

00:33:10 --> 00:33:11 don't know whether I've uttered them

00:33:11 --> 00:33:15 ever since. radiative transfer. Uh

00:33:15 --> 00:33:17 radiative transfer is the way radiation

00:33:17 --> 00:33:22 moves around uh among atoms. Uh and it's

00:33:22 --> 00:33:25 very very intense mathematics. So these

00:33:25 --> 00:33:27 scientists obviously like that kind of

00:33:27 --> 00:33:30 thing. I'm afraid I didn't. uh and have

00:33:30 --> 00:33:32 built a radiative transfer model that uh

00:33:32 --> 00:33:36 actually lets you um account for not

00:33:36 --> 00:33:38 just single scattering but multiple

00:33:38 --> 00:33:40 scattering because you've you've got to

00:33:40 --> 00:33:42 um take into account that light might

00:33:42 --> 00:33:44 scatter from one of those droplets and

00:33:44 --> 00:33:46 then hit another one and scatter from

00:33:46 --> 00:33:48 that. So you've got multiple scattering

00:33:48 --> 00:33:53 phenomena. Um and so uh they have

00:33:53 --> 00:33:56 basically done that and produced what is

00:33:56 --> 00:33:59 called the absorption coefficient of the

00:33:59 --> 00:34:01 bulk cloud liquid. That's the how it

00:34:01 --> 00:34:04 would absorb um if you just had a flask

00:34:04 --> 00:34:07 of this stuff. Now what they're saying

00:34:07 --> 00:34:09 is that they don't really know what this

00:34:09 --> 00:34:12 these droplets are, but they're not

00:34:12 --> 00:34:15 suggesting its life. Um they've they've

00:34:15 --> 00:34:18 put limits on the absorption

00:34:18 --> 00:34:24 coefficient. Um and uh essentially

00:34:24 --> 00:34:26 again paraphrasing the uh press release

00:34:26 --> 00:34:29 from f.org uh the result implies that

00:34:29 --> 00:34:32 the unknown absorber must either absorb

00:34:32 --> 00:34:36 light very efficiently, occur at a very

00:34:36 --> 00:34:39 high concentration or both. Uh my guess

00:34:39 --> 00:34:42 is it's going to be both. Um, so, uh,

00:34:42 --> 00:34:45 it's it's some sort of probably some

00:34:45 --> 00:34:47 sort of organic compound, and by that I

00:34:47 --> 00:34:49 mean one that contains carbon rather

00:34:49 --> 00:34:52 than one that contains living organisms.

00:34:52 --> 00:34:55 Um, and they've basically, you know,

00:34:55 --> 00:34:57 they've suggested some chemicals that

00:34:57 --> 00:35:01 might actually be be responsible for

00:35:01 --> 00:35:03 this. Uh, excluding, they say

00:35:03 --> 00:35:05 chlorophyll. Chlorophyll, of course,

00:35:05 --> 00:35:08 very important in life processes. uh but

00:35:08 --> 00:35:09 they're excluding they're saying they're

00:35:09 --> 00:35:12 not proposing chlorophyll as as a as an

00:35:12 --> 00:35:15 example. So uh as I said it's a story

00:35:15 --> 00:35:18 that doesn't have a conclusion uh but

00:35:18 --> 00:35:21 it's interesting to think of the the

00:35:21 --> 00:35:22 clouds of Venus that if you could

00:35:22 --> 00:35:25 collect them in a bucket or a container

00:35:25 --> 00:35:27 they could be very very dark mixtures

00:35:27 --> 00:35:31 like tar a sort of sludge of of tar

00:35:31 --> 00:35:36 which um would be interesting.

00:35:36 --> 00:35:38 Yeah, it's um

00:35:38 --> 00:35:40 it's a classic example of a failed

00:35:40 --> 00:35:43 earthlike world.

00:35:43 --> 00:35:45 >> Yes, that's right. Yes, indeed. We don't

00:35:45 --> 00:35:47 have things like this on in our planet,

00:35:47 --> 00:35:49 thankfully.

00:35:49 --> 00:35:50 >> Yeah. Um

00:35:50 --> 00:35:52 >> I think there's more um Sorry, Andrew,

00:35:52 --> 00:35:53 just to finish the story, I think

00:35:53 --> 00:35:57 there's more research being designed

00:35:57 --> 00:36:02 possibly looking uh uh with a a future

00:36:02 --> 00:36:05 mission to Venus. uh perhaps looking for

00:36:05 --> 00:36:08 fluoresence in the uh in the clouds

00:36:08 --> 00:36:10 because that would give them another

00:36:10 --> 00:36:13 angle on what this stuff is.

00:36:13 --> 00:36:16 >> Okay, we watch with interest. Uh yeah,

00:36:16 --> 00:36:18 Venus keeps throwing up curve balls. The

00:36:18 --> 00:36:19 uh

00:36:19 --> 00:36:20 >> just doesn't

00:36:20 --> 00:36:22 >> the potential for life in the clouds

00:36:22 --> 00:36:24 because of the discovery of phosphine

00:36:24 --> 00:36:28 and now this um a bucket of tar. Yay.

00:36:28 --> 00:36:31 What a place. Next holiday, I think.

00:36:31 --> 00:36:33 Well, yeah. Plus, you've got the

00:36:33 --> 00:36:34 sulfuric acid as well.

00:36:34 --> 00:36:36 >> Oh, that's true. Yes. Yes. And and the

00:36:36 --> 00:36:39 um undeniable level of heat. I think

00:36:39 --> 00:36:40 Australians could handle it and a few

00:36:40 --> 00:36:42 other places in the world, but most No,

00:36:42 --> 00:36:44 most people couldn't. It's horrible.

00:36:44 --> 00:36:46 It's an horrible place, but very pretty

00:36:46 --> 00:36:48 in the sky at the moment.

00:36:48 --> 00:36:49 >> It is.

00:36:49 --> 00:36:51 >> Uh you can read all about it at f.org as

00:36:51 --> 00:36:53 Fred said or you can read the entire

00:36:53 --> 00:36:55 paper which was published in

00:36:55 --> 00:36:57 astrobiology.

00:36:57 --> 00:36:59 And that brings us to the end. Fred,

00:36:59 --> 00:37:01 thank you very much.

00:37:01 --> 00:37:02 Uh, it's a pleasure, Andrew. Um, it's

00:37:02 --> 00:37:05 always good to chat and um, even better

00:37:05 --> 00:37:08 to chat when you're half asleep.

00:37:08 --> 00:37:10 >> You did well. You did well. For those

00:37:10 --> 00:37:13 who joined us late, um, you'll have to

00:37:13 --> 00:37:14 listen to the episode, get the full

00:37:14 --> 00:37:18 explanation of Fred's sleepiness. Um,

00:37:18 --> 00:37:20 it's got something to do with um,

00:37:20 --> 00:37:24 painkillers. Anyway, we'll get on uh,

00:37:24 --> 00:37:25 hopefully he'll brighten up for the next

00:37:25 --> 00:37:27 episode. I suspect not.

00:37:27 --> 00:37:29 >> Um, thank you, Fred. We'll catch you

00:37:29 --> 00:37:30 soon.

00:37:30 --> 00:37:32 Sounds great. Thank Thanks, Andrew.

00:37:32 --> 00:37:34 >> Professor Fred Watson, astronomer at

00:37:34 --> 00:37:36 large. And don't forget to visit us at

00:37:36 --> 00:37:38 our website between episodes, which you

00:37:38 --> 00:37:40 can do at spaceenutspodcast.com

00:37:40 --> 00:37:44 or spacenuts.io. Have a look around and

00:37:44 --> 00:37:46 um see what's there. The shop, you can

00:37:46 --> 00:37:49 send us messages, you can sign up for

00:37:49 --> 00:37:50 astronomy daily. Plenty of things to see

00:37:50 --> 00:37:51 and do. And don't forget to leave

00:37:51 --> 00:37:54 reviews about our podcast wherever you

00:37:54 --> 00:37:56 listen to us. And thanks to Hugh in the

00:37:56 --> 00:37:58 studio who couldn't be with us today

00:37:58 --> 00:38:00 because he discovered that he's um he's

00:38:00 --> 00:38:03 more at home in a starless galaxy. And

00:38:03 --> 00:38:04 from me, Andrew Dunley, thanks for your

00:38:04 --> 00:38:06 company. See you on the next episode of

00:38:06 --> 00:38:08 Space Nuts. Bye-bye.

00:38:08 --> 00:38:09 >> Space Nuts.

00:38:09 --> 00:38:11 >> You'll be listening to the Space Nuts

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