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
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Hi there. Thanks for joining us. This is
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Space Nuts. My name is Andrew Dunley,
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your host. And it is good to have your
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company as always. Uh coming up on this
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episode. Uh we're going to revisit the
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Spanish eclipse because the man of the
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moment, the man who went there and
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pointed it out to everyone and said
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that's what an eclipse looks like, he
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couldn't join us. But Fred Watson will
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talk about it. Uh we'll also be uh
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discussing the Nancy um Roman uh uh
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observatory launch which I watched
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online the other the other night which
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was spectacular. Uh and there's a
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there's a galaxy that they're looking at
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with um a bit of a frown and a scratch
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of the neck because uh it does not
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appear to have many stars. Uh it's not
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emitting starlight. How could that be?
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And we'll finish up with the mystery
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clouds of Venus. That's all coming up on
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this episode of Space Nuts.
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>> 15 seconds. Guidance is internal. 10 9g
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Ignition sequence start.
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>> Space nuts.
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>> 5 4 3 2 1 2 3 4 5 5 4 3 2 1
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>> Space Nuts.
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>> Astronauts report. It feels good.
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and he's back after traveling halfway
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around the world and returning and then
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getting his leg um amputated. Well, not
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quite, but uh he got it rebuilt. $6
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million. It was I think the price of
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that. Uh it's Professor Fred Watson,
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astronomer at large. Hello, Fred.
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>> Hi, Andrew. Thank you for that great
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intro. Yes, $6 million. Um and my health
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fund provided $42.50. So,
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>> yes, that's usually how it goes in
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Australia. Um, that's the going rate. No
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matter what it cost you to go and see a
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doctor, you get 40 bucks back.
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>> Yeah, it's a great system. Um, yeah.
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Anyway, we won't go there. That's
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politics.
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>> Yeah, that's right. But as you alluded,
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uh, I have indeed received a new knee.
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So, I had a my second T TKR, total knee
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replacement.
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>> Wow.
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>> Um, which is, uh, it was a week ago.
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Yesterday was the surgery. So, I'm still
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on painkillers, so will not make any
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sense whatsoever. Um, I might go to
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sleep halfway through the show. That's
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been one of the symptoms.
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>> Well, between you falling asleep and me
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sneezing, it should be an interesting
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show. Hay fever is running right here at
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the moment,
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>> and I I cannot control it. Um, I know
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there's medications out there, but I'm
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some I'm not allowed to take anymore
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because of my eyes.
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>> So, it's made it more complicated. So,
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um, I'm I'm I'm well armed. Look, I've
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got Oh, yes. the mandatory box of
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tissues within arms length. So hopefully
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we'll get through it, Fred. And um I'm
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glad the knee operation went well.
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You're the second person in a week that
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I've met who's had a total knee
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replacement. A friend of mine um
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>> literally stepped into a hole that he
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didn't know was there because it was
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full of grass and buckled his knee and
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the damage was too severe and they had
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to do a a knee replacement. Bit of a
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shocker that one.
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>> Yes.
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>> But um he's still on crutches.
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>> Okay. Well, I've parked my crutches,
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although I did resort to one in the
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middle of the night uh when I had to get
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up. Uh I thought I'm just going to use
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the crotch that came this time. But
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yeah, um it doesn't take long. But um
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you know, your colleague uh uh there, he
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had much more than just a knee
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replacement with that accident damage.
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Mine was just a quick one out, one in.
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Uh and so I think it's a lot more
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predictable and probably a lot easier
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for me to recover. Um, I'm sorry he's
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still on crutches and hope he I wish him
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well. We used to speak on the radio a
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long time ago.
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>> That's right. One of my old radio mates.
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>> Uh, Fred, let's talk about the Spanish
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Eclipse. I saw a lot of pictures and
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footage online. People getting very
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artistic with their photography at
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times. Uh, these things have become very
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popular.
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>> And, uh, from what I could tell, it was
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it was a little bit different because it
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wasn't sort of up there. It was over
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there. Is that how it went? It was more
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on the horizon than than you'd normally
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expect.
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>> That's right. It was um and that was
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always the issue for us uh because at
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the time of totality it was only 9°
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above the western horizon and that's
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very low down. Um but we figured that we
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would take that risk. Uh the story
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actually goes back a long way. So so we
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were leading a tour group. We had uh uh
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16 16 of us through France and Spain and
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Switzerland. We went to Large Hadron
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Collider. We went to two observatories
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in France uh or Puvance and Pipidi, both
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of which were sensational. We really
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enjoyed those visits and wound up at um
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Santandere in northern Spain. Uh we we
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got there I think three days before the
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eclipse. Um, and the first thing Mani
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and I did was to basically stake out
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where we were going to watch it from.
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Uh, because, um, in those resorts in
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northern Spain on the coast, uh, they're
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all built facing eastwards because they
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get the morning sun and often there is
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high ground behind them and and so we um
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found a spot about 2 kilometers from our
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hotel. We had a couple of vehicles so we
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could manipulate everything. Um Manne um
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bought a gazebo uh which we erected on
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our chosen spot. There was nobody there
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at that time, but we knew it was going
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to fill up. Uh so we had this gazebo. Um
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we the first night I said, "This is
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going to blow away if we just leave it
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here." So So we parked one of our
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vehicles under the gazebo and tied the
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gazebo down onto the roof of the car.
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Still there the next day. Yeah.
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>> And so the next day, but the gazebo was
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That's right. So, yeah, it turned into
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quite a big event. There were there were
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very big crowds there. We'd obviously
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chosen exactly the right spot. Um, lots
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of people. An ice cream van was there
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that turned up on day two.
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>> Oh, wow.
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>> Day tminus one. Um, a whole lot of cops
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came on horseback and in vehicles and in
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helicopters. They were obviously all
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taken completely by surprise by this
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event. What's going on up there? Um but
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yes on the afternoon so it was an
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evening eclipse the afternoon uh the sky
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was completely clear but uh towards the
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end of the afternoon this bank of cloud
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appeared in the west uh and you could
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see that it was sort of spreading
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upwards as it approached.
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>> So the sun was effectively setting into
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that. The partial phase started at half
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7. We got I spotted that with the
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binoculars. It was a magical moment when
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I first saw the mountains of the moon
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just encroaching into the sun's disc.
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This was with binoculars with filters.
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Uh and then we, you know, eclipses are
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an amazing spectacle. You've got this
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buildup over an hour or so as the moon's
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disc gradually covers the sun and then
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that time of perfection when it's when
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the two are exactly aligned. So what
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happened? We all got steadily more and
00:07:08.800 --> 00:07:10.550
more depressed as the sun was sinking
00:07:10.560 --> 00:07:13.830
into this bank of cloud. But about 2
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minutes before totality, a hole opened
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up uh right where the sun was. And when
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the total eclipse happened, we got a
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perfect view of the corona. It was just
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magical. It was clear. Um so we could
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see the outer atmosphere of the sun. The
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corona looked slightly yellowish and
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that's because the sun was so low.
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Normally pure white
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>> and pink clouds of hydrogen which were
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bigger than I've seen before. They were
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spectacular. Lots of cheers from the
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crowd. There were about 2,000 people
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there by then. Uh we in our little tent,
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there were 20 of us, too, cuz two
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members of my UK family or four members
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came out to watch. So, a good time was
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had by all.
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>> Uh and we were delighted to to get a
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great eclipse and I think everybody was
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very happy. And I spent the next
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>> I was going to say, isn't it twice in a
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row that you've been to an eclipse that
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was cloudy and it cleared up at the last
00:08:04.800 --> 00:08:05.029
second?
00:08:05.039 --> 00:08:07.510
>> Cleared up. That's right. Um not nearly
00:08:07.520 --> 00:08:09.189
twice in a It was the one before last, I
00:08:09.199 --> 00:08:09.749
think. Was
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>> Oh, yeah.
00:08:10.639 --> 00:08:13.189
>> Uh, no. Was it the last one? Yes, it was
00:08:13.199 --> 00:08:15.029
the last one. It was in Texas. That's
00:08:15.039 --> 00:08:15.830
right.
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>> Uh, and it was cloudy. Uh, and then the
00:08:18.800 --> 00:08:20.469
holes appeared and
00:08:20.479 --> 00:08:22.550
>> we we saw the eclipse. So,
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>> yeah, some somebody's looking after us.
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I don't know who is looking after us. It
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was great.
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>> Um, yeah. And that sort of wrapped up
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the tour. Then we had a couple of days.
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Uh, we had I won't bore you with the
00:08:33.680 --> 00:08:35.350
details. We had a nightmare journey
00:08:35.360 --> 00:08:36.149
home.
00:08:36.159 --> 00:08:39.750
>> Oh. which involved rebooking flights uh
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two hours before they left through to
00:08:41.519 --> 00:08:44.310
Sim from Barcelona. But anyway, that's
00:08:44.320 --> 00:08:45.509
another story.
00:08:45.519 --> 00:08:46.949
>> Travelers tales, you've got plenty of
00:08:46.959 --> 00:08:47.829
them as well.
00:08:47.839 --> 00:08:51.590
>> Yeah. Yeah. Yeah. Um I I guess the
00:08:51.600 --> 00:08:53.670
difference with that eclipse in Spain
00:08:53.680 --> 00:08:56.310
was it was happening at sunset. And
00:08:56.320 --> 00:08:57.829
normally when you watch one of these
00:08:57.839 --> 00:09:01.030
eclipses, it turns day into night and
00:09:01.040 --> 00:09:03.110
then it comes back to day again. But at
00:09:03.120 --> 00:09:05.030
sunset, I guess you sort of missed out
00:09:05.040 --> 00:09:07.190
on that kind of effect to a certain
00:09:07.200 --> 00:09:08.070
degree.
00:09:08.080 --> 00:09:09.829
>> Yeah, to a excuse me, to a certain
00:09:09.839 --> 00:09:11.910
extent because it but it got dark very
00:09:11.920 --> 00:09:14.230
quickly as it does. It's only
00:09:14.240 --> 00:09:16.790
>> when the something like 80 or 90% of the
00:09:16.800 --> 00:09:18.470
sun's disc is covered. That's the only
00:09:18.480 --> 00:09:20.470
time when you notice the that things are
00:09:20.480 --> 00:09:23.269
dimming. Um I think birds did go to
00:09:23.279 --> 00:09:24.710
sleep. We didn't really take much
00:09:24.720 --> 00:09:27.190
notice. It was um 1 minute and 3 seconds
00:09:27.200 --> 00:09:29.269
was the time of totality that we had.
00:09:29.279 --> 00:09:32.310
>> Yeah. Uh um but yes, it did get light
00:09:32.320 --> 00:09:34.949
again. Uh light enough for us to take
00:09:34.959 --> 00:09:36.550
lots of photographs of each other and
00:09:36.560 --> 00:09:38.710
all the rest of it. Uh we demolished the
00:09:38.720 --> 00:09:41.509
gazebo, gave it to a guy, a French guy
00:09:41.519 --> 00:09:43.750
who thought it was the bees knees. He he
00:09:43.760 --> 00:09:46.389
had a camper van next door. We also gave
00:09:46.399 --> 00:09:48.389
him the inflatable fridge that we
00:09:48.399 --> 00:09:49.110
bought.
00:09:49.120 --> 00:09:49.829
>> Oh my goodness.
00:09:49.839 --> 00:09:51.269
>> Did you know there was such a thing?
00:09:51.279 --> 00:09:52.470
>> I've never heard of it.
00:09:52.480 --> 00:09:54.870
>> My wife does. Uh, we had an inflatable
00:09:54.880 --> 00:09:56.949
fridge and we gave him some chairs as
00:09:56.959 --> 00:09:58.790
well because we couldn't take all this
00:09:58.800 --> 00:09:59.829
stuff back to Australia.
00:09:59.839 --> 00:10:00.710
>> Of course.
00:10:00.720 --> 00:10:01.190
>> Yeah.
00:10:01.200 --> 00:10:02.150
>> Fantastic.
00:10:02.160 --> 00:10:06.630
>> Yeah. Well, you know, I'm all set for do
00:10:06.640 --> 00:10:07.670
2028.
00:10:07.680 --> 00:10:10.150
>> Yeah. 2028. That's right. So,
00:10:10.160 --> 00:10:11.990
>> less than two years now.
00:10:12.000 --> 00:10:12.949
>> Not far.
00:10:12.959 --> 00:10:14.790
>> We just been sitting on this one for 20
00:10:14.800 --> 00:10:16.630
years when we first found out about it.
00:10:16.640 --> 00:10:18.150
But, uh, yeah, looking forward to that.
00:10:18.160 --> 00:10:20.870
In fact, uh I think that year um there's
00:10:20.880 --> 00:10:23.269
going to be three or four eclipses in
00:10:23.279 --> 00:10:25.110
our part of the world or over those next
00:10:25.120 --> 00:10:25.509
couple years.
00:10:25.519 --> 00:10:27.750
>> Each of the next few years, yeah, I
00:10:27.760 --> 00:10:31.509
think till 20 30 something. I can't
00:10:31.519 --> 00:10:33.670
remember what it 38.
00:10:33.680 --> 00:10:35.030
>> Yeah, I don't know. There there are
00:10:35.040 --> 00:10:36.630
another three. That's right.
00:10:36.640 --> 00:10:37.750
>> Yeah.
00:10:37.760 --> 00:10:39.670
>> Okay. Um well, that sounds like fun.
00:10:39.680 --> 00:10:40.949
Let's talk about something else
00:10:40.959 --> 00:10:42.630
extraordinary. Uh the other night I was
00:10:42.640 --> 00:10:45.030
sitting uh in my lounge just about to
00:10:45.040 --> 00:10:46.949
pop off to sleep and my brain said, "You
00:10:46.959 --> 00:10:48.710
know, they should be launching the Nancy
00:10:48.720 --> 00:10:51.430
Roman Telescope sometime soon, Andrew."
00:10:51.440 --> 00:10:52.790
So I thought, "Oh yeah, yeah."
00:10:52.800 --> 00:10:55.030
>> So I grabbed my iPad and I logged on and
00:10:55.040 --> 00:10:57.670
and sure enough, the countdown was 5
00:10:57.680 --> 00:10:59.670
minutes from launch. And I thought,
00:10:59.680 --> 00:11:02.150
>> "Isn't the brain an amazing thing?"
00:11:02.160 --> 00:11:02.550
>> Yeah.
00:11:02.560 --> 00:11:05.110
>> That it that it reminded me of that 5
00:11:05.120 --> 00:11:07.829
minutes before the launch. And and and I
00:11:07.839 --> 00:11:10.630
I was oblivious to it at that moment.
00:11:10.640 --> 00:11:12.550
So, I watched the whole thing. It was
00:11:12.560 --> 00:11:15.590
fantastic. Yeah, I I watched the replay
00:11:15.600 --> 00:11:18.069
the next day. I wasn't um switched on as
00:11:18.079 --> 00:11:19.509
you were. I was probably asleep actually
00:11:19.519 --> 00:11:23.030
with them with the with the painkillers.
00:11:23.040 --> 00:11:25.509
But yes, I did I did um realize that it
00:11:25.519 --> 00:11:27.829
was taking place then. Uh and yeah,
00:11:27.839 --> 00:11:29.430
flawless launch. It looked fantastic.
00:11:29.440 --> 00:11:30.790
>> It was, wasn't it?
00:11:30.800 --> 00:11:33.269
>> All 27 of those Merlin motors firing
00:11:33.279 --> 00:11:35.670
away there. M
00:11:35.680 --> 00:11:39.590
and it's now makes the 1 million is it
00:11:39.600 --> 00:11:42.310
kilometers or miles journey to
00:11:42.320 --> 00:11:44.069
>> uh yes a million miles a million and a
00:11:44.079 --> 00:11:46.470
half kilometers uh and I think it's well
00:11:46.480 --> 00:11:49.030
on the way this is to the the L2 point
00:11:49.040 --> 00:11:51.910
that point on the far side of the earth
00:11:51.920 --> 00:11:53.590
from the sun where there's this stable
00:11:53.600 --> 00:11:56.150
stable gravitational thing which we call
00:11:56.160 --> 00:11:58.790
a lrangee point um several spacecraft
00:11:58.800 --> 00:12:01.030
there already including the James Web
00:12:01.040 --> 00:12:03.509
and Gia the that European fantastic
00:12:03.519 --> 00:12:05.590
European project that's there. Few other
00:12:05.600 --> 00:12:06.069
ones
00:12:06.079 --> 00:12:07.350
>> they'll be running out of room up there.
00:12:07.360 --> 00:12:09.269
They'll have to put in traffic lights.
00:12:09.279 --> 00:12:11.430
>> So it's interesting. Um you kind of
00:12:11.440 --> 00:12:12.949
think of that. Oh, if this is a stable
00:12:12.959 --> 00:12:14.150
point, they must always be trying to get
00:12:14.160 --> 00:12:16.310
to the same point. But actually what
00:12:16.320 --> 00:12:18.069
they are, they're all in orbit around a
00:12:18.079 --> 00:12:19.350
stable point.
00:12:19.360 --> 00:12:21.829
>> So you're in orbit around nothing. Um
00:12:21.839 --> 00:12:24.069
but the gravitational forces work to
00:12:24.079 --> 00:12:25.670
sort of keep you keep you in orbit
00:12:25.680 --> 00:12:31.350
there. Um yep. So it's um yes. So so I I
00:12:31.360 --> 00:12:33.110
don't know. I haven't really looked at
00:12:33.120 --> 00:12:36.069
the commissioning schedule for the Nancy
00:12:36.079 --> 00:12:39.030
Grace Roman. Uh but um it's probably
00:12:39.040 --> 00:12:41.430
already started because they don't waste
00:12:41.440 --> 00:12:43.590
much time with these things to you know
00:12:43.600 --> 00:12:45.590
get as much data as they can just in
00:12:45.600 --> 00:12:47.910
case something catastrophic goes wrong
00:12:47.920 --> 00:12:50.790
early on. Um what we've got here is a
00:12:50.800 --> 00:12:54.470
Hubble class telescope um same sort of
00:12:54.480 --> 00:12:58.550
size as the Hubble uh 2.4 4 meters with
00:12:58.560 --> 00:13:01.670
uh the big difference that even though
00:13:01.680 --> 00:13:04.389
it's got the fine detail, the resolving
00:13:04.399 --> 00:13:06.550
power of the Hubble, it's got a 100
00:13:06.560 --> 00:13:09.590
times the field of view of the Hubble,
00:13:09.600 --> 00:13:12.790
>> which means it sees 100 times more sky.
00:13:12.800 --> 00:13:14.470
And so, you know, the Pubble's always
00:13:14.480 --> 00:13:17.430
been giving us these what you might call
00:13:17.440 --> 00:13:19.990
pinhole images, just almost looking
00:13:20.000 --> 00:13:22.949
through a straw at the sky. Uh the Nancy
00:13:22.959 --> 00:13:24.949
Grace Roman is a wide angle telescope.
00:13:24.959 --> 00:13:27.910
It's also infrared. Uh so it um it is
00:13:27.920 --> 00:13:30.949
actually seeing redder than red light.
00:13:30.959 --> 00:13:33.030
And we've got high hopes for what it
00:13:33.040 --> 00:13:35.590
might achieve with the huge galaxy
00:13:35.600 --> 00:13:38.069
surveys which hopefully will show light
00:13:38.079 --> 00:13:40.870
on would shed light on dark matter and
00:13:40.880 --> 00:13:45.829
dark energy. And um also it's got a very
00:13:45.839 --> 00:13:48.870
sophisticated coronagraph on board. And
00:13:48.880 --> 00:13:50.710
a coronagraph is a thing that blocks out
00:13:50.720 --> 00:13:52.550
the light of a star so you can look for
00:13:52.560 --> 00:13:55.590
other objects nearby. until we should
00:13:55.600 --> 00:13:58.470
start seeing images of exoplanets coming
00:13:58.480 --> 00:14:00.790
from the anti-grace Roman as well. So,
00:14:00.800 --> 00:14:02.550
it is lots to talk about down the track,
00:14:02.560 --> 00:14:03.030
Andrew.
00:14:03.040 --> 00:14:05.590
>> Yeah, very exciting. When do they expect
00:14:05.600 --> 00:14:08.550
it to actually be ready to roll? It it's
00:14:08.560 --> 00:14:10.310
a bit of a process, isn't it?
00:14:10.320 --> 00:14:11.750
>> It is. That's right. I'm not sure what
00:14:11.760 --> 00:14:14.069
the schedule is, as I was saying, but um
00:14:14.079 --> 00:14:16.389
we'll keep um we'll keep Space Not
00:14:16.399 --> 00:14:17.829
listeners posted. At the moment, the
00:14:17.839 --> 00:14:19.350
news is all good. And
00:14:19.360 --> 00:14:23.269
>> yeah, it is. It is. Uh in fact um I'm
00:14:23.279 --> 00:14:25.189
just looking.
00:14:25.199 --> 00:14:28.230
Yeah, first observations maybe early
00:14:28.240 --> 00:14:30.629
next year sometime. They haven't got
00:14:30.639 --> 00:14:33.269
>> exactly I had it in mind. It was 2027.
00:14:33.279 --> 00:14:33.750
>> Yeah.
00:14:33.760 --> 00:14:36.870
>> Um and I mean I I remember because we
00:14:36.880 --> 00:14:39.189
lived it in real time the commissioning
00:14:39.199 --> 00:14:42.470
for the Hubble telescope back in 1990. I
00:14:42.480 --> 00:14:43.990
was an astronomer at the UK Schmidt
00:14:44.000 --> 00:14:46.550
telescope then and we were getting
00:14:46.560 --> 00:14:48.470
direct reports from NASA actually about
00:14:48.480 --> 00:14:51.350
the commissioning before the interweb.
00:14:51.360 --> 00:14:55.110
Um and we very quickly realized that
00:14:55.120 --> 00:14:57.829
something was wrong uh because we got um
00:14:57.839 --> 00:14:59.750
reports of the image diameter as they
00:14:59.760 --> 00:15:01.189
went through focus
00:15:01.199 --> 00:15:03.670
>> and the image diameter never got small.
00:15:03.680 --> 00:15:05.829
So it was quite obvious very early on
00:15:05.839 --> 00:15:07.750
that um there was a problem with the
00:15:07.760 --> 00:15:09.910
Hubble and of course took them three
00:15:09.920 --> 00:15:12.949
years to build a a little device to
00:15:12.959 --> 00:15:15.509
correct for that and um uh then it was
00:15:15.519 --> 00:15:18.230
flown on a space shuttle mission and the
00:15:18.240 --> 00:15:19.350
rest is history.
00:15:19.360 --> 00:15:21.509
>> Yeah. A pufu valve I think it was they
00:15:21.519 --> 00:15:24.949
needed to put on it. Yeah. But um anyway
00:15:24.959 --> 00:15:27.189
>> did have a name costbar was it something
00:15:27.199 --> 00:15:27.750
like that.
00:15:27.760 --> 00:15:30.069
>> Something like that. Um it was lucky
00:15:30.079 --> 00:15:32.389
that it was close enough to get to. Um,
00:15:32.399 --> 00:15:33.509
>> yes, that's right.
00:15:33.519 --> 00:15:35.670
>> Can't do that with the L2.
00:15:35.680 --> 00:15:39.189
>> You can't. That's exactly right. Um,
00:15:39.199 --> 00:15:41.189
>> yes, things have moved on a bit since
00:15:41.199 --> 00:15:42.389
then. They have.
00:15:42.399 --> 00:15:44.790
>> Uh, exciting times and we will watch
00:15:44.800 --> 00:15:47.110
with interest and of course uh when they
00:15:47.120 --> 00:15:49.189
um achieve first light and we start to
00:15:49.199 --> 00:15:51.030
see some other images, we will share
00:15:51.040 --> 00:15:53.910
them with you here on Space Nuts. And
00:15:53.920 --> 00:15:56.230
you are listening to the latest edition
00:15:56.240 --> 00:15:58.230
with Andrew Dunley and Professor Fred
00:15:58.240 --> 00:15:59.829
Watson.
00:15:59.839 --> 00:16:01.350
Think
00:16:01.360 --> 00:16:03.269
we need to do a little more all weather
00:16:03.279 --> 00:16:04.629
testing.
00:16:04.639 --> 00:16:05.269
>> Amen.
00:16:05.279 --> 00:16:07.030
>> Space nets.
00:16:07.040 --> 00:16:09.189
>> Okay, Fred, let's talk about this
00:16:09.199 --> 00:16:12.629
strange galaxy. Um, some are saying it's
00:16:12.639 --> 00:16:15.030
a failed galaxy. Uh, it's been described
00:16:15.040 --> 00:16:17.110
as a starless galaxy and it's got a
00:16:17.120 --> 00:16:19.749
name. It's called Cloud9. What is this
00:16:19.759 --> 00:16:21.910
thing?
00:16:21.920 --> 00:16:26.629
Uh it's um yes it's a not a mystery
00:16:26.639 --> 00:16:28.550
galaxy in the sense that people have
00:16:28.560 --> 00:16:30.150
speculated
00:16:30.160 --> 00:16:33.910
that there may be galaxies without stars
00:16:33.920 --> 00:16:36.870
and you know we tend to think of
00:16:36.880 --> 00:16:39.350
galaxies as being made of stars because
00:16:39.360 --> 00:16:42.710
ours is Milky Way is a gigantic spiral
00:16:42.720 --> 00:16:45.430
of stars and gas and dust.
00:16:45.440 --> 00:16:46.949
Very beautiful if we could see it from
00:16:46.959 --> 00:16:49.590
the outside which sadly we we never can.
00:16:49.600 --> 00:16:54.069
Uh but um it has always been speculated
00:16:54.079 --> 00:16:56.470
that there may be
00:16:56.480 --> 00:17:00.069
uh galaxies which contain clouds of
00:17:00.079 --> 00:17:03.189
hydrogen, the raw material of stars,
00:17:03.199 --> 00:17:07.990
which basically is too hot for the
00:17:08.000 --> 00:17:10.150
clouds to collapse into individual
00:17:10.160 --> 00:17:11.829
stars. I think I've got the logic the
00:17:11.839 --> 00:17:12.949
right way there.
00:17:12.959 --> 00:17:16.230
>> Yeah. Um, so you've got the raw material
00:17:16.240 --> 00:17:20.150
of stars, but um, it doesn't form a
00:17:20.160 --> 00:17:25.110
stellar population. Um, and maybe um,
00:17:25.120 --> 00:17:27.909
it's because there's, you know, as I
00:17:27.919 --> 00:17:30.789
said, the gas is too hot. So this
00:17:30.799 --> 00:17:33.990
particular object, Cloud9, it's not very
00:17:34.000 --> 00:17:37.750
far away. Uh, it is about 14 million
00:17:37.760 --> 00:17:40.070
light years away. Uh, which puts it
00:17:40.080 --> 00:17:42.870
really on our galactic doorstep. Uh it's
00:17:42.880 --> 00:17:45.590
not far from uh a spiral galaxy called
00:17:45.600 --> 00:17:50.070
Messier 94 uh which is a lovely spiral
00:17:50.080 --> 00:17:51.590
uh if I remember rightly in the northern
00:17:51.600 --> 00:17:54.070
hemisphere sky. Uh well it must be
00:17:54.080 --> 00:17:55.510
because it's being observed by a
00:17:55.520 --> 00:17:57.669
telescope that um I never really had
00:17:57.679 --> 00:18:00.150
anything to do with but I knew its site
00:18:00.160 --> 00:18:01.590
well because it was built on a place
00:18:01.600 --> 00:18:03.830
where I used to observe a lot. Uh this
00:18:03.840 --> 00:18:07.430
is the Grand Telescopio Canaras uh which
00:18:07.440 --> 00:18:10.150
is the big Canarian telescope. It's
00:18:10.160 --> 00:18:11.590
actually the biggest optical telescope
00:18:11.600 --> 00:18:13.909
in the world. It has a 10 m mirror.
00:18:13.919 --> 00:18:17.110
>> Um, and it's located
00:18:17.120 --> 00:18:19.750
in La Palma in the Canary Islands and I
00:18:19.760 --> 00:18:21.190
used to observe there on a telescope
00:18:21.200 --> 00:18:23.510
called the William Roshaw telescope. So
00:18:23.520 --> 00:18:25.990
uh GTC as it's called Grand Telescopio
00:18:26.000 --> 00:18:30.150
Canarius has a a camera um uh called
00:18:30.160 --> 00:18:34.310
Hyper Cam uh which is the one that I
00:18:34.320 --> 00:18:37.430
think has really given us this research
00:18:37.440 --> 00:18:40.789
on Cloud9 because the uh the colleagues
00:18:40.799 --> 00:18:44.310
who observed uh this object what they
00:18:44.320 --> 00:18:46.070
did was they used that big telescope
00:18:46.080 --> 00:18:49.830
with its um wide-angle camera uh in
00:18:49.840 --> 00:18:53.830
order to get very very deep images and
00:18:53.840 --> 00:18:55.510
by deep images we mean ones that
00:18:55.520 --> 00:18:58.549
penetrate to really faint levels. Uh
00:18:58.559 --> 00:19:02.630
they got 2.336 hours of integration uh
00:19:02.640 --> 00:19:06.870
which is quite quite a long time. Uh and
00:19:06.880 --> 00:19:09.830
didn't see any stars. I think they they
00:19:09.840 --> 00:19:12.150
think they might have seen a small
00:19:12.160 --> 00:19:16.549
number of stars but not uh a what we
00:19:16.559 --> 00:19:21.590
expect in a galaxy. Um so the uh one of
00:19:21.600 --> 00:19:25.510
the authors of this paper um basically
00:19:25.520 --> 00:19:27.750
in offering an explanation of as to how
00:19:27.760 --> 00:19:31.190
you could have a galaxy with no stars uh
00:19:31.200 --> 00:19:32.950
I'll quote the leading theoretical
00:19:32.960 --> 00:19:35.350
explanation involves the ultraviolet
00:19:35.360 --> 00:19:37.350
background radiation that permeates the
00:19:37.360 --> 00:19:39.990
universe. Uh after the epoch of
00:19:40.000 --> 00:19:41.590
reionization
00:19:41.600 --> 00:19:43.110
uh that's right at the beginning this
00:19:43.120 --> 00:19:45.270
radiation field heats the gas in low
00:19:45.280 --> 00:19:48.070
mass dark matter halos to temperatures
00:19:48.080 --> 00:19:50.150
high enough that the gas cannot cool
00:19:50.160 --> 00:19:52.549
efficiency and collapse to form stars. I
00:19:52.559 --> 00:19:53.909
think that might be what I said earlier
00:19:53.919 --> 00:19:56.310
which is good. And so um when they do
00:19:56.320 --> 00:19:58.230
simulations
00:19:58.240 --> 00:20:01.430
um of uh you know the basically what
00:20:01.440 --> 00:20:03.590
this galaxy how it might have evolved
00:20:03.600 --> 00:20:05.590
sure enough it remains starless. They
00:20:05.600 --> 00:20:09.190
don't have any stars. So this looks like
00:20:09.200 --> 00:20:12.310
uh look like looks like a the first real
00:20:12.320 --> 00:20:15.270
example of something that people have
00:20:15.280 --> 00:20:18.870
thought must exist. Um and again quoting
00:20:18.880 --> 00:20:22.390
from it's Dr. Trujill Trujillo who I
00:20:22.400 --> 00:20:23.909
think I might have worked with in La
00:20:23.919 --> 00:20:27.990
Palma many many years ago uh says cloud9
00:20:28.000 --> 00:20:30.630
has a halo mass consistent with this
00:20:30.640 --> 00:20:32.470
regime. In this picture, starless
00:20:32.480 --> 00:20:36.390
galaxies are not exotic anomalies, but a
00:20:36.400 --> 00:20:38.950
natural and abundant prediction of
00:20:38.960 --> 00:20:40.870
standard cosmological models. The
00:20:40.880 --> 00:20:43.270
challenge has simply been finding them.
00:20:43.280 --> 00:20:45.830
So, um maybe it's not such an unusual
00:20:45.840 --> 00:20:49.750
thing after all. Uh but, uh something
00:20:49.760 --> 00:20:52.310
that has been predicted, but yes, the
00:20:52.320 --> 00:20:54.789
first I think the first one that we can
00:20:54.799 --> 00:20:58.070
really be sure uh is a starless galaxy.
00:20:58.080 --> 00:21:01.350
>> Yeah, very very unusual. Um, I'd suppose
00:21:01.360 --> 00:21:05.110
the description failed galaxy would be
00:21:05.120 --> 00:21:06.789
probably accurate given the
00:21:06.799 --> 00:21:07.990
circumstances.
00:21:08.000 --> 00:21:10.070
>> Yes, if you if you think of a normal
00:21:10.080 --> 00:21:12.870
galaxy as being populated by stars, it
00:21:12.880 --> 00:21:15.669
is. Um, but you you can see that there's
00:21:15.679 --> 00:21:17.430
good reason for it to fail. If the if
00:21:17.440 --> 00:21:19.350
the temperature of the background gas
00:21:19.360 --> 00:21:21.830
and the dark matter that's in it are too
00:21:21.840 --> 00:21:24.549
high for stars to form
00:21:24.559 --> 00:21:27.029
>> um and you might consider it a success
00:21:27.039 --> 00:21:30.710
because it's a purely gaseous galaxy.
00:21:30.720 --> 00:21:33.830
Yeah. Yeah. Uh I suppose one day it
00:21:33.840 --> 00:21:36.870
might merge with another galaxy and then
00:21:36.880 --> 00:21:39.430
you know all hell would break loose.
00:21:39.440 --> 00:21:40.870
>> That No, you're right. That's a good
00:21:40.880 --> 00:21:43.190
point because it's not that far from M94
00:21:43.200 --> 00:21:46.549
which is a big galaxy. Uh this is a it
00:21:46.559 --> 00:21:48.230
counts as a dwarf galaxy. I didn't
00:21:48.240 --> 00:21:50.870
really make that clear. And of course
00:21:50.880 --> 00:21:53.590
our our own galaxy has dwarf galaxies in
00:21:53.600 --> 00:21:55.510
orbit around it most of which contain
00:21:55.520 --> 00:21:59.029
stars. Uh and so and the fate of those
00:21:59.039 --> 00:22:00.950
dwarf galaxies is basically to become
00:22:00.960 --> 00:22:03.990
part of the of the bigger galaxy. So it
00:22:04.000 --> 00:22:06.710
may be that cloud 9 eventually does that
00:22:06.720 --> 00:22:09.029
and maybe the conditions will change so
00:22:09.039 --> 00:22:12.630
that the the gas becomes um uh cool
00:22:12.640 --> 00:22:15.590
enough or or otherwise relaxed enough uh
00:22:15.600 --> 00:22:18.470
in order to start form stars.
00:22:18.480 --> 00:22:20.549
>> Okay, if you want to read all about the
00:22:20.559 --> 00:22:22.950
starless galaxy cloud9 uh there's a
00:22:22.960 --> 00:22:26.470
great article on space.com.
00:22:26.480 --> 00:22:30.470
Um Fred, we got a live viewer who has it
00:22:30.480 --> 00:22:33.669
was from do actually. Hi Lynette. Um,
00:22:33.679 --> 00:22:36.070
she says, "Uh, hello from do. How long
00:22:36.080 --> 00:22:39.190
did you stay?" I assume she means Spain.
00:22:39.200 --> 00:22:40.630
Um,
00:22:40.640 --> 00:22:42.070
>> our earlier conversation.
00:22:42.080 --> 00:22:45.110
>> Yes, we were in Spain for, uh, roughly a
00:22:45.120 --> 00:22:47.190
week. Actually, uh, I didn't tell you,
00:22:47.200 --> 00:22:51.830
but I I got, um, I got
00:22:51.840 --> 00:22:54.310
thieved from by a pickpocket.
00:22:54.320 --> 00:22:55.750
>> Oh,
00:22:55.760 --> 00:22:58.390
>> yeah. Um, but very very common thing
00:22:58.400 --> 00:23:01.270
over there. It was in Bilbo and
00:23:01.280 --> 00:23:02.549
>> Oh, we went there.
00:23:02.559 --> 00:23:03.270
>> Lovely place.
00:23:03.280 --> 00:23:05.190
>> Yeah. Did you get your binoculars nicked
00:23:05.200 --> 00:23:06.070
as well?
00:23:06.080 --> 00:23:12.310
>> No. No. I I'm very very um
00:23:12.320 --> 00:23:14.549
look, we'll use the word anal about
00:23:14.559 --> 00:23:16.630
holding on to my stuff quite literally.
00:23:16.640 --> 00:23:16.870
Yep.
00:23:16.880 --> 00:23:18.630
>> I put stuff in my pockets and I'll shove
00:23:18.640 --> 00:23:20.310
my hands in my pockets and I will not
00:23:20.320 --> 00:23:21.669
take them out.
00:23:21.679 --> 00:23:22.149
>> Yeah.
00:23:22.159 --> 00:23:24.390
>> I must look weird.
00:23:24.400 --> 00:23:25.830
>> Well, you look weird anyway, Andrew. But
00:23:25.840 --> 00:23:28.630
that's, you know, not not good. Not bad
00:23:28.640 --> 00:23:30.870
news anyway. Uh but but no, you're
00:23:30.880 --> 00:23:34.310
right. Um so I'm like that too. But um I
00:23:34.320 --> 00:23:39.510
I had a a sort of manbag. Um and um I
00:23:39.520 --> 00:23:41.990
was walking back from the Guggenheim
00:23:42.000 --> 00:23:43.669
exhibition which you probably went to
00:23:43.679 --> 00:23:45.350
see as well in Bel
00:23:45.360 --> 00:23:46.950
>> to our hotel
00:23:46.960 --> 00:23:50.390
>> and I thought I noticed a bit of a
00:23:50.400 --> 00:23:52.390
disturbance behind me. I had headphones
00:23:52.400 --> 00:23:54.950
on um noise cancelling headphones cuz I
00:23:54.960 --> 00:23:55.830
was walking.
00:23:55.840 --> 00:23:58.390
>> Yeah. Um, and when I got into the hotel,
00:23:58.400 --> 00:24:01.350
I looked in my manb bag and the zip was
00:24:01.360 --> 00:24:04.789
open and I know I'd shut it up and my
00:24:04.799 --> 00:24:06.549
binoculars were missing.
00:24:06.559 --> 00:24:08.950
>> So, man said, "Go outside and have a
00:24:08.960 --> 00:24:10.710
look. They might have thrown them away."
00:24:10.720 --> 00:24:13.430
So, went outside.
00:24:13.440 --> 00:24:15.350
Here's four policemen bailing up these
00:24:15.360 --> 00:24:18.070
two guys.
00:24:18.080 --> 00:24:18.470
>> Got them.
00:24:18.480 --> 00:24:19.990
>> And they've been they've been following
00:24:20.000 --> 00:24:21.990
them because they'd created some sort of
00:24:22.000 --> 00:24:25.350
problems in a bar. Um, and I approached
00:24:25.360 --> 00:24:29.029
one of the policemen and said, "Um,
00:24:29.039 --> 00:24:30.789
I've lost a pair of binoculars." And he
00:24:30.799 --> 00:24:31.750
just said, "Yeah, we've got your
00:24:31.760 --> 00:24:32.870
binoculars."
00:24:32.880 --> 00:24:33.669
>> Wow.
00:24:33.679 --> 00:24:35.510
>> So, I got them back.
00:24:35.520 --> 00:24:37.990
>> Fantastic.
00:24:38.000 --> 00:24:40.310
>> It Yeah. These guys had tried to throw
00:24:40.320 --> 00:24:42.230
them away when they saw the police were
00:24:42.240 --> 00:24:45.029
on them and the cops had seen it. The
00:24:45.039 --> 00:24:46.070
cop who
00:24:46.080 --> 00:24:48.870
>> dealt with me spoke great English. He
00:24:48.880 --> 00:24:51.430
was an absolute gentleman. It was uh
00:24:51.440 --> 00:24:53.350
such a good experience that man insisted
00:24:53.360 --> 00:24:55.350
on taking our photographs together and
00:24:55.360 --> 00:24:57.110
things like that afterwards.
00:24:57.120 --> 00:24:58.870
>> Well, you got very lucky, Fred. Very
00:24:58.880 --> 00:24:59.430
lucky.
00:24:59.440 --> 00:25:01.190
>> Very, very lucky indeed. Yeah,
00:25:01.200 --> 00:25:03.669
absolutely lucky. I couldn't believe it.
00:25:03.679 --> 00:25:05.510
And actually those
00:25:05.520 --> 00:25:06.789
>> uh you know, I can go on about
00:25:06.799 --> 00:25:09.029
binoculars add infinitum having written
00:25:09.039 --> 00:25:10.549
the first book in English on the history
00:25:10.559 --> 00:25:13.190
of binoculars. Uh but they were a
00:25:13.200 --> 00:25:15.590
special pair as well, quite new. They're
00:25:15.600 --> 00:25:18.870
new to me. They're um basically they
00:25:18.880 --> 00:25:21.029
were made in the 60s or sorry the the '
00:25:21.039 --> 00:25:23.830
70s but they're very very good ones and
00:25:23.840 --> 00:25:25.750
um a lot of money.
00:25:25.760 --> 00:25:28.789
>> So Starchild says um we got a few live
00:25:28.799 --> 00:25:30.950
uh viewers at the moment and Starchild
00:25:30.960 --> 00:25:32.630
says quite a few thieves in the Milky
00:25:32.640 --> 00:25:34.470
Way.
00:25:34.480 --> 00:25:35.350
>> Yes, that's right.
00:25:35.360 --> 00:25:39.430
>> Yeah. Um and there was another question.
00:25:39.440 --> 00:25:42.070
Uh oh, good says good to see you two
00:25:42.080 --> 00:25:43.990
together again. Moose says how much did
00:25:44.000 --> 00:25:47.269
I miss? Uh about that much.
00:25:47.279 --> 00:25:49.350
I think we're a bit past halfway, Moose.
00:25:49.360 --> 00:25:53.269
And um another question. Um how many
00:25:53.279 --> 00:25:55.590
light years across is a dwarf galaxy? I
00:25:55.600 --> 00:25:57.830
guess they're all different sizes. They
00:25:57.840 --> 00:26:00.070
are, but it's a good question. I mean um
00:26:00.080 --> 00:26:02.789
so think of our galaxy, which is kind of
00:26:02.799 --> 00:26:06.470
100,000 lighty years across. Um and
00:26:06.480 --> 00:26:09.510
that's typical of a of a major spiral
00:26:09.520 --> 00:26:13.430
galaxy. A dwarf galaxy would probably be
00:26:13.440 --> 00:26:16.549
less than a tenth of that. Um 10,000
00:26:16.559 --> 00:26:18.870
light years, that sort of size, you
00:26:18.880 --> 00:26:21.669
know, just on on on average, that kind
00:26:21.679 --> 00:26:23.909
of that kind of size.
00:26:23.919 --> 00:26:25.750
>> Okay, thanks for the question. It
00:26:25.760 --> 00:26:27.269
doesn't happen like this very often, but
00:26:27.279 --> 00:26:28.789
today
00:26:28.799 --> 00:26:30.549
we've got an active audience. That's
00:26:30.559 --> 00:26:32.470
good.
00:26:32.480 --> 00:26:34.310
>> Yeah. All right. Uh you're listening to
00:26:34.320 --> 00:26:36.149
Space Nuts, by the way, uh with Andrew
00:26:36.159 --> 00:26:40.710
Dunley and Professor Fred Watson.
00:26:40.720 --> 00:26:43.669
Okay, we checked all four systems and
00:26:43.679 --> 00:26:44.950
>> space nets.
00:26:44.960 --> 00:26:47.830
>> Our final topic, Fred, takes us to
00:26:47.840 --> 00:26:50.310
Venus. Sunny Venus. Oh, yes. What a
00:26:50.320 --> 00:26:52.149
place. Go outside, take a deep breath,
00:26:52.159 --> 00:26:55.590
drop dead. Um, but there's some news
00:26:55.600 --> 00:26:57.669
about Venus, which involves its clouds
00:26:57.679 --> 00:26:59.510
again. Now, the last time this was big
00:26:59.520 --> 00:27:01.029
news was when they thought they might
00:27:01.039 --> 00:27:03.750
have found um signs of life in the
00:27:03.760 --> 00:27:05.909
clouds. That's still under a lot of
00:27:05.919 --> 00:27:08.710
speculation and debate. But what's the
00:27:08.720 --> 00:27:10.549
latest with these clouds? The these
00:27:10.559 --> 00:27:11.990
aren't the the ones we were talking
00:27:12.000 --> 00:27:13.590
about last time. These these are a
00:27:13.600 --> 00:27:15.990
little bit different again. Yes, they
00:27:16.000 --> 00:27:17.510
are. Yeah. So, I think that was sulfur
00:27:17.520 --> 00:27:19.269
was it sulfur dioxide? I can't remember
00:27:19.279 --> 00:27:22.310
the um the detection which uh which
00:27:22.320 --> 00:27:24.950
people got excited because it might been
00:27:24.960 --> 00:27:26.549
living organisms in the upper atmosphere
00:27:26.559 --> 00:27:28.470
of Venus, but I think that's gone away
00:27:28.480 --> 00:27:31.269
now. Um, it's great to talk about Venus,
00:27:31.279 --> 00:27:33.190
especially just now because you would
00:27:33.200 --> 00:27:35.510
know, Andrew, it's absolutely lighting
00:27:35.520 --> 00:27:37.990
up the evening sky, uh, over there in
00:27:38.000 --> 00:27:39.990
the west. It is very bright, very high
00:27:40.000 --> 00:27:41.430
in the sky.
00:27:41.440 --> 00:27:43.750
>> Beautiful object. And when we look at
00:27:43.760 --> 00:27:47.190
it, it's kind of got a yellowish color.
00:27:47.200 --> 00:27:49.430
Uh, which is because we're seeing
00:27:49.440 --> 00:27:51.750
reflections from the top of its cloud
00:27:51.760 --> 00:27:56.389
layer. Um but uh it's been known for a
00:27:56.399 --> 00:27:59.990
long time that if you photograph Venus
00:28:00.000 --> 00:28:04.630
in with ultraviolet light you you see
00:28:04.640 --> 00:28:08.149
patterns really dramatic patterns and I
00:28:08.159 --> 00:28:09.669
I haven't got one in front of me now but
00:28:09.679 --> 00:28:11.510
I do remember photographs of this that
00:28:11.520 --> 00:28:13.990
these are sort of globalized patterns
00:28:14.000 --> 00:28:17.590
that actually move uh with the the
00:28:17.600 --> 00:28:20.950
clouds of Venus. And as we know, I think
00:28:20.960 --> 00:28:23.830
most space notes uh listeners and
00:28:23.840 --> 00:28:25.350
viewers would know that we don't
00:28:25.360 --> 00:28:26.870
actually see the surface of Venus
00:28:26.880 --> 00:28:29.830
directly. We can with radar uh certain
00:28:29.840 --> 00:28:31.350
infrared observations that let you
00:28:31.360 --> 00:28:32.950
penetrate to the surface, but basically
00:28:32.960 --> 00:28:35.190
all we see uh and certainly in
00:28:35.200 --> 00:28:37.350
ultraviolet is the upper parts of the of
00:28:37.360 --> 00:28:40.389
the cloud belts, cloud layers.
00:28:40.399 --> 00:28:43.669
>> So the markings themselves uh are a
00:28:43.679 --> 00:28:47.590
puzzle. And um this is where it sort of
00:28:47.600 --> 00:28:49.190
gets interesting, although it's not one
00:28:49.200 --> 00:28:50.549
of these stories that's got a neat and
00:28:50.559 --> 00:28:53.269
tidy answer, I'm afraid. Um there's
00:28:53.279 --> 00:28:56.470
there's a chemical that is thought to be
00:28:56.480 --> 00:28:59.110
in Venus's upper atmosphere,
00:28:59.120 --> 00:29:02.789
which is called the unknown absorber.
00:29:02.799 --> 00:29:06.630
Uh and because uh it absorbs light uh in
00:29:06.640 --> 00:29:08.549
the ultraviolet, and you get dark
00:29:08.559 --> 00:29:12.950
patches from from this this stuff. Um, I
00:29:12.960 --> 00:29:14.230
was talking to somebody about this the
00:29:14.240 --> 00:29:15.669
other day and they said it sounds like a
00:29:15.679 --> 00:29:18.470
superhero, the unknown absorber. Uh,
00:29:18.480 --> 00:29:20.549
which, uh, I think probably would work
00:29:20.559 --> 00:29:22.310
well. Yeah.
00:29:22.320 --> 00:29:25.669
>> His superhero name would be the sponge.
00:29:25.679 --> 00:29:28.149
>> The sponge. That's right.
00:29:28.159 --> 00:29:33.269
So what's happened is that um a team an
00:29:33.279 --> 00:29:35.669
international team actually of basically
00:29:35.679 --> 00:29:38.310
astrobiologists people who are looking
00:29:38.320 --> 00:29:42.310
at uh the origin of life in the universe
00:29:42.320 --> 00:29:44.389
and what we need for life to form and
00:29:44.399 --> 00:29:46.149
all of those other good things not
00:29:46.159 --> 00:29:47.669
necessarily trying to find life but
00:29:47.679 --> 00:29:49.990
trying to understand life. um what
00:29:50.000 --> 00:29:53.590
they've done uh they've essentially this
00:29:53.600 --> 00:29:56.389
this research team I think they've done
00:29:56.399 --> 00:29:59.669
very cluey kind of modeling
00:29:59.679 --> 00:30:03.590
um of the droplets within the clouds of
00:30:03.600 --> 00:30:08.310
Venus to try and not identify what this
00:30:08.320 --> 00:30:12.950
unknown absorber is but sort of um place
00:30:12.960 --> 00:30:15.669
limits on its properties you know it
00:30:15.679 --> 00:30:18.230
does this but it doesn't do that uh and
00:30:18.240 --> 00:30:19.909
it does this to to this extent, but it
00:30:19.919 --> 00:30:22.470
doesn't do that to this extent. So, it's
00:30:22.480 --> 00:30:25.350
uh it's all about trying to model what
00:30:25.360 --> 00:30:28.149
cloud droplets would look like to
00:30:28.159 --> 00:30:30.470
actually reproduce what we see when we
00:30:30.480 --> 00:30:35.350
observe the planet. Um so,
00:30:35.360 --> 00:30:39.590
uh one of the authors of the paper
00:30:39.600 --> 00:30:43.350
basically poses a question. Uh, if we
00:30:43.360 --> 00:30:46.710
were to collect Venus's cloud droplets,
00:30:46.720 --> 00:30:48.870
and I'm paraphrasing here, into a
00:30:48.880 --> 00:30:52.070
bucket, how would the reformed bulk
00:30:52.080 --> 00:30:53.669
liquid appear?
00:30:53.679 --> 00:30:55.590
>> Uh, the scientist actually said a
00:30:55.600 --> 00:30:58.389
spectrometric cuette, but a bucket's as
00:30:58.399 --> 00:31:01.029
good an analogy for that as you need. If
00:31:01.039 --> 00:31:02.870
you could collect the droplets, what
00:31:02.880 --> 00:31:08.710
would it look like? Um and that is the
00:31:08.720 --> 00:31:11.750
sort of key to the modeling that's been
00:31:11.760 --> 00:31:15.909
done. Um they there's a comment um I
00:31:15.919 --> 00:31:17.269
think it might come from the original
00:31:17.279 --> 00:31:20.149
paper but um fsdoc.org has got a very
00:31:20.159 --> 00:31:23.430
nice article on this uh and I think it
00:31:23.440 --> 00:31:26.630
may even come from their press release.
00:31:26.640 --> 00:31:30.549
Uh but basically it's um likening the
00:31:30.559 --> 00:31:33.510
droplets in the clouds of Venus to
00:31:33.520 --> 00:31:37.110
cigarette smoke. Uh because um cigarette
00:31:37.120 --> 00:31:40.630
smoke is tiny particles, tar tiny tarry
00:31:40.640 --> 00:31:42.149
particles
00:31:42.159 --> 00:31:45.590
um which look sort of white or bluish
00:31:45.600 --> 00:31:47.029
because of the scattering of light.
00:31:47.039 --> 00:31:49.110
Because these things are so small they
00:31:49.120 --> 00:31:51.350
scatter light very effectively. But if
00:31:51.360 --> 00:31:53.909
you collected it into a flask, you got
00:31:53.919 --> 00:31:57.830
this horrible sludge uh t- like sludge.
00:31:57.840 --> 00:31:59.350
Of course, that is what ends up in your
00:31:59.360 --> 00:32:01.509
lungs if you're a smoker.
00:32:01.519 --> 00:32:05.110
>> Um yeah. So what they're suggesting is
00:32:05.120 --> 00:32:08.149
that there's a similar phenomenon
00:32:08.159 --> 00:32:10.950
happening in Venus's clouds. Uh because
00:32:10.960 --> 00:32:13.029
the particle size of the droplets in
00:32:13.039 --> 00:32:15.269
Venus's upper atmosphere are comparable
00:32:15.279 --> 00:32:18.230
to the particle size of cigarette smokes
00:32:18.240 --> 00:32:21.590
smoke. So even though um you know even
00:32:21.600 --> 00:32:24.389
though the clouds with the with visible
00:32:24.399 --> 00:32:27.990
light look that sort of yellowish color
00:32:28.000 --> 00:32:31.190
that we've mentioned already, the actual
00:32:31.200 --> 00:32:34.070
droplets themselves could be really
00:32:34.080 --> 00:32:36.149
really dark and it's only because they
00:32:36.159 --> 00:32:37.669
scatter the light in a certain way that
00:32:37.679 --> 00:32:40.310
they look that they look yellowish.
00:32:40.320 --> 00:32:44.710
Um so this basically this uh research is
00:32:44.720 --> 00:32:46.630
asking that question. What h what would
00:32:46.640 --> 00:32:48.789
happen if you could collect a cloud of
00:32:48.799 --> 00:32:50.470
material from the atmosphere of Venus
00:32:50.480 --> 00:32:52.789
and put it into a
00:32:52.799 --> 00:32:57.509
basically you know a a flask or a or a
00:32:57.519 --> 00:33:00.950
beaker or something like that. Um and
00:33:00.960 --> 00:33:03.669
that's where this analysis has gone and
00:33:03.679 --> 00:33:06.230
they've used something it's words that
00:33:06.240 --> 00:33:08.070
used to strike terror into me when I was
00:33:08.080 --> 00:33:10.389
a student in astronomy Andrew and I
00:33:10.399 --> 00:33:11.509
don't know whether I've uttered them
00:33:11.519 --> 00:33:15.190
ever since. radiative transfer. Uh
00:33:15.200 --> 00:33:17.430
radiative transfer is the way radiation
00:33:17.440 --> 00:33:22.070
moves around uh among atoms. Uh and it's
00:33:22.080 --> 00:33:25.830
very very intense mathematics. So these
00:33:25.840 --> 00:33:27.509
scientists obviously like that kind of
00:33:27.519 --> 00:33:30.230
thing. I'm afraid I didn't. uh and have
00:33:30.240 --> 00:33:32.870
built a radiative transfer model that uh
00:33:32.880 --> 00:33:36.470
actually lets you um account for not
00:33:36.480 --> 00:33:38.310
just single scattering but multiple
00:33:38.320 --> 00:33:40.950
scattering because you've you've got to
00:33:40.960 --> 00:33:42.710
um take into account that light might
00:33:42.720 --> 00:33:44.549
scatter from one of those droplets and
00:33:44.559 --> 00:33:46.230
then hit another one and scatter from
00:33:46.240 --> 00:33:48.630
that. So you've got multiple scattering
00:33:48.640 --> 00:33:53.430
phenomena. Um and so uh they have
00:33:53.440 --> 00:33:56.950
basically done that and produced what is
00:33:56.960 --> 00:33:59.509
called the absorption coefficient of the
00:33:59.519 --> 00:34:01.909
bulk cloud liquid. That's the how it
00:34:01.919 --> 00:34:04.950
would absorb um if you just had a flask
00:34:04.960 --> 00:34:07.430
of this stuff. Now what they're saying
00:34:07.440 --> 00:34:09.829
is that they don't really know what this
00:34:09.839 --> 00:34:12.710
these droplets are, but they're not
00:34:12.720 --> 00:34:15.589
suggesting its life. Um they've they've
00:34:15.599 --> 00:34:18.149
put limits on the absorption
00:34:18.159 --> 00:34:24.069
coefficient. Um and uh essentially
00:34:24.079 --> 00:34:26.470
again paraphrasing the uh press release
00:34:26.480 --> 00:34:29.430
from f.org uh the result implies that
00:34:29.440 --> 00:34:32.629
the unknown absorber must either absorb
00:34:32.639 --> 00:34:36.230
light very efficiently, occur at a very
00:34:36.240 --> 00:34:39.349
high concentration or both. Uh my guess
00:34:39.359 --> 00:34:42.149
is it's going to be both. Um, so, uh,
00:34:42.159 --> 00:34:45.109
it's it's some sort of probably some
00:34:45.119 --> 00:34:47.829
sort of organic compound, and by that I
00:34:47.839 --> 00:34:49.909
mean one that contains carbon rather
00:34:49.919 --> 00:34:52.389
than one that contains living organisms.
00:34:52.399 --> 00:34:55.430
Um, and they've basically, you know,
00:34:55.440 --> 00:34:57.349
they've suggested some chemicals that
00:34:57.359 --> 00:35:01.349
might actually be be responsible for
00:35:01.359 --> 00:35:03.430
this. Uh, excluding, they say
00:35:03.440 --> 00:35:05.430
chlorophyll. Chlorophyll, of course,
00:35:05.440 --> 00:35:08.150
very important in life processes. uh but
00:35:08.160 --> 00:35:09.750
they're excluding they're saying they're
00:35:09.760 --> 00:35:12.710
not proposing chlorophyll as as a as an
00:35:12.720 --> 00:35:15.670
example. So uh as I said it's a story
00:35:15.680 --> 00:35:18.630
that doesn't have a conclusion uh but
00:35:18.640 --> 00:35:21.030
it's interesting to think of the the
00:35:21.040 --> 00:35:22.790
clouds of Venus that if you could
00:35:22.800 --> 00:35:25.190
collect them in a bucket or a container
00:35:25.200 --> 00:35:27.910
they could be very very dark mixtures
00:35:27.920 --> 00:35:31.190
like tar a sort of sludge of of tar
00:35:31.200 --> 00:35:36.069
which um would be interesting.
00:35:36.079 --> 00:35:38.470
Yeah, it's um
00:35:38.480 --> 00:35:40.630
it's a classic example of a failed
00:35:40.640 --> 00:35:43.030
earthlike world.
00:35:43.040 --> 00:35:45.030
>> Yes, that's right. Yes, indeed. We don't
00:35:45.040 --> 00:35:47.670
have things like this on in our planet,
00:35:47.680 --> 00:35:49.430
thankfully.
00:35:49.440 --> 00:35:50.230
>> Yeah. Um
00:35:50.240 --> 00:35:52.310
>> I think there's more um Sorry, Andrew,
00:35:52.320 --> 00:35:53.589
just to finish the story, I think
00:35:53.599 --> 00:35:57.270
there's more research being designed
00:35:57.280 --> 00:36:02.150
possibly looking uh uh with a a future
00:36:02.160 --> 00:36:05.270
mission to Venus. uh perhaps looking for
00:36:05.280 --> 00:36:08.390
fluoresence in the uh in the clouds
00:36:08.400 --> 00:36:10.069
because that would give them another
00:36:10.079 --> 00:36:13.030
angle on what this stuff is.
00:36:13.040 --> 00:36:16.550
>> Okay, we watch with interest. Uh yeah,
00:36:16.560 --> 00:36:18.950
Venus keeps throwing up curve balls. The
00:36:18.960 --> 00:36:19.190
uh
00:36:19.200 --> 00:36:20.150
>> just doesn't
00:36:20.160 --> 00:36:22.230
>> the potential for life in the clouds
00:36:22.240 --> 00:36:24.069
because of the discovery of phosphine
00:36:24.079 --> 00:36:28.150
and now this um a bucket of tar. Yay.
00:36:28.160 --> 00:36:31.510
What a place. Next holiday, I think.
00:36:31.520 --> 00:36:33.109
Well, yeah. Plus, you've got the
00:36:33.119 --> 00:36:34.390
sulfuric acid as well.
00:36:34.400 --> 00:36:36.470
>> Oh, that's true. Yes. Yes. And and the
00:36:36.480 --> 00:36:39.030
um undeniable level of heat. I think
00:36:39.040 --> 00:36:40.790
Australians could handle it and a few
00:36:40.800 --> 00:36:42.790
other places in the world, but most No,
00:36:42.800 --> 00:36:44.470
most people couldn't. It's horrible.
00:36:44.480 --> 00:36:46.790
It's an horrible place, but very pretty
00:36:46.800 --> 00:36:48.390
in the sky at the moment.
00:36:48.400 --> 00:36:49.349
>> It is.
00:36:49.359 --> 00:36:51.750
>> Uh you can read all about it at f.org as
00:36:51.760 --> 00:36:53.750
Fred said or you can read the entire
00:36:53.760 --> 00:36:55.349
paper which was published in
00:36:55.359 --> 00:36:57.190
astrobiology.
00:36:57.200 --> 00:36:59.270
And that brings us to the end. Fred,
00:36:59.280 --> 00:37:01.109
thank you very much.
00:37:01.119 --> 00:37:02.950
Uh, it's a pleasure, Andrew. Um, it's
00:37:02.960 --> 00:37:05.349
always good to chat and um, even better
00:37:05.359 --> 00:37:08.230
to chat when you're half asleep.
00:37:08.240 --> 00:37:10.710
>> You did well. You did well. For those
00:37:10.720 --> 00:37:13.430
who joined us late, um, you'll have to
00:37:13.440 --> 00:37:14.790
listen to the episode, get the full
00:37:14.800 --> 00:37:18.230
explanation of Fred's sleepiness. Um,
00:37:18.240 --> 00:37:20.630
it's got something to do with um,
00:37:20.640 --> 00:37:24.310
painkillers. Anyway, we'll get on uh,
00:37:24.320 --> 00:37:25.829
hopefully he'll brighten up for the next
00:37:25.839 --> 00:37:27.670
episode. I suspect not.
00:37:27.680 --> 00:37:29.349
>> Um, thank you, Fred. We'll catch you
00:37:29.359 --> 00:37:30.310
soon.
00:37:30.320 --> 00:37:32.470
Sounds great. Thank Thanks, Andrew.
00:37:32.480 --> 00:37:34.230
>> Professor Fred Watson, astronomer at
00:37:34.240 --> 00:37:36.470
large. And don't forget to visit us at
00:37:36.480 --> 00:37:38.550
our website between episodes, which you
00:37:38.560 --> 00:37:40.630
can do at spaceenutspodcast.com
00:37:40.640 --> 00:37:44.630
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00:37:44.640 --> 00:37:46.870
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00:37:46.880 --> 00:37:49.109
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00:37:51.920 --> 00:37:54.310
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listen to us. And thanks to Hugh in the
00:37:56.880 --> 00:37:58.310
studio who couldn't be with us today
00:37:58.320 --> 00:38:00.470
because he discovered that he's um he's
00:38:00.480 --> 00:38:03.030
more at home in a starless galaxy. And
00:38:03.040 --> 00:38:04.870
from me, Andrew Dunley, thanks for your
00:38:04.880 --> 00:38:06.550
company. See you on the next episode of
00:38:06.560 --> 00:38:08.310
Space Nuts. Bye-bye.
00:38:08.320 --> 00:38:09.270
>> Space Nuts.
00:38:09.280 --> 00:38:11.349
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