SpaceX Tests Space-Ready Nuclear Power Using Tritium-Driven CubeSat | Space Nuts: Astronomy...
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From SpaceX Nuclear Experiments to Galactic Discoveries
Join host Andrew Dunkley and astronomer Fred Watson as they explore some of the most fascinating topics in space science, from innovative nuclear power tests in space to the expanding boundaries of our galaxy. Whether you're an astrophotography enthusiast or a space policy advocate, this episode delivers insights that broaden your cosmic perspective.
In this episode:
SpaceX's recent CubeSat launch featuring a tritium-based nuclear power source for space applications
The potential and safety considerations of nuclear energy in space missions
The possibility of nuclear weapons detection in space using neutron sensors and passive radiation monitoring
The intriguing hypothesis of dark matter stars and their potential signatures
The mystery surrounding Earth's dust origins—cosmic spherules and their unknown sources
New research indicating our galaxy's spiral arms are about 10% longer than previous estimates, based on light echoes from gamma ray bursts
The rise of smart telescopes and their role in making astrophotography more accessible for amateurs
Timestamps:
(00:00) Introduction and overview of today's headlines
(02:00) SpaceX's CubeSat with tritium power source—what's happening?
(04:33) Nuclear power in space: Safety and future applications
(11:03) Detecting nuclear weapons in space: Challenges and innovations
(22:45) Earth's dust origins: Micro-meteorites and cosmic spherules explained
Resources & Links:
SpaceX's CubeSat nitrogen launch story
Beta-voltaic nuclear power technology
NASA's Chandra X-ray Observatory
Universe Today article on Milky Way mapping
James Webb Space Telescope and dark matter research
Science Advances publication on Earth's micrometeorites
Connect with Fred Watson:
LinkedIn
Twitter
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Episode link: https://play.headliner.app/episode/34565447?utm_source=youtube
Kind: captions
Language: en
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Hi there. Thanks again for joining us.
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This is Space Nuts. My name is Andrew
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Dunley and every week we talk astronomy
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and space science and we answer audience
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questions in our alternative show which
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happens um well wherever you are. I mean
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we release it on a Monday, but that
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doesn't mean you listen to it on a
00:00:18.960 --> 00:00:22.630
Monday. Uh coming up today, we've got a
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couple of nuclear explosive stories. Uh
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SpaceX is involved in one of those and
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the other story is about uh blowing
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things up with atomic weapons from
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space. Yes, highly guaranteed, very very
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uh effective as well. Uh but I think
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there's probably a reason not to. We'll
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look at all of that. Uh we're also going
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to talk about where Earth's dust came
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from. Quite a bit of it, which might
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come as a bit of a surprise. Uh you just
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have to look under just about every bed
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and kitchen table in the world to find
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it. as much dust as there is in the
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world. But we'll see where that uh is
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headed. And our galaxy uh reaches out
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further than we thought apparently. Uh
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there's some interesting science behind
00:01:04.960 --> 00:01:07.270
that. We'll talk about it all on this
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edition of Space Nuts.
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>> 15 seconds. Guidance is internal. 10 9
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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 4 3 2 1
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>> Space Nuts. Astronauts report. It feels
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good.
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>> And joining us again to talk about all
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of that and more is Professor Fred
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Watson, astronomer at large. Hello,
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Fred.
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>> Hello, Andrew. Good to see you. Good to
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see you today. Yes. We sort of missed a
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few days, haven't we?
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>> Yes. You've been you've been off uh
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you've been off conferencing.
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>> Yes. So, the annual science meeting as
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it's called of the National Astronomy
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Society, the Astronomical Society of
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Australia. It's where all the
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professional astronomers get together
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and uh talk about what they've been
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doing, their research. Uh it was a big
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meeting. There were I would have guessed
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maybe a couple of hundred people there
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altogether. Uh that's quite big for
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astronomers and in a country that's only
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got 700 astronomers in it.
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>> Yeah.
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>> Uh but um what was interesting and what
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was very I think heartening for me was
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the number of youngsters that were
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there. I call them you because you know
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people under 50
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people um the the new generation of
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astronomers uh most of them whom I
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didn't know and they have no idea who I
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am and that's fine uh that all was okay.
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It just contrasts with a few years ago.
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So when I was the astronomer in charge
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of the of the observatory at Kuna
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Barabbran uh we were kind of the
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shopkeepers. So all these astronomers
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used to come through stay in the lodge
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and do their research using the
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telescope. So I knew a a large fraction
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of the astronomical population of
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Australia, but that's changed uh because
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my job that job is no longer mine. Uh
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and so I don't see people the same way.
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But uh it was so it was very nice to
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meet a lot of new faces and catch up
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with some very old faces as well, some
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even older than mine. Um and we also
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discussed matters such as the future of
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Australian astronomy because that's uh
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in a interesting state at the moment
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with the government having declined uh
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to uh engage in membership with the
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European Southern Observatory. We are
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now working on plan B uh and uh well it
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looks promising.
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>> Yes, fingers crossed. Uh there's a lot
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going on. Okay. Um, we should probably
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get stuck into these stories cuz there's
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a lot to discuss. The first story is a
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double banger about um nuclear energy
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and atomic weapons. Uh, we'll start off
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with the story about Space X and they're
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um they're looking at nuclear power in
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space, nuclearpowered satellites. What's
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the story here? It's a test launch
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really a launch of a a a cubat basically
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that um has not a nuclear reactor inside
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but a um basically a capsule of
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something called tritium which is
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sometimes called heavy hydrogen. It's
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hydrogen with two neutrons in it as well
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as the proton at its center and it's
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radioactive. Uh tritium is um I I
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suppose you'd call it mildly
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radioactive. Um, we used to use tritium
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standard lamps uh at the observatory
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when I was working there, which was a
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little capsule of tritium with some
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phosphor on it. Um, and the the um
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basically the electrons released by the
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tritium lit up the phosphor and and gave
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a very constant glow so we could use it
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to calibrate other other instruments.
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So, I've been close up and personal with
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um a little nuclear power source a bit
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like that, but it was just making faint
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light. This one is one that's been uh
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developed by a private company um and
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it's uh basically a company called City
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Labs uh in the United States. uh they've
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built um a little as I said it's
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effectively a cubat which has this um
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little nuclear
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not nuclear reactor but nuclear power
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source inside a tritium uh source that
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I've just been talking about which
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doesn't actually convert the electrons
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into light it converts them directly
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into electricity so they've got these
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panels on the side of it that take the
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electrons that come from the tritium and
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turn
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straight into um into electricity. It's
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called bore bhr. Uh which is a bit of a
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play on words because Neils Boore was
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one of the great founders of quantum
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theory. Uh same spelling um Danish one
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uh a Danish uh scientist uh and it
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stands for beta voltaic and a beta
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voltaque is taking the beta particles
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which are otherwise known as electrons
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uh turning them into electricity. So
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it's beta voltake orbital high
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reliability spacecraft. That's where you
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get the BR from.
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>> Uh and it's been it's been launched. So
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SpaceX's part in this story is just to
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provide the taxi uh up into um up into
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orbit. It's a trans transporter mission.
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One of um one of basically one of
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SpaceX's taxi rides to get stuff up and
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down from up to orbit. Coming down is a
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different story. Most of them just burn
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up. Uh yes, but it is uh probably the
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first cubat to include a nuclear power
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system. Uh and maybe just maybe will
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sort of illuminate the way for a new
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generation of uh of spacecraft which are
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equipped with uh with these nuclear
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power sources. I suppose they have to
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look at alternatives because we we've
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been reliant fairly reliant anyway on
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solar energy in space um particularly
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with our orbiting satellites but also
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with um the international space station
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and others u but the the time will come
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where we are in places where there won't
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be that much
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>> sunlight and in some places there won't
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be any at all and you know solar panels
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are going to be useless. Uh that's
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correct. And and we've seen already the
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um the use of these uh RTGs, radio
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isotope thermmoelectric generators,
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>> uh which are carried by both the
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Curiosity and the uh Perseverance rovers
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uh as well as spacecraft in deep space
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like uh Voyager One, Voyager 2,
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Pioneers, I think they've got them as
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well. And these are spacecraft that are
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so far from the sun that you get very
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little light from the sun uh in terms of
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um you know using it to generate
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electricity. So they've they've had
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their nuclear power sources for a long
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time. They are quite different though
00:07:58.400 --> 00:07:59.670
from what we're talking about here.
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There are I think it's 13 kg if I
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remember rightly is the amount in a
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canister of plutonium dioxide
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>> which is decaying all the time and
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getting very hot as it does that. And
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that heat is then used to generate
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electricity. Uh and it actually dies
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away as time goes on. So these uh
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nuclear RTGs, the radioisotope
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thermmoelectric generators gradually
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lose their power. Um and that's why we
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hear from time to time, and we usually
00:08:31.039 --> 00:08:34.070
report this on on Space Nuts, we hear of
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uh uh instruments on board Voyager One
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being turned off to save to save the
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power.
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>> Yeah. And that that didn't that happened
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again not so long ago, I think. But um
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>> that that's correct. Yes, it did. There
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was one turned off quite recently. But
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but perhaps more to the point and your
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uh what you've just said about there
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being some places that have no sunlight
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whatsoever. Uh that applies to the uh
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those deep craters near the moon's south
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pole. And that's where we're thinking of
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exploring. So it may be that um these
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beta voltaic arrays uh uh or devices
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might well be the future of power
00:09:14.399 --> 00:09:16.710
generation on the near the moon south
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pole because you're in places where
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there's no light whatsoever from the
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sun.
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>> Absolutely true. Darn cold too. It is.
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>> It is. It's always cold there. Yes. Yes.
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>> Indeed. Uh that's uh it's a really
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interesting story and uh we're obviously
00:09:31.120 --> 00:09:33.190
in the early phases of finding these
00:09:33.200 --> 00:09:36.550
alternatives. Is um is treatium safe?
00:09:36.560 --> 00:09:40.870
>> Uh it's probably something regarded uh
00:09:40.880 --> 00:09:44.389
treated carefully. Uh it it is it is
00:09:44.399 --> 00:09:46.550
generally safe. I mean we never took any
00:09:46.560 --> 00:09:48.389
real precautions with the device that we
00:09:48.399 --> 00:09:51.350
had on the telescope and maybe we should
00:09:51.360 --> 00:09:54.710
have done although uh most of us are
00:09:54.720 --> 00:09:57.750
still around and in fairly good health
00:09:57.760 --> 00:10:01.190
but um yes they are releasing electrons
00:10:01.200 --> 00:10:05.190
uh beta radiation. It's um uh if you if
00:10:05.200 --> 00:10:07.350
you had a high level though of tritium,
00:10:07.360 --> 00:10:09.190
if you had a you know significant amount
00:10:09.200 --> 00:10:10.870
of it, then you would have to be careful
00:10:10.880 --> 00:10:12.790
about how you handled it and where it
00:10:12.800 --> 00:10:14.470
was put and if it needed shielding and
00:10:14.480 --> 00:10:15.590
things of that sort.
00:10:15.600 --> 00:10:17.509
>> Yeah. So don't sprinkle it on your corn
00:10:17.519 --> 00:10:19.110
flakes or anything like that.
00:10:19.120 --> 00:10:20.710
>> Yes, that's right. It's best to avoid it
00:10:20.720 --> 00:10:21.350
if you can.
00:10:21.360 --> 00:10:22.710
>> Yeah.
00:10:22.720 --> 00:10:25.269
>> Sugar's damaging enough already. Um
00:10:25.279 --> 00:10:27.190
>> it is
00:10:27.200 --> 00:10:29.750
about it. If you'd like to um read up on
00:10:29.760 --> 00:10:31.670
that story about the uh the launch of
00:10:31.680 --> 00:10:34.470
the Cubat with the Tritium uh nuclear
00:10:34.480 --> 00:10:36.470
power device that they're testing, uh
00:10:36.480 --> 00:10:38.470
you can read about it at daily
00:10:38.480 --> 00:10:41.350
galaxy.com.
00:10:41.360 --> 00:10:44.310
Um let's keep on this theme, Fred,
00:10:44.320 --> 00:10:47.030
because that's the good news. Uh the bad
00:10:47.040 --> 00:10:51.430
news is um the the problem of exploding
00:10:51.440 --> 00:10:54.310
nuclear devices in space or firing
00:10:54.320 --> 00:10:56.710
nuclear devices from space to targets on
00:10:56.720 --> 00:10:59.269
Earth. That's that's a real issue. I
00:10:59.279 --> 00:11:02.790
know um was it back in the8s the Star
00:11:02.800 --> 00:11:04.470
Wars
00:11:04.480 --> 00:11:08.470
um um push was uh all the rage in the
00:11:08.480 --> 00:11:10.470
news at the time that got shut down
00:11:10.480 --> 00:11:12.230
pretty quickly.
00:11:12.240 --> 00:11:15.590
>> Star Wars was um a Reagan era
00:11:15.600 --> 00:11:17.750
initiative. Uh yes, I think it was I
00:11:17.760 --> 00:11:19.269
think it was um
00:11:19.279 --> 00:11:21.590
>> uh basically electromagnetic radiation
00:11:21.600 --> 00:11:23.430
to to zap your satellites. It wasn't
00:11:23.440 --> 00:11:25.430
nuclear though. Uh because nuclear
00:11:25.440 --> 00:11:28.230
weapons are in space are prohibited by
00:11:28.240 --> 00:11:31.670
the outer space treaty 1967.
00:11:31.680 --> 00:11:32.949
>> So what's happening?
00:11:32.959 --> 00:11:36.069
>> They're not allowed but
00:11:36.079 --> 00:11:39.110
um there may be some there uh launched
00:11:39.120 --> 00:11:40.230
by
00:11:40.240 --> 00:11:43.990
>> powers that um stretch the envelope if I
00:11:44.000 --> 00:11:46.230
can put it that way. Governments that
00:11:46.240 --> 00:11:48.310
stretch the envelope. Uh and we don't
00:11:48.320 --> 00:11:50.710
know uh we don't know if there are any.
00:11:50.720 --> 00:11:53.350
we, you know, they're banned by the uh
00:11:53.360 --> 00:11:54.949
outer space treaty, so there shouldn't
00:11:54.959 --> 00:11:58.870
be any nuclear weapons in space, but
00:11:58.880 --> 00:12:01.670
that's all very well. Um there's a lot
00:12:01.680 --> 00:12:03.829
of things that shouldn't happen that do
00:12:03.839 --> 00:12:06.550
happen. And um so it may be that perhaps
00:12:06.560 --> 00:12:09.190
there are nuclear weapons in space. So
00:12:09.200 --> 00:12:11.509
the the question is
00:12:11.519 --> 00:12:13.910
um how how do you detect them if there
00:12:13.920 --> 00:12:16.710
are these weapons? M
00:12:16.720 --> 00:12:21.350
>> um and um that's where this piece of
00:12:21.360 --> 00:12:24.470
research uh from the Massachusetts
00:12:24.480 --> 00:12:27.030
Institute of Technology has come from.
00:12:27.040 --> 00:12:31.509
It's um a a person whose name is Aric
00:12:31.519 --> 00:12:34.389
Danagulian. Uh sounds like an Armenian
00:12:34.399 --> 00:12:36.870
name, does it? Usually I on the end
00:12:36.880 --> 00:12:38.870
Armenian and associate professor of
00:12:38.880 --> 00:12:41.030
nuclear science and engineering at the
00:12:41.040 --> 00:12:43.910
Massachusetts Institute of Technology.
00:12:43.920 --> 00:12:48.550
and he has um essentially uh thought of
00:12:48.560 --> 00:12:52.550
a neat way of
00:12:52.560 --> 00:12:57.190
of building a device that you could fly
00:12:57.200 --> 00:13:01.190
in the vicinity of a satellite to detect
00:13:01.200 --> 00:13:04.629
whether it is carrying nuclear weapons.
00:13:04.639 --> 00:13:07.269
Um and it's all about the subatomic
00:13:07.279 --> 00:13:11.910
particles uh that um you know that that
00:13:11.920 --> 00:13:14.790
uh nuclear weapons are all about. It's
00:13:14.800 --> 00:13:16.310
all about
00:13:16.320 --> 00:13:18.790
>> neutrons and uh you know the nuclear
00:13:18.800 --> 00:13:20.710
nuclei of atoms that's where it all
00:13:20.720 --> 00:13:21.829
comes from.
00:13:21.839 --> 00:13:25.509
>> Um so what he's
00:13:25.519 --> 00:13:29.750
what he has suggested that I might quote
00:13:29.760 --> 00:13:33.509
um I might quote from uh from Dr. to
00:13:33.519 --> 00:13:38.949
Danagolian's work. Uh the
00:13:38.959 --> 00:13:41.110
risk is that if if you did explode a
00:13:41.120 --> 00:13:43.750
nuclear weapon in low Earth orbit, then
00:13:43.760 --> 00:13:46.389
you basically wreck low Earth orbit for
00:13:46.399 --> 00:13:48.470
everybody. It's not the blast. It's just
00:13:48.480 --> 00:13:51.670
the the subatomic particles that do it.
00:13:51.680 --> 00:13:53.990
>> Uh and so what he goes on to say is this
00:13:54.000 --> 00:13:56.870
danger is compounded by the lack of a
00:13:56.880 --> 00:13:58.870
verification mechanism for the outer
00:13:58.880 --> 00:14:03.189
space treaty. um there's no detection
00:14:03.199 --> 00:14:05.509
methodologies that have been proposed in
00:14:05.519 --> 00:14:07.350
the scientific literature. So what he's
00:14:07.360 --> 00:14:09.189
saying is here's a concept and
00:14:09.199 --> 00:14:12.790
feasibility study uh for verifying a
00:14:12.800 --> 00:14:15.350
satellite's compliance to the outer
00:14:15.360 --> 00:14:18.629
space treaty by observing the neutrons
00:14:18.639 --> 00:14:20.870
induced by spolation from the
00:14:20.880 --> 00:14:24.310
approximately giga electric vol giga
00:14:24.320 --> 00:14:27.189
electron volt protons in the inner allen
00:14:27.199 --> 00:14:29.670
radiation belt which is a slightly
00:14:29.680 --> 00:14:32.470
complicated and technical way of saying
00:14:32.480 --> 00:14:34.069
uh you've already got subatomic
00:14:34.079 --> 00:14:37.189
particles in the radiation belt around
00:14:37.199 --> 00:14:41.829
around our planet. Um if you can um
00:14:41.839 --> 00:14:47.030
basically watch the way uh a satellite
00:14:47.040 --> 00:14:49.910
responds to those protons that are in
00:14:49.920 --> 00:14:53.110
the radiation belts. Um if for example
00:14:53.120 --> 00:14:54.949
that bombardment of protons from the
00:14:54.959 --> 00:14:58.629
radiation belts causes neutrons to be uh
00:14:58.639 --> 00:15:02.069
emitted then you can uh have a fair
00:15:02.079 --> 00:15:05.590
degree of um confidence that there might
00:15:05.600 --> 00:15:07.750
be a nuclear weapon on board or a lot of
00:15:07.760 --> 00:15:10.710
nuclear file material heavy elements
00:15:10.720 --> 00:15:13.110
like uranium. That's the kind of thing
00:15:13.120 --> 00:15:17.750
that this is all about. Um and so um
00:15:17.760 --> 00:15:21.269
what uh you know what what this is all
00:15:21.279 --> 00:15:25.110
about is uh building a satellite that
00:15:25.120 --> 00:15:27.030
can detect
00:15:27.040 --> 00:15:29.269
uh neutrons
00:15:29.279 --> 00:15:33.269
uh coming from radioactive material. and
00:15:33.279 --> 00:15:37.430
he's basically suggesting a a detector
00:15:37.440 --> 00:15:40.150
uh a what he calls an inspector
00:15:40.160 --> 00:15:43.670
satellite that flies by uh the the
00:15:43.680 --> 00:15:45.189
satellite that you're interested in
00:15:45.199 --> 00:15:46.629
finding out whether it's got nuclear
00:15:46.639 --> 00:15:47.590
weapons.
00:15:47.600 --> 00:15:49.829
>> And it's got these detectors uh which
00:15:49.839 --> 00:15:51.910
are almost like X-ray detectors, the
00:15:51.920 --> 00:15:54.069
kind of things that you see now in in
00:15:54.079 --> 00:15:55.910
when you go for an X-ray, a chest X-ray.
00:15:55.920 --> 00:15:57.269
They're electronic. They're not
00:15:57.279 --> 00:15:58.790
photographic like they used to be back
00:15:58.800 --> 00:15:59.670
in the day.
00:15:59.680 --> 00:16:01.590
>> Yeah. Um, and they've got what are
00:16:01.600 --> 00:16:03.590
called neutron sensors. Uh, they're
00:16:03.600 --> 00:16:06.629
called scintillators. And you put uh you
00:16:06.639 --> 00:16:09.509
put those in a special arrangement with
00:16:09.519 --> 00:16:13.590
other basically other detectors. Uh, and
00:16:13.600 --> 00:16:16.790
um if you do that then you can you can
00:16:16.800 --> 00:16:19.509
apparently sort out the neutrons from
00:16:19.519 --> 00:16:22.470
the other natural subatomic particles
00:16:22.480 --> 00:16:24.310
that are floating around near the
00:16:24.320 --> 00:16:26.470
radiation belts. And the neutrons come
00:16:26.480 --> 00:16:28.870
from radioactive material. And you can
00:16:28.880 --> 00:16:30.470
also see the direction that they're
00:16:30.480 --> 00:16:32.949
coming from. So you can sort of point
00:16:32.959 --> 00:16:35.590
this thing towards your target satellite
00:16:35.600 --> 00:16:37.030
uh the one that you suspect might have
00:16:37.040 --> 00:16:39.189
nuclear weapons and and it will give you
00:16:39.199 --> 00:16:41.590
the direction of where it's coming from.
00:16:41.600 --> 00:16:47.189
>> Um and so uh just a quote um from again
00:16:47.199 --> 00:16:50.790
from Dr. Danagulian. Um the calculations
00:16:50.800 --> 00:16:54.150
show that a 9 unitit cubat size
00:16:54.160 --> 00:16:56.150
detection platform that's something the
00:16:56.160 --> 00:16:58.150
size of what's that about three loaves
00:16:58.160 --> 00:16:59.990
of bread something of that sort size
00:17:00.000 --> 00:17:03.430
it's quite small um it can identify a
00:17:03.440 --> 00:17:06.309
thermonuclear weapon from a distance of
00:17:06.319 --> 00:17:09.429
4 kilometers in approximately one week
00:17:09.439 --> 00:17:12.150
of observation. Now, that's quite a long
00:17:12.160 --> 00:17:13.189
time,
00:17:13.199 --> 00:17:16.230
>> but uh apparently if you could get it to
00:17:16.240 --> 00:17:18.870
within 1 kilometer, it would take you
00:17:18.880 --> 00:17:21.909
about an hour to detect a weapon.
00:17:21.919 --> 00:17:25.429
>> And that's promising. That's one flyby.
00:17:25.439 --> 00:17:28.309
That's, you know, an hour of proximity.
00:17:28.319 --> 00:17:31.029
Uh you could do that as you go past the
00:17:31.039 --> 00:17:33.590
the suspect the suspect satellite if you
00:17:33.600 --> 00:17:36.549
got an hour in in uh close contact with
00:17:36.559 --> 00:17:39.909
it or close uh proximity to it within a
00:17:39.919 --> 00:17:42.789
within a kilometer uh then you might
00:17:42.799 --> 00:17:45.510
well detect a nuclear weapon on board.
00:17:45.520 --> 00:17:46.950
And of course you could improve that if
00:17:46.960 --> 00:17:49.270
you had more than one of these inspector
00:17:49.280 --> 00:17:51.029
satellites. If you multiplied them up
00:17:51.039 --> 00:17:53.110
then you could get quite significant
00:17:53.120 --> 00:17:55.029
improvements in that performance. So
00:17:55.039 --> 00:17:57.270
it's really quite interesting. Yeah.
00:17:57.280 --> 00:18:01.909
>> Um, uh, one quote that I really liked,
00:18:01.919 --> 00:18:04.950
um, and and it's I'm going to read, uh,
00:18:04.960 --> 00:18:07.270
from Universe Today has a very nice
00:18:07.280 --> 00:18:09.270
article on this. The last sentence is,
00:18:09.280 --> 00:18:10.950
right now, nations like the USA and
00:18:10.960 --> 00:18:13.669
Russia rely on intelligence to know what
00:18:13.679 --> 00:18:15.909
the other is doing. And as we know from
00:18:15.919 --> 00:18:17.750
history, intelligence can get things
00:18:17.760 --> 00:18:20.630
wrong. You can fake intelligence, said
00:18:20.640 --> 00:18:23.110
Dr. Danagulian, but you can't fake
00:18:23.120 --> 00:18:26.310
physics. I like that. It's true. So you
00:18:26.320 --> 00:18:28.230
could do it by physics. Yeah,
00:18:28.240 --> 00:18:31.350
>> they do mention in this particular
00:18:31.360 --> 00:18:33.110
article that there's one suspect
00:18:33.120 --> 00:18:34.710
satellite that seems to have been
00:18:34.720 --> 00:18:37.510
launched by Russia. And the bottom line
00:18:37.520 --> 00:18:40.470
is that it's it's been put in an orbit
00:18:40.480 --> 00:18:42.710
that is very strange
00:18:42.720 --> 00:18:46.070
>> and very hostile in terms of its
00:18:46.080 --> 00:18:48.789
radiation uh in that area. And the
00:18:48.799 --> 00:18:51.110
question is asked, well, it says no one
00:18:51.120 --> 00:18:52.470
puts satellites there because it's
00:18:52.480 --> 00:18:54.950
highly radioactive. Why would you put a
00:18:54.960 --> 00:18:56.630
satellite in that orbit?
00:18:56.640 --> 00:18:58.789
>> So that's one. They've already they
00:18:58.799 --> 00:19:01.190
haven't identified as maybe carrying a
00:19:01.200 --> 00:19:03.590
nuclear weapon, but they've certainly
00:19:03.600 --> 00:19:05.510
identified it as suspicious.
00:19:05.520 --> 00:19:08.549
>> Yes, that's correct. And so um yes,
00:19:08.559 --> 00:19:10.549
highlighting that I think you know puts
00:19:10.559 --> 00:19:13.190
this article in context. It um it tells
00:19:13.200 --> 00:19:15.430
you that this is a real issue and um we
00:19:15.440 --> 00:19:17.110
kind of need to work on how you might
00:19:17.120 --> 00:19:20.150
detect nuclear weapons in space. it. Of
00:19:20.160 --> 00:19:21.990
course, the other side of it is if you
00:19:22.000 --> 00:19:23.990
do identify a satellite that's carrying
00:19:24.000 --> 00:19:25.909
a nuclear weapon,
00:19:25.919 --> 00:19:27.909
>> what do you do next? It's like it's like
00:19:27.919 --> 00:19:29.669
trying to teach people not to overtake
00:19:29.679 --> 00:19:31.669
in merging lanes, isn't it?
00:19:31.679 --> 00:19:35.990
>> Uh yes. Uh but um it's worse than that
00:19:36.000 --> 00:19:38.870
really because a little bit. Yeah. You
00:19:38.880 --> 00:19:41.270
know, we have nations that completely
00:19:41.280 --> 00:19:44.070
disregard international law. They invade
00:19:44.080 --> 00:19:48.070
other countries without um so much as a
00:19:48.080 --> 00:19:53.669
you know a sniff of the um um of the um
00:19:53.679 --> 00:19:55.270
all the international treaties. They
00:19:55.280 --> 00:19:57.510
just run a muck among them and away they
00:19:57.520 --> 00:19:58.310
go.
00:19:58.320 --> 00:20:00.789
>> Uh and yes so that's the possibility
00:20:00.799 --> 00:20:02.950
that we might already have them. There
00:20:02.960 --> 00:20:06.470
there is a kind of corollary corollery
00:20:06.480 --> 00:20:08.390
of this which I was thinking of when
00:20:08.400 --> 00:20:11.110
when I read this story. Um and that is
00:20:11.120 --> 00:20:16.310
that back in the 70s uh gammaray
00:20:16.320 --> 00:20:19.510
satellites were launched satellites that
00:20:19.520 --> 00:20:21.909
detect gamma radiation and that was to
00:20:21.919 --> 00:20:26.230
detect any inmosphere nuclear tests uh
00:20:26.240 --> 00:20:28.470
conducted on earth. uh because there was
00:20:28.480 --> 00:20:30.950
a test ban treaty that was signed uh
00:20:30.960 --> 00:20:33.110
that all the signatories said no we
00:20:33.120 --> 00:20:35.270
won't test uh nuclear weapons in the
00:20:35.280 --> 00:20:38.310
atmosphere. Uh but they had to verify it
00:20:38.320 --> 00:20:41.190
and so the verification process involved
00:20:41.200 --> 00:20:42.789
uh a number of satellites being launched
00:20:42.799 --> 00:20:44.549
that could detect gamma rays which would
00:20:44.559 --> 00:20:46.950
be emitted by a nuclear bomb being
00:20:46.960 --> 00:20:49.990
detonated in in the atmosphere. Uh now
00:20:50.000 --> 00:20:52.950
none were none were but those satellites
00:20:52.960 --> 00:20:55.669
are what detected gammaray bursts these
00:20:55.679 --> 00:20:57.669
um you know fascinating pulses of
00:20:57.679 --> 00:21:00.149
radiation that come from uh from
00:21:00.159 --> 00:21:02.070
explosions deep in space.
00:21:02.080 --> 00:21:04.390
>> Yeah. Of course not man-made explosions
00:21:04.400 --> 00:21:06.070
but natural ones. Yes.
00:21:06.080 --> 00:21:09.110
>> Cuz if they do start detecting nuclear
00:21:09.120 --> 00:21:12.149
weapons in space then the parties
00:21:12.159 --> 00:21:14.710
involved uh they won't say oh sorry
00:21:14.720 --> 00:21:15.990
we'll take them all down. They'll
00:21:16.000 --> 00:21:18.470
they'll find ways of hiding them.
00:21:18.480 --> 00:21:21.350
>> Probably. Yes, that's probably right.
00:21:21.360 --> 00:21:23.430
>> Gosh, it's tough, isn't it?
00:21:23.440 --> 00:21:25.029
>> Uh tough world we live in
00:21:25.039 --> 00:21:27.830
>> indeed. Uh and beyond it in some
00:21:27.840 --> 00:21:28.789
respects.
00:21:28.799 --> 00:21:30.470
>> Uh you can read that story at
00:21:30.480 --> 00:21:32.470
universetoday.com.
00:21:32.480 --> 00:21:34.470
This is Space Nuts with Andrew Dunley
00:21:34.480 --> 00:21:37.510
and Professor Fred Watson.
00:21:37.520 --> 00:21:39.110
>> Let's take a short break from the show
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Roger. Your last here also
00:23:28.240 --> 00:23:30.149
>> space nuts.
00:23:30.159 --> 00:23:34.230
>> Our next story, Fred, uh is looking at
00:23:34.240 --> 00:23:36.630
uh all the dust on Earth and where it
00:23:36.640 --> 00:23:38.549
might have come from. Now, I was
00:23:38.559 --> 00:23:41.830
thinking cats because, you know, they do
00:23:41.840 --> 00:23:44.789
shed. Uh but it's uh it's a bit more
00:23:44.799 --> 00:23:47.350
involved than that. And and what is
00:23:47.360 --> 00:23:49.110
really interesting about this story is
00:23:49.120 --> 00:23:51.270
they they think a heck of a lot of it
00:23:51.280 --> 00:23:54.710
came from one source.
00:23:54.720 --> 00:23:56.789
That's right. and it's a mysterious one
00:23:56.799 --> 00:24:00.789
as well. Um so this is quite a nice
00:24:00.799 --> 00:24:03.350
story uh from uh published in Science
00:24:03.360 --> 00:24:08.710
Advances. Um it's about uh the
00:24:08.720 --> 00:24:11.990
micrometeorites that bombard the earth
00:24:12.000 --> 00:24:15.990
and it's a bit surprising this stuff. Uh
00:24:16.000 --> 00:24:18.470
you know we think of meteorites as big
00:24:18.480 --> 00:24:19.669
chunks of rock that come through the
00:24:19.679 --> 00:24:22.230
atmosphere. they have a blaze of glory
00:24:22.240 --> 00:24:24.149
and then land on the earth somewhere.
00:24:24.159 --> 00:24:25.909
And
00:24:25.919 --> 00:24:29.029
what we've got there is a is um a free
00:24:29.039 --> 00:24:32.710
sample of of extraterrestrial material.
00:24:32.720 --> 00:24:33.990
Uh but there are also these
00:24:34.000 --> 00:24:36.230
micrometeorites which rain on the
00:24:36.240 --> 00:24:37.909
earth's atmosphere and they're dust
00:24:37.919 --> 00:24:39.909
particles as you've kind of hinted.
00:24:39.919 --> 00:24:40.310
>> Yeah.
00:24:40.320 --> 00:24:44.230
>> Uh they um and they're sort of always
00:24:44.240 --> 00:24:48.310
falling on Earth. Uh and that uh is
00:24:48.320 --> 00:24:51.669
again it's a free gift from space. Um I
00:24:51.679 --> 00:24:54.950
think so I was sort of vaguely involved
00:24:54.960 --> 00:24:57.430
with this stuff probably 50 years ago
00:24:57.440 --> 00:25:00.149
back in the 70s. I think they were then
00:25:00.159 --> 00:25:02.950
called Brownly particles. Um so I think
00:25:02.960 --> 00:25:05.430
that's what we're talking about. Yeah.
00:25:05.440 --> 00:25:08.549
Uh but they're now I think called cosmic
00:25:08.559 --> 00:25:10.710
ferals. I should check whether Brownley
00:25:10.720 --> 00:25:13.110
particles and cos cosmic ferals are the
00:25:13.120 --> 00:25:17.029
same thing. But basically what they what
00:25:17.039 --> 00:25:20.230
they are is bits of meteor meteor that
00:25:20.240 --> 00:25:23.350
have melted as they come down through
00:25:23.360 --> 00:25:26.070
the earth's atmosphere. But they
00:25:26.080 --> 00:25:27.990
they they actually survive into the
00:25:28.000 --> 00:25:30.149
inner atmosphere and they cool down and
00:25:30.159 --> 00:25:32.950
they form a little sphere because the um
00:25:32.960 --> 00:25:35.190
basically the surface tension of molten
00:25:35.200 --> 00:25:37.830
material brings them into a sphere. Uh
00:25:37.840 --> 00:25:43.190
and that uh is the story so far because
00:25:43.200 --> 00:25:46.470
that um heating that you that they
00:25:46.480 --> 00:25:48.789
experience as the as the sort of parent
00:25:48.799 --> 00:25:51.750
body, the meteor meteor or meteorite as
00:25:51.760 --> 00:25:55.269
it comes through the atmosphere, it uh
00:25:55.279 --> 00:25:57.830
kind of destroys their chemical
00:25:57.840 --> 00:25:59.590
structure. You know that the minerals in
00:25:59.600 --> 00:26:02.390
it get get metamorphosed. They get
00:26:02.400 --> 00:26:03.909
changed because they've been subject to
00:26:03.919 --> 00:26:05.350
very high temperatures.
00:26:05.360 --> 00:26:08.710
>> Yeah. Um but there is a technique uh
00:26:08.720 --> 00:26:13.029
that allows you to look at uh some of
00:26:13.039 --> 00:26:16.390
the characteristics of these objects
00:26:16.400 --> 00:26:19.750
that is not destroyed by heat and it's
00:26:19.760 --> 00:26:24.070
the oxygen isotope signature uh which
00:26:24.080 --> 00:26:25.510
we've talked about before. We've talked
00:26:25.520 --> 00:26:27.990
about isotopes and how they uh you know
00:26:28.000 --> 00:26:29.830
how we distinguish between heavy water
00:26:29.840 --> 00:26:31.750
and normal water and all of that sort of
00:26:31.760 --> 00:26:32.549
thing. M
00:26:32.559 --> 00:26:35.110
>> uh that's so it's basically the the
00:26:35.120 --> 00:26:38.789
number of neutrons in a in an atom. Um
00:26:38.799 --> 00:26:42.630
so you've got these oxygen signatures
00:26:42.640 --> 00:26:47.669
uh that um essentially uh let you uh
00:26:47.679 --> 00:26:51.430
group these cosmic sphererals, the
00:26:51.440 --> 00:26:53.110
Brownly particles if that's what they
00:26:53.120 --> 00:26:56.789
are. Um and it turns out that so so
00:26:56.799 --> 00:26:59.190
people do you know they do population
00:26:59.200 --> 00:27:01.510
census statistics on these objects to
00:27:01.520 --> 00:27:05.029
find out what uh what relationships they
00:27:05.039 --> 00:27:07.269
bear with one another.
00:27:07.279 --> 00:27:10.549
About 10% of them uh of these fererals
00:27:10.559 --> 00:27:12.549
that have been ident identified and
00:27:12.559 --> 00:27:16.710
analyzed uh collect in a group that is
00:27:16.720 --> 00:27:19.590
has got the wonderful name of group four
00:27:19.600 --> 00:27:21.430
uh which presumably means there's
00:27:21.440 --> 00:27:23.029
another three as well.
00:27:23.039 --> 00:27:27.590
>> Yeah. U and it's uh the again what makes
00:27:27.600 --> 00:27:30.789
them stand out in this group is the
00:27:30.799 --> 00:27:33.269
oxygen isotope signature that I just
00:27:33.279 --> 00:27:35.909
mentioned before. It's depleted in uh an
00:27:35.919 --> 00:27:40.149
isotope called oxygen 16. But here's
00:27:40.159 --> 00:27:42.630
where the story gets very interesting
00:27:42.640 --> 00:27:44.310
because
00:27:44.320 --> 00:27:49.029
um no known meteorites have that same
00:27:49.039 --> 00:27:51.510
oxygen isotope signature.
00:27:51.520 --> 00:27:55.110
>> And you'd expect uh if these things were
00:27:55.120 --> 00:27:58.789
common that there would be meteorites uh
00:27:58.799 --> 00:28:01.590
that match them in their composition. Uh
00:28:01.600 --> 00:28:03.990
and often with meteorites we can get an
00:28:04.000 --> 00:28:06.310
idea where they've come from. uh most of
00:28:06.320 --> 00:28:08.149
them come from the asteroid belt from
00:28:08.159 --> 00:28:11.669
collisions between asteroids. Uh so uh
00:28:11.679 --> 00:28:14.549
that um you know that is a bit
00:28:14.559 --> 00:28:16.710
mysterious that we've got these
00:28:16.720 --> 00:28:20.870
subatomic sorry these small ferals of
00:28:20.880 --> 00:28:22.230
material that have come down through the
00:28:22.240 --> 00:28:25.269
atmosphere uh and got that globular
00:28:25.279 --> 00:28:28.789
shape. Um it it's mysterious that we
00:28:28.799 --> 00:28:31.830
don't know we don't see any meteorites
00:28:31.840 --> 00:28:35.190
that match their composition. weird.
00:28:35.200 --> 00:28:38.789
>> It is weird. Yes. Uh and so what they're
00:28:38.799 --> 00:28:42.230
suggesting is that um it's basically
00:28:42.240 --> 00:28:44.149
something that that comes from an
00:28:44.159 --> 00:28:47.430
asteroid whose uh whose characteristics
00:28:47.440 --> 00:28:51.350
are unusual uh that we have not uh yet
00:28:51.360 --> 00:28:53.909
um identified it.
00:28:53.919 --> 00:28:58.070
>> Wow. Okay. So we're still looking.
00:28:58.080 --> 00:29:00.310
>> We're still looking. There's a a sort of
00:29:00.320 --> 00:29:05.510
sub mystery as well because um the a
00:29:05.520 --> 00:29:07.430
detailed analysis of this. You can break
00:29:07.440 --> 00:29:09.590
that group four stuff down into other
00:29:09.600 --> 00:29:13.029
smaller groups and uh some of them
00:29:13.039 --> 00:29:15.990
basically show signs of having had two
00:29:16.000 --> 00:29:19.990
different uh minerals in them before
00:29:20.000 --> 00:29:22.549
they entered the earth's atmosphere. Um
00:29:22.559 --> 00:29:25.750
and um one would be typical of
00:29:25.760 --> 00:29:28.470
well-known uh well-known types of
00:29:28.480 --> 00:29:31.269
asteroids and the other as I said
00:29:31.279 --> 00:29:33.909
doesn't correspond to any kind of known
00:29:33.919 --> 00:29:38.630
um group of uh of um cosmic ferals or
00:29:38.640 --> 00:29:42.549
meteorites. Uh and it's really quite
00:29:42.559 --> 00:29:44.549
remarkable that this you know we're
00:29:44.559 --> 00:29:46.870
being bombarded by dust particles that
00:29:46.880 --> 00:29:49.190
come from somewhere which we haven't
00:29:49.200 --> 00:29:50.149
identified.
00:29:50.159 --> 00:29:53.029
>> Yeah. Wow. Um, could that mean they're
00:29:53.039 --> 00:29:55.510
from beyond our system or it's just a
00:29:55.520 --> 00:29:58.710
part of the system that we
00:29:58.720 --> 00:30:00.950
>> I think it's I don't know.
00:30:00.960 --> 00:30:02.710
>> Yeah, I think it's the other way around.
00:30:02.720 --> 00:30:05.430
Um because the um the team who have done
00:30:05.440 --> 00:30:07.029
the research on this a very very
00:30:07.039 --> 00:30:08.870
thorough piece of research
00:30:08.880 --> 00:30:11.190
>> they've basically
00:30:11.200 --> 00:30:14.630
um as you would you've used simulations
00:30:14.640 --> 00:30:17.909
computer simulations to to essentially
00:30:17.919 --> 00:30:20.789
work out what conditions these things
00:30:20.799 --> 00:30:23.590
formed in when they um melted coming
00:30:23.600 --> 00:30:26.070
through the earth's atmosphere. And it
00:30:26.080 --> 00:30:28.310
suggested that the best fit they get to
00:30:28.320 --> 00:30:30.789
what they see, the the sort of textures
00:30:30.799 --> 00:30:33.990
that are in the material fit with
00:30:34.000 --> 00:30:37.750
relatively low velocities, 14 to 17
00:30:37.760 --> 00:30:39.830
kilometers/s
00:30:39.840 --> 00:30:42.470
uh which is pretty speedy when you think
00:30:42.480 --> 00:30:45.190
of it on Earth, but um uh in space
00:30:45.200 --> 00:30:47.909
that's that's a fairly modest uh space
00:30:47.919 --> 00:30:49.590
speed for a meteorite. They typically
00:30:49.600 --> 00:30:52.230
will be more like 30 kilometers/s.
00:30:52.240 --> 00:30:56.710
And so that low value uh suggests that
00:30:56.720 --> 00:31:01.269
possibly those particles originated in
00:31:01.279 --> 00:31:06.230
near-Earth asteroids um ones that are uh
00:31:06.240 --> 00:31:07.990
following a similar path through space
00:31:08.000 --> 00:31:11.269
to the Earth. Uh, and that might mean
00:31:11.279 --> 00:31:15.029
that we've got some sort of uh in in the
00:31:15.039 --> 00:31:17.350
Earth's environment, some sort of
00:31:17.360 --> 00:31:21.110
unusual asteroid that is not matched by
00:31:21.120 --> 00:31:22.870
all the ones that we know already.
00:31:22.880 --> 00:31:25.110
>> Wow, that'd be something. Uh, that's
00:31:25.120 --> 00:31:26.470
probably going to be hard to track down,
00:31:26.480 --> 00:31:27.350
though.
00:31:27.360 --> 00:31:29.110
>> Yes. Yes, that's probably right. And
00:31:29.120 --> 00:31:30.470
especially since it might not exist
00:31:30.480 --> 00:31:32.389
anymore. It may have collided and formed
00:31:32.399 --> 00:31:33.830
little bits that have
00:31:33.840 --> 00:31:35.669
>> basically rained down on the Earth.
00:31:35.679 --> 00:31:35.909
>> Yeah.
00:31:36.320 --> 00:31:38.950
>> Now, it wasn't fear, Rusty. just throw.
00:31:38.960 --> 00:31:40.310
>> No, it wasn't here. That's right. Yeah,
00:31:40.320 --> 00:31:42.710
thanks Rusty. It's not here.
00:31:42.720 --> 00:31:44.789
>> Um, for the record, Brownley particles
00:31:44.799 --> 00:31:47.269
and cosmic fererals are closely related,
00:31:47.279 --> 00:31:49.430
but they are not exactly the same thing.
00:31:49.440 --> 00:31:50.149
>> Okay,
00:31:50.159 --> 00:31:52.549
>> they represent two different stages or
00:31:52.559 --> 00:31:55.029
types of micrometeorites.
00:31:55.039 --> 00:31:57.029
>> There you go. Thank you for checking
00:31:57.039 --> 00:31:58.389
that. Yes,
00:31:58.399 --> 00:31:59.990
>> that's all right. Um, yeah, they're very
00:32:00.000 --> 00:32:01.669
close, but they're not not the same.
00:32:01.679 --> 00:32:02.950
>> So, I was on the right track.
00:32:02.960 --> 00:32:05.029
>> You were. Yes.
00:32:05.039 --> 00:32:07.909
And you can read all about that at uh
00:32:07.919 --> 00:32:11.110
the Daily Galaxy website. Um and the
00:32:11.120 --> 00:32:14.470
article was published where Fred of Lost
00:32:14.480 --> 00:32:16.070
Science Advances.
00:32:16.080 --> 00:32:17.350
>> Science advances. That's right.
00:32:17.360 --> 00:32:18.070
>> Yes.
00:32:18.080 --> 00:32:19.509
>> Want to read the whole thing before bed
00:32:19.519 --> 00:32:22.470
so you sleep well.
00:32:22.480 --> 00:32:23.190
>> Yep.
00:32:23.200 --> 00:32:24.870
>> Yeah. This is Space Nuts with Andrew
00:32:24.880 --> 00:32:28.630
Dunley and Professor Fred Watson.
00:32:28.640 --> 00:32:30.950
We choose to go to the moon in this
00:32:30.960 --> 00:32:33.430
decade and do the other things not
00:32:33.440 --> 00:32:35.830
because they are easy but because they
00:32:35.840 --> 00:32:36.470
are hard.
00:32:36.480 --> 00:32:38.470
>> These nuts.
00:32:38.480 --> 00:32:41.909
>> Our final story today takes us to the
00:32:41.919 --> 00:32:43.830
edge of our galaxy. Well, it takes us
00:32:43.840 --> 00:32:45.590
from the center of our galaxy right out
00:32:45.600 --> 00:32:47.029
to the edge of our galaxy because we're
00:32:47.039 --> 00:32:48.549
talking about the whole thing locktock
00:32:48.559 --> 00:32:52.149
and barrel. And it appears, Fred, with
00:32:52.159 --> 00:32:55.029
some very clever scientific brains in
00:32:55.039 --> 00:32:57.750
action, that our galaxy stretches out
00:32:57.760 --> 00:33:00.630
further than we thought.
00:33:00.640 --> 00:33:02.950
Uh, it does. It looks as though the
00:33:02.960 --> 00:33:04.630
spiral arms are longer than we thought
00:33:04.640 --> 00:33:05.909
they were.
00:33:05.919 --> 00:33:08.549
>> Uh, and I think this is a very nice
00:33:08.559 --> 00:33:11.110
piece of work. Uh, as as I hinted
00:33:11.120 --> 00:33:14.070
before, uh, partly because it uses a a
00:33:14.080 --> 00:33:16.230
technique that I think is really
00:33:16.240 --> 00:33:17.990
extraordinary. It's a very powerful
00:33:18.000 --> 00:33:19.830
technique uh using what we call light
00:33:19.840 --> 00:33:24.710
echoes. So um so the story basically to
00:33:24.720 --> 00:33:27.669
set this in context, it's very hard for
00:33:27.679 --> 00:33:29.669
us to produce a map of what our own
00:33:29.679 --> 00:33:31.350
galaxy looks like. And that's because
00:33:31.360 --> 00:33:34.389
we're embedded in one of the spiral
00:33:34.399 --> 00:33:37.509
arms. Uh the stars that we see when we
00:33:37.519 --> 00:33:39.430
look at the Milky Way, they're stars
00:33:39.440 --> 00:33:42.070
that fellow travelers in the spiral arms
00:33:42.080 --> 00:33:44.789
with our sun and solar system, but they
00:33:44.799 --> 00:33:46.549
only go out to a thousand lighty years
00:33:46.559 --> 00:33:48.549
or so because the spiral arms are so
00:33:48.559 --> 00:33:51.029
dusty that you can't really penetrate
00:33:51.039 --> 00:33:53.669
much beyond that. Um, and if you were
00:33:53.679 --> 00:33:57.110
relying only on visible light,
00:33:57.120 --> 00:34:00.549
uh, it would be like trying to draw a
00:34:00.559 --> 00:34:04.549
map of the whole of do from standing
00:34:04.559 --> 00:34:08.710
outside do jail there on, um, forgotten
00:34:08.720 --> 00:34:10.230
this mquarry street.
00:34:10.240 --> 00:34:11.430
>> Mcquaryy Street. Yeah.
00:34:11.440 --> 00:34:13.510
>> Yes. Yes. Oh, for the record, they're
00:34:13.520 --> 00:34:15.510
putting a they've t they've taken down
00:34:15.520 --> 00:34:17.109
the public building in front of the old
00:34:17.119 --> 00:34:19.909
do jail, which is now a tourist tourist,
00:34:19.919 --> 00:34:21.589
and they're turning it into a public
00:34:21.599 --> 00:34:23.030
common.
00:34:23.040 --> 00:34:24.790
>> I like that idea. That's that's going to
00:34:24.800 --> 00:34:26.310
look very nice when it's done.
00:34:26.320 --> 00:34:28.389
>> So So that would improve your view of
00:34:28.399 --> 00:34:30.790
the city of do, but it still might not
00:34:30.800 --> 00:34:33.349
let you make a map of DO from
00:34:33.359 --> 00:34:35.669
>> from just there. And that's how we are
00:34:35.679 --> 00:34:37.750
in our galaxy. If you're relying on
00:34:37.760 --> 00:34:39.990
visible light observations,
00:34:40.000 --> 00:34:42.149
uh you're all you're seeing when you
00:34:42.159 --> 00:34:45.510
look is the is the neighborhood of our
00:34:45.520 --> 00:34:47.349
spiral arm, a local spiral arm. You
00:34:47.359 --> 00:34:49.589
don't get any hint or inclination of the
00:34:49.599 --> 00:34:52.710
structure of the galaxy uh beyond that.
00:34:52.720 --> 00:34:55.190
And in particular,
00:34:55.200 --> 00:34:57.270
you know, if we see a a thousand lighty
00:34:57.280 --> 00:34:59.430
years or so, there's another 100,000
00:34:59.440 --> 00:35:01.030
that we're not seeing because that's
00:35:01.040 --> 00:35:04.470
about the diameter of our galaxy. So um
00:35:04.480 --> 00:35:07.589
the situation improves when you use uh
00:35:07.599 --> 00:35:09.589
infrared radiation. You can sort of
00:35:09.599 --> 00:35:12.470
penetrate uh through the dust and see
00:35:12.480 --> 00:35:14.310
actually the center towards the center
00:35:14.320 --> 00:35:16.310
of our galaxy. That's how we know about
00:35:16.320 --> 00:35:17.750
the black hole in the center of our
00:35:17.760 --> 00:35:19.270
galaxy because we could see stars
00:35:19.280 --> 00:35:22.870
orbiting around it. Um but it improves
00:35:22.880 --> 00:35:25.349
even more on a broader scale if you can
00:35:25.359 --> 00:35:27.109
use radio telescopes because you can
00:35:27.119 --> 00:35:31.349
plot uh where the clouds of hydrogen gas
00:35:31.359 --> 00:35:34.870
cold hydrogen uh which radiates in radio
00:35:34.880 --> 00:35:38.470
waves uh with a wavelength of 21 cm uh
00:35:38.480 --> 00:35:40.230
that you can plot out. But if you're
00:35:40.240 --> 00:35:42.390
going to try and draw a map, you do need
00:35:42.400 --> 00:35:43.910
to do some modeling with that. You've
00:35:43.920 --> 00:35:45.589
got to assume things about the rotation
00:35:45.599 --> 00:35:47.510
of the galaxy. So it doesn't just give
00:35:47.520 --> 00:35:50.390
you a direct map. And that could be
00:35:50.400 --> 00:35:52.230
wrong. We could have that little bit of
00:35:52.240 --> 00:35:55.109
it wrong. Uh you know the uh the stuff
00:35:55.119 --> 00:35:57.990
that comes from the radio observations.
00:35:58.000 --> 00:36:02.069
So what's happened now is it's a team uh
00:36:02.079 --> 00:36:06.069
I think they're based in Italy. Uh and
00:36:06.079 --> 00:36:09.750
what they've done is used
00:36:09.760 --> 00:36:14.150
um a direct method of kind of setting up
00:36:14.160 --> 00:36:16.950
a standard ruler. Uh because if you've
00:36:16.960 --> 00:36:18.390
got a standard ruler and you can see it
00:36:18.400 --> 00:36:20.230
in deep space, then you you know how far
00:36:20.240 --> 00:36:21.829
away it is because you know you can
00:36:21.839 --> 00:36:23.670
measure how long it appears to be. And
00:36:23.680 --> 00:36:25.270
if you know how long it is, which is
00:36:25.280 --> 00:36:27.589
what a standard ruler is, then you know
00:36:27.599 --> 00:36:30.390
how far away it is. Um and that's what
00:36:30.400 --> 00:36:32.790
they're doing. They have and and it goes
00:36:32.800 --> 00:36:34.710
back to something we mentioned earlier
00:36:34.720 --> 00:36:36.790
in the show, gammaray bursts, these
00:36:36.800 --> 00:36:39.270
burst of gamma radiation.
00:36:39.280 --> 00:36:42.630
uh those bursts uh don't just directly
00:36:42.640 --> 00:36:45.670
come to us, they also bounce off or are
00:36:45.680 --> 00:36:48.470
reflected by clouds of dust in our
00:36:48.480 --> 00:36:54.470
spiral arms. And uh so by timing how
00:36:54.480 --> 00:36:58.069
long uh it takes for these echoes as
00:36:58.079 --> 00:37:00.150
they're called light echoes even though
00:37:00.160 --> 00:37:03.349
it's gamma radiation uh to what the
00:37:03.359 --> 00:37:07.829
delay is between a light echo and the uh
00:37:07.839 --> 00:37:09.589
source itself which is the gammaray
00:37:09.599 --> 00:37:11.030
burst I should say they probably come
00:37:11.040 --> 00:37:14.550
from collapsing mass massive stars or
00:37:14.560 --> 00:37:17.430
merger of neutron stars uh very
00:37:17.440 --> 00:37:19.109
energetic events because they they're
00:37:19.119 --> 00:37:21.430
bright in gamma radiation. Uh but if you
00:37:21.440 --> 00:37:23.910
look at a light echo from a gammaray
00:37:23.920 --> 00:37:26.550
burst, it gives you a scale to this. You
00:37:26.560 --> 00:37:31.030
you know um how far uh basically it
00:37:31.040 --> 00:37:33.270
gives you a standard ruler um because
00:37:33.280 --> 00:37:35.030
you can time it accurately. You know
00:37:35.040 --> 00:37:37.990
that 300,000 kilometers/s is the speed
00:37:38.000 --> 00:37:40.230
of gamma rays through space. And you
00:37:40.240 --> 00:37:42.310
know if you know how far away it's gone
00:37:42.320 --> 00:37:43.829
in that time, then that gives you a
00:37:43.839 --> 00:37:45.190
distance measure. So you've got a
00:37:45.200 --> 00:37:48.230
standard ruler. Uh it's a very very nice
00:37:48.240 --> 00:37:51.510
way of doing this. And um using that uh
00:37:51.520 --> 00:37:55.589
these uh scientists um as I said at
00:37:55.599 --> 00:37:57.589
least the lead the lead author is
00:37:57.599 --> 00:38:00.790
certainly in Italy at Enough in Milano.
00:38:00.800 --> 00:38:03.910
Uh they uh they've done this work
00:38:03.920 --> 00:38:05.910
looking at these gammaray bursts with
00:38:05.920 --> 00:38:08.230
their light echoes and that allows them
00:38:08.240 --> 00:38:11.349
to calculate basically the size of our
00:38:11.359 --> 00:38:13.510
spiral arms without relying on any kind
00:38:13.520 --> 00:38:15.190
of modeling. M
00:38:15.200 --> 00:38:19.190
>> uh and so they think that the new
00:38:19.200 --> 00:38:22.069
observations indicate that our spiral
00:38:22.079 --> 00:38:25.430
arms are something like 10% longer than
00:38:25.440 --> 00:38:26.550
we thought they were.
00:38:26.560 --> 00:38:27.670
>> Wow. That's a lot.
00:38:27.680 --> 00:38:29.670
>> And yes, that's significant, isn't it?
00:38:29.680 --> 00:38:32.310
It's it's really um you know, this is,
00:38:32.320 --> 00:38:34.310
as I said, this is very nice uh nice
00:38:34.320 --> 00:38:35.670
astronomy.
00:38:35.680 --> 00:38:39.510
>> It is indeed. Yeah. Um of course, as you
00:38:39.520 --> 00:38:41.109
say, we we can't really look at our
00:38:41.119 --> 00:38:43.349
galaxy and we don't know exactly what it
00:38:43.359 --> 00:38:45.109
looks like. Um there's a lot of science
00:38:45.119 --> 00:38:48.150
that they've put together to try and
00:38:48.160 --> 00:38:50.150
create the image of it. And even in this
00:38:50.160 --> 00:38:52.310
particular story, uh which is in the
00:38:52.320 --> 00:38:54.390
universetoday.com, they've got an
00:38:54.400 --> 00:38:57.190
artist's impression of what this new
00:38:57.200 --> 00:38:58.230
look is like.
00:38:58.240 --> 00:38:59.670
>> Yes, that's all you can do.
00:38:59.680 --> 00:39:03.430
>> Reminds me of an upside down snail.
00:39:03.440 --> 00:39:05.349
>> It does. Yes, that's right. A bit.
00:39:05.359 --> 00:39:08.150
>> I see what you mean. Yes. Yes. It's very
00:39:08.160 --> 00:39:09.829
much very helpful.
00:39:09.839 --> 00:39:10.950
>> Or a squid.
00:39:10.960 --> 00:39:12.150
>> Could be a squid.
00:39:12.160 --> 00:39:15.030
>> Could be a squid. Yeah. Uh but in real
00:39:15.040 --> 00:39:18.390
terms, we just have to it's an educ a
00:39:18.400 --> 00:39:20.310
very very well educated guess, I
00:39:20.320 --> 00:39:21.510
suppose.
00:39:21.520 --> 00:39:24.069
>> Um it's Yes, it is. It's it's a
00:39:24.079 --> 00:39:27.349
measurement. So it's it's a it's it's an
00:39:27.359 --> 00:39:28.390
you're right. It's an artist's
00:39:28.400 --> 00:39:29.750
impression. That's really the only way
00:39:29.760 --> 00:39:31.990
we can depict the Milky Way. Some of the
00:39:32.000 --> 00:39:33.750
depictions are very very good and they
00:39:33.760 --> 00:39:35.990
rely on the very best radio and infrared
00:39:36.000 --> 00:39:38.230
observations that have been made. But
00:39:38.240 --> 00:39:40.390
this is going to modify it a little bit
00:39:40.400 --> 00:39:42.870
by our new knowledge of the spiral arms.
00:39:42.880 --> 00:39:46.550
And I should say um the um it's the
00:39:46.560 --> 00:39:50.310
Chandra satellite uh which is an X-ray
00:39:50.320 --> 00:39:54.790
observatory um by operated by NASA uh
00:39:54.800 --> 00:39:56.710
that has been used to make the
00:39:56.720 --> 00:39:59.109
measurements. And I do like the headline
00:39:59.119 --> 00:40:01.910
on a little uh NASA video that there is
00:40:01.920 --> 00:40:04.630
here which is NASA's Chandra examines
00:40:04.640 --> 00:40:06.470
Milky Way at arms length.
00:40:06.480 --> 00:40:08.150
>> Yeah.
00:40:08.160 --> 00:40:11.030
Well done. Very well done. Clever clever
00:40:11.040 --> 00:40:12.310
those words.
00:40:12.320 --> 00:40:13.750
>> Yeah, they are there some good people
00:40:13.760 --> 00:40:14.630
there.
00:40:14.640 --> 00:40:16.630
>> So, the articles in universe today, but
00:40:16.640 --> 00:40:19.829
you can read it in a deeper form through
00:40:19.839 --> 00:40:23.349
the NASA website or the uh astronomy and
00:40:23.359 --> 00:40:25.030
astrophysics journal I think is
00:40:25.040 --> 00:40:27.910
published uh the full paper which is um
00:40:27.920 --> 00:40:30.150
yeah
00:40:30.160 --> 00:40:30.630
journal
00:40:30.640 --> 00:40:33.510
>> lots of numbers in it. Yeah, lots and
00:40:33.520 --> 00:40:36.230
lots of numbers. numbers that are too
00:40:36.240 --> 00:40:39.589
big for my brain.
00:40:39.599 --> 00:40:41.910
>> All right. Uh that's where we end the
00:40:41.920 --> 00:40:43.750
show, Fred. Thank you very much.
00:40:43.760 --> 00:40:46.150
>> Oh, a pleasure. Uh some, as you said at
00:40:46.160 --> 00:40:48.870
the beginning, some nice stories there
00:40:48.880 --> 00:40:49.829
to share them with.
00:40:49.839 --> 00:40:50.870
>> Indeed.
00:40:50.880 --> 00:40:52.310
>> Uh we'll catch you real soon. Thank you,
00:40:52.320 --> 00:40:53.190
Fred.
00:40:53.200 --> 00:40:54.310
>> Always. Thanks, Andrew.
00:40:54.320 --> 00:40:55.990
>> Professor Fred Watson, astronomer at
00:40:56.000 --> 00:40:57.750
large. And uh as I say, between
00:40:57.760 --> 00:40:59.190
episodes, visit our website,
00:40:59.200 --> 00:41:00.790
spacenutspodcast.com
00:41:00.800 --> 00:41:02.870
or spacenuts.io
00:41:02.880 --> 00:41:05.670
if you're a lazy typist. And you can
00:41:05.680 --> 00:41:08.069
have a look around, visit our shop, uh,
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00:41:23.520 --> 00:41:26.230
studio because he didn't turn up today.
00:41:26.240 --> 00:41:28.309
And from me, Andrew Duckling. Whoops.
00:41:28.319 --> 00:41:29.829
Uh, thanks for your company. We'll catch
00:41:29.839 --> 00:41:31.670
you on the next episode of Space Nuts.
00:41:31.680 --> 00:41:32.630
Bye-bye.
00:41:32.640 --> 00:41:34.950
>> Space Nuts. You'll be listening to the
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