#406: Celestial Choreography & Speedy Snapshots: Deciphering Distant Star Systems & The Challenge of Cosmic Photography
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Strap in for an...
The eposode of Space Nuts is brought to you by NordPass....the password manager that will make your life so much eaier for not very much money. Check out our special offer at www.bitesz.com/nordpass - you'll be glad you did.
Strap in for an astronomical journey as Andrew Dunkley and Professor Fred Watson return to answer your burning cosmic questions in this enlightening episode of Space Nuts. Beam up to the cosmos as we tackle the challenges of snapping photos at supersonic speeds with the Breakthrough Starshot project. Viano from Florence brings into focus the hurdles of capturing clear images of distant planets when traveling at a third the speed of light. Could the blur of speed and the distortion of space-time leave us with just a glimpse of Proxima Centauri's secrets?
Next, we delve into the cosmic dance of celestial bodies. Brady from Florida, with a front-row seat to rocket launches, ponders the possibility of a moon having its own moon. Could a satellite's satellite exist, or are the gravitational tugs within our solar system too much for such a delicate balance? Professor Watson explains the intricate gravitational ballet that determines these cosmic relationships.
Then, Scott from Oregon opens a window into the fascinating world of triple star systems with a question about HD 110067. How can stars so far apart still be considered gravitationally bound? Discover the cosmic ties that bind these stellar companions across vast distances.
And for a bonus, we tackle an impromptu query from Dean about the Hubble Space Telescope's remarkable ability to maintain steady images while orbiting Earth. The secret lies in the dance of gyroscopes, but how long can this celestial photography session last?
From interstellar photography to the gravitational waltz of moons and stars, this episode is packed with insights into the mechanics of our universe. Remember to send us your space-related questions, and join us on this voyage of cosmic discovery. Subscribe to Space Nuts on your favorite podcast platform, and until our next stellar encounter, keep gazing at the stars and wondering about the wonders above.
📋 Episode Chapters
(00:00) Andrew Dunkley welcomes your questions for Space Nuts Q and A
(01:52) Riano from Florence in Italy has two questions for us
(04:13) Andrew: Breakthrough project aims to send micro spacecraft to Alpha Centauri
(10:06) I talked about pluto about 100 times, I think
(10:21) Viana raises doubts about whether taking pictures from space is feasible
(12:40) Vienna's question was about the orbits of planets
(14:06) Andrew Dunkley with professor Fred Watson on space nuts podcast
(18:05) Andrew Dunkley: Scott from Oregon questions distance of triple star system
(23:57) Fred Watson says Hubble's lifetime will eventually be limited because gyroscopes failed
Become a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts--2631155/support.
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Hi there, thanks for joining us
on Space Nuts, Q and A.
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My name is Andrew Dunkley, your
host. It's great to have your company,
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and we thank our audience for sending
in questions. We've got some new
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ones the other day, so we're
going to try and knock off a few
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of those in this episode. Viano
has got in touch with us this week.
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He's asking questions about planets and photographing
planets and missions to distant planets that
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we might be able to take a
look at, but will there be problems
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if we want to send back images. We've got a question from Brady,
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could a moon have a moon?
That is? That's a good question,
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let's look into that. And Scott
is asking about the star system HDF one
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one zero zero six seven. I'm
sure you know it well. We'll find
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out all about it this week on
Space Nuts. Fifteen second in channel ten
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nine ignition seek one space nuts or
three two space notes as when I re
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bought it. Neil's good and joining
us to tackle all of those questions with
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most insightful answers. Professor Fred what's
an astronomer at large? Hello Fred,
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Hello Andrew. Hopefully this will be
Q and A rather than Q and not
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A, which is always the risk. You know, it is a bit.
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But you know, even when we
get questions we can't answer, which
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we've actually received while we've been talking
today, we really chase them up if
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we can, so never never be
discouraged. We we do. We'd love
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to get your questions, and I
will tell you how to do that at
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the end. Let's go to our
first question, Fred, And this one,
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as I said, comes from Viano. Hey, guys, from Flo
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in Italy. So I have a
two questions for you. The first one
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is related to the break To project
with old us that they want to reach
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comoch entiality with the sort of solar
sale at around one speed of light,
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which I think it means more or
less one another kiln we just per second.
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I worked within the other cameras and
I know how difficult it is to
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find the right time configuration the optical
alensis focused and so on, and I
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was thinking that maybe it will not
be possible to take a clear picture of
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a planet if you're moving so fast
in front of What do you think about
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that? The second question is related
to the planet ORBITA. So can you
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please explain me what is that?
Defines the distance between the planet and stand
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so for sure there must be a
sort of gravity equilibrium, but I cannot
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understand why they are not in order
considering the mass or the envolumements, so
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there must be something else. And
so, guys, I started listening to
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you because of to learn us on
English. I'm pretty sure if my English
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is not so rude or in books, but based ont the looking at this
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guy, I love this US now
and I think it is great great,
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So thank you guys, my mate, Thanks Fiano. I'm a little bit
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disturbed that you think we're going to
be helpful with your English, but now
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I'm really pleased that you said us
a question. Your English is actually very
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good, and indeed we understood perfectly
what you were asking us. But thanks
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for sending in a question. It's
greatly appreciated. And having been in Florence
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fairly recently, what an amazing place
you live in, a beautiful part of
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the world. I happen to be
there at All Saints Weekend, which is
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a four day public holiday, and
there were thousands and thousands and thousands of
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people there. It was almost impossible
to move through the city square and see
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all the sites just everyone flocked to
Florence that weekend, big religious holiday.
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But what an amazing place. Yes, and beautiful part of Italy too.
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It's yeah, just extraordinary around there. Now he mentioned the Breakthrough project.
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This is the plan to send micro
spacecraft on a flyby of Alpha Centauri,
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the planets of Centaury B. Is
it? And they they won't be able
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to stop. I remember it's talking
about that. So let's just sort of
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review what Breakthrough is about and then
try and answer Viano's questions as to whether
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or not we'd be able to send
back a photo or two. This is
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actually a great question, and I
think there's quite a lot of subtlety to
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it. So it's a Breakthrough starshot
and that project was initiated by Uri Milna,
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billionaire who set up the Breakthrough Foundation
in order to study the possibilities of
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using light sales, laser driven light
sales to accelerate a spacecraft which might only
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weigh less than a kilogram, you
know, it's tiny stuff. We're talking
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about to a speed which would allow
you to reach Proxima Centaury, the nearest
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of the Alpha Centauri system, a
dwarf red dwarf star within a you know,
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within a reasonable number of years.
And so yeah, if you accelerate
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it to a third of the speed
of light one hundred thousand kilometers per seconds,
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as Fianna says, then you're probably
going to take I mean alone for
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acceleration and deceleration, you're probably going
to take less than twenty years to get
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your four light years away. And
that then you but then you faced with
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the issue and it probably wouldn't be
just one spacecraft. I think it will
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be a little flotilla of sail driven
spacecraft which would fly along the laser line
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accelerated. Sorry, there's the people
are people are complaining about our rooster Andrew.
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They think he's they think he's a
cockrel. He's not. He's a
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dog with a stupid voice. And
he does that when someone turns up.
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He does even when not when somebody
turns up, he just does it because
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it just doesn't occur. Well,
look, I've counseled him the nature of
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little terriers or little terrors, whichever
way you want to look at anyway,
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So yeah, you whizz through the
proximate centaury system and he does have planets
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one hundred thousand kilometers per second,
you've got cameras that are supposed to be
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able to photograph planets. You want
to photograph them in enough detail that you
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can actually see what's going on on
their surface. That is an incredibly difficult
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problem. The nearest thing I can
draw up parallel to, which was very
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successful was New Horizons fly by the
Poluto system back in twenty fifteen. Is
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that right? Fourteenth of July twenty
fifteen. I think that was it?
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Let me check brains, Yeah,
you check that, and the actually I
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might have the fourteen might be something
else, because my recollection is that the
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fly by velocity the fourteen was the
fourteenth of July twenty fifteen. There you
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go, that's got it right,
yeh. Check. Check the other figure
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for me, though, Andrew,
because I think, if I remember rightly,
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the fly by velocity was fourteen kilometers
per Second's yeah, I haven't got
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that, but I will look it
up now, okay, just to make
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sure. So, and that was
an amazing feat of engineering. Twenty three
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kilometers per second, okay, twenty
three, So I'm mixing up the fourteen
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of the day. Yeah, twenty
three kilometers per second. That are you
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sure that was the fly by velocity. That sounds more like the maximum velocity.
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Well, hang on, I'll keep
looking. Yeah, I think it.
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I think it was the fastest spacecraft
ever launched because at one point in
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its trajectory probably new horizons flew within
twelve and a half thousand kilometers of Pluto
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at a relative velocity of eleven kilometers
eleven Okay, that sounds more like it.
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Yes, eleven kilometers per second.
It's a very small percentage of one
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hundred thousand kilometers per second, which
is what the fly by speed will be
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for any breakthrough space shot star shot
initiatives. But it was highly successful what
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they had to do because you can't
control this in real time, Andrew,
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because you've got you know, I
can't remember what the time delay was,
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but it was minutes out to get
the signal out there, and this thing
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flashes by. So they had a
pre arranged sequence of shots the camera angles
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to get not just Pluto as if
as they flew by, but Pluto's moons,
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all of them, including the biggest
one care on they did. They
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did fantastic planning and built into the
engineering of this so that when you know,
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the spacecraft got within x thousand kilometers
of Pluto. This sequence started and
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it was executed perfectly. It was
just a choreographed set of imagery. And
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of course, I guess we're all
familiar with the dramatic pictures that were returned
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six hours be time delay six hours. There you go. Yeah, so
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thank you. I'm glad. It's
a long time ago. What's that it's
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nine years ago since all the Gift
talks I talked about about one hundred times,
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I think, so I knew the
numbers. But receding in the past
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anyway. So the issue that that
Vianna raises, we have a different set
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of circumstances here. We've got these
tiny little machines which have cameras on board
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pointing hopefully in the right direction.
You've got a four and a half year
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time lag back to Earth, so
there's no chance whatsoever of pointing the thing.
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It has to all be done robostically. So you can have sensors on
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board that will look for the brightest
object in the field of view and basically
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point your camera towards it. But
one hundred thousand kilometers per second, there
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are also what we call relativistic effects. The geometry of space changes, so
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you're not just taking you know,
saying that well, we know where these
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things are, we can point the
camera at them. You've got to take
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into account the fact that space is
distorted by the relative velocity one hundred thousand
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kilometers per second, third of the
speed of light, which will change the
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directions of the things that you're looking
in. It basically squash squashes the stars
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forward in your field of view in
that relativistic effect. So all those phenomena
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and I think, you know,
if the animal's amazing doubts about whether this
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is feasible, I think is right
on the money, because I think it
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is so difficult to do. We
don't even know whether the technology would work
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to get us there in that length
of time. But it's a very interesting
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problem and it's one that needs to
have interesting answers. Indeed, I mean
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buried and play. Other effects like
the distance of the planet from the stars,
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exposure times. Yeah, there's so
many other factors that need to be
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back and I'm sure the scientists involved
would take that into account, but there's
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certain things they won't be able to
control. And when you're talking robotics,
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once they're on their way, that's
it. You're not really going to be
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able to do much once they get
too far away to to take those photographs
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and transmit them back. You just
just going to sit and wait and hope
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and pray that it all works and
then four and a half years less you
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get your pictures. But yeah,
and it's just your lucky blob. Yeah.
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Now, the other bit of question
was about the orbits of planets,
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and it is. It's a great
it's you know why planet's in a particular
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orbit. There's the orbit is basically
dictated very much by the distance the two
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go completely together. In fact,
the mass of the object itself is of
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less important. For example, you
know, if you're in Earth orbit,
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if you're at four hundred kilometers,
you've got to have a certain velocity to
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stay in orbit, whether you're a
cube SAT or whether you are the International
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Space Station much more massive than a
cube SAT. So it's all about the
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orbital velocity and the distance from the
Sun. That's what dictates basically where planets
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stay. They've obviously formed there at
those distances. We think the gas giants
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are gas giants because they're beyond the
frost line, so that they grew big
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as they accumulated ice and that made
them, you know, give them the
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possibility of accumulating still more material to
gas around them. I hope that answers
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the question beyond Bianna. Thanks very
much and so good to hear from you,
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and hope all is well in Florence. This is Space Nuts Andrew Dunkley
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with Professor Fred Watson Space Buds.
Now, Fred, we've got a text
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question that's come in from Brady.
Hello from the great state of Florida,
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with a great view of all the
launches here, are you lucky Duck?
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I was wondering if a moon could
have a moon also, would that be
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called a moon? Moon? Love
listing to you all every week, Brady.
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Thanks Brady, very jealous of where
you are. I'd love to be
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able to sit and watch a few
launches from Florida. What a mesmerizing place.
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I've been lucky enough to visit there
and found it all very extraordinary.
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Could a moon have a moon?
Fred? Just a footnote to that.
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I'll be there in about three weeks, and yes you will. By the
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time this episode's out of me,
you're probably already. But moon of the
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moon, Yes, such an object
will be defined as a sub satellite,
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so satellites are moons. It satellites
the technical term that we use nowadays.
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People think of them as artificial satellites, but actually the word means the satellite
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of a planet, something going around
a planet. A sub satellite will be
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something going around a satellite, And
the the answer is yes, it could.
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Theoretically, you could have a sub
satellite, you could have a moon
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of a moon, but the odds
are that they're quite rare. And the
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reason for that is that we know
of none in the Solar System. Of
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all the two or three hundred moons
that we know in the Solar System,
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I can't remember the exact number now, none of them have a sub satellite.
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None of them have a moon.
So that is probably because theory suggests
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that, and this would depend on
what the planet was like the planet that
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these things are going around. It's
the tidal effects of the planet that are
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probably what would disturb or what has
disturbed any possible sub satellites in the Solar
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System. So what I'm saying is
in the Solar System at least, the
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reason why we don't find moons of
moons is because of the gravitational pull of
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the planets themselves. These actually make
the would make it unstable, so you
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lose the moon of the moon.
The moon itself might stay there, but
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this other moon going around it might
be too unstable. And it's all of
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00:16:52.759 --> 00:16:56.559
it just because of the tidal effects, that's the gravitational pulling effects of the
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planet itself. But that might not
always be the case. It's the case
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in the Solar System, but it
might not always be the case. And
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00:17:06.119 --> 00:17:15.839
there is at least one basically one
planet, which is Kepler sixteen twenty five
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00:17:15.960 --> 00:17:23.319
B, which which could in theory
have a satellite, and in theory could
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have a sub satellite. So that's
just because of the gravitational you know,
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distribution between the parent star which is
Kepler one six two five and the planet
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Kepler one six two five B.
That's that's one suggestion. But as far
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00:17:38.759 --> 00:17:42.920
as we know, there are any
in the Solar system, Okay, So
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for it to happen, the circumstances
have to be exactly right, exactly that's
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00:17:48.880 --> 00:17:52.039
right, to be a bit special. The answer to your question for two
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00:17:52.079 --> 00:17:55.279
hundred and ninety three moons in the
Solar system, Oh there you go,
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00:17:55.799 --> 00:17:59.400
two ninety three. Thank you,
at last count, At last count,
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00:18:00.599 --> 00:18:03.839
thanks Brady. I like your name
better moon Moon. That works for the
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00:18:03.920 --> 00:18:07.880
moon. Yes, this is space
Nuts. Andrew Dunkley here with Professor Fred
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00:18:07.920 --> 00:18:23.279
Watson. Three four Space Nuts.
Now we've got a question from Scott Hey.
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00:18:23.359 --> 00:18:29.599
This has Scott from Oregon. I
recently became aware of HD eleven zero
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00:18:29.720 --> 00:18:37.319
zero six seven system because apparently it
has six exo planets that are orbiting in
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00:18:37.480 --> 00:18:44.079
like a I I think, perfect
mathematical arrangement or something. But my real
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00:18:44.160 --> 00:18:48.440
question is really about like it's a
part of a triple star system, and
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00:18:48.480 --> 00:18:56.160
at least according to the information I
found, the companion planet is it's actually
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00:18:56.160 --> 00:19:04.240
a companion binary star system is thirteen
thousand, four undred astronomical units from the
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00:19:04.319 --> 00:19:07.799
primary star. And I'm just kind
of curious, is why when something is
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00:19:07.839 --> 00:19:12.440
that paraway, is it kind of
considered still like a triple star syst.
213
00:19:14.079 --> 00:19:18.599
I just assumed the you know,
we're I mean, that seems like a
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00:19:18.640 --> 00:19:22.359
really far distance for them to still
be kind of considered together. So I'm
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00:19:22.359 --> 00:19:26.599
just go curious start how they caind
of categorize these things. Thanks, thank
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00:19:26.599 --> 00:19:30.799
you, Scott. That is a
great question a triple star system, but
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00:19:32.079 --> 00:19:37.440
he's questioning distance and whether or not. It could actually be that. Yeah,
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00:19:37.480 --> 00:19:41.839
that's how far is too far for
a binary slash triple star system.
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00:19:44.480 --> 00:19:49.039
That's look at again. This is
a great question, and it's it's really
220
00:19:49.720 --> 00:20:00.640
all about gravitational what we call gravitational
binding. So that's star HD sixty seven
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00:20:02.480 --> 00:20:07.759
is gravitationally bound to this spectroscopic binary
system, which is called HD eleven zero
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00:20:07.799 --> 00:20:17.599
one zero six. Now you know
that eleven double zero sixty seven is interesting
223
00:20:17.640 --> 00:20:22.240
because of these six planets which are
in a lovely orbital resonance with each other.
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00:20:23.119 --> 00:20:29.640
It's at a distance of one hundred
and five light years. But Scott's
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00:20:29.680 --> 00:20:33.079
question isn't really about the planet.
There's the star and its planets. It's
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00:20:33.119 --> 00:20:40.000
about this companion binary system. What
do we mean by a spectroscopic binary system?
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00:20:40.319 --> 00:20:44.319
A binary system is two stars orbiting
around the common center of gravity,
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00:20:44.400 --> 00:20:48.880
usually called the Barry center. If
it's spectroscopic, it means we can't see
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00:20:48.880 --> 00:20:52.160
them as two separate stars. We
can see them as a single star in
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any telescope. But we know it's
two stars because the spectroscope of the spectrograph
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00:21:00.039 --> 00:21:07.000
reveals by the Doppler effect that there
are two sets of barcodes which are moving
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00:21:07.119 --> 00:21:11.960
relative to one another as the stars
orbits each other. So it's by using
233
00:21:11.000 --> 00:21:15.359
the spectroscope that we know that there
is a pair of stars there rather than
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00:21:15.400 --> 00:21:22.960
just a single one, whereas HG
double one double zero sixty seven itself is
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00:21:23.000 --> 00:21:30.519
said to be part of this as
a triple star system. So Scott quotes,
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00:21:30.519 --> 00:21:33.599
and I haven't actually verified this,
but I'm sure he's right. Thirteen
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00:21:34.039 --> 00:21:41.799
four hundred astronomical units of separation between
them. Now, that's about a quarter
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00:21:42.240 --> 00:21:49.000
of a light year. A light
year is about sixty three three hundred astronomical
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00:21:49.160 --> 00:21:52.960
units, or what's an astronomical unit
distance from the Earth to the Sun one
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hundred and fifty million kilometers. So
an astronomical unit is a unit we use
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00:22:00.079 --> 00:22:03.480
within the Solar system. Tend to
use light years beyond the Solar system,
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00:22:04.200 --> 00:22:07.359
but for a triple star system,
that is quite a long way off.
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00:22:07.400 --> 00:22:11.759
Thirteen thousand and four audio astronomical units. As I said, it's roughly a
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00:22:11.839 --> 00:22:15.839
quarter of a light year. I'm
going to throw in a coincidence here,
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00:22:15.079 --> 00:22:22.240
Andrew that you probably don't know about, but the number of astronomical units in
246
00:22:22.279 --> 00:22:25.440
a light year is, as I
said, about sixty three thousand, three
247
00:22:25.519 --> 00:22:29.559
hundred is very very similar to the
number of inches in a mile, which
248
00:22:29.559 --> 00:22:33.200
is about sixty three thousand and three. Right. Wow, it's a nice
249
00:22:33.240 --> 00:22:37.079
coincidence that we can't use anymore because
we're electric here, well anyway, except
250
00:22:37.359 --> 00:22:42.359
they can use it in America they
can, yes, But so what means
251
00:22:42.480 --> 00:22:49.000
what defines it as these two are
the binary and the star itself HD eleven
252
00:22:49.079 --> 00:22:55.200
zeros or A sixty seven, what
makes it a triple star system. It's
253
00:22:55.240 --> 00:23:00.000
because they are gravitationally bound. The
movement of the two relative to each other
254
00:23:00.279 --> 00:23:03.880
tell you that they are in orbits
around their common center of gravity. And
255
00:23:03.960 --> 00:23:11.440
so once again that's detected spectroscopically and
probably actually also by the Gaya astrometry spacecraft,
256
00:23:11.480 --> 00:23:15.519
which can measure the positions of stars
very very accurately. Indeed, so
257
00:23:15.079 --> 00:23:21.319
I think that is why it's termed
a triple system rather than just two stars
258
00:23:21.319 --> 00:23:23.759
that have to be near each other. It's because they've got movements that suggest
259
00:23:23.799 --> 00:23:29.039
that they're gravitationally bound to each other. They are dancing. They're dancing what
260
00:23:29.119 --> 00:23:32.279
a lot of the most book,
Yes, yeah, well a dance like
261
00:23:32.359 --> 00:23:37.640
me. One of them is going
to fall over real quick indeed, so
262
00:23:37.960 --> 00:23:44.079
there you ask God. Hopefully that
will appease you at least answer your question.
263
00:23:44.799 --> 00:23:47.200
We've got one without notice, and
I know you love those Fred.
264
00:23:48.640 --> 00:23:56.799
This comes from a Facebook user listener, Dean A. Fellas. A question
265
00:23:56.920 --> 00:24:02.240
for you, how does Hubble maintain
a steady image of targets while in orbit?
266
00:24:03.119 --> 00:24:10.720
It's stabilized, and what stabilizes it
are gyroscopes, which are an absolutely
267
00:24:10.839 --> 00:24:17.519
vital part of the mechanism that operates
Hubble, and in fact it's why Hubble's
268
00:24:17.559 --> 00:24:25.799
lifetime will eventually be limited because the
gyroscopes did fail. I think they need
269
00:24:25.839 --> 00:24:27.880
three. I think they can just
about manage with two, but they need
270
00:24:27.920 --> 00:24:36.119
three to work properly. Back in
the day, two thousand, probably two
271
00:24:36.200 --> 00:24:45.000
thousand and eleven ish thereabouts, trying
to think when the yeah, I think
272
00:24:45.000 --> 00:24:51.920
twenty eleven was when the last Hubble
mission, Hubble repair mission went up,
273
00:24:51.960 --> 00:24:55.960
and it was to repair or to
replace gyroscopes. That was in the last
274
00:24:56.039 --> 00:25:00.279
year or so of the Space Shuttle, because the Space Shuttle was the only
275
00:25:00.359 --> 00:25:04.160
vehicle then available that could reach the
orbit of the of the Hubble Space Station
276
00:25:04.519 --> 00:25:10.400
sorry Hubble space Telescope at six hundred
kilometers, so it's gyroscopes which have failed.
277
00:25:11.160 --> 00:25:14.759
They're still working pretty well as far
as I know, but maybe again
278
00:25:14.759 --> 00:25:17.440
they will fail and that will bring
the mission to an end, because you
279
00:25:17.440 --> 00:25:22.240
want me to point the telescope,
Yes, exactly, And that was twenty
280
00:25:22.279 --> 00:25:27.039
twenty three, I think when Yeah, No, it was a while further
281
00:25:27.720 --> 00:25:32.079
further back than that. I remember
us talking about those gyro failures. Wasn't
282
00:25:32.079 --> 00:25:37.160
that long ago? There might have
been other ones, could have been been
283
00:25:37.240 --> 00:25:40.279
since that mission. I mean,
Hubble's been up there at it for a
284
00:25:40.359 --> 00:25:45.039
very long time. Things don't last
for four years. Yeah, it's incredible,
285
00:25:45.119 --> 00:25:49.799
isn't it. Of course there are
going to be new telescopes like James
286
00:25:49.799 --> 00:25:53.640
web in Action and the new one
that he says set up, and of
287
00:25:53.680 --> 00:25:59.319
course we talked about one Lancy Grace
Roman Times, yeah, which is also
288
00:25:59.359 --> 00:26:02.519
going to be launched in a few
years. So plenty more going up there
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00:26:02.559 --> 00:26:07.039
to continue the work. But yeah, thanks for the question. Lovely to
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00:26:07.079 --> 00:26:10.599
hear from your dean, And if
you do have questions for us, please
291
00:26:10.839 --> 00:26:15.559
send them to us via our website, space nuts podcast dot comspacenuts dot io
292
00:26:15.799 --> 00:26:19.799
and send it to us simply by
clicking on the relative button you can click
293
00:26:19.839 --> 00:26:23.599
on the AMA tab where you can
send us audio or text questions, or
294
00:26:23.640 --> 00:26:26.640
on the right hand side this this
weird green button that says send us your
295
00:26:26.680 --> 00:26:32.599
questions. When you hover over it, it turns purple. Yeah. I
296
00:26:32.599 --> 00:26:34.480
don't know, but you can send
us your question there as long as you've
297
00:26:34.519 --> 00:26:41.440
got a device with a microphone.
All good, and don't forget to tell
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00:26:41.519 --> 00:26:44.160
us who you are and where you're
from, and we'll do our best to
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give you an answer. Fred.
That's the end of another episode. Thank
300
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you, sir, pleasure, good
questions and great stuff. Keep them coming
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in, folks. It's great to
Yeah, all right, Fred, catching
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next week. Thank you, Professor
Fred Watson Astrong at Large. And thanks
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00:27:02.119 --> 00:27:04.920
to Hue in the studio who were
funneled through a couple of late questions that
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00:27:06.000 --> 00:27:08.640
we managed to well. We put
one on the back burner and we tackled
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00:27:08.640 --> 00:27:11.559
the other. And from me Andrew
Unkley, thanks for joining us. Catch
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00:27:11.559 --> 00:27:17.119
you on the very next episode of
Space Nuts. Bye bye. You'll be
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00:27:17.279 --> 00:27:25.039
listening to the Space Nuts podcast available
at Apple Podcasts, Spotify, iHeartRadio,
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00:27:25.400 --> 00:27:29.839
or your favorite podcast player. You
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