April 28, 2024

#412: Cosmic Queries: A Voyage to Voyager & Defending Astronauts Beyond Earth

#412: Cosmic Queries: A Voyage to Voyager & Defending Astronauts Beyond Earth

Prepare to illuminate the mysteries of cosmic luminescence with Andrew Dunkley and Professor Fred Watson in this enlightening Q&A episode of Space Nuts. Our stellar duo navigates the void to answer Lee from New York's luminary question: How much...

Prepare to illuminate the mysteries of cosmic luminescence with Andrew Dunkley and Professor Fred Watson in this enlightening Q&A episode of Space Nuts. Our stellar duo navigates the void to answer Lee from New York's luminary question: How much light is there in space? Could we see Voyager 1 in its distant travels, or would it merely be a shadow against the cosmic tapestry? Fred sheds light on the subject, revealing the surprising capabilities of the human eye in the darkest reaches.
Next, Fenton from Minnesota proposes an ingenious method for shielding astronauts from the relentless radiation beyond the Van Allen Belts. Could a miniaturized version of these protective fields be the key to safe space exploration? Fred unpacks the complexities of cosmic radiation and the futuristic technologies that might one day safeguard our interstellar voyagers.
Robert from Vienna ponders a parallel universe where our moon is not the cratered time capsule we know, but an icy or hazy sphere like Europa or Titan. Would our understanding of the solar system's history be drastically different? And would astronauts have dared to tread on such enigmatic surfaces? The answers might just surprise you.
Finally, Duncan from Weymouth queries the nomenclature of the outer planets, challenging the distinction between 'ice giants' and 'rock giants.' Fred clarifies the frosty moniker, explaining why Uranus and Neptune's chilly atmospheres earn them this cool classification.
From the potency of starlight to the protective puzzles of space travel, this episode of Space Nuts is a cosmic cornucopia of knowledge. Remember to share your own astronomical inquiries via the Space Nuts website, and join us as we continue to unravel the universe's most perplexing enigmas. Until we next embark on our celestial sojourn, keep pondering the heavens and stay tuned for more galactic revelations.
Support our journey through the cosmos by visiting https://www.spreaker.com/podcast/space-nuts--2631155/support. Your support helps us keep the starlight shining on these interstellar discussions. Until the next transmission, keep your telescopes trained and your curiosity alight.

This episode is brought to you with the support of NordPass...the password manager you need to make life less stressful...and by using our special deal...for not very much money. Plus you'll be helping support our show. For details visit www.bitesz.com/nordpass

 

 

WEBVTT

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Hi there, thanks for joining us
on a Q and A edition of Space

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Nuts. I'm Andrew Dunkley, your
host once again. Thanks for joining us

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and good to have your company on
this edition. We're answering some questions about

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light in space. This one comes
from Lee's asked a very interesting question.

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I've never actually thought about this particular
concept, but it's a question that I

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think is worth answering for sure,
That's why we included it. Fenton wants

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to know about shielding astronauts in the
outer reaches of the Solar System, and

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he's got an idea on how to
do that. Robert wants to talk about

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things we learned from the Moon and
what if our moon wasn't the same as

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the Moon is now, would our
learnings be different. That's a really interesting

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question. And Duncan wants to talk
about ice giants and why are they ice

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giants? Why don't we call them
something else? That's all coming up shortly

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on this edition of Space Nuts ten
nine ignition Space Nuts or three two Space

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Nurse as when I we bought it. Bill's good. Once again, we

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welcome the one and only Fred.
What's an astronomer? At Tello? Fred?

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Hello and how have you been since
we lost I haven't moved from this

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seat you all that time? Well, it's I can see you glued to

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your chair there very much. So
shall we get straight into it and answer

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some questions from our audience? We
will, it is that's what we're here

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for. This first one, Fred
comes from Lee. He lives in New

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York City. He's asking how much
light is in space? You'll qualify that

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question. For example, if you
were to visit Voyager one where Voyager one

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is today, would you be able
to see it? Would you see just

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a silhouette? Would you be able
to make out details and colors if there

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are any colors on it? What
about if you and voyage were midway between

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the Sun and Alpha Centauri. Can
we know a reasonably accurate answer or is

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it pure speculation? Thanks love the
show. Lee from New York, I've

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never thought about that. I mean, we take for granted light on Earth

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because we're illuminated by the Sun,
but it's a bit different in other parts

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of the Solar System and the universe
in general. So yeah, if we

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could just go snap, we're out
there next to Voyager one, could we

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actually see it? Is it illuminated
in any way. Is it being illuminated

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by something? What would it be
like? The answer is yes, you'd

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see it. And so we're talking
really now about the sensitivity of the human

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eye, because with a camera,
you know, with the long exposure settings

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and things, you'd be able to
see in great detail. But thinking about

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the human eye. So I used
to work, as you know, signing

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Spring Observatory. I spent many hours
outside at night. There. It is

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a place that is truly dark.
There's no interference from street lights. There

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are a few blobs of light on
the horizon, but nothing that affects the

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pristine darkness of the night sky.
And on a starry night, with the

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sun not in the sky, you
can see quite clearly. There's enough light

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from the stars themselves to let you
see where you're going, let you walk

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around and be quite confident that you're
not going to fall off the mountain,

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as I nearly did one night when
it was cloudy. I went out without

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my torch and thought, oh yea'll
see by the stars. But fortunately,

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unfortunately the cloud had come in.
I could see anything, and I nearly

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fell off the mountain. I didn't
in the end, but a long drop

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three. Yes it is. Yes, it's quite a long drop anyway,

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if you you know, normally on
the starry nights, you will see by

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the light of the stars. Now, where Voyager is Voyager one, I

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just looked it up. It is
at a distance from the Sun in astronomical

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units, which is one hundred and
sixty three astronomical units. That's one hundred

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and sixty three times the number of
times the distance between the Earth and the

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Sun. So that's one hundred and
fifty million kilometers. Multiply that by one

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hundred and sixty three and you will
get what do you get? So I

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was looking for eighty kilometers, but
it's not there. I'll have to do

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the numbers anyway, it doesn't matter. The main thing is its distance is

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twenty two point five y five light
hours away. That's how long it takes

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the signal to get from Voyager to
Earth. It's almost a day. It's

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almost a light day away. So
at that distance from the Sun one hundred

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and sixty odd astronomical units, there's
still significant light coming from the Sun.

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Not to mention Venus and you know, Jupiter, the other planets, mostly

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the Sun. Though you're being illuminated
by the sun, so that's certainly opposite

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as compared with just being illuminated by
the starry sky, which is what I

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was just talking about. So you'd
see it really clearly. You wouldn't have

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any problem making it out, assuming
you I was dark adapted, so it's

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fairly bright out there. We talked
about the sensitivity of the human eye,

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as you referred to how small amount
of a light can we see as human

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beings. I think there were some
experiments let me think it one photon or

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one yes, that's right. We
might have talked about this. There were

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experiments done that showed that the human
eye is capable of detecting single photons.

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It was under special circumstances, but
that is just extraordinary when you think that

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the human eye can also cope with
broad daylight. That's the amazing thing about

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the human eye. It can.
You know, it's quite happy to see

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light at one brightness and then a
light that's only a million as bright if

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I deal with that, and that's
a combination of what's called retinal bleaching and

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the iris of your eye opening and
closing. It's all those things come together

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to give you this unbelievably versatile and
sensitive tool with which we can look at

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the surroundings. Whether it's the rock
face I'm looking at now, because that's

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what about yea it consists of,
or whether it's you know, the night

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sky where you're looking at faint objects
in the sky. It's quite amazing.

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So even if you win deeper into
space, way beyond our solar system,

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you you would probably still see objects
that you were near. There be enough

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light from the stars. The Milky
Way is bright. It would it would

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you know, even if, as
as Lee says, if even if you

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were halfway between the Sun and Alpha
Centauri, you'd still see it because of

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the ambient light that's coming from from
the stars. Yeah, and you'd still

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see color because that's well, yeah, it's dark enough, it might turn

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into the grays, which happened.
Yeah, and I think that's likely.

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I think I don't think you would
see color. You would. You would

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where it is now, there's enough
light coming from the Sun that you'd see

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color. But I think when you
got further out you would start to just

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see the you know, the as
you said that that feed that's sort of

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pale gray appearance where you look at
very low low light levels, indeed where

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the color cells aren't recept Mmm,
they got LEI the answer of questions yes

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to all of the above, basically
question excellent question. All Right, let's

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move on. This is from Fenton. Yeah, hello Fred and Andrew.

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This is Fenter contacting from Saint Paul, Minnesota in the US. I sort

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of have a different type of astrophysical
question for you, and this is on

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how to shield astronauts from radiation outside
of the Van Allen I was curious if

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you know of any pending technologies that
would allow this of this choice would some

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people would say is lead? But
I can think of several reasons why this

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is not a good idea. How
about a miniature down Allen Belt which could

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surround a spacecraft? How does that
sound? How could this become a reality?

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Thank you very much. I hope
you liked the question. I now

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thanks vent and Venton always has these
intriguing thoughts. I've noticed in the times

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that we've heard from him. Maybe
we should start by explaining what the Van

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Allen Belt is. For those of
us who just can't remember, like me,

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it's sort the Van Allen Belt,
so that basically the the you know,

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the magnetic shielding around the Earth,
which is caused by the magnetism of

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the Earth. It's caused by the
fact that we've got an iron core and

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basically it's in two parts. It's
solid and liquid, so it acts like

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a dynamo. It's rotating, and
that gives us this exactly the protection that

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Fenton is talking about. I was
going to refer I'm a bit annoyed.

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Actually lost it. There is a
very nice article on it's actually on the

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BBC's website, their Sky at Night
website. There's a lovely article on exactly

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this here I found it. I
hadn't lost it. How astronauts can hide

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from radiational mars and it goes into
the exactly the problem that Fenton's talking about.

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How do you present how do you
prevent astronauts basically becoming irradiated and over

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time it's basically lethal because of the
cosmic radiation that's coming down through space and

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it does sell damage in your body
and it can actually trigger cancer. So

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the whole study of this is sorry, the thrust of this article BBC Sky

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at Night Magazine is to discuss how
you might protect astronauts from the radiation and

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that's not just on Mars but en
route. Okay, the solution that Fenton

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has suggested is covered in a paragraph. I'm going to read it because we've

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quoted where the sources for example.
All right, let me go back up

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with prograph. One method of helping
astronauts to avoid the radiation on Mars is

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active shielding. For example, superconducting
electromagnets could be used to create a powerful

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magnetic field to deflect the incoming charged
radiation particles away, just as the Earth's

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field does. That's the Lanele belt. The problem is that such solutions can

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demand a lot of power to run, and the technology is a long way

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from being fully developed. An easier
alternative is passive shielding, simply placing a

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thick bulk of shielding material between the
crew habitat and the sky. And then

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they go on to consider different materials. Aluminium aka aluminum, the metal that

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spacecraft are constructed from, is actually
a pretty bad radiation shield and they say,

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when hit by an energetic cosmic ray, is atoms can shatter and fly

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onwards to create even more radiation particles
and Martian soil the regulith which if you're

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on Mars, you might think about
digging a hole there. It's got the

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same problem, but it's actually abundant, and so you could use that to

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dig a pole. If you put
the two to three meter layer on top

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of your habitat, then you'll get
some protection. But the thing that surprised

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me Andrew is once again it comes
from this same article. Hydrogen is the

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best shielding material as it's light atoms. Yeah, it's light atoms, and

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by light I mean not heavy.
Its light atoms don't create as much secondary

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radiation, and so tanks of rocket
fuel or water which is rich in hydrogen,

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placed over crew quarters could double up
as effective radiation shields. I've heard

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that before that one way of protecting
your spacecraft as it flies to Mars is

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put it in a tank of water. It's the last thing you'd expect to

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do, but water is a good
childing material. And they also point out

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the alternative of hydrogen rich plastics like
polyethylene, could be used to cement regular

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grains together this is on Mars and
improve their shielding effect. So if you

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want to read more about this,
it's an article that originally appeared in the

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August twenty two issue of BBC Sky
at Night magazine and it covers pretty well

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amost the ideas that have been that
have been suggested for this radiation issue.

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It's one that's got to you know, it's going to find an answer soon

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because put all, Elon and his
starship is getting nearer to thinking about going

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to Mars. I don't think it's
ever going to happen, but that's uh,

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that's something he'll definitely be thinking about. Yes, indeed, he's too

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busy dealing with the Australian government at
the moment. Indeed, that's right,

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some of the content on Twitter that
the government wants to get rid of simply

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because of its volatility. But anyway, that's a different story. But there's

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plenty of water on Mars, so
maybe maybe creating those water barriers is probably

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the simplest thing to do. You've
already got the material there, if you've

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if you've landed in the right spot
where you've got whatever, that's the question.

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Yes, indeed, well done,
Fent, and you actually happened across

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some of the answers to in asking
your question. Uh, this is based

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out's Andrew and here with Professor Fred
Watson. Three four space nuts. Now

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Fred our next question comes from Robert. Hi, guys, love your show.

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Sorry for the long question, but
feel free to paraphrase or shorten it.

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Our moon is heavily created and has
given us a lot of insight into

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the history of the Solar System and
perhaps how the planet's formed. But what

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if we had a moon like the
icy moon Europa or the shrouded in Hayes

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Titan, both of which don't show
immediate evidence of cratering. Would our theory

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about how the planets developed would be
different? What other insights about our Solar

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System would be missing or would we
be missing? And lastly, would we

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have spent or would we have sent
people to land on such moons? I

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e? Would they be more dangerous
for astronauts? Cheers Robert in Vienna,

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Austria. Wow, I don't think
we've had a question from Vienna before,

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have we? Lovely to hear from
you, Robert. I think I think

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Robert might have been in touch once
before. It's here from Vienna. Yeah,

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I was in Vienna at the beginning
of last year and I think I

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think we got something around about the
same time. And I was at the

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u ND when I was the copyhoss
beating Anyway, that's another issue. What

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if we had Yeah, it's a
really interesting question. What would we not

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know about the Solar System if our
moon was basically one that had been resurfaced

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in recent years, Because that's what
makes us surface smooth. That's how we

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recognize the fact that the universe sorry
that the It's how we recognize the age

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of a surface is by how many
creators it's got the oldest, the older

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the surface, the more craters it
has. And so the moon's south southern

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region, which is heavily created,
as is the backside, tell us that

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early on in the Solar System's history
it was very wild and wily place,

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with things charging about all over and
causing these craters. Now, if we

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had a moon that was like Europa
that had you know, I see guysers

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on it, that basically covered up
the craters, would we have known about

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that? My guess is yes we
would, because we'd see other bodies within

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the Solar System, like you know, other moons, like places like Series,

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the biggest of the asteroids, the
dwarf planet that dominates the asteroid belt,

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that's heavily created. Parts of Pluto
are heavily created Mi Mas one of

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Saturn's moon. His moons is heavily
created too, so we'd know about it

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by looking at other objects, even
if our own moon was smoothly surfaced.

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It's but the Roberts last point on
this, would we have sent people to

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land on such a moon? I
think I don't know. That's a really

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good question. I mean, we
have sent people to land on our moon

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as it stands, with an ancient
surface. In fact, where they landed

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were more recent than the heavily created
surfaces, because there were, principally in

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the Maria the basalt planes. So
maybe that suggests that we would have landed

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people on Europa as well, because
I think we probably, Yeah, we

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probably would because it would have a
solid surface, there'd be places, because

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it would be so close to us, we'd be able to examine and find

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the right landing points. Might be
a bit more difficult with a moon that

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shrouded in gas. Yeah, yeah, that's right, and especially a place

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like Tyson. I still think we'd
have done it. Actually, I think,

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you know, the JFKs promised to
put past lots on the moon would

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have still held good even if it
had been a very different place. If

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it had been like EO. It
might have been a different story where you

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know you've got the most volcanically active
body in the entire Solar system with stuff

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going off all over the place.
I think we might have been a bit

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00:19:26.720 --> 00:19:33.079
more reluctant to land on EO.
Yes, possibly, so it would be

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interesting to have something different. But
then if we'd always if we'd always had

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an ice moon, we probably would
have caught a question from Robert asking if

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we had a rocky moon. Now
would interpretation of the formattage and planets if

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there was a rocky moon next us
instead of an im Yes, in an

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00:19:53.519 --> 00:19:57.000
alternative universe, Robert, you would
have flipped your question. But to hear

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from you, hope it all is
well in Austria. Our final question for

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this episode comes from Duncan. Hello, Duncan here from Weymouth in the UK.

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Again, of course just looking,
was just doing some reading and I

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noticed that Uranus and Neptune are often
referred to as ice giants. Now,

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given that ice is basically just sort
of like a rock form of water or

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CO two or whatever else, but
basically just the solid form of it,

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why are they not just called rock
giants? Why do we make the definition

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of ice rather than just calling them
rock It just seems odd because the little

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planets in the Inner Solar System are
referred to as rocky planets, So given

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that they're also apparently rocky, why
are they not called rocky giants? Okay,

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00:21:02.319 --> 00:21:07.519
thank you boy, thanks. Duncan
appreciate your questions as always. Yeah,

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00:21:07.519 --> 00:21:11.039
why do we call them ice giants
just for the sake of the exercise,

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00:21:11.279 --> 00:21:17.759
because there's gas giants and ice giants, Yeah, except one is a

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subset of the other. And so
all four of the outer planets Jupiter,

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00:21:22.839 --> 00:21:26.880
Saturn, Neptune, sorry, Uranus
and Neptune, they're all gas giants because

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00:21:26.920 --> 00:21:34.640
they have high mass, you know, much more in the case of Jupiter,

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00:21:34.720 --> 00:21:41.240
certainly than our own planet. They've
got the giants that big, they've

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00:21:41.240 --> 00:21:48.480
got high mass, and they don't
have a visible surface, which is why

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00:21:48.519 --> 00:21:52.640
they call gas giants, because all
we see is a gassy envelope. Just

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00:21:52.680 --> 00:21:57.160
to go to the last of Duncans
questions there, we wouldn't call the inner

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00:21:57.200 --> 00:22:02.759
planet's rocky giants because not giants.
They're kind of normal planet size. You

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00:22:02.799 --> 00:22:06.519
know. If you think of the
Earth as being your standard planet, then

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00:22:07.039 --> 00:22:12.680
Mercury Venus and Mars are similar in
size, all smaller venuses about the same

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00:22:12.720 --> 00:22:17.799
size, but Mercury and Mars,
of course are smaller. So it's only

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when you compare with the size of
Earth that you'd start talking about giants because

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00:22:22.160 --> 00:22:25.559
they are much much bigger than Earth. And so that's the gas giants.

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00:22:26.279 --> 00:22:33.400
So why are Urinous and Neptune called
ice giants? Horse They have hazes of

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00:22:33.640 --> 00:22:40.119
ice in their atmosphere. So,
and that's the trick. It's not a

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00:22:40.160 --> 00:22:44.640
solid surface, it's not rock.
It's a haze. It's kind of like

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00:22:44.720 --> 00:22:49.680
a dust of ice which permeates their
atmosphere, and it's water ice in fact,

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00:22:51.559 --> 00:22:56.559
mostly So that's why they called ice
giants, because unlike Saturn and Jupiter,

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00:22:57.200 --> 00:23:03.400
which don't have these hazes, the
outer the rocky rocky sorry, the

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00:23:03.440 --> 00:23:07.519
two outer planets Uranus and Neptune do
they have ice hazes in their atmosphere,

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00:23:07.559 --> 00:23:14.319
hence the name. Okay, because
the last episode we learned there wasn't much

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00:23:14.480 --> 00:23:19.880
water in Jupiter. That's right,
in the two outer I guess giants.

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00:23:21.119 --> 00:23:22.519
Yeah, it sounds like there is. Is that why they're a different color?

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00:23:23.440 --> 00:23:29.440
Yes, yes, I think that's
right there. And also their atmospheric

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00:23:29.480 --> 00:23:33.319
constituents are different. They don't have
the same belt structure that Saturn and Jupiter

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00:23:33.400 --> 00:23:37.960
do. It may be that that's
because any belts that exist are much lower

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00:23:38.000 --> 00:23:42.599
in the atmosphere and so you don't
see them. Yeah. I mean there's

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00:23:42.680 --> 00:23:53.799
there's a strong body of advocacy within
the space fraternity to get get more spacecraft

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00:23:55.039 --> 00:23:59.880
out to Uranus and Neptune, because
they're the two planets about which we know

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00:24:00.160 --> 00:24:06.000
least and it will be good to
know more. Yeah. Well, if

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00:24:06.000 --> 00:24:08.319
you sit down in snow for long
enough, your rainus turns into our ice.

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00:24:11.880 --> 00:24:17.240
I couldn't help it. Sorry,
Yeah, which is why we call

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00:24:17.279 --> 00:24:23.559
it Urinus. Yeah, it's just
a joke. You've got to tell you

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00:24:23.920 --> 00:24:30.240
to Yes, I blame Johannes Border, who is the person who chose the

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00:24:30.319 --> 00:24:37.319
name. It's fine in German.
Is nothing wrong than ruins, all the

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00:24:37.400 --> 00:24:41.880
jokes, all right. So,
yes, they're ice giants for a very

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00:24:41.880 --> 00:24:45.559
good reason, Duncan, because they've
got ice in them in the atmosphere.

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00:24:45.559 --> 00:24:49.599
But technically speaking, they are in
fact gas giants. But yes, differentiate

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00:24:49.640 --> 00:24:55.440
them because of their substantially different atmospheres. There you are, thanks Duncan.

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Great to hear from you. Great
to hear from everybody. Thanks for sending

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00:24:57.400 --> 00:25:00.519
in your questions. Don't forget.
You can see in questions via our website,

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00:25:00.519 --> 00:25:04.680
spacenuts podcast dot com, space nuts
dot io, and all you have

280
00:25:04.799 --> 00:25:08.000
to do is click on the various
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281
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button below, which, yes,
it's down there somewhere I don't know,

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one of those places. Fred has
always Thank you so much, pleasure and

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00:25:37.759 --> 00:25:41.559
you see you, Sue. Okay, Fred Wat's an astronomer at large.

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We'll catch him on the next episode
of Space Nuts. We might catch you

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00:25:45.559 --> 00:25:51.279
then as well, because not to
you today, didn't even call in sick.

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00:25:51.400 --> 00:25:53.960
I need a note and from me
Andrew dot Thanks very much for your

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00:25:53.960 --> 00:25:57.359
company. We'll see you again soon
on the next episode of Space Nuts.

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00:25:57.559 --> 00:26:06.599
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