July 13, 2023

#360: Collaboration vs. Competition: Advancing Space Exploration Together & Other Space Questions

#360: Collaboration vs. Competition: Advancing Space Exploration Together & Other Space Questions

Discover the unexpected twist that ignited our curiosity, the twist that pushed the boundaries of our understanding of the cosmos. Rusty from Donnybrook and Russ from Stylebridge brought forth questions that transformed our podcast into an...

Discover the unexpected twist that ignited our curiosity, the twist that pushed the boundaries of our understanding of the cosmos. Rusty from Donnybrook and Russ from Stylebridge brought forth questions that transformed our podcast into an intergalactic journey, delving into the mysteries of the Milky Way's metallicity profile and the mind-bending concept of our universe residing within a black hole. As we explored these audacious ideas, we found ourselves diving deeper into the enigma of space, forging a bond with our listeners who share our passion for astrobiology. But little did we know, these questions were just the beginning - a beginning that would unravel even more captivating mysteries. Stay tuned to uncover the next twist in this cosmic tale. In this episode, you will be able to: · Get the lowdown on how Metallicity is intertwined with the presence of complex life across our galaxy. · Journey through the awe-inspiring, enigmatic universe of black holes, detailing their size and properties. · Walk through the cosmic annals as you perceive past events due to the speed of light. · Examine the Big Bang, divulging the key contribution of population three stars during this pivotal cosmic event. · Get to grips with the perplexing concepts of Redshift, time dilation, and the paths of space objects. Time Travel in Astronomy: How the Universe Reveals Its Past I think he's actually right...I think he's on the right track, because whilst the formal definition of a black hole...is a point in space with infinite density...that suggests that if its density is infinite, that its dimensions are zero...But I'm thinking that physicists know that 'physics'...never works that way. You can't have something with no volume and no dimensions and yet still exert a gravitational force The resources mentioned in this episode are: · Check out the integrated metallicity profile of the Milky Way published in Nature Astronomy. · Learn more about the metallicity of stars and its importance in the search for life on other planets. · Explore the concept of living inside a giant black hole and the theories surrounding it. · Find out if the entire universe could be a quantum object and what that means for our understanding of reality. · Discover the different sizes of black holes, including supermassive and intermediate black holes. · Learn about the formal definition of a black hole and its dimensions. · Watch the video on YouTube for a visual explanation of black holes. · Consider the implications of black holes on our understanding of physics and the laws of the universe. · Dive deeper into the topic of black holes by reading scientific articles and books on the subject. · Stay tuned for future episodes of the show for more fascinating discussions and questions. The Size of Black Holes Alright, time for a real brain-boggler: Do black holes have a size? Now, this might sound like a straightforward question, but in reality, it's anything but. The nature and properties of black holes are one of the greatest mysteries of our universe. In technical terms, black holes are described as a "singularity," which implies zero dimensions. But could there be more to it than that? Black holes became an engaging topic when Andrew and Fred touched upon how their "size" led to several theories and ideas. Both agreed that the definition and understanding of black holes are fluid, leaving a lot of room for scientific debate. Fred even hinted at the possibility of revisiting the no hair theorem, which describes the limited number of detectable attributes of a black hole. So, despite the name, black holes are anything but an empty subject! Apogee and Earth's Climate Now, let's talk about something a touch closer to home - the Earth's climate. You might have heard the term "apeelian," which refers to when our blue planet is furthest from the Sun. It's a regular, annual occurrence, but does it have a significant effect on our climate? From a layman's perspective, it might seem like it should. But hold onto your hats - the reality is quite different! In engaging conversation with Andrew, Fred clarified a common misconception about the apogee and its impact on our climate. As it turns out, the difference in distance doesn't have much effect at all! The tilt of Earth's axis and seasonal changes have a lot more to do with our climate than our planet's solar proximity. It's one of those delightful bits of information that make you appreciate just how complex and finely balanced our planet's systems are. The Size of Black Holes Alright, time for a real brain-boggler: Do black holes have a size? Now, this might sound like a straightforward question, but in reality, it's anything but. The nature and properties of black holes are one of the greatest mysteries of our universe. In technical terms, black holes are described as a "singularity," which implies zero dimensions. But could there be more to it than that? Black holes became an engaging topic when Andrew and Fred touched upon how their "size" led to several theories and ideas. Both agreed that the definition and understanding of black holes are fluid, leaving a lot of room for scientific debate. Fred even hinted at the possibility of revisiting the no hair theorem, which describes the limited number of detectable attributes of a black hole. So, despite the name, black holes are anything but an empty subject! The key moments in this episode are:
00:00:00 - Introduction,
00:03:14 - Metallicity and Complex Life,
00:07:59 - Looking for Life in Other Galaxies,
00:10:13 - Apogee and Earth's Climate,
00:11:23 - Conclusion,
00:17:23 - The Size of Black Holes,
00:22:54 - Looking Back in Time,
00:26:06 - Light Travel Time,
00:27:18 - Paradigm Shift,
00:28:43 - Uncertainty in Early Universe Models,
00:34:12 - "Redshift and Energy Conservation",
00:37:11 - "Time Dilation and Atomic Frequencies",
00:41:40 - "Origin of Interstellar Objects",
00:44:30 - "Collaboration vs. Competition in Space Exploration",
00:45:18 - "The Changing Landscape of the Space Race",
00:52:27 - Introduction,
00:52:30 - Appreciation for Hugh,
00:52:44 - Conclusion,
00:52:50 - Farewell,
00:53:02 - Podcast Information,

 

 

WEBVTT

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Hi once again, and thank you
for joining us. This is Space Nuts.

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My name is Andrew Dunkley, your
host. It's great to have your

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company. And as this is the
three hundred and sixtieth episode, like we

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do every fifth episode, it is
dedicated one hundred percent to audience questions.

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We will be covering black holes,
strangely enough, exo planets, XO asteroids,

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time dilation, red shift, the
balance of power in the space race

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as it stands now and what we
think about that and metallicity all coming up

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on this episode of Space Nuts.
Channel nine. Magnian sequenced Space Nuts three

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two Space Nuts as an actual board
it deal good. Yes, And joining

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me to answer all questions known to
mankind is Professor Fred Watson, Astronomer at

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Large. Hello Fred, it might
be not just human kind, but it

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might be alien kind as well.
It could be Yeah, it's all sorts

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of possibilities, indeed, But yes, how have you beaten? Or not

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so bad? Thank you? My
nearest and dearest has got the most awful

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cold, so I expected them to
be soon. So yeah, who knows

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what I'll be what stays I'll be
in next time we speak? Yes,

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well, fingers crossed that you managed
to avoid it. My dad's got at

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the moment. Two was down Newcastle
Away to celebrate my brother's sixtieth birthday last

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week. So he co hosts with
Tim Gibbs Astronomy Daily. So yeah,

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we had a good time. It's
nice to catch up with family. And

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I played golf in the most brutal
wind known to mankind or humankind last Saturday.

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I don't know if it was windy
in Sydney. I imagine it was,

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but yeah it was. It was
O God, I should blow the

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dog off a chain. Then I
played. I played golf in at a

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lovely course called the Vintage in the
hunt of Valley. All right. Of

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course I've always wanted to play very
challenging, so yeah, why don't we

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make it harder and play in a
young forty killer a forty mile an hour

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wind. I think it was one
of your bulls that ended up in our

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boat. God a prosiably you're here. It was at Northwestly, so it

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could have gone your way. But
it was brutal out there, absolutely brutal.

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But I actually played quite well despite
the conditions. But very good,

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lovely, lovely part of the world. Wow, what a golf course,

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Gosh walked into the locker room and
thought, all g I don't belong here.

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This is way too out of my
league places too that I feel like.

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That's about Yeah, all right,
let's get down to business. We've

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got a bunch of questions from our
audience who stick with us regardless of what

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the reality is. But let's go
to one of our regulars, and that

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is Rusty from Donnie Brooks. Hey, guys, it's Rusty and donnybrook Well,

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here we are. We're appilion and
midwinter and we're having some of the

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coldest mornings I can remember. But
I hope you guys are keeping warm and

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you're keeping well. In June,
only twenty second of June this year,

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there was an integrated medalicity profile of
the Milky Way reashed in Nature Astronomy,

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and one of the findings was that
the peak medalicity in our own galaxy is

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it about twenty five thousand lachis from
the galactic center. It trails off again

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shortly after getting to our distance,
which is twenty six They quote twenty six

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thousand lachies to be very low,
about a third of the medalicity of our

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own son By the time we get
to the edge of the galaxy at fifty

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thousand nachies. So I'm thinking about
the Drake equation, and it would see

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that middle rich locality would be one
of the things that complex life like ours

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is indeed of. So it might
be a good place to start looking in

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other galaxies, not this particular distance, because I believe it changes from galaxy

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to galaxy. Anyway, what are
you thinking? Cheers, thanks for Rusty.

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Yeah, that's a good question.
And of course we are looking for

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signs of civil civilizations elsewhere. We're
looking close at a home for signs of

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life too. But yeah, I
suppose we have talked in the past about

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places that look more likely than others. Has Rusty got a point with the

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metallicity theory, Yeah, and indeed
it's well built into, you know,

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the interests of austrobiologists looking for signs
of life on other worlds. And so

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just to to you know, give
the backstory here, metallicity is it's a

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measure of the extent to which metals
are present in the atmosphere of a star,

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and by metals, astronomers mean everything
everything other than hydrogen and helium.

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Hydrogen helium metals everything else is.
So oxygen is, you know, carbon

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is. It's a different definition from
what chemists call metals. So a metal

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for an astronomer is pretty well anything
you like. But all of that,

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let's just keep it simple. Yeah, And in many ways there's a good

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reason for that, because hydrogen and
helium were formed in the Big Bang,

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so they are primordial. They've been
there since the beginning of the universe.

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But the other chemicals haven't. The
other elements. They've been formed in the

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atmospheres of stars through many, many
generations of stars in our universe, and

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so with each new generation the metallicity
is enhanced. You you generate more metals,

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i e. Things other than hydrogen
and helium, and when that star

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either explodes or you know, turns
into a planetary nebula or whatever at the

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end of its life, it essentially
enriches the interstellar medium, that's the very

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very very rarefied gas between the stars. It enriches that with higher metallicity compounds.

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So metallicity is a measure of how
much metal there is in a star's

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atmosphere, and normally you do it
and indeed this is exactly what's quoted in

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the paper that Rusty referred to.
You normally do it by looking at the

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ratio of iron to hydrogen the atmosphere
of a star. That's that's termed the

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metal licacy, and it's effectively zero
for it kind of calibrated to be zero

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for solar type star stars like the
Sun. So things that have got more

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iron in them than the Sun will
be said to be metal rich. Things

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that have less iron would be said
to be metal poor. And I think

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Rusty's reasoning is correct that it's probably
a consequence of the fact that we are

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we are a planet of a metal
rich star that gives the Earth all the

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different kind of chemical elements that we
need to form life, particularly carbon,

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oxygen, hydrogen, nitrogen in a
phosphorus, and those other things that living

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organisms seem to need. So you
would naturally look for metal rich stars if

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you are looking for planets that might
host life. And so, yeah,

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I think Rust's comments on the money, so in a sense it's you know,

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he's pointed out this Nature Astronomy paper, which indeed shows that the metallicity

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in our galaxy, among stars in
our galaxy, and the four hundred billion

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of themselves plenty to choose from but
that you can plot a curve that shows

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how that changes with distance from the
galactic center. This is exactly what rust

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is talking about, and it peaks
more or less at the solar radius where

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we are, and that's very useful
because they're the nearest stars to us,

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and those are the ones that are
easiest to look for extra planets or to

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look for biomarkers in their exoplanets.
We're only just starting to do this by

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analyzing the atmospheres of extra planets,
and the James Webb telescope has been success

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for at some level. With that
we've found you and I've talked about.

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I think sulfurd outside was the most
perhaps exotic compound that's been found by James

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web Space telescope in the atmosphere of
an exoplanet. So yeah, that's where

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we're looking. Rusty makes a comment
tub we'll be looking at the same radius

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in other galaxies, and I think
he's right that the metalistic gradient doesn't or

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the profile doesn't necessarily follow what we
have in our own Milky Way galaxy.

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But the problem with those stars in
other galaxies is they're very difficult to observe

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because they're a long way away we
can, and I think there is one

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example, might be two of an
extra galactic in other words, outside our

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own galaxy, exoplanet, in other
words, outside our own solar system.

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I think there was one picked up
in Andromeda, in the Andromeda galaxy.

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Okay, might be more than that, but it's certainly good news for our

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own galaxy. And very briefly,
Rusty mentioned Appelion at the beginning, which

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is the time which the Earth is
that it's most distant from the Sun.

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It coincides with I think it's the
third of July is usually when it is,

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if I remember rightly, But I
always used to feel when I lived

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in Scotland, where in January it's
freezing cold and pretty miserable, and yet

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we are nearest to the Sun on
the third of January, which tells you

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that the distance of the Earth from
the Sun doesn't actually make too much difference

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to the climate. It's all about
the tilt of the Earth's axis of the

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season. Well, I think I
read the other day that June was one

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was the hottest month on record.
Yes, that's for globally. Yeah,

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yeah, we were freezing here.
Well that's right, Yes, we we

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are in the upside down part of
the planet. So were things like that

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we do? Okay, thanks,
I see. I suppose the question would

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be is if we were going to
be looking for potential life region in Andromeda,

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we could analyze the stars there and
see where the peak point is.

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Yeah, I'm sure that's been done
because the stars in are well observed.

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I haven't got a reference to that
in my head, but it's an interesting

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thing to look for, so which, yeah, it would be. Yes,

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Okay, thanks Rusty. Good thinking
before we move to the next question.

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For those who are not TikTok users, we do a promo every week

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on TikTok before we record the show
proper, and we usually end up with

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a dad joke. Unfortunately, it's
starting to catch on. This comes from

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Misty West, who's one of our
regular listeners and contributors occasionally. Where do

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Bad Rainbows Go? Fred, He's
got a good run at solving these Yeah,

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yeah, I'm not sure I'm going
to get this. Will do or

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I'll put you out of your misery? Where do bad Rainbow Go? Prism

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It's wait for it. It's a
light sentence and gives them time to reflect.

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That's pretty good. I like that
very it's very good. Yeah,

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okay, let's move on to our
next question, which comes from Russ.

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Guess what it's about. No introduction
needed, No introduction, r H.

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Friend Andrew, It's russif from stale
Bridge. I love the show's always and

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I have another question about black holes, which I'm sure you're delighted to hear.

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It is related to our universe.
Apparently, according to scientific discoveries,

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if you took all the matter in
our universe and you compacted it down so

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it creates a black hole, the
advent horizon would be larger than the than

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our visible universe. All so there
is as we look out into space further

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and further, the space is expanding
quicker and quicker. We get to a

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pope where it's apparently exceeds the speed
of what the speed of light, which

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would mean that like could not escape. Does this mean that we are living

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inside us? Has been speculated a
giant black hole already? Why are your

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views on this? I'd love to
know? Thanks a lot. All right,

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Why, let's hope all the black
holes in the universe don't decide to

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have a convention soon. If that's
the case, yeah, it will be

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dark yeah, it will be very
duch. Look, I actually find that

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how to believe the event if you
combined all the matter in the universe into

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a black hole, maybe maybe it
would maybe the horizon would be comparable in

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size with the universe visible universe.
Yeah, yeah, that's right. Yes,

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that well, that's right. That's
the that's the tricky bit, because

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the universe may be infinite. That's
the really you know, that's the snag

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with all these discussions. But it's
been the idea of are we living in

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a black hole? Has really within
a black hole event horizon has been around

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for quite a long time. It
probably goes back to the likes of Roger

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Penrose back in the maybe in the
even in the nineties, eighties and nineties.

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So I've never I've never really um
got excited by this idea because I

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think it just adds a complication to
something that's already really complicated. And you

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know, in terms of that lie
being stopped because where the universe is expanding,

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it faster than the speed of light
and things of that, or yes,

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we do know that happens. I
don't think you need a black hole

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event horizon too to postulate that.
So I'm not. I'm not big on

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the idea of the universe being that
that we are within the event horizon,

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the set of massive objects. But
I who am I to complain if if

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people, you know, come to
the conclusion that that's the case. I

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saw an interesting headline in it was
a new scientist. Didn't read the article.

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I just saw the headline as it
went past, which was, it's

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the entire universe a quantum object.
I think that's what it was, something

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like that. So are we all
completely entangled with each other? Well?

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You can take that question on many
different levels. Yeah you can, and

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it just makes people's brains hurt,
particularly mine. That's about but not not

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likely that we're all, you know, in a I don't like. Look,

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yes, I'd like to sit down
and read some of the detailed discussions

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of this, which I have to
say I've never done. I've just thought,

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look, that's too hard. It
is bad enough to understand what's in

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the universe already without throwing throwing in
this idea. I'm not a cosmologist by

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training, although it worked a lot
with cosmologists because I've built instruments that provide

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them with the data they need and
indeed managed surveys that provide them with the

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data they need. But the stuff
that they do with them is quite mind

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blowing. I worked with a cosmologist
once because it was his nickname, because

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every time you asked him a question
or asked him to explain something, he'd

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say because that's a because modelogist a
cors models. Just because the ladyship should

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have saved that for the dad joke. Actually, you know the problem is

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because when we were record, we
go out live sometimes that they're coming in

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thick and fast. OVISTI is really
thrilled that she achieved her one an only

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chance to stump you, Fred to
be foot, I do like I like

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the prison will they do though it's
a good one. Okay from black holes

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too? Black holes? Hello Andrew, Fred and Chew in the studio.

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This is pictures here in Auckland,
New Zealand. Um. I'm going to

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bring up an old chess nut,
which then about black holes. Um,

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and it's something I just can't get
my head around. With black holes.

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I get the hole mass of a
black hole, like they can calculate the

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mass of a black hole by by
the gravitational influence of the surrounding space and

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the size of the event horizon and
all that kind of stuff. I get

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that, I think i'd get that. Well, I don't get is when

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they say, yea black holes got
no size. But how do they know

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it's got no size? They've already
established that the regular laws of physics stand

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apply when they come blake holes,
and nothing can escape from a black hole,

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not even lights, so nothing,
nothing can escape from their event horizon,

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so it's impossible to image anything from
within there. So how do they

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know there's actually got no size?
How dow the's not a it's not a

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ball in the middle of the gravity, well the size of a football or

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the size of a golf ball or
something like that. And you know,

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how do they know it's got no
size at all? That's basically my questian

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they and I hope I don't get
even more confused by the answer. But

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thank you very much, thank you, Petras. I think what you'll find

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in a black hole is an object, the shape of a pen as they've

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got to go somewhere. Could be
the shape of one sock as well.

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Yes, that's that's a thought,
that's a definite thought. Um. But

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when we talk about black holes.
We do actually assign sizes to them,

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super mess if black holes, intermediate
black holes, etc. So we do

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know that there are various sizes.
But I'm thinking he's talking about a different

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element of the black hole theory.
Well, yes, so Petrius mentions that

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that they come in different masses,
but it's the physical dimensions that's a this

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issue here, and I think I
think he's actually right. I think he's

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on the right track because whilst the
formal definition of a black hole, at

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least as I was taught, it
is a point in space with infinite density.

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That suggests that if it's if it's
density is infinite, that it's dimensions

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a zero because it's got mass masses
sorry, densities mass over volume. So

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if you have zero volume, doesn't
matter what the mass is, it's going

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to have infinite density. So that
formal definition. But I have read articles

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and papers which talk about black holes
actually having physical dimensions. In other words,

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their density is not quite infinity.
It's nearly infinity, but not quite.

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But they still show the properties of
black holes. And actually the other

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thing that plays into this is that
the black hole properties are varied. It

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in between For example, a rotating
black hole, which has quite different characteristics

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from a non rotating black hole.
And you can you don't need to look

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very far on the on the web
to find numerous accounts of these different things

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rotating black holes. I think they're
called K double R black holes. Should

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know all this, shouldn't I.
It's a long times for Tello done it.

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There was a point I was going
to make. Yeah, that's right.

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There is another aspect of black holes
which is called which I like very

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much. It's called a no hair
theorem. Beg gave a friend I wrote

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about in one of my books,
and I can't remember anything about it.

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No, the no hair theorem says
that there are only certain things that you

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can detect about a black hole,
and I can't remember what they are,

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like charge and you know, masks
and things of that sort. But no,

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I really need to to to revise
the no hair theorem. It will

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be very easy because I can't remember
which book it's in. I think it's

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in Cosmic Chronicles. I wrote about
the no hair theorem to simply because I

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quite like the idea. So what
was the answer to the question. I

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think the answers petris Is is right
that maybe some black holes do have physical

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dimensions because they're not quite fitting the
formal definitions. That's the thing that I

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would look for, and I probably
will or go and have a look for

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it, just to check whether I'm
talking complete rubbage. But I think I

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do recall reading about black holes which
are not infinitesimal in slides. In other

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words, just to type the loose
end here, they're not a singularity,

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because that's the point about point with
zero dimensions, it's a singularity. Is

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most of them are, but some
of them are maybe, or maybe maybe

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most of them are, but some
of them are. Yeah, it's a

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great question. All right, Thank
you Petris for your question. This is

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Spacens with andrewd Ankley and Professor Fred
Watson. Space puts. Okay, Fred,

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we might as well just keep on
churning through questions. The next one

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comes from Mikey. Hey, Fred, Hey, Andrew, this is Mikey

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from Illinois. I hope you guys
are doing well. And so here's my

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question. When we watch an exo
planet passing from another star, say five

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hundred light years away, are we
seeing that planet pass in front of its

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star five hundred years ago. I'm
assuming the answers, Yes, but this

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popped into my head this morning while
making today's coffee, and I just never

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considered it. Can't wait to hear
the answers. Guys, thank you so

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much. I absolutely love the show, and thanks for always giving me something

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to chee. It must be desperate
monkey, but anyway, I'll appreciate.

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I appreciate it. Uh. And
it's funny what pops into ahead when you're

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making coffee. I would suspect the
answers yes as well, Fred, because

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everything we see is historical. That's
correct, absolutely so. Yeah, the

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planet passing in front of its parent
star, that happened five hundred years ago

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and hopefully still happening now, but
we don't know. And because absolutely everything

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in the universe, no matter what
we observe, we're looking back in time,

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we tend to we there's you know, we tend to ignore the actual

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physicality of what's happening. The fact
that in our time frame now that planet

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is still going around its parents star, but we're only seeing it as it

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was five hundred years ago. That
has no relevance in astronomy. All we

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can learn about or make any reference
to, is what happened at the look

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back time. You know that you're
looking back five hundred years, so if

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it's a five hundred light year away
star, so yeah, that's that's the

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answer. Um, yeah, it's
it's hard to get your head around,

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but you know, you could be
looking at a star and it doesn't exist

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anymore because it's so far away.
It's it's you know, we're seeing it

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who knows how many thousands of years
later, possibly longer, and it might

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as well, you might well have
destroyed itself by the time we've seen it,

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but we're seeing it historically. Yes, that's right, and there's no

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way. So what I was trying
to say before, it's all about causality

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as well, because causing effect can
only take place at the speed of light,

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so there's no you know the fact
that's yes. For example, if

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that star five hundred light years away
detonated into a supernova, that radiation that

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would come from the supernover hasn't reached
the Earth yet, and so from our

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perspective, that star is still there. But eventually we would recognize that no,

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it's not still there because it's is
blown up. But it blew up,

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you know, however, many hundred
years ago it was, so it's

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it's a slight it is to particularly
people coming fresh to astronomy. It's slightly

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odd concept that we're always looking back
in time, but we are just one

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nuance to that though. If you've
got an extra planet going around a star

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that's five hundred light years away,
yes, when when the planets on the

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back side of the star or behind
the star, its distance is slightly more

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than it is when it's in front
of the star, and that's reflected in

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the light travel talent. So there
is a slight correction that you would need

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to make if you're and these corrections
are made where people observe these extra planets

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for the different light travel time from
when the star planets behind the starter when

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it's in front of the star.
In fact, it was that process,

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not with extra planets, but with
Jupiter moons that led strong work called Ruber

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in the sixteen seventies, I think
to work out what the speed of light

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was in Denmark. That's strong.
Thank go all right, thank you,

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Mikey. We will go from Mikey
to Michael. Hey, guys, this

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is Michael. I'm from Toronto,
Canada. It's my second question to the

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podcast. A feature of science is
that new breakthroughs can lead to major revisions

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of our previous last theories. We've
seen this time and again over a few

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millennia. Say where we've gone from
geocentrism to the now, the discovery of

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the cosmic web and everything in between. Could we be at such a turning

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point now thanks to observations from JWST, having ostensibly found galaxies that are too

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mature to be explained by the Big
Bang. What if rather than the Big

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Bang, we had massive supernova population
three stars, which are hypothetical and I

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don't think they'd been the third yet. Could this have given us the same

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evidence that we instead credit the Big
Bang? Wid Maybe we're engaging in underdetermination

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of theory by data or is there
could there be evidence that these galaxies were

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observing from far back our galaxies galaxies
of population three stars themselves, But because

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we don't know enough about the way
these these stars evolved, it's thrown off

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our models or what the early universe
and early galaxies looked like in an earlier

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epoch. Thanks guys, Wow,
Marcolet is deep. That's so deep,

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Like you know, I don't think
lot's penetrating well. I think Michael's questions

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are great, Well, it is
so. Yes, the Gimes Webb telescope

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has shown as galaxies that are more
evolved than we would it would expect for

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their age, for the age of
the universe as we see it at that

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time. But that doesn't mean that
we've got the basic paradigm of the Big

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Bang ron because it's supported by so
many other, you know, observations like

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the cosmic microad background radiation, the
whole the whole deal suggests that we are

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on the right track with the Big
Bang. There are some nuances. We

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get two different values for the for
the current expansion of the universe. It's

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what's called a cosmological tension because when
you look at the expansion of the universe

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measure as measured today and as measured
as measured from galaxies around us today compared

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with what it's what you get by
measuring the cosmic microwave background radiation the flash

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of the Big Bang. You get
two different answers this, but it's like

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five percent different. So that's that's
something that when I started work in astronomy,

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people would have would have been delighted
to get an error of five percent

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because the errors were more like one
hundred percent back in those days. Anyway,

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I think. I think, however, Michael makes a very good point

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with the idea that possibly we are
underestimating things like the influence of population three

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stars, about which we don't know
what are their Population three stars are the

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first stars to form in the universe, where all they had was hydrogen and

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helium. None of these metals that
we were talking about a few minutes ago

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had come into existence. So they
were the first, the first generation of

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stars, and you know, it
may be that their influence on galaxy evolution

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is something that needs revised. I
don't think we're going to push back the

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date of the Big Bang any further. I think that's pretty well understood thirty

351
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point eight billion years ago. But
our the studying of the earliest galaxies,

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the first galaxies to come into being, is based on therrestical ideas that we

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may well be changing because of new
observation. So I think Michael Lake's a

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00:31:11.279 --> 00:31:18.799
good point. He does whatever he
said. Yeah, Um, I love

355
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the way people really think about some
of the some of the mysteries and things

356
00:31:22.480 --> 00:31:30.039
that we're trying to unravel in astronomy
and space science, including a question without

357
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notices come in due to our live
casting of the recording session. Here it

358
00:31:37.880 --> 00:31:42.519
is. It's from a meal has
a question about how fluids work in the

359
00:31:42.599 --> 00:31:47.279
human body in space, like stomach
fluids and blood and all that sort of

360
00:31:47.279 --> 00:31:52.119
stuff. What happens in zero G
with with all your bodily fluids. Certainly

361
00:31:52.119 --> 00:31:56.359
know what happens in one G and
I don't like it. Yeah, they

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00:31:56.400 --> 00:32:00.279
do, that's right. Well,
if you know, this is the m

363
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one of the the key pillars of
space medicine. I guess one of the

364
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things that really people had to struggle
with when humans were first going into space.

365
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So hard does the hard does all
the work? You don't have gravity

366
00:32:16.039 --> 00:32:22.359
to help you, and that means
that you need to keep your cardiovascular system

367
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in really good nick, And that's
why they all do a couple of hours

368
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on a treadmill every day or on
a bike or whatever when they're got long

369
00:32:30.240 --> 00:32:35.680
periods in orbit. So I think
it's pretty well understood from a medical perspective,

370
00:32:35.799 --> 00:32:39.440
just how how these fluids keep on
going around? You do want?

371
00:32:39.640 --> 00:32:46.799
You know? There are aspects I
guess that well, you know, like

372
00:32:46.960 --> 00:32:52.440
the way our digestive processes work.
They tend to need help from gravity because

373
00:32:52.440 --> 00:33:00.119
everything's going downhill. But when you
think of many animals, who's who's our

374
00:33:00.200 --> 00:33:06.079
just processes are taking place horizontally,
well it still works, and so that

375
00:33:06.400 --> 00:33:08.960
would suggest that gravity is not playing
that important to role on that. But

376
00:33:09.160 --> 00:33:14.240
as I said, yes, well
understood. Yeah, the fluid in the

377
00:33:14.319 --> 00:33:17.640
eyes is one of the yes areas. Yeah right, that's right, yes,

378
00:33:17.839 --> 00:33:23.240
with I pressure and things of that
sort. Good stuff. Yeah,

379
00:33:23.279 --> 00:33:29.519
good question. All right. Another
one, this comes from Josh Hey,

380
00:33:29.599 --> 00:33:34.720
Andrew and Fred. My name's josh
from Sydney. I'm a longtime listener,

381
00:33:35.000 --> 00:33:39.000
first time question ask her. I
absolutely loved the show. Thank you both

382
00:33:39.359 --> 00:33:45.759
so much for producing it putting it
online. So my question is about the

383
00:33:45.839 --> 00:33:53.160
consolation of energy and the red shifting
of photons. So so when we look

384
00:33:53.160 --> 00:34:02.440
at the cosmic microwave background radiation as
the universe is expanding, those photons are

385
00:34:02.480 --> 00:34:08.840
getting red shifted, but that also
means that they're losing energy. So so

386
00:34:08.960 --> 00:34:15.000
where does that lost energy go because
it has to be concerted, right,

387
00:34:16.599 --> 00:34:22.679
Okay, thank you, Joshua.
Redshift is starting to become a popular area

388
00:34:22.800 --> 00:34:28.199
of inquiry. I'm finding we've getting
We've been getting a few questions about it

389
00:34:28.280 --> 00:34:34.199
lately, and it's the you know, probably the pillar of our understanding of

390
00:34:34.239 --> 00:34:38.639
the wider universe is redshift as well, very important. So Josh is absolutely

391
00:34:38.719 --> 00:34:46.119
right that a redshift represents a loss
of energy. Now I followed up on

392
00:34:46.199 --> 00:34:51.239
this once, possibly because of an
earlier question, or it may have been

393
00:34:51.280 --> 00:34:53.960
a question on the radio show.
I did follow up on that, and

394
00:34:54.000 --> 00:35:07.639
I think the answer is now it's
worse than forty two that the it contributes

395
00:35:07.719 --> 00:35:13.519
to the overall energy of the universe
itself, if I remember rightly reading on

396
00:35:13.599 --> 00:35:20.880
this, Because because Josh is right, energy is conserved, photons are losing

397
00:35:21.000 --> 00:35:28.719
energy, and I think, I
mean, it's tempting to say, well,

398
00:35:28.719 --> 00:35:32.119
it contributes to the expansion energy of
the universe, but that's a sort

399
00:35:32.119 --> 00:35:37.159
of circular argument and I don't think
it can be that, but I will

400
00:35:37.239 --> 00:35:40.639
check on it again. I do
remember exploring this idea in some depth,

401
00:35:40.719 --> 00:35:45.360
but it was so long as forgotten
the details. So it does go somewhere,

402
00:35:45.400 --> 00:35:49.000
that's the bottom line. It doesn't
go somewhere. It probably goes into

403
00:35:49.039 --> 00:35:52.800
that cup of coffee that was it. I can't remember who was making it,

404
00:35:53.159 --> 00:35:58.079
and one of our I think it
was Mikey. Mikey, that's right,

405
00:35:58.159 --> 00:36:04.159
Mikey's cup of coffee. So yes, but but you, But Josh

406
00:36:04.199 --> 00:36:08.519
is absolutely right that that red shifting
is a loss of energy from the light

407
00:36:08.679 --> 00:36:14.079
or it's changed the energy of the
light and it does go somewhere, Okay,

408
00:36:14.239 --> 00:36:16.920
warms up the universe. That could
be the bottom line. Once again,

409
00:36:17.000 --> 00:36:22.239
we demonstrate our pros for giving you
adequate answers. I don't think that's

410
00:36:22.320 --> 00:36:28.000
anything like adequate. I'm embarrassed to
be here. I think most most of

411
00:36:28.000 --> 00:36:30.519
our listeners know more than we do. Yes, and then they ask us

412
00:36:30.599 --> 00:36:36.320
questions about it. I think that
that might be the whole thing. You

413
00:36:36.360 --> 00:36:39.400
know, he is a conspiracy theory
that the whole reason why space Nuts is

414
00:36:39.440 --> 00:36:46.119
there is to make our listeners feel
more intelligent, feel more intelligent because they

415
00:36:46.159 --> 00:36:52.119
are. Yeah, it's working all
right, Thanks Josh. This is space

416
00:36:52.239 --> 00:37:04.360
Nuts sort of with Andrew Dankley and
Professor Fred Watson space Nets Like I will

417
00:37:04.360 --> 00:37:07.000
cram a few more questions in before
we wrap it up. The next one

418
00:37:07.079 --> 00:37:15.760
comes from DJI. This is DJ
from Indianapolis, Indiana in the United States.

419
00:37:16.159 --> 00:37:22.519
My question is about time dilation.
I've heard it said that one way

420
00:37:22.559 --> 00:37:28.079
that you would be able to see
the dilation would be spaceship is traveling past

421
00:37:28.199 --> 00:37:30.880
Earth, and you can see into
it like through a window, and you

422
00:37:30.880 --> 00:37:34.679
would see that clock and the spaceship
they're traveling close to the speed of light.

423
00:37:34.920 --> 00:37:39.400
You would actually see it ticks slowly
in yours. Since our second is

424
00:37:39.480 --> 00:37:44.960
no longer determined by the speed of
the Earth but by the ssium adam electron

425
00:37:45.039 --> 00:37:49.400
spin, does that change as well? So if you're in the spaceship going

426
00:37:49.440 --> 00:37:58.880
the speed of light and that sasium
adam electron spin is nine billion whatever times

427
00:37:58.880 --> 00:38:08.280
a second, does it now been
four billion times a second or two billion

428
00:38:08.320 --> 00:38:15.119
times a second if you're going close
to the speed of light or does it

429
00:38:15.639 --> 00:38:24.679
not know the difference? Hopefully that
was clear enough to get him answered.

430
00:38:25.880 --> 00:38:30.360
I really enjoy the show. Thanks
guys, and welcome to our world.

431
00:38:30.440 --> 00:38:37.679
DJA. It is so Yeah,
you might want to explain what he means

432
00:38:37.719 --> 00:38:40.880
by the way, we've changed the
definition of a second. Yeah, so

433
00:38:42.119 --> 00:38:51.760
a seconds defined in atomic atomic frequencies. It's it's gone from you know.

434
00:38:51.800 --> 00:38:54.039
You know, we've known for many
years and the Earth is a pretty poor

435
00:38:54.079 --> 00:39:00.440
time keeper in terms of its rotation
because the rotation changes. So if you're

436
00:39:00.440 --> 00:39:04.760
going to define a second as being
one three thousand, six hundreds of an

437
00:39:04.760 --> 00:39:07.119
hour and an hour as one twenty
fourth of our evolution of the Earth,

438
00:39:07.840 --> 00:39:14.320
then it's it's going to change over
time. So it's been defined in terms

439
00:39:14.400 --> 00:39:20.920
of I'm not sure whether it's still
defined in terms of vibrations of a caesium

440
00:39:20.920 --> 00:39:25.480
atom, but it certainly used to
be. But that here's the thing though,

441
00:39:27.159 --> 00:39:34.239
in terms of the relativistic time dilation, that as far as the caesium

442
00:39:34.280 --> 00:39:37.840
clock in your in the spacecraft is
concerned, it's still vibrating at the same

443
00:39:37.920 --> 00:39:46.039
rate. It's that an observer who's
in a different reference frame sees it basically

444
00:39:46.119 --> 00:39:52.400
vibrating slower. And that's how it
would look if you could see the vibrations

445
00:39:52.400 --> 00:39:57.320
of a caesium atom in a passing
spacecraft, they would look to be slower

446
00:39:57.360 --> 00:40:04.239
because because time is taking place more
slowly apparently, But for the for the

447
00:40:04.239 --> 00:40:07.039
people in the spacecraft, it's still
the sagothic change. We talked about this

448
00:40:07.159 --> 00:40:13.159
last week with someone questioning the gravitational
effect of a black hole with people on

449
00:40:13.199 --> 00:40:15.400
a planet. In the movie Into
Stellar, how they portrayed data seven you

450
00:40:15.440 --> 00:40:20.559
know, seven years pass for every
hour, which was an extreme example.

451
00:40:20.840 --> 00:40:27.280
But also you know, if we
were in a different place in the galaxy

452
00:40:27.920 --> 00:40:30.960
and we could observe people in another
part of the galaxy, they would either

453
00:40:31.000 --> 00:40:36.320
look like they're moving faster like an
ant hill or slower, depending on which

454
00:40:36.320 --> 00:40:39.840
part of the galaxy you were in
and the time dilation effect. Yeah,

455
00:40:40.039 --> 00:40:45.519
right, if you could absorb,
observe, Yeah, if you're if you're

456
00:40:45.519 --> 00:40:50.400
in a you're this is we're now
talking about gravitational time dilation, yes,

457
00:40:51.280 --> 00:40:55.360
rather than the velocity time dilation,
which is what DJ was. Look the

458
00:40:55.400 --> 00:41:00.880
two fates. I always got those
two mixed up. Wells, shame on

459
00:41:00.920 --> 00:41:09.840
you, Andrew. So so yeah, the issue is that it's it's always

460
00:41:09.920 --> 00:41:14.639
about reference frames. It's about how
you see, you know, how you

461
00:41:14.800 --> 00:41:20.719
a world reference frame sees somebody else
and other things going on in a different

462
00:41:20.719 --> 00:41:23.840
reference frame. So that yes,
if you were at a different point in

463
00:41:23.880 --> 00:41:29.159
the gravitational well you would you would
see talent progressing at the different speed,

464
00:41:29.239 --> 00:41:31.599
and it would depend on where you
were in the gravitational well as whether that

465
00:41:31.679 --> 00:41:35.719
was faster or slower. Exactly as
you've said, perfect, All right,

466
00:41:35.800 --> 00:41:40.239
thanks JJ. The next question comes
from Colin. Hi. This is Carlin

467
00:41:40.639 --> 00:41:50.400
from Aballene, Texas. And in
your last episode you had the researchers say

468
00:41:50.800 --> 00:41:58.320
they calculated the trajectory of the comment
or asteroid that was outside our solar system.

469
00:41:58.960 --> 00:42:04.599
But couldn't it just as easily come
shrug the orc cloud because it surrounds

470
00:42:04.679 --> 00:42:12.719
us here. Thank you, Thank
you, Colin, We do too,

471
00:42:13.079 --> 00:42:17.400
Thanks Colin. Um. I think
we can dismiss the aort cloud theory because

472
00:42:17.440 --> 00:42:22.960
of the speed of these particular things. See, you don't leave me,

473
00:42:22.159 --> 00:42:25.159
you don't need me, and you
don't I'm just remembering what you taught me,

474
00:42:25.199 --> 00:42:32.159
Fred. Yeah, that's right.
So um Or cloud comets come in

475
00:42:32.760 --> 00:42:38.400
at certain velocities. I can't remember
what the maximum is for a cloud commet,

476
00:42:39.400 --> 00:42:46.000
but I've read wait for it you
you ought to know? Oh well

477
00:42:46.039 --> 00:42:50.239
that was a good one. Yeah, that's so good one. I like

478
00:42:50.360 --> 00:42:55.079
that one. You ought to take
notice of the blocked cloud. Yes,

479
00:42:55.840 --> 00:43:02.199
anyway, Yeah, Orts was a
very very competent astronomer who did a fantastic

480
00:43:02.239 --> 00:43:08.320
amount of interesting science in the early
post war years. Perst second, anyway,

481
00:43:09.039 --> 00:43:15.480
that's all about so work. Cloud
comets coming from the old cloud at

482
00:43:15.599 --> 00:43:22.239
velocity x, but something interstellar would
come in at two x or x plus

483
00:43:22.320 --> 00:43:24.920
fifty kilometers per second or something like
that. They're they're much faster, So

484
00:43:24.960 --> 00:43:31.639
that that's the that's a critical difference
between you know, an exo asteroid perhaps,

485
00:43:31.920 --> 00:43:37.719
or or or a comet asteroid of
body that's come out from the old

486
00:43:37.760 --> 00:43:43.440
cloud. So it's all about it's
a matter of degree. Yeah, if

487
00:43:43.480 --> 00:43:47.920
if an exo asteroid just happened to
impact something in the or cloud and send

488
00:43:47.920 --> 00:43:53.239
it hurdling our way, you'd still
know the difference, wouldn't you. Yeah,

489
00:43:53.480 --> 00:43:59.880
you, um, you probably would
actually because you know, I mean

490
00:44:00.199 --> 00:44:02.480
this is along the lines of the
theory of that object that we're talking about

491
00:44:02.840 --> 00:44:07.039
last week, that it may have
been disturbed by Planet Night, had they

492
00:44:07.079 --> 00:44:12.760
gravitational tugged by Planet Night. Yeah, but it's still coming in at an

493
00:44:12.840 --> 00:44:17.480
excess velocity. That's correct. All
right, very good, Thank you,

494
00:44:17.519 --> 00:44:22.599
Colin. Lovely to hear from you. And we've got our final question for

495
00:44:22.639 --> 00:44:30.239
this week from Andreas. Hi Andreas
from Sweden here and thanks for a great

496
00:44:30.599 --> 00:44:35.320
podcast. So I have a question
I would like to get your input on

497
00:44:36.119 --> 00:44:37.159
as you can, as we can, all field, the world is kind

498
00:44:37.159 --> 00:44:43.320
of moving in our direction having two
major bay power blocks, Like on the

499
00:44:43.360 --> 00:44:45.639
one side we have the US and
Europe and on the other side we have

500
00:44:45.760 --> 00:44:50.199
China Russia. So which kind of
breaks back the feeling of the old space

501
00:44:50.320 --> 00:44:55.840
range in the US and sub which
propels things forward and about. But if

502
00:44:55.840 --> 00:45:00.519
we look from the perspective of humanity, do you believe having these two competing

503
00:45:00.519 --> 00:45:05.800
blocks, it's better? And if
we all came together, it's like one

504
00:45:05.920 --> 00:45:09.880
happy space family reaching the stars together. So what do you think is better

505
00:45:09.920 --> 00:45:16.760
for a scientific progress and expiration?
Is it collaboration or competition? Altima,

506
00:45:17.719 --> 00:45:22.079
great question, Andrea so well.
As a matter of fact, he's forgotten

507
00:45:22.079 --> 00:45:27.000
North Korea. I just finished watching
season three for All Mankind and they were

508
00:45:27.000 --> 00:45:31.800
the first to step on Mars.
Oh okay, so I hope that wasn't

509
00:45:31.800 --> 00:45:36.920
a spoiler for anybody. Good growth. Sorry, block here is too late.

510
00:45:37.199 --> 00:45:39.639
Yeah, the space race has changed. It used to be the US

511
00:45:39.800 --> 00:45:45.000
and Russia and or the Soviet Union, and now it's the USA, Europe

512
00:45:46.159 --> 00:45:52.159
and Russia and China. Although they
do tend to work independently, they do

513
00:45:52.239 --> 00:45:57.639
collaborate. But what we are seeing
is that we've got collaboration from just about

514
00:45:57.639 --> 00:46:00.039
all on Sundry, maybe to a
lesser degree each China, but they're not

515
00:46:00.159 --> 00:46:06.920
completely blocking everybody out, and one
would hope, and we do see this

516
00:46:07.000 --> 00:46:09.519
a lot in astronomy and space science, is that they do share data,

517
00:46:09.559 --> 00:46:15.760
they do share information, they do
share resources, they work together. So

518
00:46:15.920 --> 00:46:20.440
I from my perspective, I think
it's good the way things are going at

519
00:46:20.480 --> 00:46:24.639
the moment. What worries me is
that someone will get somewhere or find something

520
00:46:24.679 --> 00:46:29.039
and say, well, we we're
not going to share that. We're going

521
00:46:29.079 --> 00:46:31.639
to mind the hell out of it
and keep it for ourselves. Um.

522
00:46:32.320 --> 00:46:39.280
I don't know, it's it's a
I'd rather be a cooperative venture than one

523
00:46:39.320 --> 00:46:44.480
of conflict, although conflict has also
proven to be the mother of invention in

524
00:46:44.639 --> 00:46:49.119
history, in the history of humanity. So cut oath ways, as far

525
00:46:49.159 --> 00:46:52.079
as I think that's andreasis points,
isn't it that soon? You know,

526
00:46:52.159 --> 00:47:02.760
we we gained enormously in the nineteen
sixties by that geopolitical competition between the Soviet

527
00:47:04.000 --> 00:47:09.280
Yes and the Western Bloc, in
particular between Soviet Union and NASA SOU.

528
00:47:13.000 --> 00:47:21.199
But I do think, you know, you've got to kind of bring together.

529
00:47:22.199 --> 00:47:25.800
There are a number of ways of
looking at this, maybe space can

530
00:47:27.320 --> 00:47:32.639
be a beneficial thing in terms of
international relations rather than in terms of technological

531
00:47:32.679 --> 00:47:38.280
development. So you're still seeing,
i suppose, the last vestiges of that

532
00:47:38.320 --> 00:47:45.559
with the International Space Station, which
still has Russian and American astronauts and cosmonauts

533
00:47:45.760 --> 00:47:55.119
basically collaborating in a fantastic way.
And so space diplomacy I think still has

534
00:47:55.119 --> 00:48:05.679
a place in the the world's future, and I've often wondered whether, yes,

535
00:48:05.760 --> 00:48:10.679
there's there's certainly competition at the moment, and a lot of that is

536
00:48:10.679 --> 00:48:14.360
is to do with the rise of
China, the fact that you have a

537
00:48:14.440 --> 00:48:17.639
nation here that wants to assert itself
as a as a world player on a

538
00:48:17.679 --> 00:48:22.599
world stage, with a different political
system from what the Western world has,

539
00:48:23.519 --> 00:48:30.519
and that's that is perhaps one of
the reasons why we're seeing such really capable

540
00:48:30.760 --> 00:48:40.840
and quite notable achievements from the China
China National Space Agency Administration SAM. I

541
00:48:40.960 --> 00:48:50.159
think perhaps looking further into the future, when we're talking about flights to Mars

542
00:48:50.960 --> 00:48:57.000
human exploration of Mars, I suspect
that will turn out to be so expensive

543
00:48:58.679 --> 00:49:05.159
that the only way we'll really make
it work effectively would be to have international

544
00:49:05.239 --> 00:49:08.599
cooperation, and it may well be
that we might see a new era of

545
00:49:09.840 --> 00:49:16.840
warm and fuzzy international corporation, perhaps
comparable with what we saw around the time

546
00:49:16.840 --> 00:49:21.480
of the end of the Cold War. When that would say, though,

547
00:49:21.519 --> 00:49:27.840
the war in Ukraine did lead to
space tensions between the US and Russia,

548
00:49:28.679 --> 00:49:31.800
but it was something that was happening
on Earth that caused that. Yeah,

549
00:49:31.840 --> 00:49:36.599
and I'm pretty sure the people that
were in space at the time really didn't

550
00:49:36.639 --> 00:49:39.559
want to have a bar of it, but they were following orders. Yes,

551
00:49:39.639 --> 00:49:45.960
that's right. I can't rememb whether
or mentioned that when I was at

552
00:49:45.000 --> 00:49:51.400
the Committee on the Peaceful Uses of
Outer Space that meeting in February, that

553
00:49:51.480 --> 00:49:55.159
those geopolitical tensions were very, very
evident in some of the comments that were

554
00:49:55.199 --> 00:50:01.159
being made by delegates of certain nations, and it was all about the war

555
00:50:01.239 --> 00:50:07.000
in Ukraine. So there is so
when you've got something like that going on,

556
00:50:07.039 --> 00:50:15.320
then it really clouds the issue.
But all credit to astronauts cosmonauts for

557
00:50:15.559 --> 00:50:20.880
sticking together up there in the International
Space Station and to their respective space agencies

558
00:50:20.920 --> 00:50:30.360
for actually negotiating diplomatically. Ross Cosmos
had a Buyer brand head who has now

559
00:50:30.400 --> 00:50:36.599
been removed. He's now in Ukraine. Actually this Dimitri R. Godson was

560
00:50:36.639 --> 00:50:38.119
that his name? Yeah, that
sounds about right. Yeah, yeah,

561
00:50:38.639 --> 00:50:46.199
he's so. And we've had far
kind of fewer belligerent signals from ros Cosmos

562
00:50:47.039 --> 00:50:52.000
since then, although you know,
the internal politics might be the saying,

563
00:50:52.119 --> 00:50:57.360
but we've got you know, still
in the space station itself. It is

564
00:50:57.559 --> 00:51:01.400
business as usual, which is quite
a quite extraordinary, quite extra it is.

565
00:51:01.480 --> 00:51:09.079
It is, it seems in terms
of space exploration and even being close

566
00:51:09.159 --> 00:51:14.880
to home orbiting in the International Space
Station, they tend to leave the politics

567
00:51:14.880 --> 00:51:19.639
to the politicians and up there,
away from it all, it's a it's

568
00:51:19.639 --> 00:51:23.199
a different world and they all get
along most famously much of the time,

569
00:51:23.440 --> 00:51:28.480
as far as we're aware. And
yeah, and I hope it stays that

570
00:51:28.559 --> 00:51:34.119
way. And yeah, I hope
you're right about the future of exploration to

571
00:51:34.239 --> 00:51:38.840
Mars. Maybe maybe it will require
international cooperation and to make it, to

572
00:51:38.920 --> 00:51:42.760
make it happen, bring everybody together. I think that would be a great

573
00:51:42.800 --> 00:51:47.559
thing. Thank you so much.
Andrea's a fantastic question. We don't usually

574
00:51:47.559 --> 00:51:53.079
get into politics, but that was
that was a good one. That brings

575
00:51:53.159 --> 00:51:54.719
us to the end of the show. Of course, if you do have

576
00:51:54.840 --> 00:51:59.320
questions for us, you can send
them through our website. The AMA table

577
00:51:59.400 --> 00:52:01.440
or the send us you or Voice
message tab is the way to go.

578
00:52:01.960 --> 00:52:06.440
You can send us text questions as
well. Don't forget to tell us who

579
00:52:06.440 --> 00:52:09.000
you are and where you're from,
and peruse the Space Nuts shop while you're

580
00:52:09.039 --> 00:52:14.199
there. There's nothing worth buying,
but do you do it anyway. Thank

581
00:52:14.239 --> 00:52:16.280
you. As always, Fred has
been a great pleasure. Great to spend

582
00:52:16.320 --> 00:52:22.119
some time helping people understand space and
everything, and although half the time they

583
00:52:22.159 --> 00:52:27.760
help us understand a bit more too, so good Thank you, Fred,

584
00:52:28.440 --> 00:52:31.719
pleasure I was always Andrew look forward
to speaking next week. We will.

585
00:52:31.800 --> 00:52:37.599
And thanks to Hugh in the studio
for sending messages through from our live audience

586
00:52:37.639 --> 00:52:40.320
when we while we were according today, oh my gosh, I said something

587
00:52:40.400 --> 00:52:44.480
nice about Hugh that won't happen again. And from me Andrew, don't clear

588
00:52:44.519 --> 00:52:46.239
you. Thanks for your company on
this edition of Space Nuts. Catch you

589
00:52:46.280 --> 00:52:52.280
on the next episode. Bye bye. You'll be listening to this Space Nuts

590
00:52:52.320 --> 00:53:00.360
podcast available at Apple Podcasts, Google
Podcasts, Spotify, iHeart Radio, or

591
00:53:00.440 --> 00:53:05.079
your favorite podcast player. You can
also stream on demand at bites dot com.

592
00:53:05.480 --> 00:53:09.480
This has been another quality podcast production
from sites dot com,

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