Probing the Dark Unknowns: Seeking Clarity on Dark Matter and Energy | #385
In a serendipitous moment, Andrew Dunkley's passion for astronomy was sparked by a chance encounter with a telescope at a friend's house. Little did he know that a simple gaze through the lens would ignite a lifelong curiosity for the mysteries of the...
In a serendipitous moment, Andrew Dunkley's passion for astronomy was sparked by a chance encounter with a telescope at a friend's house. Little did he know that a simple gaze through the lens would ignite a lifelong curiosity for the mysteries of the universe. As he delved into books, documentaries, and conversations with fellow enthusiasts, his thirst for cosmic knowledge only grew stronger. What cosmic wonders await those who seek to understand the stars and galaxies?
In this episode, you will be able to:
· Explore the fascinating world of galaxies' rotation curves and their intriguing variations. · Discover the hidden secrets of spiral arms visibility through the lens of infrared observations. · Understand how gravity bends space and its profound implications on the universe.
· Uncover the crucial distinctions between dark matter and dark energy, unraveling cosmic mysteries.
"You can do anything in science fiction.' - Andrew Dunkley
Bending of Space due to Gravity
Gravitational influence on the bending of space is a central concept in Einstein's theory of relativity. It proposes that the force of gravity resulting from an object's mass distorts space around it. This remarkable insight about the interplay between gravity and spacetime allows us to understand extraordinary phenomena, such as the distortion of star positions during an eclipse. This theory immensely enriches our understanding of the universe and shapes our perception of space and time.
The resources mentioned in this episode are:
· Visit spacenutspodcast.com to send in your own audio or text questions for the show.
· Check out the AMA link on the website to submit your questions for the next episode. ·
Click on the tab on the right-hand side of the homepage to send in your audio questions. · Listen to the Space Nuts podcast on Apple Podcasts, Google Podcasts, Spotify, iHeartRadio, or your favorite podcast player. ·
Stream on demand at bitesz.com to catch up on previous episodes. ·
The key moments in this episode are:
00:00:00 - Thank you and break announcement
00:02:22 - Q&A Episode Introduction
00:08:01 - Understanding Gravity
00:11:14 - Theoretical Walk on a Neutron Star
00:16:46 - Clarification on Biochemical Processes
00:17:25 - RNA as the precursor to DNA and proteins
00:18:57 - Dark energy and dark matter web
00:22:17 - Universe's expansion and the role of dark energy
00:25:03 - White holes and dark matter
00:29:13 - Period of inflation and the speed of light
00:34:21 - The World Wide Web nickname
00:36:14 - Speed of light and space travel
00:37:22 - Counting stars in the Milky Way
00:43:16 - Planetary diversity and moon composition
00:47:22 - Tipler cylinder and time travel
00:51:37 - The spacecraft design and terraforming challenges
00:52:29 - Science fiction and John Birmingham's latest series
00:53:38 - The Super Dunk series and a request to the author
00:54:27 - Audience engagement and question submissions
00:55:23 - Conclusion and farewell
Variation of Rotation Curves
The variation of rotation curves is an intriguing aspect of galaxies that fascinates astronomers. It refers to the speed at which stars and other celestial objects move around the center of a galaxy, and how this speed impacts the overall shape and structure of the galaxy. This element of astrophysics provides critical insights into how galaxies evolve over time, contributing significantly to our understanding of the universe's dynamics.
Infrared Observations and Spiral Arms
Infrared observations are pivotal to astronomy, allowing us to perceive celestial bodies and phenomena that remain concealed in other wavelengths. One interesting feature that can be detected in this way is the dust in...
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Hi, Andrew Dunkley here, and
just want to say thank you for listening
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to Space Nuts throughout twenty twenty three. Fred and I are taking just a
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couple of weeks off, but we
will be back early January. In the
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meantime, here's a repeat episode from
early twenty twenty three, one of our
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Q and A episodes, Space Nuts. Hello, and welcome to Space Nuts.
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My name is Andrew Dunkley, your
host. It's so good to have
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your company. And being episode three
hundred and forty five, we dedicate the
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entire show to questions from the audience, and we're going to do a bit
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of a mix of audio and text
questions today. We'll fit in as many
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as we can. We've got five
hundred of them here. We might get
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two or three, we'll see how
we go. We'll be looking at the
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rotation curve of galaxies and walking on
neutron stars. Will also be chasing up
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the previous episodes, talk on asteroids, dark matter, dark energy, white
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holes, the period of inflame,
and much much more. Coming up on
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this episode of Space Nuts fifteen in
Channel ten nine ignition sequence Space Nuts or
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three two Space Nurse, as the
Nights reported, Bils good and joining me
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to answer all of those questions and
more is Professor Fred Watson, an astronomer
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at large. Hello Fred, Hello
Andrew, it's great to see you again.
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You too, after it's been so
long, been so very long.
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Tongue in cheek. Yeah, well, actually we should just blow the whistle.
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We're doing catch up episodes because you're
going to be away for a bit.
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I'm going to be away for a
bit. Adds up to a long
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period of time where we won't be
able to record, so we're working ahead
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of time. But for you who
are listening, it is at the right
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time anyway, so it doesn't really
matter that I'm explaining that like I am.
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We might as well get stuck straight
into it because we've got a lot
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to do, so we will just
go straight into question one, which comes
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from Rusty and our favorite wa town
of Donnybrook. Hey, Fred, and
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Andrew was Rusty and Dinnybrook. I
hope you are keeping cool in our extended
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summertime here in Australia. Fred,
you once famously remarked on this show that
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spiral galaxies, when viewed in infrared
light, completely lose their spirals. You
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don't see them at all. In
infrared. And so I'm wondering, since
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most of the visible light is from
the spirals, and almost all of the
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ultra violet light is also from the
spirals, how does the rotation curve vary
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with wavelength? Thank you? All
right, thank you. Nice to hear
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from you, one of our regulars. Yeah, we did talk about that
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before, and it became apparent that
when you view a galaxy spiral galaxy through
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infrared, there are no spirals.
And yeah, it's got rusty thinking.
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Rusty has an interesting mind. He
thinks about a lot of things. Yeah,
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And actually, Andrew and Rusty,
what's given the lie to my comment
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about the spiral arms disappearing in the
infrared is some beautiful James Webb's based telescope
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images of galaxies wow, which have
sensational spiral arms. Okay, but you're
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you're seeing. So what I said
in the originally is that if you look
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in the infrared, you're you're seeing
dominant galaxies dominated by old stars, and
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they tend to be yellowish in color
rather than rather than in you know,
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rather than blue and white as the
young stars are. And so they they
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do. And it is true that
the galaxy itself has this underlying population of
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these elderly stars that have been there
a long time. So you're an elderly
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star. Well, yes, no, I'm just old. Im there's you
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know, there's just no bitting about
the book, in fact, bordering on
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the ancient. I think they could
say so anyway. Yeah, so,
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so there's an underlying population of old
stars, including me and he, and
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they tend not to delineate the spiral
arms. Then if you look at you
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know, most most images of galaxies, and particularly the early black and white
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ones which were sensitive to the blue
actually rather than the red, they show
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the spiral arms because because that's where
the young energetic stars are, the white
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or bluish in color, and they
show up. Now, spiral arms are
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we know, the host the location
of many young stars because the spiral arms
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are caused by sound waves effectively passing
through them and basically sparking them into ignition.
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And so you get short lived,
very bright stars which show up as
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bluish objects in the spiral alarms.
Now, why does the Hubble, sorry,
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why does the James Webb space telescope
show galaxies with lovely spiral alarms?
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And the answer is that what you're
seeing there is the dust in these in
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these spiral arms, predolently the dust, and that dust is being also pushed
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into a spiral shape by the shockwave
the density wave that's passing through them and
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causing the style formation that reveals the
spiral arms the stars themselves the right.
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So that's just by way of a
caveat to what I said, as Rusty
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quoted me as famously having said that
the spiral arms disappear, and it's it's
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still true, but it's certain wavelengths
of light, which brings me to Russy's
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question, how do the rotation curves
vary with wavelength? So if you are
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always looking at stars, you're going
to see you know, you're seeing objects
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whose spectrum is going from from the
ultraviolet to the infrared, but it's the
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same object and so it's the same
moving with the same velocity. So in
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that regard, you know, looking
at stars in different wavebands, you're still
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going to see the same velocities.
But it extends even further than that.
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And that is because and this was
actually some of the work that Ken Freeman
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here in Australia and Vera Rubin did
in the United States back in the seventies,
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demonstrating the rotation curves of galaxies are
flat. They don't behave as you
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would expect if you look at clouds
of gas with radio telescopes, the sort
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of you know, cold hydrogen in
space, which emits at its radiation of
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twenty one centimeters. It's in the
radio spectrum that follows the same rotation curve
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as the stars do, so in
that regard they are the rotation curves are
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independent of wavelength. Okay, very
good. That was simple. Yeah,
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a long answer to a short question, but a good question, Rusty,
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as Andrew says, you always think
outside the box. You do. Indeed,
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Thanks Rusty, and now we'll move
on to North Carolina, which is
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a long long way from Donnybrook.
And one about female listeners. We don't
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get too many questions from our female
listeners, so it's nice when we do.
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Hello, Nan, I'm confused about
gravity, she says, you'd be
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the only one I heard it described
as the curving of space due to the
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mass of an object. Thus,
an object in the vicinity of another object
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falls into the curve, causing the
object to follow the curve. When referring
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to the formation of stars, the
description seems to be that the gas is
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squeezed until it becomes hot enough to
ignite. This is also described as gravity
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acting on the gas. That seems
to be a different action of gravity than
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the bending of space. Help me
understand, Thanks, Nan, what a
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great question. Yeah, that's a
fabulous question. So, yes, it
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was Einstein who said that gravity is
the phenomenon. It's a geometrical phenomenon,
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is what is said. It's actually
about space being bent by any mass that's
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within it, and so, and
that's fairly easy to get your head around
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for something like the Sun, where
you've got this giant ball of gas which
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is gravitationally distorting the space around it. And that's demonstrated by the fact that
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when you look at the Sun in
eclipse, you see stars in the background
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looking to be in the wrong direction, which is how they proved that Einstein's
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theory was correct. But it's probably
less easy to get your head around that
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when you're thinking just of a giant
cloud of gas. So, if you've
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got a blob of gas in space, and that gas is gravitating because it's
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made of matter, then even though
it's pretty tenuous, is out the word,
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Yeah, it's a ten us object. It's not solid like a planet,
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it will still distort the space around
it, and the effect of that
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is once again that the outer edges
of that space will be bent less than
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the regions towards the center where the
mass is concentrated, and you'll get this
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compression effect. The gas will slide
down the bend space, and the effect
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of it is the temperature increasing and
eventually that cloud of gas turns into a
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star. It's the you know,
the mantra is that what is it?
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Matter tells space, how to bend
space, tells matter how to move right.
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That's the That's the and I can't
think it might be John Wheeler who
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said that, Okay, decades ago, but that's the bottom line. Very
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clever. Okay, we're getting through
on fast. We need to slide.
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It's just too quick for my brain. We can easily see. Thank you,
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Nan. Let's go to our next
question, and this one's a sort
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of a speculator from Russ. Hi. Guys love the show. It's Russ
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here from Stalebridge in the UK.
My question is more of a journey that
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we could take. Let's take out
the physics of the impossible. I we
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won't be able to do it.
But let's have a walk across the surface
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of a neutron star. What would
we be seeing on the surface? What
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does what would the surface look like? Would it be glowing, would it
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be white, would it be in
redescent? What sort of colors would we
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be seeing? If we bend down
and touch the surface, what would it
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feel like if we were able to
jump off a little step, maybe your
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foot high? How fast woud we
be going when we hit the surface.
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If we looked up into space,
what would we see? Just can we
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just have a theoretical walk across the
surface of a neutron star? Thanks very
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much, love the show, guys, Take care, Okay, thank you,
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Russ. We have talked about neutron
stars before. I think the very
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first thing that we can say is, as soon as you walk on a
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neutron star, you're you're a mountain
climber. Yeah, because the mountains are,
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as we discussed before, millimeters high, yeah, a few millimeters.
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Actually, something happens to you before
that though, you die of a horrible,
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painful, immediate prispy death. Well
your spaghettifying, all right, just
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like because like a black hole,
you know, the gradient the gravity gradient
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around a neutron star is very steep, so your head's feeling, you know,
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as you walk, your head is
feeling less gravity than your feet,
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and you spaghettified. Basically, it's
not very nice, not pretty. So
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but yeah, what an interesting question. And I think it, I think,
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and I ought to check this,
but I think the surface of a
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neutron star is very very radiative,
so it's beaming out light and I think
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it's probably ultraviolet because it's such high
energy. So it's all the good stuff
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like the human body loves exactly.
Well, you've got now everything else,
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You've got everything. It's it's not
just the gravity and the the blinding intensity
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of the radiation. You've also got
intense magnetic fields that I'll probably screw your
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insides up completely. Stepping off a
doorstep would happen because the doorsteps already been
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squashed as being something less than a
micron high, So there's not much to
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do with looking at the sky from
the neutron star. Yeah, you would
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see it probably would look a bit
weird because there would be definitely gravitational distortion
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effects in the space around you,
and that might cause some strange effects,
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particularly near your horizon with you know, stars compressed one way or the other.
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So it would be an environment that
is very very different, you know,
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assuming that we could magically somehow survive
it, it would be very very
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different from anything we experience on Earth. And that is I guess typical of
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astronomy all pretty well, all the
objects we talk about. If you transported
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yourself from Earth to one of those
objects, no matter what it was,
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even if it's an asteroid, the
phenomena that you would encounter will be so
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different from what we have on our
own planet that it makes for very interesting
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thought experiments and very interesting really and
I hope very interesting podcasts. Indeed,
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in fact, we are so well
adjusted to our own planet because we've spent
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hundreds of thousands and more tens of
thousands of years adapting to this environment,
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just about anywhere else we could go
would not be good for us. No,
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that's right, unless we could find
another planet exactly the same as ours
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in terms of every ways and proximity. Yeah, well, it's you know,
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going around a star like the Sun
rather than a red dwarf that's going
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to spit out all the time.
Yes, No, I mean it's not
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surprising. You know, we've evolved
as creatures of the Earth, so we
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are very well adapted to it.
And you can kind of imagine how many
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million years it might take for humans
to adapt to being on a neutron star
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if they're good. Yes, I
think supermodels would adapt well because they like
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being skinny. Yeah, skinny is
one thing, but spaghettiveations another. The
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one good thing about a neutron star
is that you could walk all the way
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around it in a you know,
much of ours. Is that right?
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Because they're not very big? Are
they the side of a city? That's
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right? So yeah, yeah,
slums down third, it might be thirty
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killing time bus or get mugged.
Probably get mugged the neutron bus. Are
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all right? Thank you, Rus, lovely to hear from you, and
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thanks to Rusty and Nan for sending
in questions to us on this episode three
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hundred and forty five of Space Nuts. Space Nuts. All right, we'll
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just carry right on, Fred because
we have a question from Jeff. This
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is a follow up to something we
talked about in the last episode. Hey
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freend Andrew Jeff in Ohio US eight
here. They just want to clarify a
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couple of biochemical things from the urosl
and an asteroid discussion, and ask a
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question as well about dark matter dark
energy. So, yes, biological processes
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on Earth that make proteins use all
l amino acids, but some biological organisms
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actually use d amino acids make d
amino acids. For example, Anthrax makes
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a polymer out of glutamic acid that's
all D or mostly D. And also
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when we're talking about trying to find
DNA in an asteroid, there's a leading
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hypothesis that actually RNA was the world
before DNA and protein showed up that it
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not only held it genetic material like
DNA does, but also catalyze reactions like
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proteins do, and we still see
evidence of that today. So my question
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about dark matter dark energy, I'm
slightly familiar with these two concepts being described
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as a web that kind of holds
galaxies together and keeps them from playing apart.
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And I think there was some kind
of modeling that showed that, or
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at least try to model what that
web might look like maybe a few years
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ago. And Science or Nature,
did you talk a little bit more about
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the background on this dark energy dark
matter WAB. I'd like to know a
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little bit more on the background,
so I can kind of run of it
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from there. Thanks you guys,
keep up the good work. Really love
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the show. Thank you about Thank
you Jeff, And wow, what on
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a Stuid fellow? He knows his
stuff about RNA and DNA, and yeah,
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very very clever. Brought up some
interesting points I didn't know. Is
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he right that the Earth was probably
more RNA than DNA in the beginning and
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something changed. I'm not sufficiently engaged
with the world of evolutionary biologis and I
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before. I'm very glad that Jeff
put those ideas there, because, yeah,
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we'll follow up on that. Yeah, and I find out what the
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story is that. But his main
question was about one of our favorite topics,
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dark energy and dark matter. And
yeah, he did describe them as
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the web that holds galaxies together.
And we have said before that if there
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was none of these galaxies would just
spin themselves into oblivion. They just go
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in all directions, I suppose,
So yeah, how does it work?
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I suppose was what he wanted to
know. Yeah, so giant space spiders.
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God, you've cut to the chase. David Bowie was right, spiders
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from Mars. There you are spiders
from Mars. Yeah, So we need
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to disentangle dark matter and dark energy
though, because dark energy is not something
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that's part of the web that just
talking about, just talking about the cosmic
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web, which is structures of matter
within the universe. Now, there were
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structures of matter we think were instrumental
in the creation, just as you said,
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Andrew of galaxies, because we find
that when you build models of the
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way the Big Bang evolves, you
end up with this web of material.
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It's almost like a foam, if
I can put it that way, very
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much like cells of a honeycomb,
with the walls between the honeycomb forming the
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structure of the web, which is
there in both dark matter and normal matter.
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The dark matter probably was the first
thing to sort of crystallize into this
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web shape after the Big Bang,
with the normal matter being gravitationally attracted to
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it because dark matter outweighs normal matter
by five to one or thereabouts. So
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that's the hydrogen that followed the dark
matter, and that hydrogen then collapsing into
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stars, gas clouds, galaxies and
all the stuff that we're familiar with now.
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But dark energy is probably uniform throughout
the universe, so it's not part
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of this web structure. The web
structure is just for matter, whether it's
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dark matter or what we call baryonic
matter, which is the matter that we
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can detect that forms the web.
But dark energy doesn't. Dark energy seems
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to be a property of space itself, irrespective of what structures you build inside
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it. The dark energy is there, and the effect of dark energy,
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of course, is what we see
with the galaxy. Sorry, with the
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universe accelerating in its expansion, as
it has been doing for about the last
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five billion years. We think that
before that it wasn't accelerating in its expansion,
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even though dark energy was there.
But the galaxies were close enough together
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that their mutual gravitational attraction resisted the
effect of dark energy. And it was
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only as the universe continued to expand
that the galaxies became far enough apart that
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their gravitational pulled towards each other was
not strong enough to overcome the accelerating effect
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of the dark energy. So that
acceleration is something we've only seen for about,
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you know, half the age of
the universe. Before that, it
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were the universe's expansion was probably slowing
down any furious as to what changed.
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Yeah, the fact that the galaxies
became far enough apart that the gravitational pull
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between them wasn't breaking the yes,
the expansion, and so that allowed the
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dark energy to so we were we
were dominant. We were basically holding it
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back until it reached a release point. And ye, where she went where
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she went quite gradually. But it's
sort of like when you blow up a
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balloon. When you first start to
blow up a balloon, it's really it's
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a hard thing to do, and
then it suddenly gets easier. That's a
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really good analogue actually, because what
you're feeling at first, when you're puffing
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hard against the resist resistance of the
of the of the you know, the
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rubber or whatever really it is,
and that then gets beyond a certain point
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where it's really easy to blow it
up, and if you do it too
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much, it bursts, which is
probably what the universe will do in the
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big Rip in a few trillion years
time or next week, whichever is longer,
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whichever comes sooner. Yes, that's
right. Yeah, Well I hope
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that explain or helps to explain some
of the you know, the confusion there.
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Jeff separate dark energy and dark matter
out in your mind, because they're
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quite different things. But the dark
matter is what forms that web like structure
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that basically is the scaffolding, scaffolding
on which the objects in the universe were
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built. Yes, and as we've
mentioned in previous episodes, they're just badly
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named dark edge. You'll probably be
called something else so that there's no confusion.
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But that yeah, that's where the
sort of crossed up dark matter would
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have been better as invisible matter.
I think, yeah, but dark seems
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to be the buzzword it does,
all right, Thank you, Jeff.
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We've got a text question from Austin, Texas. It's kaos. He says,
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Hello Andrew and Professor Watson. I
will preface this question by saying that
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it may not have a conclusive answer
because it details in the theoretical I was
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pondering the concept of white holes being
mathematically understood but not observed. I wonder
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if white holes could lurk in the
dark matter spectrum of the universe. Just
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like we can't detect the or understand
dark matter slash dark energy, could it
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be possible that white holes exist within
this yet to be understood spectrum of the
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universe. Thanks for a great show. Every week. Much love to y'all.
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I hope I said that right from
Texas. Yehare, that's what it
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had not me him. Good bro, that's very flavorous of it. And
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yeah, some bootscooters are lurking somewhere. There are probably, Yeah, so
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that's an interesting thought. Let's explore
that a little bit, the idea that
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maybe in the dark matter universe,
which we can't detect directly, there are
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objects akin to black holes and white
holes. Let's let's do it both ways,
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okay, And Carlos is absolutely right
that the mathematics of black holes or
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the mathematics of gravitation, let you
conjecture that there are such things as white
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holes. And when you're working in
the equations, I think what you do
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is you reverse the sign of time, so you put times going negative,
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and you've got a white hole instead
of a black hole. But we see
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nothing in the universe that actually could
be one of those, because unlike a
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black hole where nothing gets out,
with a white hole, nothing gets in.
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Yeah, and you'd think you'd notice
that, but I guess that the
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bottom line here is when you all
right, let's think about dark matter,
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we think it is some kind of
species of sub atomic particle and perhaps many
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different species of sub atomic particle excuse
me, which doesn't interact with normal particles.
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So it doesn't interact with light.
We can't see it shining. It
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doesn't interact with matter, you know, it doesn't seem to react with that
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with normal matter. All it does
is displays gravity. It has gravity,
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and that's how we detect it because
as exactly as you said earlier on,
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when we look at the way galaxies
work, if you spot a rotating galaxy
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and if all that you can all
that was in there is all that you
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can see, if that's all there
is, then it should have flown itself
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apart gazillion years ago, maybe on
a millennia ago, but a long time
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ago. It should. It should
can't exist without the idea that there is
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some invisible material holding it together.
And when you do the theory, you
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get the calculation or you get the
almost a picture that shows you that these
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galaxies are embedded in halos of this
mysterious dark matter. Now, dark matter
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reveals itself by its gravity, and
so gravity behaves normally as far as dark
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matter is concerned, which suggests that
if you had a dark matter black hole,
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it would exhibit its forces or exhibit
its present in exactly the same way
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as a normal matter black hole does, because it would be a singularity with
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intense gravitational field around it, which
would pull other stuff in, whether that
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was gas being accreted like it is
at the center of a galaxy, whether
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it's a supermassive black hole, or
you know an x red binary where you've
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got a companion star that's leaking material
onto the black hole and causing it to
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release X rays. All of that
should still hold good, so that what
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you see in the black hole universe
in real normal matter burialic matter, you
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should also see in dark matter.
Right, okay, interesting, sobly probably
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not is what the answer is,
which saved us a lot of time.
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But we were going slow at the
start, so that's fine. I've actually
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discovered a white hole. Where is
it? It's called my bank account.
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Nothing gets in, yest in,
but things get out. Yeah, yes,
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that sounds like a white hole.
It's definitely a white hole. All
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right, thanks Carlos. Let us
move on to Duncan. I think Duncan's
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sent us a few questions in recently, so let's tackle this particular one.
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I think he's looking at the period
of inflation. Hello Duncan here from Weymouth
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in the UK, questioned about a
period of inflation after the Big Bang when
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the universe expanded faster than the speed
of light. Was that faster than the
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actual speed of light? Or was
it that the speed of light at that
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time was faster than it was now. I'm just thinking that if the speed
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of light in itself at that time
was faster, could it be that there
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is some property of the universe in
which light is able to travel faster than
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what it does currently in the current
vacuum. And if we could discover what
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that particular property of the universe back
then was, then maybe there would be
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some way that obviously in the distance
future or current technology to create a drive
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that goes faster than it. I
don't know, it's just the obviously were
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limited to the speed of light.
But if the speed of light in itself
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could be increased, then who knows? Anyway, Thanks for you help keep
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up the good work. Well,
okay, thank you, Duncan. Always
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good to hear from you. And
now I understand how the Americans have learned
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to pronounce things differently to us because
of Duncan's accent. I picked up something
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an American pronunciation in there. I
can't remember what the word was now,
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but yeah, that's what I was
going to ask you. Yeah, I
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just went straight out of my head. It's very late on a Friday here,
348
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so my brain decides to give up
once I've once I've walked out of
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the office. But a period of
inflation, yeah, we know, you
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know more, immediately after the Big
Bang, the universe expanded, it faster
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than the speed of light, and
then it slowed down, and now it's
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accelerating again. Weird does Duncan's theories
sit. There's two different things we're talking
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about here, Andrew and Duncan.
So the when you think about inflation,
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the speed of light doesn't matter because
it's the fabric of space, whatever that
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is. It's you know, it's
space itself that's expanding. And you know,
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you could only talk about being faster
than the speed of light if you
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think of two points within that space, how fast are they receding from one
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another? And it may well be
faster than the speed of light. In
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fact, it would have to be
just because of the way the inflation took
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place. It was an extraordinary period
in the universe's history. But it is
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the space that's that's that's that's expanding
very fast, and that doesn't impact the
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speed of things going through it.
So one of the basic foundations of cosmology
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as we understand it, our theory
of the origin and evolution of the universe.
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One of its basic principles is that
the speed of light is a constant,
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that it has always been the same
ever since the beginning it was three
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hundred thousand kilometers per second. There
are probably still people I hadn't really course
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up with this work yet, but
sorry recently, I haven't caught up with
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it recently. This is work that
was done a decade or more ago by
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colleagues here in Australia, in fact, principally at the University of New South
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Wales, who were observing different distant
quasars and there was just some evidence in
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those there were spectra. They were
taking the rainbow spectra of these quasars and
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look at the features in them.
There was evidence that hinted that some thing
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was varying, that one of the
fundamental physics principles was different then than it
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is now. Because when you're looking
at as you're looking a long time back
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into the past, and the inference
was that it was either the charge on
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the electron or the speed of light
that was different. That work was always
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greeted with a reception that was less
than worn by the astrophysical community. And
378
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I know why because I've seen the
data and it is really, it was
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really, you know, it was
right on the limit of detectability, this
380
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this effect that they were highlighting.
And I suspect that more recent observations because
381
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we've now observed quais as to death
in that, you know, in the
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last twenty years or so, I
think with those more recent observations it might
383
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have gone away. However, might
not have done. And I would not
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be surprised if we hear from one
of the proponents of that that work and
385
00:34:08.920 --> 00:34:14.199
one of the people who carried it
out, who is a good friend.
386
00:34:15.960 --> 00:34:19.880
I'm going to tell the standard joke
about this gentleman. I hope if he's
387
00:34:19.920 --> 00:34:23.880
listening you won't mind. His name
is John Webb. And the thing about
388
00:34:23.920 --> 00:34:27.920
John Webb was you never met up
with him at the University of New South
389
00:34:27.960 --> 00:34:30.800
Wales. It was always in New
York, of Cambridge or Paris or somewhere.
390
00:34:30.800 --> 00:34:35.079
It was always somewhere else, which
is why he became known as the
391
00:34:35.159 --> 00:34:39.280
Worldwide One. Yes, I remember
this once before. That's a great Yeah,
392
00:34:39.360 --> 00:34:43.199
that's a great nickname. Yeah,
great, it is a great nickname.
393
00:34:43.360 --> 00:34:45.800
Is a great guy as well.
Yeah, you know, and I'd
394
00:34:46.400 --> 00:34:51.639
be nice to try to catch up
with him in Cairo or somewhere to find
395
00:34:51.679 --> 00:34:57.440
out whether he's still whether whether those
ideas are still prevalent. Yeah, I
396
00:34:57.480 --> 00:35:04.679
should look it up. I have
a listener from Kune Barrabin who emails me
397
00:35:04.800 --> 00:35:07.480
quite regularly and listens to Space,
and that's H Barry. He sent me
398
00:35:07.559 --> 00:35:14.039
some nicknames the other day. Keith
kat E t H. It's the nickname
399
00:35:14.119 --> 00:35:20.079
of a bloke with named Keith,
but he only has one eye, so
400
00:35:20.199 --> 00:35:27.960
he's lost his eye. Keith.
Well, I love it. That's a
401
00:35:28.119 --> 00:35:30.320
very clever nickname, very clever nicknase. It's a good one. Yeah.
402
00:35:30.320 --> 00:35:35.199
It's nearly as good as the guy
with the shovel on his shoulder, isn't
403
00:35:35.199 --> 00:35:39.639
it. What's that Doug Dog?
Yeah, yeah, yeah, the guy
404
00:35:39.719 --> 00:35:45.760
floating in the ocean, Bob,
there's a shovel on his shoulder, Douglas.
405
00:35:47.280 --> 00:35:51.639
We could go on forever, but
we probably lose our entire audience.
406
00:35:52.880 --> 00:35:55.800
You've done, Duncan, Yes,
just to return to it. I think
407
00:35:57.320 --> 00:36:02.079
you know, it really is very
principle of our understanding of the universe that
408
00:36:02.159 --> 00:36:09.800
the speed of light hasn't there,
and so engineering the speed of light itself
409
00:36:09.880 --> 00:36:14.639
down the truck is something that I
suspect we would never get to. Okay,
410
00:36:15.239 --> 00:36:19.199
and not for want of trying.
We're trying ways of speeding up our
411
00:36:19.480 --> 00:36:23.079
capacity to move through the universe.
But yeah, getting to the speed of
412
00:36:23.159 --> 00:36:24.840
light, I mean, if we
can get to a fraction of it,
413
00:36:24.920 --> 00:36:30.480
that'll be an achievement. But yeah, full speed of light probably way out
414
00:36:30.519 --> 00:36:34.559
of our realm, given how much
energy is required. Thank you. Duncan
415
00:36:35.000 --> 00:36:38.960
loved the question. This is space
Nuts Andrew Dunkley here with Professor Fred Watson,
416
00:36:44.719 --> 00:36:49.960
Spacenuts. Okay, let us continue
and our next audio question comes from
417
00:36:50.199 --> 00:36:54.880
Mark. Hey, guys, this
is Mark from Baton Rouge, Louisiana.
418
00:36:55.679 --> 00:37:00.119
I really love your shirt. I
understand that one of the lines of reasoning
419
00:37:00.280 --> 00:37:05.840
pointing toward the existence of dark matter
has to do with the comparison of the
420
00:37:06.000 --> 00:37:12.239
rotational period of galaxies to the amount
of matter that they contain. However,
421
00:37:12.400 --> 00:37:16.000
I've seen various estimates of the number
of stars in the Milky Way galaxy,
422
00:37:16.480 --> 00:37:22.159
ranging anywhere from one hundred to about
four hundred billion stars. This is quite
423
00:37:22.159 --> 00:37:27.679
a large Arab war, I would
say, and I'm curious how they can
424
00:37:27.760 --> 00:37:31.440
make this comparison if astronomers are this
unsure of the number of stars in our
425
00:37:31.480 --> 00:37:37.199
own galaxy, much less other galaxies. Thanks, guys, I hope to
426
00:37:37.239 --> 00:37:44.199
get an answer. We hope to
give you on one day. Actually you're
427
00:37:44.239 --> 00:37:47.400
asking the right block because Fred has
been counting stars for all of his career.
428
00:37:49.159 --> 00:37:54.079
Pretty well, that's right, And
yes they you know, the way
429
00:37:54.199 --> 00:38:02.199
you estimate the number of stars in
a galaxy is certainly in our own galaxy.
430
00:38:05.639 --> 00:38:09.039
You're what you're trying to do is
find a way of measuring its mass
431
00:38:10.119 --> 00:38:17.559
and then you turn that into stellar
masses. But one stellar mass does not
432
00:38:17.679 --> 00:38:22.159
necessarily equal one star. So some
of the work, in fact, I
433
00:38:22.320 --> 00:38:28.559
was involved with this work decade or
so ago, by trying to measure the
434
00:38:28.599 --> 00:38:37.679
mass of our galaxy by using the
escape velocity of stars. If you think
435
00:38:37.679 --> 00:38:43.760
about the way stars some stars might
escape from the galaxy, then you can
436
00:38:44.119 --> 00:38:46.519
use that if you this is we
did this with the rave experiment, the
437
00:38:46.639 --> 00:38:52.760
radio velocity experiment, you can actually
deduce back what the mass of the galaxy
438
00:38:52.880 --> 00:38:59.559
is within that radius with it where
the particular star is. Actually it's within
439
00:38:59.639 --> 00:39:02.400
the radi of the Sun, the
Sun's distance from the center of the galaxy,
440
00:39:02.719 --> 00:39:08.519
and you get if I remember Odi, we got one point for trillion
441
00:39:10.920 --> 00:39:17.760
trillion solar masses for the mass of
the galaxy. But that includes dark matter,
442
00:39:19.679 --> 00:39:23.519
so it's not individual stars. So
you know, you've got to know
443
00:39:23.719 --> 00:39:30.079
something about the universe before you make
these calculations, and looking at other galaxies,
444
00:39:30.639 --> 00:39:36.880
it's easier you don't count the individual
stars in the galaxy. And it's
445
00:39:36.920 --> 00:39:39.440
only recently that we've been able to
see the individual stars in the galaxy,
446
00:39:39.920 --> 00:39:47.119
although back in the nineteen twenties Hubble
was observing Cepheid variable stars in the Andromeda
447
00:39:47.159 --> 00:39:51.599
galaxy and that was an early step
in that direction. But most of the
448
00:39:51.679 --> 00:39:53.960
stars in a galaxy are too faint
to do that, and Allly sees this
449
00:39:54.119 --> 00:40:01.519
glow which collects them together. But
by observing so what you're doing is you're
450
00:40:01.599 --> 00:40:08.440
looking at the luminous characteristics of a
galaxy, the stuff that is emitting lines.
451
00:40:09.800 --> 00:40:14.840
Even if you can't see the individual
stars, and from that you can
452
00:40:15.039 --> 00:40:19.639
deduce the stellar mass content that is
emitting the light. In other words,
453
00:40:20.119 --> 00:40:23.199
you've got some handle on the normal
matter. And it turns out that that
454
00:40:23.480 --> 00:40:31.079
is far too little to keep the
galaxy held together. And so that difference
455
00:40:31.119 --> 00:40:36.840
between one hundred and four hundred so
you know, stars in our own sorry,
456
00:40:36.920 --> 00:40:39.159
four one hundred and four hundred billion
stars in our own galaxy. Yes,
457
00:40:39.199 --> 00:40:45.599
it's a four to one error,
but it's still well within the limits
458
00:40:45.719 --> 00:40:50.760
that would be imposed by dark matter. The dark matter itself is much more
459
00:40:50.800 --> 00:40:52.960
than that, is what I'm trying
to say. It doesn't matter whether it's
460
00:40:52.000 --> 00:40:57.480
one one hundred billion or four hundred
billion, the dark matter content has to
461
00:40:57.559 --> 00:41:00.559
be still much more. Okay,
so it is. It's a good question
462
00:41:00.719 --> 00:41:05.000
mark, and you know, it
goes to the heart of how we understand
463
00:41:05.079 --> 00:41:09.920
these things. The it's not just
the rotation of galaxies, of course,
464
00:41:10.000 --> 00:41:16.920
that leads us to believe dark matter
is real. Another very strong pointer to
465
00:41:17.280 --> 00:41:22.679
the existence of dark matter is the
distortion of space by clusters of galaxies and
466
00:41:22.760 --> 00:41:25.760
galaxies themselves. Once Again, if
you look at a galaxy, the space
467
00:41:25.800 --> 00:41:32.719
around it is distorted to the far
more than you could account for simply by
468
00:41:32.760 --> 00:41:37.280
the luminous matter in the galaxy.
It's it's got much more to it.
469
00:41:37.679 --> 00:41:42.039
And that's why we're so booked on
the idea of dark matter, because all
470
00:41:42.079 --> 00:41:45.280
the tests seems to should suggest it's
there. Yeah. Wow, Okay,
471
00:41:45.679 --> 00:41:51.239
I've been trying to count the stars. I'm up to five. So you've
472
00:41:51.280 --> 00:41:52.880
been observing the Southern Cross then,
yeah, I've been. That's as far
473
00:41:52.920 --> 00:41:58.159
as I got. Yeah, oh, hang on to the sun six.
474
00:41:59.119 --> 00:42:02.440
There you've making progress. Well done, you are, Thank you Mark.
475
00:42:02.639 --> 00:42:07.400
And now we've got a question from
Nick. Who is another sandgroper? Do
476
00:42:07.440 --> 00:42:12.960
you know the term sandgroper fruit?
They don't. That's what we call West
477
00:42:12.960 --> 00:42:16.639
Australians. They're sand gropers. So
South Australians are crow eaters. I know
478
00:42:16.760 --> 00:42:21.800
where that comes from. Crow eaters
because back in the day, during the
479
00:42:21.840 --> 00:42:24.519
gold Rush I think or something around
that era, there wasn't much food,
480
00:42:24.599 --> 00:42:29.280
so they used to eat crows.
They used to shoot them. They called
481
00:42:29.320 --> 00:42:34.119
them something else, they called them
desert pigeons or something, but they used
482
00:42:34.119 --> 00:42:37.960
to shoot crows and cook them and
eat them, so they became crows.
483
00:42:37.079 --> 00:42:42.960
I'm still to find out why West
Australian is called a sandgroper though, but
484
00:42:43.000 --> 00:42:45.760
I'm going to find out. I'm
sure it's on the interwebs somewhere anyway.
485
00:42:45.800 --> 00:42:51.960
This sandgroper is Nick from Perth,
who has a question about planetary diversity.
486
00:42:52.840 --> 00:42:58.119
It is a given that the planets
of our Solar system formed by accretion from
487
00:42:58.159 --> 00:43:01.519
a disc of dust and gas circling
around the young Sun, that's the sixth
488
00:43:01.679 --> 00:43:07.440
star in the sky. Gravity inspired
differentiation leading to more dust on the inner
489
00:43:07.519 --> 00:43:14.000
disk and gas of the outer of
the outer resulting in the inner rocky planets
490
00:43:14.000 --> 00:43:17.400
and the outer gas giants all good. Aside from those groupings, what fascinates
491
00:43:17.519 --> 00:43:23.679
me is the lack of homogeneity between
the planets and moons around the gas giants
492
00:43:23.719 --> 00:43:28.519
within these two groupings. They are
so different, all of them. How
493
00:43:28.599 --> 00:43:31.880
did that happen? Can Professor Watson
recommend some reading on the matter. Should
494
00:43:31.880 --> 00:43:36.320
I buy his books? Well?
That's simple answer is yes, Nick.
495
00:43:37.159 --> 00:43:44.159
But it's an interesting observation though,
because we've got rocky planets inside, we've
496
00:43:44.239 --> 00:43:51.119
got gas giants further out, and
yet they've got rocky moons surrounding them,
497
00:43:51.280 --> 00:43:54.480
and ice moons and all this other
weird stuff. Why is it, so
498
00:43:58.079 --> 00:44:02.360
yeah, and which book is it
in? The best one actually is probably
499
00:44:02.400 --> 00:44:08.360
the Kids book. It's the one
where I think I went into the most
500
00:44:08.440 --> 00:44:12.440
detail about planet formation, which I
probably shouldn't have done in the Kids but
501
00:44:12.559 --> 00:44:16.920
but never mind, it was it
was fun to write. So we think
502
00:44:17.039 --> 00:44:27.039
we understand why there is this differentiation
between the inner rocky planets and the outer
503
00:44:27.719 --> 00:44:34.679
gassy ones because of the existence of
the frost line. So if you look
504
00:44:34.760 --> 00:44:44.960
at the distance from the Sun where
water freezes, basically, it's it's kind
505
00:44:45.000 --> 00:44:46.840
of beyond it's the outer edge of
the gold what you might call the outer
506
00:44:47.000 --> 00:44:51.599
edge of the Goldilocks zone. Yees
too hot and it's not too called for
507
00:44:51.719 --> 00:44:54.400
liquid water to exist, and so
you've got and it's between the old bits
508
00:44:54.440 --> 00:45:00.800
of Mars and Jupiter basically, And
that's what you'd expect because the we think
509
00:45:00.920 --> 00:45:07.199
that the idea of water, which
is by far the commonest to element molecule
510
00:45:07.239 --> 00:45:14.440
in the universe, freezing and causing
an increase in the mass of the outer
511
00:45:14.840 --> 00:45:17.400
worlds as the planets were forming.
We think that's why they were able to
512
00:45:17.480 --> 00:45:22.800
hold onto a gas assemblop and become
gas giants, whereas that the inner rocket
513
00:45:22.840 --> 00:45:28.000
planets were within the frost line,
and so it was you know, they
514
00:45:28.039 --> 00:45:32.800
weren't able to do that. So
so that's a neat explanation. But then
515
00:45:35.079 --> 00:45:43.920
the moons themselves, you know,
Nick is quite right that the moons themselves
516
00:45:43.960 --> 00:45:50.079
are diverse, but they are all
basically rocky bodies, rather like asteroids,
517
00:45:51.159 --> 00:45:57.000
with some of them have gotten over
an over layer of water and an overlayer
518
00:45:57.039 --> 00:45:59.440
of ice on top of that.
Many of them, which we've talked about
519
00:45:59.440 --> 00:46:04.039
many times, for some are just
rock like Eo, Some are just lumps
520
00:46:04.079 --> 00:46:08.000
of In fact, some are probably
more like Pommis Phobos. The moon of
521
00:46:08.119 --> 00:46:15.119
Mars is diverse in that regard,
in that more than fifty percent of its
522
00:46:15.199 --> 00:46:21.079
his mass is empty space, which
is what gives it that low density.
523
00:46:21.480 --> 00:46:27.559
So there is still diversity among the
moons even when you consider that. Yes,
524
00:46:27.639 --> 00:46:31.760
they're all basically made of rock,
but maybe the gas giants are as
525
00:46:31.800 --> 00:46:36.360
well. We don't know whether they
have a rocky core. Yes, yeah,
526
00:46:36.400 --> 00:46:38.480
that's one of the mysteries, isn't
it. So it's possible that guest
527
00:46:38.559 --> 00:46:44.199
giants are something of an illusion in
some respects. That's right. They might
528
00:46:44.280 --> 00:46:50.559
be just rocky planet's masquerading as something
else. Yeah, just got massive atmospheres.
529
00:46:51.119 --> 00:46:53.800
Yeah, big atmosphere. Yeah,
it's like a big hairdo really his
530
00:46:54.119 --> 00:47:00.960
which you don't know anything about.
Actually I did once. I'm rapidly catching
531
00:47:00.079 --> 00:47:04.199
up to you as you can see. Yes, all right, Thank you,
532
00:47:04.320 --> 00:47:08.559
Nick, and enjoy groping the sand
whatever that means in Western Australia.
533
00:47:08.639 --> 00:47:14.239
Love Western Australia. Beautiful, beautiful
place. To our final question, Fred,
534
00:47:14.440 --> 00:47:21.039
and it comes from one of our
favorite terraforming experts and sci fi writers.
535
00:47:22.760 --> 00:47:28.079
I'm going to introduce him the way
he introduces us. Hello Martin,
536
00:47:28.760 --> 00:47:38.079
Hello space. That markin Berming Gorvain
here writer extraordinaire in many genres. Today
537
00:47:38.639 --> 00:47:45.039
we're going to terror form a completely
theoretical object. And I would just like
538
00:47:45.159 --> 00:47:53.800
to know what you would see if
you were on a tiplar cylinder and a
539
00:47:55.599 --> 00:48:08.280
circling around it overhead was a a
space ship that Professor Tepplai tells you would
540
00:48:08.320 --> 00:48:14.800
be going back in time. Love
your show. I can't wait for the
541
00:48:14.920 --> 00:48:20.360
answer, Berman Borvain in Potnic,
Maryland, USA, over and out.
542
00:48:20.960 --> 00:48:23.320
Thank you Martin. He's really stretching
now, isn't he. Now. I
543
00:48:23.480 --> 00:48:27.960
just tried to look up what a
tipless cylinder is also known as a tiplar
544
00:48:28.039 --> 00:48:31.039
time machine. It's a hypothetical object
theorized to be a potential mode of time
545
00:48:31.119 --> 00:48:37.199
travel, although results have shown that
a tipless cylinder could only allow time travel
546
00:48:37.440 --> 00:48:44.199
if its length were infinite with the
existence of negative energy. So yeah,
547
00:48:44.480 --> 00:48:49.840
I'm actually looking at the same page
as right and true if it's if its
548
00:48:49.920 --> 00:48:54.000
length were infinite or with the existence
of negative energies. So you've got two
549
00:48:54.079 --> 00:49:01.480
alternatives there, and infinite length is
tricky, does a bit make negative energy
550
00:49:01.719 --> 00:49:07.840
is even trickier. That's why we're
probably never going to build one. But
551
00:49:07.960 --> 00:49:14.239
what an interesting idea it was.
It was it actually is something that falls
552
00:49:14.320 --> 00:49:20.880
out of the equations of relativity,
and in fact, it was mathematicians looking
553
00:49:20.960 --> 00:49:28.679
at those equations back in the nineteen
twenties that produced this idea of as you
554
00:49:28.719 --> 00:49:32.840
said, a hypothetical object theory ez
to be a potential mode of time travel,
555
00:49:35.119 --> 00:49:43.960
and it's because of its effect on
the closure of off space time.
556
00:49:44.039 --> 00:49:47.880
You might put it that way.
The gravitational potential is such that you get
557
00:49:49.960 --> 00:49:54.079
instead of space time being a nice
you know, a nice lattice of stuff,
558
00:49:54.119 --> 00:49:57.159
a bit. I always think of
space time as being like one of
559
00:49:57.199 --> 00:50:01.800
those climbing frames that you find in
kids kids parks, the old fashioned ones.
560
00:50:01.800 --> 00:50:06.079
Anyway, they're not like that anymore. But they were just a you
561
00:50:06.159 --> 00:50:09.840
know, a regular set of things
are arranged in right angles, and it
562
00:50:09.960 --> 00:50:15.519
gave you a three dimensional structure that's
you know, that's normal space time.
563
00:50:16.639 --> 00:50:21.199
Ben space time is when somebody every
stands on one of those and that's what
564
00:50:21.920 --> 00:50:27.159
that's what the what The equations of
relativity shows that when you put matter in
565
00:50:27.239 --> 00:50:30.559
there, they bend. But when
you think of all this happening around an
566
00:50:30.599 --> 00:50:37.639
infinitely long cylinder, you get the
the structure of space itself closes on its
567
00:50:37.840 --> 00:50:40.000
on itself. If I can put
it that way so that you you've got
568
00:50:42.119 --> 00:50:45.400
a way of moving around in time
as well as space, that's the that's
569
00:50:45.480 --> 00:50:52.440
the idea. There's there's also a
phenomenon called frame dragging, which we know
570
00:50:52.559 --> 00:50:58.159
is a real phenomenon of relativity.
It's there was certain I forgot which spacecraft
571
00:50:58.239 --> 00:51:05.039
it was. Won't come back to
me. There was one particular spacecraft that
572
00:51:05.440 --> 00:51:09.599
was put into orbits around the Earth
that was designed to demonstrate that the Earth
573
00:51:09.639 --> 00:51:16.960
as it rotates drags space time with
it. This frame dragging phenomenon. So
574
00:51:17.039 --> 00:51:20.679
we needed to give a story on
that a while back. I think we
575
00:51:20.760 --> 00:51:23.280
did two. Yeah, I think
we did two. And so the cylinder
576
00:51:23.320 --> 00:51:29.440
itself is it's spinning along its long
axis, will create this frame dragging effect,
577
00:51:29.960 --> 00:51:35.719
warping space time in such a way
that you might be able to travel
578
00:51:35.760 --> 00:51:39.400
backwards in time. That's the bottom
line, okay, And so I forgot
579
00:51:39.599 --> 00:51:45.159
what Martian's question was. What would
a spacecraft look like it was going backwards
580
00:51:45.159 --> 00:51:49.679
in time? It probably just like
playing a movie in reverse. Probably.
581
00:51:52.119 --> 00:51:57.079
Sadly, the boot was put in
by a number of people, including a
582
00:51:57.159 --> 00:52:07.480
follow called Stephen Hawking. He through
a relativistic argument the idea of a tipless
583
00:52:07.559 --> 00:52:12.480
cylinder, suggesting that it would never
it would never be able to be built,
584
00:52:13.159 --> 00:52:16.800
which means you couldn't terraform one.
Basically, that's right, it's forgotten,
585
00:52:17.199 --> 00:52:21.559
forgotten. Terr reforming was at the
heart of Martin's question, as it
586
00:52:21.559 --> 00:52:25.239
always is. And terr reforming a
tipless cylinder, Yeah, that would be
587
00:52:25.280 --> 00:52:30.239
tricky. That would be very tricky. You know, you're a sci fi
588
00:52:30.400 --> 00:52:35.679
writer, Martin, I'm just do
it, just do it. It can
589
00:52:35.760 --> 00:52:38.639
do anything in science fiction. Well, you know that. You know that's
590
00:52:38.760 --> 00:52:44.079
the candise, Sandra you doing.
I'm currently reading the latest John Birmingham series.
591
00:52:44.159 --> 00:52:47.320
Johnson, Oh yeah, an English
author, but he's Australian based and
592
00:52:47.440 --> 00:52:53.880
he's just released He always releases books
in threes. All his stories have three
593
00:52:54.079 --> 00:52:59.840
volumes, and I mean halfway through
the second of three books in his latest
594
00:53:00.000 --> 00:53:05.559
series, and it's a it's just
a classic outer space war story, which
595
00:53:05.639 --> 00:53:09.639
is he he hasn't done ones like
that before. He's done other really interesting
596
00:53:09.719 --> 00:53:15.400
stories about monsters coming out of other
dimensions and eating humans. And he did
597
00:53:15.480 --> 00:53:17.719
one about a big blob that came
from out of space and wiped out half
598
00:53:17.760 --> 00:53:22.920
of America and half of Canada and
what happened to the world. That one
599
00:53:22.039 --> 00:53:25.159
was called Without America. He writes
brilliantly, and I'm really enjoying this,
600
00:53:25.719 --> 00:53:31.199
this latest series, which is he
hasn't released the third book yet, but
601
00:53:31.239 --> 00:53:36.159
it's due out this year, so
I'm slowly reading the second one so I
602
00:53:36.199 --> 00:53:38.639
can get straight into the third one
when it comes out. It's great stuff.
603
00:53:40.960 --> 00:53:45.400
Once did a gig with him.
Oh did you in Brisbane? Yeah?
604
00:53:46.239 --> 00:53:51.000
Yeah? I love his writing style, really do. My favorite character
605
00:53:51.119 --> 00:53:55.960
of his is super Dave, Super
Dave. Yeah, and then that series
606
00:53:57.039 --> 00:54:01.320
has since been recalled renamed the Super
Day Series because it sort of took over.
607
00:54:02.840 --> 00:54:06.559
So we've got to look out for
the super dunk theory. Oh go
608
00:54:07.239 --> 00:54:13.559
superdum series. Enough. If you're
listening, John, this is it super
609
00:54:13.599 --> 00:54:16.320
dumply Yeah, yeah, yeah.
Give me put in a kind word to
610
00:54:16.400 --> 00:54:22.599
your publishers for me. That'd be
nice. That will never happen. All
611
00:54:22.719 --> 00:54:24.760
right, Thank you very much,
Martin. Always good to hear from you.
612
00:54:25.280 --> 00:54:28.039
We're going to wrap it up there, Fred, I think we got
613
00:54:28.079 --> 00:54:30.719
through a fair bit today. But
again i'll remind people, because we've now
614
00:54:30.800 --> 00:54:35.199
exhausted quite a few of our questions
to send them in via our website,
615
00:54:35.679 --> 00:54:38.679
Space nuts podcast dot com. Click
on the AMA link to send text or
616
00:54:38.679 --> 00:54:42.920
audio questions, or just click on
the tab on the right hand side of
617
00:54:42.960 --> 00:54:45.960
the homepage where you can send audio
questions. Don't forget to tell us who
618
00:54:46.000 --> 00:54:49.840
you are and where you're from.
You can record your questions via any device
619
00:54:49.920 --> 00:54:53.079
with a microphone. Basically, it's
that simple. And check out all the
620
00:54:53.119 --> 00:54:57.159
other stuff on the website while you're
there, Fred, thank you as always.
621
00:54:57.239 --> 00:54:59.800
It's a great pleasure, and yeah, it's good to get through some
622
00:54:59.840 --> 00:55:04.280
of the questions and hear from the
audience. Indeed, the top five or
623
00:55:04.360 --> 00:55:08.519
sence than we did sounds great.
Thanks Andrew, we'll see you next time.
624
00:55:08.599 --> 00:55:13.239
Indeed we will Fred Watson, astronomer
at large part of the team here
625
00:55:13.559 --> 00:55:16.400
at Space Nuts. And thanks to
Hugh in the studio who actually turned up
626
00:55:16.400 --> 00:55:21.320
for work today, and from me
Andred Hunkley, get you on the very
627
00:55:21.400 --> 00:55:25.639
next episode of Space Nuts. Bye
byepauts. You'll be listening to the Space
628
00:55:25.719 --> 00:55:35.039
Nuts podcast available at Apple Podcasts,
Google Podcasts, Spotify, iHeartRadio, or
629
00:55:35.119 --> 00:55:38.679
your favorite podcast player. You can
also stream on demand at bites dot com.
630
00:55:39.239 --> 00:55:44.199
This has been another quality podcast production
from nights dot com.
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