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This is geology, B. 
I'm all of us trampled. 

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People who study the Earth, have
an enormous advantage over those

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who study other celestial bodies
such as other planets and the 

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Stars. 
That's because we live on the 

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earth. 
So we can explore its surface at

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will sample and analyzes rocks. 
Listen to its earthquakes and 

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drill holes into it, to get at 
least a few miles below the 

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surface. 
So why would we want to look to 

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another planet or even to 
another solar system to help us 

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understand the Earth down? 
Mackenzie is Professor of Earth 

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Sciences at University, the best
known for discovering the theory

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of plate. 
Tectonics in the late 1960s. 

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He is also among many other 
subjects, made fundamental 

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contributions to our 
understanding of the Moon, Mars,

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and Venus Dan. 
Mackenzie welcome to geology B. 

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Thank you. 
I know one shouldn't really 

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attach labels to people but I 
think of you as an earth 

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scientist. 
So when you first turn your 

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attention to Venus, did you do 
that? 

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Because you are anyway, 
expanding your research beyond 

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the Earth. 
Or was it because you actually 

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thought Venus might offer us 
some Clues as to how things work

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here on Earth. 
My interest is being in 

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essentially how the rocky 
planets behave and if you work 

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on the earth who got one, you've
no idea how special and what 

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actually governs things here. 
And whether if you had another 

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rocky planet, whether it would 
look the same, it's always a 

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help to look at more than one 
thing that was really why I got 

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interested. 
I'd always been interested in 

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Venus, but the problem with 
Venus is that it's covered with 

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clouds made out of sulfuric acid
and these never clear. 

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So nobody had the slightest idea
before radar as to what was 

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underneath the clouds. 
So yes, we knew how big it was. 

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It's more or less the same size 
as the Earth, more or less, the 

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same mass of the Earth. 
And if the next plan is in, from

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the earth, towards the Sun. 
So it seemed really quite likely

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that We would learn something by
looking at Venus and that was 

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really why I applied to be an 
investigational Magellan 

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program, which was a spacecraft,
which would being sent to Venus.

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So, with Magellan, we finally 
could look under the clouds as 

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you say with radar and it was 
very successful at doing that, 

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the main purpose was to map the 
surface, but you had an idea 

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that we could do something else 
with the data that was sent back

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from the spacecraft. 
Once it was in orbit around 

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Venus, I was more interested In 
the interior of the planet. 

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Because on Earth, the plates are
moved by convective forces. 

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And what I wanted to know was 
whether the same things 

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happening on Venus and if so, we
could learn a lot about it 

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because we didn't really 
understand what actually 

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controlled the plate motions 
that we can see it all going on,

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but it was really quite strange 
notion that cats. 

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So Caps of the earth whose 
distance across is perhaps 

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10,000 kilometers like the 
Pacific. 

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Just to be clear. 
These spherical caps are the 

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plates of plate tectonics. 
Yes. 

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And the elastic part of these 
things is about 30 kilometers 

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thick, that these should 
actually move as rigid caps as 

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most extraordinary notion. 
We're all quite used to it now 

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because, you know, we can 
actually see that motion with 

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GPS with earthquakes and things,
but before we actually could see

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it. 
I mean, nobody really would have

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taken that seriously. 
So what actually controls what's

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going on that was what 
interested me is where the Venus

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was doing the same thing and if 
so could we learn about what was

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going on from essentially 
looking at the gravity field, 

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which is something that you get 
for free. 

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There goes base. 
Craft going around in orbit 

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around the planet, Venus 
undergoes the acceleration due 

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to gravity. 
But the gravity field of planets

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Venus of the earth is not just 
that of a point Mass, it 

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actually all the things like 
mountains and stuff or produce 

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gravity Fields. 
So you can learn the very great 

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deal about what's going on 
inside the planet by looking at 

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the gravity field, which is 
controlled by essentially 

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density variations inside the 
planet and that was what I hope 

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to be able to do. 
But the mountains on Earth and 

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on Venus are pretty small 
compared to the planets 

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themselves. 
So these must have been pretty A

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small fluctuations or they're 
not very big on Earth the few 

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parts in 100,000, there's a 
method by which you can actually

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track the spacecraft using 
Doppler and you can measure the 

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velocities of the spacecraft at 
the other side of the solar 

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system to a few tens of microns.
The second set is perhaps a foot

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an hour is about the source of 
be that you've measure. 

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And if you take the change with 
time, that tells you the 

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acceleration, In the direction 
which are looking so by using 

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this, which is actually how NASA
navigates it spacecraft. 

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So I didn't have to do anything 
special. 

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They were doing this anyway. 
You can actually see the gravity

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field of the planet directly as 
a sort of map from the way that 

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you're looking. 
And this was what really 

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interested me. 
But the problem was that when 

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they spacecraft was closest to 
Venus. 

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And so the most sensitive to its
gravity, it was making images of

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the surface only when it was far
away. 

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Was it actually pointing back to
the Earth. 

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And so, I had this frustrating 
business for the first, 

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something like two years and 
spacecraft. 

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You didn't measure any gravity 
at all and that was very 

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frustrating. 
I just had to live with this 

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hoping that the spacecraft would
not fail before. 

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Actually, it could do something,
which was my principal motive. 

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For being involved, 
unfortunately, the Imaging 

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failed, but we still have 
communications with it, so I 

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was. 
Alright. 

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So here we had a failure on the 
spacecraft. 

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That actually was a good thing 
for you, save me, but then 

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something else happened. 
It's of course, it costs 40 

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million dollars a year to keep 
the spacecraft running. 

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And once all the people who were
making images of the surface 

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when they're longer interested, 
then NASA of course its initial 

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reaction was To shut the 
spacecraft down but we persuaded

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them not to at least for a 
couple of years and then they 

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got finally. 
So frustrated, they used little 

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bit of fuel that was left to 
actually put the spacecraft into

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Venus, right? 
Destroy it and that stopped all 

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argument. 
How long did you actually have 

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then to make these measurements 
it takes in ass about 250 days 

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to rotate and the spacecraft 
will be. 

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It doesn't rotate. 
So you get one. 

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Look at Hope. 
About once every 250 days. 

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So the mapping took or I think 
about two years and that after 

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that we then got three Cycles 
looking at the gravity so it was

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a very slow business. 
So you said, you could measure 

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the speed of the spacecraft to 
enormous accuracy, using the 

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Doppler effect on the radio 
signal coming from the 

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spacecraft. 
But how does that tell you what?

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The gravity field is does it 
speed up a bit when the gravity 

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is a little bit stronger and 
slow down a bit when the gravity

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is a bit weak. 
Aker yes. 

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The gravity field is just the 
accelerations and that's the 

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gravity field at the satellite. 
So that's a straight measurement

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at the satellite. 
You just have to look at the 

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rate at which the velocity 
changes and that's the gravity 

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in the direction. 
You're looking. 

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It's not the gravity at the 
surface. 

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That's a more complicated thing 
is because it's a very 

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straightforward measurement. 
Trust direct from the Doppler 

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shift and that's what I actually
use the Doppler shift itself. 

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Okay, so you've got the gravity 
fluctuations. 

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Now, what did that tell you? 
What I did was to look at the 

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relationship between the gravity
and the shape of the plant, 

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that's about your fee. 
And what I was interested in was

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essentially, the thickness. 
What on Earth is the thickness 

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of the plates in Venus, there's 
a layer which essentially quite 

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strong and can support short, 
horizontal wavelength features. 

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So small mountains, there are 
completely supported by this 

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elastic layer. 
And when you look at the 

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gravity, there's things you Just
looking at the mass essentially 

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that would be short wavelength 
features just to interjection 

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explain a couple of things here.
Short wavelength, now means 

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special wavelength in other 
words, distance scales on the 

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surface. 
Nothing to do with the 

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wavelength of the Doppler signal
that you're listening to and by 

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elastic layer. 
You mean, even though it bends, 

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it's a rigid layer as opposed to
a mushy ductile layer. 

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That wouldn't hold anything up 
at all. 

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Yes, but Anyway, what we knew 
was that long wavelength 

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features, like for instance, too
bad, these are not supported 

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elastically except at their 
edges May float. 

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They're like icebergs floating 
in the mantle, the crust of the 

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earth that partner we're used to
has a lower density than the 

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interior. 
So, if you have a thick layer of

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the crust, it essentially, 
floats in the material below. 

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The gravity field from a 
floating object, It is nothing. 

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So, the topography then, is what
we call compensated, which means

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that it doesn't produce a 
gravity field and a changeover 

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from things which do produce 
gravity field to things, which 

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don't obviously tells you just 
like, you know, walking on ice. 

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You can tell how thick the ice 
is by how much it bends that 

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tells you the thickness of the 
elastic. 

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Learn this is what we wanted to 
get at. 

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What I wanted to look at was the
relationship of the How do you 

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feel to essentially the surface 
Topography of the planet? 

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Also an iceberg. 
Marooned on a totally rigid 

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plate and reaching the same 
height as the floating one. 

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In other words, with identical, 
topography will increase the 

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gravity because the whole of the
iceberg is so to speak extra 

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mass without any low density. 
Compensation below it and 

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Venus's plate will be somewhere 
in between and we're in between 

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it is Is what you're finding 
out. 

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Yes, it's not quite as simple as
that because there's also 

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another effect, which is that on
Earth, the mantle is is actually

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convicting, it's sufficiently 
fluid. 

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Its viscosity is low enough. 
That actually, there are regions

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where the mantle is coming up 
and going down just like putting

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water in a saucepan and boiling,
it. 

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And that also produces a gravity
field because it pushes the 

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surface where it's Me up. 
It pushes the surface up when 

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it's going down, it pushes the 
surface down. 

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Let me try and explain how this 
affects the gravity field. 

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If we think about a hot spot 
where the mantle is coming up, 

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the density, there is less than 
its surroundings because of 

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thermal expansion, that would 
have the effect of lowering the 

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gravity field above it. 
But as you said, it also pushes 

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up on the plate that lies above 
it, bending it. 

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So it bulges upward and the 
extra material, In the Bulge 

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increases the gravity. 
It turns out that this increase 

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outweighs the decrease from the 
lower density of the material 

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below with the net result that 
gravity increases by about a 

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third of what we would expect 
from the effect of the surface 

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bulge alone. 
So you have to have enough 

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information to be able to 
distinguish between these two 

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things. 
And the way in which you do that

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is that actually the signal, the
amount of gravity you get Km of 

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elevation is different in the 
two cases. 

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So that was what I wanted to get
at and that means essentially 

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working over a range of 
wavelengths and seeing where 

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changes from floating to being 
essentially supported 

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elastically and that we could do
and what we found, which 

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surprised me very much actually 
when we found it was that the 

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elastic layer on Venus is 230 
kilometers. 

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And that's the same as the 
thickness on Earth. 

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But only the thickest part of 
things on Earth are the thickest

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part on Earth is old oceanic 
plates. 

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And where the surface rocks are 
very old where there are more 

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than a thousand million years 
old underneath those, the plates

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of called, they've got strong, 
they got elastic and they are 

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also about 30 km thick, but the 
bottom of that layer, the 

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thickness of the ice. 
They're governed by the 

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temperature and the bottom of 
that left and both places is 

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about 450 degrees Centigrade. 
The surface temperature of Venus

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is about 420 degrees, Centigrade
so I not expected to see 

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anything like that. 
I hadn't expected Venus have any

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strength at all. 
Expected us to be looking at the

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convective signal from the 
mantle convection. 

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We could also see that clearly, 
but we could see both things but

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the The thing that really 
surprised me was how thick the 

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elastic level. 
So you are thinking that because

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Venus was so hot, the Rocks had 
to be so weak. 

231
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That really all the mountains 
would be sinking into the bottom

232
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and bit more like the floating 
icebergs situation or any rather

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than the rigid plate situation. 
Exactly. 

234
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We had no previous knowledge, 
you can already tell. 

235
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This, of course, if there are 
mountains on being as which is 

236
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supported by the convection, you
really need both the topography 

237
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and the gravity before you can 
tell. 

238
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That being pushed down by 
convective, circulation 

239
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underneath, or whether they're 
supported elastic key. 

240
00:14:13,200 --> 00:14:16,800
And once we got the gravity, we 
could see that very clearly. 

241
00:14:17,300 --> 00:14:20,000
So, how can such incredibly hot 
rocks? 

242
00:14:20,000 --> 00:14:24,800
Be so strong on Venus, that was 
the great surprise. 

243
00:14:24,800 --> 00:14:29,500
And that course, particularly 
David coasted in Minnesota. 

244
00:14:30,700 --> 00:14:35,500
To look at the role of water. 
We knew that quite small amounts

245
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of water in rocks, made them 
week. 

246
00:14:38,900 --> 00:14:42,100
But what he found was that 
really quite minut. 

247
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Amounts of water were important,
just simply transferring the 

248
00:14:46,700 --> 00:14:49,800
samples. 
He was going to test from the 

249
00:14:49,800 --> 00:14:54,200
oven in which they were dried to
The Apparition which was going 

250
00:14:54,200 --> 00:14:56,900
to test. 
They absorbed enough water from 

251
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the atmosphere just on that 
transfer. 

252
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To change their properties. 
And this we had really no idea 

253
00:15:04,000 --> 00:15:08,400
about before Venus. 
We know that the Earth has got 

254
00:15:08,900 --> 00:15:14,200
about 100 parts per million of 
water in the mantle and Dave 

255
00:15:14,200 --> 00:15:16,600
because it experiments 
particularly show that this is 

256
00:15:16,600 --> 00:15:21,500
quite enough to make it soft and
really very soft whereas Venus 

257
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because it's extremely hot and 
also its atmosphere is extremely

258
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dry if you would condense all 
the water in Venus's atmosphere,

259
00:15:30,400 --> 00:15:34,500
The sphere onto the surface, you
get oceans, which about 10 cm 

260
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thick. 
It's really as dry as a bone and

261
00:15:37,400 --> 00:15:40,800
it's very hot. 
So it's like they've caused it's

262
00:15:40,800 --> 00:15:46,100
often and that affects both the 
elastic properties and also the 

263
00:15:46,100 --> 00:15:51,500
viscosity of the correcting 
mantle and that then really 

264
00:15:51,600 --> 00:15:54,600
solve the problem. 
But we had previously really no 

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idea that is very small amount 
of water on Earth in the mantle 

266
00:16:00,100 --> 00:16:02,800
play. 
Important role particularly in 

267
00:16:02,800 --> 00:16:05,900
plate tectonics. 
Then when we looked at Venus 

268
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most of the planet is absolutely
not like the Earth. 

269
00:16:11,300 --> 00:16:14,300
It is not covered with moving 
plates. 

270
00:16:15,000 --> 00:16:19,300
There are a few places on the 
planet, which do look quite like

271
00:16:19,300 --> 00:16:22,900
some of the features on plate 
boundaries, but most of the 

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00:16:22,900 --> 00:16:25,900
planet is not like that at all. 
It's just covered with lava 

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flows. 
It's essentially a one plate 

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00:16:27,900 --> 00:16:30,600
planet. 
Now, as far as we can tell, Ow. 

275
00:16:31,200 --> 00:16:34,500
And for me a justification for 
looking at another planet, we 

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00:16:34,500 --> 00:16:38,000
had no idea that water was so 
important. 

277
00:16:38,600 --> 00:16:42,700
That's fascinating that by 
looking at Venus and seeing how 

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00:16:42,900 --> 00:16:46,200
dry it was and how different it 
behave from the earth that 

279
00:16:46,600 --> 00:16:49,700
really made us look again at the
importance of water on Mars, 

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00:16:49,700 --> 00:16:52,900
even though we already knew how 
much water there was in the 

281
00:16:52,900 --> 00:16:55,500
rocks on Earth, we just didn't 
understand its significance. 

282
00:16:56,200 --> 00:16:59,700
We hadn't really thought that 
such small amounts of water 

283
00:16:59,700 --> 00:17:03,100
could matter. 
Or that the experiments that we 

284
00:17:03,100 --> 00:17:07,000
were doing, which we thought 
were dry, not actually, as dry, 

285
00:17:07,000 --> 00:17:10,000
as we thought they were this 
mattered. 

286
00:17:10,300 --> 00:17:16,000
I mean, yeah, it's a very nice 
illustration of how you need 

287
00:17:16,200 --> 00:17:20,700
both the observations from The 
Real World. 

288
00:17:20,700 --> 00:17:24,000
And also, then to do lab 
experiments properly, control 

289
00:17:24,000 --> 00:17:26,200
lab experiments to see what's 
going on. 

290
00:17:26,599 --> 00:17:29,800
And that was really, a very nice
illustration of the importance 

291
00:17:29,800 --> 00:17:32,300
of both. 
'The, I'm struck that since you 

292
00:17:32,300 --> 00:17:35,400
found out that even a tiny 
amount of water can make rock 

293
00:17:35,400 --> 00:17:37,800
softer. 
It's all the more surprising 

294
00:17:37,800 --> 00:17:41,200
that on Earth, the spherical 
caps, which you referred to 

295
00:17:41,200 --> 00:17:46,300
earlier, which can be 10,000 km 
wide move about as rigid plates.

296
00:17:46,800 --> 00:17:52,200
Well, yeah, that was why they 
took such a long time for 

297
00:17:52,200 --> 00:17:55,500
Georgia's to recognize, but 
plate motions on Earth. 

298
00:17:55,800 --> 00:18:00,000
And I mean, this, this sort of 
behavior is really only true for

299
00:18:00,000 --> 00:18:02,600
the As she anak awesome. 
The plates conscience. 

300
00:18:02,600 --> 00:18:05,600
Deform like entering and much 
more distributed. 

301
00:18:05,700 --> 00:18:08,900
If you look at a map of 
earthquakes from Northern India 

302
00:18:09,600 --> 00:18:13,200
2000 km North from the whole of 
that region is deforming. 

303
00:18:13,800 --> 00:18:16,600
And in the oceans that's 
absolutely not the case. 

304
00:18:16,600 --> 00:18:18,800
The plate. 
Boundary beneath Japan is really

305
00:18:18,800 --> 00:18:21,000
sharp. 
It's just one big fault which 

306
00:18:21,000 --> 00:18:23,300
moves in the Japanese 
earthquake. 

307
00:18:23,400 --> 00:18:26,900
It moves, 70 meters. 
Now the really isn't anything 

308
00:18:26,900 --> 00:18:30,200
like that on the continents. 
It was really only there. 

309
00:18:30,300 --> 00:18:34,000
Suppression of the oceans, which
showed what was going on. 

310
00:18:34,000 --> 00:18:37,500
And once we had a good 
understanding of that, we then 

311
00:18:37,500 --> 00:18:40,400
could go back to the contents 
and see what was going on. 

312
00:18:40,600 --> 00:18:43,600
And of course, GPS, we knew what
was going on really from 

313
00:18:43,600 --> 00:18:48,400
earthquake and from magnetic 
anomalies in the oceans but any 

314
00:18:48,400 --> 00:18:51,300
remaining doubts were completely
squashed by the GPS 

315
00:18:51,300 --> 00:18:55,300
measurements, much easier to do 
GPS on land, and it's just to do

316
00:18:55,300 --> 00:18:58,900
it at Sea and that's being done 
all over the world's continents 

317
00:18:58,900 --> 00:19:01,700
and confirmed. 
Absolutely everything that we 

318
00:19:01,700 --> 00:19:05,300
thought was the case from the 
earthquakes for my last 

319
00:19:05,300 --> 00:19:07,000
question. 
I want to come back to your 

320
00:19:07,000 --> 00:19:10,100
point that we had to look at 
another planet to get a better 

321
00:19:10,100 --> 00:19:13,700
perspective on our own and the 
fact that we're advancing by 

322
00:19:13,700 --> 00:19:16,800
Leaps and Bounds. 
Now in our ability to look at 

323
00:19:16,800 --> 00:19:21,100
planets around other stars, in 
fact we found over 4,000 of them

324
00:19:21,100 --> 00:19:22,700
and the numbers increasing 
rapidly. 

325
00:19:23,700 --> 00:19:25,700
I'm wondering if you think 
that's going to help us 

326
00:19:25,700 --> 00:19:28,800
understand more about the Earth 
and how it got to be where it is

327
00:19:28,800 --> 00:19:31,200
in our solar system. 
I'm sure. 

328
00:19:31,300 --> 00:19:35,500
Well up until discovery of all 
these exoplanets, we only really

329
00:19:35,500 --> 00:19:40,700
had one solar system to look at.
And furthermore, the things that

330
00:19:40,700 --> 00:19:43,700
happened which formed it 
happened. 

331
00:19:43,700 --> 00:19:47,600
Four and a half thousand million
years ago and the events are 

332
00:19:47,600 --> 00:19:50,300
clearly very strange. 
There's a lot of very odd 

333
00:19:50,300 --> 00:19:52,600
things. 
One of the ones which is very 

334
00:19:52,600 --> 00:19:56,200
simple State is a lot of 
meteorites, the rocky 

335
00:19:56,200 --> 00:20:02,200
meteorites, contain these small 
spheres of rock which is 

336
00:20:02,400 --> 00:20:06,600
actually mostly Olivine, which 
is the same composition as the 

337
00:20:06,600 --> 00:20:09,300
Earth and these things have 
obviously been molten. 

338
00:20:10,100 --> 00:20:13,400
That's very cool because of 
surface tension, they're all 

339
00:20:13,400 --> 00:20:15,500
mixed up. 
There are some extremely high 

340
00:20:15,500 --> 00:20:19,200
temperature once a much lower 
temperature ones and the Matrix,

341
00:20:19,400 --> 00:20:23,800
a lot of it is Clay. 
Its it contains water so So how 

342
00:20:23,800 --> 00:20:26,800
in the world are these things 
formed and how they put 

343
00:20:26,800 --> 00:20:29,300
together, the composition of the
earth. 

344
00:20:29,400 --> 00:20:35,300
Looks like essentially one set 
of these meteorites and we have 

345
00:20:35,300 --> 00:20:38,600
a whole lot of really, quite 
speculative theories about this 

346
00:20:38,900 --> 00:20:43,400
but we've daily, don't know. 
And that the whole process is go

347
00:20:43,400 --> 00:20:47,600
on as a star forms, rather hard 
to image. 

348
00:20:47,600 --> 00:20:52,400
That is a long way away in 
clouds of dust and they form a 

349
00:20:52,408 --> 00:20:54,600
great variety. 
Of different sizes. 

350
00:20:54,600 --> 00:20:58,500
And during the formation of 
these stars and their planetary 

351
00:20:58,500 --> 00:21:03,800
systems, the big ones evolved 
very fast explode and do a lot 

352
00:21:03,800 --> 00:21:07,500
of radioactive material, which 
we can see in the meteorites 

353
00:21:07,500 --> 00:21:11,700
that when they were formed, 
certain of the elements were 

354
00:21:11,700 --> 00:21:14,500
extremely radioactive and then 
they decayed. 

355
00:21:15,100 --> 00:21:20,100
We only really understood that 
once we saw how stars, formed in

356
00:21:20,100 --> 00:21:24,300
these clouds, and I'm quite sure
the same scheme to Be true of 

357
00:21:24,300 --> 00:21:28,000
all the rest of how the solar 
system was put together once we 

358
00:21:28,000 --> 00:21:32,600
can image these remote ones that
we've now discovered. 

359
00:21:32,900 --> 00:21:35,800
But yeah, technology is 
marvelous. 

360
00:21:35,900 --> 00:21:41,300
It just Marches On and all kinds
of things will become possible 

361
00:21:41,500 --> 00:21:45,100
in the not very distant future 
and I'm quite sure there are 

362
00:21:45,100 --> 00:21:47,400
lots of them. 
We're going to find some, which 

363
00:21:47,400 --> 00:21:51,600
are forming now and that will be
an enormous help to 

364
00:21:51,600 --> 00:21:56,600
understanding how Solar system 
got put together because the 

365
00:21:56,600 --> 00:22:00,900
problem is we don't even know 
how common solar system like 

366
00:22:00,900 --> 00:22:04,300
ours is because we live on this 
one. 

367
00:22:04,900 --> 00:22:09,100
We know that we need water to 
live and all the rest of it. 

368
00:22:09,600 --> 00:22:12,500
How common is that? 
We don't know if it wasn't like 

369
00:22:12,500 --> 00:22:16,300
that, we wouldn't be here to 
look be looking at it so that 

370
00:22:16,300 --> 00:22:19,900
extremely difficult to know how 
to attack problems and this 

371
00:22:20,300 --> 00:22:23,700
especially when there is 
complicated as this and one of 

372
00:22:23,700 --> 00:22:28,100
the things which has really come
from looking at the planets of 

373
00:22:28,300 --> 00:22:30,800
this solar system is 
particularly come from their 

374
00:22:30,800 --> 00:22:34,400
satellites and they're all 
different. 

375
00:22:34,500 --> 00:22:39,500
They just extraordinary variety 
and quite astonishing that they 

376
00:22:39,500 --> 00:22:41,800
look as different as they are. 
We don't know much about the 

377
00:22:41,800 --> 00:22:46,000
insides yet most of them anyway 
but they are quite different 

378
00:22:46,000 --> 00:22:49,400
from each other and so 
presumably the same is going to 

379
00:22:49,400 --> 00:22:52,700
be true of solar systems that 
they're going to be completely 

380
00:22:52,700 --> 00:22:54,300
variable. 
Not set me. 

381
00:22:54,300 --> 00:22:57,300
What's coming out from the 
little bit of knowledge that we 

382
00:22:57,300 --> 00:22:59,900
have of them so far. 
Definitely going to do another 

383
00:22:59,900 --> 00:23:01,800
podcast with you. 
When we have enough data on 

384
00:23:01,800 --> 00:23:04,100
these new solar systems will be 
dead. 

385
00:23:08,400 --> 00:23:10,700
Dan Mackenzie. 
Thank you very much. 

386
00:23:11,000 --> 00:23:11,500
Good.
