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[Andy Freeberg] I'm here with Rich Vondrak, the Project Scientist for LRO
and Rich you're going to explain to me a little bit about the LRO spacecraft and tell me what this is gonna do here?
[Rich Vondrak] Okay
[Andy] So this is LRO in all it's deployed glory right?
This kind of square shape is to fit a lot inside right?
[Rich] That's right, the inside here is a large propulsion tank.
The LRO spacecraft with fuel weighs about 2 tons
but the spacecraft without the fuel, before it's fueled, weighs only about one ton.
So it's like having an automobile where your automobile has as much
gasoline in it as the whole weight of your car.
And we need that in order to stay in orbit.
We also have an adjustable high-gain antenna system
that's always pointed at the Earth, to take the measurements we make
and send them back to Earth so that
they can be analyzed by the scientist on the mission.
[Andy] And that can send a lot of data back with this one right here right?
[Rich] An awful lot of data, much more than any planetary mission has ever returned before.
[Andy] Okay so how about if I say I'm building my map of the Moon and you explain how you're doing it. All right so,
the first thing I'm going to want with a map is I'm going to want pictures. I'm going to want images of the Moon.
[Rich] That's right.
[Andy] So what on LRO is going to be able to do that?
[Rich] We have a camera system, called the LRO Camera or LROC.
It has two very high resolution
cameras so objects that are the size of this table
or this big, can be detected.
[Andy] Or maybe a lunar rover for example?
[Rich] A lunar rover, we expect that when we go over the Apollo sites we'll be able to
image the lunar module, the lunar rovers, see the tracks the
astronauts left as they disturbed the surface.
[Andy] So now we sort of have some images, but I want to know kind of
in three dimensions what this looks like. What am I looking at for sure, is it a hill or is it a valley?
[Rich] That's right, what we lack now is an accurate
topographic map of the Moon. With LRO
we have a laser altimeter system so every second we'll
have 140 spots deposited on the surface, it'll measure the return
with this system and then measure the distance to the surface
the roughness of the surface, and by looking at the five spots
together we'll know the tilt of the surface.
[Andy] Those are two sort of basic, tangible ones, but you're going to want to know
temperatures, I think that's a big deal on the Moon right?
[Rich] Yes, because the Moon goes through
large temperature variations, unlike the Earth where our atmosphere
redistributes the temperature variations
so that we don't have large temperature variations like you do on the Moon
Also, some places on the Moon we think are shadowed
from sunlight, so they get very cold.
So we want to measure temperatures around the Moon. To do that we have
this instrument at the top called the Diviner
experiment. By looking at the day/night variations we can understand
what the surface properties are and understand
parameters like rock abundance, you know, whether it's a smooth, hard soil
or whether it's rubbly like gravel. A surface texture that you cannot see
with the imager even at 50 centimeters.
[Andy] Right so a sandy area, when it goes from day to night, will change temperature differently than a rocky area when it goes from day to night.
[Rich] Right. The heating and cooling runs at different rates depending on the surface characteristics.
[Andy] Interesting.
[Rich] We also have a UV-spectrometer called LAMP.
And this instrument will use starlight to
image the dark regions where the Sun doesn't shine.
And by looking at the reflectivity of
the starlight and ultraviolet it can tell whether there's water frost on the surface or not.
[Andy] So that kind of does a lot of the mapping, is there anything in particular
can you talk about the one we missed that's kind of a more unique type of camera?
[Rich] Right, we have here at the bottom this large instrument, which is
the neutron detector. It's call LEND,
for Lunar Exploration Neutron Detector, and it's being
supplied by Russia and in regions where we think there is water
the hydrogen associated with the water will
cause the neutron flux to decrease. So LEND will
search for these regions where there's decreased neutron flux
in order to measure hydrogen abundance.
[Andy] So we're missing one big one, this whole big brown thing right here.
Can you explain to me what that is?
[Rich] Yeah, that one was added late in the mission.
And what it is an advanced radar system. What this system
will do, it will send radio waves to the surface and measure the reflection
of the surface in radio waves and it uses several
techniques to see if there's the signature, first of all of surface roughness,
and then also to see if there's some unique signatures associated with buried water ice.
on the lunar surface.
[Andy] All right, well thank you very much for showing this to me, we'll look forward to
seeing what it starts sending back once we get it into orbit.
[Rich] We're ready to go and enthusiastic to look at the data.
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