WEBVTT
Kind: captions
Language: en-US

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[Please stand by for realtime captions.] &gt;&gt; Good
evening everyone and thank you for coming

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to the USGS [Indiscernible - speaker too far
from the microphone] my name is [Indiscernible

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name] and thank you again for coming. Tonight
I have the pleasure of having Justin Haggerty

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from the USGS aster geology partner and Dr.
Haggerty 419 98, 2001, University of New Mexico

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and Dr. Harry joined USGS in four [Indiscernible
- speaker too far from the microphone] and

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focused on the composition of information
[Indiscernible - muffled] the geologic evolution

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of [Indiscernible - muffled] presidential
early career awards

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in 2012 [Indiscernible - muffled] information
and evolution of [Indiscernible - muffled].

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He is now the director of the USGS geology
center and to support the geological findings

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USGS geology [Indiscernible - speaker too
far from the microphone] in the general public's

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pursuit innovative and [Indiscernible - muffled].

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[Applause]

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Hello everybody . Amazing turnout thank you
for coming out tonight. I'm excited to get

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this presentation for a lot of reasons tonight.
First and foremost this is my first trip to

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Menlo Park I know that there is a little bit
of a transition going on with Menlo right

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now but I'm excited to have the opportunity
to be here tonight. I'm also excited by the

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fact that many of you may know that aster
geology actually had its first beginning here

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in Menlo Park and Jane Shoemaker the founder
of astro geology first started with this concept

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of astro geology in the early 60s here reporting
at this center of operations in Arizona. Another

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Reno the reason I'm doing this presentation
tonight is that within even the USGS whenever

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I travel to all of the different centers it
is everybody knows about astro geology which

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is really interesting is my opportunity to
tell all of you about who we are and what

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we do and where we came from and what we're
doing now in the work we're doing in the future

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and it is my goal by the end of this presentation
that you see why I'm so excited to be a part

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of astrogeology to be part of the legacy and
to have the opportunity to work with so many

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incredibly talented people courting incredible
work and as a matter fact I think online tonight

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we have several folks from the center who
are joining us and everybody in flight staff

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and thank you for joining us. You probably
heard already I use the phrase astrogeology

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several times and it's interesting this cannot
as aster apology. Aster apology. We actually

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-- [Indiscernible - muffled] so we will talk
more about the work that we do in astrogeology.

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I want to start off with talking a little
bit about our founder Dr. Shoemaker who again

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basically started the field of astrogeology
and let me ask a question before I go much

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further. How many of you actually know the
meaning of the word astrogeology with a show

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of hands really quickly. About five years
ago it sounded interesting but where does

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it mean and where does it come from and [Indiscernible
- muffled] origin

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for the training of the Apollo astronaut.
That's something that they have as a provision

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was to work very closely with NASA to make
sure we can train and unfortunately due to

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a medical condition he was not able to become
an astronaut so he wanted to make sure that

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he could do the next best thing which is to
train people that were going to go there so

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that basically
they wanted to make sure that people could

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go would be [Indiscernible - muffled] and
another defining characteristic [Indiscernible

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- muffled] ideas making sure everybody's on
board and I have never had the opportunity

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to meet Dr. -- but I've heard many stories
about how of a visionary he was and the pursuit

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that he engaged in. I was fortunate enough
to meet his colleagues and his wife, Carolyn

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Shoemaker and [Indiscernible - muffled] which
is really important thing to have the fact

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that not only was he able to do that but he
was able to inspire and engage individuals

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for the vision to be implemented and I think
we have a long-standing sentiment to that

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quality of having astrogeology continue to
be here many years after its foundation. Many

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people tend to ask why would Jean actually
want to go all the way out to [Indiscernible

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- muffled] in the middle of nowhere to actually
do that kind of research . There is a variety

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of reasons for the main reason is there is
a variety what we call terrestrial analog

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in the air and what I mean by that is if there
is a geologic process that we can investigate

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in detail here and we suspect that those processes
are active or present if we can understand

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them very well here and when we observe them
on the planet we make sure that we can use

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our knowledge from here and make inferences
about those features may have been formed

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and evolved in other planetary surfaces. An
example is [Indiscernible - muffled] there

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is other features similar to that solar system
and more importantly when Jean was looking

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in Arizona in addition to being one of the
most gorgeous features in the world he understood

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that the Grand Canyon represented one of those
features that maintain a record of a variety

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of geological processes. As such it was important
when he brought the astronauts out to bring

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them to places like the ring Canyon so they
can see for themselves that record of geologic

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processes and what they look like and understand
how they form and train the fundamentals on

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geologic processes. Another reason why Arizona
was of interest was because of the crater,

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east of Arizona located in [Indiscernible]
this is a feature that was initially thought

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to be volcanic and Jean had a role in helping
to define that this was actually produced

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by a large-scale [Indiscernible] so in addition
to finding things like Ira Nichols and factors

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[Indiscernible - muffled] near the crater
Jean also found evidence of a rare mineral

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that at the time it was thought to be produced
only in the high pressure high energy environment

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that could only be impacted by what we see
in the crater. Understanding that this is

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preserved impact crater on the earth located
next to some of these other geological features

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you can actually go there and see the processes
and understand how important the process like

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this is because if you look at other planet
[Indiscernible - muffled] water erosion impact

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craters are in massive important process for
the entirety of the solar system and we have

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the best preserved ones here and right outside
our back door it's really important for us

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to go there and understand it and make implications
for other type features on [Indiscernible

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- muffled]. &gt;&gt; [Indiscernible - muffled] you
see a variety of other geological panic features

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and this is a really important volcanic [Indiscernible]
from the perspective it shows a wide variety

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of volcanic types and compositions and as
you start to look at it a lot of the flow

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features look very reminiscent of the salt
and fleecy another planet including [Indiscernible

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- muffled] so provide a great opportunity
to show the astronauts what well-preserved

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features look like in the way they understand
that and they take that knowledge and apply

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it to other surfaces on places like the [Indiscernible
- muffled] so for example your start to look

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at some of these features in detail and compare
them to what you see on the [Indiscernible

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- muffled] you can see fascinating comparisons.
When the astronauts were able to get to the

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lunar surface they medially started to see
a lot of those features again that they saw

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while they were in northern Arizona and a
variety of volcanic activity so they were

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well prepared after going to the training
in northern Arizona to make inferences about

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what these features were and why they were
important for the human revolution. Many of

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you recognize the footprint from the Apollo
astronauts. The footprint represents quite

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a few things. It represents the vision, it
represents the work by many many people and

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thankfully astrogeology was in large part
of helping to get that footprint on the surface

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of the moon and in particular some of the
things we assisted with were helping to testing

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of the Apollo astronauts as well as tools
. We also helped to identify and characterize

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and [Indiscernible - muffled] for the Apollo
astronauts and we also participate in something

00:13:11.369 --> 00:13:16.129
known as [Indiscernible - muffled]. What that
means is as you collect information about

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the things that are there you want to find
out tasks for where the us nuts are going

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to go so they can make the most observations
and the thing we are most known for is training

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the Apollo astronauts. So the training could
be done anywhere and much of that training

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was actually done by the space Center in Houston,
Texas. It became clear that they want to make

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sure that they [Indiscernible - muffled] everything
and environmental similar to what they could

00:14:00.230 --> 00:14:05.129
possibly get and you have seen the surface
in northern Arizona is similar to that. So

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they tested the terrains and areas that had
the Sultan materials and because of that they

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were able to fully test all of these things
before they got to the moon and they were

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assured that this would operate the tools
would operate efficiently. Over on the right

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we have Apollo 17 astronaut Dr. Eric Jack
Schmidt who is also a geologist and the reason

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I we're showing this image is because it represents
a unique thing that is now commonplace in

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terms of mission operation and it was used
basically with a television camera and television

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at that time was novel technology and there
were some people thought it should not be

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used or would not be used as part of the Apollo
program. But during the training of the astronauts

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in northern Arizona it was found that the
it was critical that the television cameras

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could be held while the astronauts is conducting
activities so the experts could say don't

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go there, you should go here, something like
that. Because of that the it really helped

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them to determine that they needed to have
that technology . As I mentioned in northern

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Arizona is a fantastic analog in a way however,
we do have the [Indiscernible - muffled] relatively

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large to us but we did not have an area where
it represented large amounts of craters in

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close proximity to each other so when you
look at this portion of the moon there about

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the same size of the area you can see here
a little dense coverage but we wanted to make

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sure we have something to try and help the
astronauts train in an environment like that

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and I can't imagine how something like that
would have been. [Indiscernible - muffled]

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they took an image of that from Oracle mission
to the Apollo and try to reproduce that as

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closely as they possibly could and logistically
trying to see how it will be for the astronauts

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to weave in and out of these craters and also
in doing that it gave them some insight into

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what the craters actually tell us about services.
[Indiscernible - muffled] ratio and also understanding

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the relationship of the crater to one another
and how they interoperate to tell a story

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about the surface history. If you want one
comparison of an overlay of [Indiscernible

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- muffled] it is a perfect match. There able
to take that information again do some training

00:17:33.160 --> 00:17:34.160
with the astronauts while they were here so
perhaps more importantly help us understand

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those relationships spatially and horizontally
and vertically to one another such that we

00:17:37.130 --> 00:17:42.290
can [Indiscernible - muffled] first geologic
map of the planetary [Indiscernible - muffled]

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so this is the Apollo mission and geologic
maps for all missions based on these relationships

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and their absolutely fascinating. I mentioned
that first finding was more in detail but

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here is the [Indiscernible - muffled] ended
up not going very far it was quite a miracle

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to actually get that at all but what they
did is help them understand where they wanted

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to go to makes observations and collect additional
samples. Perhaps most importantly the thing

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we were involved in was the astronauts training
and one thing that many people may not be

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aware of is outside of [Indiscernible - muffled]
the majority of the Apollo astronauts were

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[Indiscernible - muffled] and well there were
certainly exceptional and intelligent not

00:18:34.600 --> 00:18:40.990
all of that not all of them had background
in geology so they had to take a crash course

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to understand what the geologic principles
were so they can basically be the version

00:18:48.470 --> 00:18:52.490
of Dr. Shoemaker while they were out there
making sure that they collect the samples

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that they needed to collect. So Jean along
with the colleagues throughout USGS, NASA

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and other institutions altogether decided
that they were going to put together a program

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of study for those astronauts and they would
take them to other locations I showed you

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earlier, the Grand Canyon, [Indiscernible
- muffled] to help train them in basic fundamentals

00:19:15.169 --> 00:19:22.760
of geology so when they went to the moon they
could make key observations. The Apollo 14

00:19:22.760 --> 00:19:27.169
the astronauts were getting really really
good at making these observations and collecting

00:19:27.169 --> 00:19:32.940
samples and it became apparent that they needed
to go further to make more observations. So

00:19:32.940 --> 00:19:38.090
the decision was made to come up with rover
allowed the astronauts to travel greater distances

00:19:38.090 --> 00:19:46.510
to find new discoveries and collect more [Indiscernible
- muffled]. In order to be prepared for was

00:19:46.510 --> 00:19:52.490
to have enrolled they want to make sure they
have the training and astrogeology [Indiscernible

00:19:52.490 --> 00:19:58.139
- muffled] deciding to build what you see
her rover geological [Indiscernible - muffled]

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a budget of about $1900 to put this thing
together which is about $16,000 of today's

00:20:06.799 --> 00:20:14.490
money which is still pretty [Indiscernible
- muffled] so they put the astronauts on this

00:20:14.490 --> 00:20:21.130
vehicle and it turned 90 degrees relative
to the front and rear and you can get into

00:20:21.130 --> 00:20:26.630
a lot of really interesting
places. So they are able to train on that

00:20:26.630 --> 00:20:32.549
before the end up going to the moon. Here
is the version that did get sent looks like

00:20:32.549 --> 00:20:39.320
and if you're interested in seeing what over
looks like we still have the actual one in

00:20:39.320 --> 00:20:46.870
our lobby suddenly encourage everyone to check
that out. This is the one that again they

00:20:46.870 --> 00:20:53.820
used on the moon and it's actually very [Indiscernible
- muffled] with the exception of the tires

00:20:53.820 --> 00:20:59.039
we don't have pressurized wheels but other
than that everything is functioning the same

00:20:59.039 --> 00:21:07.279
so after hearing when the Apollo astronauts
came back lessons learned they continuously

00:21:07.279 --> 00:21:14.490
cited their experiences in Arizona and the
things they learned, resources and education

00:21:14.490 --> 00:21:18.600
and they found out that more often than not
that they learn a lot from things that did

00:21:18.600 --> 00:21:23.750
not go right and during training in Arizona
a lot of it did not go right and they had

00:21:23.750 --> 00:21:29.480
to come up with new ways of doing things so
they could continue with the mission and that

00:21:29.480 --> 00:21:35.171
actually came into being pretty handy later
in the expedition where [Indiscernible - muffled]

00:21:35.171 --> 00:21:48.169
one of them actually broke loose and
[Indiscernible - muffled] regular soil of

00:21:48.169 --> 00:21:56.380
the region around the rover getting into all
the rover pieces and [Indiscernible - muffled]

00:21:56.380 --> 00:22:01.110
the astronauts themselves it actually became
quite dangerous so USGS had to come to the

00:22:01.110 --> 00:22:11.420
rescue one more time and they had to make
a geologic map that we gave them an actually

00:22:11.420 --> 00:22:18.799
[Indiscernible - muffled] and that's perfectly
fine because it helps them come up with a

00:22:18.799 --> 00:22:27.710
greater solution. One of the things that I
will notice possibly an urban legend but interesting

00:22:27.710 --> 00:22:35.120
and fun story to tell so [Indiscernible - muffled]
he was one of the [Indiscernible] focus during

00:22:35.120 --> 00:22:39.659
Apollo 17 and he liked to tell a story that
Jack Schmidt was coming back on one of the

00:22:39.659 --> 00:22:46.679
[Indiscernible - muffled] rover and as he
was coming back he had to look up to decide

00:22:46.679 --> 00:22:53.210
any thought he saw this really interesting
color and he said that's amazing I would love

00:22:53.210 --> 00:23:00.009
to get a sample of that. He radioed back down
and said hey, I think I found something and

00:23:00.009 --> 00:23:04.429
no, your resources are low we have to get
back to [Indiscernible - muffled] and he said

00:23:04.429 --> 00:23:14.700
he had a mechanical failure [Indiscernible
- muffled] wrap the sample and brought one

00:23:14.700 --> 00:23:17.220
back. Turns that additional cameras were [Indiscernible
- muffled] but it turns out that these samples

00:23:17.220 --> 00:23:20.519
these beads are very different colors but
some of the samples collected actually was

00:23:20.519 --> 00:23:23.320
exceptionally [Indiscernible - muffled] for
our understanding and further analyses within

00:23:23.320 --> 00:23:27.059
the past 10 years has shown us that these
beads are [Indiscernible - muffled] and some

00:23:27.059 --> 00:23:32.680
of the collections of the unique samples that
were able to be identified with some of the

00:23:32.680 --> 00:23:40.269
training that they had to let to collect these
fascinating samples that tell us a lot more

00:23:40.269 --> 00:23:46.190
about the moon that we would not have had
the samples not been collected. Another exciting

00:23:46.190 --> 00:23:51.299
time in our history and a history of Astra
geology as well but as things started to come

00:23:51.299 --> 00:23:55.770
to an end
thanks to some of the collections of these

00:23:55.770 --> 00:23:59.840
unique samples that were able to be identified
by somebody who is looking out to them because

00:23:59.840 --> 00:24:04.110
of some of the training they had they were
able to collect these fascinating samples

00:24:04.110 --> 00:24:10.110
that tell us a lot more about them had we
not had those samples collected. That was

00:24:10.110 --> 00:24:16.330
an exciting time in our history not only NASA
history but the country's history of the world's

00:24:16.330 --> 00:24:21.570
history and astrogeology but as things started
to come to an end: budget started to decline

00:24:21.570 --> 00:24:27.000
and got a little bit scary for everyone and
everyone said okay, what's next? It was not

00:24:27.000 --> 00:24:31.759
clear what the next plan was going to be and
if astrogeology is going to survive so thankfully

00:24:31.759 --> 00:24:39.070
some of the center directors who came before
me had a vision to say we may not be doing

00:24:39.070 --> 00:24:43.409
them anymore NASA still has a plan we need
to make sure that we can do whatever we can

00:24:43.409 --> 00:24:48.630
to support Nassau to the best of our abilities
regardless where they go. Since that time

00:24:48.630 --> 00:24:56.600
we have been involved pretty much every successful
active mission to the solar system and my

00:24:56.600 --> 00:25:02.809
precursor science center director one of his
favorite things to say was

00:25:02.809 --> 00:25:08.649
USGS has been involved in every successful
mission all of the ones that were not successful

00:25:08.649 --> 00:25:14.850
we were not involved in so just letting you
know that if you want to have a successful

00:25:14.850 --> 00:25:19.950
mission make sure we are involved. Since that
time we have been involved with everything

00:25:19.950 --> 00:25:24.159
missions to Mercury, the inner solar system
in creating this beautiful mosaic you see

00:25:24.159 --> 00:25:28.240
here and going all the way out to the outer
reaches of the solar system to Pluto again

00:25:28.240 --> 00:25:35.340
and the mosaic involved in here and moon and
Mars clearly important that we have people

00:25:35.340 --> 00:25:41.630
in all aspects of the solar system. One of
the things that's really interesting is that

00:25:41.630 --> 00:25:47.279
we also made a conscious decision to broaden
the level of experience and depth of expense

00:25:47.279 --> 00:25:51.640
in our workforce and a lot of people what
they seem to think when we say that we do

00:25:51.640 --> 00:25:56.179
planetary science they think it's an exclusive
field, that's a really unique expertise and

00:25:56.179 --> 00:26:00.399
it turns out planetary science is far more
than that. It is all of these different things

00:26:00.399 --> 00:26:05.480
combined so we have been able to build a workforce
over the years and up to today where we have

00:26:05.480 --> 00:26:09.710
people who do all of these different things
that we come together as a team to do some

00:26:09.710 --> 00:26:15.570
really fascinating work to make sure we can
explore the entirety of the solar system.

00:26:15.570 --> 00:26:22.320
What you see here is our business model for
how we are now the orders of NASA in terms

00:26:22.320 --> 00:26:27.759
of supporting the like lifecycle of planetary
spacecraft missions and it's an endless loop

00:26:27.759 --> 00:26:32.450
where you start with research operations as
a scientist,

00:26:32.450 --> 00:26:36.830
they have data and to make an observation
and generate new knowledge and new questions

00:26:36.830 --> 00:26:41.130
and those new questions then need an answer
and they can be answered to development of

00:26:41.130 --> 00:26:45.140
instruments and missions that can then go
to planetary bodies and make observations

00:26:45.140 --> 00:26:50.799
to help answer those questions. Once the data
are collected from those missions something

00:26:50.799 --> 00:26:56.879
needs to be done with that data raw planetary
spacecraft data needs a lot of work for it

00:26:56.879 --> 00:27:03.679
to be useful to scientists and make interpretations.
What you can see here is we go then to the

00:27:03.679 --> 00:27:07.850
next stage where you take that raw data and
create the spatial data infrastructure and

00:27:07.850 --> 00:27:12.860
make the data ready for scientists to make
interpretations. Those data that need to be

00:27:12.860 --> 00:27:18.090
archived and disseminated throughout the world
to other planetary scientists so they in turn

00:27:18.090 --> 00:27:22.850
can make you observations that generates new
questions that continues the cycle. In the

00:27:22.850 --> 00:27:28.730
middle is our support staff, our administrative
staff or I.T. staff the heart of our operation

00:27:28.730 --> 00:27:32.909
and they're the ones helping to make sure
we continue to be able to operate at the level

00:27:32.909 --> 00:27:39.220
that we do. At the top of that diagram use
of research operations. We have world-class

00:27:39.220 --> 00:27:43.070
scientists in our group and I would love to
be able to tell you every single project that

00:27:43.070 --> 00:27:47.870
all of them work on, it's simply not enough
time and hopefully we will have some of them

00:27:47.870 --> 00:27:51.870
come out and give similar presentations on
all the work they do but two examples I have

00:27:51.870 --> 00:27:58.049
your one on the left is an image of the surface
of Mars. The Rocky the way the color and material

00:27:58.049 --> 00:28:04.320
is the way of an impact crater in this impact
crater was observed by an orbital mission

00:28:04.320 --> 00:28:09.420
around Mars through an instrument called high-rise.
As this instrument was being flown through

00:28:09.420 --> 00:28:16.289
the surface of Mars it would take an observation
or a time and come back and take another observation

00:28:16.289 --> 00:28:20.960
and in doing that they found that one of these
impact craters in particular the first time

00:28:20.960 --> 00:28:25.120
around they do not see anything of particular
interest in next time they came around they

00:28:25.120 --> 00:28:30.029
saw these dark streaks you see here these
tens of meters long dark streaks and that

00:28:30.029 --> 00:28:36.429
told him that there appear to be some sort
of active geologic process and with NASA school

00:28:36.429 --> 00:28:40.370
at the time being to follow the water there
were a lot of people that thought perhaps

00:28:40.370 --> 00:28:44.429
this could be signs of flowing liquid water
of the on the surface of Mars.

00:28:44.429 --> 00:28:48.860
Turns out that's a really difficult thing
to do but our signs have been able to put

00:28:48.860 --> 00:28:55.320
together some really fascinating products
to take a look at in immense detail and do

00:28:55.320 --> 00:28:59.370
in a reliable manner such that they can come
up with an alternative hypothesis that suggests

00:28:59.370 --> 00:29:06.030
it was not water at all it was slope activated
sand flows that were a result of interactions

00:29:06.030 --> 00:29:10.850
with with events and that sort of thing. It
made a lot of people within NASA a little

00:29:10.850 --> 00:29:15.789
bit angry that it was not water in fact, we
now refer to the gentleman with this discovery

00:29:15.789 --> 00:29:22.270
as the dream crusher but there is still an
active debate as to whether or not these are

00:29:22.270 --> 00:29:28.999
actually strictly sand drive features or something
else entirely. Over on the right you may have

00:29:28.999 --> 00:29:34.860
seen there is an article that came out yesterday
talking about one of the moons around Saturn

00:29:34.860 --> 00:29:40.710
and this is something we have been doing a
lot of work on lately. And it is covered on

00:29:40.710 --> 00:29:45.320
the outside by an icy sphere and its thought
there might actually be a liquid water ocean

00:29:45.320 --> 00:29:50.759
underneath that icy sphere so the long stretches
you see there are actually long sisters that

00:29:50.759 --> 00:29:59.280
have water organisms where water is heated
and is extruded onto the surface in the firm

00:29:59.280 --> 00:30:09.519
form of volcanism. and we have made sure that
all this data is put together that we are

00:30:09.519 --> 00:30:14.539
100% certain that the pixels are in place
when you see these features that are active

00:30:14.539 --> 00:30:19.600
we can make certain that they are really active
in representing the processes we believe that

00:30:19.600 --> 00:30:27.769
they are which in this case appears to be
liquid water oceans underneath the icy surface.

00:30:27.769 --> 00:30:33.320
We also have a variety of people in our group
that are active in planetary spacecraft missions.

00:30:33.320 --> 00:30:41.870
The most active ones being the Rovers on Mars
including MSL, and we have people who actually

00:30:41.870 --> 00:30:46.470
do things that are quite similar to what the
Apollo astronauts did back in the day which

00:30:46.470 --> 00:30:51.440
is to help them make observations, collect
those observations, make new plans and decide

00:30:51.440 --> 00:30:56.399
where Rover is going to go the next day and
what new observations is going to make and

00:30:56.399 --> 00:31:02.879
what new sciences being drive from those observations.
It turns out that one of our scientists actually

00:31:02.879 --> 00:31:08.580
was able to put together this selfie which
is one of the most popular imagers of the

00:31:08.580 --> 00:31:13.740
Mars curiosity Rover. Over the years after
several decades more and more missions are

00:31:13.740 --> 00:31:18.120
going to more and more location psychology
increasing and getting better we increasingly

00:31:18.120 --> 00:31:23.559
get more and more data all the time and to
the point that becomes a little bit difficult

00:31:23.559 --> 00:31:31.159
to handle. We at astrogeology we have the
imaging note of NASA's planetary data system

00:31:31.159 --> 00:31:36.169
and what that means is that we have data from
all spacecrafts that have been active since

00:31:36.169 --> 00:31:42.180
the beginning of the spacecraft exploration
era. That's a lot a lot of data we have about

00:31:42.180 --> 00:31:46.840
three petabytes of data that we store in our
centers which is quite a bit for a center

00:31:46.840 --> 00:31:53.259
that only about 65 people in size. The largest
center for data in the USGS

00:31:53.259 --> 00:31:59.120
that maintains a lot of data on behalf of
USGS and we are second only to them in terms

00:31:59.120 --> 00:32:05.879
of the amount of data we have. It is one thing
to store the data and it's another to make

00:32:05.879 --> 00:32:10.730
it usable to the planetary science community
so we have come develop a software package

00:32:10.730 --> 00:32:15.940
called ices. We had the day before the other
group you might be thinking up and is referred

00:32:15.940 --> 00:32:23.570
to integrated software imagers and spectrometers
and it standardizes it and makes it usable

00:32:23.570 --> 00:32:29.059
in a way you can extract it and send it to
people throughout the world so they can make

00:32:29.059 --> 00:32:33.200
sciences scientific observation so some examples
of that include things like these elevation

00:32:33.200 --> 00:32:38.780
models and this is a digital elevation model
proportion of the surface of Mars where the

00:32:38.780 --> 00:32:45.279
long axis represents kilometers in length.
The main reason for looking at these 3-D structures

00:32:45.279 --> 00:32:49.480
is to provide you with a new perspective looking
at things even when you looked at it in two

00:32:49.480 --> 00:32:53.869
dimensions for a long time so when you see
it in three dimensions it open up the relationships

00:32:53.869 --> 00:32:58.639
between features telling you more about how
those features may have formed and involved

00:32:58.639 --> 00:33:06.700
and how they're relative to one another. Another
thing we do is provide global mosaics in the

00:33:06.700 --> 00:33:11.460
planetary science community. It may not seem
like a big deal because what some people think

00:33:11.460 --> 00:33:15.720
happens is that if spacecraft goes to a planet,
it parks in front of the planet and takes

00:33:15.720 --> 00:33:20.770
this amazing one-shot image high-resolution
image of the planet and then you're done.

00:33:20.770 --> 00:33:25.929
Unfortunately does not work like that. The
orbiters go around over and over and over

00:33:25.929 --> 00:33:31.220
again and take millions of data points and
millions of images and it's up to us to take

00:33:31.220 --> 00:33:35.429
all those images, stitched them together and
produce this seamless mosaic similar to what

00:33:35.429 --> 00:33:41.549
you see that provides global geologic context
for planetary [Indiscernible]. These are a

00:33:41.549 --> 00:33:45.970
few additional examples of some the work that
comes out as a result of taking the raw data

00:33:45.970 --> 00:33:50.240
putting it through your software package and
the software package has been open source

00:33:50.240 --> 00:33:54.220
to the community so we are not getting back
from the entirety of the world in terms of

00:33:54.220 --> 00:34:00.200
how to produce the best possible spacecraft
of software extraction data. You can see a

00:34:00.200 --> 00:34:07.210
variety of examples here of topographic light
imaging as well as correcting distortions

00:34:07.210 --> 00:34:12.980
in data but what you see in the center is
a lending ellipse that was generated through

00:34:12.980 --> 00:34:17.260
putting together a variety of data sets for
the surface of Mars prior to the landing of

00:34:17.260 --> 00:34:23.149
the Mars curiosity Rover and it was our focus
to help NASA and JPL to help understand where

00:34:23.149 --> 00:34:27.980
they wanted to go why they wanted to go there
and certified the site. Perhaps more poorly

00:34:27.980 --> 00:34:34.659
we are not involved in the next generation
of rovers to the surface of Mars the Mars

00:34:34.659 --> 00:34:40.159
2020 Rover which will hopefully be launching
in July. What you may not recognize is that

00:34:40.159 --> 00:34:44.320
there is a time difference between Mars and
the earth in terms of how it takes the data

00:34:44.320 --> 00:34:49.919
to get here so you can actually have a lot
of things that happen as a spacecraft is coming

00:34:49.919 --> 00:34:55.850
down that can be quite devastating and it
happens before we even have any time to do

00:34:55.850 --> 00:35:00.390
anything about it so the idea was to come
up with an autonomous system such that the

00:35:00.390 --> 00:35:05.670
spacecraft itself can make real-time observations,
found out if they is any danger the landing

00:35:05.670 --> 00:35:11.200
ellipse and to actually make real-time adjustments
if needed. Our folks worked very closely with

00:35:11.200 --> 00:35:15.540
the Jet Propulsion Laboratory to make sure
this autonomous offer was loaded on board

00:35:15.540 --> 00:35:19.490
along with the orbital map data that was loaded
onto the spacecraft as well

00:35:19.490 --> 00:35:26.680
that could do real-time comparison. Another
thing that I refer to we have done is planetary

00:35:26.680 --> 00:35:33.050
geologic mapping. One of the main things this
is a long-standing program and has been happening

00:35:33.050 --> 00:35:37.980
ever since 1963 and continue to do mapping
today and it is our goal to the mapping of

00:35:37.980 --> 00:35:42.990
every solid body in the entire solar system.
But the one I'm sure you hear is one that

00:35:42.990 --> 00:35:46.400
actually just came out and this is one of
the moon and you think haven't we already

00:35:46.400 --> 00:35:51.000
done all the geological mapping we needed
to do on the moon? Turns out a lot of the

00:35:51.000 --> 00:35:55.480
geological mapping that was done was done
in a regional scale at a variety of different

00:35:55.480 --> 00:36:00.130
scales by different groups using different
methods so much so you can actually take to

00:36:00.130 --> 00:36:03.260
the different regions on the moon that had
been mapped by different entities put them

00:36:03.260 --> 00:36:09.160
together and they would not allow the different
units, different interpretations and it was

00:36:09.160 --> 00:36:13.321
an arduous effort for us to have to go through
and make all of those adjustments to make

00:36:13.321 --> 00:36:20.290
sure you can provide one unified seamless
geologic map. This is a huge and ever and

00:36:20.290 --> 00:36:24.780
it's meant to be largely impactful to your
understanding of the moon but also for potential

00:36:24.780 --> 00:36:30.400
for humans to go to the moon in 2024 using
this information. I should also note that

00:36:30.400 --> 00:36:35.190
another thing we do is what we call planetary
nomenclature and what that means is take for

00:36:35.190 --> 00:36:39.930
example an impact crater and if you have one
person naming it one thing and another person

00:36:39.930 --> 00:36:44.640
any get another thing we have no idea potentially
what one is talking about is or what is referred

00:36:44.640 --> 00:36:49.090
to the same thing and calling it different
things. So the international astronomical

00:36:49.090 --> 00:36:55.450
Union charted us to maintain an active database
of all planetary names so that there is a

00:36:55.450 --> 00:37:00.050
standardized way for everybody to refer to
the same things throughout the solar system

00:37:00.050 --> 00:37:05.770
so you have to actually go through a process
to get a name for new features that are discovered

00:37:05.770 --> 00:37:11.600
and we help to maintain that selection for
new features. One of the things restarted

00:37:11.600 --> 00:37:15.390
over the last couple of years is getting back
to one of the things we did early in our history

00:37:15.390 --> 00:37:22.410
wishes to rest or analog studies. For sometime
we were super active in primarily planetary

00:37:22.410 --> 00:37:27.600
orbital and robotic lending missions and with
the goal of potentially having humans going

00:37:27.600 --> 00:37:33.000
back to the moon as early as 2024 we wanted
to make sure that we were as educated as we

00:37:33.000 --> 00:37:37.400
could possibly be about all the various terrestrial
analogs throughout the world so we could be

00:37:37.400 --> 00:37:41.470
some of the world experts in helping to train
the next generation of astronauts before they

00:37:41.470 --> 00:37:47.860
go to the moon. We also work very closely
with other USGS centers including those in

00:37:47.860 --> 00:37:53.230
Hawaii , at the Hawaiian Volcano Observatory.
I alluded to you earlier that the volcanic

00:37:53.230 --> 00:37:59.120
features on the moon those orange grass beats
and the spot that they were produced by feature

00:37:59.120 --> 00:38:03.150
very similar to this so we had folks who went
out there and helped take observations of

00:38:03.150 --> 00:38:09.310
this active flow so that they could get a
sense of how these were produced and when

00:38:09.310 --> 00:38:19.930
they're found on the planetary surfaces we
can infer processes just like this. So again

00:38:19.930 --> 00:38:25.200
we are doing this in anticipation of the next
generation of astronauts going to the moon

00:38:25.200 --> 00:38:30.740
by 2024 and this is the class it just graduated
and thankfully we were able to work very closely

00:38:30.740 --> 00:38:35.570
with this class over the last year or so as
they came out to northern Arizona to work

00:38:35.570 --> 00:38:41.280
with us and our NASA colleagues to start going
back to these places that the Apollo astronauts

00:38:41.280 --> 00:38:46.386
went going to the crater into the Grand Canyon
and checking out the San Francisco volcanic

00:38:46.386 --> 00:38:52.080
field and being active participants to understand
the fundamentals of geology. This is the goal

00:38:52.080 --> 00:38:57.910
that NASA set forth for how we want to try
and get to the moon by 2024 and in addition

00:38:57.910 --> 00:39:02.330
to us helping to train the next generation
of astronauts we are also going to be involved

00:39:02.330 --> 00:39:06.920
in every single one of these stages that you
see here with the ultimate goal of the first,

00:39:06.920 --> 00:39:11.660
getting humans to the moon by 2024 but then
as you can see in the upper right corner you

00:39:11.660 --> 00:39:17.840
can see the goal of hopefully trying to get
humans to Mars within the next decade. In

00:39:17.840 --> 00:39:21.750
the meantime we want to make sure that we
can help take that information and engage

00:39:21.750 --> 00:39:25.230
and inspire the world so we can create the
next generation of monetary scientists and

00:39:25.230 --> 00:39:29.600
the next generation of astronauts who want
to go and explore some of these questions

00:39:29.600 --> 00:39:33.760
so if you have been to our science center
lately we've made a lot of changes to try

00:39:33.760 --> 00:39:38.990
to get people more engaged with the products
we make and here we have an example of a topographic

00:39:38.990 --> 00:39:44.840
sandbox that several you may have seen. We
have one as well and over on the right we

00:39:44.840 --> 00:39:49.290
have a scale model of asteroid and asteroids
are really important as well for a variety

00:39:49.290 --> 00:39:53.520
of reasons. There are new initiatives in terms
of understanding them for potential resource

00:39:53.520 --> 00:39:58.640
mining and also for planetary sensory so we
want to make sure people understand what these

00:39:58.640 --> 00:40:02.870
things are and what they look like and help
engage them and inspire the next generation

00:40:02.870 --> 00:40:08.300
we want to inspire kids locally at the state
level and at the country level throughout

00:40:08.300 --> 00:40:13.330
the world and as it's our hope that perhaps
you can even inspire children in the galaxy

00:40:13.330 --> 00:40:30.170
far far away. Thank you so much for your attention.

00:40:30.170 --> 00:40:38.160
[Applause] &gt;&gt;
The flyers for that are on the back table

00:40:38.160 --> 00:40:44.330
but if you have any questions for Justin.
There's a microphone right here please just

00:40:44.330 --> 00:40:51.490
orderly lineup and if you're not able to get
up here raise your hand and I can read the

00:40:51.490 --> 00:40:54.650
microphone over to you.

00:40:54.650 --> 00:41:16.900
We have plenty of time for questions. &gt;&gt; Just
to get a handle on the size of the database

00:41:16.900 --> 00:41:29.010
that's involved , how many what's the storage
size of mosaic like the mosaic of the moon

00:41:29.010 --> 00:41:32.920
you're showing .

00:41:32.920 --> 00:41:37.700
The mosaics themselves tend to be tens of
hundreds of gigabytes in some they can be

00:41:37.700 --> 00:41:44.100
as large as terabytes but tens to hundreds
of gigabytes and that if you take that many

00:41:44.100 --> 00:41:56.700
start putting them all together that's when
you start adding to petabyte size. &gt;&gt; Do you

00:41:56.700 --> 00:42:07.200
communicate to these fellows from other countries
and Russian, Canadian and a productive of

00:42:07.200 --> 00:42:08.510
a collaboration you have been.

00:42:08.510 --> 00:42:15.900
That's something we have done as the relatively
new director I want to make a more concerted

00:42:15.900 --> 00:42:18.700
effort to make sure we are engaging with our
international colleagues. We do work pretty

00:42:18.700 --> 00:42:25.110
regularly with our colleagues in Berlin, and
Canadian space agency and throughout the European

00:42:25.110 --> 00:42:30.310
space agency's and even with the Japanese
space agency. Those have been hit and miss

00:42:30.310 --> 00:42:35.130
but I would like to make it much more concerted
effort to make sure we are all working together

00:42:35.130 --> 00:42:39.270
sharing data in a standardized way so that
we have all have access to the same data and

00:42:39.270 --> 00:42:42.750
can work together to make new discoveries.

00:42:42.750 --> 00:42:52.940
What was the most surprising discovery from
the samples that the astronauts collected

00:42:52.940 --> 00:42:55.100
on the moon?

00:42:55.100 --> 00:43:02.000
You're asking somebody who's exceptionally
biased about that. My own personal bias is

00:43:02.000 --> 00:43:07.210
as you heard in my instruction there is a
radioactive trace element called thorium and

00:43:07.210 --> 00:43:13.430
thorium is a heat producing radioactive element
that was pretty surprisingly discovered on

00:43:13.430 --> 00:43:15.930
the moon I don't think people thought it was
going to be there and it was certainly not

00:43:15.930 --> 00:43:20.210
in any large quantities and it turns out that
thorium is one of the key elements to help

00:43:20.210 --> 00:43:24.930
us understand the illusion of the moon and
why you have the Celtic volcanism focused

00:43:24.930 --> 00:43:31.430
squarely on this side of the moon so making
that the story and combining it with orbital

00:43:31.430 --> 00:43:37.820
observations of very large aerial abundances
of thorium across the near side of the moon

00:43:37.820 --> 00:43:42.980
was one of the major discoveries. But there
is you discoveries made all the time again

00:43:42.980 --> 00:43:49.410
water was one of them that was never expected.
There is a right of other things. There are

00:43:49.410 --> 00:43:55.260
some organics that have been discovered as
well now that we are able to the text abundances

00:43:55.260 --> 00:44:00.010
a really small small levels that were not
expected that may have been from impacts from

00:44:00.010 --> 00:44:06.020
organic meteorite so there's a lot of the
scar is actually that have been made or lost

00:44:06.020 --> 00:44:09.830
the reason we continue to make more and more.
People think that we have been there done

00:44:09.830 --> 00:44:16.770
that but because of new technologies that
can be applied we are making new discoveries

00:44:16.770 --> 00:44:18.340
all the time.

00:44:18.340 --> 00:44:24.300
Maybe a follow-up question to the collaboration
question. Is it true that China is going to

00:44:24.300 --> 00:44:27.900
be exploring the moon actively soon?

00:44:27.900 --> 00:44:31.810
They are, actually.

00:44:31.810 --> 00:44:33.720
Will be be collaborating on their side of
the moon?

00:44:33.720 --> 00:44:39.350
It is a little difficult right now is a little
bit difficult for us to work with China as

00:44:39.350 --> 00:44:45.360
a federal government agency but there are
other entities, space ask for example working

00:44:45.360 --> 00:44:51.550
with the Chinese government to some extent
so it is the idealized version would be yes

00:44:51.550 --> 00:44:55.680
all of us would work together it is a little
bit difficult right now though. But yes, they

00:44:55.680 --> 00:45:02.990
do have active rovers in orbit right now.
&gt;&gt; Thank you for coming out in for the talk.

00:45:02.990 --> 00:45:08.840
It was quite good. Can you elaborate more
on distribution of the thorium and is it in

00:45:08.840 --> 00:45:15.990
fact distributed because the moon was tightly
locked or other -- I'm just wondering more

00:45:15.990 --> 00:45:17.120
about the relationship.

00:45:17.120 --> 00:45:22.570
I might have to talk to you about this off-line
because I can go on for hours but I will tell

00:45:22.570 --> 00:45:31.360
you that the model at least as we thought
was that thorium used to be globally distributed

00:45:31.360 --> 00:45:36.110
and it was caught between the thick layer
of the cross and the mantle and this really

00:45:36.110 --> 00:45:40.730
thin layer of heat producing elements basically
thorium, uranium and other heat producing

00:45:40.730 --> 00:45:48.220
elements. There was a giant in fact called
South Pole Aitken basin and it was a glancing

00:45:48.220 --> 00:45:53.390
blow and only an impact that size would have
completely destroyed the moon but in this

00:45:53.390 --> 00:45:59.450
instance because it was a glancing blow the
ideas that it took this material full of thorium

00:45:59.450 --> 00:46:06.120
and concentrated it to the impact on the near
side and that material then got transmitted

00:46:06.120 --> 00:46:11.520
to the interior of the moon the mantle down
below and all of it was concentrated right

00:46:11.520 --> 00:46:16.880
below the near side of the moon where the
decay of the thorium went to the heat producing

00:46:16.880 --> 00:46:21.410
to the production of heat nothing of the mental
irruption of the volcanism only on the near

00:46:21.410 --> 00:46:29.230
side of the moon. That's the quick summary
but I'm happy to talk more about it afterwards.

00:46:29.230 --> 00:46:36.130
Are there any uses of
AI in your tools and technology for some Voyager

00:46:36.130 --> 00:46:45.081
lending suffer right obstacle avoidance and
also navigation on the penitentiary. &gt;&gt; We

00:46:45.081 --> 00:46:49.080
are always exploring new technologies and
techniques and we are involving artificial

00:46:49.080 --> 00:46:56.741
intelligence and machine learning technologies
that were using to investigate the planetary

00:46:56.741 --> 00:47:00.930
surfaces that reminds me that we are also
investigating the use of augmented reality

00:47:00.930 --> 00:47:05.270
and virtual reality as well particularly in
the training of the astronauts and as they

00:47:05.270 --> 00:47:14.470
come out, we're going to be experimenting
with the use of AR as you move forward. &gt;&gt; Did

00:47:14.470 --> 00:47:21.730
I hear correctly that some of the sealed lunar
samples in Houston have been opened or will

00:47:21.730 --> 00:47:23.920
be opened or have been opened?

00:47:23.920 --> 00:47:29.040
Yes. The ones you are referring to
was one of the drive tubes from Apollo 16

00:47:29.040 --> 00:47:32.140
so the astronauts when they went there instead
of drilling they took a two and they were

00:47:32.140 --> 00:47:39.040
able to hammer down and seal it for posterity
effectively and bring it back and it had been

00:47:39.040 --> 00:47:43.930
since the 60s that that drive drive to was
closed and sealed and it was recently opened

00:47:43.930 --> 00:47:50.240
within this last year and a of my PhD advisor
is actually one of the persons involved in

00:47:50.240 --> 00:47:54.250
this sample analyzing so I'm inspecting to
see some really fascinating discoveries to

00:47:54.250 --> 00:47:55.530
come out of that.

00:47:55.530 --> 00:47:58.840
So the research is certainly not complete
yet?

00:47:58.840 --> 00:48:00.300
Correct.

00:48:00.300 --> 00:48:06.860
Was the intent to preserve this for modern
technique or for new generations?

00:48:06.860 --> 00:48:11.480
Exactly. And to make comparisons over time
see how things may have changed. One of the

00:48:11.480 --> 00:48:14.781
really interesting thing is that people are
interested in is a concept known as the space

00:48:14.781 --> 00:48:21.480
weathering. The hope is that with the drive
tube you're going to retain kind of that stratigraphy

00:48:21.480 --> 00:48:28.510
of the concept you see what the space weathering
affected the uppermost parts of the drive

00:48:28.510 --> 00:48:33.280
tube as opposed to something down lower so
that's why to be something that had not been

00:48:33.280 --> 00:48:37.550
identified at that time. There is any process
that people are really exceptionally interested

00:48:37.550 --> 00:48:41.580
in that can now be investigated with that
concept in mind but yes you technologies as

00:48:41.580 --> 00:48:54.360
well. &gt;&gt; Earlier you touched a little bit
about the imagery that comes from your department.

00:48:54.360 --> 00:49:00.100
How much is it that your group does is everything
that I see here the pictures I see in the

00:49:00.100 --> 00:49:05.050
news and the media the ones that look amazing
is that from your group or is that from a

00:49:05.050 --> 00:49:09.020
different group and can you talk a little
bit about how long it takes to put those together

00:49:09.020 --> 00:49:15.160
and how realistic they are? The colors are
amazing and thinking about the colors, there's

00:49:15.160 --> 00:49:16.260
another real colors.

00:49:16.260 --> 00:49:21.800
A lot of great questions. In general, we work
with a lot of different entities all that

00:49:21.800 --> 00:49:25.610
the planetary science community to generate
those but yes, in a lot of instances we are

00:49:25.610 --> 00:49:30.460
responsible for some of the things you see
particularly those large global mosaics. Those

00:49:30.460 --> 00:49:35.120
do take an immense amount of time . Like I
said there's millions of data points and it

00:49:35.120 --> 00:49:43.000
takes our supercomputing clusters it takes
are educated dedicated staff and the army

00:49:43.000 --> 00:49:47.030
of students to go through and process all
of this information to make sure it aligns

00:49:47.030 --> 00:49:54.260
perfectly and happens in fits and starts and
can happen over years. The colors you actually

00:49:54.260 --> 00:50:01.070
saw our real colors but many instances are
the ones you see will be filters that are

00:50:01.070 --> 00:50:06.200
used by instruments to look at different wavelengths
that will tell us about the compositions of

00:50:06.200 --> 00:50:10.760
different materials when you look at them
through a different filter or lens. You always

00:50:10.760 --> 00:50:15.290
want to be a little bit aware so for example
one of the things we recently generated is

00:50:15.290 --> 00:50:20.350
a topographic map of the moon that we actually
converted to a rock in the putdown in our

00:50:20.350 --> 00:50:26.260
education and outreach center for kids to
come out and walk on. It is in blues and greens.

00:50:26.260 --> 00:50:31.461
Is a color ramp that we chose to better represent
the differences in topography and the question

00:50:31.461 --> 00:50:37.450
we get all the time well, we did not realize
Mars was green. Why is that? It gives us the

00:50:37.450 --> 00:50:42.260
opportunity why you have that difference in
color skills because they will tell you slightly

00:50:42.260 --> 00:50:46.050
different things and bring things out in a
way that you may not have expected if you

00:50:46.050 --> 00:51:02.460
are looking at visible light only. Did that
answer your question? Yeah. &gt;&gt; Is any of your

00:51:02.460 --> 00:51:12.950
groups work include establishing colonies
on the moon for extended stays and if so,

00:51:12.950 --> 00:51:22.870
does it include energy production and if so,
thorium have anything to do with that?

00:51:22.870 --> 00:51:29.390
I'm so happy their survey questions about
thorium. To answer the first question in terms

00:51:29.390 --> 00:51:33.970
of actually building anything or having an
actual colony building partner not so much

00:51:33.970 --> 00:51:38.430
involved in but the second part of your question
terms of energy resources we are getting more

00:51:38.430 --> 00:51:43.200
involved in. You may be familiar with the
fact that the USGS here is responsible for

00:51:43.200 --> 00:51:49.740
finding a lot of energy deposits and resources
so why not take that expertise in applied

00:51:49.740 --> 00:51:54.360
to understanding another planetary surface
so we are actually currently involved in several

00:51:54.360 --> 00:51:59.630
different initiatives to explore resources
on the moon as well as resources on things

00:51:59.630 --> 00:52:05.053
like asteroids. Thorium while it is largely
disseminated across the near side of the moon

00:52:05.053 --> 00:52:09.570
and concentrated in such a way that it would
look like it will be useful it is not in such

00:52:09.570 --> 00:52:14.540
large abundances that would make a primary
resource unfortunately but that's why we are

00:52:14.540 --> 00:52:19.990
exporting things like solar illumination,
trying to find areas where for example there

00:52:19.990 --> 00:52:25.650
is permanent exposure to light all the time.
On the moon there's areas of permanent light

00:52:25.650 --> 00:52:30.340
and eras of permanent shadow in both of those
are interesting from an energy resource perspective

00:52:30.340 --> 00:52:36.170
one because permanent light you can use solar
panels in one from the permanent dark is eras

00:52:36.170 --> 00:52:41.430
where we think there might be large concentrations
of water ice and that's one of the goals ideally

00:52:41.430 --> 00:52:46.290
of the Artemis mission to go to the South
Pole and help determine whether or not these

00:52:46.290 --> 00:52:51.440
concentrations of water ice are really water
ice or not. The observations we are getting

00:52:51.440 --> 00:52:54.940
our telling us two different things. One is
thing it could be large concentrations of

00:52:54.940 --> 00:53:02.190
water ice and other suggested could be solar
wind and planted hydrogen that looks to remote-sensing

00:53:02.190 --> 00:53:06.940
data like water and hydrogen so it will be
really important for us to go up there to

00:53:06.940 --> 00:53:11.210
find out if these are actually real ice deposit
because if they are they can be utilized for

00:53:11.210 --> 00:53:12.400
future colonization.

00:53:12.400 --> 00:53:22.050
I'm sure you know about the HBO series from
the earth to the moon in a particular episode

00:53:22.050 --> 00:53:27.930
where they talk about the astral geology astrogeology
which is one of my favorite episodes but as

00:53:27.930 --> 00:53:36.830
I learned tonight they totally shortchange
Dr. Shoemaker it appears because I think they

00:53:36.830 --> 00:53:45.450
mention MIT or Caltech some Dr. silver which
I'm sure was a good fellow who did good work

00:53:45.450 --> 00:53:51.340
but they did not mention Shoemaker at all
as I recall and I'm just curious maybe 40

00:53:51.340 --> 00:53:55.770
off-color comments you think you got shortchanged
in that episode?

00:53:55.770 --> 00:54:04.350
I will certainly admit I am biased and even
though I never got opportunity to get to know

00:54:04.350 --> 00:54:09.090
Jean he was exceptionally influential in a
lot of the levels but he was not the only

00:54:09.090 --> 00:54:13.930
one there were people like others and people
that were in involved in all stages and they

00:54:13.930 --> 00:54:19.490
work together as a team I'm sure they butted
heads and they had a strong opinion some more

00:54:19.490 --> 00:54:25.240
prominent than others because they were willing
to be at the front of the crowd but I would

00:54:25.240 --> 00:54:29.170
say that it would have been nice to see a
little bit more about Jean but it really was

00:54:29.170 --> 00:54:34.480
a team of people who did all that work so
it's fair that the information they provided

00:54:34.480 --> 00:54:41.450
would've been nice to see a little bit more
about that. &gt;&gt;

00:54:41.450 --> 00:54:49.120
While we still have you on the horn so to
speak of your perspective as a science director,

00:54:49.120 --> 00:54:57.700
what would you give in terms of your advice
for geologists who are now selecting a program

00:54:57.700 --> 00:54:58.870
of study.

00:54:58.870 --> 00:55:05.960
The thing we find most often when we are trying
to inspire and engage next-generation there's

00:55:05.960 --> 00:55:12.580
this concept of planetary science is this
unique singular thing that is only made for

00:55:12.580 --> 00:55:17.310
a few people to do and as I try to allude
to in that one diagram planetary science is

00:55:17.310 --> 00:55:23.600
this amalgamation of a white righty of expertise
and skill sets and it will be to let people

00:55:23.600 --> 00:55:29.300
know that any skill that you have as long
as he wanted with passionately can be brought

00:55:29.300 --> 00:55:34.490
to bear in terms of being part of our team
to help make some new discovery so you have

00:55:34.490 --> 00:55:39.980
to be a geologist or you don't have to be
just a computer scientist you can be a variety

00:55:39.980 --> 00:55:47.450
of things to help become part of our team.

00:55:47.450 --> 00:55:55.773
Please join me in giving him another round
of applause. Thank you, Justin.

00:55:55.773 --> 00:55:56.773
[Applause]

00:55:56.773 --> 00:56:09.970
Thank you all for joining us tonight and drive
safe home and see you next month.

00:56:09.970 --> 00:56:29.200
[Event concluded]

