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So, in my job as the spacecraft science phase 
lead, I get to work hand-in-hand with the  

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scientists and the navigation team to plan 
out this mission and how OSIRIS-REx is going  

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to execute this. For me personally this is an 
ideal combination. I've always loved deep space  

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exploration and the science behind it, so I get to 
work one-on-one with the science teams to identify  

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really what their science goal is and translate 
that for the spacecraft team to something that  

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we can actually execute, piece by piece, as 
the spacecraft goes through its commanding.

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So, one of the challenges that OSIRIS-REx has 
been facing is the microgravity environment that  

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we are in when we orbit Bennu. We don't have the 
strong pull of gravity below us, so instead, the  

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non-gravitational forces in the spacecraft affect 
our trajectory a lot more than what we're used to.

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So over the course of a few weeks, we could 
end up on a number of different trajectories,  

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and that means our uncertainty in planning and 
our responsibility to keep the spacecraft safe  

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is very challenging. So we have to constantly 
update our pointing on board the spacecraft,  

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both for maneuvers and for 
science pointing purposes.  

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And we have to constantly reanalyze the 
sun angles on the spacecraft to make sure  

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that the power and thermal and telecom attitudes 
are safe for the spacecraft to navigate.

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So, when we're orbiting around Bennu, the 
force of gravity on the spacecraft is about  

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one millionth what the force of 
gravity at Mars is for our spacecraft,  

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so that's a significant change in 
the forces that spacecraft feels,  

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and it means that the non-gravitational forces, 
such as solar radiation pressure, are within an  

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order of magnitude of gravity, which is a very 
new environment for us to be operating in.

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So, OSIRIS-REx comes with an instrument suite that 
was uniquely designed to observe the asteroid,  

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but the spacecraft itself was also designed 
to observe this asteroid. Our science mission  

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requires us to observe and map all over the 
surface of the asteroid under a number of  

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different lighting conditions. To support that, 
all of our subsystems have been tuned for this  

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purpose. So our solar arrays are gimballed so 
we can continue to keep a power positive margin  

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as we look at different sun angles and different 
sites around the surface of the asteroid. Our  

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thruster suites, we have very low thrust engines 
that allow us to do very tiny, precision pointing  

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maneuvers around the asteroid. On board, our 
software, for instance, has a targeting software.  

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It allows us to load up a list of targets from 
the science teams and tell the spacecraft to  

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execute them autonomously as it maps out the 
surface of Bennu for us, and additionally, we  

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have an engineering camera which we use to support 
the optical navigation that this mission needs.

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So, before launch we expected that the surface of 
Bennu would be covered in a fine-grained material  

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much like the lunar regolith on the surface of the 
Moon. This was supported by the observations that  

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the science teams had done of Bennu before 
launch. They used ground-based astronomy,  

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radio astronomy, and infrared imaging to deduce 
the thermal inertia of the surface material on  

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Bennu. When we got to Bennu, we found, to our 
surprise, that instead it's covered in a lot of  

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rocky material and it's a much rougher surface 
than we were expecting. We've had to adapt our  

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science plan and our sample acquisition plan 
to this new rocky surface of Bennu instead.

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Before launch, we had developed two methods to 
guide ourselves in for TAG. We had a primary  

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method which was to use our lidar to do a ranging 
acquisition. As we approach the TAG site and  

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guide ourselves in, that was our primary method 
that we did the majority of our development on.  

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We developed a backup method using natural 
feature tracking which is an optical navigation  

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used on board autonomously to image the site, 
compare it to a catalog, and guide ourselves in.  

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When we got to Bennu, the rocky surface of 
Bennu really changed our entire approach to TAG.  

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Originally, we had expected to be able to find a 
25 meter radius site that could be safe to TAG in,  

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that would be full of this fine-grained material, 
and wouldn't have uneven surfaces that could  

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be dangerous for the spacecraft. Unfortunately, 
Bennu did not know about our expectations for it,  

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and when we got there, we found that there weren't 
sites large enough to meet that need. Without that  

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large site, the lidar approach could no longer 
support the increased performance that we needed,  

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and the natural feature tracking 
with its higher precision targeting  

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could get us to a site that was smaller and could 
fit within the smaller smooth surfaces of Bennu.

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So, we've just completed our Match 
Point rehearsal, and we got to see  

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a second demonstration of how well NFT 
has been used to predict our TAG profile.  

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And in our last rehearsal, we 
saw NFT come in within two meters  

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of the TAG site which is really impressive 
when you consider that our original design  

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was to come within 25 meters of a TAG site. So 
NFT's onboard performance and the tuning that  

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our ground team has done to perfect NFT over 
the last few years has allowed us to get an  

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order of magnitude better performance out of the 
spacecraft than it was designed for, and that's  

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what we need to be able to TAG successfully 
on this small TAG site that Bennu has for us.

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For me the most exciting part about OSIRIS-REx has 
been the same thing that causes the challenges:  

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it's the dynamic nature of this mission and how 
much we are dependent on what we learn from the  

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asteroid. Every few weeks our trajectory has to 
change, and we're having to redesign the mission  

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as we fly it which gives us a whole new challenge 
for mission operations we haven't had before.  

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Traditionally, mission operations, from 
a spacecraft engineer point of view,  

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we operate the spacecraft, and we don't always 
see the results of data we're taking for a long  

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time. On Bennu the science observations 
and the results we're getting out of that,  

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feed right back into the spacecraft trajectory 
and our overall proximity operations phase,  

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so we get to see first-hand what we're 
learning about this asteroid with the  

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science teams, which has been a really rewarding 
experience for our team and for me personally.

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[Room Tone]

