The application
deadline for the NASA Planetary Science Summer School at the Jet
Propulsion Laboratory in Pasadena, California is approaching, and I
realized that I hadn't yet written about my own PSSS experience six
years ago. Rereading our paper and looking at photos just now, I remembered that I had met a few of my friends and colleagues through
that experience. I present to you:
Ganymede Interior,
Surface, and Magnetometer Orbiter, or, GISMO.
Planetary Science
Summer School is a one-week bootcamp. Fourteen of us planetary
science and engineering graduate students and post-docs gathered for
the first session of PSSS in July 2010. We had been emailing back and
forth for a month or so, throwing around ideas and getting to know
each other. It was through these exchanges that we settled on our
mission to Ganymede, Jupiter's largest moon and the only moon known
to have its own magnetosphere (magnetic field).
I was assigned the
positions of Planetary Protection (protecting other worlds from us)
and Education & Public Outreach (EPO). I was tasked with
creating our protocols and objectives for protecting Ganymede and
nearby worlds such as Europa from contamination and educating the
public, especially students.
Protecting the solar system from us humans - July 2010 |
Additionally, I
chose to be on the non-icy surfaces team and the instruments team. On
the non-icy surface team, we focused and advocated for studying the
interesting surface and subsurface features that Ganymede has to
offer, that aren't ice. On the instruments team, we determined which
sensors we'd need to carry in order to complete our science
objectives. We had to make difficult choices when we didn't have
enough money, didn't have enough data bandwidth downlink, didn't have
enough power, or was too heavy to carry all that we wanted to fly.
What impressed me
the most about the experience was how quickly we were able to design
a planetary exploration mission to another world. With the help of experts from JPL's Team X, in just a week, we wrote a mission design paper and an
hour-long presentation with technical details and budgets in line
with a NASA New Frontiers program mission. The science objectives of
the GISMO probe were to study:
- the magnetic field
- the interior
- the surface
- the atmosphere
This was my first
time at JPL, so I was glad we also got to see the sights. We got a
tour of the Mars Exploration Rover mission (Spirit and Opportunity)
facilities including rover mock-ups, testbeds, and the controls that
give the rovers their schedule. We saw the Mars Science Laboratory
Curiosity in the clean room before it was launched. It was nice to
roam the campus-like grounds, including spending time with the deer.
We even saw a show at the Hollywood Bowl, BBC's Planet Earth with the
Los Angeles Philharmonic.
Me with a Mars rover mock-up - July 2010 |
Mars rover testbed - July 2010 |
Curiosity on a test run in the JPL cleanroom before its stroll on Mars - July 2010 |
In addition to our
NASA presentation that week, we also presented our paper at the Lunar
and Planetary Science Conference, the American Astronomical Society's
Division for Planetary Science Conference, the American Geophysical
Union conference, and the Institute for Electrical and Electronics
Engineers' Aerospace conference. If there ever is a NASA mission to
Ganymede in the future, I hope that the creators of that mission
build upon what we started with GISMO.
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