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NASA's
Mars Odyssey Shifting Orbit for Extended Mission
Friday, October 10, 2008
Credit:
NASA / JPL
The longest-serving of six
spacecraft now studying Mars is up to new tricks for a third
two-year extension of its mission to examine the most Earthlike
of known foreign planets.
NASA's Mars Odyssey is altering
its orbit to gain even better sensitivity for its infrared
mapping of Martian minerals. During the mission extension through
September 2010, it will also point its camera with more
flexibility than it has ever used before. Odyssey reached Mars in
2001.
The orbit adjustment will allow Odyssey's Thermal
Emission Imaging System to look down at sites when it's
mid-afternoon, rather than late afternoon. The multipurpose
camera will take advantage of the infrared radiation emitted by
the warmer rocks to provide clues to the rocks' identities.
"This will allow us to do much more sensitive
detection and mapping of minerals," said Odyssey Project
Scientist Jeffrey Plaut of NASA's Jet Propulsion Laboratory,
Pasadena, Calif.
The mission's orbit design before now
used a compromise between what works best for the Thermal
Emission Imaging System and what works best for another
instrument, the Gamma Ray Spectrometer.
On commands from
its operations team at JPL and at Denver-based Lockheed Martin
Space Systems, Odyssey fired thrusters for nearly 6 minutes on
Sept. 30, the final day of the mission's second two-year
extension.
"This was our biggest maneuver since
2002, and it went well," said JPL's Gaylon McSmith, Odyssey
mission manager. "The spacecraft is in good health. The
propellant supply is adequate for operating through at least
2015."
Odyssey's orbit is synchronized with the sun.
The local solar time has been about 5 p.m. at whatever spot on
Mars Odyssey flew over as it made its dozen daily passes from
between the north pole region to the south pole region for the
past five years. (Likewise, the local time has been about 5 a.m.
under the track of the spacecraft during the south-to-north leg
of each orbit.)
The push imparted by the Sept. 30
maneuver will gradually change that synchronization over the next
year or so. Its effect is that the time of day on the ground when
Odyssey is overhead is now getting earlier by about 20 seconds
per day. A follow-up maneuver, probably in late 2009 when the
overpass time is between 2:30 and 3:00 p.m., will end the
progression toward earlier times.
While aiding
performance of the Thermal Emission Imaging System, the shift to
mid-afternoon is expected to stop the use of one of three
instruments in Odyssey's Gamma Ray Spectrometer suite. The
suite's gamma ray detector needs a later-hour orbit to avoid
overheating of a critical component. The suite's neutron
spectrometer and high-energy neutron detector are expected to
keep operating.
The Gamma Ray Spectrometer provided
dramatic discoveries of water-ice near the surface throughout
much of high-latitude Mars, the impetus for NASA's Phoenix Mars
Lander mission. The gamma ray detector has also mapped global
distribution of many elements, such as iron, silicon and
potassium, a high science priority for the first and second
extensions of the Odyssey mission. A panel of planetary
scientists assembled by NASA recommended this year that Odyssey
make the orbit adjustment to get the best science return from the
mission in coming years.
Increased sensitivity for
identifying surface minerals is a key science goal for the
mission extension beginning this month. Also, the Odyssey team
plans to begin occasionally aiming the camera away from the
straight-down pointing that has been used throughout the mission.
This will allow the team to fill in some gaps in earlier mapping
and also create some stereo, three-dimensional imaging.
Odyssey
will continue providing crucial support for Mars surface missions
as well as conducting its own investigations. It has relayed to
Earth nearly all data returned from NASA rovers Spirit and
Opportunity. It shares with NASA's Mars Reconnaissance Orbiter
the relay role for Phoenix. It has made targeted observations for
evaluating candidate landing sites.
Mars Odyssey,
launched in 2001, is managed by JPL, a division of the California
Institute of Technology, Pasadena, for NASA's Science Mission
Directorate, Washington. Lockheed Martin Space Systems, Denver,
is the prime contractor for the project and built the spacecraft.
Investigators at Arizona State University, Tempe, operate the
Thermal Emission Imaging System. Investigators at the University
of Arizona, Tucson, head operation of the Gamma Ray Spectrometer.
Additional science partners are located at the Russian Aviation
and Space Agency, which provided the high-energy neutron
detector, and at Los Alamos National Laboratories, New Mexico,
which provided the neutron spectrometer.
Source:
NASA / JPL

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