[meteorite-list] Mars Express Orbiter Buzzes Martian Moon Phobos

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Mon, 30 Dec 2013 15:55:01 -0800 (PST)
Message-ID: <201312302355.rBUNt1Gi028715_at_zagami.jpl.nasa.gov>

http://news.discovery.com/space/mars-express-orbiter-buzzes-martian-moon-phobos-131230.htm

Mars Express Orbiter Buzzes Martian Moon Phobos
by Ian O'Neill
Discovery News
December 30, 2013
 
On Sunday, at 5:17 p.m. GMT (12:17 p.m. EST), Europe's Mars Express orbiter
successfully completed a daring low-pass of Mars? largest moon Phobos.

In an effort to precisely measure the gravitational field of the moon,
the 10 year-old mission was sent on a trajectory that took it only 45
kilometers (28 miles) from the dusty surface, the closest any spacecraft
has ever come to the natural satellite.

At the time of flyby, Mars Express was transmitting a "continuous radio
signal across 208 million km of space" to NASA's radio antennae near Madrid,
Spain, wrote Daniel Scuka at ESA's European Space Operations Centre, Darmstadt,
Germany, in a blog update. The 70 meter radio antenna is part of NASA's
Deep Space Network (DSN), which precisely tracked the spacecraft's signal.
Post-flyby, NASA's 70 meter Goldstone DSN antenna in the Mojave Desert,
Calif., and ESA's 35 meter antenna at New Norcia in Australia continued
to track the mission.

During the flyby, DSN operators reported "a slight effect in the Doppler
residuals," meaning that, as expected, Phobos' gravity had accelerated
Mars Express' orbital velocity very slightly. Through careful analysis
of the Doppler shifting of the radio signal Phobos' gravity can be measured,
allowing scientists to discern its mass and density - the most precise
measurement to date.

All focus was on the spacecraft's ability to send a continuous stream
of data back to Earth, so close-up snapshots were not a possibility.

"In order to perform the Phobos flyby radio science measurements, the
spacecraft needed to have its high gain antenna dish pointed at Earth
for the entire duration of the flyby operations," said Scuka. "This meant
that we were not able to conduct observations with any of the other instruments
(which would need to be pointed at Mars)."

However, the operation allowed the spacecraft to beam back an extra 200
Gigabits of observational data, including imagery of Phobos during an
earlier 500 kilometer pass of the moon.

The successful flyby marks the end of months of planning by the ESA team
managing Mars Express that, as of last week, has been in Mars orbit for
10 years. This flyby opportunity will hopefully provide further clues
to the origin of the knobbly 13.4 kilometer (8.3 mile) wide moon that
orbits Mars only 6,000 kilometers (3,700 miles) from the planet's surface.

By precisely measuring the gravitational influence on a spacecraft during
flyby, planetary scientists will better understand the moon's composition.
During previous flybys, scientists calculated that the moon must be one-third
empty space, which means the object may be a "rubble pile" - an agglomeration
of smaller rocks hold together under a mutual gravity. But did the material
come from a cataclysmic Mars impact? Or was Phobos, and its smaller satellite
sibling Deimos, once an asteroid that got captured by Mars' gravity?

Those answers may not come until we can carry out a dedicated sample return
mission of the moon's regolith, but the flyby will certainly aid our understanding
of Phobos' internal structure.
Received on Mon 30 Dec 2013 06:55:01 PM PST