[meteorite-list] Fresh Look At Dwarf Planet Ceres

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Tue Oct 10 19:09:30 2006
Message-ID: <200610102309.QAA13478_at_zagami.jpl.nasa.gov>

http://news.bbc.co.uk/1/hi/sci/tech/6037844.stm

Fresh look at dwarf planet Ceres
By Molly Bentley
BBC News
October 10, 2006

First impressions count - unless you're Ceres.

Last month, the asteroid was re-classified as a dwarf planet by the
International Astronomical Union (IAU), and now new images of its
surface reveal a surprisingly diverse surface terrain, scientists say.

"We thought Ceres had a flat surface," said Benoit Carry, from the
Observatoire Paris-Meudon, "but our images show that it is rich in
surface features."

Carry's team has produced 360 infrared images of Ceres while observing
it in rotation at the Keck observatory in Mauna Kea.

The results were presented here at the Division of Planetary Sciences
meeting in Pasadena, California.

The subdued black and white images, which map 80% of the dwarf planet,
suggest a textured surface, but not its physical properties.

Dark and bright spots in the images might be crater impacts, mineral
deposits or the effects of space weathering, said Mr Carry.

3D model

The images are the first of an asteroid/dwarf planet using infrared and
advanced adaptive optics, a technique that uses deformable mirrors on a
telescope to correct the blurring caused by turbulence in Earth's
atmosphere.

"Imagine looking at a coin at the bottom of a pool of water," said
Christophe Dumas, an astronomer from the European Southern Observatory
(Eso), "that's exactly what's happening with an astronomical image; it's
all distorted."

Adaptive optics corrects for the distortion in real time. The success of
the combined technique on Ceres recommends its use on other relatively
small objects, such as the large asteroid Vesta, said Dr Dumas.

The infrared images were also used to create the first colourful 3D
model of Ceres. The blue in the 3D model corresponds to the dark patches
in the infrared, the yellow to the bright. The blackout at the edges is
due to insufficient data at the poles.

The ground-based infrared images are not as sharp as those captured in
the visible wavelength by the Hubble Space Telescope in 2002-2003, but,
when compared, the two sets provide a "perfect match" of surface
features, said Dr Dumas.

Making the grade

The Keck results also support Ceres' suspected oblate shape, which
scientists say could be the result of as much as 25% water ice in it
mantle. If so, the amount may be greater than all the fresh water on Earth.

"We think Ceres still contains pristine water from when the Solar System
was formed," said Dr Dumas.

If there was water in the interior, it might be migrating to the surface
through natural channels, he said, collecting minerals along with it,
and perhaps contributing to the mottled pattern in the Keck images.

The next step is to use spectral analysis to decode the chemical
composition of the surface, he said.

Whatever its composition, Ceres never accumulated enough of it to make
planetary grade, by today's standards. It missed being a planet "by that
much," said Mr Carry.

But that wasn't always the case. Once the largest main-belt asteroid,
now the smallest recognised dwarf planet, Ceres was originally
classified as a planet when Sicilian astronomer Father Giuseppe Piazzi
discovered it in 1801.

The US space agency is preparing a spacecraft known as Dawn. It is set
for launch next year and will use an ion engine to visit the asteroid
Vesta in 2011, and Ceres in 2015.
Received on Tue 10 Oct 2006 07:09:28 PM PDT