[meteorite-list] SMART-1 Images: Tectonic 'Wrinkles' in Crater De Gasparis

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Wed Mar 22 21:17:41 2006
Message-ID: <200603221854.k2MIsBG28145_at_zagami.jpl.nasa.gov>

http://www.esa.int/SPECIALS/SMART-1/SEME93OVGJE_0.html

Tectonic 'wrinkles' in Crater De Gasparis
SMART-1
European Space Agency
22 March 2006

This image, taken by the Advanced Moon Imaging Experiment (AMIE) on
board ESA's SMART-1 spacecraft, shows Crater De Gasparis on the Moon.
 
The AMIE camera obtained this image on 14 January 2006 from a distance
of about 1090 kilometres with a ground resolution of approximately 100
metres per pixel.

Crater De Gasparis is located close to the Mare Humorum, at longitude
51.2? West and latitude 26.0? South, on the lower left quarter of the
Moon's Earth-facing side. It has a diameter of about 30 kilometres and
can be seen with the naked eye from Earth.

The criss-cross patterns in it are called "rilles" (these are features
where the surface has sunk down to form a trench).

These rilles coincide with deep tectonic faults that have been active
over a long period of lunar geological evolution. They are the result of
stresses due to all the tidal forces and volcanic expansion over the
lunar mantle during the last stages of lava flooding of Oceanus
Procellarum.

The fact that the rilles cross the crater means that they formed after
the crater. This is a good example for how geologists can determine the
relative history of the Moon's surface.

This crater is named after the Italian astronomer Annibale de Gasparis
(1819-1892). De Gasparis was director of the observatory in Naples, Italy.

 
 
For more information:
 
Jean-Luc Josset, SPACE-X Space Exploration Institute
E-mail: jean-luc.josset _at_ space-x.ch

Bernard H. Foing, ESA SMART-1 Project Scientist
E-mail: bernard.foing _at_ esa.int
Received on Wed 22 Mar 2006 01:54:10 PM PST