Released 22 April 2004

Our group is from Saratoga Springs, NY and is called the Saratoga Springs NASA Club. It contains approximately 30 students between 9th and 12th grade who have been participating since September of 2001. We also worked with a small group of students from Chekhov, Russia in order to do a joint MSIP project. Chekhov is the sister city of Saratoga Springs. Their group contains kids of the same age group as our NASA Club. Our group, along with a few students from the Chekhov branch, visited Arizona State University in November of 2003.

The image we targeted is in the Southern Hemisphere and is at -67 degrees N.

We chose this area because of the presence of craters in the vicinity, which we hope will help with our thesis about the presence of craters that contain lobates as use for evidence that there might once have been water in this area.

This image is causing us considerable difficulty due to the presence of a structure that resembles a lake located in the center of the crater.

Image information: VIS instrument. Latitude -67.1, Longitude 55.3 East (304.7 West). 19 meter/pixel resolution.

NASA and Arizona State University's Mars Education Program is offering students nationwide the opportunity to be involved in authentic Mars research by participating in the Mars Student Imaging Project (MSIP). Teams of students in grades 5 through college sophomore level have the opportunity to work with scientists, mission planners and educators on the THEMIS team at ASU's Mars Space Flight Facility, to image a site on Mars using the THEMIS visible wavelength camera. For more information go to the MSIP website: http://msip.asu.edu.

Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.