Mission Mars Odyssey - 1

<h1>PIA01147: Craters on Crater</h1><div class="PIA01147" lang="en" style="width:553px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01147_fig1.jpg"></a><br><b>Context image for PIA01147<br />Craters on Crater</b></p><p>Several craters were formed on the rim of this large crater. The movement of material downhill toward the floor of the large crater has formed interesting patterns on the floors of the smaller craters.</p><p>Image information: VIS instrument. Latitude -37.8N, Longitude 200.9E. 17 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01147" onclick="window.open(this.href); return false;" title="Voir l'image PIA01147: Craters on Crater sur le site de la NASA">Voir l'image PIA01147: Craters on Crater sur le site de la NASA.</a></div>
PIA01147: Craters on Crater
<h1>PIA01148: Big Fracture</h1><div class="PIA01148" lang="en" style="width:585px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01148_fig1.jpg"></a><br><b>Context image for PIA01148<br />Big Fracture</b></p><p>This large fracture occurs on the lava flows of Ceraunius Tholus.</p><p>Image information: VIS instrument. Latitude 23.1N, Longitude 267.1E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01148" onclick="window.open(this.href); return false;" title="Voir l'image PIA01148: Big Fracture sur le site de la NASA">Voir l'image PIA01148: Big Fracture sur le site de la NASA.</a></div>
PIA01148: Big Fracture
<h1>PIA01213: Noctis Labyrinthus</h1><div class="PIA01213" lang="en" style="width:559px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01213_fig1.jpg"></a><br><b>Context image for PIA01213<br />Noctis Labyrinthus</b></p><p>Sand sheets cover most of the walls and floors of this part of Noctis Labyrinthus.</p><p>Image information: VIS instrument. Latitude -5.7N, Longitude 264.3E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01213" onclick="window.open(this.href); return false;" title="Voir l'image PIA01213: Noctis Labyrinthus sur le site de la NASA">Voir l'image PIA01213: Noctis Labyrinthus sur le site de la NASA.</a></div>
PIA01213: Noctis Labyrinthus
<h1>PIA01214: Ascraeus Mons</h1><div class="PIA01214" lang="en" style="width:567px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01214_fig1.jpg"></a><br><b>Context image for PIA01214<br />Ascraeus Mons</b></p><p>This image shows a small portion of the flank of Ascraeus Mons.</p><p>Image information: VIS instrument. Latitude 10.7N, Longitude 258.5E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01214" onclick="window.open(this.href); return false;" title="Voir l'image PIA01214: Ascraeus Mons sur le site de la NASA">Voir l'image PIA01214: Ascraeus Mons sur le site de la NASA.</a></div>
PIA01214: Ascraeus Mons
<h1>PIA01215: Noachis Terra</h1><div class="PIA01215" lang="en" style="width:552px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01215_fig1.jpg"></a><br><b>Context image for PIA01215<br />Noachis Terra</b></p><p>This closed depression is located in Noachis Terra. To the south a channel leads to second region of erosion.</p><p>Image information: VIS instrument. Latitude -46.4N, Longitude 5.1E. 17 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01215" onclick="window.open(this.href); return false;" title="Voir l'image PIA01215: Noachis Terra sur le site de la NASA">Voir l'image PIA01215: Noachis Terra sur le site de la NASA.</a></div>
PIA01215: Noachis Terra
<h1>PIA01242: Sand Dunes</h1><div class="PIA01242" lang="en" style="width:550px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01242_fig1.jpg"></a><br><b>Context image for PIA01242<br />Sand Dunes</b></p><p>This extensive dune field in located on the floor of a large unnamed crater in Noachis Terra.</p><p>Image information: VIS instrument. Latitude -43.7N, Longitude 34.7E. 17 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01242" onclick="window.open(this.href); return false;" title="Voir l'image PIA01242: Sand Dunes sur le site de la NASA">Voir l'image PIA01242: Sand Dunes sur le site de la NASA.</a></div>
PIA01242: Sand Dunes
<h1>PIA01293: Cavi Angusti</h1><div class="PIA01293" lang="en" style="width:149px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01293_fig1.jpg"></a><br><b>Context image for PIA01293<br />Cavi Angusti</b></p><p>This region of plateaus near the south polar cap is called Cavi Angusti.</p><p>Image information: VIS instrument. Latitude -76.1N, Longitude 283.0E. 35 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01293" onclick="window.open(this.href); return false;" title="Voir l'image PIA01293: Cavi Angusti sur le site de la NASA">Voir l'image PIA01293: Cavi Angusti sur le site de la NASA.</a></div>
PIA01293: Cavi Angusti
<h1>PIA01294: Melas Chasma</h1><div class="PIA01294" lang="en" style="width:551px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01294_fig1.jpg"></a><br><b>Context image for PIA01294<br />Melas Chasma</b></p><p>This image shows part of the floor of Melas Chasma. Layered materials and sand are common in this section of canyon.</p><p>Image information: VIS instrument. Latitude -12.2N, Longitude 287.8E. 17 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01294" onclick="window.open(this.href); return false;" title="Voir l'image PIA01294: Melas Chasma sur le site de la NASA">Voir l'image PIA01294: Melas Chasma sur le site de la NASA.</a></div>
PIA01294: Melas Chasma
<h1>PIA01307: Ascraeus Mons</h1><div class="PIA01307" lang="en" style="width:574px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01307_fig1.jpg"></a><br><b>Context image for PIA01307<br />Ascraeus Mons</b></p><p>These lava flows and collapse features are part of Ascraeus Mons.</p><p>Image information: VIS instrument. Latitude 17.6N, Longitude 262.9E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01307" onclick="window.open(this.href); return false;" title="Voir l'image PIA01307: Ascraeus Mons sur le site de la NASA">Voir l'image PIA01307: Ascraeus Mons sur le site de la NASA.</a></div>
PIA01307: Ascraeus Mons
<h1>PIA01312: Coprates Chasma</h1><div class="PIA01312" lang="en" style="width:548px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01312_fig1.jpg"></a><br><b>Context image for PIA01312<br />Coprates Chasma</b></p><p>This image shows part of Coprates Chasma.</p><p>Image information: VIS instrument. Latitude -15.3N, Longitude 301.2E. 17 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01312" onclick="window.open(this.href); return false;" title="Voir l'image PIA01312: Coprates Chasma sur le site de la NASA">Voir l'image PIA01312: Coprates Chasma sur le site de la NASA.</a></div>
PIA01312: Coprates Chasma
<h1>PIA01313: Ceraunius Tholus</h1><div class="PIA01313" lang="en" style="width:577px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01313_fig1.jpg"></a><br><b>Context image for PIA01313<br />Ceraunius Tholus</b></p><p>This image shows part of the summit caldera of Ceraunius Tholus. Channels are common on the flanks of this volcano.</p><p>Image information: VIS instrument. Latitude 23.9N, Longitude 262.7E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01313" onclick="window.open(this.href); return false;" title="Voir l'image PIA01313: Ceraunius Tholus sur le site de la NASA">Voir l'image PIA01313: Ceraunius Tholus sur le site de la NASA.</a></div>
PIA01313: Ceraunius Tholus
<h1>PIA01314: Two Craters</h1><div class="PIA01314" lang="en" style="width:556px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01314_fig1.jpg"></a><br><b>Context image for PIA01314<br />Two Craters</b></p><p>The two craters in this image are located in Zephyria Planum. The crater floors appear to be modified only by deposits of fine materials.</p><p>Image information: VIS instrument. Latitude 0.3N, Longitude 155.5E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01314" onclick="window.open(this.href); return false;" title="Voir l'image PIA01314: Two Craters sur le site de la NASA">Voir l'image PIA01314: Two Craters sur le site de la NASA.</a></div>
PIA01314: Two Craters
<h1>PIA01315: Resistant Ridges</h1><div class="PIA01315" lang="en" style="width:546px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01315_fig1.jpg"></a><br><b>Context image for PIA01315<br />Resistant Ridges</b></p><p>The ridges on the floor of this crater are made of a more resistant material that their surroundings. Erosion is removing the less resistant material.</p><p>Image information: VIS instrument. Latitude -19.4N, Longitude 66.3E. 17 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01315" onclick="window.open(this.href); return false;" title="Voir l'image PIA01315: Resistant Ridges sur le site de la NASA">Voir l'image PIA01315: Resistant Ridges sur le site de la NASA.</a></div>
PIA01315: Resistant Ridges
<h1>PIA01316: Lycus Sulci</h1><div class="PIA01316" lang="en" style="width:571px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01316_fig1.jpg"></a><br><b>Context image for PIA01316<br />Lycus Sulci</b></p><p>Lycus Sulci is a complex area of ridges and valleys that surrounds the northern and western margins of Olympus Mons. How it formed is unknown.<p>Image information: VIS instrument. Latitude 20.7N, Longitude 211.3E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01316" onclick="window.open(this.href); return false;" title="Voir l'image PIA01316: Lycus Sulci sur le site de la NASA">Voir l'image PIA01316: Lycus Sulci sur le site de la NASA.</a></div>
PIA01316: Lycus Sulci
<h1>PIA01325: Different Textures</h1><div class="PIA01325" lang="en" style="width:577px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01325_fig1.jpg"></a><br><b>Context image for PIA01325<br />Different Textures</b></p><p>From smooth topped mesas to rugged lowlands, this region of Mars near Huo Hsing Vallis presents several different surface textures.<p>Image information: VIS instrument. Latitude 29.6N, Longitude 67.2E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01325" onclick="window.open(this.href); return false;" title="Voir l'image PIA01325: Different Textures sur le site de la NASA">Voir l'image PIA01325: Different Textures sur le site de la NASA.</a></div>
PIA01325: Different Textures
<h1>PIA01326: Radial Grooves</h1><div class="PIA01326" lang="en" style="width:587px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01326_fig1.jpg"></a><br><b>Context image for PIA01326<br /> Radial Grooves</b></p><p>The surface of the ejecta surrounding this crater is scored with fine radial grooves. The grooves were formed during the impact event.</p><p>Image information: VIS instrument. Latitude 34.8N, Longitude 102.4E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01326" onclick="window.open(this.href); return false;" title="Voir l'image PIA01326: Radial Grooves sur le site de la NASA">Voir l'image PIA01326: Radial Grooves sur le site de la NASA.</a></div>
PIA01326: Radial Grooves
<h1>PIA01327: Aram Chaos</h1><div class="PIA01327" lang="en" style="width:564px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01327_fig1.jpg"></a><br><b>Context image for PIA01327<br />Aram Chaos</b></p><p>Aram Chaos is a complex region which contains layered material with different surface textures and heavily fractured material forming chaos.<p>Image information: VIS instrument. Latitude 1.7N, Longitude 340.0E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01327" onclick="window.open(this.href); return false;" title="Voir l'image PIA01327: Aram Chaos sur le site de la NASA">Voir l'image PIA01327: Aram Chaos sur le site de la NASA.</a></div>
PIA01327: Aram Chaos
<h1>PIA01328: Eumenides Dorsum</h1><div class="PIA01328" lang="en" style="width:569px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01328_fig1.jpg"></a><br><b>Context image for PIA01328<br />Eumenides Dorsum</b></p><p>In this image the action of the wind is forming yardangs. The top layer of material is being removed by the wind, revealing an older surface below -- like the crater at the bottom of the frame.<p>Image information: VIS instrument. Latitude 11.2N, Longitude 199.4E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01328" onclick="window.open(this.href); return false;" title="Voir l'image PIA01328: Eumenides Dorsum sur le site de la NASA">Voir l'image PIA01328: Eumenides Dorsum sur le site de la NASA.</a></div>
PIA01328: Eumenides Dorsum
<h1>PIA01329: Alba Patera</h1><div class="PIA01329" lang="en" style="width:602px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01329_fig1.jpg"></a><br><b>Context image for PIA01329<br />Alba Patera</b></p><p>These lava flows and channels are part of Alba Patera, a large collapsed volcano in the Tharsis region.<p>Image information: VIS instrument. Latitude 44.0N, Longitude 244.8E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01329" onclick="window.open(this.href); return false;" title="Voir l'image PIA01329: Alba Patera sur le site de la NASA">Voir l'image PIA01329: Alba Patera sur le site de la NASA.</a></div>
PIA01329: Alba Patera
<h1>PIA01358: Flow and Fracture</h1><div class="PIA01358" lang="en" style="width:569px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01358_fig1.jpg"></a><br><b>Context image for PIA01358<br />Flow and Fracture</b></p><p>In this part of the Tharsis region, old lava flows have been fractured. Younger lava flows are unfractured (flow at bottom).<p>Image information: VIS instrument. Latitude 9.3N, Longitude 282.2E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01358" onclick="window.open(this.href); return false;" title="Voir l'image PIA01358: Flow and Fracture sur le site de la NASA">Voir l'image PIA01358: Flow and Fracture sur le site de la NASA.</a></div>
PIA01358: Flow and Fracture
<h1>PIA01359: Hide and Seek</h1><div class="PIA01359" lang="en" style="width:565px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01359_fig1.jpg"></a><br><b>Context image for PIA01359<br />Hide and Seek</b></p><p>Exhumation of craters, the uncovering of old craters hidden from view by younger surface material, is common in many regions of Mars. This crater and its covering material are located in Amazonis Planitia.<p>Image information: VIS instrument. Latitude 3.7N, Longitude 194.9E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01359" onclick="window.open(this.href); return false;" title="Voir l'image PIA01359: Hide and Seek sur le site de la NASA">Voir l'image PIA01359: Hide and Seek sur le site de la NASA.</a></div>
PIA01359: Hide and Seek
<h1>PIA01396: Funky Floors</h1><div class="PIA01396" lang="en" style="width:583px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01396_fig1.jpg"></a><br><b>Context image for PIA01396<br />Funky Floors</b></p><p>The material covering the floors of these two craters looks very different from the surrounds. The unusual markings of the floor material indicates that a volatile, such as ice, has affected the appearance of the surface.<p>Image information: VIS instrument. Latitude 29.7N, Longitude 54.3E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01396" onclick="window.open(this.href); return false;" title="Voir l'image PIA01396: Funky Floors sur le site de la NASA">Voir l'image PIA01396: Funky Floors sur le site de la NASA.</a></div>
PIA01396: Funky Floors
<h1>PIA01707: Northern Crater</h1><div class="PIA01707" lang="en" style="width:604px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01707_fig1.jpg"></a><br><b>Context image for PIA01707<br />Northern Crater</b></p><p>Many craters in the northern plains look like the one in this image -- interior filled almost to the rim, narrow and steep ejecta surrounding the rim, little or no remaining distant ejecta. It is assumed that the climate in the region has affected the appearance of these craters.<p>Image information: VIS instrument. Latitude 52.5N, Longitude 186.3E. 20 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01707" onclick="window.open(this.href); return false;" title="Voir l'image PIA01707: Northern Crater sur le site de la NASA">Voir l'image PIA01707: Northern Crater sur le site de la NASA.</a></div>
PIA01707: Northern Crater
<h1>PIA01771: Flank Flows</h1><div class="PIA01771" lang="en" style="width:578px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01771_fig1.jpg"></a><br><b>Context image for PIA01771<br />Flank Flows</b></p><p>The narrow, channelized lava flows in this image occur on the flank of Olympus Mons.<p>Image information: VIS instrument. Latitude 15.9N, Longitude 223.1E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01771" onclick="window.open(this.href); return false;" title="Voir l'image PIA01771: Flank Flows sur le site de la NASA">Voir l'image PIA01771: Flank Flows sur le site de la NASA.</a></div>
PIA01771: Flank Flows
<h1>PIA01772: Graben</h1><div class="PIA01772" lang="en" style="width:603px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01772_fig1.jpg"></a><br><b>Context image for PIA01772<br />Graben</b></p><p>Paired fractures with a downdropped block between them are termed graben. Graben are common on Alba Patera, where this image is located.<p>Image information: VIS instrument. Latitude 43.7N, Longitude 245.8E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01772" onclick="window.open(this.href); return false;" title="Voir l'image PIA01772: Graben sur le site de la NASA">Voir l'image PIA01772: Graben sur le site de la NASA.</a></div>
PIA01772: Graben
<h1>PIA01773: Deuteronilus</h1><div class="PIA01773" lang="en" style="width:603px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01773_fig1.jpg"></a><br><b>Context image for PIA01773<br />Deuteronilus</b></p><p>The martian region called Deuteronilus is characterized by hills and mesas surrounded by broad debris slopes. Some of the slopes have surface markings that may indicate volatiles are mixed in with the debris.<p>Image information: VIS instrument. Latitude 41.9N, Longitude 18.1E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01773" onclick="window.open(this.href); return false;" title="Voir l'image PIA01773: Deuteronilus sur le site de la NASA">Voir l'image PIA01773: Deuteronilus sur le site de la NASA.</a></div>
PIA01773: Deuteronilus
<h1>PIA01774: Acheron Fossae</h1><div class="PIA01774" lang="en" style="width:593px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01774_fig1.jpg"></a><br><b>Context image for PIA01774<br />Acheron Fossae</b></p><p>This heavily dissected surface is located within the Acheron Fossae region.<p>Image information: VIS instrument. Latitude 34.5N, Longitude 218.9E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01774" onclick="window.open(this.href); return false;" title="Voir l'image PIA01774: Acheron Fossae sur le site de la NASA">Voir l'image PIA01774: Acheron Fossae sur le site de la NASA.</a></div>
PIA01774: Acheron Fossae
<h1>PIA01864: Aeolis Planum</h1><div class="PIA01864" lang="en" style="width:559px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01864_fig1.jpg"></a><br><b>Context image for PIA01864<br />Aeolis Planum</b></p><p>The wind is eroding some of the materials in this region more readily than others, indicating a complex surface history.<p>Image information: VIS instrument. Latitude -3.1N, Longitude 145.5E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01864" onclick="window.open(this.href); return false;" title="Voir l'image PIA01864: Aeolis Planum sur le site de la NASA">Voir l'image PIA01864: Aeolis Planum sur le site de la NASA.</a></div>
PIA01864: Aeolis Planum
<h1>PIA01865: Wind and Lava</h1><div class="PIA01865" lang="en" style="width:566px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01865_fig1.jpg"></a><br><b>Context image for PIA01865<br />Wind and Lava</b></p><p>In this image wind seems to be the dominant process, but lava flows are still recognizable from the surface texture. It appears that the lava flow (top left) is relatively thin, and the material below is easily eroded by the wind.<p>Image information: VIS instrument. Latitude 8.5N, Longitude 233.6E. 18 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01865" onclick="window.open(this.href); return false;" title="Voir l'image PIA01865: Wind and Lava sur le site de la NASA">Voir l'image PIA01865: Wind and Lava sur le site de la NASA.</a></div>
PIA01865: Wind and Lava
<h1>PIA01866: Sacra Mensa</h1><div class="PIA01866" lang="en" style="width:578px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA01866_fig1.jpg"></a><br><b>Context image for PIA01866<br />Sacra Mensa</b></p><p>Tectonic activity in this region has not only fractured the surface, but has tilted some of the fracture blocks.<p>Image information: VIS instrument. Latitude 24.6N, Longitude 293.5E. 19 meter/pixel resolution.</p><p>Please see the <a href="http://themis.asu.edu/terms" target="_blank">THEMIS Data Citation Note</a> for details on crediting THEMIS images.</p><p>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.</p><p>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.</p><br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA01866" onclick="window.open(this.href); return false;" title="Voir l'image PIA01866: Sacra Mensa sur le site de la NASA">Voir l'image PIA01866: Sacra Mensa sur le site de la NASA.</a></div>
PIA01866: Sacra Mensa

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