Mission Mars Odyssey - 6

<h1>PIA10062: Crater Rim Slump</h1><div class="PIA10062" lang="en" style="width:575px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10062_fig1.jpg"></a><br><b>Context image for PIA10062<br />Crater Rim Slump</b></p><p>This unnamed crater is located in Syrtis Major Planum. The inner portion of the rim at the top of the image has failed in a mode termed 'slump.' A large section has slid to the floor creating a landslide-type deposit and leaving relatively smooth cliff face.<p>Image information: VIS instrument. Latitude 3.8N, Longitude 71.1E. 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/PIA10062" onclick="window.open(this.href); return false;" title="Voir l'image PIA10062: Crater Rim Slump sur le site de la NASA">Voir l'image PIA10062: Crater Rim Slump sur le site de la NASA.</a></div>
PIA10062: Crater Rim Slump
<h1>PIA10063: Olympus Mons</h1><div class="PIA10063" lang="en" style="width:560px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10063_fig1.jpg"></a><br><b>Context image for PIA10063<br />Olympus Mons</b></p><p>Part of the escarpment of the Olympus Mons volcano is shown in this VIS image.<p>Image information: VIS instrument. Latitude 21.3N, Longitude 230.3E. 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/PIA10063" onclick="window.open(this.href); return false;" title="Voir l'image PIA10063: Olympus Mons sur le site de la NASA">Voir l'image PIA10063: Olympus Mons sur le site de la NASA.</a></div>
PIA10063: Olympus Mons
<h1>PIA10064: Aeolis Planum</h1><div class="PIA10064" lang="en" style="width:580px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10064_fig1.jpg"></a><br><b>Context image for PIA10064<br />Aeolis Planum</b></p><p>The linear texture of Aeolis Planum in this VIS image was created by wind erosion.<p>Image information: VIS instrument. Latitude 1.4N, Longitude 141.1E. 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/PIA10064" onclick="window.open(this.href); return false;" title="Voir l'image PIA10064: Aeolis Planum sur le site de la NASA">Voir l'image PIA10064: Aeolis Planum sur le site de la NASA.</a></div>
PIA10064: Aeolis Planum
<h1>PIA10065: Landslide</h1><div class="PIA10065" lang="en" style="width:563px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10065_fig1.jpg"></a><br><b>Context image for PIA10065<br />Landslide</b></p><p>This landslide is lacated within an unnamed crater in Terra Cimmeria.<p>Image information: VIS instrument. Latitude -28.8N, Longitude 136.9E. 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/PIA10065" onclick="window.open(this.href); return false;" title="Voir l'image PIA10065: Landslide sur le site de la NASA">Voir l'image PIA10065: Landslide sur le site de la NASA.</a></div>
PIA10065: Landslide
<h1>PIA10066: Channels</h1><div class="PIA10066" lang="en" style="width:536px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10066_fig1.jpg"></a><br><b>Context image for PIA10066<br />Channels</b></p><p>Many drainage channels are visible in this image of Promethei Terra.<p>Image information: VIS instrument. Latitude -38.1N, Longitude 106.6E. 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/PIA10066" onclick="window.open(this.href); return false;" title="Voir l'image PIA10066: Channels sur le site de la NASA">Voir l'image PIA10066: Channels sur le site de la NASA.</a></div>
PIA10066: Channels
<h1>PIA10067: Dunes</h1><div class="PIA10067" lang="en" style="width:541px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10067_fig1.jpg"></a><br><b>Context image for PIA10067<br />Dunes</b></p><p>This field of dark dunes is located on the western floor of Hale Crater.<p>Image information: VIS instrument. Latitude -35.8N, Longitude 322.8E. 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/PIA10067" onclick="window.open(this.href); return false;" title="Voir l'image PIA10067: Dunes sur le site de la NASA">Voir l'image PIA10067: Dunes sur le site de la NASA.</a></div>
PIA10067: Dunes
<h1>PIA10068: Dao Vallis</h1><div class="PIA10068" lang="en" style="width:567px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10068_fig1.jpg"></a><br><b>Context image for PIA10068<br />Dao Vallis</b></p><p>This VIS image shows a complex portion of the Dao Vallis channel.<p>Image information: VIS instrument. Latitude -35.9N, Longitude 91.9E. 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/PIA10068" onclick="window.open(this.href); return false;" title="Voir l'image PIA10068: Dao Vallis sur le site de la NASA">Voir l'image PIA10068: Dao Vallis sur le site de la NASA.</a></div>
PIA10068: Dao Vallis
<h1>PIA10069: Windstreaks</h1><div class="PIA10069" lang="en" style="width:579px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10069_fig1.jpg"></a><br><b>Context image for PIA10069<br />Windstreaks</b></p><p>This image shows a portion of the Syrtis Major Planum. There are several windstreaks with the classic dark rim/bright interior appearance. Some of the windstreaks also have an additional dark streak oriented further southward than the main streaks. This indicates a change in wind regime in the region.<p>Image information: VIS instrument. Latitude 9.4N, Longitude 69.4E. 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/PIA10069" onclick="window.open(this.href); return false;" title="Voir l'image PIA10069: Windstreaks sur le site de la NASA">Voir l'image PIA10069: Windstreaks sur le site de la NASA.</a></div>
PIA10069: Windstreaks
<h1>PIA10133: Southwest Candor Chasma and Surroundings</h1><div class="PIA10133" lang="en" style="width:800px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10133_fig1.jpg"></a><br />Annotated Version</p><p>This view, covering an area approximately 580 kilometers (360 miles) wide, includes the southwestern portion of Mars's Candor Chasma, part of the large canyon system named Valles Marineris.</p><p>The image is excerpted from a larger image (available at <a href="http://themis.asu.edu/zoom-20041008A">http://themis.asu.edu/zoom-20041008A</a>) based on observations by the Thermal Emission Imaging System camera on NASA's Mars Odyssey orbiter.</p><p>The annotated version shows the location of a study area within Mars' Candor Chasma within regional context.</p><p>Rock layers in the indicated study area have been observed by the High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter.</p><p>Illumination is from the left, and north is up.<br /><br /><a href="http://photojournal.jpl.nasa.gov/catalog/PIA10133" onclick="window.open(this.href); return false;" title="Voir l'image PIA10133: Southwest Candor Chasma and Surroundings sur le site de la NASA">Voir l'image PIA10133: Southwest Candor Chasma and Surroundings sur le site de la NASA.</a></div>
PIA10133: Southwest Candor Chasma and Surroundings
<h1>PIA10150: Hypansis Vallis</h1><div class="PIA10150" lang="en" style="width:582px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10150_fig1.jpg"></a><br><b>Context image for PIA10150<br />Hypansis Vallis</b></p><p>The channel in this VIS image is called Hypansis Vallis.<p>Image information: VIS instrument. Latitude 9.9N, Longitude 314.1E. 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/PIA10150" onclick="window.open(this.href); return false;" title="Voir l'image PIA10150: Hypansis Vallis sur le site de la NASA">Voir l'image PIA10150: Hypansis Vallis sur le site de la NASA.</a></div>
PIA10150: Hypansis Vallis
<h1>PIA10151: Argyre Dunes</h1><div class="PIA10151" lang="en" style="width:539px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10151_fig1.jpg"></a><br><b>Context image for PIA10151<br />Argyre Dunes</b></p><p>The dark dunes in this VIS image are located in western Neredum Montes, near the margin of the Argyre Basin.<p>Image information: VIS instrument. Latitude -41.6N, Longitude 306.7E. 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/PIA10151" onclick="window.open(this.href); return false;" title="Voir l'image PIA10151: Argyre Dunes sur le site de la NASA">Voir l'image PIA10151: Argyre Dunes sur le site de la NASA.</a></div>
PIA10151: Argyre Dunes
<h1>PIA10152: Liu Hsin Crater</h1><div class="PIA10152" lang="en" style="width:567px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10152_fig1.jpg"></a><br><b>Context image for PIA10152<br />Liu Hsin Crater</b></p><p>The western floor of Liu Hsin Crater contains many, small, isolated dark dunes.<p>Image information: VIS instrument. Latitude -53.1N, Longitude 188.0E. 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/PIA10152" onclick="window.open(this.href); return false;" title="Voir l'image PIA10152: Liu Hsin Crater sur le site de la NASA">Voir l'image PIA10152: Liu Hsin Crater sur le site de la NASA.</a></div>
PIA10152: Liu Hsin Crater
<h1>PIA10153: Hydraotes Chaos</h1><div class="PIA10153" lang="en" style="width:580px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10153_fig1.jpg"></a><br><b>Context image for PIA10153<br />Hydraotes Chaos</b></p><p>Different levels of downcutting give a stepped appearance to the mesas in this region of Hydroates Chaos.<p>Image information: VIS instrument. Latitude 1.2N, Longitude 325.5E. 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/PIA10153" onclick="window.open(this.href); return false;" title="Voir l'image PIA10153: Hydraotes Chaos sur le site de la NASA">Voir l'image PIA10153: Hydraotes Chaos sur le site de la NASA.</a></div>
PIA10153: Hydraotes Chaos
<h1>PIA10154: Large Landslide</h1><div class="PIA10154" lang="en" style="width:212px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10154_fig1.jpg"></a><br><b>Context image for PIA10154<br />Large Landslide</b></p><p>The large landslide at the bottom of this INFRARED image is located in Ophir Chasma. Although the resolution is less than a VISIBLE image, the large size of the feature is more completely covered by the wider frame size of the THEMIS infrared camera.<p>Image information: IR instrument. Latitude -6.8N, Longitude 308.2E. 98 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/PIA10154" onclick="window.open(this.href); return false;" title="Voir l'image PIA10154: Large Landslide sur le site de la NASA">Voir l'image PIA10154: Large Landslide sur le site de la NASA.</a></div>
PIA10154: Large Landslide
<h1>PIA10155: Dunes</h1><div class="PIA10155" lang="en" style="width:571px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10155_fig1.jpg"></a><br><b>Context image for PIA10155<br />Dunes</b></p><p>Dark dunes swirl within a crater on the floor of a larger unnamed crater of the margin of Syrtis Major. Small individual dunes are located just outside the rim of the small crater.<p>Image information: VIS instrument. Latitude 3.1N, Longitude 57.6E. 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/PIA10155" onclick="window.open(this.href); return false;" title="Voir l'image PIA10155: Dunes sur le site de la NASA">Voir l'image PIA10155: Dunes sur le site de la NASA.</a></div>
PIA10155: Dunes
<h1>PIA10156: Lava Flows</h1><div class="PIA10156" lang="en" style="width:554px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10156_fig1.jpg"></a><br><b>Context image for PIA10156<br />Lava Flows</b></p><p>The extensive lava flows in this image are part of the Arsia Mons volcanic complex.<p>Image information: VIS instrument. Latitude -21.7N, Longitude 242.4E. 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/PIA10156" onclick="window.open(this.href); return false;" title="Voir l'image PIA10156: Lava Flows sur le site de la NASA">Voir l'image PIA10156: Lava Flows sur le site de la NASA.</a></div>
PIA10156: Lava Flows
<h1>PIA10157: Polar Outliers</h1><div class="PIA10157" lang="en" style="width:390px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10157_fig1.jpg"></a><br><b>Context image for PIA10157<br />Polar Outliers</b></p><p>Something cold for Christmas Day! These layered mounds are south polar layered deposits that are no longer part of the south polar cap. Their location marks a time when the permanent polar cap was more extensive. Happy Holidays from THEMIS!<p>Image information: VIS instrument. Latitude -79.1N, Longitude 95.1E. 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/PIA10157" onclick="window.open(this.href); return false;" title="Voir l'image PIA10157: Polar Outliers sur le site de la NASA">Voir l'image PIA10157: Polar Outliers sur le site de la NASA.</a></div>
PIA10157: Polar Outliers
<h1>PIA10158: Landslides</h1><div class="PIA10158" lang="en" style="width:539px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10158_fig1.jpg"></a><br><b>Context image for PIA10158<br />Landslides</b></p><p>The landslides in this VIS image occur along the eastern cliff of one of the many graben that make up Noctis Labyrinthus.<p>Image information: VIS instrument. Latitude -10.7N, Longitude 265.0E. 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/PIA10158" onclick="window.open(this.href); return false;" title="Voir l'image PIA10158: Landslides sur le site de la NASA">Voir l'image PIA10158: Landslides sur le site de la NASA.</a></div>
PIA10158: Landslides
<h1>PIA10159: Dust Devil Tracks</h1><div class="PIA10159" lang="en" style="width:569px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10159_fig1.jpg"></a><br><b>Context image for PIA10159<br />Dust Devil Tracks</b></p><p>The dust devil tracks in this VIS image are located along Nia Vallis. The Argyre Basin is located to the northwest of this image.<p>Image information: VIS instrument. Latitude -59.7N, Longitude 325.7E. 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/PIA10159" onclick="window.open(this.href); return false;" title="Voir l'image PIA10159: Dust Devil Tracks sur le site de la NASA">Voir l'image PIA10159: Dust Devil Tracks sur le site de la NASA.</a></div>
PIA10159: Dust Devil Tracks
<h1>PIA10160: Canyon Ridges</h1><div class="PIA10160" lang="en" style="width:567px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10160_fig1.jpg"></a><br><b>Context image for PIA10160<br />Canyon Ridges</b></p><p>These majestic ridges and their shadows mark the boundary between the Valles Marineris canyon system and Noctis Labyrinthus.<p>Image information: VIS instrument. Latitude -7.3N, Longitude 266.7E. 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/PIA10160" onclick="window.open(this.href); return false;" title="Voir l'image PIA10160: Canyon Ridges sur le site de la NASA">Voir l'image PIA10160: Canyon Ridges sur le site de la NASA.</a></div>
PIA10160: Canyon Ridges
<h1>PIA10161: Channels</h1><div class="PIA10161" lang="en" style="width:541px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10161_fig1.jpg"></a><br><b>Context image for PIA10161<br />Channels</b></p><p>Channels dissect the nothern rim of this relatively large unnamed crater in northern Terra Cimmeria.<p>Image information: VIS instrument. Latitude -30.9N, Longitude 133.0E. 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/PIA10161" onclick="window.open(this.href); return false;" title="Voir l'image PIA10161: Channels sur le site de la NASA">Voir l'image PIA10161: Channels sur le site de la NASA.</a></div>
PIA10161: Channels
<h1>PIA10162: Timbuktu</h1><div class="PIA10162" lang="en" style="width:551px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10162_fig1.jpg"></a><br><b>Context image for PIA10162<br />Timbuktu</b></p><p>If your New Year's resolution is to travel - try Timbuktu Crater on the margin of Capri Chasma, Mars. The crater hosts a variety of geologic features including fractures, channels, landslides and others. Have a great New Year's Day!<p>Image information: VIS instrument. Latitude -5.7N, Longitude 322.2E. 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/PIA10162" onclick="window.open(this.href); return false;" title="Voir l'image PIA10162: Timbuktu sur le site de la NASA">Voir l'image PIA10162: Timbuktu sur le site de la NASA.</a></div>
PIA10162: Timbuktu
<h1>PIA10163: Confined Flow</h1><div class="PIA10163" lang="en" style="width:564px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10163_fig1.jpg"></a><br><b>Context image for PIA10163<br />Confined Flow</b></p><p>The lava flow in the lower portion on this VIS image is confined within the fault block walls of a graben. The graben are an extension of Sirenum Fossae into Daedalia Planum.<p>Image information: VIS instrument. Latitude -23.7N, Longitude 223.0E. 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/PIA10163" onclick="window.open(this.href); return false;" title="Voir l'image PIA10163: Confined Flow sur le site de la NASA">Voir l'image PIA10163: Confined Flow sur le site de la NASA.</a></div>
PIA10163: Confined Flow
<h1>PIA10164: Dust Devil Tracks</h1><div class="PIA10164" lang="en" style="width:564px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10164_fig1.jpg"></a><br><b>Context image for PIA10164<br />Dust Devil Tracks</b></p><p>These dark tracks mark the passage of dust devils in this region of Terra Sirenum. A major dust storm raged in this region for several months in 2007, many of the tracks may have been formed during that event.<p>Image information: VIS instrument. Latitude -60.1N, Longitude 187.4E. 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/PIA10164" onclick="window.open(this.href); return false;" title="Voir l'image PIA10164: Dust Devil Tracks sur le site de la NASA">Voir l'image PIA10164: Dust Devil Tracks sur le site de la NASA.</a></div>
PIA10164: Dust Devil Tracks
<h1>PIA10165: Wind Power</h1><div class="PIA10165" lang="en" style="width:579px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10165_fig1.jpg"></a><br><b>Context image for PIA10165<br />Wind Power</b></p><p>The power of the wind to reshape the surface is readily exposed in the equatorial region of mars south and east of Olympus Mons. The materials here have been sculpted and resculpted by thousands, if not hundreds of thousand, years of exposure to the wind.<p>Image information: VIS instrument. Latitude 8.2N, Longitude 226.1E. 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/PIA10165" onclick="window.open(this.href); return false;" title="Voir l'image PIA10165: Wind Power sur le site de la NASA">Voir l'image PIA10165: Wind Power sur le site de la NASA.</a></div>
PIA10165: Wind Power
<h1>PIA10250: Arcuate Collapse</h1><div class="PIA10250" lang="en" style="width:550px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10250_fig1.jpg"></a><br><b>Context image for PIA10250<br />Arcuate Collapse</b></p><p>This region near the highland/lowland boundary appears to be breaking into curved-edged blocks. If one looks closely you will see that the block edges are created by arcs of collapse pits which expand until a complete margin is created.<p>Image information: VIS instrument. Latitude -2.2N, Longitude 172.3E. 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/PIA10250" onclick="window.open(this.href); return false;" title="Voir l'image PIA10250: Arcuate Collapse sur le site de la NASA">Voir l'image PIA10250: Arcuate Collapse sur le site de la NASA.</a></div>
PIA10250: Arcuate Collapse
<h1>PIA10251: Ophir Chasma</h1><div class="PIA10251" lang="en" style="width:570px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10251_fig1.jpg"></a><br><b>Context image for PIA10251<br />Ophir Chasma</b></p><p>This region of Ophir Chasma contains old landslide deposits and layered deposits. Wind and perhaps water have sculpted the layered deposits.<p>Image information: VIS instrument. Latitude -3.6N, Longitude 287.5E. 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/PIA10251" onclick="window.open(this.href); return false;" title="Voir l'image PIA10251: Ophir Chasma sur le site de la NASA">Voir l'image PIA10251: Ophir Chasma sur le site de la NASA.</a></div>
PIA10251: Ophir Chasma
<h1>PIA10252: Landslides</h1><div class="PIA10252" lang="en" style="width:542px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10252_fig1.jpg"></a><br><b>Context image for PIA10252<br />Landslides</b></p><p>Landslides are a common feature of Valles Marineris.<p>Image information: VIS instrument. Latitude -13.2N, Longitude 301.3E. 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/PIA10252" onclick="window.open(this.href); return false;" title="Voir l'image PIA10252: Landslides sur le site de la NASA">Voir l'image PIA10252: Landslides sur le site de la NASA.</a></div>
PIA10252: Landslides
<h1>PIA10253: Channels</h1><div class="PIA10253" lang="en" style="width:561px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10253_fig1.jpg"></a><br><b>Context image for PIA10253<br />Channels</b></p><p>Located near Hellas Basin, this crater contains fine scale channels that originate on the rim and appear to have created an alluvial fan. This type of channeled feature is common in the desert southwest of the US.<p>Image information: VIS instrument. Latitude -28.3N, Longitude 84.6E. 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/PIA10253" onclick="window.open(this.href); return false;" title="Voir l'image PIA10253: Channels sur le site de la NASA">Voir l'image PIA10253: Channels sur le site de la NASA.</a></div>
PIA10253: Channels
<h1>PIA10254: Wind Action</h1><div class="PIA10254" lang="en" style="width:569px;text-align:left;margin:auto;background-color:#000;padding:10px;max-height:150px;overflow:auto;"><p><a href="/figures/PIA10254_fig1.jpg"></a><br><b>Context image for PIA10254<br />Wind Action</b></p><p>Long term unidirectional winds have carved grooves into the material of this image. The material may have originated as volcanic ash erupted from Apollonaris Patera, a volcano just out of the image to the south.<p>Image information: VIS instrument. Latitude -7.0N, Longitude 174.2E. 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/PIA10254" onclick="window.open(this.href); return false;" title="Voir l'image PIA10254: Wind Action sur le site de la NASA">Voir l'image PIA10254: Wind Action sur le site de la NASA.</a></div>
PIA10254: Wind Action

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