Today's VIS image shows a small section of Mangala Valles. Mangala Valles is a complex channel more than 900km long (560 miles). The channel system starts near Mangala Fossae, a large tectonic feature that intersects the volcanic plains of Daedalia Planum. Like other channels in the region, Mangala Valles flows northward, eventually emptying into southern Amazonis Planitia. Visible at the top of the image are tear-drop shaped hills within the channel. These features are called streamlined islands and the narrow "tail" points down stream.
Orbit Number: 84304 Latitude: -16.0319 Longitude: 210.534 Instrument: VIS Captured: 2020-12-15 20:48
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Science Mission Directorate, 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.
Name | Value | Additional Values |
---|---|---|
Target | Mars | |
System | ||
Target Type | Planet | |
Mission | 2001 Mars Odyssey | |
Instrument Host | Mars Odyssey | |
Host Type | Orbiter | |
Instrument | Thermal Emission Imaging System (THEMIS) | |
Detector | ||
Extra Keywords | Grayscale, Thermal, Volcano | |
Acquisition Date | ||
Release Date | 2021-02-22 | |
Date in Caption | 2020-12-15 | |
Image Credit | NASA/JPL-Caltech/ASU | |
Source | photojournal.jpl.nasa.gov/catalog/PIA24411 | |
Identifier | PIA24411 |