|
Collection:
|
|
NASA Planetary Photo Journal Collection
Collection
NASA Planetary Photo Journal Collection
Collection
|
|
Title:
|
|
Final Noctis
|
|
Original Caption Released with Image:
|
Context image for PIA09975 Final Noctis The major Martian dust storm of 2007 filled the sky with dust and produced conditions that prevented the THEMIS VIS camera from being able to image the surface. With no new images being acquired, we've dug into the archive to highlight some interesting areas on Mars. The this week's region is Noctis Labyrinthus. Noctis Labyrinthus is located at the western end of Valles Marineris. This maze-like feature of deep intersecting valleys was formed by tectonic forces and extensive faulting. Image information: VIS instrument. Latitude -7.5N, Longitude 259.1E. 18 meter/pixel resolution. Please see the THEMIS Data Citation Note for details on crediting THEMIS images. Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time. NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.
Original_Caption_Rel eased_with_Image
Context image for PIA09975 Final Noctis The major Martian dust storm of 2007 filled the sky with dust and produced conditions that prevented the THEMIS VIS camera from being able to image the surface. With no new images being acquired, we've dug into the archive to highlight some interesting areas on Mars. The this week's region is Noctis Labyrinthus. Noctis Labyrinthus is located at the western end of Valles Marineris. This maze-like feature of deep intersecting valleys was formed by tectonic forces and extensive faulting. Image information: VIS instrument. Latitude -7.5N, Longitude 259.1E. 18 meter/pixel resolution. Please see the THEMIS Data Citation Note for details on crediting THEMIS images. Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time. NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.
Original Caption Released with Image
|
|
Image Credit:
|
|
NASA/JPL/ASU
Image_Credit
NASA/JPL/ASU
Image Credit
|
|
Produced By:
|
|
Arizona State University
Produced_By
Arizona State University
Produced By
|
|
Mission:
|
|
2001 Mars Odyssey
Mission
2001 Mars Odyssey
Mission
|
|
Spacecraft:
|
|
2001 Mars Odyssey
Spacecraft
2001 Mars Odyssey
Spacecraft
|
|
Target Name:
|
|
Mars
Target_Name
Mars
Target Name
|
|
Is a satellite of:
|
|
Sol (our sun)
Is_a_satellite_of
Sol (our sun)
Is a satellite of
|
|
Instrument:
|
|
Thermal Emission Imaging System
Instrument
Thermal Emission Imaging System
Instrument
|
|
Product Size:
|
|
1297 samples x 2775 lines
Product_Size
1297 samples x 2775 lines
Product Size
|
|
facet_what:
|
|
Sun
facet_what
Sun
facet_what
|
|
facet_what:
|
|
Mars
facet_what
Mars
facet_what
|
|
facet_what:
|
|
2001 Mars Odyssey
facet_what
2001 Mars Odyssey
facet_what
|
|
facet_what:
|
|
Thermal Emission Imaging System (THEMIS)
facet_what
Thermal Emission Imaging System (THEMIS)
facet_what
|
|
facet_where:
|
|
Jet Propulsion Laboratory
facet_where
Jet Propulsion Laboratory
facet_where
|
|
facet_where:
|
|
Denver
facet_where
Denver
facet_where
|
|
facet_where:
|
|
Mars
facet_where
Mars
facet_where
|
|
facet_where:
|
|
Arizona
facet_where
Arizona
facet_where
|
|
facet_where:
|
|
California
facet_where
California
facet_where
|
|
facet_where:
|
|
Washington
facet_where
Washington
facet_where
|
|
facet_where:
|
|
Jet Propulsion Laboratory (JPL)
facet_where
Jet Propulsion Laboratory (JPL)
facet_where
|
|
facet_where:
|
|
Washington, D.C.
facet_where
Washington, D.C.
facet_where
|
|
facet_when:
|
|
2007
facet_when
2007
facet_when
|
|
facet_when_year:
|
|
2007
facet_when_year
2007
facet_when_year
|
|
Image #:
|
|
PIA09975
|
|
UID:
|
|
SPD-PHOTJ-PIA09975
UID
SPD-PHOTJ-PIA09975
UID
|
|
orignial url:
|
orignial_url
orignial url
|
