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Dr. Phil Varghese
August 24, 2004
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NASA/JPL-Caltech
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Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike.
Mars Odyssey All Stars: Cerberus Crack
This mosaic of infrared images shows the abundance and location of hematite at Opportunity's landing site, Meridiani Planum. On Earth, hematite is a mineral that typically forms in water.
Meridiani Planum
Morning clouds fill Coprates Chasma on Mars in this Nov. 25, 2015, image from the THEMIS camera on NASA's Mars Odyssey. No orbiter systematically observed Mars in morning sunlight before 2015. The ...
Mars Odyssey View of Morning Clouds in Canyon
NASA Science missions circle Earth, the Sun, the Moon, Mars and many other destinations within our solar system, including spacecraft that look out even further into our universe. The Science Fleet...
SMD Spacecraft Fleet
Hills abound in this portion of Mars located in the Vastitas Borealis region of the high northern plains. These hills are part of Scandia Colles. Note that some of the hills have aprons surrounding...
Bumpy Terrain in Vastitas Borealis
Olympica Fossae is a complex channel located on the volcanic plains between Alba Mons and Olympus Mons. The sinuosity of the large channel in the middle of this image from NASA's 2001 Mars Odyssey ...
Olympica Fossae
This image combines two products from the first pointing at the Martian moon Phobos by the THEMIS camera on NASA's Mars Odyssey orbiter, on Sept. 29, 2017. Surface-temperature information from obse...
Temperature Gradient on Martian Moon Phobos
Six views of the Martian moon Phobos captured by NASA's Odyssey orbiter as of March 2020. The orbiter's THEMIS camera is used to measure temperature variations that suggest what kind of material th...
Odyssey's Six Views of Phobos
Mars is experiencing large regional dust storms over its northern hemisphere during the past week.
The Martian Dust Storm of June 2018
NASA is advancing the Journey to Mars by starting the conversation about where humans may one day land on the Red Planet.
Mars Exploration Zone Layout Considerations
The floor of this unnamed crater in Aonia Terra has been filled with multiple layers of material.
Layered Fill
Valleys much younger than well-known ancient valley networks on Mars are evident near the informally named "Heart Lake" on Mars. This map presents color-coded topographical information overlaid ont...
Landscape of Former Lakes and Streams on Northern Mars
Odyssey launched on Boeing's Delta II 7925 that uses nine strap-on solid rocket motors.
Odyssey Launches Boeing's Delta II 7925
In Ares Vallis, teardrop mesas extend like pennants behind impact craters, where the raised rocky rims diverted the floods and protected the ground from erosion.
Mars Odyssey All Stars: Ares Vallis
This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT).
Downslope of the Fan
Mars radiation levels are two to three times higher than around Earth.
Mars radiation levels
Taken on April 24, 2019, this rainbow-colored image shows the Martian moon Phobos, as viewed by NASA's 2001 Mars Odyssey orbiter using its infrared camera, THEMIS. Each color represents a different...
Odyssey Views Phobos: April 24, 2019
First THEMIS Image of Mars
First THEMIS Image of Mars
The channels in this VIS image are part of Tyrrhena Fossae on the northern flank of Tyrrhenus Mons.
Tyrrhena Fossae
This series of images was taken in visible-wavelength light as the THEMIS camera on NASA's Mars Odyssey scanned across the Martian moon Phobos on Sept. 29, 2017. The apparent motion is due to progr...
Series of Images from THEMIS Scanning Phobos
A "Grand Canyon of Mars" slices across the Red Planet near its equator.
Mars Canyon with Los Angeles for Scale
On the southwest edge of the immense volcanic region of Tharsis, lava from its giant volcanoes flowed down to meet the old cratered landscape of Terra Sirenum.
Terra Sirenum
This map of Mars indicates locations of new craters that have excavated ice (blue) and those that have not (red). The underlying map is based on the brightness, or albedo, of the Martian surface.
Locations of Ice-Exposing Fresh Craters on Mars
This view combines information from two instruments on NASA's Mars Reconnaissance Orbiter to map color-coded composition over the shape of the ground in a small portion of the Nili Fossae plains re...
Rocks Here Sequester Some of Mars' Early Atmosphere
2021_WindingTributary.jpg
Winding Side Canyon (Louros Valles)
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