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Dr. Phil Varghese
August 24, 2004
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NASA/JPL-Caltech
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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
Chasma Boreale is a long, flat-floored valley that cuts deep into Mars' north polar icecap
Mars Odyssey All Stars: Chasma Boreale
This false color image shows a region with craters of different ages located at the margin of Acidalia Planitia. This image was collected during the Northern Spring season.
Cratered Acidalia Planitia
The dunes in this VIS image are located in Aonia Terra.
Dunes in Aonia Terra
This graphic shows the ongoing contributions of NASA’s rovers and orbiters during a Martian dust storm that began on May 30, 2018.
Mars Storm Watch Observations
A "Grand Canyon of Mars" slices across the Red Planet near its equator.
Mars Canyon with Los Angeles for Scale
Ius Chasma is unique from the other chasmata of Valles Marineris in possessing mega gullies on both sides of the chasma. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
Investigating Mars: Ius Chasma
Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data from three different NASA Mars orbiters.
Multiple Instruments Used for Mars Carbon Estimate
Five decades of successful NASA missions to the Red Planet, 1965-2015.
50 Years of Mars Exploration
Buzz Aldrin, an Apollo 11 astronaut who walked on the moon, makes a holographic appearance in 'Destination: Mars,' a mixed-reality tour of a part of Mars that NASA's Curiosity rover has explored.
Buzz Aldrin
This mosaic image of Valles Marineris - colored to resemble the martian surface - comes from the Thermal Emission Imaging System (THEMIS), a visible-light and infrared-sensing camera on NASA's Mars...
The Grand Canyon of Mars-Valles Marineris
Bright blue marks a deposit of chloride (salt) minerals in the southern highlands of Mars in this false-color image, which highlights mineral composition differences.
Chloride Salt Deposit in Southern Highlands of Mars (Annotated)
This image shows the context for orbital observations of exposed rocks that had been buried an estimated 5 kilometers (3 miles) deep on Mars.
Nature's Drilling Exposes Deeply Buried Minerals
This image superimposes Gamma-Ray Spectrometer data from NASA's Mars Odyssey orbiter onto topographic data from the laser altimeter on NASA's Mars Global Surveyor.
Potassium Concentrations on Mars
This image is near the southern edge of a low, broad volcanic feature called Syrtis Major.
Syrtis Major
At the time this video was released, the Odyssey team had successfully completed the third trajectory correction maneuver to adjust the spacecraft's flightpath toward its final aimpoint for entry i...
Challenges of Getting to Mars: Interplanetary Cruise
This image of a crater in Acidalia Planitia was acquired March 8, 2003, during northern summer.
Acidalia Planitia Crater
A sea of dark dunes, sculpted by the wind into long lines, surrounds the northern polar cap covering an area as big as Texas.
Mars Odyssey All Stars: Polar Dunes
Download a PDF of the 2001 Mars Odyssey Arrival Press Kit.
2001 Mars Odyssey Arrival Press Kit
This region of Terra Sabaea contains areas with high densities of small craters.
Lot of Craters in Terra Sabaea
This view of an area about 140 kilometers (about 90 miles) wide in the Meridiani Planum region of Mars shows the region around NASA's Mars Exploration Rover Opportunity.
Orbital View of Opportunity's Region
Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is one of both tectonically fractured rocks (top of image) and volcanic flows (mi...
Echus Chasma
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
Sand-laden jets shoot into the polar sky in this view by noted space artist Ron Miller.
Sand-Laden Jets
Mars radiation levels are two to three times higher than around Earth.
Mars radiation levels
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