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The Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey spacecraft has completed an unprecedented full decade of observing Mars from orbit.
Tenth Anniversary Image from Camera on NASA Mars Orbiter
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
Oblique view of Gale Crater from the North
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
Oblique view of Gale Crater from the North (Unannotated)
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
Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike.
Mars Odyssey All Stars: Cerberus Crack
Wind shadow and real shadow combine to give a striking image of a comet.
THEMIS Images as Art
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
Fans and ribbons of dark sand dunes creep across the floor of Bunge Crater in response to winds blowing from the direction at the top of the picture.
Mars Odyssey All Stars: Bunge Crater Dunes
A false-color mosaic focuses on one junction in Noctis Labyrinthus where canyons meet to form a depression 4,000 meters (13,000 feet) deep.
Mars Odyssey All Stars: Noctis Canyon
West of Valles Marineris lies a checkerboard named Noctis Labyrinthus, which formed when the Martian crust stretched and fractured.
Mars Odyssey All Stars: Noctis Vista
Although it is 45 kilometers (28 miles) wide, countless layers of ice and dust have all but buried Udzha Crater.
Mars Odyssey All Stars: Udzha Crater
Sand dunes shaped like blue-black flames lie next to a central hill within an unnamed, 120-kilometer-wide (75-mile-wide) crater in eastern Arabia on Mars.
Mars Odyssey All Stars: Arabia Dunes
Chasma Boreale is a long, flat-floored valley that cuts deep into Mars' north polar icecap
Mars Odyssey All Stars: Chasma Boreale
If a meteorite breaks in two shortly before hitting the ground, the typical bowl shape of a single impact crater becomes doubled.
Mars Odyssey All Stars: Dual Crater
A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 meters (3,300 feet) wide.
Mars Odyssey All Stars: Dunes Engulf 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
Although this may look like a hostile alien life form, it's actually a complex line of sand dunes near the northern ice cap of Mars.
Mars Odyssey All Stars: Reptilian Dunes
Bacolor Crater is a magnificent impact feature about 20 kilometers (12 miles) wide.
Mars Odyssey All Stars: Bacolor Crater
Mars Odyssey Project Manager Gaylon McSmith, of NASA's Jet Propulsion Laboratory
Mars Odyssey Project Manager Gaylon McSmith
Valles Marineris, the "Grand Canyon of Mars," sprawls wide enough to reach from Los Angeles to nearly New York City, if it were located on Earth. The red outline box shows the location of a second, full-resolution image.
Valles Marineris, the "Grand Canyon of Mars"
This image shows a 90-mile-wide portion of the giant Valles Marineris canyon system. Landslide debris and gullies in the canyon walls on Mars can be seen at 100 meters (330 feet) per pixel.
Close View of Valles Marineris
Martian Pit Feature Found by Seventh Graders
Martian Pit Feature Found by Seventh Graders
Orbital View of Opportunity's Region
Orbital View of Opportunity's Region
Stages in the seasonal disappearance of surface ice from the ground around the Phoenix Mars Lander are visible in these images taken on Feb. 8, 2010, (left) and Feb. 25, 2010, during springtime on northern Mars.
Ice Around Phoenix Lander Continues to Lessen in Spring
Phoenix Lander Amid Disappearing Spring Ice
Phoenix Lander Amid Disappearing Spring Ice
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