The volcanic flows in image from NASA's 2001 Mars Odyssey spacecraft are located south of Ascraeus Mons and east of Pavonis Mons.

The volcanic flows in image from NASA's 2001 Mars Odyssey spacecraft are located south of Ascraeus Mons and east of Pavonis Mons.
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Today's VIS image shows a section of Ares Vallis. Ares Vallis is a large channel that arises in Iani Chaos, passes through Margaritifer Terra, and then empties into Chryse Planitia. Orbit Number 80624 Latitude 0.445959 Longitude 342.666 Instrument VIS Captured 2020-02-16 21 33
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Landslides
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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. The chasma stretches for 960 km (600 miles) from Melas Chasma to the west and Capri Chasma to the east. Landslide deposits, layered materials and sand dunes cover a large portion of the chasma floor. This image is located in eastern Coprates Chasma. The branching features near the bottom of the image are spurs of rock in the cliff face. The rock is more resistant to erosion that fine materials like sand and dust. Those materials are visible below the spurs, and then onto the canyon floor. Unlike the large landslide deposits, these small fans of material build up over time as the material above erodes. There are sand dunes along the edge of the fans in this image. The Odyssey spacecraft has spent over 15 years in orbit around Mars, circling the planet more than 69000 times. It holds the record for longest working spacecraft at Mars. THEMIS, the IR/VIS camera system, has collected data for the entire mission an
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This complex channel is located in the Nili Fossae region as seen by NASA's 2001 Mars Odyssey spacecraft.
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This image from NASA's 2001 Mars Odyssey spacecraft shows the floor of an unnamed crater east of Aram Chaos and Ares Vallis. There are two distinct elevations on the crater floor, which may indicate layered fill material.
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Candor Chasma Plateau
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This image is located in the Tyrrhena Terra region. The cause of the bright markings/material is unknown. It is possible that the formation of the channels are exposing a series of bright layered material
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An extensive field of small, dark dunes in located on the floor of the unnamed crater in Arabia Terra
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The mitten-shaped feature in Candor Chasma is a landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft.
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This image from NASA's 2001 Mars Odyssey spacecraft shows dune forms on the floor of Orson Welles Crater, an impact crater in the Coprates quadrangle named for the actor.
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This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows terminating at the foot of canyon walls in Echus Chasma. These lava flows are also fractured into large plates in this region.
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Today's VIS image shows the southeastern portion of Micoud Crater. Micoud Crater is located in Vastitas Borealis. A small group of sand dunes is located on the floor of the crater, visible in the upper left portion of the image. Orbit Number 78913 Latitude 50.1533 Longitude 16.7858 Instrument VIS Captured 2019-09-29 00 35
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Larger Landslide
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Olympus Mons is surrounded by a steep escarpment called Olympus Rupes. This image from NASA's 2001 Mars Odyssey spacecraft shows this escarpment and lava flows that plunged over it.
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Shadows cast by the high walls and high hills within Candor Chasma are visible in this image from NASA's 2001 Mars Odyssey spacecraft. The local time is near 5:00 in the afternoon.
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Candor Chasma
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Coprates Chasma is one of the numerous canyons that make up Valles Marineris. The chasma stretches for 960 km (600 miles) from Melas Chasma to the west and Capri Chasma to the east. Landslide deposits, layered materials and sand dunes cover a large portion of the chasma floor. This image is located in central Coprates Chasma. The floor of the chasma is covered by a complex deposit of material. This chaotic surface differs from most of the floor of the canyon and indicate a local process, perhaps a very large landslide or failure of the cliff face. The Odyssey spacecraft has spent over 15 years in orbit around Mars, circling the planet more than 69000 times. It holds the record for longest working spacecraft at Mars. THEMIS, the IR/VIS camera system, has collected data for the entire mission and provides images covering all seasons and lighting conditions. Over the years many features of interest have received repeated imaging, building up a suite of images covering the entire feature.
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Dunes forms top this sand sheet in the plains of Aonia Terra in this image captured by NASA's Mars Odyssey.
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Sulci Collapse Pits
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This image from NASA's 2001 Mars Odyssey shows the central portion of the complex caldera at the summit of Olympus Mons.
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Image Number: 6145-44891204Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Martian Geological FeaturesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1324×2924
2001 Mars Odyssey
Mars|