This image of Occator Crater's northern wall was obtained by NASA's Dawn spacecraft on June 16, 2018 from an altitude of about 21 miles (33 kilometers). The sub-spacecraft position from which this image was taken is about 25.8 degrees north latitude and 242.1 degrees east longitude.

This image of Occator Crater's northern wall was obtained by NASA's Dawn spacecraft on June 16, 2018 from an altitude of about 21 miles (33 kilometers). The sub-spacecraft position from which this image was taken is about 25.8 degrees north latitude and 242.1 degrees east longitude.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of This image of Occator Crater's northern wall was obtained by NASA's Dawn spacecraft on June 16, 2018 from an altitude of about 21 miles (33 kilometers). The sub-spacecraft position from which this image was taken is about 25.8 degrees north latitude and 242.1 degrees east longitude. by Piemags/PL Photography Limited is available for licensing today.

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Today's VIS image shows part of the floor of Firsoff Crater. Located in Arabia Terra, Firsoff Crater, and the neighboring Crommelin Crater, contain large layered deposits on the crater floor. The north side of the smaller crater at the bottom of the image shows the layering. Wind action has modified the deposit. Firsoff Crater is 90 km in diameter (56 miles). Orbit Number 94812 Latitude 2.77617 Longitude 350.268 Instrument VIS Captured 2023-04-30 02 58
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Claritas Fossae. Located between the lava plains of Daedalia Planum and Solis Planum, Claritas Fossae is a graben filled highland. Graben are formed by tectonic activity, where extensional forces stretch the surface allowing blocks of material to slide down between paired faults. These linear grabens are termed fossae. This region of Mars had very active tectonism and volcanism, resulting in the huge volcanos like Arsia Mons and deep chasmata of Valles Marineris. Claritas Fossae was formed prior to the large lava flows of the Tharsis region. Orbit Number 91446 Latitude -36.8955 Longitude 262.397 Instrument VIS Captured 2022-07-26 23 05
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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Coprates Chasma, including a large sand sheet and smaller dunes.
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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Iani Chaos. The brighter floor material is being covered by sand, probably eroded from the mesas of the Chaos.
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This image captured NASA's Mars Odyssey shows part of a landslide deposit in Melas Chasma.
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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the canyon wall of Melas Chasma.
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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a complex region of channels which dissect the margin of Arabia Terra where elevations lower into Acidalia Planitia.
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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Gusev Crater.
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This image shows the north central cliff face of Hebes Chasma. The cliff face and downslope movement of material is very different in appearance than the same features of the large mesa in the center of the chasma. Hebes Chasma is an enclosed basin not connected to Valles Marineris. 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. From the deepest chasma to the tallest volcano, individual dunes inside craters and dune fields that encircle the north pole, channels carved by water and lava, and a variety of other feature, THEMIS has imaged them all. For the next several months the image of the day
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This VIS image shows layering of surface materials in Meridiani Planum. TES (Thermal Emission Spectrometer) initially detected hematite in a surface layer, which was confirmed by THEMIS (THrmal EMision Imaging System). These findings supported a water rich origin of the hematite and led to the selection of the site for the Opportunity MER (Mars Exploration Rover). The TES instrument was located on the Mars Global Surveyor spacecraft. THEMIS is onboard the Mars 2001 Odyssey spacecraft. Orbit Number 89658 Latitude 1.83323 Longitude 0.267191 Instrument VIS Captured 2022-03-01 17 54
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This image shows the eastern portion of Hebes Chasma. The ridge that is casting a shadow at the bottom of the image is likely a large tectonic fault. All of the materials on the floor of the chasma are from the cliff faces. The deposition and erosion of the materials in this image are very different from the those of the large central mesa. Hebes Chasma is an enclosed basin not connected to Valles Marineris. 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. From the deepest chasma to the tallest volcano, individual dunes inside craters and dune fields that encircle the north pole, channels carved
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This NASA 2001 Mars Odyssey image shows part of the floor of Coprates Chasma.
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Lava flows of Daedalia Planum can be seen at the top and bottom portions of this image from NASA's 2001 Mars Odyssey spacecraft. The ridge and linear depression in the central part of the image are part of Mangala Fossa, a fault bounded graben.
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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 brighter materials at the bottom of the image are layered deposits. It is unknown how deep these canyon deposits were when they formed. The layering is only visible due to erosion, making it difficult to estimate the original thickness. While layered deposits can be found on the floor of Coprates Chasma, they are most commonly found along the lower elevations and at the bottom of the cliff faces in the canyon. 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 pr
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Today's VIS image shows part of Gale Crater, including the large layered deposit on the crater floor. The Curiosity Rover is located in Gale Crater. Gale crater is 150km (90 miles) in diameter. Orbit Number 88942 Latitude -4.53543 Longitude 137.674 Instrument VIS Captured 2022-01-01 18 55
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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit in Ganges Chasma.
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Small unnamed channels drain the surface in this region of Arabia Terra were captured by NASA's Mars Odyssey on August 3, 2010.
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The two landslides in this image are located in Aeolis Mensae
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Image Number: 6145-45263522Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Mars Geological FeaturesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1024×1024