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Pavonis Chasma

Today's VIS image shows part of Pavonis Chasma, a collapsed region on the northeastern flank of Pavonis Mons. Pavonis Mons is the central volcano of the three large Tharsis volcanoes. In order fr...

http://themis.asu.edu/zoom-20240521a

Wind Erosion

Today's VIS image shows part of the surface between Aeolis Planum and Zephyria Planum in Elysium Planitia. Long term winds have eroded the surface in this region. Ridge features align with wind d...

http://themis.asu.edu/zoom-20240520a

Arsia Mons

Today's VIS image shows a cross section of the western side Arsia Mons, from the rim of the summit caldera at the top of the image, to the collapse features at the bottom of the image. A large vo...

http://themis.asu.edu/zoom-20240516a

Gale Crater

Today's VIS image shows part of Gale Crater. Gale Crater forms a large natural repository for a lot of Martian geologic history. This ancient impact scar has a diameter of about 150 kilometers (9...

http://themis.asu.edu/zoom-20240514a

Sacra Sulci

Today's VIS image shows part of Sacra Sulci, the complex northern flowing channel system that becomes Kasei Valles when it turns to flow eastward into Chryse Planitia. The image shows several typ...

http://themis.asu.edu/zoom-20240513a

Ius Chasma

Ius Chasma is at the western end of Valles Marineris, south of Tithonium Chasma. Valles Marineris is over 4000 kilometers long, almost as wide as the United States. Ius Chasma is almost 850 kilom...

http://themis.asu.edu/zoom-20240510a

Arsinoes Chaos

Today's VIS image shows part of Arsinoes Chaos. Chaos terrain is typified by regions of blocky, often steep sided, mesas interspersed with deep valleys. With time and erosion the valleys widen an...

http://themis.asu.edu/zoom-20240509a

Ius Chasma

Ius Chasma is at the western end of Valles Marineris, south of Tithonium Chasma. Valles Marineris is over 4000 kilometers long, almost as wide as the United States. Ius Chasma is almost 850 kilom...

http://themis.asu.edu/zoom-20240506a

Olympus Mons Flank

Today's VIS image is located on the western flank of Olympus Mons. Thin lava flows cover the sides of the volcano. The dark band in the lower part of the image is the escarpment called Olympus Ru...

http://themis.asu.edu/zoom-20240502a

Ascraeus Mons Flank

This VIS image shows a cross section of the western flank of Ascraeus Mons. Ascreaus Mons is the northernmost volcano of the three large Tharsis volcanoes. In order from north to south the volcan...

http://themis.asu.edu/zoom-20240501a

Arsia Mons Flank

The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). There are collapse features on all three volcanoes, on the southwestern and northea...

http://themis.asu.edu/zoom-20240430a

Olympus Rupes

Olympus Rupes is the name of the large escarpment surrounding Olympus Mons. The escarpment is a cliff where there is a large elevation change over a short distance. The elevation change from the ...

http://themis.asu.edu/zoom-20240429a

Ascraeus Mons Flank

This VIS image shows a cross section of the southwestern flank of Ascraeus Mons. Ascreaus Mons is the northernmost volcano of the three large Tharsis volcanoes. In order from north to south the v...

http://themis.asu.edu/zoom-20240426a

Nili Patera Dunes

Today's VIS image shows part of Nili Patera. Nili Patera is the northern caldera in the immense volcanic complex of Syrtis Major Planum. The dunes are moving westward across the top of these anci...

http://themis.asu.edu/zoom-20240425a

Zephyria Planum

Today's VIS image shows part of Zephyria Planum. Zephyria Planum is located south of Elysium Planitia. Long term winds have eroded the surface of Zephyria Planum, removing poorly cemented materia...

http://themis.asu.edu/zoom-20240423a

Sirenum Fossae

Today's VIS image shows a portion of Sirenum Fossae. The linear features are tectonic graben. Graben are formed by extension of the crust and faulting. When large amounts of pressure or tension a...

http://themis.asu.edu/zoom-20240422a

Arsia Mons

Today's VIS image is located on the northeastern flank of Arsia Mons. Arsia Mons is the southernmost of the Tharsis volcanoes. It is 450 km (270 miles) in diameter, almost 20 km (12 miles) high, ...

http://themis.asu.edu/zoom-20240419a

Olympus Mons

Today's VIS image is located on the western flank of Olympus Mons. Olympus Mons is the largest volcano in the solar system, reaching heights over 25 km (16 miles) tall from base to summit, with t...

http://themis.asu.edu/zoom-202404178898688a

Ascraeus Mons

This VIS image shows the upper elevations of Ascraeus Mons. Ascreaus Mons is the northernmost volcano of the three large Tharsis volcanoes. In order from north to south the volcanoes are Ascreaus...

http://themis.asu.edu/zoom-20240416a

Wind Erosion

In regions of poorly cemented surface materials it is possible to create large features due to just the action of the wind. The equatorial region between Olympus Mons and Apollinaris Mons is domi...

http://themis.asu.edu/zoom-20240412a

Pavonis Mons Summit

This VIS image shows a cross section of Pavonis Mons, including part of the summit caldera. A large volcanic crater known as a caldera is located at the summit of all of the Tharsis volcanoes. Th...

http://themis.asu.edu/zoom-20240411a

Wind Erosion

Today's VIS image shows the surface between Aeolis Planum and Zephyria Planum in Elysium Planitia. Long term winds have eroded the surface in this region. Features align with wind direction, in t...

http://themis.asu.edu/zoom-20240409a

Northern Crater

Today's VIS image shows a unnamed crater located in the northern plains. At some point after the crater was formed a layer of material covered the entire region. The coating layer is being eroded...

http://themis.asu.edu/zoom-20240408a

Chaos

In planetary nomenclature, the descriptor term chaos means "distinctive area of broken terrain". The general morphology of chaos is steep-sided mesas in close proximity. This image is located nor...

http://themis.asu.edu/zoom-20240405a

Iani Chaos

In planetary nomenclature, the descriptor term chaos means "distinctive area of broken terrain". The general morphology of chaos is steep-sided mesas in close proximity. The initial breakup of th...

http://themis.asu.edu/zoom-20240404a

Unusual Crater

Today's VIS image shows part of an unusual unnamed crater in northern Arabia Terra. The crater is not round, has different floor elevations and a fairly steep inner rim. Release Date:  Wed,...

http://themis.asu.edu/zoom-20240403a

Olympus Mons

Today's VIS image shows part of the upper elevations of Olympus Mons, including part of the summit caldera (top of image). Scarps and extensional features (graben) record multiple stages of calde...

http://themis.asu.edu/zoom-20240402a

Ascraeus Mons Summit

This VIS image shows part of the summit of Ascraeus Mons. Ascraeus Mons is the northernmost and tallest of the three large aligned Tharsis volcanoes. Calderas are found at the tops of volcanoes a...

http://themis.asu.edu/zoom-20240401a

Layers

Today's VIS image is located Arabia Terra near Chryse Planitia. The image shows several different surface layers. Release Date:  Fri, 2024-03-29 Themes: 

http://themis.asu.edu/zoom-20240329a

Coprates Chasma

Today's VIS image shows a cross section of Coprates Chasma. The floor of the canyon is covered by large landslide deposits. Coprates Chasma is one of the numerous canyons that make up Valles Mari...

http://themis.asu.edu/zoom-20240327a

Olympus Mons

Today's VIS image shows the upper elevations of Olympus Mons, including part of the summit caldera (top of image). Scarps and extensional features (graben) record multiple stages of caldera colla...

http://themis.asu.edu/zoom-20240326a

Coprates Chasma

Today's VIS image shows a cross section of Coprates Chasma. Sand dunes and a large landslide deposit are visible on the floor of the canyon. Coprates Chasma is one of the numerous canyons that ma...

http://themis.asu.edu/zoom-20240325a

Pavonis Mons Summit

This VIS image shows a cross section of Pavonis Mons, including the summit caldera. A large volcanic crater known as a caldera is located at the summit of all of the Tharsis volcanoes. These cald...

http://themis.asu.edu/zoom-20240322a

Olympia Undae

This VIS image of Olympia Undae was collected during north polar spring. The dunes are still partially covered by the winter frosts; as the region heats up the frost will dissipate to reveal the ...

http://themis.asu.edu/zoom-20240321a

Wind Erosion

Today's VIS image shows the surface between Aeolis Planum and Zephyria Planum in Elysium Planitia. Long term winds have eroded the surface in this region. Ridge features align with wind direction...

http://themis.asu.edu/zoom-20240320a

Arsia Mons Summit

A large volcanic crater known as a caldera is located at the summit of all of the Tharsis volcanoes. These calderas are produced by massive volcanic explosions and collapse.Today's VIS image show...

http://themis.asu.edu/zoom-20240318a

Olympus Mons

Today's VIS image shows the lower elevations of Olympus Mons. Near the bottom of the image is part of the escarpment that marks the edge of the volcano. The escarpment is a cliff face that can be...

http://themis.asu.edu/zoom-20240315a

Olympus Mons Summit

Today's VIS image shows the upper elevations of Olympus Mons, including part of the summit caldera. Scarps and extensional features (graben) record multiple stages of caldera collapse at the summ...

http://themis.asu.edu/zoom-20240314a

Olympus Mons Flank

Today's VIS image is located on the eastern flank of Olympus Mons. Olympus Mons is the largest volcano in the solar system, reaching heights over 25 km (16 miles) tall from base to summit, with t...

http://themis.asu.edu/zoom-20240313a