Results tagged “MARS”

Stratigraphy In Cross Crater On Mars

Cross Crater, about 65 kilometers in diameter, is located in the highlands of the Terra Sirenum region of Mars.

A Tale of Collapsed Terrain On Mars

North of Ganges Chasma lies Orson Welles Crater, whose floor contains broken up blocks we call chaotic terrain and which is the source for the major outflow channel Shalbatana Vallis.

The 17th flight of NASA's Ingenuity Mars Helicopter on Dec. 5 pushed the total flight time past the 30-minute mark.

Icy Cliffs and Impact Craters On Mars

We've come to understand in recent years that about a third of Mars has ice just below the surface.

Scientists with NASA's Perseverance Mars rover mission have discovered that the bedrock their six-wheeled explorer has been driving on since landing in February likely formed from red-hot magma.

This image shows the edge of the Martian South Polar layered deposit. The stack of fine layering is highlighted by the rays of the polar sun.

Chaotic Terrain in Aromatum Chaos

This observation show us chaotic terrain in Aromatum Chaos, with collapse features and potential dikes.

Context Camera imagery reveals dark streaks extending east of minor crater rims within and around Holmes Crater.

This HiRISE image shows the central pit feature of an approximately 20-kilometer diameter complex crater in located at 304.480 degrees east, -11.860 degrees south, just north of the Valles Marineris.

The Floor Of Soffen Crater On Mars

Dr. Gerald A. Soffen (February 7, 1926 -- November 22, 2000) was a project scientist for the NASA's Viking program of Mars landers.

NASA's Curiosity rover captured a remarkable image from its most recent perch on the side of Mars' Mount Sharp.

Seismic data collected in Elysium Planitia, the second largest volcanic region on Mars, suggest the presence of a shallow sedimentary layer sandwiched between lava flows beneath the planet's surface.

A Scarp In The Arabia Region On Mars

Pictured here appears to be the edge of a blast radius of a large meteorite impact crater with smaller and more recent cratering interrupting its circumference.

Capri Chasma is located in the eastern portion of the Valles Marineris canyon system, the largest known canyon system in the Solar System.

Recently downlinked imagery of a September flight has allowed the rover imaging team to put together a video of rotorcraft performing to near-perfection.

Secondary Craters On Mars

This image of a southern mid-latitude crater was intended to investigate the lineated material on the crater floor.

A Martian Dust Avalanche

Relatively dark slope streaks are common on steep dust-mantled slopes of Mars. When imaged under high sun illumination they appear to be just a dark stain without topographic relief.

Noctis Labyrinthus, "the labyrinth of the night," sits at the western end of the largest canyon of the solar system Valles Marineris.

The purpose of this observation is to image dunes where substantial gullies formed in the previous Mars winter (2013).

Polar Sand Dunes On Mars

Mars has a vast sea of sand dunes in the high latitude region encircling its north polar cap, known as the North Polar erg. These dunes are made up of basalt and gypsum sand grains.

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