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Erosion in North Arabia Terra

The objective of this observation is to examine an upper plains unit that is eroding. The image field includes a higher unit with fractures and hollows forming. This scene is also visible in Context Camera data.

ID: ESP_057494_2230
date: 1 November 2018
altitude: 299 km

uahirise.org/hipod/ESP_057494_
NASA/JPL-Caltech/University of Arizona

Dynamic Mars

This picture managed to capture a small avalanche in progress, right in the color strip. The small white cloud in front of the brick red cliff is likely carbon dioxide frost dislodged from the layers above, caught in the act of cascading down the cliff. It is larger than it looks, more than 20 meters across, and (based on previous examples) it will likely kick up clouds of dust when it hits the ground.

More: uahirise.org/hipod/ESP_042572_

NASA/JPL-Caltech/University of Arizona

A Mesa in the Plain of No Place

This observation was requested to image a small mesa to determine superposition relationships between the mesa, fractures, pitted mounds and flows. Utopia Planitia (that can translate to “plain of no place”) is the largest recognized impact basin on Mars and in the Solar System with an estimated diameter of 3,300 kilometers (2,100 miles).

uahirise.org/hipod/ESP_075454_

NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Collapse Terrain near Orson Welles Crater

Between Orson Welles and Ganges Chasma is a region where materials subsided and collapsed over underground cavities that had once held aquifers.

Full image: uahirise.org/anaglyph/ESP_0845

NASA/JPL-Caltech/University of Arizona

Total Chaos

This disrupted surface is characterized by a collection of rounded to flat-topped mounds of various sizes connected by narrow flat floors, typical of the aptly named “chaotic terrain” on Mars. What could have caused this flat surface to break into pieces?

More: uahirise.org/hipod/ESP_083952_

NASA/JPL-Caltech/University of Arizona

HiRISE 3D: This is NOT Shai-Hulud

This large, hulking formation is actually an elongated mound in Phlegra Montes. There are indications of ancient glacial flow.

Full image: uahirise.org/anaglyph/ESP_0846

NASA/JPL-Caltech/University of Arizona

A Frosty Start to Southern Summer

In this image, the bright material that appears to be filling in cracks in the surface and these craters is seasonal frost, a byproduct of Mars’ major atmospheric component freezing onto the ground to create landscapes below -100 Celsius.

More: uahirise.org/hipod/ESP_083343_

NASA/JPL-Caltech/University of Arizona

We had an opportunity this afternoon to talk about our camera and Mars to an hydrology and atmospheric space science class today. Thank you for coming to visit!

HiRISE 3D: A Low Ridge

This image shows interesting interactions between a low ridge (wrinkle ridge? flow front?) and pre-existing topography.

Full image: uahirise.org/anaglyph/ESP_0845

NASA/JPL-Caltech/University of Arizona

There’s No Place Like Terby!

This HiRISE image captures the side of an approximately 2-km thick mesa within Terby Crater. This mesa consists of thick sequences of layered rocks that are peeking through a smooth, dark deposit that was once more expansive. These layered rocks may have formed in a very deep and expansive lake that filled the greater Hellas basin.

More: uahirise.org/hipod/ESP_083921_

NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Phlegra Montes

This is a 3D image of a candidate safe landing site near ice.

Full image: uahirise.org/anaglyph/ESP_0846

NASA/JPL-Caltech/University of Arizona

Fragmented Crater Floor Materials

This HiRISE image shows some unusual blocks within two adjoining craters near the highland-lowland boundary of Mars. The blocks could be associated with the collapse of the crater floor and their unusual shapes suggest that they have been subject to significant erosion.

More: uahirise.org/hipod/ESP_084214_

NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Crater!

You can never really go wrong with a 3D image of an impact crater on Mars.

Full image: uahirise.org/anaglyph/ESP_0848

NASA/JPL-Caltech/University of Arizona

Cones and Ridges

Also visible in Context Camera data, the objective of this public target suggestion via HiWish is to determine the nature of a field of cones and two ridges that appear to flank them. This locale is in Acidalia Planitia, not far from the higher terrain of Arabia Terra in the Northern Hemisphere of Mars.

ID: ESP_075484_2225
date: 3 September 2022
altitude: 301 km

uahirise.org/hipod/ESP_075484_
NASA/JPL-Caltech/University of Arizona

Layering in the Medusae Fossae Formation

An adjacent observation shows nice fine layering within an upper section of the Medusa Fossae Formation (MFF). It looks like the layering may actually be quite continuous laterally. The MFF a large collection of soft, easily eroded deposits that extends discontinuously for more than 5,000 kilometers.

ID: ESP_075451_1735
date: 31 August 2022
altitude: 266 km

uahirise.org/hipod/ESP_075451_
NASA/JPL-Caltech/University of Arizona

HiRISE 3D: A Ridge in a Lava Flow

This ridge appears to be the contact between adjacent lava flow units. Stereo will help discern the overlapping relationships and morphology of the contact.

Full image: uahirise.org/anaglyph/ESP_0845

NASA/JPL-Caltech/University of Arizona

A Ridge on a Crater Floor

Also available in Context Camera data, the objective of this observation is to determine the nature of a narrow, unbranched ridge on the floor of an impact crater. It may be a dike, so it may tell us where mineral deposits may lie. This image is located in the Sinus Sabaeus region, an ancient cratered surface that has been modified by a combination of impact cratering, fluvial, wind, and possible volcanic processes.

uahirise.org/hipod/ESP_075431_

HiRISE 3D: Layering in a Meridiani Planum Crater

The objective of this observation is to look for layering along walls of this large, geologically fresh impact crater.

Full image: uahirise.org/anaglyph/ESP_0845

NASA/JPL-Caltech/University of Arizona

Zen Gardens on Mars

Scientists have not previously seen these patterns elsewhere on Mars. They are particularly conspicuous here because of the contrast between the bright boulders and the darker soil. Some process has evidently sorted and segregated the larger boulders from the finer soil. Exactly what that process is presents a perplexing puzzle.

More: uahirise.org/hipod/ESP_084798_

NASA/JPL-Caltech/University of Arizona

Mysterious Light-Toned Deposit in Vinogradov Crater

The southeastern floor of Vinogradov is covered with several mysterious light-toned, sub-meter scale “blobs” that lack obvious layering. In some places the light-toned material appears to have filled pre-existing craters giving them a circular appearance.

This material may be related to ejecta from a nearby crater, eroded from the rim of Vinogradov or emplaced by some other process.

uahirise.org/hipod/ESP_037163_

NASA/JPL/University of Arizona

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HiRISE (NASA)

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