A Cluster of Mounds in Terra Cimmeria

This observation shows a cluster of mounds exhibiting low thermal inertia relative to the surroundings. Are these (igneous/mud) volcanoes? Erosional remnants? Higher resolution may help resolve stratigraphic relationship to nearby materials. Compositional information may help constrain the dating of the origin of these mounds.

ID: ESP_075558_1515
date: 8 September 2022
altitude: 254 km

uahirise.org/hipod/ESP_075558_
NASA/JPL-Caltech/University of Arizona

In a Southern Mid-Latitude Crater

The objective of this observation is to examine small gullies in a crater. Pictures like this will give us a better knowledge of the full range of gully sizes and shapes. Also visible in this field of view are cracks that may be forming from pits. HiRISE will be able to resolve pits in the cracks if they are there. If there are pits, it may be due to ground ice sublimating then causing the ground to collapse.

uahirise.org/hipod/ESP_075555_

HiRISE 3D: Raised Glacier-Like Forms in Arabia Terra

Glacier-like forms are interesting due to their raised nature, showing possible previous extent of caldera ice fill. GLF also appears to have a sedimentary fan from ice build up.

Full image: uahirise.org/anaglyph/ESP_0851

NASA/JPL/University of Arizona

Dunes or Bantha?

This group of dunes almost looks like a wandering herd of Bantha on Tattooine. Our goal with this observation is seasonal dune and frost deposition and sublimation. High resolution can provide for detailed surface measurements. These dunes are within in impact crater in the Northern Hemisphere of Mars.

ID: ESP_075556_2430
date: 8 September 2022
altitude: 314 km

uahirise.org/hipod/ESP_075556_
NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Mesa Stratigraphy at Terby Crater

This sequence of exposed stratigraphy across the three mesas in the northeastern portion of Terby Crater likely capture a diverse range of sedimentary rock types.

Full image: uahirise.org/anaglyph/ESP_0850

NASA/JPL-Caltech/University of Arizona

A Layered Plateau in Pavonis Mons

This plateau is one of the few hypothesized glaciovolcanic landforms on Mars with well-exposed areas and meter-scale and smaller structures. The large outcrops are the only ones in the plateau that face the inferred down-flow direction of the ancient glacier that left a fan-shaped deposit.

uahirise.org/hipod/ESP_075541_
NASA/JPL-Caltech/University of Arizona

Inverted Channels near Juventae Chasma

This image shows several long, sinuous features on the plains near Juventae Chasma. These features have been explained as former stream channels now preserved in inverted relief.

Inverted relief occurs when a formerly low-lying area becomes high-standing. For instance, depressions may become filled with lava that is more resistant to erosion.

uahirise.org/hipod/PSP_003223_
NASA/JPL-Caltech/University of Arizona

Slope Streaks in Terra Sabaea

Slope streak formation is among the few known processes currently active on Mars. While their mechanism of formation and triggering is debated, they are most commonly believed to form by downslope movement of extremely dry sand or very fine-grained dust in an almost fluidlike manner (analogous to a terrestrial snow avalanche) exposing darker underlying material.

uahirise.org/hipod/PSP_001808_
NASA/JPL-Caltech/University of Arizona

HiRISE 3D: A Fresh 500-meter Diameter Impact Crater

Now, who doesn’t like a 3D image of an impact crater? (If you know anyone, start naming names.)

Full image: uahirise.org/anaglyph/ESP_0844

NASA/JPL-Caltech/University of Arizona

Abounding in Megabreccia!

This image offers us unique color coverage of the beautifully exposed and sharp-edged megabreccias. Nili Fossae has long been a perennial runner-up choice for possible landing spots for exploration. Megabreccia are very large clasts of broken up rock, and the ones in this observation appear be layered and have structure.

ID: ESP_075534_2005
date: 6 September 2022
altitude: 278 km

uahirise.org/hipod/ESP_075534_
NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Possible Hydrothermal Setting in Northeast Syrtis Major

Large fractures and light-toned materials are on full display in this 3D image.

uahirise.org/anaglyph/ESP_0850

NASA/JPL-Caltech/University of Arizona

A Channel West of Eberswalde Crater

This observation focuses on the transition from a smaller to a larger channel or valley in one of the feeder channels upstream of the Eberswalde delta. Eberswalde Crater has often been on the shortlist for potential landing sites, including for the Curiosity rover that landed in Gale Crater.

ID: ESP_075525_1555
date: 6 September 2022
altitude: 256 km

uahirise.org/hipod/ESP_075525_
NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Pits Sourcing a Channel

This image shows collapse pits at the edge of an infilled basin adjacent to the heavily faulted Ceraunius Fossae. These pits may be volcanic. A channel originates from one of the pits and continues into the basin.

Full image: uahirise.org/anaglyph/ESP_0756

Chaos Terrain near Hecates Tholus

The blocks/pieces here could formerly have been part of the flank of Hecates Tholus and they could have been flipped during their possibly violent creation, in which case they could be exposing parts of the volcano normally hidden. One of the big blocks targeted here displays a banding that appears to be caused by ridges.

uahirise.org/hipod/ESP_075518_
NASA/JPL-Caltech/University of Arizona

HiRISE 3D: Nirgal Vallis Headwaters

Our goal is to take a look at the head wall of the origin of Nirgal Vallis and also to look for layers and small scale erosional features.

Full image: uahirise.org/anaglyph/ESP_0850

NASA/JPL-Caltech/University of Arizona

Brain Terrain on the Floor of a Crater

The objective of this observation is to examine “brain terrain” on part of the floor of a crater in Claritas Fossae. Pictures like this can help us understand past climate and why nearby craters have slight differences in the expression of brain terrain. In some areas, the coverage is complete; in this one, only part of the floor is covered in brain terrain.

uahirise.org/hipod/ESP_075501_
NASA/JPL-Caltech/University of Arizona

Scalloped Depressions with Layers

This image, of the northern plains of Mars, is marked by depressions in a layer of material that covers the region. The depressions, several of which have coalesced together, have scalloped edges and layers in their walls.Their presence has led to hypotheses of the removal of subsurface material, possibly ground ice, by sublimation (evaporation). This process is believed to be ongoing today.

uahirise.org/hipod/PSP_002439_
NASA/JPL-Caltech/University of Arizona

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HiRISE (NASA)

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