HiPOD: A Candidate Recent Impact Site

Why do we initially say “candidate”? Before HiRISE acquires an image, the Context Camera on MRO might observe something that could be an impact, but their resolution is not like ours. In one of their images, there was a large diffuse dark blast zone that was not present in an earlier observation, so that team asked HiRISE to acquire a picture to confirm if this is an impact crater.

https://uahirise.org/hipod/ESP_074999_1845
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiPOD: Layering in Arabia Terra

The objective of this observation is to search for layering in Arabia. In Context Camera data, the layering shows up in buttes, ridges, and the edges of mesas. Our image may be able to see many more of these layers. This image will also help us to determine the horizonatal extent of layering in the region.

ID: ESP_074982_2100
date: 25 July 2022
altitude: 290 km

https://uahirise.org/hipod/ESP_074982_2100
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiRISE 3D: Ridges in Huygens Crater

We acquired this image to investigate the timing relationship between the wrinkle ridges and the quasi-circular mesas.

https://www.uahirise.org/anaglyph/ESP_074203_1640_ESP_082102_1640_RED
NASA/JPL-Caltech/UArizona

HiPOD: Channel, Fan, Crater

The objective of this observation is to examine a channel on a crater wall, where a fan has formed at the base. Images like this, also found in Context Camera data, may help us better understand how craters are degraded. This particular crater is one of many located to the northwest of the massive Hellas impact basin.

ID: ESP_074982_1570
date: 25 July 2022
altitude: 257 km

https://uahirise.org/hipod/ESP_074982_1570
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiRISE 3D: A Partly Filled Impact Crater near Nicholson Crater

This anaglyph shows an infilled and possibly exhumed crater. HiRISE resolution can examine the shape of the crater fill and any wall layering.

https://www.uahirise.org/anaglyph/ESP_082242_1830_ESP_082176_1830_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: A Circular Landform within an Impact Crater

This circular formation appears to have the land around it sloping to its edge. The formation then looks to rise out of the ground with various others different formations around it. There also what appears to be a small crater on the top. When viewing this area using infrared background, the land formation has several markings on one side more than the other.

https://uahirise.org/hipod/ESP_074972_2085
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiRISE 3D: Light-Toned Outcrops in Aurorae Chaos

This image was requested to fill in HiRISE coverage where there is an existing CRISM instrument data.

https://www.uahirise.org/anaglyph/ESP_074259_1725_ESP_082224_1725_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: A Patchy Outcrop of Light-Toned Materials

This observation targets a small region of patchy light-toned materials visible in Context Camera images. These outcrops are small, precluding geomorphological analysis and assignment of a stratigraphic position relative to the surrounding materials. The shape of this material closely resembles sinuous, light-toned outcrops elsewhere in Terra Cimmeria.

https://uahirise.org/hipod/ESP_074952_1480
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiRISE 3D: Floor of East Candor Chasma

This 3D image shows intricate folding and deformational structures within the layered deposits in east Candor Chasma.

https://www.uahirise.org/anaglyph/ESP_082278_1720_ESP_082423_1720_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: Bedrock Exposures in Nirgal Vallis

This observation covers two tributaries and the main channel of Nirgal Vallis. The channel is approximately 610 kilometers long and is named after Nergal, the Babylonian god of war and counterpart to the Roman god of war, Mars. Mars Orbiter Camera image show light-toned bedrock; our high resolution picture can gives us a better view of the channel form and bedrock stratigraphy.

https://uahirise.org/hipod/ESP_074945_1515
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiRISE 3D: Chryse Chaos

This observation was taken to document stratigraphic relationships between chaos blocks and adjacent geologic units.

https://www.uahirise.org/anaglyph/ESP_082356_1885_ESP_082290_1885_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: Light-Toned Materials within Iani Chaos

The objective of this observation is to get high resolution image to see more details about the light-toned deposits: could they be more sulfates or other hydrated materials? Iani Chaos is a region of chaos terrain at the south end of the Ares Vallis outflow channel. The chaotic terrain is believed to have formed by the removal of subsurface water or ice, resulting in flooding at the surface.

https://uahirise.org/hipod/ESP_074944_1800
NASA/JPL-Caltech/UArizona
#Mars

HiRISE 3D: Ridges in Meridiani Planum

This anaglyph shows us wrinkle ridge-like features in layered deposits.

https://www.uahirise.org/anaglyph/ESP_082355_1805_ESP_082289_1805_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: Gullies in a Crater near Newton Crater

The objective of this observation is to observe gullies in a crater. Pictures like this will help us increase our knowledge of the distribution of Martian gullies. Some of the gullies have quite wide, branched alcoves, and there are ridges of material at the base. The floor of this crater is covered with pits and contains some small ring mold craters.

https://uahirise.org/hipod/ESP_074936_1380
NASA/JPL-Caltech/UArizona
#Mars #science #NASA

HiRISE 3D: Yardangs in the Aeolis Region

Hypothesis: Three different generations of yardang-forming materials are recorded here. Alternative: One generation of deposits, but multiple directions for strong-wind erosion.

https://www.uahirise.org/anaglyph/ESP_082336_1800_ESP_082204_1800_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: A Source of Stratified Fan Material

This public suggestion from HiView requested an image to help determine the relationship between the crater wall and fan deposits on the crater floor. The stratified fan material in the southeast quadrant of Baltisk Crater may have its source in the wall where glacial landforms have been observed. Or, the stratified fan material could have been transported into the crater and prior to deposition.

https://uahirise.org/hipod/ESP_074761_1370
NASA/JPL-Caltech/UArizona

HiRISE 3D: Not Quite Mount Doom

These cones were interpreted to be volcanic in origin despite a distinct lack of volcanic activity in this area. Whether volcanism has occurred here recently or not is a key constraint on polar history and has implications for any possible basal melting of the polar ice deposits that may have occurred.

https://www.uahirise.org/anaglyph/ESP_027077_2605_ESP_026958_2605_RED
NASA/JPL-Caltech/UArizona
#Mars #science

HiPOD: Light Toned in Aureum Chaos

The objective of this observation is to examine a light-toned, layered butte in a region of chaos. The field of view also inculdes several small outcrops of light-toned deposits. The OMEGA experiment on Mars Express discovered clay minerals in a variety places in Aureum Chaos. Clay minerals need water to form, so the area may once have contained large amounts of water.

https://uahirise.org/hipod/ESP_074918_1755
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Potential Landing Site in the Coprates Region

This image shows a central hill exposing crustal bedrock enriched in low calcium pyroxenes and possibly in clays, located 2 km north of a proposed landing ellipse.

https://www.uahirise.org/anaglyph/ESP_027393_1675_ESP_028448_1675_RED
NASA/JPL-Caltech/UArizona

HiPOD: Ridges in Hellas Planitia

Also visible in Context Camera data, the objective of this observation is to examine curved ridges and a network of straight ridges. One area of the curved ridges appears superposed on a section of the very eroded rim of an impact crater.

ID: ESP_074902_1420
date: 19 July 2022
altitude: 261 km

https://uahirise.org/hipod/ESP_074902_1420
NASA/JPL-Caltech/UArizona
#Mars #science #NASA