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HiRISE 3D: Crevasse-Like Features in the Utopia Region

A formation like these demands to have a stereo pair for a future digital terrain model. It’s a retarget to also look for changes.

bit.ly/hi3d-24-may-2023
NASA/JPL-Caltech/UArizona

HiPOD 24 May 2023: Layers in the Center of Cerulli Crater

The objective of this observation is to determine the nature of what looks like layers. The layers seem to be associated with mantle material moving off knobs. It may be that the mantle slides off the knobs and gets twisted. This image shows a simple view of what is going on.

uahirise.org/hipod/ESP_023104_
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Chain of Mounds in the Tharsis Region

Here is part of a series of elongate mounds aligned with fissures in Tharsis. The mounds have summit craters in various stages of degradation—possible cinder cones.

bit.ly/hi3d-24-may-23
NASA/JPL-Caltech/UArizona

HiPOD 23 May 23: Dune Monitoring in Mawrth Vallis

This location was a candidate landing site for the ExoMars mission. It’s a dune field that has never been imaged before by HiRISE, and we can use it as part of a monitoring series to spot ripples on the dunes and changes over time.

uahirise.org/hipod/ESP_073467_
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Candidate Future Landing Site in the Oxia Palus Region

Another good reminder of how HiRISE images can be used for future missions to characterize potential landing sites.

bit.ly/hi3d-22-may-23
NASA/JPL-Caltech/UArizona

HiPOD 22 May 2023: Ridges in Huygens Crater

With this observation, we want to investigate the timing relationship between the wrinkle ridges and the quasi-circular mesas we see here. The floor of this 450-km diameter crater named after Dutch astronomer Christian Huygens (1629-1695) has an unusual texture. Smooth-topped mesas are scattered across a more rugged surface. The mesas are testament to a former smooth layer of material that is in the process of eroding away.

uahirise.org/hipod/ESP_073135_

HiRISE 3D: Basal Units in the North Polar Region

“Basal” refers to the bottom layer or base of something, in this case, of the stunning cliffs here.

bit.ly/hi3d-19-may-23
NASA/JPL-Caltech/UArizona

HiPOD 19 May 2023: Inverted Channels in Saheki Crater

The large alluvial fans in the southern Martian highlands have the potential to provide key insights into the history of water on the planet’s surface. The ridges on these fans are inferred to be the preserved remains of the fluvial channels responsible for fan formation. Saheki is 82 kilometers in diameter and was named after Tsuneo Saheki, a Japanese amateur astronomer (1916-1996).

uahirise.org/hipod/ESP_042368_
NASA/JPL-Caltech/UArizona

HiRISE 8K: Layering in Western Arabia Terra

With terrain like that in Arabia Terra, it’s considered imperative to get more images to create stereo pairs for 3D images.

Full cutout on Flickr:
flic.kr/p/2oAUKmv

NASA/JPL-Caltech/UArizona

Made with HiRISE: Adeline Horst, jewelry and gemstone designer, uses HiRISE color images for inspiration in new work.

uahirise.org/epo/made-with-hir

HiRISE 3D: In Syrtis Major

This image was taken to increase our coverage of the region, and examine volcanics and sulfates near smectite plains.

bit.ly/hi3d-18-may-23
NASA/JPL-Caltech/UArizona

HiPOD 18 May 2023: Stratigraphy of a Kaporo Crater Mound

Kaporo Crater contains a divided central mound of layered deposits that indicate multiple unconformities in the stratigraphy. An unconformity is a buried erosion surface, where the bedding layers do not match. This re-image will help to resolve bedding orientation and bed thicknesses to understand variation in the stratigraphy and the unconformity between the lower and upper portions of the mound.

uahirise.org/hipod/ESP_073466_

HiRISE 3D: A Rocky Massif

This may be part of the peak ring of a largely obliterated large crater, and may contain megabreccia.

bit.ly/hi3d-17-may-23
NASA/JPL-Caltech/UArizona

HiPOD 17 May 2023: Like Little Stars

This observation is part of a long-term monitoring campaign of this site to track the wind orientation and seasonal activity. The terrain is considered “non cryptic”, which means that we want to study seasonal processes at a site where the surface and surface ices are different than most of the other parts of the South Polar terrain.

uahirise.org/hipod/ESP_073243_
NASA/JPL-Caltech/UArizona

HiClip mini 4K: Kull wahad!

This observation features a very large dune field near the center of an unnamed impact crater.

This is a non-narrated clip with ambient sound. See description for more information.

youtu.be/80xVAtnR-kA

NASA/JPL-Caltech/UArizona

HiRISE 3D: A Gullied Crater in Tempe Terra

A small crater in Tempe Terra shows evidence of possible water gullies. Tempe Terra is a region that shows evidence of water as well as potential glacial features called eskets.

Anaglyph details page: bit.ly/hi3d-16-may-23

NASA/JPL-Caltech/UArizona

HiPOD 16 May 2023: Layered Deposits on West Candor Chasma

This image shows us an extensive and stunning array of well-exposed faults. This observation is very important for understanding the mechanics of faulting in these deposits and the tectonic history of the area. Candor is one of the largest canyons in the Valles Marineris system, and its formation still remains unclear.

uahirise.org/hipod/ESP_073232_
NASA/JPL-Caltech/UArizona

HiRISE 3D: The Western Rim of a Well-Preserved Crater

Given the relative sharpness of the rim, this is a very well-preserved impact crater that looks stunning in 3D.

bit.ly/hi3d-15-may-23
NASA/JPL-Caltech/UArizona

HiPOD 15 May 2023: A Fault-Deformed Crater

This small 1.5-kilometer diameter crater has an unusual oval shape. It is situated on a wrinkle ridge (a thrust fault) that appears to have been deformed by the tectonic activity, rather than postdating it. As these same wrinkle ridges deform the Oxia Planum ExoMars landing site area, we could learn about the wider tectonic setting of this landing site from craters like this.

uahirise.org/hipod/ESP_073230_
NASA/JPL-Caltech/UArizona

HiRISE 3D: Dune Changes near Martz Crater

This image was acquired to observe any wind-driven changes since an earlier observation in 2008.

bit.ly/hi3d-12-may-23
NASA/JPL-Caltech/UArizona

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HiRISE (NASA)

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