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HiPOD: Layers in a Low Latitude Crater

The objective of this observation is to examine thin layers in a small crater on the floor of a larger crater. These thin, regular layers may be evidence that a lake once sat in the larger crater. This is scene is also visible in a Context Camera image.

uahirise.org/hipod/ESP_074692_
NASA/JPL-Caltech/UArizona

HiRISE 3D: Mounds in Oxia Colles

This landform shows distinctive layering in CTX, and is similar to other buttes to the far north east which have been observed to have Mawrth-like stratigraphy.

Full image: uahirise.org/anaglyph/ESP_0771
NASA/JPL-Caltech/UArizona

HiPOD: An Inverted Channel West of Idaeus Fossae

This observation shows a multithreaded, inverted fluvial channel located to the west of Idaeus Fossae. The formation may date back to the mid-Noachian epoch, billions of years ago. There is also evidence for lateral channel migration and is possibly associated with fan deposits in an impact crater to the east.

uahirise.org/hipod/ESP_074497_
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Southern Canyon Wall in East Coprates Chasma

The walls here potentially expose pristine crustal material. This is an area of interest that could be accessed and is within a potential future rotorcraft mission traverse.

Full image: uahirise.org/anaglyph/ESP_0782
NASA/JPL-Caltech/UArizona

HiPOD: Fluvial Landforms in Granicus Valles

In this image, large, streamlined features and grooves have been carved by enormous water volumes into the floor of Granicus and point to the direction of flow towards the northwest. The floods of Granicus Valles are thought to have formed later in Mars history during the Amazonian epoch, several billion years ago.

uahirise.org/ESP_080319_2105
NASA/JPL-Caltech/UArizona

HiRISE 3D: He’s Baaaaack!

Yes, it’s the (in)famous formation first imaged in low-resolution by the Viking probe back in 1976. We’ve imaged it before, but now you can view it in 3D glory!

uahirise.org/anaglyph/ESP_0805
NASA/JPL-Caltech/UArizona

HiPOD: Curving Ridges in Aeolis Planum

Multiple processes, which may have occurred billions of years apart, are reflected in this HiRISE image of Aeolis Planum.

Cutting across the scene are curvilinear ridges. These likely represent ancient, meandering river channels that flowed across the surface and buried themselves over time. The channels have subsequently been exposed to the surface by the wind, forming the cross-cutting ridges.

uahirise.org/ESP_079382_1735
NASA/JPL-Caltech/UArizona

How Tiny Red Stars Can Test Ideas about the Origin of Life

Ultracool dwarf stars lack the UV light thought to be needed to kick-start life

sciencenews.org/article/dwarf-

HiRISE 3D: Streamlined Features in Athabasca Valles

The rationale for this observation was elegantly simple: to extend coverage of spectacular landscape.

Full image: uahirise.org/anaglyph/ESP_0805

NASA/JPL-Caltech/UArizona

HiPOD: A Sedimentary Fan in Southeast Gale Crater

This image covers a fan of sedimentary rock on the southeast crater floor. Ridges on the fan surface may be composed of coarse-grained sediment deposited in ancient streams. More recent wind erosion of the surrounding finer sediments could have left these channel deposits elevated in “inverted relief.” A closeup shows some of these ridges, as well as light-toned layers of sediment.

uahirise.org/ESP_079699_1740
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Recent Impact near Hebrus Valles

This impact occurred inside a double quasi-concentric circular graben structure. These features have been interpreted as the result of compaction of soft sediments filling a large crater basin.

Full image: uahirise.org/anaglyph/ESP_0727
NASA/JPL-Caltech/UArizona

HiPOD: Muddy Mounds

Mud volcanoes form as gas and liquid-rich sediment interacts underground. Over time, this slurry of mud is brought to the surface and forms a rounded mound. Scientists are interested in studying mud volcanoes on Mars because the material forming the mound has the potential to be organic in nature and would give insight into possible microbial life below the surface.

uahirise.org/hipod/ESP_080034_
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Crater and Its Frozen Ejecta

A post in two pics: the classic bowl-shaped crater and some of the higher-standing ejecta to the immediate north.

Full image: uahirise.org/anaglyph/ESP_0806

NASA/JPL-Caltech/UArizona

HiPOD: A Three-in-One in Meridiani Planum

With this observation, we were able to get three targets of interest in a single image: good candidates for recurring slope lineae on the slopes, small gullies and the entire impact crater itself. Meridiani straddles the Martian equator and is one of the most investigated regions of Mars.

ID: ESP_074482_1795
date: 16 June 2022
altitude: 268 km

uahirise.org/hipod/ESP_074482_
NASA/JPL-Caltech/UArizona

A Fissure Vent East of Olympus Mons

This fissure is one of many in the volcanic plains east of Olympus Mons. The purpose of the image is to resolve any erupted material and overlap the adjacent HiRISE stereo pair to expand DTM coverage.

Full image: uahirise.org/anaglyph/ESP_0807

NASA/JPL-Caltech/UArizona

HiPOD: Out of Eberswalde

This observation shows us the most prominent of several channels around the margin of the basin upstream of the Eberswalde delta. With a closer look and stereo pair at some point, we can study the channel in better detail and determine valley dimensions.

ID: ESP_074470_1555
date: 16 June 2022
altitude: 258 km

uahirise.org/hipod/ESP_074470_
NASA/JPL-Caltech/UArizona

HiRISE 3D: In Ares Vallis

Our science goal is to document stratigraphic relationships between chaos blocks and adjacent geologic units.

Full image: uahirise.org/anaglyph/ESP_0807

NASA/JPL-Caltech/UArizona

HiPOD: Ridges near Nilosyrtis Mensae

The objective of this observation is to determine the nature of a group of ridges. They may be inverted terrain. The surface of Nilosyrtis Mensae is classified as fretted terrain. This terrain contains cliffs, mesas, and wide flat valleys. Surface features are believed to have been caused by debris-covered glaciers.

ID: ESP_074466_2100
date: 15 June 2022
altitude: 285 km

uahirise.org/hipod/ESP_074466_
NASA/JPL-Caltech/UArizona

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HiRISE (NASA)

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