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HiRISE 3D: Cliffs and Patterned Ground near Hellas Basin

There is basketball-like patterned ground here that also surrounds the steep, rocky cliffs.

Full image: uahirise.org/anaglyph/ESP_0406

NASA/JPL-Caltech/UArizona

HiPOD: An Inlet Valley to Jezero Crater

Our science goal is to study the fluvial bedforms in this inlet valley located to the west of Jezero. With stereo and a digital terrain model, we can obtain information about cross-sections in the topography.

uahirise.org/hipod/ESP_074413_
NASA/JPL-Caltech/UArizona

HiRISE 3D: A Tyrrhena Terra Crater with Altered Minerals

Not much by way of an image rationale, but the bedrock and dark dunes in this 3D image are worth staring at for a while.

Full image: uahirise.org/anaglyph/ESP_0410

NASA/JPL-Caltech/UArizona

HiPOD: Crater on a Wrinkle Ridge

This observation can inform us about the impact cratering process here along this wrinkle ridge, as well as see if there are any flow ejecta on the side of the crater wall. We can also take a look at the topography of the wrinkle ridge and its direction and shape.

uahirise.org/hipod/ESP_074392_
NASA/JPL-Caltech/UArizona

HiRISE 3D: Would You Land Here?

While it might look tempting, our 3D images of areas within potential landing ellipses can help us determine where safe places are for future missions.

Full image: uahirise.org/anaglyph/ESP_0273

NASA/JPL-Caltech/UArizona

HiPOD: Steep Southern Slopes

Slopes in southern Coprates Chasma, to be exact. We have very little existing imagery along this portion of Coprates’s south wall. This observation will fill in the gaps and get unique coverage as we also look for colorful slopes of mafic materials.

uahirise.org/hipod/ESP_074392_
NASA/JPL-Caltech/UArizona

The Search For “Brain Coral” On Mars: It’s not just dried up lakes and river valleys that suggest the action of liquid water on the Martian surface, say planetary geologists.

discovermagazine.com/the-scien

HiRISE 3D: Streamlined Features in Olympica Fossae

Always a scenic target in a dusty region with few other good targets.

Full image: uahirise.org/anaglyph/ESP_0284

NASA/JPL-Caltech/UArizona

HiPOD: The Joy of Frost

We have imaged this area many times before, and like those previous observations, we want to monitor these very active polar pit gullies for frost and fresh deposits.

uahirise.org/hipod/ESP_074390_
NASA/JPL-Caltech/UArizona

HIPOD: Wrinkles in Rock

The bedrock in this region of Arabia Terra has been worn away by the wind, revealing their internal structure and geologic history.

The wavy lines are individual layers of sand and dust, originally laid down as the bedrock was forming. These patterns indicate that the bedrock formed as layers of sand and dust lost their confrontation with the relentless Martian wind in a desert-like environment.

uahirise.org/hipod/PSP_003418_
NASA/JPL-Caltech/UArizona

HiPOD: The Case of the Martian Boulder Piles

What organized these boulders into neatly-spaced piles? In the Arctic back on Earth, rocks can be organized by a process called “frost heave.” With frost heave, repeatedly freezing and thawing of the ground can bring rocks to the surface and organize them into piles, stripes, or even circles.

More: uahirise.org/hipod/ESP_053924_

NASA/JPL-Caltech/UArizona

HiPOD: A Volcano of Mud or Lava?

This image shows a hill with a central crater. Such features have been interpreted as both mud volcanoes (really a sedimentary structure) and as actual volcanoes (the erupting lava kind). They occur on the floor of Valles Marineris below a closed topographic contour that could have held a lake, and the compaction of wet sediments may have created mud volcanoes.

uahirise.org/hipod/ESP_054649_
NASA/JPL-Caltech/UArizona

HiPOD: Bedrock Exposed in the Rim of Hale Crater

Hale Crater is a large impact crater (more than 100 kilometers) with a suite of interesting features such as active gullies, active recurring slope lineae, and extensive icy ejecta flows. There are also exposed diverse (colorful) bedrock units.

Note: North is down, so that the slope is down to the bottom of the cutout and illumination from the upper right.

uahirise.org/hipod/ESP_054701_
NASA/JPL-Caltech/UArizona

New Map Reveals Secrets of Io, the Solar System’s Most Volcanic Moon

The best-yet map of active volcanoes on Jupiter’s moon Io hints at a hidden magma ocean—and more

scientificamerican.com/article

HiClip mini 4K: Ab antiquo

This observation was acquired to look at contact between light-toned deposits and chaos mounds. This is a non-narrated clip with ambient sound.

youtu.be/oTDsEGIJPoY

HiPOD: Rising above It in Amazonis Planitia

This image shows a bright, rectangular-looking landform surrounded by a dark floor. How did this feature get here if it looks so different than its surroundings?

The feature resembles a plateau. Dark streaks mark steep slopes on its sides while the top appears flat. The slope streaks are not all the same age, as we see a variation in colors from faint to dark.

More: uahirise.org/hipod/ESP_055022_

NASA/JPL-Caltech/UArizona

HiPOD: A Fan with Inverted Channels

This image shows inverted channels within a fan whose origin could be either fluvial (produced by the action of a stream) or alluvial (created by sedimentary deposits).

If the fan is alluvial, then it formed on dry land. If the fan is fluvial, then it could have formed in water, like a delta.

More: uahirise.org/hipod/ESP_055505_

NASA/JPL-Caltech/UArizona

HiPOD: Gullies in Ius Chasma

Pristine gullies are common on steep slopes in the middle latitudes of Mars, where they are shaped by the action of carbon dioxide frost. There are also pristine gullies in equatorial Valles Marineris where little carbon dioxide frost is deposited.

More: uahirise.org/hipod/ESP_080617_

NASA/JPL-Caltech/UArizona

Atomic Oxygen Detected on Venus

New data provide direct evidence for the existence of atomic oxygen in Venus's upper atmosphere, enabling new science on our sister planet.

skyandtelescope.org/astronomy-

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HiRISE (NASA)

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