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HiRISE 3D: A Low Mound East of Echus Chasma
Our science goal is to determine if flow units sourced from area and nearby possible low shield volcanoes. A DTM can help to measure height.

uahirise.org/anaglyph/ESP_0787
NASA/JPL-Caltech/UArizona

HiPOD 26 Jul 23: No Devil in These Details

But there are layers in the details! Our science goal for this observation is to get a high resolution image to see more details about the light-toned deposits in this part of Iani Chaos. Could they be sulfates or other hydrated materials? Iani Chaos is a region of chaos terrain at the southern end of the Ares Vallis outflow channel.

uahirise.org/hipod/ESP_073876_
NASA/JPL-Caltech/UArizona

HiClip mini 4K: Like unto the Aiel Waste

This image features a section of Gorgonum Chaos, a set of canyons that may once have contained a lake. Some of the first gullies on Mars were located here.

This is a non-narrated clip with ambient sound.

youtu.be/yzJLs5EQg1k

HiRISE 3D: Dune Monitoring in Terra Cimmeria

Sooner or later, and it’s usually later, there will be changes over time.

uahirise.org/anaglyph/ESP_0789
NASA/JPL-Caltech/UArizona

HiPOD 25 Jul 23: Of RSL and ILD

Previous images of this area shows what appear to be recurring slope lineae (RSL) behavior coming from an interior layered deposit (ILD) on the north face. One image showed RSL, a follow-up indicated the RSL was not as lengthy, and another showed it as being subsequently longer. More images that show incremental changes are needed to confirm this as RSL. Additionally, these interior layered deposits might be composed of sulfate.

uahirise.org/hipod/ESP_073878_

HiRISE 3D: Layered Materials on the Floor of Ritchey Crater

This has been one of the potential landing sites for the Mars Science Laboratory (now in Gale Crater), and high resolution was requested to assess the safety and evaluate the slopes.

uahirise.org/anaglyph/ESP_0419
NASA/JPL-Caltech/UArizona

HiPOD 24 Jul 23: Where the Wind Blows

With this observation, we look at changes since 2010 and with other subsequent images that we have acquired of this area. Bidirectional wind regimes were detected here, so tighter imaging will help understand when east- or west-blowing winds dominate. Dunes are particularly suited to comprehensive planetary studies because they are abundant over a wide range of elevations and terrain types.

uahirise.org/hipod/ESP_073531_
NASA/JPL-Caltech/UArizona
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HiRISE 10K: Light-Toned and Rugged

This image footprint shows us a stunning view of light-toned substrate and rocky outcrops.

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

NASA/JPL-Caltech/Arizona

HiRISE 3D: Ridges and Cracks on a Crater Floor

The objective of this observation is to examine ridges and cracks on the floor of an impact crater, with many more details than the Context Camera image.

uahirise.org/anaglyph/ESP_0618

HiPOD 21 Jul 23: Elysium Lava Plains and Craters

Unlike on Earth, there are lots of craters on this lava plain, and you might notice that some of the craters have dark interiors and a spray of darker material around them, but most don't. This difference is telling you something about the difference in age of these craters.

More: uahirise.org/hipod/ESP_078208_

NASA/JPL-Caltech/UArizona

Made with HiRISE: Elyn Zimmerman

HiRISE images provide inspiration for this Los Angeles-based artist. Read the profile and view some of her work: uahirise.org/epo/made-with-hir

HiRISE 8K: On the Rim of Hale Crater

Possible clays may have been detected on the southeast rim. And the view is spectacular!

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

NASA/JPL-Caltech/Arizona

HiRISE 3D: Steeply Mesmerizing

This image footprint shows us a small part of the caldera wall that is Pavonis Mons.

uahirise.org/anaglyph/ESP_0785
NASA/JPL-Caltech/UArizona

HiPOD 20 Jul 23: Channel within a Valley in Northern Arabia Terra

The valley containing this channel measures 1.5 km across, while the channel itself spans just 200 m. Several rock layers are visible along the channel walls, and dunes fill the channel floor. The channel cuts back and forth across the valley floor, which suggests surface water was present in the valley over long time periods.

More: uahirise.org/hipod/ESP_079084_

NASA/JPL-Caltech/UArizona

HiRISE 4K: Ripples within Slope Streak Beds

Recently formed slope streaks are typically darker than their surroundings and appear to fade (i.e., brighten) over time.

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

NASA/JPL-Caltech/Arizona

HiRISE 3D: From Valley to Inverted Channel

This terrain transitions from geologically older to younger, and there might have been a possible paleolake here.

uahirise.org/anaglyph/ESP_0789
NASA/JPL-Caltech/UArizona

HiPOD 19 Jul 23: Pitted Mounds in Acidalia Planitia

This image in the Acidalia Planitia region of Mars shows numerous round hills that have a large circular depression on their tops. These pitted mounds may be ancient mud volcanoes that formed when liquid mud erupted from underground due to shaking from a nearby Marsquake.

More: uahirise.org/hipod/ESP_078491_

NASA/JPL-Caltech/UArizona

HiClip mini 4K: Colors of the Undiscovered Country

Nili Fossae is one of our favorite places to image, not the least of all the incredibly dense terrain here where clays have been detected. This is a non-narrated clip with ambient sound.

youtu.be/S3IICNEaeDo

HiRISE 3D: Streamlined Landforms adjacent to Shalbatana Vallis

These formations show multiple levels of fluvial dissection.

uahirise.org/anaglyph/ESP_0788
NASA/JPL-Caltech/UArizona

HiPOD 18 Jul 23: Scarps and Pits

Some areas of Mars show a kind of selective erosion. In this image, an overlapping pit formed between one level of the surface and another. One idea is that the ground once contained significant amounts of ice in layers a few meters thick that have evaporated. Without the ice, the ground surface subsides and collapses down to a new and somewhat level surface.

More: uahirise.org/hipod/ESP_078316_

NASA/JPL-Caltech/UArizona

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HiRISE (NASA)

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