Mars Express Images Reveal Mars’ Pockmarked Surface https://www.universetoday.com/articles/mars-express-images-reveal-mars-pockmarked-surface
@uahirise
Images from the High Resolution Imaging Science Experiment (HiRISE) on board the Mars Reconnaissance Orbiter (NASA). We are based out of the Lunar and Planetary Laboratory at the University of Arizona in Tucson, AZ. https://uahirise.org
Mars Express Images Reveal Mars’ Pockmarked Surface https://www.universetoday.com/articles/mars-express-images-reveal-mars-pockmarked-surface
Terraforming Mars Isn’t a Climate Problem—It’s an Industrial Nightmare - Universe Today https://www.universetoday.com/articles/terraforming-mars-isnt-a-climate-problemits-an-industrial-nightmare
NASA’s DART spacecraft changed an asteroid’s orbit around the sun https://www.sciencenews.org/article/spacecraft-changed-asteroid-orbit-nasa
3D image shows a slope of layers throughout the entire scene. This is a smal part of Candor Chasma, within the giant Valles Marineris canyon system on Mars. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: In Candor Chasma
These layers are well-exposed over a wide range of elevations. And also look spectacular in 3D.
https://www.uahirise.org/anaglyph/ESP_037586_1725_ESP_037731_1725_RED
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
HiPOD: Slope Streakin’
This image shows many slope streaks of various orientations at fairly high latitude. Our goal is to monitor for seasonality and directionality of streak formation.
https://uahirise.org/hipod/ESP_076768_2115
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiPOD: Boundary Boulders
With the resolution of HiRISE we can see that the reason one side of the boundary is darker than the other is due to the many boulders strewn across the darker side.
https://uahirise.org/hipod/ESP_071923_2260
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiPOD: Varied Types of Rock in a Crater in Eos Chasma
This image shows a crater on the floor of Eos Chasma, part of the Valles Marineris canyon system. Craters on Mars are useful for geologists because they provide cross-sections into the subsurface.
https://uahirise.org/hipod/ESP_072413_1700
Aerial view of a rugged, cratered terrain with deep shadows highlighting the uneven surface and rocky formations on the surface of Mars.
HiPOD: Collapsed Material to the North of Ganges Chasma
This public target suggestion via HiWish shows a collapsed crustal block within an approximately 2-kilometer deep crustal depression.
https://uahirise.org/hipod/ESP_076765_1765
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
3D image shows an impact crater with a very eroded rim on the Sorth Polar layered deposits of Mars. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: A Crater on the Sorth Polar Layered Deposits
This crater has not been imaged in HiRISE before, and obtaining a diameter measurement will improve knowledge of age and accumulation rate of the SPLD.
https://www.uahirise.org/anaglyph/ESP_040097_0970_ESP_040334_0970_RED
#Mars #NASA #science
HIPOD: Mounds in Oxia Colles
This landform shows distinctive layering in Context Camera image data, and is similar to other buttes to the far northeast of this locale.
https://uahirise.org/hipod/ESP_076751_2015
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiRISE 3D: Monitoring Wind Streak and Intracrater Dunes
We obtained this image four Mars years after earlier stereo in 2007. This anaglyph would allow paired DTMs to be constructed with the previous one to assess changes.
https://www.uahirise.org/anaglyph/ESP_037669_1920_ESP_037603_1920_RED
HiPOD: The Upper Section of a Channel in Gale Crater
This observation features an upper section of a canyon channel system that incising Mount Sharp in Gale Crater. A HiRISE image was requested as the canyon system is analogous to Gediz Vallis.
https://uahirise.org/hipod/ESP_076745_1750
#Mars
3D image shows a large mound rising above otherwise flat terrain that is likely an ancient flow of some kind. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: A Flow Obstacle in a Debris Apron
Our goal here is to investigate flow dynamics around what might be a “nunatak.” On Earth a nunatak is an isolated mountain peak that once projected through a continental ice sheet.
https://www.uahirise.org/anaglyph/ESP_090107_2215_ESP_090608_2215_RED
HiPOD: The Upstream Edge of a Crater in Athabasca Valles
This image provides a closer look at lava-topography interactions in this area. Athabasca Valles is a young outflow channel system on Mars that may have been carved by catastrophic water floods.
https://uahirise.org/hipod/ESP_076652_1885
HiPOD: Those Transversing Dunes
This wonderful image was acquired to study basin-driven wind regimes with what the suggester termed an “epic Argyre rim dune field under adiabatic flow.”
More: https://uahirise.org/hipod/ESP_076726_1355
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiPOD: Defrosting Dunes in Kaiser Crater
The dark sand dune at the center of this observation is covered in a blanket of white seasonal ice in the winter. In this Martian springtime image, the western slope of the dune is partly defrosted.
https://uahirise.org/hipod/ESP_072042_1330
#Mars #science
HiRISE 10K: Bright and Dark Terrain in Noctis Labyrinthus
This image shows the transitional terrain where the linear troughs and rounded pits of Noctis Labyrinthus merge with the larger chasmata of Valles Marineris.
Full cutout on Flickr: https://flic.kr/p/2rYJ9Ac
#Mars #NASA #science
*crater’s*
HiPOD: Glacial Flow Meets Central Pit
This observation features a thin glacial flow into an impact crater’ central pit. This image can be useful for constraining ice dynamics. Additionally, differential erosion of the crater slopes is also visible.
https://uahirise.org/hipod/ESP_076718_2150
#Mars
3D images shows a large flow feature that extends across the width of a very ancient and eroded impact crater. There is a small breach in the rim at one point. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: Viciously Viscous
Perhaps “vicious” is too harsh. Here we see a glacial like flow lobe crosses this crater floor from the northeast to southwest.
https://www.uahirise.org/anaglyph/ESP_037659_1420_ESP_028943_1420_RED
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
HiRISE 8K: Dune Composition
Dunes and sand ripples of various shapes and sizes, such as this cutout, show the natural beauty created by physical processes.
Full cutout on Flickr: https://flic.kr/p/2rYsM8s
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
3D image shows a shallow depression, a constriction, in part of the terrain in Grjota Valles on Mars. There is also a large mound within the constriction. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: In Grjota Valles
This image shows a constriction in Grjota Valles, eroded by water or lava but now filled by lava. Topography of locations like this provides useful constraints on the dynamics of water and lava flows.
https://www.uahirise.org/anaglyph/ESP_037617_1920_ESP_029468_1920_RED
Image cutout shows a large depression called a graben on the surface of Mars. The floor of the depression appears relatively smooth. The sides of the graben appear to have layering.
Enhanced color cutout shows a closeup of one of the graben walls, that expose the layers in better resolution. Some of the layers are light-toned in color.
HiPOD: Layering in a Graben Wall
A short but elegant rationale: “nice layering apparent in Mars Orbiter Camera images, worth a closer look for regional stratigraphy.” Graben are depressions that form along parallel faults due to tectonic extension.
https://uahirise.org/hipod/ESP_076715_2265
Close-up of a textured surface showing concentric circular patterns with fine ridges and grooves in grayscale.
HiRISE 4K: Weird Crater Features
In a Context Camera image of this area, the crater floor has hollows and a high density of pits.
Full cutout on Flickr: https://flic.kr/p/2rYiTR6
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
3D image shows a part of an eroded impact crater with incised gullies on the wall and folded terrain at the bottom of the slope. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: A Crater in Utopia Planitia
This 3D image shows us the eastern part of an old impact crater with incised gullies and a deformed floor. The entire crater is about 10 km across.
https://www.uahirise.org/anaglyph/ESP_037646_2290_ESP_028719_2290_RED
NASA/JPL-Caltech/University of Arizona
HiPOD: Knobs in East Candor Chasma
This features an interesting area of possible deformation of lacustrine sediment. This observation was requested to support geologic mapping. Candor Chasma is one of the largest canyons that make up Valles Marineris.
https://uahirise.org/hipod/ESP_076713_1730
3D image shows part of a glacial flow feature down the side of a steep slope on the surface of Mars. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: A Nice Flow Feature
This 3D image shows us a lobate flow feature with mantling deposit infill.
https://www.uahirise.org/anaglyph/ESP_037714_1435_ESP_037648_1435_RED
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
Image cutout shows a very large and dark dune field on the surface of Mars. There are ripples and gullies on the dunes as well as visible dust devil tracks throughout the scene, which is less than 5 km (3 miles) across.
HiPOD: Landscape Evolution
This overlaps with a previous image we obtained in 2009 and we have also taken six additional images to monitor gully formation. We want to see how any dune ripples have moved since then.
https://uahirise.org/hipod/ESP_076710_1275
NASA/JPL-Caltech/University of Arizona
3D images shows several small mounds rising above the surface of Mars near an area called Hypanis Valles. The scene is less than 5 km, or 3 miles, across.
HiRISE 3D: Candidate Landing Site near Hypanis Valles
If a rover were to land here, our 3D image can help with assessing how well it could traverse the terrain.
https://www.uahirise.org/anaglyph/ESP_037717_1920_ESP_037651_1920_RED
NASA/JPL-Caltech/University of Arizona
#Mars #NASA #science
The source link is included on the page where ALL the details are listed.