HiRISE (NASA)
HiRISE is a high resolution camera onboard the Mars Reconnaissance Orbiter (NASA). We take images of the surface of Mars. Based out of UArizona in Tucson.
Joined Aug 2018
The Canyon Floor in East Coprates Chasma
The walls (both south and north of this site) potentially expose pristine crustal material. This is an area of interest that could be accessed and is within a potential future rotorcraft landing site.
ID: ESP_075407_1650
date: 28 August 2022
altitude: 263 km
https://uahirise.org/hipod/ESP_075407_1650
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiRISE Epigrammata
“As an endless dream it went on…to find all gods dead, all wars fought, all faiths in man shaken….”
—F. Scott Fitzgerald, “This Side of Paradise”
NASA’s Hubble, MAVEN Help Solve the Mystery of Mars’ Escaping Water – Scientists know that over the last 3 billion years, at least some water went deep underground, but what happened to the rest?
HiRISE 4K: Possible Clays near Margaritifer Chaos
The existence of clay minerals is especially interesting on Mars since we want to know under what conditions these minerals formed. Could it have been the presence of water?
Full cutout on Flickr: https://flic.kr/p/2qiy6Ym
HiRISE 3D: A Possible Future Landing Site in Coprates Chasma
Anaglyph images from HiRISE provide additional detail to characterize hazards within a possible landing ellipse.
Full image: https://www.uahirise.org/anaglyph/ESP_026549_1675_ESP_035265_1675_RED
NASA/JPL-Caltech/University of Arizona
Irregular Graben Features
The graben in this image contains an unusually tall cone with very even sides, and the surrounding terrain is darker in the direction of prevailing wind. This observation could bring out some of the detail around this unusual feature and show possible changes that have occurred over the last ten Earth years in case this area is thermally active.
https://uahirise.org/hipod/ESP_075384_1510
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiRISE 3D: To Measure Heights and Widths of Raised Ridges in a Sedimentary Deposit
When an observation title kinda says it all.
https://www.uahirise.org/anaglyph/ESP_084367_1560_ESP_083866_1560_RED
On Thick Ice
In this fascinating image, we see fractured mounds on thick carbon dioxide ice that may be diapirs or deflation over subglacial topography. The pits may show signs of ongoing collapse. A diapir is a relatively mobile mass that intrudes into preexisting rocks. Diapirs commonly intrude vertically through more dense rocks.
ID: ESP_075399_0920
date: 27 August 2022
altitude: 246 km
https://uahirise.org/hipod/ESP_075399_0920
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiRISE 3D: Gullies!
These gullies on the wall of an impact crater look great in Context Camera data, and now we take an even closer 3D look.
https://www.uahirise.org/anaglyph/ESP_084333_1355_ESP_084122_1355_RED
NASA/JPL-Caltech/University of Arizona
#Mars #science #3D
Resistant Material in Olympus Mons Aureole Ridges
The question of how the Olympus Mons aureole formed has wide-ranging implications for Mars paleoclimate, including whether a northern ocean existed. The properties of the resistant material exposed within aureole blocks can help test the merits of competing hypotheses for the aureole’s formation.
https://uahirise.org/hipod/ESP_075502_2110
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
Tangential Craters within Ptolemaeus Crater
This image shows two small craters, just touching on their rims, in the much larger Ptolmaeus Crater, which is located in the Martian Southern Hemisphere. These craters are called “tangential craters.”
The more degraded and filled-in crater is approximately 3 kilometers in diameter, and there is an unusual feature near the center.
More: https://uahirise.org/hipod/ESP_020065_1335
NASA/JPL-Caltech/University of Arizona
Gigas Sulci
A sulcus (or sulci, plural) is defined as “subparallel furrows and ridges.” This is a purely descriptive term for landforms that could have a variety of origins.
At this location appears to be a graben (which is a fault-bounded valley) on a large scale, and locally (such as in this image) became a vent region for lava flows.
ID: ESP_040661_1890
date: 30 March 2015
altitude: 272 km
https://uahirise.org/hipod/ESP_040661_1890
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiRISE 10K: Layers in Western Arabia Terra
Extensive erosion in this region has exposed numerous rock layers. Layers are visible on the flanks of some hills and on the basement (the lowest rock unit) between the hills.
Full cutout on Flickr: https://flic.kr/p/2qhtV6V
HiRISE 3D: Inverted Channel and Possible Lake Deposits
The former channel had material that was more resistant to erosion than the surrounding terrain, so now stands in positive-relief in our image.
https://www.uahirise.org/anaglyph/ESP_076462_1725_ESP_084242_1725_RED
NASA/JPL-Caltech/University of Arizona
#Mars #science #3D
Phyllosilicate-Rich Terrain in the Ejecta of an Impact Crater
The cutout shows the plains adjacent to the crater’s northwestern rim in enhanced contrast, highlighting the range of compositions sampled by the crater that exhibit a range of colors. Phyllosilicate-rich materials on Mars most commonly have relatively orange colors, whereas some of the bluer material visible here may have been less altered by interaction with water.
More: https://uahirise.org/hipod/ESP_084119_1760
NASA/JPL/University of Arizona
HiRISE 8K: Layers in Northeast Sinus Meridiani
The objective of this image is to examine the exposure of thin layers along the walls of a few-kilometer-wide valley in Sinus Meridiani.
Full cutout on Flickr: https://flic.kr/p/2qhhewm
#Mars #science
HiRISE 3D: Potential Fan Deposit in Crater near Mawrth Vallis
A fanlike deposit (visible in CTX) emerges from a valley on an impact crater wall. Detailed study of this fan could help in understanding the depositional environment and hydrologic system in the region.
https://www.uahirise.org/anaglyph/ESP_084491_1990_ESP_084425_1990_RED
NASA/JPL-Caltech/University of Arizona
#Mars #science
Colorful Terrain Southwest of Dawes Crater
In between the craters and sand cover, the bedrock here shows a range of colors, likely reflecting a range of rock compositions that were perhaps jumbled up by the Dawes and other nearby impacts that occurred over Martian history. The enhanced color cutout shows some green/blue blocks that may contain the igneous minerals pyroxene or olivine.
https://uahirise.org/hipod/ESP_084041_1685
NASA/JPL-Caltech/University of Arizona
#Mars #science #NASA
HiRISE 4K: A Ridge Network in Nili Fossae
The objective of this observation is to examine a network of small ridges. The scene is also visible in Context Camera imagery.
Full cutout on Flickr: https://flic.kr/p/2qh6vz9
HiRISE 3D: A Small Delta or Fan
Delta or fan deposits indicate past water activity. HiRISE can resolve sedimentary characteristics such as layering, stratigraphic relationship to the surrounding geologic setting that cannot be resolved by other camera experiments.
https://www.uahirise.org/anaglyph/ESP_075524_2125_ESP_084359_2125_RED
NASA/JPL-Caltech/University of Arizona
#Mars #science #3D
HiRISE (NASA)
HiRISE is a high resolution camera onboard the Mars Reconnaissance Orbiter (NASA). We take images of the surface of Mars. Based out of UArizona in Tucson.
Joined Aug 2018