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
HiRISE 8K: Bright Streaks and Dark Fans
The conditions must be just right for the bright frost to condense.
Full cutout on Flickr: https://flic.kr/p/2prSfq6
HiRISE 3D: Like a Big Pizza Pie…
Only this one is seen from the Mars sky! This image shows a pie-like feature which is hypothesized to be the result of subsurface sediment mobilization.
Full image: https://www.uahirise.org/anaglyph/ESP_077213_1985_ESP_080747_1985_RED
HiPOD: Terrain in Hebes Chasma
Hebes Chasma is an isolated depression to the north of Valles Marineris, with no outflow channels. Some material on the walls of the chasma is different from the central mesa. We obtained this observation to investigate a possible landslide within the stratified sediments from one of the chasma’s walls.
ID: ESP_074722_1785
date: 5 July 2022
altitude: 267 km
https://uahirise.org/hipod/ESP_074722_1785
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 4K: Isolated Araneiform Topography
Have you ever found that to describe something you had to go to the dictionary and search for just the right word?
Full cutout on Flickr: https://flic.kr/p/2prGXV7
NASA/JPL-Caltech/UArizona
HiRISE 3D: Layered Ejecta
This double pic shows an impact crater with its ejecta blanket that has withstood erosion to be elevated above the surrounding terrain.
Full image: https://www.uahirise.org/anaglyph/ESP_080686_1810_ESP_045225_1810_RED
HiPOD: A Clay-Rich Mound in an Eroded Plateau
These mounds contain bright-toned material which have been found to be clay-bearing with data from the CRISM instrument on MRO. This particular example contains both aluminum and iron/magnesium bearing clays. These regions of bright-toned material are layered down to the meter scale and are heavily fractured, reminiscent of the clay-bearing deposits at Mawrth Vallis.
https://uahirise.org/hipod/ESP_074720_2030
NASA/JPL-Caltech/UArizona
#Mars #science
HiClip mini 4K: Ridges of Times Past
Also visible in Context Camera data, objective of this observation is to determine the nature of a field of ridges near Apollinaris Sulci. (This is a non-narrated clip with ambient sound.)
HiPOD: Dunes of an Unnamed Crater
This scene is located within an unnamed impact crater to the northwest of the larger Antoniadi Crater in the Northern Hemisphere of Mars. We obtained this image to observe possible changes in dune position, and for more coverage of star dunes, which are dunes with arms radiating from a central peak. Star dunes are more common on Mars than on Earth.
https://uahirise.org/hipod/ESP_074717_2065
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
How the Shapes of Martian Sand Dunes Reveal the Planet’s winds – https://www.astronomy.com/science/the-shapes-of-martian-sand-dunes-reveal-the-planets-winds/
HiRISE 3D: Nili Patera Dunes
We acquired this observation to provide further high resolution images of the Nili Patera dune field.
https://www.uahirise.org/anaglyph/ESP_040654_1890_ESP_040021_1890_RED
NASA/JPL-Caltech/UArizona
HiPOD: Dunes on the Floor of Huggins Crater
Dunes are particularly suited to comprehensive planetary studies because they are abundant over a wide range of elevations and terrain types. A global scale study of Martian dunes serves a dual purpose in furthering understanding of both climatic and sedimentary processes, two fundamental topics currently driving Martian science.
https://uahirise.org/hipod/ESP_074727_1310
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiPOD: The Hills in Ganges Chasma
Ganges Chasma is in the northeast portion of Valles Marineris, and opens into outflow channels that flowed to the north.
Scattered hills on the canyon floor may be remnants of chaos terrain that formed from collapse of the canyon. Some of the bedrock has diverse colors as we see in the enhanced-color cutout.
https://uahirise.org/hipod/ESP_054609_1720
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Light-Toned Layered Deposits Exposed along Coprates Chasma Floor
Context Camera data shows exposure of light-toned layered deposits at this location. Our resolution can take a closer look at the details in the layering.
Full image: https://www.uahirise.org/anaglyph/ESP_032931_1645_ESP_040975_1645_RED
Channels near Huygens Crater
The objective of this observation is to examine channels on the outside of an impact crater. They lead away from the rim, and perhaps they were formed by the heat of the impact melting ground ice. There are many additional channels located in this general area, and much ice may have been present in the ground. This scene is also covered in Context Camera data.
https://uahirise.org/hipod/ESP_074717_1640
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Dune Monitoring in a Northern Mid-Latitude Crater
This was part of a seasonal series to track changes over time. This image had less frost than previous observations.
https://www.uahirise.org/anaglyph/ESP_080585_2230_ESP_080097_2230_RED
NASA/JPL-Caltech/UArizona
Megaripple Stripes on Mars
Among the undulating topography of this dune field in Rabe Crater, one notable feature is the presence of distinct megaripple stripes. Intermediate in size relative to larger dunes and smaller ripples, these megaripples gather in parallel rows, their formation guided by wind patterns and the distribution of grain sizes.
ID: ESP_058009_1355
date: 11 December 2018
altitude: 250 km
https://uahirise.org/hipod/ESP_058009_1355
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Volcanoes and Collapses
This image of Hephaestus Fossae shows a volcanic area where collapses like this happen. Chains of large elliptical pits mark the path that underground molten rock took.
https://www.uahirise.org/anaglyph/ESP_080227_2015_ESP_079739_2015_RED
NASA/JPL-Caltech/UArizona
Hematite in Capri Chasma
The Thermal Emission Spectrometer on the Mars Global Surveyor detected hematite along the chasma floor and edges of these mesas in Capi Chasma. Hematite on Earth is typically formed in aqueous environments or by aqueous alteration, so its presence warranted investigation by the two Mars Exploration Rovers, Spirit and Opportunity, that found a significant amount of the mineral.
https://uahirise.org/hipod/ESP_022698_1670
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Light-Toned Exposures near Voeykov Crater
Our goal here is a comparison with CaSSIS DTM and stratigraphy. CaSSIS also identified peculiar color variation here.
https://www.uahirise.org/anaglyph/ESP_080340_1465_ESP_080274_1465_RED
NASA/JPL-Caltech/UArizona
The Floor of Mawrth Vallis
CRISM data shows a localized, unique spectral phase consistent with poly-hydrated sulfate or zeolite here on the Mawrth Vallis channel floor, with implications for the regional history. This target provides both color coverage and stereo over the outcrop. We can also look for textual differences between new hydrated mineral and adjacent clays.
date: 21 May 2011
altitude: 285 km
https://uahirise.org/hipod/ESP_022578_2030
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
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