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
Noachian Bedrock Diversity
In an adjacent image we acquired in 2008, there was terrific color and texture diversity, so this observation was acquired to extend coverage. There are clays mixed with unaltered mafics in this area as well. “Noachian” refers to the early geologic period after Mars formed, 3 to 4 billion years ago.
ID: ESP_022601_1975
date: 23 May 2011
altitude: 279 km
https://uahirise.org/hipod/ESP_022601_1975
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Terracing Inside and Outside a Degraded Crater Rim
This image shows multiple bands on the inside and outside of a crater rim that may be terraces. Are they paired topographically?
Full image: https://www.uahirise.org/anaglyph/ESP_040785_2135_ESP_041286_2135_RED
HiRISE 3D: A Buffet of Secondary Craters
This observation is part of a study that aims to characterize how secondary crater shape depends on distance from source craters and hence impact velocity.
Full image: https://www.uahirise.org/anaglyph/ESP_040927_1880_ESP_041428_1880_RED
HiRISE 3D: A Possible Fresh, Small Crater in Arcadia Planitia
With this anaglyph, we can look for rocks, textures and excavated stratigraphy.
Full image: https://www.uahirise.org/anaglyph/ESP_041348_2225_ESP_015898_2225_RED
NASA/JPL-Caltech/UArizona
HiPOD: Colorful Impact
Our enhanced image reveals colors ranging from red to green to blue. These are infra-red shifted colors (infrared-red-blue) so it’s different than what we would see with our eyes.
HiPOD: Seasonal Flows in the Central Mountains of Hale Crater
The recurring slope lineae (RSL) in Hale have an unusually “reddish” color compared to most RSL, perhaps due to oxidized iron compounds, like rust. Since HiRISE color is shifted to infra-red wavelengths, they are actually especially bright the near-infrared just beyond the range of human vision.
HiPOD: Layering in Spallanzani Crater
In this image, we can see quite a spectacular layering pattern inside an impact crater called Spallanzani. Seeing layering is always exciting to geologists because it implies that the region has experienced multiple climatic conditions or geologic processes through time.
HiRISE 3D: Dunes in 3D
These dunes are also visible in MOC images.
https://www.uahirise.org/anaglyph/ESP_041434_1910_ESP_040023_1910_RED
NASA/JPL-Caltech/UArizona
HiPOD: Yardangs in Arsinoes Chaos
The slightly curving, sublinear bright terrain is composed of yardangs. Yardangs are portions of rock that have been sand blasted into long, skinny ridges by saltating (or bouncing) sand particles blowing in the wind.
HiPOD: A Polar Smile
This image represents one of many monitoring sites at the South Pole residual cap (SPRC). Images are taken throughout the Martian year to document changes in carbon dioxide ice coverage.
This image shows a popular spot where one of the features resembles a smiley face that is approximately 500 meters across. If you smile at Mars, sometimes it smiles back.
https://uahirise.org/hipod/ESP_039115_0945
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Crater Ejecta Crosscut by Channels in Aeolis Dorsa
One of our goals is to seek confirmation of multiple episodes of flow: are the channels filled by fluvial materials, debris flows, or something else?
Full image: https://www.uahirise.org/anaglyph/ESP_080437_1735_ESP_080727_1735_RED
HiPOD: Valleys in Deltoton Sinus
The objective of this observation is to examine valleys on the wall of an old crater. These valleys are wide, and then they get narrow and become very steep. There may have been waterfalls here. The scene can be found in Context Camera data. The name means “bay of the triangle” and its location makes triangle with Iapygia and Oenotria.
https://uahirise.org/hipod/ESP_074704_1750
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
HiRISE 3D: Ridges on the Floor of Shalbatana Vallis
These curved ridges are real, and they’re spectacular!
https://www.uahirise.org/anaglyph/ESP_080233_1885_ESP_080589_1885_RED
NASA/JPL-Caltech/UArizona
#Mars #science #3D
HiPOD: In an Unnamed Crater
Also available in Context Camera data, we acquired this observation to examine gullies in a small, southern mid-latitude crater. Images like this one will help us increase our inventory of Martian gullies. This scene is located in Terra Sirenum, in the Southern Hemisphere of Mars.
https://uahirise.org/hipod/ESP_074698_1340
NASA/JPL-Caltech/UArizona
#Mars #science #NASA
The Rings of Uranus Glow in Epic JWST Photo
https://www.scientificamerican.com/article/the-rings-of-uranus-glow-in-epic-jwst-photo/
HiRISE 3D: Layered Late-Stage Fan in Gale Crater
Our rationale is to search for boulders for comparison to Gediz Vallis ridge currently adjacent to the Curiosity rover.
Full image: https://www.uahirise.org/anaglyph/ESP_080187_1755_ESP_080332_1755_RED
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.