TagsAeolis Mons Arizona State University ASU atmosphere Bagnold Dunes Beautiful Mars Cape Tribulation channels craters Curiosity dunes dust Endeavour Crater Gale Crater High Resolution Imaging Science Experiment HiRISE Malin Space Science Systems Marathon Valley MARCI Mars Color Imager Mars Exploration Rover Mars Odyssey Mars Reconnaissance Orbiter Mars Science Laboratory mass wasting MER Mount Sharp MRO MSL MSSS Murray Formation NASA Naukluft Plateau Opportunity Pahrump Hills sand dunes Stimson Formation storms THEMIS Themis Image of the Day Thermal Emission Imaging System University of Arizona volcanics weather wind
- CRISM: Compact Reconnaissance Imaging Spectrometer for Mars
- CTX: Context Camera
- HiRISE: High Resolution Imaging Science Experiment
- MARSIS: Mars Advanced Radar for Subsurface and Ionosphere Sounding
- SHARAD: Shallow Radar
- THEMIS: Thermal Emission Imaging System
- All Mars missions list
- Mars 2020 Rover
- Mars Atmosphere and Volatile Evolution Mission (MAVEN)
- Mars Exploration Rovers (MER)
- Mars Express (MEX)
- Mars Odyssey
- Mars Orbiter Mission (MOM) / Mangalyaan
- Mars Reconnaissance Orbiter (MRO)
- Mars Science Laboratory (MSL)
Tag Archives: periglacial processes
THEMIS Image of the Day, June 23, 2017. Do you see what I see? Make a wish and then break the wishbone! (THEMIS Art #132) More THEMIS Images of the Day by geological topic.
Periglacial terrain. Beautiful Mars series.
Lineated terrain — At first glance, these appear as ridges, but a closer inspection shows patterned ground on a (roughly) level surface. In the absence of a slope, how did these form? Beautiful Mars series.
Possible glacial-like outwash systems in Phlegra Montes. Beautiful Mars series.
Wondrously, wickedly wavy. Beautiful Mars series.
Planetary Geomorphology Image of the Month, July 2015: Alex Barrett (Open University, UK). The following images show the walls of a two kilometre diameter impact crater in Utopia Planitia on Mars. This region is part of the low lying Northern … Continue reading
The mid-latitudes of Mars (about 30 to 60 degrees, north and south) are covered in ice-rich mantling deposits in varying states of degradation. This mantle is thought to be deposited as snow during periods when the angle of the tilt … Continue reading