TagsAeolis Mons Arizona State University ASU atmosphere Beautiful Mars Cape Tribulation channels craters Curiosity dunes dust Endeavour Crater ESA 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: NASA
Disrupted terrain in southern Elysium Planitia. Beautiful Mars series.
Floor of Ius Chasma. Beautiful Mars series.
THEMIS Image of the Day, January 23, 2017. Today’s VIS image shows dust devil tracks in Argyre Planitia. The dark streaks are made by dust devil activity scouring the surface and removing the lighter toned dust to reveal the darker … Continue reading
Sol 1586-88, January 20, 2017, update by USGS scientist Ken Herkenhoff: MSL drove another 13 meters on Sol 1585, again placing the rover in a good position for contact science. But the telemetry also showed that ChemCam had been marked … Continue reading
Sol 1585, January 19, 2017, update by USGS scientist Ken Herkenhoff: After a 31-meter drive on Sol 1584, MSL is in position for contact science on a block of bedrock in front of the rover. So, as MAHLI/MARDI uplink lead … Continue reading
The large dark feature is a classic Martian sand dune. Most sand on Earth is made from the mineral quartz, which is white and bright. On Mars, most sand is composed of dark basalt, a volcanic rock. For this reason, … Continue reading
Sol 1584, January 19, 2017. Curiosity drove some 30 meters (100 feet) south from yesterday’s position, and its sand-patch-dodging path has brought it slightly closer to Ireson Hill. Seen in the Navcam composite below, the hill is now about 100 … Continue reading
Landforms at west end of Her Desher Vallis. Beautiful Mars series.
THEMIS Image of the Day, January 20, 2017. Today’s false color image shows part of the floor of Gale Crater and the northern side of Mt. Sharp (Aeolis Mons). The blue-colored areas on the crater floor are likely dunes made … Continue reading
Ed. note: The following is an except from a story in Nature; full story here. Adam Steltzner rose to engineering stardom in 2012, when NASA’s Curiosity rover plummeted to a perfect landing on Mars, thanks to a daring, fiery manoeuvre … Continue reading
Unusual gullied slope in southern mid-latitudes. Beautiful Mars series.
Sol 1584, January 18, 2017, update by USGS scientist Lauren Edgar: On Sol 1583 Curiosity drove 16 m, which set us up for touch-and-go contact science today. I was the GKOP again, and it was a fun day of planning … Continue reading
THEMIS Image of the Day, January 19, 2017. Today’s false color image shows part of the interior of Hale Crater. The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create … Continue reading
Roadside bedrock outcrops are all too familiar for many who have taken a long road trip through mountainous areas on Earth. Martian craters provide what tectonic mountain building and man’s TNT cannot: crater-exposed bedrock outcrops. Although crater and valley walls … Continue reading
Sol 1583, January 18, 2017. After driving 16 meters (55 feet) south-southwest, Curiosity used its Navcam to image Ireson Hill (left) and a more distant butte almost superimposed. From this point Ireson Hill lies about 100 meters away, while the … Continue reading