Tag Archives: dunes

HiRISE: Frosty alcoves on Kaiser Crater dunes

Kaiser Crater hosts a large field of sand dunes. Every winter the dunes are covered with a layer of seasonal carbon dioxide ice (dry ice). In early spring the ice begins to sublimate (going directly from solid ice to gas). … Continue reading

Posted in Reports | Tagged , , , , , , , , , , | Comments Off

HiRISE: Barchan dunes, Dulovo Crater region

Barchan dunes in the Dulovo Crater region. Beautiful Mars series.

Posted in Reports | Tagged , , , , , , , , , | Comments Off

HiRISE: Crater floor with dunes and mounds

Uncomplicated. Beautiful Mars series.

Posted in Reports | Tagged , , , , , , , , , | Comments Off

HiRISE: Landforms north of Allegheny Vallis

Landforms in a crater north of Allegheny Vallis. Beautiful Mars series.

Posted in Reports | Tagged , , , , , , , , , , | Comments Off

HiRISE: Tracking dune changes in Chasma Boreale

Tracking dune changes in Chasma Boreale. Beautiful Mars series.

Posted in Reports | Tagged , , , , , , , , , , | Comments Off

HiRISE: Just rise above it

Just rise above it. Beautiful Mars series.

Posted in Reports | Tagged , , , | Comments Off

THEMIS: Dunes on floor of Juventae Chasma

THEMIS Image of the Day, August 19, 2016. Today’s image shows part of the southern margin of Juventae Chasma. Also visible are sand dunes located on the floor of the canyon. More THEMIS Images of the Day by geological topic.

Posted in Reports | Tagged , , , , , , , , , , , | Comments Off

THEMIS: Dark dune in Terra Sabaea crater

THEMIS Image of the Day, August 12, 2016. The large isolated dune in this VIS image is located on the floor of an unnamed crater in Terra Sabaea. Its dark tone suggests that the dune sand is largely dust-free, probably … Continue reading

Posted in Reports | Tagged , , , , , , , , , | Comments Off

Large aeolian ripples on Mars

Planetary Geomorphology Image of the Month, July 30, 2016: Ryan C. Ewing (Texas A&M University).  Ripples cover the surfaces of sand dunes on Earth and Mars. On Earth, ripples formed in typical aeolian sand (e.g., 0.1 and 0.3 mm) range … Continue reading

Posted in Reports | Tagged , , , , | Comments Off

HiRISE: North polar gypsum dunes

These sand dunes are a type of aeolian bedform and partly encircle the Martian North Pole in a region called Olympia Undae. Unlike most of the sand dunes on Mars that are made of the volcanic rock basalt, these are … Continue reading

Posted in Reports | Tagged , , , , , , , , , | Comments Off