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OPP-SOL341-1.jpg
OPP-SOL341-1.jpgCorrugated Iron and "Sponge-like" Material, such as...Space Trash! - Sol 341 (Superdefinition; credits: Dr G. Barca)57 visitenessun commentoMareKromium
PSP_008426_2595_RED_abrowse-00.jpg
PSP_008426_2595_RED_abrowse-00.jpgPolygons, Crater Layers, and Defrosting Dunes (ctx frame - MULTISPECTRUM-2; credits: Lunexit)57 visiteThe North Polar Region is surrounded by a large sea (erg) of dark sand dunes that become covered by seasonal CO2.
As the Northern Hemisphere begins to warm in the Spring, the frozen CO2 sublimates.

The wind blows from an East-Northeasterly direction and leaves dark streaks behind (exposed basalt) from the evaporating Carbon Dioxide. This image displays defrosting sand dunes in an unnamed crater.
MareKromium
OPP-SOL162-1P142569702RAD3221P2387L257C1.jpg
OPP-SOL162-1P142569702RAD3221P2387L257C1.jpgMonochrome Mars - Sol 162 (Multispectral Color Imagery; credits: Lyle.org)57 visitenessun commentoMareKromium
PHOE-SOL031-md_7790-1.jpg
PHOE-SOL031-md_7790-1.jpgHollows, Pebbles and other "Things" near Phoenix - Sol 31 (ctx frame; natural but enhanced colors; credits: Dr M. Faccin)57 visitenessun commentoMareKromium
SOL14126-El_Dorado_streaks.gif
SOL14126-El_Dorado_streaks.gifThe "Darkening" of El Dorado - Sol 1042/1081 (GIF-Movie; credits:Lyle.org)57 visitenessun commentoMareKromium
PSP_008191_2645_RED_abrowse.jpg
PSP_008191_2645_RED_abrowse.jpgNorth Polar Scarp (MULTISPECTRUM; credits: Lunexit)57 visitenessun commentoMareKromium
PHOE-SOL035-lg8635-8642-8643.jpg
PHOE-SOL035-lg8635-8642-8643.jpgCircuits - Sol 35 (natural colors; credits: Dr G. Barca)57 visitenessun commentoMareKromium
PSP_006567_2220_RED_abrowse-00.jpg
PSP_006567_2220_RED_abrowse-00.jpgFlooded Terrain in Terra Sabaea (MULTISPECTRUM; credits: Lunexit)57 visiteTwo distinctly different terrain types are visible in this image of the Northern Lowlands of Mars: an older, heavily cratered landscape has been inundated by much younger flows.
The valley floors are filled with flows that have relatively smooth surfaces and very few superposed impact craters.

In contrast, the mesas and hills making up the older terrain have blocky surfaces, perhaps fragmented by ancient impacts.
MareKromium
PSP_007055_2015_RED_abrowse-2.jpg
PSP_007055_2015_RED_abrowse-2.jpgVolcanic and Clay Materials near Nili Fossae (edm n. 2)57 visitenessun commentoMareKromium
PSP_007055_2015_RED_abrowse-1.jpg
PSP_007055_2015_RED_abrowse-1.jpgVolcanic and Clay Materials near Nili Fossae (edm n. 1)57 visitenessun commentoMareKromium
PHOE-SOL038-2.jpg
PHOE-SOL038-2.jpgPossible "Audio Signals" from Vastitas Borealis - Sol 38 (credits: Dr M. Faccin)57 visitenessun commento2 commentiMareKromium
PHOE-SOL037-lg9455-9466-9467.jpg
PHOE-SOL037-lg9455-9466-9467.jpgVastitas' Foreshortening - Sol 37 (Superdefinition + MULTISPECTRUM; credits: Dr G. Barca & Lunexit)57 visitenessun commentoMareKromium
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