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Risultati della ricerca nelle immagini - ""V""
PSP_003193_0850_RED_browse_00.jpg
PSP_003193_0850_RED_browse_00.jpgMartian Spring: the "V" Fans (context image)57 visiteSouthern Spring sunshine is causing the seasonal Carbon Dioxide (CO2) Cap at the South Pole to evaporate.
This process happens fitfully, as small and large spots expose bare ground, which warms up, causing small spots to grow.
The defrosting areas are controlled by small scale differences in topography, which cause some areas of frost to be sheltered longer than others.
Once dust has accessed the surface it is blown in directions controlled by the local winds, making a distinctive fan. When the wind changes direction the fans broaden or may show multiple orientations.
It has also been proposed that dust is carried to the top of translucent seasonal carbon dioxide ice by release of gas held under pressure by the ice cap. When the pressure is released, like pulling the cork out of a champagne bottle, the gas escapes, carrying dust with it.
MareKromium
PSP_003193_0850_RED_browse_01.jpg
PSP_003193_0850_RED_browse_01.jpgMartian Spring: the "V" Fans (extra-detail mgnf)69 visitenessun commentoMareKromium
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as15-93-12704.JPGAS 15-93-12704 - The "Herschel" Legacy57 visiteImage Collection: 70mm Hasselblad
Mission: 15
Magazine: 93
Magazine Letter: P
Latitude: 38,0° North
Longitude: 33,0° West
Film Type: SO-368
Film Width: 70 mm
Film Color: color
Feature(s): HERSCHEL "C", HERSCHEL "U" and HERSCHEL "V"
MareKromium
 
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