| Ultimi arrivi - Mars from Orbit (from July 2009) |
North_Polar_Regions-North_Polar_Erg-PCF-LXTT.jpgNorthern Dunes (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visiteCaption NASA:"This region of North Polar Dunes has less dune materials than other portions of the North Polar Erg. This allows the base (assumption) that the dunes are moving across to be observed".MareKromiumSet 12, 2008
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Channels-Drainage_Channels-PCF-LXXT.JPGDraining Channels near Moreux Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)56 visitenessun commentoMareKromiumSet 08, 2008
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Channels-Clanis_Vallis-MO.JPGClanis Vallis (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromiumSet 05, 2008
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Volcanic_Features-Lava_Flows-Elysium_Mons-PCF-LXTT-20080325a.jpgLava Channels from Elysium Mons (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromiumSet 03, 2008
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Landslides-Melas_Chasma-20080204a-PCF-LXTT.jpgHuge Landslide in Melas Chasma (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visiteCaption NASA:"This landslide in Melas Chasma is so large that a single THEMIS VIS image can cover only a portion of the deposit.
This image clearly shows the sub-radial grooves typical of the surface of landslides on Mars".
MareKromiumAgo 28, 2008
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Landslides-Melas_Chasma-20071114a-PCF-LXTT.jpgLandslide in Melas Chasma (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromiumAgo 28, 2008
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Channels-Unnamed_Channel_in_Granicus_Vallis-20080430a~0.jpgGranicus Vallis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)71 visiteCaption NASA:"Granicus Vallis originates from fracture systems of the Elysium Volcanic Complex. This channel system was likely produced by volcanic flows".
MareKromiumAgo 25, 2008
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Channels-Unnamed_Channel-20071213a~0.jpgUnnamed Channel (Natural Colors/Tri-Chromatic Version; credits: Dr Paolo C. Fienga - Lunexit Team)60 visitenessun commentoMareKromiumAgo 25, 2008
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Channels-Unnamed_Channel_in_Auqakuh_Vallis.jpgUnnamed Channel in Auqakuh Vallis (Natural Colors/Tri-Chromatic Version; credits: Dr Paolo C. Fienga - Lunexit Team)61 visiteCaption NASA:"This VIS image shows a small portion of Auqakuh Vallis. Several tributaries enter the main channel in the center and upper portions of the image".MareKromiumAgo 25, 2008
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North_Polar_Features-The_Erg-PCF-LXTT-3.jpgNorth Polar Erg (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visiteCaption NASA:"A vast Region of sand dunes is located on the margin of the North Polar Cap of Mars. This 'sea' of sand is call "Polar Erg".
Coord.: 80,5° North Lat. and 183,5° East Long.
MareKromiumAgo 23, 2008
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Linear_Ridges-PCF-LXTT.jpgLinear Ridges (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)55 visitenessun commentoMareKromiumAgo 14, 2008
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Clouds-PCF-LXTT.jpgNorth Polar Clouds and Surface (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visiteCaption NASA:"When winds that have swept across the North Polar Ice encounter a trough in the ice, the laminar flow slows at the base of the trough, producing a turbulent wind regime that is easily recognized in the clouds formed in the trough".
MareKromiumLug 31, 2008
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