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Piú votate - Mars from Orbit (from July 2009)
Sirenum_Fossae-20090624a.jpg
Sirenum_Fossae-20090624a.jpgFissure in the Eastern End of Sirenum Fossae (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)57 visitenessun commentoMareKromium55555
(3 voti)
South_Polar_Features-Swiss_Cheese_Terrain-20090610a-PCF-LXTT.jpg
South_Polar_Features-Swiss_Cheese_Terrain-20090610a-PCF-LXTT.jpgSouth Polar "Swiss-Cheese Surface Features" (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)58 visiteCaption NASA:"As Spring turns to Summer, the frost cover has been removed from the South Polar Cap. The surface textures seen in this VIS image are created by action of the Sun on the icy cap".

Coord.: 86,9° South Lat. and 354,6° East Long.
MareKromium55555
(3 voti)
Clouds-Soth_Polar_Regions-20090417a-PCF-LXTT-1.jpg
Clouds-Soth_Polar_Regions-20090417a-PCF-LXTT-1.jpgSouthern Storm (1 - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)70 visiteCaption NASA:"Right now, most of the Southern Hemisphere of Mars is covered by Dust Storms, blocking our view of the Surface. Bright cloud tops dominate these two VIS images".MareKromium55555
(3 voti)
South_Polar_Features-Inca_City-MO-20090414a.jpg
South_Polar_Features-Inca_City-MO-20090414a.jpgAngustus Labyrintus - a.k.a.: Inca City (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)58 visiteCaption NASA:"This VIS image shows a portion of Angustus Labyrinthus, a Region of Intersecting Linear Ridges near the South Pole of Mars".

Coord.: 81,7° South Lat. and 296,8° East Long.
3 commentiMareKromium55555
(3 voti)
South_Polar_Features-Swiss_Cheese_Terrain-20090401a-PCF-LXTT.jpg
South_Polar_Features-Swiss_Cheese_Terrain-20090401a-PCF-LXTT.jpgSwiss-cheese Terrain (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)57 visiteCoord.: 87,1° South Lat. 355,7° East Long.MareKromium55555
(3 voti)
Dunes-Thaumasia_Region-20090320a-2.jpg
Dunes-Thaumasia_Region-20090320a-2.jpgThe Bright Dunes of Thaumasia (Natural Colors; credits: Lunar Explorer Italia)58 visiteCaption NASA:"Small, bright Dunes are numerous in the Channels of Southern Thaumasia Planum".

Coord.: 29,0° South Lat. and 290,6° East Long.
MareKromium55555
(3 voti)
Channels-Unnamed_Channel-20090316a.jpg
Channels-Unnamed_Channel-20090316a.jpgUnnamed Channel (Natural Colors/Tri-Chromatic Version; credits: Dr Paolo C. Fienga - Lunexit Team)57 visiteCoord.: 38,8° South Lat. and 199,8° East Long.MareKromium55555
(3 voti)
Aeolian_Features-Yardangs-Eolis_Planum-PCF-LXTT.jpg
Aeolian_Features-Yardangs-Eolis_Planum-PCF-LXTT.jpgFeatures of Eolis Planum (Saturated Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)57 visitenessun commentoMareKromium55555
(3 voti)
South_Polar_Feartures-Layers-20090223a-PCF-LXTT.jpg
South_Polar_Feartures-Layers-20090223a-PCF-LXTT.jpgSouth Polar Spring (Darkened Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)58 visiteCoord. 84,4° South Lat. and 313,9° East Long.1 commentiMareKromium55555
(3 voti)
Vastitas_Borealis-NP-MO-20090219a.jpg
Vastitas_Borealis-NP-MO-20090219a.jpgVastitas' Texture (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Finega - Lunar Explorer Italia)58 visiteCaption NASA:"The Northern Plains of Mars contain an abundance of different textures and appearances. This Region contains mounds separated by channels with an unusual floor pattern. Just how this texture formed is unknown".

Coord.: 70,0° North Lat. and 55,9° East Long.
MareKromium55555
(3 voti)
Aeolian_Features-Inverted_Channels-ER-MO.jpg
Aeolian_Features-Inverted_Channels-ER-MO.jpgInverted Topography (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visiteCaption NASA:"The system of sinuous ridges seen at the top of the image is the remnants of a channel system. In this case the channel has been filled by a material more resistant to erosion than the surroundings.
As the surround material was eroded away the resistant channel fill was left behind, forming a ridge where the channel had once been. This reversal of topography - from a channel to a ridge - is termed Inversion or Inverted Topography".
MareKromium55555
(3 voti)
Channels-Unnamed_Channel_in_Tempe_Fossae-MO.jpg
Channels-Unnamed_Channel_in_Tempe_Fossae-MO.jpgUnnamed Channel in Tempe Fossae (Natural Colors/Tri-Chromatic Version; credits: Dr Paolo C. Fienga - Lunexit Team)59 visiteCaption NASA:"The Channel in this VIS image is in the Tempe Fossae Region, just West of Sytinskaya Crater".MareKromium55555
(3 voti)
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