| Piú votate - Mars Reconnaissance Orbiter (MRO) |
ESP_021551_1710_RED_abrowse-PCF-LXTT.jpgElorza Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)226 visitenessun commentoMareKromium
(2 voti)
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PSP_003249_1510_RED_abrowse-00.jpgMineral Diversity inside Ritchey Crater (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)302 visitenessun commentoMareKromium
(2 voti)
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PSP_003249_1510_RED_abrowse-01.jpgMineral Diversity inside Ritchey Crater (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)302 visitenessun commentoMareKromium
(2 voti)
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ESP_021705_1510_RED_abrowse-00-PCF-LXTT-0.jpgHydrated Minerals (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)434 visitenessun commentoMareKromium
(2 voti)
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ESP_021705_1510_RED_abrowse-01-PCF-LXTT-1.jpgHydrated Minerals (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)434 visitenessun commentoMareKromium
(2 voti)
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PSP_006724_2165_RED_abrowse-PCF-LXTT.jpgUnnamed Channel in Utopia Planitia (Absolute Natural Colors; credits for the additional process. and coloring: Dr Paolo C. Fienga - Lunexit Team)237 visiteSeen here are gullies in an Unnamed Northern Crater. The Crater is well-preserved as indicated by its sharp Rim and steep Walls.
Gullies are rarer in the Northern Hemisphere, possibly because there are fewer Slopes for them to form on compared to the heavily cratered Southern Highlands.
This image captures a wide range of Gully morphologies. The Gullies on the North Wall (such as the South-facing Wall) are more abundant and evenly-spaced than those on the East and South Walls and they extend up to the Crater Rim on the northern side. These differences might occur because of differences in sunlight exposure and temperature variations.
The Crater Floor has a linear texture suggestive of flow. Ice-rich material might have moved off the Crater Walls, driven by gravity, and flowed towards the Crater center.MareKromium
(2 voti)
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PSP_006959_2610_RED_abrowse-PCF-LXTT.jpgFrozen Dunes (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)167 visitenessun commentoMareKromium
(2 voti)
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PSP_003162_1445_RED_browse-00-PCF-LXTT.jpgUnnamed Southern Crater with deep Gullies and Fill (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)141 visitenessun commentoMareKromium
(2 voti)
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PSP_004311_1050_RED_abrowse-PCF-LXTT.jpgBasal Exposure of South Polar Layered Deposits - SPLD (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)133 visitenessun commentoMareKromium
(2 voti)
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PSP_006250_2200_RED_abrowse-PCF-LXTT-0.jpgFeatures of Nilosyrtis Region (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)145 visitenessun commentoMareKromium
(2 voti)
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PSP_006998_2060_RED_abrowse.jpgRecent Impact? (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)241 visitenessun commentoMareKromium
(2 voti)
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PSP_007006_1765_RED_abrowse-PCF-LXTT.jpgLayered Surface Features in Aureum Chaos (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)285 visitenessun commentoMareKromium
(2 voti)
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