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Chaotic_Terrain-Iani_Chaos-20050505a-PCF-LXTT.jpgFeatures of Iani Chaos (Enhanced and Saturated Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 171 visitenessun commentoMareKromiumOtt 06, 2011
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Dunes-Dark_Dunes-Chasma_Boreale-PIA07350-01.jpgDark Dunes in Chasma Boreale (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)147 visiteCaption NASA originale:" This MGS-MOC image shows Dark Sand Dunes overlying an eroded, layered substrate in Chasma Boreale, amid the materials of the Martian North Polar Cap".
Location near: 84,5° North Lat. and 358,3° West Long.
Image width: ~3 Km (~1,9 mi)
Season: Northern SummerMareKromiumOtt 06, 2011
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Craters-Unnamed_Defrosting_Crater-PIA03921-01.jpgUnnamed Defrosting Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)231 visiteCaption NASA originale:"This MGS-MOC image shows a Surface in the South Polar Region, covered by CO2 Frost. In this springtime scene, the Frost has begun to sublime so that Sandy Surfaces exhibit an abundance of Dark Spots. The circular depression is probably the remains of an Impact Crater. In summer, the Spotted Surfaces in this image would be darker than their surroundings, because they are patches of Windblown Sand".
Location near: 67,6° South Lat. and 254,3° West Long.
Image width: ~3 Km (~1,9) mi
Illumination from: upper left
Season: Southern SpringMareKromiumOtt 05, 2011
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Craters-Unnamed_Crater_with_Windstreak-PIA07508-01.jpgUnnamed Crater wth Windstreak (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)234 visiteCaption NASA originale:"This MGS-MOC image shows a 1,2 Km North Mid-Latitude Unnamed Crater with a bright Windstreak".
Location near: 30,8° North Lat. and 131,8° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Northern Summer
MareKromiumOtt 05, 2011
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Craters-Newton_Crater-PCF-LXTT-04.jpgNewton Crater's Gullies (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)258 visitenessun commentoMareKromiumOtt 05, 2011
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Dunes-Noachis_Terra-01.jpgDark Dunes in Noachis Terra (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)159 visiteCaption originale:"This MGS-MOC image shows Dark Sand Dunes and relatively small, light-toned, windblown Ripples on the Floor of an Unnamed Crater located in central Noachis Terra".
Location near: 50,0° South Lat. and 353,7° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: upper left
Season: Southern AutumnMareKromiumOtt 05, 2011
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Craters-Unnamed_Crater_in_Terra_Cimmeria-MGS-PCF-LXTT.jpgUnnamed Impact Crater wth Gullies (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)207 visiteCaption NASA originale:"This MGS-MOC image shows a 1,5 mt (~5 feet) per pixel view of an Unnamed Crater in the Terra Cimmeria Region of Mars. Several Gullies extend from near the top of the Crater Rim, downslope toward the Floor of the Crater. Liquid water might have played a role in their genesis".
Location near: 37,7° South Lat. and 191,6° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: upper left
Season: Southern SummerMareKromiumOtt 05, 2011
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Craters-Unnamed_Crater_in_Terra_Tyrrhena-MGS-04.jpgUnnamed Crater and Dunes in Terra Tyrrhena (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team142 visitenessun commentoMareKromiumOtt 05, 2011
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Craters-Unnamed_Crater_in_Terra_Tyrrhena-02.jpgUnnamed Crater and Dunes in Terra Tyrrhena (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)132 visiteCaption originale:"This MGS-MOC image shows a portion of a Field of Dark Sand Dunes superposed on the light-toned Floor of an Unnamed Crater in Eastern Tyrrhena Terra. The orientation of the Dunes — with the steep faces toward the South — suggests that winds generally blew from North to South at the time the Dunes were formed".
Location near: 14,6° South Lat. and 262,3° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Southern SummerMareKromiumOtt 05, 2011
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Craters-Crater_Cluster-Meridiani_Planum-PIA07151_modest-01.jpgCrater Cluster in Meridiani Planum (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)127 visitenessun commentoMareKromiumOtt 05, 2011
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Volcanoes-Ascraeus_Mons-PIA07149-PCF-LXTT-1.jpgAscraeus Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)265 visiteCaption NASA originale:"This red wide angle Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows Ascraeus Mons, the northernmost of the three Tharsis Montes shield volcanoes. Ascraeus Mons is about 460 Km (~286 mi) across and its summit is at an elevation of about 18 km (11 mi) above the "Martian Datum" (or Mars' Ground Zero, such as the elevation designated as 0 km). The center of the Summit Caldera is near 11° North Lat. and 104° West Long.". MareKromiumOtt 04, 2011
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Craters-Unnamed_Crater-PIA06699-PCF-LXTT.jpgDark Slope Streaks (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)122 visiteCaption NASA:"Dark Slope Streaks are a common feature on the Slopes thickly-mantled by Dust in the Tharsis, Arabia, and Western Amazonis Planitia egions of Mars. Less common are light-toned Slope Streaks, which often occur in the same area as Dark Streaks. They are most common in Arabia Terra, and some are shown in this MGS image. Slope Streaks are probably the result of sudden Avalanches of extremely dry Dust. The behavior of the avalanching dust is somewhat fluid-like and it is a phenomenon often observed during the Martian year.
MareKromiumOtt 04, 2011
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