| Ultimi arrivi - A Tribute To Mars Global Surveyor |
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)127 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)124 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)260 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)118 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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Phlegra_Montes-PIA08743-1-PCF-LXTT.jpgFeatures of Phlegra Montes (2 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)191 visiteImage information: VIS instrument;
Latitude: 45,6° North;
Longitude: 168,7° East;
Resolution: 19 meter/pixel.MareKromiumOtt 04, 2011
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Phlegra_Montes-PIA08743-2-PCF-LXTT.jpgFeatures of Phlegra Montes (1 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)194 visiteImage information: VIS instrument;
Latitude: 45,6° North;
Longitude: 168,7° East;
Resolution: 19 meter/pixel.MareKromiumOtt 04, 2011
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Chaotic_Terrain-Eos_Chaos-01.jpgFeatures of Eos Chaos: Circular Butte (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)223 visiteLocation near: 12,9° South Lat. and 49,5° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Southern SummerMareKromiumOtt 01, 2011
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Chaotic_Terrain-Eos_Chaos-04.jpgFeatures of Eos Chaos: High Slope (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)208 visiteLocation near: 12,9° South Lat. and 49,5° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Southern SummerMareKromiumOtt 01, 2011
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Craters-Kunowsky_Crater-2004_06-PCF-LXTT.jpgFrost and Wavy Clouds on Kunowsky Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)204 visiteCaption NASA originale:"This red wide angle MGS-MOC image, acquired in March 2004, shows Kunowsky Crater ringed by seasonal Frost. Kunowsky Crater is about 67 Km (~42 mi) in diameter. Wavy Clouds form to the East of the Crater in early Spring as winds circulate from West to East. The Crater is located at about 57,1° North Lat. and 9,7° West Long.". MareKromiumSet 30, 2011
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Craters-Benedictus_XVI_Crater-PIA07838-PCF-LXTT.jpgImpact Crater with Frost Deposits (Benedictus XVI Crater - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 193 visiteLocation near: 37,5° South Lat. and 222,1° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: upper left
Season: Southern WinterMareKromiumSet 30, 2011
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Craters-Unnamed_Impact_Crater-PIA07836-PCF-LXTT.jpgUnnamed Impact Crater wth "Black Rim" in Vastitas Borealis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)216 visiteCaption NASA originale:"This MGS-MOC image shows a nearly-filled (and very old) impact crater on the Northern Plains".
Location near: 47,3° North Lat. and 294,0° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Northern Summer MareKromiumSet 30, 2011
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North_Polar_Features-Dunes-Dark_Dunes-PCF-LXTT.jpgDark Dunes in Vastitas Borealis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)181 visiteCaption NASA originale:"This MGS-MOC image shows dark North Polar Dunes overlying other materials in the North Polar Region".
Location near: 79,1° North Lat. and 228,8° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Northern SummerMareKromiumSet 30, 2011
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