| Ultimi arrivi - Mars Reconnaissance Orbiter (MRO) |
ESP_023531_1840-00.jpgSkylight on the Dusty Slopes of Arsia Mons (CTX Frame and EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)223 visiteMars Local Time: 14:08 (Early Afternoon)
Coord. (centered): 3,7° North Lat. and 248,5° East Long.
Spacecraft altitude: 263 Km (such as about 164,4 miles)
Original image scale range: 26,3 cm/pixel (with 1 x 1 binning) so objects ~ 79 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 4,1°
Sun-Mars-Spacecraft (or "Phase") Angle: 30,4°
Solar Incidence Angle: 34° (meaning that the Sun is about 56° above the Local Horizon)
Solar Longitude: 339,1° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumAgo 19, 2011
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Syrtis_Major_Planum-ESP_023089_1960_RED_abrowse-PCF-LXTT.jpgFeatures of Syrtis Major Planum (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)237 visiteMars Local Time: 14:06 (Early Afternoon)
Coord. (centered): 15,7° North Lat. and 74,2° East Long.
Spacecraft altitude: 277,8 Km (such as about 173,6 miles)
Original image scale range: 27,8 cm/pixel (with 1 x 1 binning) so objects ~ 55,6 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 6,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 39,7°
Solar Incidence Angle: 44° (meaning that the Sun is about 46° above the Local Horizon)
Solar Longitude: 320,1° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumAgo 18, 2011
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Craters-Iazu_Crater-ESP_023092_1775_RED_abrowse-PCF-LXTT.jpgThe Eastern half of Iazu Crater - Meridiani Planum (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)199 visiteMars Local Time: 14:11 (Early Afternoon)
Coord. (centered): 2,7° South Lat. and 354,9° East Long.
Spacecraft altitude: 272,8 Km (such as about 170,5 miles)
Original image scale range: 27,3 cm/pixel (with 1 x 1 binning) so objects ~ 82 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 10,6°
Sun-Mars-Spacecraft (or "Phase") Angle: 25°
Solar Incidence Angle: 35° (meaning that the Sun is about 55° above the Local Horizon)
Solar Longitude: 320,2° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumAgo 17, 2011
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ESP_021527_1960_RED_abrowse-01-PCF-LXTT.jpgFeatures of Tharsis (EDM - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)191 visitenessun commentoMareKromiumAgo 15, 2011
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ESP_021527_1960_RED_abrowse-00-PCF-LXTT.jpgFeatures of Tharsis (CTX Frame - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)177 visiteMars Local Time: 15:06 (Early Afternoon)
Coord. (centered): 15,8° North Lat. and 238,2° East Long.
Spacecraft altitude: 275,1 Km (such as about 171,9 miles)
Original image scale range: 55 cm/pixel (with 2 x 2 binning) so objects ~1 mt and 65 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 6,2°
Sun-Mars-Spacecraft (or "Phase") Angle: 65,2°
Solar Incidence Angle: 60° (meaning that the Sun is about 30° above the Local Horizon)
Solar Longitude: 245,6° (Northern Fall)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumAgo 15, 2011
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ESP_021464_1900_RED_abrowse-PCF-LXTT-00.jpgFissure in Cerberus Fossae (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)179 visiteMars Local Time: 15:05 (Early Afternoon)
Coord. (centered): 10,1° North Lat. and 157,6° East Long.
Spacecraft altitude: 295,6 Km (such as about 184,7 miles)
Original image scale range: 29,6 cm/pixel (with 1 x 1 binning) so objects ~89 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 21,2°
Sun-Mars-Spacecraft (or "Phase") Angle: 74,9°
Solar Incidence Angle: 56° (meaning that the Sun is about 34° above the Local Horizon)
Solar Longitude: 242,5° (Northern Fall)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumAgo 15, 2011
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ESP_021464_1900_RED_abrowse-PCF-LXTT-01.jpgFissure in Cerberus Fossae (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)195 visitenessun commentoMareKromiumAgo 15, 2011
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ESP_023164_1020_RED_abrowse-PCF-LXTT-01.jpgFeatures of the SPLD (EDM - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)179 visitenessun commentoMareKromiumAgo 15, 2011
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ESP_023164_1020_RED_abrowse-PCF-LXTT-00.jpgFeatures of the SPLD (CTX Frame - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)196 visiteMars Local Time: 14:46 (Early Afternoon)
Coord. (centered): 77,9° South Lat. and 203,8° East Long.
Spacecraft altitude: 250,1 Km (such as about 156,3 miles)
Original image scale range: 50 cm/pixel (with 2 x 2 binning) so objects ~1 mt and 50 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 7,5°
Sun-Mars-Spacecraft (or "Phase") Angle: 70,8°
Solar Incidence Angle: 66° (meaning that the Sun is about 24° above the Local Horizon)
Solar Longitude: 323,4° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumAgo 15, 2011
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PSP_005160_1150_RED_abrowse-PCF-LXTT-01.jpgGullies in Mantle Terrain in Sisyphi Planum (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 226 visiteCaption NASA:"This EDM shows the Boundary between one of the Alcoves and the surrounding Mantled Terrain. Numerous Fissures arranged forming Polygons some 3 to 10 meters (3,3 to 11 yards) across are visible in the image. These are similar to features found in Terrestrial Periglacial Regions such as Antarctica, where ice is present at or near the Surface. Antarctica's Polygons form by repeated expansion and contraction of the soil-ice mixture due to seasonal temperature oscillations; this results in Polygonal Networks of Stress Fractures".MareKromiumAgo 12, 2011
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PSP_005160_1150_RED_abrowse-PCF-LXTT-00.jpgGullies in Mantle Terrain in Sisyphi Planum (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 215 visiteCaption NASA:"This observation shows the East-facing Walls of an Unnamed Crater in Sisyphi Planum, near the South Polar Regions. Gullies, as well as Mantle Terrain and Polygons are also visible; these features suggest that at some point in time, liquid and ice may have been present at and near the Surface. The Gullies, which are rather eroded, have ample Alcoves and subdued Channels; dark patches and Ripples in the bottom of the Channels indicate that the most recent activity was Aeolian (such as "wind-driven") in Nature. Mantle Terrains are characterized by their smooth Surface and light, uniform color. They are widely interpreted as Terrains blanketed by a mixture of Ice and Dust, deposited under climatic conditions different from that of today. The Gullies in this image have Alcove Areas that seem to have cut through the Mantle Terrain, exposing the underlying materials". MareKromiumAgo 12, 2011
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ESP_023077_1225_RED_abrowse-PCF-LXTT.jpgFeatures of Peneus Patera (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)194 visitenessun commentoMareKromiumAgo 09, 2011
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