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SOL858-2P202552105EFFAS00P2669L4M1-01.jpgSunset over Gusev Crater - Sol 858 (by Dr Paolo C. Fienga - Lunar Explorer Italia)227 visitenessun commentoMareKromiumOtt 27, 2011
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Chaotic_Terrain-Margaritifer_Terra-PIA14970-PCF-LXTT.jpgChaotic Terrain in Margaritifer Terra (Slightly Saturated Absolute Natural Colors; credits for the additoonal process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visiteOrbit Number: 43456
Latitude: 18,596° South
Longitude: 333,761° East
Instrument: VIS
Captured: October, 1st, 2011
Mars Local Time (M.L.T.): 09:54 (Morning Hours)
MareKromiumOtt 27, 2011
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Craters-Unnamed_Secondary_Crater-Terra_Cimmeria-PIA14980-PCF-LXTT.jpgPossible Secondary Crater in Terra Cimmeria (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia) 193 visiteOrbit Number: 43050
Latitude: 21,179° South
Longitude: 163,038° East
Instrument: VIS
Captured: August, 28, 2011
MareKromiumOtt 27, 2011
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Channels-Drainage_Channels-PIA14971-PCF-LXTT.jpgDrainage Channels on the Rim of Bakhuysen Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)190 visiteOrbit Number: 43492
Latitude: 23,6637° South
Longitude: 14,8281° East
Instrument: VIS
Captured: October, 4th, 2011
Mars Local Time (M.L.T.): 09:02 (Morning Hours)
MareKromiumOtt 27, 2011
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PSP_006913_1765_RED_abrowse-PCF-LXTT-1.jpgPossible MSL Landing Site in Miyamoto Crater (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 201 visiteMiyamoto Crater is located in the South-Western portion of Meridiani Planum (and to the South-West of the Mars Exploration Rover Opportunity Landing Site). This image shows fairly smooth plains and some areas covered by Windstreaks, suggesting that wind is an active process here, depositing surface material downwind in the form of Streaks.
This possible Landing Site is adjacent to the hematite-bearing plains unit where the Opportunity Rover sits. The CRISM instrument has detected phyllosilicates (clay minerals) at this Site, which scientists believe to have formed in the presence of water. The MSL rover would investigate the mineral diversity here, which includes Phyllosilicates and Sulfates.MareKromiumOtt 26, 2011
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Volcanic_Regions-Rocky_Outcrops-MGS-01.jpgStreamlined Rocky Outcrops near Olympus Mons (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia) 243 visiteCaption NASA originale:"This MGS-MOC image shows wind-eroded "Streamlined" Rocky Outcrops overlying Lava Flow Surfaces located to the West of Olympus Mons. Outcrops with this appearance are also called Yardangs. Yardangs typically form in Sedimentary Rock or Volcanic Ash that contains some amount of Sand. The weathering of the Rock due to the Aeolian action cause the release of sand-sized particles from the Outcrops and, in time, such a form of erosion slowly shape the rock into the classic, inverted boat hull-like shapes of Yardangs".
Location near: 13,2° North Lat. and 160,1° West Long.
Image width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Northern SpringMareKromiumOtt 26, 2011
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Channels-Unnamed_Channel_in_Stygis_Catena-PIA07133-01.jpgAncient Riverbed in Stygis Catena (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)167 visiteCaption NASA originale:"This MGS-MOC image shows a Trough (Trough ---> canale) in the Stygis Catena Region, East of the Martian Volcano Elysium Mons. The Trough probably formed by collapse (Collapse ---> geol. "cedimento" del terreno). Large, dark Boulders can be seen on the Trough Floor in this Volcanic Region. The image is located near 24,4° North Lat. and 210,4° West Long. The image covers an area about 3 km (approx. 1,9 mi) wide and sunlight illuminates the scene from the lower left".MareKromiumOtt 26, 2011
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ESP_023777_1335_RED_abrowse.jpgUnnamed Southern Crater with Gullies (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)155 visiteMars Local Time: 14:23 (Early Afternoon)
Coord. (centered): 46,3° South Lat. and 18,9° East Long.
Spacecraft altitude: 252,8 Km (such as about 158,0 miles)
Original image scale range: 25,3 cm/pixel (with 1 x 1 binning) so objects ~ 76 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 3,0°
Phase Angle: 50,3°
Solar Incidence Angle: 52° (meaning that the Sun is about 38° above the Local Horizon)
Solar Longitude: 349,1° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumOtt 26, 2011
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ESP_023780_0935_RED_abrowse.jpgSouth Polar Residual Cap "Intraseasonal Change" Monitoring (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)143 visiteMars Local Time: 18:04 (Middle Afternoon)
Coord. (centered): 86,7° South Lat. and 355,4° East Long.
Spacecraft altitude: 245,4 Km (such as about 153,4 miles)
Original image scale range: 49,1 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 47 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 2,5°
Phase Angle: 84,2°
Solar Incidence Angle: 86° (meaning that the Sun is about 4° above the Local Horizon)
Solar Longitude: 349,3° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumOtt 26, 2011
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ESP_023779_0930_RED_abrowse.jpgSouth Polar Residual Cap "Intraseasonal Change" Monitoring (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)152 visiteMars Local Time: 17:36 (Middle Afternoon)
Coord. (centered): 86,8° South Lat. and 15,7° East Long.
Spacecraft altitude: 247,5 Km (such as about 154,7 miles)
Original image scale range: 49,5 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 49 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 1,4°
Phase Angle: 85,9°
Solar Incidence Angle: 85° (meaning that the Sun is about 5° above the Local Horizon)
Solar Longitude: 349,2° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumOtt 26, 2011
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ESP_023829_1350_RED_abrowse-PCF-LXTT-00.jpgLarge Southern Dunefield (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)180 visiteMars Local Time: 14:22 (Early Afternoon)
Coord. (centered): 44,9° South Lat. and 38,7° East Long.
Spacecraft altitude: 251,1 Km (such as about 157,0 miles)
Original image scale range: 50,2 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 51 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,3°
Phase Angle: 51,9°
Solar Incidence Angle: 52° (meaning that the Sun is about 38° above the Local Horizon)
Solar Longitude: 351,2° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumOtt 26, 2011
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ESP_023829_1350_RED_abrowse-PCF-LXTT-01.jpgLarge Southern Dunefield (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)183 visiteMars Local Time: 14:22 (Early Afternoon)
Coord. (centered): 44,9° South Lat. and 38,7° East Long.
Spacecraft altitude: 251,1 Km (such as about 157,0 miles)
Original image scale range: 50,2 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 51 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,3°
Phase Angle: 51,9°
Solar Incidence Angle: 52° (meaning that the Sun is about 38° above the Local Horizon)
Solar Longitude: 351,2° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumOtt 26, 2011
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