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South_Polar_Features-PIA13991-PCF-LXTT.jpgSouth Polar "Trough Clouds" (Enhanced Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)197 visiteCaption NASA:"Polar Surface Winds can reach high velocities. These Winds can cause Clouds to form when they flow into Troughs and become chaotic. This VIS image shows Trough Clouds as linear bands".
Orbit Number: 40916
Latitude: 86,459° South
Longitude: 100,949° East
Instrument: VIS
Captured: March, 6th, 2011
Mars Local Time (M.L.T.): 07:28 (Early Morning Hours)
MareKromium
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OPP-SOL2597-1P358738714EFFB900P2420R2M1-PCF-LXTT.jpgThe Sandy Waves of Meridiani Planum - Sol 2597 (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visitenessun commentoMareKromium
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ESP_021591_1640_RED_abrowse-PCF-LXTT.jpgChaotic Terrain (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visitenessun commentoMareKromium
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ZZ-Mercury-Global_View_of_the_Surface-PIA14081-PCF-LXTT.jpgNorth Polar Highly Cratered Terrain (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visiteDate Acquired: March 29, 2011
Image Mission Elapsed Time (MET): 209895911
Image ID: 65416
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filer: 7 (748 nanometers wavelength)
Center Latitude: 81,2° North
Center Longitude: 72,3° East
Resolution: 166 mt/pixel (0,10 miles/pixel)
Scale: the bottom of this image is about 84 Km (approx. 52 miles) acrossMareKromium
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ZZ-Mercury-Terminator-PIA14195-PCF-LXTT.jpgMercurian Terminator (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visiteDate acquired: March 31, 2011
Image Mission Elapsed Time (MET): 210035203
Image ID: 71446
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
WAC filter: 7 (748 nanometers)
Center Latitude: 83,17° South
Center Longitude: 250,9° East
Resolution: 1833 mt/pixel
Scale: the center of this image is about 1970 Km (approx. 1225 miles) acrossMareKromium
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PSP_008774_1755_RED_abrowse-PCF-LXTT.jpgLayers and more Inverted Topography (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visitenessun commentoMareKromium
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ESP_022637_2090_RED_abrowse.jpgFlow Features between Tartarus Montes and Phlegra Dorsa (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)197 visitenessun commentoMareKromium
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SOL544-2N174667255EFFACEHP0775R0M1-PCF-LXTT.jpgTAU Monitoring during a Sunny Day in Gusev Crater - Sol 544 (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)197 visitenessun commentoMareKromium
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ESP_023234_1460_RED_abrowse-PCF-LXTT-01.jpgThe "Colourful" Floor of Hellas Planitia (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)197 visitenessun commentoMareKromium
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PSP_003617_1835_RED_abrowse-PCF-LXTT-01.jpgFeatures of Aram Chaos (EDM n.1 - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)197 visiteCaption NASA:"This image captures an enigmatic approximately 6 Km-wide area in central Aram Chaos, a Region that is about 1000 Km in diameter and it is located East of Valles Marineris and just North of the Equator. The image depicts the edge of a light-toned cap unit forming two large sheets in the middle of this Chaotic Terrain. This cap unit is heavily eroded forming the 'icing' texture and terminates with a sharp approximately 300 mt Cliff going diagonally across the area". MareKromium
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OPP-SOL2676-PIA14506-PCF-LXTT.jpgApproaching "Spirit Point" - Sol 2676 (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)197 visiteCaption NASA:"NASA's Mars Exploration Rover Opportunity used its PanCam to capture this view of a portion of Endeavour Crater's Rim after a drive during the Rover's 2676th Martian Day, or Sol, of working on Mars (such as August, 4th, 2011). The drive covered 396 feet (120,7 meters) and put the Rover with about that much distance to go before reaching the chosen Arrival Site at the Rim, called "Spirit Point".
Endeavour Crater has been the Rover Team's destination for Opportunity since the Rover finished exploring Victoria Crater in August 2008. Endeavour, with a diameter of about 14 miles (approx. 22 Km), offers access to older geological deposits than any Opportunity has seen before". This view looks toward a portion of the Rim, South of Spirit Point, including Terrain that Opportunity may explore in the future".MareKromium
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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)197 visitenessun commentoMareKromium
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