| Risultati della ricerca nelle immagini - "Layered" |
ESP_020086_2020_RED_abrowse-00.jpgUnnamed Crater with Light-toned Layered Bedrock (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)73 visitenessun commentoMareKromium
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ESP_020732_2000_RED_abrowse-PCF-LXTT-01.jpgLight-Toned Layered Rocks in Arabia and East Xanthe Regions (EDM n.1 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)126 visiteMars Local Time: 15:31 (Middle Afternoon)
Coord. (centered): 19,9° North Lat. and 342,5° East Long.
Spacecraft altitude: 284,8 Km (such as about 178,0 miles)
Original image scale range: 57,0 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 71,0 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 5,9°
Sun-Mars-Spacecraft (or "Phase") Angle: 66,2°
Solar Incidence Angle: 61° (meaning that the Sun is about 29° above the Local Horizon)
Solar Longitude: 207,0° (Northern Fall)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromium
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ESP_020732_2000_RED_abrowse-PCF-LXTT-02.jpgLight-Toned Layered Rocks in Arabia and East Xanthe Regions (EDM n.2 - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)127 visiteMars Local Time: 15:31 (Middle Afternoon)
Coord. (centered): 19,9° North Lat. and 342,5° East Long.
Spacecraft altitude: 284,8 Km (such as about 178,0 miles)
Original image scale range: 57,0 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 71,0 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 5,9°
Sun-Mars-Spacecraft (or "Phase") Angle: 66,2°
Solar Incidence Angle: 61° (meaning that the Sun is about 29° above the Local Horizon)
Solar Longitude: 207,0° (Northern Fall)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromium
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ESP_021947_1300_abrowse-PCF-LXTT-00.jpgLayered Landscape in Argyre Planitia (an Image-Mosaic in Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)262 visitenessun commentoMareKromium
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ESP_023803_1345_RED_abrowse.jpgClay-bearing Layered Deposit located within an Unnamed Crater, North of Proctor Crater (Absolute Natural Colors; credits for the additoonal process. and color.: Dr Paolo C. Fienga - Lunexit Team)206 visiteMars Local Time: 14:19 (Early Afternoon)
Coord. (centered): 45,4° South Lat. and 28,0° East Long.
Spacecraft altitude: 253,0 Km (such as about 158,1 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: 6,5°
Sun-Mars-Spacecraft (or "Phase") Angle: 55,9°
Solar Incidence Angle: 51° (meaning that the Sun is about 39° above the Local Horizon)
Solar Longitude: 350,2° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromium
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ESP_023827_1835_RED_abrowse.jpgLayered Cliffs in Libya Montes (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)176 visiteMars Local Time: 14:07 (Early Afternoon)
Coord. (centered): 3,4° North Lat. and 85,9° East Long.
Spacecraft altitude: 277,1 Km (such as about 173,2 miles)
Original image scale range: 55,4 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 66 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 11,8°
Sun-Mars-Spacecraft (or "Phase") Angle: 44,5°
Solar Incidence Angle: 33° (meaning that the Sun is about 57° above the Local Horizon)
Solar Longitude: 351,1° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer ItaliaMareKromium
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ESP_024553_1500-PCF-LXTT-003.jpgSouthern Layered Features (Absolute Natural Colors; credits for the additonal process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)242 visiteMars Local Time: 14:38 (early afternoon)
Coord. (centered): 29,9° South Lat. and 71,8° East Long.
Spacecraft altitude: 263,1 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: 7,7°
Phase Angle: 48,6°
Solar Incidence Angle: 54° (meaning that the Sun is about 36° above the Local Horizon)
Solar Longitude: 19,0° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromium
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ESP_024886_1765_RED-PCF-LXTT-00.jpgPeri-Equatorial Layered Features (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)217 visiteCoord. (centered): 3,5° South Lat. and 335,5° East Long.MareKromium
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ESP_024886_1765_RED-PCF-LXTT-01.jpgPeri-Equatorial Layered Features (EDM - Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)223 visiteCoord. (centered): 3,5° South Lat. and 335,5° East Long.MareKromium
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Juventae_Chasma-PIA12489.jpgBright Layered Deposits near Juventae Chasma (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)54 visiteThis view shows color variations in bright Layered Deposits on a plateau near Juventae Chasma in the Valles Marineris egion of Mars. A brown mantle covers portions of the bright deposits. The view covers an area about of 1,2 Km (three-fourths of a mile) across.
The image comes from an observation made by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter on May 2, 2007.
Researchers have found that these bright Layered Deposits contain Opaline Silica and Iron Sulfates, consistent with low-temperature, acidic aqueous alteration of basaltic materials. They conclude that aqueous activity affected this plateau after formation of the nearby canyons. Although the source of water and sediment remains uncertain, the strong correlation between fluvial landforms and bright Layered Deposits in this Region argues for sustained precipitation, surface runoff, and fluvial deposition occurring during Mars' Hesperian Era on the plateaus adjacent to Valles Marineris and along portions of the canyon walls.
This image is one product from HiRISE observation PSP_003579_1755, centered at 4,7° South Lat. and 296,4 East Long.MareKromium
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Juventae_Chasma-PIA13278.jpgLayered Hill in Juventae Chasma (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)55 visitenessun commentoMareKromium
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Layers-PIA15561-PCF-LXTT.jpgPossible Layered Fill on the Floor of an Unnamed Crater (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)119 visiteOrbit Number: 45215
Latitude: 2,442° North
Longitude: 343,953° East
Instrument: VIS
Captured: February, 23rd, 2012
Mars Local Solar Time: 06:02 (Early Morning Hours)MareKromium
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