| Risultati della ricerca nelle immagini - "Coprates" |
Chasmas-Coprates_Chasma-PIA17224-PCF-LXTT-IPF.jpgFeatures of Coprates Chasma (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)66 visiteIn this VIS image, taken by the NASA - Mars Odyssey Orbiter on March, 11, 2013 and during its 49.862nd orbit around the Red Planet, we can see that a large Landslide Deposit fills a portion of the Floor of Coprates Chasma: a huge and extremely long Canyon located the Coprates Quadrangle of Mars, at 13,4° South Latitude and 61,4° West Longitude. Coprates Chasma (---> the Abyss of Coprates) is part of the enormous Valles Marineris Canyon System and its length is of approx. 966 Km (such as about 599,88 miles).
Latitude (centered): 12,850° South
Longitude (centered): 293,254° East
Instrument: VIS
This frame (which is an Original Mars Odyssey Orbiter b/w frame published on the NASA - Planetary Photojournal with the ID n. PIA 17224) has been additionally processed, magnified, contrast enhanced and then colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - Mars Odyssey Orbiter and then looked down, towards the Surface of Mars), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team.MareKromium
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Coprates_Catena-PIA14518-PCF-LXTT.jpgFeatures of Coprates Catena (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)200 visitenessun commentoMareKromium
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Coprates_Catena-h0438_0000_nd3-00.jpgSulphates in Coprates Catena? (CTX Frame - Natural Colors; credits for the Additional Process. and Color.: Dr Paolo C. Fienga - Lunexit Team)76 visitenessun commentoMareKromium
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Coprates_Catena-h0438_0000_nd3-01.jpgSulphates in Coprates Catena? (EDM - Natural Colors; credits for the Additional Process. and Color.: Dr Paolo C. Fienga - Lunexit Team)93 visitenessun commentoMareKromium
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Coprates_Chasma-20071130a-PCF-LXTT.jpgHuge Landslied in Coprates Chasma (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Elisabetta Bonora and Paolo C. Fienga - Lunexit Team)54 visitenessun commentoMareKromium
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Coprates_Chasma-Chaotic_Terrain-MO-PCF-LXTT.jpgChaotic Terrain in Coprates Chasma (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)79 visitenessun commentoMareKromium
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Coprates_Chasma-PIA02173-00.jpgFeatures of Coprates Chasma (Original NASA/2001 Mars Odyssey Orbiter b/w Frame) 53 visiteImage information: VIS instrument;
Latitude: - 14,8° North;
Longitude: 304,3° East;
Resolution: 17 meter/pixel.
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Coprates_Chasma-PIA02173-01.jpgFeatures of Coprates Chasma (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 170 visiteImage information: VIS instrument;
Latitude: 14,8° South;
Longitude: 304,3° East;
Resolution: 17 meter/pixel.MareKromium
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Coprates_Chasma-PIA13786-PCF-LXTT.jpgFeatures of Coprates Chasma (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)58 visitenessun commentoMareKromium
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Coprates_Chasma-PIA17517-PCF-LXTT-IPF.jpgFeatures of Coprates Chasma (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)56 visiteIn this VIS image, taken by the NASA - Mars Odyssey Orbiter on August 12th, 2013, and during its 51.735th orbit around the Red Planet, we can see part of the Floor of Coprates Chasma, including a large Sand Sheet and a few smaller Dunes.
Latitude (centered): 13,967° South
Longitude (centered): 296,942° East
Instrument: VIS
This frame (taken from an Original Mars Odyssey Orbiter b/w and Map-Projected frame published on the NASA - Planetary Photojournal with the ID n. PIA 17517) has been additionally processed, magnified, contrast enhanced, Gamma corrected and then colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - Mars Odyssey Orbiter and then looked down, towards the Surface of Mars), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team.MareKromium
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Coprates_Labes-PIA16271-PCF-LXTT-IPF.jpgCoprates Labes (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)61 visiteThe finely ridged Materials visible in the upper portion of this NASA - Mars Odyssey Orbiter image - taken by the Spacecraft during its 49.450th orbit around the Red Planet - are huge Landslide (associated, most likely, with Mudslide) Deposits called Coprates Labes. These Deposits are found on the Floor of Coprates Chasma: a huge Canyon characterized by very steep Walls which is located in the Coprates Quadrangle of Mars, at 13,4° South Latitude and 61,4° West Longitude. Coprates Chasma is just a portion of the Valles Marineris Canyon System; it is approx. 966 Km (such as a little less than 600 miles) long and it got its name after a so-called "Classical Albedo Feature".
Latitude (centered): 11,7442° South
Longitude (centered): 292,003° East
Instrument: VIS
Captured: February, 5th, 2013
This frame (which is an Original Mars Odyssey Orbiter b/w frame published on the NASA - Planetary Photojournal with the ID n. PIA 16271) has been additionally processed and then colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - Mars Odyssey Orbiter and then looked down, towards the Surface of Mars), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team.MareKromium
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Coprates_Labes_Canyon-Tra_000849_1675_red~0.jpgCoprates Labes (possible True Colors; credits: Lunar Explorer Italia)106 visiteCoprates Labes is a Martian canyon, part of the huge Valles Marineris System. Valles Marineris most likely formed through tectonic processes, with extensional stresses leading to collapse of the terrain that now lies at the base of the canyons. Filling most of this image, we see a raised block on the canyon bottom, which is quite possibly a horst—a block bounded by faults that separate it from sunken blocks on each side. The raised block is heavily eroded, possibly by wind; this erosion has exposed its internal layering, especially at the Southeastern margin of the block.
Here we see asymmetric erosion features with shallow slopes trailing off to the North-West, suggesting that southeasterly winds dominate the flow through this Region. The arrangement of dunes and ripples in the lower right portion of the image confirms this prevailing wind direction.
Finally, dark-toned material appears to have flowed from North-East to South-West along the block, possibly moving in a very fluid debris flow. MareKromium
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