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Risultati della ricerca nelle immagini - "Canyon"
Coprates_Catena-h0438_0000_nd3-00-PCF-LXTT.jpg
Coprates_Catena-h0438_0000_nd3-00-PCF-LXTT.jpgFrame Mars Express n. h0438_0000_nd3 (natural colors - elab. Lunexit) 58 visitenessun commentoMareKromium
Coprates_Catena-h0438_0000_nd3-00.jpg
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
Coprates_Catena-h0438_0000_nd3-01.jpg
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)94 visitenessun commentoMareKromium
ESP_012195_1750_RED_abrowse.jpg
ESP_012195_1750_RED_abrowse.jpgMartian Grand Canyon! (Natural Colors; credits: Lunar Explorer Italia)56 visitenessun commentoMareKromium
PIA11377.jpg
PIA11377.jpgMartian "Opal" (natural colors; credits: Lunexit)64 visiteNASA's Mars Reconnaissance Orbiter has revealed Martian rocks containing a hydrated mineral similar to Opal.

The rocks are light-toned and appear cream-colored in this natural-color image taken by the High Resolution Imaging Science Experiment (HiRISE) camera. Images acquired by the orbiter reveal that different layers of rock have different properties and chemistry.
The Opal minerals are located in distinct beds of rock outside of the large Valles Marineris Canyon System and are also found in rocks within the canyon. The presence of opal in these relatively young rocks tells scientists that water, possibly as rivers and small ponds, interacted with the surface as recently as two billion years ago, one billion years later than scientists had expected.

The discovery of this new category of minerals spread across large regions of Mars suggests that liquid water played an important role in shaping the Planet's Surface and possibly hosting life.
MareKromium
PSP_005109_1770_RED_browse-PCF-LXTT.jpg
PSP_005109_1770_RED_browse-PCF-LXTT.jpgPeri-Equatorial Canyon and Winstreak (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 98 visitenessun commentoMareKromium
PSP_010423_1720_RED_abrowse.jpg
PSP_010423_1720_RED_abrowse.jpgSteep Canyon's Wall, South of Jus Chasma (Natural - but enhanced - Colors; credits: Lunar Explorer Italia)57 visitenessun commentoMareKromium
Psp_009408_1715_red.jpg
Psp_009408_1715_red.jpgShadowland (possible True Colors; credits: Lunar Explorer Italia)54 visiteMars Local Time: 15:31 (middle afternoon)
Coord. (centered): 8,3° South Lat. and 266,4° East Long.
Spacecraft altitude: 263,4 Km (such as about 164,6 miles)
Original image scale range: 52,7 cm/pixel (with 1 x 1 binning) so objects ~1,58 mt across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 10,5°
Phase Angle: 53,3°
Solar Incidence Angle: 61° (meaning that the Sun is about 29° above the Local Horizon)
Solar Longitude: 105,3° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium
Psp_009557_1905_red.jpg
Psp_009557_1905_red.jpgChannels in Athabasca Valles (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)55 visiteMars Local Time: 15:32 (middle afternoon)
Coord. (centered): 10,3° North Lat. and 157,0° East Long.
Spacecraft altitude: 292,6 Km (such as about 182,9 miles)
Original image scale range: 29,3 cm/pixel (with 1 x 1 binning) so objects ~88 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 19,7°
Phase Angle: 35,8°
Solar Incidence Angle: 52° (meaning that the Sun is about 38° above the Local Horizon)
Solar Longitude: 110,6° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium
Troughs-Tharsis_Region-PIA04103-000.jpg
Troughs-Tharsis_Region-PIA04103-000.jpgWhat's inside the Trough? (CTX Frame - Original NASA/MGS/MSSS b/w Frame)56 visiteCaption NASA originale:"This MGS-MOC image shows Channels carved by catastrophic Floods in the Tharsis Region of Mars. This area is located North/West of Jovis Tholus, and East of the large Martian Volcano Olympus Mons. The Terrain is presently mantled with fine Dust".

Location near: 10,5° North Lat. and 203,4° West Long.
Image width: width: ~3 Km (~1,9 mi)
Illumination from: lower left
Season: Northern Autumn
Valles_Marineris-h0442_0008_nd3.jpg
Valles_Marineris-h0442_0008_nd3.jpgPortion of the Valles Marineris Canyon System (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga)73 visitenessun commentoMareKromium
Valles_Marineris-h0471_0001_nd3.jpg
Valles_Marineris-h0471_0001_nd3.jpgPortion of the Valles Marineris Canyon System (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga)68 visitenessun commentoMareKromium
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