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| Ultimi arrivi - Mars Reconnaissance Orbiter (MRO) |
Psp_009684_1695_red.jpgExposure of Light-Toned Layering along Wallrock in Coprates Chasma (possible True Colors; credits: Lunar Explorer Italia)59 visiteMars Local Time: 15:32 (middle afternoon)
Coord. (centered): 10,2° South Lat. and 290,8° East Long.
Spacecraft altitude: 260,8 Km (such as about 163,0 miles)
Original image scale range: 26,1 cm/pixel (with 1 x 1 binning) so objects ~78 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 2,5°
Phase Angle: 59,7°
Solar Incidence Angle: 62° (meaning that the Sun is about 28° above the Local Horizon)
Solar Longitude: 115,1° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 22, 2008
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Psp_010345_2150_red.jpgPits in Cyane Fossae (Saturated Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)59 visiteMars Local Time: 15:30 (middle afternoon)
Coord. (centered): 34,4° North Lat. and 239,0° East Long.
Spacecraft altitude: 285,7 Km (such as about 178,6 miles)
Original image scale range: 57,2 cm/pixel (with 1 x 1 binning) so objects ~1,72 mt across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,3°
Phase Angle: 50,5°
Solar Incidence Angle: 50° (meaning that the Sun is about 40° above the Local Horizon)
Solar Longitude: 139,8° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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Psp_010369_2065_red.jpgScoured Crater Rim (possible True Colors; credits: Lunar Explorer Italia)63 visiteMars Local Time: 15:30 (middle afternoon)
Coord. (centered): 26,3° North Lat. and 304,3° East Long.
Spacecraft altitude: 290,2 Km (such as about 181,4 miles)
Original image scale range: 29 cm/pixel (with 1 x 1 binning) so objects ~87 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 8,1°
Phase Angle: 57,9°
Solar Incidence Angle: 50° (meaning that the Sun is about 40° above the Local Horizon)
Solar Longitude: 140,7° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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PSP_010281_1510_RED_abrowse-00.jpgSedimentary Layers in Columbus Crater (ctx frame - possible True Colors; credits: Lunar Explorer Italia)59 visiteThis image covers a portion of the North-Eastern Inner Wall of Columbus Crater, located in the Southern Hemisphere of Mars and is approx. 100 Km (about 60 miles) in diameter.
Layered sedimentary rocks are found on the Crater Walls and Floor, and may have been deposited by water or by wind. These rocks have subsequently been eroded to expose their successive layers in cross-section.
The near-infrared spectrometer CRISM has revealed that these layers contain various hydrated minerals.
Mars Local Time: 15:42 (middle afternoon)
Coord. (centered): 28,6° South Lat. and 194,3° East Long.
Spacecraft altitude: 256,0 Km (such as about 160,0 miles)
Original image scale range: 25,6 cm/pixel (with 1 x 1 binning) so objects ~77 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,5°
Phase Angle: 70,9°
Solar Incidence Angle: 70° (meaning that the Sun is about 20° above the Local Horizon)
Solar Longitude: 137,3° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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PSP_010281_1510_RED_abrowse-01.jpgSedimentary Layers in Columbus Crater (edm - possible True Colors; credits: Lunar Explorer Italia)58 visiteVisible in this edm is a north-facing slope (roughly 250 meters, or 800 feet, across) exposing finely layered sedimentary rock.
In this possibly true-color view, layers with a dark silver-gray appearance may be intrinsically darker, or may have a texture that more effectively collects dark sand particles, than adjacent layers with a brighter appearance.MareKromiumDic 21, 2008
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Psp_009717_2545_red.jpgSmall Crater on Arcuate Ridge, West of Olympia Mensae (possible True Colors; credits: Lunar Explorer Italia)57 visiteMars Local Time: 14:53 (early afternoon)
Coord. (centered): 74,3° North Lat. and 93,7° East Long.
Spacecraft altitude: 314,9 Km (such as about 196,8 miles)
Original image scale range: 31,5 cm/pixel (with 1 x 1 binning) so objects ~95 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 1,9°
Phase Angle: 55,2°
Solar Incidence Angle: 57° (meaning that the Sun is about 33° above the Local Horizon)
Solar Longitude: 116,3° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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Psp_009731_2165_red.jpgPeriglacial Modification of a Fairly Fresh Crater in Utopia Planitia (possible True Colors; credits: Lunar Explorer Italia)60 visiteMars Local Time: 15:19 (early afternoon)
Coord. (centered): 36,0° North Lat. and 80,7° East Long.
Spacecraft altitude: 295,3 Km (such as about 184,6 miles)
Original image scale range: 29,5 cm/pixel (with 1 x 1 binning) so objects ~89 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 8,4°
Phase Angle: 53,4°
Solar Incidence Angle: 45° (meaning that the Sun is about 45° above the Local Horizon)
Solar Longitude: 116,8° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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Psp_009729_1735_red.jpgTerraced Fan in Aeolis Planum Region (possible True Colors; credits: Lunar Explorer Italia)60 visiteThis image shows the South-Western Region of a degraded crater’s floor, located near the Equator. The high-standing ridge near the left side of the scene is a terrace that slumped off the crater’s rim (located to the far left of this frame, but out of the image). The bumpy terrain near the bottom of the image is also material that has slumped off the crater rim.
The center of the image contains a terraced fan. The fan emanates from a valley (not pictured, located in the lower part of the scene) that intersects the crater’s south rim, which suggests that the valley might have transported fluid, likely water, into the crater. If this happened, then the fan marks where the flow deposited its sediment.
Mars Local Time: 15:29 (early afternoon)
Coord. (centered): 6,5° South Lat. and 141,2° East Long.
Spacecraft altitude: 266,7 Km (such as about 166,7 miles)
Original image scale range: 26,7 cm/pixel (with 1 x 1 binning) so objects ~80 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 6,2°
Phase Angle: 63,8°
Solar Incidence Angle: 59° (meaning that the Sun is about 31° above the Local Horizon)
Solar Longitude: 116,8° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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PSP_009713_2415_RED.jpgVastitas' Rocky Terrain (possible True Colors; credits: Lunar Explorer Italia)60 visiteMars Local Time: 15:10 (early afternoon)
Coord. (centered): 61,4° North Lat. and 208,0° East Long.
Spacecraft altitude: 310,1 Km (such as about 193,8 miles)
Original image scale range: 31,0 cm/pixel (with 1 x 1 binning) so objects ~93 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,3°
Phase Angle: 50,8°
Solar Incidence Angle: 51° (meaning that the Sun is about 39° above the Local Horizon)
Solar Longitude: 116,2° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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PSP_009714_1725_RED.jpgPeriequatorial Surface Sample (natural colors; credits: Lunar Explorer Italia)61 visiteMars Local Time: 15:31 (middle afternoon)
Coord. (centered): 7,5° South Lat. and 191,3° East Long.
Spacecraft altitude: 265,0 Km (such as about 165,6 miles)
Original image scale range: 26,5 cm/pixel (with 1 x 1 binning) so objects ~80 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,1°
Phase Angle: 59,8°
Solar Incidence Angle: 60° (meaning that the Sun is about 30° above the Local Horizon)
Solar Longitude: 116,2° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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Psp_009698_1705_red.jpgNoctis Labyrinthus Region (possible True Colors; credits: Lunar Explorer Italia)93 visiteMars Local Time: 15:26 (early afternoon)
Coord. (centered): 9,3° South Lat. and 266,9° East Long.
Spacecraft altitude: 268,1 Km (such as about 167,5 miles)
Original image scale range: 26,8 cm/pixel (with 1 x 1 binning) so objects ~80 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 19,2°
Phase Angle: 75,1°
Solar Incidence Angle: 60° (meaning that the Sun is about 30° above the Local Horizon)
Solar Longitude: 115,7° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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Psp_009659_2425_red.jpgTerrain in Vastitas Borealis (possible True Colors; credits: Lunar Explorer Italia)60 visiteMars Local Time: 15:08 (early afternoon)
Coord. (centered): 62,4° North Lat. and 241,9° East Long.
Spacecraft altitude: 309,5 Km (such as about 193,4 miles)
Original image scale range: 61,9 cm/pixel (with 1 x 1 binning) so objects ~1,86 mt across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,3°
Phase Angle: 50,8°
Solar Incidence Angle: 51° (meaning that the Sun is about 39° above the Local Horizon)
Solar Longitude: 114,3° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromiumDic 21, 2008
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