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Piú votate - Mars Reconnaissance Orbiter (MRO)
PSP_010047_1745_RED-00.jpg
PSP_010047_1745_RED-00.jpgStar-like shaped Hill in Terra Tyrrhena (possible True Colors; credits: Lunar Explorer Italia)65 visiteMars Local Time: 15:34 (middle afternoon)
Coord. (centered): 5,2° South Lat. and 99,6° East Long.
Spacecraft altitude: 264,2 Km (such as about 165,1 miles)
Original image scale range: 26,4 cm/pixel (with 1 x 1 binning) so objects ~52,9 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 1,6°
Phase Angle: 59,6°
Solar Incidence Angle: 58° (meaning that the Sun is about 32° above the Local Horizon)
Solar Longitude: 128,4° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
1 commentiMareKromium55555
(3 voti)
PSP_010008_1555_RED.jpg
PSP_010008_1555_RED.jpgCentral Uplift of Unnamed Crater in Terra Tyrrhena (possible True Colors; credits: Lunar Explorer Italia)62 visiteMars Local Time: 15:41 (middle afternoon)
Coord. (centered): 24,4° South Lat. and 87,5° East Long.
Spacecraft altitude: 259,4 Km (such as about 162,1 miles)
Original image scale range: 25,9 cm/pixel (with 1 x 1 binning) so objects ~1,04 mt across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 7,8°
Phase Angle: 64,1°
Solar Incidence Angle: 70° (meaning that the Sun is about 20° above the Local Horizon)
Solar Longitude: 127,0° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
PSP_009917_1665_RED.jpg
PSP_009917_1665_RED.jpgUnnamed Rayed Crater (natural colors; credits: Lunar Explorer Italia)59 visiteMars Local Time: 15:28 (early afternoon)
Coord. (centered): 13,4° South Lat. and 48,2° East Long.
Spacecraft altitude: 276,5 Km (such as about 172,8 miles)
Original image scale range: 27,7 cm/pixel (with 1 x 1 binning) so objects ~83 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 22,5°
Phase Angle: 79,7°
Solar Incidence Angle: 62° (meaning that the Sun is about 28° above the Local Horizon)
Solar Longitude: 123,6° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
PSP_009765_1780_RED.jpg
PSP_009765_1780_RED.jpgPossible Skylight Near Arsia Mons (possible True Colors; credits: Lunar Explorer Italia)65 visiteMars Local Time: 15:29 (early afternoon)
Coord. (centered): 2,1° South Lat. and 237,8° East Long.
Spacecraft altitude: 159,8 Km (such as about 162,4 miles)
Original image scale range: 26 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: 5,4°
Phase Angle: 61,0°
Solar Incidence Angle: 57° (meaning that the Sun is about 33° above the Local Horizon)
Solar Longitude: 118,1° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia

Nota Lunexit: "Skylight" ----> curiosa, ma bella, espressione NASA che indica un pozzo da collasso a camino verticale.
MareKromium55555
(3 voti)
PSP_009863_1465_RED.jpg
PSP_009863_1465_RED.jpgPotentially Well-Preserved Flow-Ejecta Crater in Northeastern Hellas Planitia (possible True Colors; credits: Lunar Explorer Italia)61 visiteMars Local Time: 15:38 (middle afternoon)
Coord. (centered): 33,2° South Lat. and 86,6° East Long.
Spacecraft altitude: 255,2 Km (such as about 159,5 miles)
Original image scale range: 51,1 cm/pixel (with 1 x 1 binning) so objects ~1,53 mt across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 1,9°
Phase Angle: 76,9°
Solar Incidence Angle: 75° (meaning that the Sun is about 15° above the Local Horizon)
Solar Longitude: 121,6° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
PSP_009878_2605_RED.jpg
PSP_009878_2605_RED.jpgUnconformity in Gemina Lingula Layered Deposits (possible True Colors; credits: Lunar Explorer Italia)64 visiteMars Local Time: 15:15 (early afternoon)
Coord. (centered): 80,3° South Lat. and 22,6° East Long.
Spacecraft altitude: 340,6 Km (such as about 212,9 miles)
Original image scale range: 34,1 cm/pixel (with 1 x 1 binning) so objects ~1,02 mt across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 21,1°
Phase Angle: 45,9°
Solar Incidence Angle: 63° (meaning that the Sun is about 27° above the Local Horizon)
Solar Longitude: 122,2° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
PSP_009789_1660_RED.jpg
PSP_009789_1660_RED.jpgCoprates' Wall (possible True Colors; credits: Lunar Explorer Italia)66 visiteMars Local Time: 15:42 (middle afternoon)
Coord. (centered): 14,1° South Lat. and 306,6° East Long.
Spacecraft altitude: 289,5 Km (such as about 180,9 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: 26,4°
Phase Angle: 46,9°
Solar Incidence Angle: 65° (meaning that the Sun is about 25° above the Local Horizon)
Solar Longitude: 118,9° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
PSP_009849_1485_RED.jpg
PSP_009849_1485_RED.jpgCentral Uplift and Impact Melt in Unnammed Crater in Hesperia Region (possible True Colors; credits: Lunar Explorer Italia)63 visiteMars Local Time: 15:38 (middle afternoon)
Coord. (centered): 31,3° South Lat. and 108,7° East Long.
Spacecraft altitude: 253,2 Km (such as about 158,3 miles)
Original image scale range: 50,7 cm/pixel (with 1 x 1 binning) so objects ~1,52 mt across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 0,4°
Phase Angle: 74,6°
Solar Incidence Angle: 74° (meaning that the Sun is about 16° above the Local Horizon)
Solar Longitude: 121,1° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
PSP_007779_2570_RED_abrowse~0.jpg
PSP_007779_2570_RED_abrowse~0.jpgDunes of the High Northern Latitudes (MULTISPECTRUM; credits: Lunexit)87 visiteIn this image, we can see that the North Pole is surrounded by a vast “sea” of Basaltic Sand Dunes. In Northern Winter a Seasonal Polar Cap composed of CO2 ice (dry ice) forms and the surrounding dunes become covered with frost. In the Spring, the ice sublimates (evaporates directly from ice to gas) loosening and moving tiny dust particles.
The bright portions of the dunes in this image are areas still covered with seasonal frost while dark spots are areas where the frost is gone or dark dust has cascaded down the sides of the dune.
The dunes imaged here are similar to Barchan dunes that are commonly found in desert regions on Earth. Barchan dunes are generally crescent-shaped with a steep slip face bordered by horns oriented in the downwind direction. Barchan dunes form by winds blowing mainly in one direction and thus are good indicators of the dominant wind direction when the dunes formed.
MareKromium55555
(3 voti)
PSP_007678_2050_RED_abrowse~0.jpg
PSP_007678_2050_RED_abrowse~0.jpgProposed MSL Landing Site in Mawrth Vallis (MULTISPECTRUM; credits: Lunexit)57 visiteMawrth Vallis has a rich mineral diversity, including clay minerals that formed by the chemical alteration of rocks or loose “regolith” (soil) by water.

The CRISM instrument on the MRO Spacecraft has detected a variety of clay minerals here that could signify different processes of formation. The high resolution of the HiRISE camera helps us to see and trace out layers, polygonal fractures and, with CRISM, examine the distribution of various minerals across the surface.

This surface is scientifically compelling for the Mars Science Laboratory (MSL) Rover, although some of the terrain might be somewhat rough. Scientists use HiRISE images to find the safest possible Landing Site for the Rover.
This is one of four candidate landing sites in the Mawrth Vallis region.
MareKromium55555
(3 voti)
PSP_009751_1645_RED.jpg
PSP_009751_1645_RED.jpgPit in Southeastern Syria Planum (possible True Colors; credits: Lunar Explorer Italia)66 visiteMars Local Time: 15:32 (middle afternoon)
Coord. (centered): 15,4° North Lat. and 261,7° East Long.
Spacecraft altitude: 251 Km (such as about 156,9 miles)
Original image scale range: 25,1 cm/pixel (with 1 x 1 binning) so objects ~75 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 5°
Phase Angle: 68°
Solar Incidence Angle: 64° (meaning that the Sun is about 26° above the Local Horizon)
Solar Longitude: 117,6° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
Psp_009758_2030_red.jpg
Psp_009758_2030_red.jpgExtremely Unusually-looking Northern Dunefield (possible True Colors; credits: Lunar Explorer Italia)73 visiteMars Local Time: 15:24 (early afternoon)
Coord. (centered): 22,7° North Lat. and 65,8° East Long.
Spacecraft altitude: 282,4 Km (such as about 176,5 miles)
Original image scale range: 28,3 cm/pixel (with 1 x 1 binning) so objects ~56,5 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 4,8°
Phase Angle: 51,5°
Solar Incidence Angle: 47° (meaning that the Sun is about 43° above the Local Horizon)
Solar Longitude: 117,8° (Northern Summer)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium55555
(3 voti)
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