Inizio Registrati Login

Elenco album Ultimi arrivi Ultimi commenti Più viste Più votate Preferiti Cerca

Inizio > MARS > Mars Reconnaissance Orbiter (MRO)

Piú viste - Mars Reconnaissance Orbiter (MRO)
ESP_020580_2035_RED_abrowse-01.jpg
ESP_020580_2035_RED_abrowse-01.jpgLava Flow constricted between Topographic Obstacles (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)243 visiteMars Local Time: 15:35 (Middle Afternoon)
Coord. (centered): 23,1° North Lat. and 172,8° East Long.
Spacecraft altitude: 288,7 Km (such as about 180,4 miles)
Original image scale range: 57,8 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 73 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 4,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 57,4°
Solar Incidence Angle: 61° (meaning that the Sun is about 29° above the Local Horizon)
Solar Longitude: 199,9° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_020871_2055_RED_abrowse-PCF-LXTT.jpg
ESP_020871_2055_RED_abrowse-PCF-LXTT.jpgElysium Montes (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)242 visitenessun commentoMareKromium
ESP_024553_1500-PCF-LXTT-003.jpg
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 Italia
MareKromium
PSP_006998_2060_RED_abrowse.jpg
PSP_006998_2060_RED_abrowse.jpgRecent Impact? (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)240 visitenessun commentoMareKromium
ESP_022999_1335_RED_abrowse-PCF-LXTT-01.jpg
ESP_022999_1335_RED_abrowse-PCF-LXTT-01.jpgUnnamed Crater with Gullies (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C . Fienga - Lunar Explorer Italia)240 visitenessun commentoMareKromium
ESP_023920_1180-PCF-LXTT-1.jpg
ESP_023920_1180-PCF-LXTT-1.jpgFeatures of an Unnamed Southern Channel (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)240 visiteMars Local Time: 14:38 (Early Afternoon)
Coord. (centered): 61,6° South Lat. and 79,2° East Long.
Spacecraft altitude: 251,6 Km (such as about 157,3 miles)
Original image scale range: 25,2 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: 8,7°
Sun-Mars-Spacecraft (or "Phase") Angle: 61,9°
Solar Incidence Angle: 66° (meaning that the Sun is about 24° above the Local Horizon)
Solar Longitude: 354,8° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_020930_1870_RED_abrowse-PCF-LXTT.jpg
ESP_020930_1870_RED_abrowse-PCF-LXTT.jpgPossible Olivine-rich Terrain in Terra Margaritifer (Absolute Natural Colors; credits for the additional process. and coloring: Dr Paolo C. Fienga - Lunexit Team)239 visitenessun commentoMareKromium
ESP_024025_1005-PCF-LXTT-01.jpg
ESP_024025_1005-PCF-LXTT-01.jpgFeatures of Promethei Lingula Region (CTX Frame "B" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)239 visiteMars Local Time: 15:51 (Middle Afternoon)
Coord. (centered): 79,5° South Lat. and 111,8° East Long.
Spacecraft altitude: 264,9 Km (such as about 165,6 miles)
Original image scale range: 53,0 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 59,0 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: POLAR STEREOGRAPHIC
Emission Angle: 22,0°
Sun-Mars-Spacecraft (or "Phase") Angle: 72,4°
Solar Incidence Angle: 84° (meaning that the Sun is about 6° above the Local Horizon)
Solar Longitude: 359,0° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_024460_1835_RED-PCF-LXTT.jpg
ESP_024460_1835_RED-PCF-LXTT.jpgFeatures of Libya Montes (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)239 visiteCoord. (centered): 3,7° North Lat. and 85,6° East Long.MareKromium
ESP_020917_2075_RED_abrowse-PCF-LXTT.jpg
ESP_020917_2075_RED_abrowse-PCF-LXTT.jpgUnnamed Craters in Acidalia Planitia (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)238 visitenessun commentoMareKromium
PSP_006724_2165_RED_abrowse-PCF-LXTT.jpg
PSP_006724_2165_RED_abrowse-PCF-LXTT.jpgUnnamed Channel in Utopia Planitia (Absolute Natural Colors; credits for the additional process. and coloring: Dr Paolo C. Fienga - Lunexit Team)236 visiteSeen here are gullies in an Unnamed Northern Crater. The Crater is well-preserved as indicated by its sharp Rim and steep Walls.
Gullies are rarer in the Northern Hemisphere, possibly because there are fewer Slopes for them to form on compared to the heavily cratered Southern Highlands.

This image captures a wide range of Gully morphologies. The Gullies on the North Wall (such as the South-facing Wall) are more abundant and evenly-spaced than those on the East and South Walls and they extend up to the Crater Rim on the northern side. These differences might occur because of differences in sunlight exposure and temperature variations.

The Crater Floor has a linear texture suggestive of flow. Ice-rich material might have moved off the Crater Walls, driven by gravity, and flowed towards the Crater center.
MareKromium
ESP_023094_1640_RED_abrowse.jpg
ESP_023094_1640_RED_abrowse.jpgThe Wall of Coprates Chasma (Enhanced and Darkened Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)236 visitenessun commentoMareKromium
2237 immagini su 187 pagina(e) 1 - 6 7 8 9 10 11 12 13 14 15 - 187

 
 

Powered by Coppermine Photo Gallery