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Risultati della ricerca nelle immagini - "Proximities"
Collapse_Features-PIA13734.jpg
Collapse_Features-PIA13734.jpgCollapse Features near Alba Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)105 visitenessun commentoMareKromium
ESP_012570_1670_RED_abrowse.jpg
ESP_012570_1670_RED_abrowse.jpgLight and Intermediate-Toned Material near Morava Valles (Natural Colors; credits: Lunar Explorer Italia)54 visitenessun commentoMareKromium
ESP_020551_1545_RED_abrowse.jpg
ESP_020551_1545_RED_abrowse.jpgMass Wasting near Claritas Fossae (Absolute Natural Colors; credits for the additional process. and color.: Dr Gianluigi Barca - Lunexit Team)198 visitenessun commentoMareKromium
ESP_024055_2045_RED_abrowse-PCF-LXTT-00.jpg
ESP_024055_2045_RED_abrowse-PCF-LXTT-00.jpgSpring on Mars! (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)172 visiteMars Local Time: 14:17 (Early Afternoon)
Coord. (centered): 24,5° North Lat. and 341,2° East Long.
Spacecraft altitude: 297,9 Km (such as about 186,2 miles)
Original image scale range: 59,6 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 79 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 16,5°
Phase Angle: 27,2°
Solar Incidence Angle: 41° (meaning that the Sun is about 49° above the Local Horizon)
Solar Longitude: 0,1° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_024055_2045_RED_abrowse-PCF-LXTT-01.jpg
ESP_024055_2045_RED_abrowse-PCF-LXTT-01.jpgSpring on Mars! (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)179 visiteMars Local Time: 14:17 (Early Afternoon)
Coord. (centered): 24,5° North Lat. and 341,2° East Long.
Spacecraft altitude: 297,9 Km (such as about 186,2 miles)
Original image scale range: 59,6 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 79 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 16,5°
Phase Angle: 27,2°
Solar Incidence Angle: 41° (meaning that the Sun is about 49° above the Local Horizon)
Solar Longitude: 0,1° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Dr Paolo C. Fienga - Lunar Explorer Italia
MareKromium
ESP_024584_1655-PCF-LXTT-00.jpg
ESP_024584_1655-PCF-LXTT-00.jpgProximities of the Valles Marineris Canyon System (CTX Frame "A" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)210 visiteMars Local Time: 14:30 (early afternoon)
Coord. (centered): 14,2° South Lat. and 302,2° East Long.
Spacecraft altitude: 266,9 Km (such as about 166,8 miles)
Original image scale range: 53,4 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 60 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 6,4°
Phase Angle: 49,1°
Solar Incidence Angle: 44° (meaning that the Sun is about 46° above the Local Horizon)
Solar Longitude: 20,1° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium
ESP_024584_1655-PCF-LXTT-01.jpg
ESP_024584_1655-PCF-LXTT-01.jpgProximities of the Valles Marineris Canyon System (CTX Frame "B" - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)213 visiteMars Local Time: 14:30 (early afternoon)
Coord. (centered): 14,2° South Lat. and 302,2° East Long.
Spacecraft altitude: 266,9 Km (such as about 166,8 miles)
Original image scale range: 53,4 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 60 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 6,4°
Phase Angle: 49,1°
Solar Incidence Angle: 44° (meaning that the Sun is about 46° above the Local Horizon)
Solar Longitude: 20,1° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium
ESP_026356_1960_RED_NOMAP_browse-PCF-LXTT.jpg
ESP_026356_1960_RED_NOMAP_browse-PCF-LXTT.jpgUnusually-looking Landforms near Grota Valles (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)111 visiteThe Landforms visible in this observation are quite diverse, with a segment of the Cerberus Fossae (such as a deep Trough extending East-West) and Surrounding Terrain that has been eroded by some Fluid, either Water (actually Mud) or Lava. There are also many Boulders in places, either on steep Slopes or excavated by Impact Craters. The high Hills are Islands of older Terrain surrounded by younger Lavas.

Mars Local Time: 15:08 (Early Afternoon)
Coord. (centered): 15,724° North Lat. and 162,022° East Long.
Spacecraft altitude: 281,3 Km (such as about 175,8 miles)
Original image scale range: 28,1 cm/pixel (with 1 x 1 binning) so objects ~ 84 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 4,7°
Sun - Mars - MRO (or "Phase") Angle: 40,5°
Solar Incidence Angle: 45° (meaning that the Sun is about 45° above the Local Horizon)
Solar Longitude: 81,7° (Northern Spring - Southern Autumn)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer Italia
MareKromium
MA_ADIM_VALLIS-440-20090629-6393-6-co-01_H1-1.jpg
MA_ADIM_VALLIS-440-20090629-6393-6-co-01_H1-1.jpgProximities of Ma'adim Vallis (Natural Colors; credits: ESA)69 visiteCaption ESA:"Mars Express image of a Region close to Ma’adim Vallis, one of the largest - after Vallis Marineris - canyons on Mars.
The imaged Region lies South-East of Ma’adim Vallis; the pictures are centred at about 29° South Lat. and 182° East Long. and have a ground resolution of 15 mt/pixel.

Ma’adim Vallis is located between the Volcanic Province of Tharsis, which harbours 4 volcanoes, including the largest in the Solar System, and the Hellas Planitia Impact Basin.
The canyon, approx. 20 Km wide and 2 Km deep, originates in the Southern Highlands close to the so-called ‘Dichotomy Boundary’ and ends in Gusev Crater.
The Dichotomy Boundary is a narrow Region separating the cratered Highlands, located mostly in the Southern Hemisphere of Mars, from the Northern Hemisphere's Lowland Plains".
MareKromium
OPP-SOL036-P2274_L257-B067R1-PCF-LXTT~0.jpg
OPP-SOL036-P2274_L257-B067R1-PCF-LXTT~0.jpgMeridiani Planum - Sol 36 (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)168 visitenessun commentoMareKromium
OPP-SOL036-PCF-LXTT-IPF.jpg
OPP-SOL036-PCF-LXTT-IPF.jpgOpportunity's Backshell and Parachute - Sol 36 (Absolute Natural Colors; credits for the additional process. and color. Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)114 visitenessun commentoMareKromium
OPP-SOL1160-1N231175962EFF8293P0765R0M1-PCF-LXTT.jpg
OPP-SOL1160-1N231175962EFF8293P0765R0M1-PCF-LXTT.jpgHorizon with Small Dunefield near Victoria - Sol 1160 (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)139 visitenessun commentoMareKromium
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