| Ultimi arrivi - Mars in JPEG2000 |
ESP_024227_1595-1.jpgUnnamed Crater in Ladon Valles (Absolute Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)208 visiteMars Local Time: 14:25 (Early Afternoon)
Coord. (centered): 20,5° South Lat. and 330,0° East Long.
Spacecraft altitude: 260,9 Km (such as about 163,1 miles)
Original image scale range: 52,2 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 57 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 1,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 41,6°
Solar Incidence Angle: 43° (meaning that the Sun is about 47° above the Local Horizon)
Solar Longitude: 6,8° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Drr Gianluigi Barca and Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumNov 18, 2011
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ESP_024227_1595-2.jpgUnnamed Crater in Ladon Valles (Absolute Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)214 visiteMars Local Time: 14:25 (Early Afternoon)
Coord. (centered): 20,5° South Lat. and 330,0° East Long.
Spacecraft altitude: 260,9 Km (such as about 163,1 miles)
Original image scale range: 52,2 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 57 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 1,3°
Sun-Mars-Spacecraft (or "Phase") Angle: 41,6°
Solar Incidence Angle: 43° (meaning that the Sun is about 47° above the Local Horizon)
Solar Longitude: 6,8° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Drr Gianluigi Barca and Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumNov 18, 2011
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ESP_022657_1260_RED_abrowse-PCF-LXTT-05.jpgDust Devils' Tracks in Noachis Terra (Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)190 visiteMars Local Time: 14:28 (Early Afternoon)
Coord. (centered): 53,8° South Lat. and 357,1° East Long.
Spacecraft altitude: 253,0 Km (such as about 158,2 miles)
Original image scale range: 25,3 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: 5,4°
Sun-Mars-Spacecraft (or "Phase") Angle: 47,2°
Solar Incidence Angle: 43° (meaning that the Sun is about 47° above the Local Horizon)
Solar Longitude: 300,5° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Drr Gianluigi Barca and Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumNov 18, 2011
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ESP_022657_1260_RED_abrowse-PCF-LXTT-04.jpgDust Devils' Tracks in Noachis Terra (Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)206 visiteMars Local Time: 14:28 (Early Afternoon)
Coord. (centered): 53,8° South Lat. and 357,1° East Long.
Spacecraft altitude: 253,0 Km (such as about 158,2 miles)
Original image scale range: 25,3 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: 5,4°
Sun-Mars-Spacecraft (or "Phase") Angle: 47,2°
Solar Incidence Angle: 43° (meaning that the Sun is about 47° above the Local Horizon)
Solar Longitude: 300,5° (Northern Winter)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Drr Gianluigi Barca and Paolo C. Fienga - Lunar Explorer ItaliaMareKromiumNov 18, 2011
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ESP_023007_1410-PCF-LXTT-01.jpgFlow Features on a steep Unnamed Crater Slope (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)146 visitenessun commentoMareKromiumAgo 07, 2011
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ESP_023007_1410-PCF-LXTT-00.jpgFlow Features on a steep Unnamed Crater Slope (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)151 visitenessun commentoMareKromiumAgo 07, 2011
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ESP_023045_1380-PCF-LXTT-00.jpgFlow Features inside Newton Crater (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)154 visitenessun commentoMareKromiumAgo 07, 2011
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Volcanic_Features-Fissure-Cerberus_Fossae-TRA_000827_1875-PCF-LXTT.jpgDeep inside Cerberus Fossae (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)200 visitenessun commentoMareKromiumAgo 04, 2011
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Chrise_Planitia-PIA14462-PCF-LXTT.jpgFeatures of Chrise Planitia (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)179 visiteThe suggested area in this observation is characterized by a group of Cones, such as "shield-like" features, and round Mounds. They are a few hundred meters to kilometers in diameter, but their heights are still unknown.MareKromiumLug 17, 2011
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Claritas_Fossae-PIA14461-PCF-LXTT.jpgFeatures of Claritas Fossae (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)185 visiteThe Claritas Fossae Region is characterised by systems of "Graben" running mainly North-West to South-East. A Graben forms when a block of the Planet's Crust drops down between two Faults, due to extension, or pulling, of the Crust itself.
MareKromiumLug 17, 2011
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Crack_of_Unknown_Origin-ESP_022298_1555-GB-PCF-LXTT-03.jpgPossible Evidence of relatively recent Seismic Activity on Mars (credits for the Research and additional process.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)434 visitenessun commentoMareKromiumGiu 11, 2011
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Crack_of_Unknown_Origin-ESP_022298_1555-GB-PCF-LXTT-02.jpgPossible Evidence of relatively recent Seismic Activity on Mars (credits for the Research and additional process.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)231 visitenessun commentoMareKromiumGiu 11, 2011
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