| Risultati della ricerca nelle immagini - "Lava" |
Crater-Unnamed_Crater_and_Lava_Flows_in_Amazonis_Planitia-PCF-LXTT.jpgUnnamed Crater and Lava Flows in Amazonis Planitia (Absolute Natural Colors; credits for the additional process. and color.: Drr Gianluigi Barca and Paolo C. Fienga - Lunexit Team)183 visitenessun commentoMareKromium
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ESP_014184_2070_RED_abrowse.jpgLava Flows in Amazonis Planitia (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)210 visitenessun commentoMareKromium
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ESP_017546_1965_RED_abrowse-PCF-LXTT.jpgFeatures of Amazonis Planitia (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)187 visiteMars Local Time: 15:10 (early afternoon)
Coord. (centered): 16,1° North Lat. and 205,7° East Long.
Spacecraft altitude: 283,3 Km (such as about 177,0 miles)
Original image scale range: 56,7 cm/pixel (with 2 x 2 binning) so objects ~ 1 mt and 70 cm across are resolved
Map projected scale: 50 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 2,3°
Phase Angle: 47,3°
Solar Incidence Angle: 45° (meaning that the Sun is about 45° above the Local Horizon)
Solar Longitude: 81,9° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromium
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ESP_017888_1950_RED_abrowse.jpgOlympus' Lava Flows (Extremely Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)54 visiteThe flanks of Olympus Mons are covered with Lava Flows (one on top of the other) Most of these Flows are relatively narrow, with a channel running down the middle. They appear similar to the Lava Flows found on Mt. Etna in Sicily (Italy).
However, in this image, we see these typical Flows partially covered by another, more recent one. This last one also shows a Central Channel, and it is about 10 times wider than the more typical Lava Flows. At the center of the HiRISE image the Channel disappears.
This is probably because the Channel was blocked here and Lava spilled out of it and covered a broad, fan-shaped, area. The eruption that produced this unusual flow was probably more vigorous and perhaps lasted longer than the more common ones.MareKromium
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ESP_018534_1985_RED_abrowse-PCF-LXTT1.jpgLava Flows at the base of Olympus Mons (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)104 visitenessun commentoMareKromium
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ESP_018665_1920_RED_abrowse.jpgLava Channel (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)86 visitenessun commentoMareKromium
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ESP_020580_2035_RED_abrowse-00.jpgLava Flow constricted between Topographic Obstacles (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)231 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 ItaliaMareKromium
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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)238 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 ItaliaMareKromium
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ESP_020827_1595_RED_abrowse-PCF-LXTT.jpgOlivine-rich Terrain (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)102 visitenessun commentoMareKromium
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ESP_024572_1900-PCF-LXTT-2.jpgLava Flows (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)183 visiteMars Local Time: 14:28 (early afternoon)
Coord. (centered): 10,0° North Lat. and 267,5° East Long.
Spacecraft altitude: 270,1 Km (such as about 168,8 miles)
Original image scale range: 27,0 cm/pixel (with 1 x 1 binning) so objects ~ 81,0 cm across are resolved
Map projected scale: 25 cm/pixel
Map projection: EQUIRECTANGULAR
Emission Angle: 2,0°
Phase Angle: 34,6°
Solar Incidence Angle: 37° (meaning that the Sun is about 53° above the Local Horizon)
Solar Longitude: 19,7° (Northern Spring)
Credits: NASA/JPL/University of Arizona
Additional process. and coloring: Lunar Explorer ItaliaMareKromium
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ESP_024587_1465_RED-PCF-LXTT-00.jpgUnnamed Crater partially invaded by Lava Flow (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)211 visiteCoord. (centered): 33,3° South Lat. and 222,7° East Long.MareKromium
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ESP_024587_1465_RED-PCF-LXTT-01.jpgUnnamed Crater partially invaded by Lava Flow (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)216 visiteCoord. (centered): 33,3° South Lat. and 222,7° East Long.
MareKromium
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