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Inizio > MARS > Mars Reconnaissance Orbiter (MRO)

Piú votate - Mars Reconnaissance Orbiter (MRO)
ESP_022343_1735_RED_abrowse-PCF-LXTT.jpg
ESP_022343_1735_RED_abrowse-PCF-LXTT.jpgFaulted, Layered Deposits in Candor Chasma (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)183 visiteAcquisition date: May, 3, 2011
Mars Local Time: 14:34 (Early Afternoon)
Latitude (centered): 6,6° South
Longitude (East): 284,1°
Spacecraft Altitude (such as "Range to Target Site"): 269,1 Km (168,2 miles)
Original Image Scale Range: 26,9 cm/pixel (with 1 x 1 binning) so objects ~81 cm across are resolved
Map Projected Scale: 25 cm/pixel
Map Projection: EQUIRECTANGULAR
Emission Angle: 12,6°
Sun-Target-MRO (such as "Phase") Angle: 29,6°
Solar Incidence Angle (S.I.A.): 41°, with the Sun about 49° above the Local Horizon
Solar Longitude: 285,6° (Northern Winter)
MareKromium55555
(2 voti)
ESP_019351_1795_RED_abrowse-01-PCF-LXTT.jpg
ESP_019351_1795_RED_abrowse-01-PCF-LXTT.jpgCollapse Pit on the S/E Flank of Pavonis Mons (EDM - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)206 visiteCaption NASA:"The interior of the Pit consists of sediment-covered Boulders that range in size from approximately 5 meters (approximately 16 ft) to less than 1 meter (approximately 3 feet) in diameter. The interior region of the Pit appears to slope towards the North-West. Such Pits may form from collapse of a surface "roof" below which Lava may long ago have flowed, or as a result of removal of subsurface material due to erosion or extension".MareKromium55555
(2 voti)
ESP_019351_1795_RED_abrowse-00-PCF-LXTT.jpg
ESP_019351_1795_RED_abrowse-00-PCF-LXTT.jpgCollapse Pit on the S/E Flank of Pavonis Mons (CTX Frame - Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)199 visiteCaption NASA:"This image is located on the South/Eastern Flank of Pavonis Mons, a large Volcano located in the Tharsis Region of Mars. The dark, circular Pit Feature roughly in the middle of the image is about 180 meters at its widest diameter. The Pit appears to be surrounded by small sand dunes".

Acquisition date: 12 September 2010
Mars Local Time: 15:33 (Middle Afternoon)
Latitude (centered): 0,5° South
Longitude (East): 248,6°
Spacecraft Altitude (such as "Range to Target Site"): 256,4 Km (160,2 miles)
Original Image Scale Range: 25,6 cm/pixel (with 1 x 1 binning) so objects ~77 cm across are resolved
Map Projected Scale: 25 cm/pixel and North is up
Map Projection: EQUIRECTANGULAR
Emission Angle: 3,2°
Sun-Target-MRO (such as "Phase") Angle: 51,8°
Solar Incidence Angle (S.I.A.): 55°, with the Sun about 35° above the Local Horizon
Solar Longitude: 147,2° (Northern Summer)
MareKromium55555
(2 voti)
ESP_022212_1650_RED_abrowse-PCF-LXTT-1.jpg
ESP_022212_1650_RED_abrowse-PCF-LXTT-1.jpgInteresting Surface Features in Syria Planum (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 261 visiteCaption NASA:"This observation was to offer us a two-for-one treat: a small Volcano and a Double Crater with Ejecta Ridges caused by a binary impact. However, with little data volume, we were not able to get both targets, so we used a manual delay to image the Double Crater. A possible re-image of this area might focus on the Volcano. The site appears fairly dusty and there may not be much fine-scale structure to see.
Syria Planum is a broad Plateau, forming part of the Tharsis Region, which is home to the largest Volcanos in the Solar System. Some of these, Arsia Mons and Pavonis Mons, are also known as "Shield Volcanoes".
MareKromium55555
(2 voti)
PSP_002157_1715_red-PCF-LXTT-02.jpg
PSP_002157_1715_red-PCF-LXTT-02.jpgRecent Impact near Arsia Mons' Summit (CTX and EDM in Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)304 visitenessun commentoMareKromium55555
(2 voti)
ESP_022290_1735_RED_abrowse-PCF-LXTT.jpg
ESP_022290_1735_RED_abrowse-PCF-LXTT.jpgFeatures of Candor Chasma (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)217 visitenessun commentoMareKromium55555
(2 voti)
PSP_002909_2000_RED_abrowse-PCF-LXTT.jpg
PSP_002909_2000_RED_abrowse-PCF-LXTT.jpgFeatures of Olympus Mons (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)214 visitenessun commentoMareKromium55555
(2 voti)
ESP_022251_1485_RED_abrowse.jpg
ESP_022251_1485_RED_abrowse.jpgUnnamed Southern Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)190 visitenessun commentoMareKromium55555
(2 voti)
ESP_022299_2040_RED_abrowse.jpg
ESP_022299_2040_RED_abrowse.jpgFresh Impacts (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)244 visitenessun commentoMareKromium55555
(2 voti)
ESP_022250_2065_RED_abrowse.jpg
ESP_022250_2065_RED_abrowse.jpgDark Dunes in Lobo Vallis (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 227 visitenessun commentoMareKromium55555
(2 voti)
ESP_022277_1760_RED_abrowse.jpg
ESP_022277_1760_RED_abrowse.jpgFeatures of Ophir Chasma (Absolute Natural Colors; credits for the addtional process. and color.: Dr Paolo C. Fienga - Lunexit Team)185 visitenessun commentoMareKromium55555
(2 voti)
ESP_022262_1475_RED_abrowse-00-PCF-LXTT.jpg
ESP_022262_1475_RED_abrowse-00-PCF-LXTT.jpgUnnamed Southern Crater with Gullies (CTX Frame - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)234 visitenessun commentoMareKromium55555
(2 voti)
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