| Piú votate - Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas) |
Volcanoes-Olympus_Mons_Caldera-2-015-090204_1-0037_01-6v-PCF-LXTT.jpgOlympus Mons' Caldera (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)241 visitenessun commentoMareKromium
(6 voti)
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Volcanoes-Olympus_Mons_Caldera-4-015-090204_1-0037_01-6v-PCF-LXTT.jpgOlympus Mons' Caldera (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)236 visitenessun commentoMareKromium
(6 voti)
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Volcanoes-Olympus_Mons_Caldera-3-015-090204_1-0037_01-6v-PCF-LXTT.jpgOlympus Mons' Caldera (Absolute Natural Colors; credits for the additional process. and color: Dr Paolo C. Fienga - Lunexit Team)240 visitenessun commentoMareKromium
(6 voti)
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CR-h0330_0000_nd3-PCF-LXTT.jpgFrame h0330_0000_nd3 - Pollack Crater and Surroundings (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)198 visitenessun commentoMareKromium
(6 voti)
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Aeolian_Features-Yardangs-h0522_0000_re3.jpgAeolian Surface Features (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)87 visitenessun commentoMareKromium
(6 voti)
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Coprates_Catena-h0438_0000_nd3-01.jpgSulphates in Coprates Catena? (EDM - Natural Colors; credits for the Additional Process. and Color.: Dr Paolo C. Fienga - Lunexit Team)109 visitenessun commentoMareKromium
(6 voti)
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Craters-Crater_Field-h1640_0000_nd3.jpgHeavily Cratered Region and Candidate Migrating Dunefields (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)83 visitenessun commentoMareKromium
(6 voti)
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Coprates_Catena-h0438_0000_nd3-00-PCF-LXTT.jpgFrame Mars Express n. h0438_0000_nd3 (natural colors - elab. Lunexit) 77 visitenessun commentoMareKromium
(6 voti)
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RupesTenuis-428-20081205-5872-6-co-01-RupesTenuis_H1.jpgNorth Polar Features: Rupes Tenuis (Natural Colors; credits: Lunar Explorer Italia)73 visiteCaption ESA:"ESAs Mars Express Orbiter imaged the snow-laden region of Rupes Tenuis on the Martian North Pole on July, 29th, 2008.
Rupes Tenuis is located at the southern edge of the Martian North Polar Cap, approx. 5500 Km North-East of the Tharsis Province.
The image shows an area located at about 81 North Lat. and 297 East Long. and has a ground resolution of approx. 41 mt/pixel. It covers an area of about 44.000 Km2 (such as almost as large as the Netherlands)".
Nota Lunexit: secondo noi, questa "immagine" (che in realt dovrebbe essere un fotomosaico) NON E' reale. L'immagine...NON E' un'immagine reale di Marte ( solo una ricostruzione virtuale, nello stile tipico della - sempre pi ambigua e sopravvalutata - ESA). MareKromium
(6 voti)
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Deuteronilus_Mensae_Region-PCF-LXTT.jpgDeuteronilus Mensae (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia70 visiteThis image shows the Deuteronilus Mensae Region on Mars, an area primarily characterized by (peri)glacial features.
It was taken on 14 March 2005 (orbit number 1483) by the High Resolution Stereo Camera (HRSC) onboard ESA's Mars Express with a ground resolution of approx. 29 mt per pixel.
The area is located on the Northern edge of Arabia Terra and borders the Southern High- and Northern Lowlands, at approx. 39° North Lat. and 23° East Long. MareKromium
(6 voti)
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Hellespontus_Region_and_Reull_Vallis.jpgHellespontus and Reull Region (MULTISPECTRUM processing, from an idea of Keith Laney)68 visitenessun commentoMareKromium
(6 voti)
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Hebes_Chasma.jpgHebes Chasma (Natural Colors + MULTISPECTRUM; credits: ESA and Lunexit)71 visiteThe Region is an "Enclosed Trough" situated in Valles Marineris, the Grand Canyon of Mars, where water is believed to have flowed.
The High Resolution Stereo Camera (HRSC) on ESA's Mars Express studied the area providing new pictorial clues to its history.
Hebes Chasma is located at approx. 1° South Lat. and 282° East Long. Image data was obtained on 16 September 2005 with a ground resolution of approx. 15 mt/pixel.
The Region is an enclosed, almost 8 Km-deep trough in the most northern part of Valles Marineris, the 3000-Km long Grand Canyon of Mars.
The steep flanks of the trough show branched incisions and small veins of rock. Below the flanks, run-off and material from larger landslides is also visible.
A flat-topped mountain is located in the centre of Hebes Chasma.
It reaches 8000 mt above the graben floor and rises to almost the same height as the plains surrounding the trough. MareKromium
(6 voti)
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