| Piú votate - Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas) |
Craters-Huygens_Crater-Rim-ESA-PCF-LXTT.jpgDrainage Channels on the Rim of Huygens Crater (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)184 visitenessun commentoMareKromium
(4 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)183 visitenessun commentoMareKromium
(4 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)71 visitenessun commentoMareKromium
(4 voti)
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Coprates_Catena-h0438_0000_nd3-00-PCF-LXTT.jpgFrame Mars Express n. h0438_0000_nd3 (natural colors - elab. Lunexit) 58 visitenessun commentoMareKromium
(4 voti)
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Ma_AdimVallis-ESA-PF.jpgMa'adim Vallis (possible Natural Colors; credits ESA - additional color. and process. Dr Paolo C. Fienga)66 visiteMars Express image of a region close to Ma’adim Vallis, one of the largest canyons on Mars. After Valles Marineris, Ma’adim Vallis is one of the largest 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 approx. 15 mt/pixel.
Ma’adim Vallis is located between the Volcanic Region of Tharsis, which harbours four volcanoes, including the largest in the Solar System, and the Hellas Planitia Impact Basin.
The canyon, about 20 Km wide and 2 Km deep, originates in the southern highlands close to the ‘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.
Nota Lunexit: a nostro avviso questa "immagine" NON E' VERA! E' un disegno. Al limite, è la trasposizione digitale di un frame RAW originale unprocessed (ma ne dubitiamo). MareKromium
(4 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)55 visiteCaption ESA:"ESA’s 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 realtà dovrebbe essere un fotomosaico) NON E' reale. L'immagine...NON E' un'immagine reale di Marte (è solo una ricostruzione virtuale, nello stile tipico della - sempre più ambigua e sopravvalutata - ESA). MareKromium
(4 voti)
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Phobos-401-20080729-5851-6-na-1a-Phobos-Flyby_H1.jpgPhobos in HR (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)55 visiteCaption ESA:"On July 23, 2008, the High Resolution Stereo Camera on board the ESA’s Mars Express took the highest-resolution full-disc image yet of the surface of the moon Phobos.
The image data were acquired from a distance of about 97 Km from Phobos' Surface, with a spatial resolution of about 3,7 mt/pixel, during orbit 5851.
These images have surpassed all previous images from other missions in continuous coverage of the illuminated surface at the highest spatial resolution of 3,7 mt/pixel".
This image has been geometrically corrected and exhibits the original illumination and photometric conditions". MareKromium
(4 voti)
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Phobos-402-20080729-5851-6-GRUNT-01-Phobos-Flyby_H1.jpgPhobos and two possible Landing Sites for "GRUNT" (natural colors; credits: Lunexit)54 visiteCaption ESA:"HRSC Stereo Channel 1 image of Phobos with a resolution of 3,7 mt/pixel at its best. The inset to the right shows the potential Landing Region and Sites for the Russia’s Phobos-Grunt sample return mission, due for launch in 2009". MareKromium
(4 voti)
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Phobos-403-20080729-5850-6-SRC-01_H1.jpgPhobos and two possible Landing Sites for "GRUNT" (natural colors; credits: Lunexit)54 visiteCaption ESA:"HRSC Super-resolution channel (SRC) image taken on July, 22, 2008 from a distance of approix. 4500 Km, showing the illuminated edge of the potential Landing Site of the Russian "Phobos-Grunt" Mission.
MareKromium
(4 voti)
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Craters-Pollack_Crater-H1201_0001_ND3_crop_wide-0.jpgPollack Crater and "White Rock" (RAW Frame; credits: ESA - Mars Express)55 visitenessun commentoMareKromium
(4 voti)
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A-h0751_0000_re2.jpgFrame Mars Express RAW n. h0751_0000_re254 visite
(4 voti)
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A-h0751_0000_gr2.jpgFrame Mars Express RAW n. h0751_0000gr254 visite
(4 voti)
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