| Piú viste - Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas) |
Tiu_Valles-ESA-PCF-LXTT.jpgTiu Valles (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)70 visiteThis image taken by the High Resolution Stereo Camera (HRSC) on board Mars Express shows the mouth of the Tiu Valles Channel System on the Red Planet. The picture was taken in orbit 3103 on 10 June 2006 with a ground resolution of approx. 16 mt/pixel. Visible in the lower part of the image are remnants of a once 'Streamlined' Island. The upper part of the scene covers the mouth of the Tiu Valles nearly in its entire width, approx. 55 Km.
Its winding, meandering Ridges, bound by depressions are eye-catching. The processes that formed these odd structures are still unknown. Possibly, during flooding events, water or water-rich surface layers came in contact with lava from the surrounding areas, which then might have led to the formation of these mysterious ridges.
The Region is located at approx. 27° North Lat. and 330° East Long. The Sun illuminates the scene from the North West, the lower left-hand side in the image. MareKromium
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Volcanoes-Arsia_Mons-Eruption-06.gifArsia Mons is erupting? (a GIF-Movie in processed Natural Colors by Dr Marco Faccin - Lunexit Team)69 visiteSolo un'annotazione "tecnica": notate come l'Atmosfera di Marte (tutt'altro che impercettibile ed ultra-sottile...) si evidenzia sul bordo del Pianeta colorandosi, di fotogramma in fotogramma, dello stesso colore della Dominante propria del Filtro impiegato.
Un altro straordinario Lavoro del nostro Marco Faccin, che ringraziamo di Cuore!MareKromium
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MA_ADIM_VALLIS-440-20090629-6393-6-co-01_H1-1.jpgProximities of Ma'adim Vallis (Natural Colors; credits: ESA)69 visiteCaption ESA:"Mars Express image of a Region close to Ma’adim Vallis, one of the largest - after Vallis Marineris - 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 15 mt/pixel.
Ma’adim Vallis is located between the Volcanic Province of Tharsis, which harbours 4 volcanoes, including the largest in the Solar System, and the Hellas Planitia Impact Basin.
The canyon, approx. 20 Km wide and 2 Km deep, originates in the Southern Highlands close to the so-called ‘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".MareKromium
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Aeolian_Features-Windstreaks-h0165_0068_nd3-PCF-LXTT.jpgWindstreaks (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)69 visitenessun commentoMareKromium
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IaniChaos-ESA-PF.jpgIani Chaos (possible Natural Colors; credits ESA - additional color. and process. Dr Paolo C. Fienga)68 visiteIani Chaos on Mars, an area where Light Toned Deposits, or LTD, are known to be present. An analysis of data and images from Mars Express suggests that several LTD, some of the least understood structures on Mars, were formed when large amounts of groundwater burst on to the Surface. Scientists propose that groundwater had a greater role in shaping the Martian Surface than previously believed, and may have sheltered primitive life forms as the Planet started drying up.
This image was obtained with the High Resolution Stereo Camera on board ESA’s Mars Express Spacecraft.
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
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Valles_Marineris-h0471_0001_nd3.jpgPortion of the Valles Marineris Canyon System (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga)68 visitenessun commentoMareKromium
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Claritas_Fossae-1-029-290304-0068-6-co-02.jpgClaritas Fossae (1 - ESA/ DLR/ FU Berlin - G. Neukum)67 visiteCaption ESA originale:"These Mars Express images show Claritas Fossae, an ancient tectonic region on Mars, west of Solis Planum, a tectonic and volcanic area south-east of the Tharsis volcano group.
The images were taken by the High-Resolution Stereo Camera (HRSC) on Mars in orbit 68 from an altitude of 271 Km. The images are centred at 255,7° East and 30,9° North. North is on the left".
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Cydonia_Region-h3253_0000_s12-2.jpgDo you recognize this place? (natural colors; credits: Dr G. Barca & Lunexit)67 visiteUn semplice "Space-quiz": che Regione è quella che vedete in questo frame? Le Vostre risposte - motivate - possono essere inserite nei "Commenti".MareKromium
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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)67 visitenessun commentoMareKromium
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NP-h1169_0000_p12-00.jpgFrame Mars Express RAW n. h1169_0000_p1266 visiteMareKromium
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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
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Aeolian_Features-Windstreak-h0232_0000_nd3-01-PCF-LXTT.jpgWindstreaks (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)64 visitenessun commentoMareKromium
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