| Piú viste - Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas) |
Craters-Hale_Crater-134-021104-0533-6-co-02.jpgHale Crater (Natural Colors; credits: G. Neukum (FU Berlin) et al. - Mars Express - DLR - ESA)84 visitenessun commento
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Reull_Vallis-ESA-2-PCF-LXTT.jpgPseudo-Lake in Reull Vallis (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)83 visiteLa "risposta" Lunexit, in Absolute Natural Colors, ad uno degli orrori più grandi "Made by ESA": un (brutto e pure - leggermente - sfuocato) Mars Express Frame, colorato in arancio-giallo, verde e azzurro (!) il quale fece gridare (i soliti tre pseudo-Ricercatori prezzolati) al "Lago di Reull" (guardate il frame che precede).
Nessun "Lago", Signori: solo un Canyon colmo di sabbie ferrose ed ossidate! Meditateci sopra...MareKromium
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L-h0513_0009_nd2-00.jpgFrame Mars Express RAW n. h0513_0009_nd281 visiteMareKromium
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NP-h1169_0000_nd2-00.jpgFrame Mars Express RAW n. h1169_0000_nd280 visiteMareKromium
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Craters-Unnamed_Crater_in_Promethei_Terra-PCF-LXTT.jpgUnnamed Crater in Promethei Terra (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)78 visitenessun commento
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Lava_Flows-Daedalia_Planum-PCF-LXTT.jpgDaedalia Planum (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)77 visitenessun commentoMareKromium
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Coprates_Catena-h0438_0000_nd3-00.jpgSulphates in Coprates Catena? (CTX Frame - Natural Colors; credits for the Additional Process. and Color.: Dr Paolo C. Fienga - Lunexit Team)76 visitenessun commentoMareKromium
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Volcanoes-Ascraeus_Mons-1-027-150304-0068-6-co-01.jpgAscraeus Mons from Mars Express (1 - ESA/ DLR/ FU Berlin - G. Neukum)75 visiteDue immagini in colori naturali del Vulcano Ascraeus Mons e dei suoi rilievi assolutamente affascinanti.
Ed eccoVi la Caption ESA originale:"This colour image shows a larger portion of the southern flank of Ascraeus Mons. The lighter, pink areas on the colour image, are clouds.
The visible lava tubes are caused by the crusting (or cooled lava) which occurs over a lava channel, a covering making the channel into a tunnel.
When lava production ceases, the tunnel empties and the roof of the tunnel falls in, making an elongated depression.
Occasionally, the depression forms a chain of small pits over an emptied lava tunnel. Pit chains and lava tunnels are common on the Martian surface and are also seen on other terrestrial planets and the Moon".
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Valles_Marineris-h0442_0008_nd3.jpgPortion of the Valles Marineris Canyon System (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga)73 visitenessun commentoMareKromium
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MaunderCrater.jpgMaunder Crater (Natural Colors + MULTISPECTRUM; credits: ESA & Lunexit)72 visiteThe above image shows the striking Maunder crater lying at approx. 50° South Lat. and 2° East Long., in the Noachis Terra Region on Mars.
The High Resolution Stereo Camera (HRSC) on ESA’s Mars Express orbiter took pictures of the Noachis Terra Region during orbits 2412 and 2467 on 29 November and 14 December 2005, respectively, with a ground resolution of approx. 15 mt/pixel.
The Sun illuminates the scene from the North-East (top left in the image).
Maunder crater, named after the British Astronomer Edward W. Maunder, is located halfway between Argyre Planitia and Hellas Planitia on the Southern Highlands of Mars.
With a diameter of 90 Km and a depth of barely 900 mt, the Crater is not one of the largest impact craters on Mars at present, but it used to be much deeper. It has since been filled partially with large amounts of material.MareKromium
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Claritas_Fossae-5-098-140904-0508-6-3d-01-ClaritasFossae_hires.jpgClaritas Fossae (5 - ESA/ DLR/ FU Berlin - G. Neukum)71 visitenessun commento
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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
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