Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas)
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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
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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
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Phobos-404-20080729-5181-6-an-01-Phobos-Flyby_2_H1.jpgPhobos in 3D (red-cyan anaglyph)54 visiteCaption ESA:"On July 23, 2008, the High Resolution Stereo Camera on board ESA’s Mars Express took the highest-resolution full-disc image yet of the surface of the moon Phobos.
This image data was acquired from a distance of about 97 Km with a spatial resolution of about 3,7 m/pixel".MareKromium
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Phobos-405-N-High_Res-ME_full-00.jpgPhobos from Mars Express (Original ESA HR-RAW Frame)346 visitenessun commento
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Phobos-406-Mars_Express-stereoME_full.jpgPhobos from Mars Express (HR and Stereo View)184 visitePhobos in versione "stereo", ripreso da una distanza di circa 200 Km dalla Sonda Europea Mars Express. Sulla Sn dell'immagine si può vedere molto bene il famoso "Stickney Crater", di oltre 10 Km di diametro.
Notevole il quantitativo di crateri e crepacci visibili che caratterizza l'intera superficie di questa Luna Marziana e che ci racconta, in play-back, di un passato turbolento.
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PrometheiPlanum.jpgPromethei Terra (Natural Colors + MULTISPECTRUM; credits: ESA & Lunexit)53 visitePromethei Planum, an area seasonally covered with layer of ice more than 3500 mt thick layer of ice in the Martian South Polar Region, was the subject of the High Resolution Stereo Camera’s focus on 22 September 2005 as Mars Express was in orbit above the Red Planet.
Promethei Planum lies at approx. 76° South Lat. and 105° East Long.
An approx. 100 Km-large and 800 mt-deep impact crater is visible in the Northern part of the image. The crater’s interior is partly covered in ice.
In the centre of the image are structures that may have been created by basaltic lava flow from a volcano. This area is covered in ice. The dark dunes towards the bottom of the image are most likely made up of dust originating from this lava flow or volcanic ash.
A broad sheet of ice, which is an extension of the South Polar Ice Cap is located South of the lava flow. The steep flanks clearly show white, clean ice. The thickness of the ice is between 900 and 1100 mt.MareKromium
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Reull_Vallis-ESA-1-PCF-LXTT.jpgPseudo-Lake in Reull Vallis (Absurde Colors; credits: ESA/DLR/FU Berlin, Dr G. Neukum)97 visite...senza parole...MareKromium
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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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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
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SouthPole-MG_SP_Fig02a_H.jpgThe South Pole of Mars (natural colors; credits: Lunexit)54 visiteCaption ESA:"This is a mosaic of images taken by the Mars Express’s Visible and Infrared Mineralogical Mapping Spectrometer, OMEGA.
It shows the Residual South Polar Cap at the end of Northern Winter on the Red Planet. The cap appears clearly asymmetric, its centre being displaced by 3° from the Geographic Pole".MareKromium
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South_Polar_Regions-Rupes_Tenuis-ESA-PF.jpgRupes Tenuis (possible Natural Colors; credits ESA - additional color. and process. Dr Paolo C. Fienga)55 visiteESA’s Mars Express orbiter imaged the snow-laden Region of Rupes Tenuis on the Martian North Pole on 29 July 2008.
Rupes Tenuis is located at the Southern Edge of the Martian North Polar Cap, approx. 5500 Km northeast of the Tharsis Volcanic Region.
The images are at about 81° north and 297° east and have a ground resolution of approx. 41 mt/pixel. They cover an area of about 44.000 square/Km, almost as large as the Netherlands.
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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South_Polar_Regions-h0231_0000_nd3-01.jpgFrame Mars Express n. h0231_0000_nd3 (natural colors - elab. Lunexit)53 visite
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