| Piú votate - Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas) |
CR-h0550_0000_nd3-01-PCF-LXTT.jpgFrame h0550_0000_nd3-01 - Rayed Crater and Collapse Features (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)228 visitenessun commentoMareKromium
(4 voti)
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Tiu_Valles-ESA-PCF-LXTT.jpgTiu Valles (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)81 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
(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)87 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, č la trasposizione digitale di un frame RAW originale unprocessed (ma ne dubitiamo). MareKromium
(4 voti)
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SouthPole-MG_SP_Fig02a_H.jpgThe South Pole of Mars (natural colors; credits: Lunexit)65 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
(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)64 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)64 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-404-20080729-5181-6-an-01-Phobos-Flyby_2_H1.jpgPhobos in 3D (red-cyan anaglyph)64 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
(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)63 visitenessun commentoMareKromium
(4 voti)
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B-h0032_0000_bl3-00.jpgFrame Mars Express RAW n. h0032_0000_bl364 visite
(4 voti)
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Hellas_Planitia-H0572_0000_ND2_H-PCF-LXTT.jpgFrame H0572_0000_ND2: Hellas Planitia Region212 visiteCaption ESA:"The HRSC on board ESA's Mars Express Spacecraft obtained this image on July, 1st, 2004 during orbit 572 with a ground resolution of approx. 45,1 mt per pixel.
The scene shows a portion of Hellas Planitia, a Region which is about 234 Km wide in the North, 345 Km in the South, about 898 Km in length, and centred at approx. 89° East Long. and 29° South Lat.
This image represents an area on the Northern Eastern Rim of Hellas Planitia, also known as the Hellas Impact Basin in Mars's Southern Hemispere. The Basin is thought to have formed around 3900 Million Years ago in a single massive impact".MareKromium
(3 voti)
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Hesperia_Planum-224co01_H-PCF-LXTT.jpgHuge Massif in Hesperia Planum241 visiteCaption ESA:"The HRSC on ESA's Mars Express obtained this image on June, 13th, 2004, during orbit 506 with a ground resolution of approx. 37,6 mt per pixel.
This view shows a portion of the Hesperia Planum Region, containing the Massif, and located at approx. 30,3° South Lat. and 97,8° East Long.".MareKromium
(3 voti)
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Unusually_looking_Surface_Feature-Pit-h1323_0000_nd3.jpgExtremely unusually-looking Surface Feature (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)114 visitenessun commentoMareKromium
(3 voti)
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