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Inizio > MARS > Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas)

Piú viste - Mars through Mars Express (ESA - Original Raw Frames & Orbital Panoramas)
Kasei_Valles_and_Sacra_Fossae-448-20091007-6241-6-co-01_H1.jpg
Kasei_Valles_and_Sacra_Fossae-448-20091007-6241-6-co-01_H1.jpgKasei Valles and Sacrae Fossae (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)56 visiteCaption ESA:"Mars Express flew over the boundary between Kasei Valles and Sacra Fossae and imaged the Region, acquiring spectacular views of the Chaotic Terrain in the area.
The image is centred at about 12° North Latitude and 285° East Longitude and have a ground resolution of approx. 21 mt/pixel.
They cover about 225 x 95 Km (or 21.375 sq Km); an area roughly half the size of the Netherlands".
MareKromium
Claritas_Fossae-4-096-140904-0508-6-co-01-ClaritasFossae_hires.jpg
Claritas_Fossae-4-096-140904-0508-6-co-01-ClaritasFossae_hires.jpgClaritas Fossae (4 - ESA/ DLR/ FU Berlin - G. Neukum)55 visiteCaption ESA originale:"The lava blankets of the Solis Planum area cover the eastern parts of the older Claritas Fossae ridge and surround some of the higher ground. The geological history of this region can be reconstructed by analysing the layers of tectonic grabens, impact craters, volcanic features and even small valley networks. The complexity of Claritas Fossae Region suggests that some of the events took place at the same time. Furthermore, the detailed view of the large southern impact crater shows patches of dark material which are located near the central and marginal parts of the impact crater floor. This material may be of volcanic origin".
A-h0751_0000_bl2.jpg
A-h0751_0000_bl2.jpgFrame Mars Express RAW n. h0751_0000_bl255 visite
Craters-Pollack_Crater-H1201_0001_ND3_crop_wide-0.jpg
Craters-Pollack_Crater-H1201_0001_ND3_crop_wide-0.jpgPollack Crater and "White Rock" (RAW Frame; credits: ESA - Mars Express)55 visitenessun commentoMareKromium
Phobos-401-20080729-5851-6-na-1a-Phobos-Flyby_H1.jpg
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
RupesTenuis-428-20081205-5872-6-co-01-RupesTenuis_H1.jpg
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
South_Polar_Regions-Rupes_Tenuis-ESA-PF.jpg
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
Volcanic_Features-Biblis_Patera-213-190705-1034-6-nd-01-BiblisP_H.jpg
Volcanic_Features-Biblis_Patera-213-190705-1034-6-nd-01-BiblisP_H.jpgBiblis Patera (EDM - credits: ESA/DLR/FU Berlin (G. Neukum))54 visiteOriginal ESA caption:"This image taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, shows the Biblis Patera Volcano, located in the Western part of the Tharsis rise on Mars.
The HRSC obtained this image on 8 November 2004 during orbit 1034 with a ground resolution of approx. 10,8 mt per pixel. Its shows the region of Biblis Patera at approx. 2,0° North and 236,0° East.
North is to the right".
A-h0751_0000_gr2.jpg
A-h0751_0000_gr2.jpgFrame Mars Express RAW n. h0751_0000gr254 visite
A-h0751_0000_re2.jpg
A-h0751_0000_re2.jpgFrame Mars Express RAW n. h0751_0000_re254 visite
B-h0032_0000_bl3-00.jpg
B-h0032_0000_bl3-00.jpgFrame Mars Express RAW n. h0032_0000_bl354 visite
Craters-Pollack_Crater-H1201_0001_ND3_crop_wide-3.jpg
Craters-Pollack_Crater-H1201_0001_ND3_crop_wide-3.jpgPollack Crater and "White Rock" (Natural Colors - Tri-Chromatic Version; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)54 visitenessun commentoMareKromium
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