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Ultimi arrivi - Mars from Orbit (from July 2009)
Chaotic_Terrain-Memnonia-PIA08104-2.jpg
Chaotic_Terrain-Memnonia-PIA08104-2.jpgChaotic Terrain between Memnonia Fossae and Elysium Planitia (2 - Original NASA/JPL/ASU b/w Frame)55 visitenessun commentoApr 27, 2006
Chaotic_Terrain-Memnonia-PIA08104-1.jpg
Chaotic_Terrain-Memnonia-PIA08104-1.jpgChaotic Terrain between Memnonia Fossae and Elysium Planitia (1 - Original NASA/JPL/ASU b/w Frame)56 visiteCaption NASA originale:"These arcuate fractures are located on the margin between Memnonia Fossae and Elysium Planitia".

Image information: VIS instrument;
Latitude: 1,4° North;
Longitude: 177,5° East;
Resolution: 18 meter/pixel.
Apr 27, 2006
Craters-Crater_Cluster-PIA08088-1.jpg
Craters-Crater_Cluster-PIA08088-1.jpgSeeps, Dust and Landslides in a Crater Cluster (Original NASA/2001 Mars Odyssey Orbiter b/w Frame)56 visiteImage information: VIS instrument;
Latitude: 18,8° North;
Longitude: 18,5° East;
Resolution: 18 meter/pixel.

Apr 22, 2006
Hills-Knob-Elysium_Planitia-PIA08079-00.jpg
Hills-Knob-Elysium_Planitia-PIA08079-00.jpgBizarre "Knob" in Elysium Planitia (Original NASA/JPL/ASU b/w Frame)54 visiteImage information: VIS instrument;
Latitude: 1,1° South;
Longitude: 156,0° East;
Resolution: 18 meter/pixel.
Apr 18, 2006
Candor_Chasma-03.jpg
Candor_Chasma-03.jpgCandor Chasma from MGS and 2001 Mars Odyssey83 visiteCaption originale:"The 2001 Mars Odyssey Spacecraft includes an imaging device called THEMIS which scans strips of Mars in various wavelengths. Although numerous excellent images have been returned, unfortunately quirks and light leak defects in the camera system prevent straightforward registration of images obtained in different wavelengths. The first RGB color image released from Mars Odyssey is shown in the context of a color image from Mars Global Surveyor with a faked green channel. The THEMIS image appears too dark and saturated to me but I have preserved the color balance as released. Detailed criticism must be qualified by knowledge of the heroic measures taken to 'rescue' this RGB color image. The dark gray terrain in the valley floor shows as brownish to olive greenish in the closeup, and an orange region in the lower right is seen as the edge of a larger reddish area in the central interior of Candor Chasma".Apr 09, 2006
Chasmas-Echus_Chasma-PIA08022-01.jpg
Chasmas-Echus_Chasma-PIA08022-01.jpgDust Avalanches in Echus Chasma (2)61 visitenessun commentoApr 01, 2006
Chasmas-Echus_Chasma-PIA08022-00.jpg
Chasmas-Echus_Chasma-PIA08022-00.jpgDust Avalanches in Echus Chasma (1)56 visiteImage information: VIS instrument;
Latitude: 3,6° North;
Longitude: 280,9° East;
Resolution: 18 meter/pixel.
Apr 01, 2006
Aeolian_Features-DD_Tracks-PIA02185-1.jpg
Aeolian_Features-DD_Tracks-PIA02185-1.jpgDeep Dust Devil Tracks between Brashear and Ross Crater (Original NASA/JPL/ASU b/w Frame)62 visiteCaption originale:"Dust Devil activity in this region between Brashear and Ross Craters is very common.
Large areas full of DD tracks surround the South Polar Region of Mars.

Image information: VIS instrument;
Latitude: - 55,2° North;
Longitude: 244,2° East;
Resolution: 17 meter/pixel.
Feb 18, 2006
Chaotic_Terrain-Aram_Chaos-PIA02175-00.jpg
Chaotic_Terrain-Aram_Chaos-PIA02175-00.jpgFeatures of Aram Chaos (Original NASA/JPL/ASU b/w Frame)58 visiteCaption NASA:"This image of part of Aram Chaos shows two different surface textures with distinctly different brightnesses. The lighter layer appears to be on top (therefore younger) than the darker surface".

Image information: VIS instrument;
Latitude: 2,1° North;
Longitude: 338,7° East;
Resolution: 17 meter/pixel.
Feb 16, 2006
Coprates_Chasma-PIA02173-00.jpg
Coprates_Chasma-PIA02173-00.jpgFeatures of Coprates Chasma (Original NASA/2001 Mars Odyssey Orbiter b/w Frame) 56 visiteImage information: VIS instrument;
Latitude: - 14,8° North;
Longitude: 304,3° East;
Resolution: 17 meter/pixel.

Feb 11, 2006
South_Polar_Regions-Clouds-PIA02171-2.jpg
South_Polar_Regions-Clouds-PIA02171-2.jpgClouds (RAW and b/w NASA Original Frame)56 visiteIn questa immagine si possono vedere delle sottili (quasi trasparenti...) formazioni nuvolose che sovrastano le Regioni Presso-Sud Polari di Marte. L'evidente sottigliezza delle nuvole è indicativa della circostanza per cui esse dovrebbero essere composte in larga prevalenza da ghiaccio d'acqua. Da ricordare, quindi, che le formazioni nuvolose "spesse", su Marte, sono invece prevalentemente costituite da polveri.

Image information: VIS instrument;
Latitude: 86,7° South;
Longitude: 212,3° East;
Resolution: 17 meter/pixel.
Feb 11, 2006
Craters-Holden_Crater-PIA03694-2.jpg
Craters-Holden_Crater-PIA03694-2.jpgDeposits inside Holden Crater (2)55 visitenessun commentoGen 25, 2006
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