Mars from Orbit (from July 2009)
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Chaotic_Terrain-Aram_Chaos-PIA08760-01.jpgFeatures of Aram Chaos (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 155 visiteImage information: VIS instrument;
Latitude: 3,8° North;
Longitude: 339,0° East;
Resolution: 18 meter/pixel.MareKromium
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Chaotic_Terrain-Aram_Chaos-PIA14149-PCF-LXTT.jpgAram Chaos (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)243 visitenessun commentoMareKromium
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Chaotic_Terrain-Aureum_Chaos-PIA07931-PCF-LXTT-01.jpgFeatures of Aureum Chaos (Extremely Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)184 visiteNote: the THEMIS VIS camera is capable of capturing color images of the Martian Surface using 5 different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, 3 of the 5 filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image.
These 3 images are then combined to produce a full color, single image BUT, since the THEMIS color filters DO NOT span the full range of colors seen by the human eye, a color THEMIS image DOES NOT represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the 3-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. The long edges of THEMIS color images typically contain color artifacts that do not represent or imply actual Surface Variations.
Image information: VIS instrument;
Latitude 3,6° South;
Longitude 332,9° East (such as 27,1° West);
Resolution: 35 meter/pixel.MareKromium
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Chaotic_Terrain-Aureum_Chaos-PIA07932-PCF-LXTT.jpgFeatures of Aureum Chaos (Extremely Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)184 visiteNote: the THEMIS VIS camera is capable of capturing color images of the Martian Surface using 5 different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, 3 of the 5 filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image.
These 3 images are then combined to produce a full color, single image BUT, since the THEMIS color filters DO NOT span the full range of colors seen by the human eye, a color THEMIS image DOES NOT represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the 3-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. The long edges of THEMIS color images typically contain color artifacts that do not represent or imply actual Surface Variations.
Image information: VIS instrument;
Latitude 3,6° South;
Longitude 332,9° East (such as 27,1° West);
Resolution: 35 meter/pixel.MareKromium
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Chaotic_Terrain-Aureum_Chaos-PIA14987-PCF-LXTT.jpgFeatures of Aureum Chaos (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 174 visiteOrbit Number: 43169
Latitude: 4,036° South
Longitude: 333,407° East
Instrument: VIS
Captured: September, 7th, 2011
Mars Local Time (M.L.T.): 18:50 (Late Afternoon)
MareKromium
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Chaotic_Terrain-Aurorae_Chaos-PIA14376-PCF-LXTT.jpgFeatures of Aurorae Chaos (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)166 visitenessun commentoMareKromium
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Chaotic_Terrain-Avernus_Chaos-PIA08719-00.jpgFeatures of Avernus Chaos (Original NASA/JPL/ASU b/w Frame)53 visiteImage information: VIS instrument;
Latitude: 1,3° South;
Longitude: 173,4° East;
Resolution: 18 meter/pixel.
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Chaotic_Terrain-Avernus_Chaos-PIA08719-01.jpgFeatures of Avernus Chaos (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 155 visiteImage information: VIS instrument;
Latitude: 1,3° South;
Longitude: 173,4° East;
Resolution: 18 meter/pixel.MareKromium
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Chaotic_Terrain-Cerberus_Fossae.jpgChaotic Terrain in Cerberus Fossae (Original NASA/JPL/ASU b/w Frame)86 visiteNella Regione Marziana conosciuta con il tenebroso nome di "Cerberus Fossae" possiamo vedere, grazie a questa splendida 'veduta orbitale' ottenuta dalla Sonda NASA "2001 - Mars Odyssey", un terreno ricco di intriganti e variegati rilievi.
Qualche cratere relativamente recente (che reca segni di wind-streaks scuri) e qualcuno più antico e semi-sepolto; delle colline che sembrano poggiare sopra un "basamento" e poi - forse una delle caratteristiche più inquietanti di questo scorcio di Marte - dei profondi e scoscesi crepacci frastagliati.
Questo tipo di zona viene definito "chaos" e si tratta di un'area che è stata - letteralmente - privata di sostegno sotterraneo e che quindi è "crollata su sè stessa" (---> "Chaos" is typically interpreted to be a collapse terrain; it is the blocky landscape after the transport and removal of subsurface support).
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Chaotic_Terrain-Elysium_Chaos-PIA08641-00.jpgChaotic Terrain in Elysium Planitia (1 - Original NASA/JPL/ASU b/w Frame)54 visiteImage information: VIS instrument;
Latitude: - 0,8° North;
Longitude: 172,5° East;
Resolution: 18 meter/pixel.
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Chaotic_Terrain-Elysium_Chaos-PIA08641-01.jpgChaotic Terrain in Elysium Planitia (1 - Absolute Natural Colors; credits for the additoonal process. and color.: Dr Paolo C. Fienga - Lunexit Team)143 visiteImage information: VIS instrument;
Latitude: - 0,8° North;
Longitude: 172,5° East;
Resolution: 18 meter/pixel. MareKromium
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Chaotic_Terrain-Elysium_Chaos-PIA08641-02.jpgChaotic Terrain in Elysium Planitia (2 - Original NASA/JPL/ASU b/w Frame)55 visiteImage information: VIS instrument;
Latitude: - 0,8° North;
Longitude: 172,5° East;
Resolution: 18 meter/pixel.
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