Mars from Orbit (from July 2009)
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Aeolian_Features_and_Yardangs-Daedalia_Planum-PIA13846-PCF-LXTT-2.jpgFeatures of Daedalia Planum (RED Filters ON - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)362 visitenessun commentoMareKromium
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Arabia_Terra-PIA08730-2.jpgFeatures of Arabia Terra (Original NASA/2001 Mars Odyssey Orbiter b/w Frame))54 visiteImage information: VIS instrument;
Latitude: 16,7° North;
Longitude: 350,0° East;
Resolution: 18 meter/pixel.
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Arabia_Terra-PIA08730-2.jpgFeatures of Arabia Terra (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 187 visiteImage information: VIS instrument;
Latitude: 16,7° North;
Longitude: 350,0° East;
Resolution: 18 meter/pixel.MareKromium
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Arabia_Terra-PIA13381.jpgUnnamed Drainage Channels in Arabia Terra (Enhanced Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)168 visitenessun commentoMareKromium
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Aram_Chaos-PIA13744.jpgFeatures of Aram Chaos (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)124 visitenessun commentoMareKromium
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Aram_Chaos-R2200155-10-PCF-LXTT.jpgFeatures of Aram Chaos (Enhanced Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team) 185 visitenessun commentoMareKromium
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ArcadiaPlanitia-PIA12215.jpgFresh Impact in Arcadia Planitia (Natural Colors; credits: Lunexit)55 visiteThe team operating the Context Camera (CTX) aboard NASA's Mars Reconnaissance Orbiter frequently discovers new dark spots on Mars that, upon closer examination, turn out to be brand new impact craters. Sometimes only a single crater is present, but often there is a cluster of several craters.
Depending on the patterns and size, Crater Clusters are interpreted as indicating that the incoming meteorite broke apart before it hit the Surface.
In some cases, clusters could be formed by ejecta from other, larger impact craters.
Shown above are subframes of two Context Camera images of terrain in Western Arcadia Planitia (near 46,7° North Latitude and 183,2° West Longitude). Each covers an area about 6,5 Km (about 4 miles) across.MareKromium
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Argyre_Basin-20080213a-PCF-LXTT.jpgFeatures of Argyre Basin (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)68 visitenessun commentoMareKromium
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Argyre_Planitia-PIA14043-PCF-LXTT.jpgGullies in Argyre Planitia (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)218 visitenessun commentoMareKromium
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Argyre_Planitia-PIA14773-PCF-LXTT.jpgUnnamed Crater with Gullies in Argyre Planitia (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)139 visiteOrbit Number: 42770
Latitude: 36,424° South
Longitude: 316,348° East
Instrument: VIS
Captured: August, 5th, 2011
Mars Local Time (M.L.T.): 22:44 (Late Evening Hours)
MareKromium
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Arsia_Chasmata-PIA13499.jpgArsia Mons Chasmata (Absolute Natural Colors; additional process.: Dr Paolo C. Fienga - Lunexit Team)101 visitenessun commentoMareKromium
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Ascraeus_Mons-PIA13209.jpgPortion of the N/W Flank of Ascraeus Mons (Enhanced and Saturated Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)59 visitenessun commentoMareKromium
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