| Ultimi arrivi - Mars from Orbit (from July 2009) |
Trough-Patapsco_Vallis-PIA12455.jpgZig-Zagging Trough (Natural - but enhanced - Colors; credits: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromiumFeb 07, 2010
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Craters-Arkhangelsky_Crater-20100202a.jpgSmall Dunefield in Arkhangelsky Crater (Saturated Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team) 58 visitenessun commentoMareKromiumFeb 02, 2010
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Yardangs-20100129a.jpgYardangs in Zephyria Planum (Absolute Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)59 visitenessun commentoMareKromiumFeb 02, 2010
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Slope_Streaks-Terra_Sabaea-PIA12430.jpgUnnamed Crater in Terra Sabaea (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)81 visitenessun commentoMareKromiumGen 28, 2010
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Channels-Nirgal_Vallis-20100107a.jpgFeatures of Nirgal Vallis (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)58 visitenessun commentoMareKromiumGen 28, 2010
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Channels-Naktong_Vallis-PIA12419-PCF-LXTT.jpgNaktong Vallis, on Martian Equator (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)59 visitenessun commentoMareKromiumGen 28, 2010
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Aeolian_Features-Yardangs_in_Tharsis_Region-20100126a.jpgWindwork in Tharsis (False Colors; credits: Dr Paolo C. Fienga - Lunexit Team)61 visitenessun commentoMareKromiumGen 26, 2010
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Volcanoes-AlbaMons-20100108a-1.jpgFlows and Collapse Pits on the S/W Flank of Alba Mons (Strongly Enhanced Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)61 visitenessun commentoMareKromiumGen 24, 2010
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Channels-Hephaestus_Fossae-20100111a.jpgHephaestus Fossae (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)58 visiteThe Channels visible in this VIS image are called "Hephaestus Fossae" and were most likely formed by Lava Flows and Eolian Erosion, rather than Water Erosion.
MareKromiumGen 21, 2010
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Craters-Unnamed_Crater-PIA12431.jpgDunefield (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromiumGen 21, 2010
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Channels-Patapsco_Vallis-20100113a.jpgPatapsco Vallis and Elysium Fossae (Enhanced Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)83 visiteThis VIS image shows two different types of "Linear Depressions".
The wide depression on the left of the frame is a wide trough known as "Elysium Fossae", which most likely formed due to tectonic activity.
The Fossae is probably bounded on both sides by faults.
The narrow depression on the right of the frame, instead, is a Lava Channel called Patapsco Vallis.
This Channel has Lava Flows on both sides which were probably formed by over spilling of lava as it flowed down the Channel.
Both these features are located East of Elysium Mons.MareKromiumGen 21, 2010
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Gullies-ArgyrePlanitia-PIA12408.jpgDeep Gullies on the Western Rim of Argyre Basin (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)59 visiteThe Gullies seen in this VIS image are located on the Western Rim of the Argyre Basin.
Coord.: 47,6 ° South Latitude and 305,2° East Longitude
Resolution: approx. 40 meter/pixel.MareKromiumDic 23, 2009
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