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SOL0813-2P198554476EFFAR00P2408R1M1.jpg
SOL0813-2P198554476EFFAR00P2408R1M1.jpgPanorama - Sol 813 (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)63 visitenessun commentoMareKromium55555
(1 voti)
SOL0813-2P198554525EFFAR00P2408R1M1.jpg
SOL0813-2P198554525EFFAR00P2408R1M1.jpgPanorama - Sol 813 (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)66 visitenessun commentoMareKromium55555
(1 voti)
ESP_018469_1630_RED_abrowse.jpg
ESP_018469_1630_RED_abrowse.jpgRocky Features in Mangala Valles (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromium55555
(1 voti)
ESP_018464_2040_RED_abrowse-1~0.jpg
ESP_018464_2040_RED_abrowse-1~0.jpgMawrth Vallis (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)64 visitenessun commentoMareKromium55555
(1 voti)
PSP_001507_1400_RED_browse.jpg
PSP_001507_1400_RED_browse.jpgMantling Material (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)63 visitenessun commentoMareKromium55555
(1 voti)
ESP_018485_1765_RED_abrowse.jpg
ESP_018485_1765_RED_abrowse.jpgPeri-Equatorial Scarp and Fans (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)65 visitenessun commentoMareKromium55555
(1 voti)
ESP_018496_1510_RED_abrowse.jpg
ESP_018496_1510_RED_abrowse.jpgColumbus Crater (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)86 visitenessun commentoMareKromium55555
(1 voti)
ESP_018482_2790_RED_abrowse-01.jpg
ESP_018482_2790_RED_abrowse-01.jpgNorth Polar Layered Deposits (EDM - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)79 visite2 commentiMareKromium55555
(1 voti)
Pandora-PIA12690.jpg
Pandora-PIA12690.jpgPandora58 visiteCaption NASA:"The Cassini Spacecraft captured this close view of Saturn's moon Pandora during the Fly-By on June, 3, 2010.

Pandora is approx. 81 Km (a little mora than 50 miles) across and orbits beyond Saturn's thin F-Ring, which is shepherded by Pandora and Prometheus.
This view looks toward the Saturn-facing side Pandora. North on Pandora is up and rotated 20° to the left.

The image was taken in Visible Light with the Cassini Spacecraft narrow-angle camera. The view was obtained at a distance of approx. 101.000 Km (about 63.000 miles) from Pandora and at a Sun-Pandora-Spacecraft, or Phase, Angle of 28°.
Image scale is 603 meters (1980 feet) per pixel".
MareKromium55555
(1 voti)
Craters-Unnamed_Crater-PIA13309.jpg
Craters-Unnamed_Crater-PIA13309.jpgUnnamed Crater in Utopia Planitia (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)64 visiteA small Channel enters this Unnamed Crater in Arabia Terra. There appears to be a small Fan - or Delta - formed where the Channel meets the Crater Floor.

Orbit Number: 37714
Latitude: 34,823° North
Longitude: 356,522° East
Instrument: VIS
Captured: 2010, June, 15th
MareKromium55555
(1 voti)
Windstreaks-PIA13292.jpg
Windstreaks-PIA13292.jpgWindstreaks in Tharsis (Natural Colors; credits: Dr Paolo C. Fienga - Lunexit Team)65 visiteThis VIS image shows are region of lava covered plains east of Olympus Mons. Winds are common in the area and have created Windstreaks downwind of Craters in the Region and on the Lava Flows.

Orbit Number: 37693
Latitude: 22,596° North
Longitude: 240,567° East
Instrument: VIS
Captured: 2010, June, 13th
MareKromium55555
(1 voti)
PSP_003180_0945_RED_abrowse-00.jpg
PSP_003180_0945_RED_abrowse-00.jpgSouth Polar Dust Fans (CTX Frame - Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)62 visiteDuring the long and dark night of Martian Winter at the South Pole, CO2 in its solid form ("dry ice") accumulates and forms the so-called "Seasonal South Polar Cap". Afterwards, as the Sun comes up in the Spring, the ice evaporates in a complex way.
This observation shows Dark Dust being blown across the Seasonal South Polar Cap. The dust comes from the Surface beneath the ice: it either starts at spots bare of ice, or it's possible that it's lofted from below the ice in geyser-like plumes.

Local winds blow the dust from its source, forming a long Fan. When the wind changes direction, a new Fan is formed pointing in the new direction In this image we can see that the wind has blown in a number of directions.
These data will be used to study - among other things - the Weather Patterns near the South Pole.
MareKromium55555
(1 voti)
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