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SOL1069-3.jpgSalts and Sulphates - Sol 1069 (possible True Colors; credits: Dr G. Barca & Lunexit)55 visitenessun commentoMareKromium
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SOL1096-3.jpgRover Tracks, Salt and Sulphates - Sol 1096 (possible True Colors; credits: Dr G. Barca & Lunexit)55 visitenessun commentoMareKromium
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SOL1113-3.jpgLook who's there... (mgnf and possible True Colors - credits: Dr G. Barca & Lunexit) - Sol 111355 visitenessun commentoMareKromium
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SOL1131-3.jpgBoulders - Sol 1131 (possible True Colors; credits: Dr G. Barca & Lunar Explorer Italia)55 visitenessun commentoMareKromium
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SOL422-MF1.jpgAntenna MAST and orange Surface - Sol 422 (possible True Colors; credits: Dr M. Faccin & Lunar Explorer Italia)55 visitenessun commentoMareKromium
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SOL1172-4.jpgDistant Hills - Sol 1172 (possible True Colors; credits: Dr G. Barca & Lunar Explorer Italia)55 visitenessun commentoMareKromium
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Craters-Unnamed_Crater-Terra_Sabaea-PCF-LXTT.jpgUnnamed Crater in Terra Sabaea (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)55 visitenessun commentoMareKromium
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Tethys-PIA10527.jpgThe Odyssey on Tethys...55 visiteCaption NASA:"This Cassini Spacecraft image provides a view of the southern portion of Tethys' Trailing Hemisphere.
Prominent features include the huge canyon, Ithaca Chasma, approximately centered in this view, as well as Demodocus and Telemus, large basins just to the right of the rift.
Features on Tethys are named for characters in Homer's Odyssey.
The image was taken in visible green light with the Cassini Spacecraft narrow-angle camera on Oct. 10, 2008 at a distance of approx. 417.000 Km (about 259.000 miles) from Tethys and at a Sun-Tethys-Spacecraft, or Phase, angle of 55°.
Image scale is roughly 2 Km (a little more than 1 mile) per pixel".MareKromium
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PSP_004078_2015_RED_browse-01.jpgLayered Rocks within Becquerel Crater (enhanced natural colors; credits: Lunar Explorer Italia)55 visiteRhythmic bedding in sedimentary bedrock within Becquerel Crater on Mars is suggested by the patterns in this image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
Three dimensional analysis based on stereo pairs of images confirmed the regularity of repetition in the thickness of the beds. In the left half of this image, some of the rhythm is apparent as a series of bundles of about 10 individual layers per bundle. By corresponding to a known 10-to-one pattern in changes in the tilt of Mars' Rotation Axis, this pattern suggests the periodicity in the rock layers results from cyclical changes in the Planet's tilt.
This view covers an area about 1150 meters (0,7 miles) wide. Individual layers in the scence average 3,6 meters (12 feet) thick. The view is presented in enhanced natural colors emphasizing the differing compositions of surface material. Sand trapped in relative low points in the terrain appears grey-blueish. Sedimentary rocks appear brown.
Faulting apparent in the image suggests that the deposits are hardened rock, not softer material. Tilting of the layers in different ways and the surface topography made the three-dimensional analysis necessary for determining the thickness of layers.
This image is a portion of the HiRISE image catalogued as PSP_004078_2015, taken on June 10, 2007.
The location of the imaged area is at 22° North Latitude, 352° East Longitude, within the Arabia Terra Region.MareKromium
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SOL1387-1.jpgMineral Diversity - Sol 1387 (possible True Colors; credits: Dr G. Barca)55 visitenessun commentoMareKromium
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Titan-N00124860.jpgTitan in possible True Colors (credits by Lunar Explorer Italia)55 visiteCaption NASA:"N00124860.jpg was taken on December 05, 2008 and received on Earth December 06, 2008. The camera was pointing toward TITAN that, at the time, was approximately 176.792 Km away.
The image was taken using the CL1 and CB3 filters". MareKromium
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OPP-SOL1716-5.jpgPaving and Pebbles - Sol 1716 (possible True Colors; credits: Dr G. Barca & Lunexit)55 visitenessun commentoMareKromium
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