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OPP-SOL1457-1~0.jpg
OPP-SOL1457-1~0.jpg"Shedding" Surface... - Sol 1457 (Superdefinition + MULTISPECTRUM; credits: Dr G. Barca & Lunexit)58 visiteUn pizzico di ironia per un rilievo superficiale indefinibile (to shed ----> cambiare pelle, rinnovare il pelo).MareKromium
Seeps-MedusaeFossae.gif
Seeps-MedusaeFossae.gifSeepage in Medusae Fossae (GIF-Movie; credits for the additional proecss.: Mars Unearthed)58 visitenessun commentoMareKromium
The_Rings-PIA10426.jpg
The_Rings-PIA10426.jpgThe C-Ring and the Upper Atmosphere of Saturn (MULTISPECTRUM-2; credits: Lunexit)58 visiteCaption NASA:"Saturn's C-Ring emerges from behind the Planet's hazy limb. This view looks toward the sunlit side of the Rings from about 15° below the Ring-Plane.

The image was taken in visible light with the Cassini Spacecraft narrow-angle camera on June 17, 2008. The view was obtained at a distance of approx. 937.000 Km (such as about 582.000 miles) from Saturn.
Image scale is roughly 5 Km (a little more than 3 miles) per pixel".
MareKromium
PSP_007143_1370_RED_abrowse.jpg
PSP_007143_1370_RED_abrowse.jpgGully Alcoves (MULTISPECTRUM; credits: Lunexit)58 visiteSeveral characteristics of crater wall gullies are visible in this image that provide possible insight into the formation mechanisms of gullies on Mars.

Gullies near the left side (North) of the image are deeper and originate in alcoves near the rim of the Crater. Gullies near the middle of the image are shallow and contain a more complex array of small channels. These smaller gullies initiate from a uniform elevation within the Crater Wall rather than at the Crater Rim. This suggests that the materials which flow down the Crater slopes to form the gullies originates at a specific layer exposed in the Crater Wall.
The undulating pattern of ridges on the Crater Floor (lower side of the image) appear similar to features interpreted as elsewhere on Mars that involve ice-rich materials.
MareKromium
PIA10139-FansField~0.jpg
PIA10139-FansField~0.jpgFans Field (MULTISPECTRUM; credits: Lunexit)58 visiteAt the very beginning of Spring in the Southern Hemisphere on Mars the ground is covered with a seasonal layer of CO2 ice.
In this image there are 2 lanes of undisturbed ice bordered by 2 lanes peppered with Fans of dark dust.

When we zoom in to the image, we see that the Fans are seen to be pointed in the same direction, dust carried along by the prevailing wind. The Fans seem to emanate from spider-like features.

Image Data: the image is centered at -86,4° Latitude and 99,1° East Long.
The range to the target site was 276,1 Km (about 172,6 miles). At this distance the image scale is 55,2 cm/pixel (with 2x2 binning) so objects ~166 cm across are resolved.
The image was taken at 16:27 MLT (middle afternoon), with the Sun just 2° above the Local Horizon.
MareKromium
Phobos-MEXP-2-h3868_0000_H.jpg
Phobos-MEXP-2-h3868_0000_H.jpgPhobos, the "Doomed Moon", from Mars Express (MULTISPECTRUM; credits: Lunexit)58 visiteCaption ESA:"An image of Phobos by the High-Resolution Stereo Camera on board Mars Express taken on January 10, 2007.

The larger and inner of the two Martian Moons is seen here floating just above the Martian Limb. The image has been enhanced slightly to bring out the detail on the moon".
MareKromium
OPP-SOL1589-1.jpg
OPP-SOL1589-1.jpgUnexplainable "Red Spot" inside Victoria - Sol 1589 (ctx frame - natural colors; credits: Dr M. Faccin)58 visiteLe rocce laminari che vengono inquadrate in questo bellissimo frame già costituiscono - in sè - un enigma; ma ancora più enigmatica è la piccola "striscia" (una sorta di "graffio") color rosso acceso che si può distinguere nel quadrante inferiore Dx del frame.
Ipotesi? Nulla di "esotico".

Probabilmente si tratta di un image-artifact (diremmo derivante da perdita di segnale) il quale, durante il processo di colorizzazione del frame (posto in essere dal sempre bravissimo Dr Faccin), ha deciso di acquisire una "autonoma dignità"...
MareKromium
PHOE-SOL061-lg16227-16228-16229.jpg
PHOE-SOL061-lg16227-16228-16229.jpgThe SUPER-Clean Solar Panels of Phoenix - Sol 61 (Superdefinition; credits: Dr G. Barca)58 visitenessun commentoMareKromium
Phobos-404-20080729-5181-6-an-01-Phobos-Flyby_2_H1.jpg
Phobos-404-20080729-5181-6-an-01-Phobos-Flyby_2_H1.jpgPhobos in 3D (red-cyan anaglyph)58 visiteCaption ESA:"On July 23, 2008, the High Resolution Stereo Camera on board ESA’s Mars Express took the highest-resolution full-disc image yet of the surface of the moon Phobos.
This image data was acquired from a distance of about 97 Km with a spatial resolution of about 3,7 m/pixel".
MareKromium
SOL831-1_copia2.jpg
SOL831-1_copia2.jpgAntenna MAST with Cables and Circuits on Spirit - Sol 831 (natural colors; credits: Dr G. Barca)58 visitenessun commentoMareKromium
PSP_006755_2030_RED_abrowse-4.jpg
PSP_006755_2030_RED_abrowse-4.jpgUnusual Surface Features in Mawrth Vallis Channel: the "Black Box" (EDM - credits for the additional process.: Dr Gianluigi Barca - Lunexit Team)58 visitenessun commentoMareKromium
PSP_006755_2030_RED_abrowse-3.jpg
PSP_006755_2030_RED_abrowse-3.jpgUnusual Surface Features in Mawrth Vallis: the "Worm-like Dunes" (EDM - credits for the additional process.: Dr Gianluigi Barca - Lunexit Team)58 visitenessun commentoMareKromium
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