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Craters-Unnamed_Crater-PCF-LXTT.jpgUnusually-looking Unnamed Crater (Saturated Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia)57 visiteCaption NASA:"At one time the Floor of this Unnamed Crater located to the West of Hellas Basin, was completely filled with material from Rim to Rim. As this image shows, part of that fill material is being removed. The hole that is formed shows that the fill material was layered and a very rough surface is located at the bottom of the hole".MareKromium
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SOL1252-2P237513744ESFAUCMP2576R3M1.jpgBoulders... - Sol 125257 visitenessun commentoMareKromium
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OPP-SOL1232-1N237560312EFF85W0P1993R0M1.jpgClearing Skies over Meridiani... (3) - Sol 123257 visitenessun commentoMareKromium
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SOL1254-2N237599908EFFAUCMP1936R0M1.jpgFoggy days over Gusev Crater... - Sol 125457 visitenessun commentoMareKromium
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The_Rings-PIA08985.jpgMoons...57 visiteCaption NASA:"The effects of three of Saturn's Ring Moons can be spotted in this single narrow-angle camera view.
The image has been strongly enhanced to better show the wakes on both sides of the Encke Gap caused by Pan (left of center), as well as a hint of the edge waves in the narrow Keeler Gap caused by Daphnis (just below center).
Bright Prometheus (on the right) pulls away from its latest close encounter with the F-Ring. The aftereffects of its recent passes are visible in the Ring's inner edge.
This view looks toward the unilluminated side of the Rings from about 10° above the Ping-Plane.
Saturn's shadow cuts across the Rings at the top of the scene.
The image was taken in visible light with the Cassini spacecraft narrow-angle camera on June 5, 2007 at a distance of approx. 2,3 MKM (about 1,4 MMs) from Pan.
Image scale is about 13 Km (approx. 8 miles) per pixel".MareKromium
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Saturn-PIA08987.jpgNorthern Latitudes57 visiteCaption NASA:"Incredible swirling details in Saturn's Northern Clouds can be seen in this dazzling view. Shadows cast by the Rings embrace the Northern Hemisphere.
The view looks toward the unilluminated side of the Rings from about 16° above the Ring-Plane.
The image was taken with the Cassini spacecraft wide-angle camera on June 10, 2007 using a spectral filter sensitive to wavelengths of infrared light centered at 939 nanometers. The view was acquired at a distance of approx. 1,3 MKM (such as about 800.000 miles) from Saturn. Image scale is roughly 72 Km (about 45 miles) per pixel".MareKromium
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HerculesGCluster-A2151LRGB.jpgThe "Hercules' Galaxy Cluster"57 visite"...Ed è per questo che mi chiamano cinico.
Per questo mi dicono che sono freddo come il marmo di una tomba.
Solo perchè - e non senza sforzi!... - riesco a vedere la Realtà per ciò che è. Davvero.
Senza maschere.
Senza finzioni.
Senza illusioni.
Vedere ed interpretare le cose che accadono per quello che esse sono realmente, eliminando le facili speculazioni emotive, la retorica, l'ipocrisia, il quieto vivere, e tutto quanto costituisce ciò che io chiamo "Scudo dell'Io", significa essere VIVI.
Significa non aver svenduto la propria Anima al miglior offerente.
Significa avere ancora sangue nelle vene, carne sopra le ossa e pensieri nella mente.
Significa essere Uomini.
Significa, in ultima analisi, "essere liberi".
Ma l'ipocrisia...L'ipocrisia che ci avvolge, dolce, suadente e sottile, coprendo le nostre miserie con una coltre di confortevole nebbia, chiama "lupi" coloro che comprendono la Realtà.
Bene.
E allora, come lessi da qualche parte, "Se io sono realmente un lupo, guardati dalle mie zanne!"...".
P.C. Floegers - "Conversations for Tomorrow"MareKromium
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South_Polar_Features-Defrosting_Dunes-2005_06-PCF-LXTT.jpgDefrosting Dunes (Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunexit Team)57 visitenessun commentoMareKromium
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The_Rings-PIA08988.jpgBright Region in the C-Ring57 visiteCaption NASA:"This bright, isolated plateau in the middle of the C-Ring displays interesting internal variations in brightness. The plateau is not high in terms of elevation, but rather in terms of its particle density (seen here as brightness), which is several times higher than the surrounding Ring Structure.
Ring scientists are working to understand what produces the sharp boundaries of the plateau features, as well as the nature of the internal variations in brightness.
This view looks toward the sunlit side of the Rings from about 18° below the Ring-Plane.
The image was taken in visible light with the Cassini spacecraft narrow-angle camera on June 12, 2007 at a distance of approx. 230.000 Km (about 143.000 miles) from Saturn. Image scale is roughly 1 Km (3353 feet) per pixel".MareKromium
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HD98800-PIA09939.jpgEvidence for Strange Stellar Family57 visiteThis artist concept depicts a Quadruple-Star System called HD 98800. The System is approx. 10 MY old, and is located 150 LY away in the constellation TW Hydrae.
HD 98800 contains four stars, which are paired off into doublets, or binaries.
The stars in the binary pairs orbit around each other, and the two pairs also circle each other like choreographed ballerinas. One of the stellar pairs, called HD 98800B, has a disk of dust around it, while the other pair does not.
Although the four stars are gravitationally bound, the distance separating the two binary pairs is about 50 astronomical units (AU) -- slightly more than the average distance between our sun and Pluto.
Using NASA's Spitzer Space Telescope, scientists finally have a detailed view of HD 98800B's potential planet-forming disk. Astronomers used the telescope's infrared spectrometer to detect the presence of two belts in the disk made of large dust grains. One belt sits approx. 5.9 AU away from the central binary, or about the distance from the sun to Jupiter, and is likely made up of asteroids and comets. The other belt sits at 1.5 to 2 AU, comparable to the area where Mars and the asteroid belt sit, and is made up of sand-sized dust grains.
MareKromium
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NGC-2237_and_NGC-2244.jpgHot Stars in the Rosette Nebula57 visiteWinds and radiation from massive hot stars in the Rosette Nebula have cleared the natal gas and dust from the center of the nearby star-forming region. They also pose a danger to planet forming disks around young, cooler stars in the neighborhood. This Spitzer Space Telescope (SST) infrared image of dust clouds near the Rosette's central region, shows the cleared-out cavity.
The view spans about 45 LY at the the nebula's estimated distance of 5.200 LY. MareKromium
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as17-153-23589.jpgAS 17-153-23589 - Wallace Crater57 visiteImage Collection: 70mm Hasselblad
Mission: 17
Magazine: 153
Magazine Letter: MM
Revolution: 39
Latitude: 20,4° North
Longitude: 8,3° West
Lens Focal Length: 80 mm
Camera Altitude: 103 Km
Sun Elevation (on Local Horizon): 1°
Mission Activity: REV 39
Film Type: SO-368
Film Width: 70 mm
Film Color: colorMareKromium
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