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Inizio > SOLAR SYSTEM > Saturn: the "Ringed Beauty" and His Moons

Piú viste - Saturn: the "Ringed Beauty" and His Moons
Enceladus-N00036991.jpg
Enceladus-N00036991.jpgEnceladus fly-by (7) - from approx. 54.000 Km55 visitenessun commento
Enceladus-N00036994.jpg
Enceladus-N00036994.jpgEnceladus fly-by (8) - from approx. 52.000 Km55 visitenessun commento
Enceladus-N00037005.jpg
Enceladus-N00037005.jpgEnceladus fly-by (10) - from approx. 35.000 Km55 visitenessun commento
Enceladus-N00037009.jpg
Enceladus-N00037009.jpgEnceladus fly-by (11) - from approx. 33.000 Km55 visitenessun commento
Enceladus-N00037024.jpg
Enceladus-N00037024.jpgEnceladus fly-by (14) - from approx. 22.000 Km55 visitenessun commento
Enceladus-N00037036.jpg
Enceladus-N00037036.jpgEnceladus fly-by (15) - from approx. 18.000 Km55 visitenessun commento
Saturn-PIA07560.jpg
Saturn-PIA07560.jpgSaturn and Tethys55 visiteOriginal caption:"Saturn poses with Tethys in this Cassini view. The C ring casts thin, string-like shadows on the Northern Hemisphere. Above that lurks the shadow of the much denser B-Ring. Cloud bands in the atmosphere are subtly visible in the south. Tethys is 1071 Km (about 665 miles) across.
Cassini will perform a close flyby of Tethys on Sept. 24, 2005. This image was taken on June 10, 2005, in visible green light with the Cassini spacecraft wide-angle camera at a distance of approx. 1,4 MKM (such as about 900.000 miles) from Saturn. The image scale is 81 Km (about 50 miles) per pixel".
Mimas Map-PIA06255.jpg
Mimas Map-PIA06255.jpgMimas' Map55 visiteOriginal caption:"This map of the surface of Saturn's moon Mimas illustrates the Regions that were imaged by Cassini during the spacecraft's flyby of the moon on Aug. 2, 2005. At closest approach, the spacecraft passed within approx. 62.900 Km above the Moon's surface. The colored lines delineate the Regions that were imaged at differing resolutions. The closest images were obtained near closest approach. Mimas has never been imaged this closely before. The flyby provided the best views yet of the South Pole of Mimas and some of its northern latitudes, as well as distant views of the giant crater Herschel, near the terminator.
The highest resolution images show the trailing hemisphere of Mimas, opposite Herschel. Several fracture systems have been seen in the region in NASA Voyager images, like Pelion Chasma and Tintagil Chasma. Images obtained from this Cassini encounter may help test whether these canyons and others on Mimas' surface, are related to the formation of Herschel (...)".
Enceladus-GroundTrack-PIA07723_modest.jpg
Enceladus-GroundTrack-PIA07723_modest.jpgEnceladus: the "Ground-Track"55 visiteThis graphic shows Cassini's path, or Ground Track, as it crossed over the surface of Enceladus near the time of closest approach during the flyby on July 14, 2005. The Ground Track is indicated by a yellow line, marked by increments of 10" before and after closest approach. The spacecraft came within 175 Km from the surface of Enceladus at closest approach.
The red contour encloses the Region on Enceladus around the South Pole that is the approx. boundary of the warm region, as measured by the Composite Infrared Spectrometer (CIS) on Cassini. As previously announced, temperatures observed within this region reached as high as 110 Kelvin (about -260 Fahrenheit). (...) Results like these, pouring in from various Cassini instruments, indicate the warm South Polar Region and, in particular, the 'tiger stripe' fractures straddling the South Pole, as the sources of heat, water vapor and small, icy particles.
Enceladus is a surprisingly active moon. Why its South Pole is the site of this activity is a mystery.
Japetus.jpg
Japetus.jpgThe "Great - and anomalous - Walls" of Japetus55 visiteUn nuovo lavoro del Dr Feltri sulle raw images di Cassini. Ma sentiamo che cosa Lui stesso racconta:"...fermo restando che i Thunderbolts hanno indovinato parte della Verità, le cose sono alquanto più complicate di quanto pensano. Dal punto di vista 'architettonico' è interessante il "muro" sinaptico verticale semicircolare che divide il cratere più grande da quello intermedio. Come già visto in Endurance, la parete verticale si è leggermente distaccata dalla superficie orizzontale superiore, il che costituisce un indizio consistente sulla formazione indipendente delle 2 superfici perpendicolari (e addio alla teoria dei Crateri da Impatto...) le quali si sono prima connesse e poi distaccate (un po' come piastrelle posizionate su un gradino). Tale circostanza porta ad una coesistenza di matrici biogeniche e forze elettromagnetiche, non essendo a mio parere plausibile una spiegazione che tenti di attribuire queste formazioni ad una sola Teoria Esplicativa...".

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Atlas-PIA07592.jpg
Atlas-PIA07592.jpgAtlas, from 489.000 Km55 visiteOriginal caption:"The 'flying saucer' in this image is the small moon Atlas (20 Km or about 12 miles across), whose shadowy profile reveals its flattened shape. This image looks down onto the outer A-Ring and through the Encke and Keeler Gaps.
Two distinct, thin strands in the F-Ring are visible here, silhouetted against the Planet. Saturn's extended, high-altitude haze is seen near lower right.
The image was taken in visible green light with the Cassini spacecraft narrow-angle camera on Aug. 2, 2005, at a distance of approx. 489.000 Km (such as about 304.000 miles) from Atlas and at a Sun-Atlas-spacecraft angle of 138°. The image scale is 3 Km (about 2 miles) per pixel".
Tethys-N00040077.jpg
Tethys-N00040077.jpgTethys Fly-By (7)55 visitenessun commento
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