Ancora Saturno: la NASA scopre un nuovo anello

[2di7]

La Nasa ha scoperto un nuovo grande anello di Saturno

Pasadena (California, Usa), 7 ott. (Ap) - Il telescopio spaziale della Nasa, Spitzer, ha scoperto il più grande anello di Staturno mai osservato prima di oggi. Il laboratorio californiano ha annunciato che l'anello si situa alla periferia del sistema di Saturno, in un'orbita inclinata di 27 gradi rispetto al principale anello conosciuto. Saturno ne conta sette principali. Il nuovo anello è composto di ghiaccio e di polvere allo stato di particelle, in una atmosfera di -157 gradi Celsius. L'anello è molto esteso e non è facile vederlo, perchè non riflette la luce visibile. Il telescopio Spitzer ha potuto localizzarlo grazie ai raggi infrarossi. In effetti, malgrado il suo intenso freddo, l'anello brilla sotto l'effetto di radiazioni termiche. La massa dell'anello comincia a circa sei milioni di chilometri dal pianeta e si estende su 11,9 milioni di chilometri.

Fonte: apcom.net

[WALTHARI]

non si conosce mai abbastanza l'universo....

[Morlok]

WALTHARI ha scritto:

non si conosce mai abbastanza l'universo....

Magari l'universo, noi siamo ancora a zonzo nel cortile di "casa"!

[WALTHARI]

Morlok ha scritto:

WALTHARI ha scritto:

non si conosce mai abbastanza l'universo....

Magari l'universo, noi siamo ancora a zonzo nel cortile di "casa"!

vero...sig

[2di7]

NASA's Spitzer Space Telescope has spotted a nearly invisible ring around Saturn -- the largest of the giant planet's many rings. The ring is so diffuse that it reflects little sunlight, or visible light that we see with our eyes. But its dusty particles shine with infrared light, or heat radiation, that Spitzer can see.

This artist's conception simulates an infrared view of the giant ring. Saturn appears as just a small dot from outside the band of ice and dust. The bulk of the ring material starts about six million kilometers (3.7 million miles) away from the planet and extends outward roughly another 12 million kilometers (7.4 million miles). The ring's diameter is equivalent to roughly 300 Saturns lined up side to side.

The inset shows an enlarged image of Saturn, as seen by the W.M. Keck Observatory at Mauna Kea, Hawaii, in infrared light. The ring, stars and wispy clouds are an artist's representation.

Image credit: NASA/JPL-Caltech/Keck



This diagram illustrates the extent of the largest ring around Saturn, discovered by NASA's Spitzer Space Telescope. The ring is huge, and far from the gas planet and the rest of its majestic rings.

The bulk of the ring material starts about six million kilometers (3.7 million miles) away from the planet and extends outward roughly another 12 million kilometers (7.4 million miles). The diameter of the ring is equivalent to 300 Saturns lined up side to side. The ring is thick too -- it's about 20 times as thick as the diameter of the planet. In fact, the entire volume of the ring is big enough to hold one billion Earths!

Saturn's newest halo is tilted at about 27 degrees from the main ring plane and encompasses the orbit of the moon Phoebe. Both the ring and Phoebe orbit in the opposite direction of Saturn's other rings and most of its moons, including Titan and Iapetus.

Why did it take so long to find something so big? The answer is that the ring is very tenuous, made up of a sparse collection of ice and dust particles. If you could transport yourself to the ring, you wouldn't even know you were there because the particles are so far apart. There's not a lot of sunlight out at Saturn, so this small density of particles doesn't reflect much visible light. Spitzer was able to spot the band because it sees infrared light, or heat radiation, from objects. Even though the ring material is very cold, it still gives off heat that can Spitzer can see.

The discovery offers a possible solution to the mystery of the moon Iapetus. Years after Giovanni Cassini discovered Iapetus in 1671, he correctly deduced that one side of the moon is white and the other dark in a pattern that some say resembles the yin-yang symbol or a tennis ball. Astronomers think it is possible that the newfound ring, which orbits in the opposite direction of Iapetus, is the cause of the two-faced coloring. As the ring circles around, particles could be drifting inward and splattering the icy moon on the face like bugs on a windshield.

The pictures of Saturn, Phoebe and Iapetus were taken by NASA's Cassini spacecraft. The ring is an artist's illustration.

The size of Phoebe relative to Iapetus has been enlarged to better show Phoebe. Phoebe is about 200 kilometers (124 miles) in diameter, while Iapetus is about 1,500 kilometers (932 miles) across.

Image credit: NASA/JPL-Caltech

Altre info: http://www.nasa.gov/mission_pages/spitz ... 91006.html