Wednesday, March 21, 2012

Saturn's Rings



Looking at the solar system, what do you notice that is different between the terrestrial planets and the giant planets besides their weights and sizes? That’s right, all the giants planets have rings circling around them. Jupiter, Uranus, Saturn and Neptune, they all have rings. These rings are magnificent and spectacular to look at if you have a decent back yard telescope. They are made of different materials, have different sizes, and color. Saturn’s rings stand out as the most magnificent because of their large size and shape.
Back in 1610, Galileo was able to discover the rings of Saturn using his newly invented telescope. He was the first one to look at the Saturn’s rings but did not know what they were. He called them ears of Saturn as the rings appeared to him as two smaller planets on Saturn’s sides. The discovery had puzzled astronomers for a long time during the time. The launches of NASA’s Voyage 1, Voyage 2 and the Cassini helped us learned about these spectacular rings.

The rings of Saturn are actually a ring system, which is about 1 kilometer in thickness and about 282000 km in size. The ring system consists of billions of particles and the sizes range from tiny dust particle to a km in diameter. The ring system has 5 major rings, G, F, A, B, C, D with G being the farthest and D being the closest from the Planet. The letter name is in the order of which the rings were discovered. Each of these major rings also consists of individual, smaller rings, called ringlets. The gap between ring A and B is called the Cassini Division, which is the largest gap between the rings, about 4700 km. The main element that make up the rings are pure water ice and dust.
We still do not know the origin of these rings exactly. A theory is that these rings formed from the debris of Saturn’s moon that was ripped apart by Saturn’s tidal force. Another theory is that they form from the debris of a disruption of Saturn’s moons.
            The A, B, C rings are called the main rings as they are the largest in size and the most dense. B ring is the most massive of all the rings. The D, G, F rings are fainter and dustier. They are called dusty rings. D ring is the faintest and closest to Saturn.
           

 Reference:
http://en.wikipedia.org/wiki/Rings_of_Saturn
http://pds-rings.seti.org/saturn/
http://csep10.phys.utk.edu/astr161/lect/saturn/rings.html
http://nineplanets.org/saturn.html

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