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Saturn
Rings of Saturn
Saturn has seven rings which surround it at its equator without touching the planet. Each ring is a mass of billions of orbiting pieces of ice and rock. It consists of tiny grains of dust to wide chunks of ice of about 10 metres. The A, B, C and F rings are brighter while the D, G, and E rings are very faint. The gravitational pull of the planet and its satellites help the rings to be held together in orbit.
Spaceship to Saturn
Pioneer-Saturn was the spaceship launched by the US in 1973. In 1979 it reached about 21,000 kilometres near Saturn and detected that the planet has stronger magnetic field than the Earth. In 1977 Voyager-I and Voyager-2 of the US confirmed the presence of seven rings surrounding Saturn.
Observation of Saturn's rings
Saturn's rings was discovered by Galileo in 1610. In 1655 the Dutch scientist Christiaan Huygens found out that the rings are flat and solid, and inclined to the planet's orbital plane. Years later Cassini discovered the gap between every ring. In 1789, French scientist Pierre Simon Laplace stated that the rings are formed of many small components. James Clerk Maxwell in 1857 confirmed that a large number of tiny particles together form the rings of Saturn.
Saturn
Distance from the sun in km.: 1429.4 million
Diameter at equator in km.: 120,536
Mass with respect to the earth: 95. 184 (earth=1)
Gravity with respect to the earth: 1.07
Period of revolution: 29% earth years (approx.)
Period of rotation: 10 hours and 39 minutes
Density (g/cm³): 0.69
Temperature: -178°C
Satellites: 33
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