Alpha Centauri's Universe Planetarium: Exploration Of Saturn
    These pages covers both text and graphics on Saturn and its lesser moons.
   
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Planetary Profile: Saturn Lithograph From NASA
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  • Distance from the Sun:
    1426.73 x 106 km
    9.54 A.U.
  • Mean Equatorial Radius:
    58,232 km
    9.14 of Earth's radius
  • Mass:
    5,684.60 x 1023 kg
  • Density:
    0.69 gm/cm3
  • Gravity:
    8.96 m/s2
    0.92 of Earth's gravity
  • Escape Velocity:
    35.47 km/s
  • Sidereal Rotation Period (Earth hours):
    10.66
  • Sidereal Orbit Period (Earth years):
    29.42 years
Natural Satellites Of Saturn
Click on links to learn more about
the moons of Saturn.

.....Saturn, the sixth planet from the Sun, is one of the five planets visible from Earth without a telescope. Since the 17th century, when Saturn's dazzling, complex ring system was first observed by the Italian astronomer Galileo Galilei, the planet has stood as a symbol of the majesty, mystery, and order of the physical universe. Over the past 20 years, we have discovered that the other gas giants--Jupiter, Uranus, and Neptune--also have rings; however, Saturn's ring system is the most extensive and brilliant. Although the origin of the rings is unknown, scientists hope to uncover clues by studying the planet's history.

.....A giant, gaseous planet, Saturn has an intriguing atmosphere. Alternate jet streams of east-west and west-east circulation can be traced in the motions of the cloud tops; the speeds of these jet streams reach as much as 500 meters per second (1,100 miles per hour) and are responsible for the banded appearance of the clouds. The atmosphere consists mostly of hydrogen and helium, but also includes trace amounts of other elements. Electrical processes and heat from internal planetary sources enrich the layered chemical mix of the atmosphere, which probably transitions from superheated water near the core to the ammonia ice clouds that are observed at the cloudtop. The planet's atmosphere also features storm structures similar to Jupiter's famous Great Red Spot.

.....Although Galileo was the first to see Saturn's rings (in 1610), it wasn't until 1659 that the Dutch astronomer Christiaan Huygens, using an improved telescope, observed that the are actually separate from the planet. In 1676, the French-Italian astronomer Jean Dominique Cassini first observed what appeared to be a division between the rings now known as the Cassini division. Improvements in telescopy over the next three centuries revealed much about the mysterious planet: the banded atmosphere, the storm "spots," and a very apparent "flattening" at the poles, three features Saturn was observed to share with Jupiter.

.....Over the past two decades, a series of spacecraft have flown by Saturn, giving us our first close-up looks of the planet, and revealing information about Saturn's magnetic field and previously unobserved rings and moons. Some moons were found to be covered with very smooth ice. Also, visible and infrared observations of Saturn showed us a surprising mix of thermal patterns among the cloud bands, suggesting internal processes yet to be understood.

.....The Voyager spacecraft discovered hundreds of ringlets within Saturn's major rings. Some have small moons flanking them (called "shepherding" moons. The "F ring" appears to have regularly spaced "knots" due to gravitational interaction with the tiny moons Prometheus and Pandora. Shadowy "spokes" were seen to develop and dissipate in the rings. Ring particles were found to be composed mostly of water ice, and to range in size from dust motes to houses. . The rings may be the remnants of moons destroyed by tidal interaction with Saturn's gravity. They may include remnants of comets that passed too close to Saturn and were likewise destroyed.

.....Today we know Saturn to have 7 major ring divisions and 18 moons. Titan--the largest Saturnian moon --has held the attention of scientists most. A bit larger than the planet Mercury, Titan is shrouded by a thick nitrogen atmosphere that might be similar to what Earth's was like long ago. Further study of this moon promises to reveal much about planetary formation, and perhaps about the primordial Earth as well.

.....Cassini/Huygens, a joint U.S.-European orbiter/probe mission to Saturn and Titan, was launched in October 1997, and will arrive at the Saturnian system in 2004. Cassini/Huygens' 4-year scientific mission is dual: to complete a multispectral, orbital surveillance of Saturn, and to investigate Titan. Cassini/Huygens will measure the planet's magnetosphere, atmosphere, and rings, and observe some of its icy satellites and Titan during close flybys. The orbiter investigation of Titan will be augmented by an instrumented probe-called the Huygens Probe-that will descend through Titan's atmosphere and send back data about the atmosphere and surface. If the Cassini/Huygens mission goes as planned, theories of the solar system's evolution and chemical processes on primordial Earth may be improved.

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