Saturn: the "Lord of the Rings"
 
by Karl W. Schmidt

 

History

In 1610, the Italian astronomer Galileo
was the first human to see the rings of Saturn. Galileo described the rings as "handles", not knowing they were separate from the planet. It wasn’t until 1655 that a Dutch astronomer, Christian Huygens, was able to note that the rings were a separate entity. In the early 1980’s, the Voyager 2 spacecraft took the first close-up images of Saturn and its rings. Voyager showed that the rings were made up of rock and ice particles. These particles varied in size from pebbles to giant boulders. The Hubble Space Telescope captured breath-taking pictures of our ringed planet in the early 1990’s. In 2004, another spacecraft, Cassini, will bring us close-up pictures of Saturn as well as land a probe on Saturn’s moon Titan.

 

Intrinsic Properties

Saturn is the sixth planet from the Sun, and the second largest planet in the solar system. It is about 9.4 times the size of the Earth. The rings of Saturn extend roughly 81,000 miles (135,000 km) from the center of the planetary disk. From Earth, the maximum size of Saturn's disk is 20 arcseconds, and together with its rings it displays the apparent size of 46 arcseconds. Saturn reaches a brightness of zero magnitude. Saturn has 18 known moons, Titan being the largest. Over a 30-year period we will witness different views of the rings (open or edge-on) because they are inclined 27 degrees to Saturn’s orbit.
 

 

Observing Saturn

In March 2004, Saturn is at its best. It is high in the sky, almost overhead, in the feet of the constellation Gemini. This is prime time for viewing because we are looking through thin atmosphere and steady air currents.  When observing the rings, you will notice a division known as the Cassini division. This is an area sparse of rocks and particles that make up the rings. The Cassini division is easily visible in small telescopes, such as a 60mm refractor. A 10-inch or larger telescope will show another, smaller gap in the rings called the Encke division. Other observable characteristics include atmospheric features such as belts, zones, spots, and polar caps. Filters will help enhance these atmospheric features (blue #80A or yellow #12). 

This map shows you where to find Saturn in 2004. In March, Gemini is high overhead after dusk. Saturn is the brightest starlike object in this region, with the exception of Sirius, the Dog Star, which is south in the constellation Canis Major.

Images of Saturn on this page are Copyright NASA,The Voyager Project, AURA/STScI. All rights reserved.

 

 

 

 

 

 

 

Useful Saturn Links

Download this handy program that shows the current positions of Saturn's moons, as well as their magnitudes. Also has an animate feature.

Current Positions of Saturn's Moons. This page will show you which of Saturn's many moons are where before you go observing.

The SEDS solar system page, featuring articles about Saturn and its moons.

NASA's Saturn Photo Gallery: a compilation of photos taken by various spacecraft that have imaged the Ringed Planet.