Rings of Saturn
The rings of Saturn are the planetary rings around the planet Saturn, which can be seen with a small telescope. They consist of many small particles, ranging in size from microscopic to the size of a bus (or bigger) that form clumps that move around Saturn. The particles in the rings are made almost entirely of water ice,[1] with just a small amount of dust and other chemicals. There are some gaps in the rings. The moon Pan causes the gap called the "Encke gap" in Saturn's A ring.[2] The Cassini Division, discovered by Giovanni Domenico Cassini, is a gap between the A ring and the B ring. It is a product of orbital resonance.
Rings Of Saturn Media
Detail of Galileo's drawing of Saturn in a letter to Belisario Vinta (1610)
Simulated image using color to present radio-occultation-derived particle size data. The attenuation of 0.94-, 3.6-, and 13-cm signals sent by Cassini through the rings to Earth shows abundance of particles of sizes similar to or larger than those wavelengths. Purple (B, inner A Ring) means few particles are
A 2007 artist's impression of the aggregates of icy particles that form the portions of Saturn's rings which appear solid from a distance. These elongated clumps are continually forming and dispersing. The largest particles are a few meters across.
Saturn ring spokes PIA11144 secs15.5to23 20080926
References
- ↑ The Rings of Saturn (1995-11-21)Csep10.phys.utk.edu. Retrieved 2012-01-20.
- ↑ Cassini Solstice Mission: Pan (2004-07-01)Saturn.jpl.nasa.gov. Retrieved 2012-01-20.