Thursday, November 7, 2013

The Moons and Rings of Saturn

Picture taken from Voyager. The colors are to depict
different chemical make-up of the rings. 

Hallie Stolte 
Picture from NASA Cassini Mission


Overview
Saturn is a gas giant that is the second largest planet in our solar system after Jupiter. It is mostly known for its incredible rings. There are 53 confirmed moons and 9 potential moons. The Saturn system is very complex because the moons orbit with in the rings and are an integral part of ring system. Some of the moons are called "shepherd moons" because they orbit within the rings and interact in a way that causes the ring material to be guided into a certain position. The Cassini mission was launched in 1997 and has recently discovered a lot about the moons and rings of Saturn. Part of the mission was to drop a probe on to one of Saturn's moons, Titan. This has lead to many discoveries about Titan. One important discovery is how similar is is to Earth. Scientist are using Titian to model the early stages of Earth’s development.


Enceladus
Enceladus is one of Saturn’s moons located in Saturn’s outermost ring (the E-ring). It has recently become and important moon because of the Cassini mission. Uniquely, this moon is known for it its icy volcanic activity. The Cassini mission discovered that this icy material was contributing to the formation of the E-ring. The material comes from under the surface of the moon and is ejected out into the atmosphere of the moon and even ejected beyond the atmosphere. The material that doesn’t leave the atmosphere falls back to the moon like snow, and the material that does escape contributes to the material in the E-ring. Following this discovery, the Cassini mission discovered that some of the E-ring material contained sodium salts. It was then theorized that the jets of Enceladus came from a liquid source that lay under the surface of the moon. The sodium salts gave way to the idea that this liquid source was actually a salt-water ocean.


Rings
Galileo first saw the rings of Saturn in 1610. The rings were named using alphabetical letters as they were discovered. Each ring orbits at a different speed around Saturn because of Kepler’s third law. Each ring also has its own unique make up and density. The rings span about 200 times the diameter of Saturn. They are composed of frozen material that originated from of asteroids, dust, and broken moons. Before the Cassini mission, “ghostly” shadows were spotted on the rings. These shadows are called spokes and have just recently started to be understood with the Cassini mission. The spokes form in a matter of minutes and only last for a few hours. They are still not well known, and scientists hope to learn more about their cause with Cassini.




Questions: (To answer some of these questions you will have to explore the links above)

What is the order of the rings starting with the ring closets to Saturn?
a.    A, B, C, D, E, F, G
b.    G, F, E, D, C, B, A
c.    D, C, B, A, F, G, E
d.    C, A, F, G, D, B, E

Which is not true regarding the moons of Saturn? (Use this link)
a. Titan is so massive that its gravity affects other moons orbits
b. Some of the moons orbit in the opposite direction as everything else.
c.  Half of Lapetus is very dark while the other side is very bright.
d.  Titan is the largest moon in the solar system

Which statement about Enceladus is not true?
a.  Its jets contribute to the formation of Saturn's E-ring
b.  It is located in the E-ring
c.  It might have a salt-water ocean beneath its surface
d.  It has eruptions of icy material
e. All statements are true

In the mosaic infrared mapping of Titan there are orange spots. What do these represent?
a. Lakes
b. Volcanic activity
c. Evaporated Material
d. Bedrock of water and ice

When were the spokes first seen? (use this link)
a.  In 1997, when the Cassini was launched
b.  In 2004, when Cassini began to orbit
c.  In 1979, with the pioneer
d.  In 1981, with the Voyager 2 flyby

Browse the gallery in the NASA website. What is the rose?
a. An anomaly on Saturn’s B-ring
b. A vortex on Saturn’s pole
c. A dust cloud in the Saturn system
d. A storm on Titan


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