Saturn
– Then & Now
Galileo
first observed Saturn through his telescope in July, 1610. He had already
announced his discovery of the moons of Jupiter, but Saturn, the furthest
planet then known and twice as far away as Jupiter, was even more mysterious
and difficult to understand. To GalileoÕs surprise, Saturn wasnÕt just one
planet, but three! A big middle
planet with a small planet or moon on each side, and the three were almost
touching. Galileo drew it like
this:
Other astronomers, whose
telescopes were not as good as GalileoÕs, saw a single oval planet. After a few years, Galileo again
studied Saturn, and in 1616 made this sketch:
Above: GalileoÕs sketch of Saturn from
1616. Does it look like a ring to
you? . (Image credit: Albert Van Helden/Science History Publications Ltd.)
Galileo
described the appearance as a planet with handles. How would you describe the planet in his sketch? Although we can easily make out the
appearance of a ring, Neither Galileo nor fellow astronomers guessed that
SaturnÕs shape was due to a ring.
Theories of handles and ovals and triple planets lasted another 40
years, until Dutch astronomer Christian Huygens finally discovered the rings of
Saturn.
What
did YOU See with MicroObservatory?
How does Saturn appear in
your image taken by MicroObservatory?
Can you tell that the planet has rings or, like Galileo, can you imagine
them more as handles, or even a triple planet? To see your image of Saturn more
clearly, you may want to open it in our MicroObservatory
image processing software.
Above: Archive MicroObservatory image of
Saturn. Do you see rings or handles?
Saturn
– 400 Years Later
Saturn has been explored by
four NASA spacecraft since 1979, and close-up views of the rings have shown how
complex and spectacular they are.
We now know that the rings are made up of billions of particles of ice
and rock, varying in size between a few centimeters to a few meters. Despite
the fact that the rings are 250,000km across (Ring-tip to ring-tip would stretch from the Earth to
the Moon!) the rings are less than a kilometer thick, and in some places much
thinner. The brightness of the
rings depends on their thickness, and also how big the ring material particles
are. This image from the Cassini
probe shows the amazing structure and variation in the rings.
Above: An eclipse of the Sun – by
Saturn! This was taken by the Cassini spacecraft as it passed around the night
side of the planet. (Image credit:
JPL/NASA)
The rings of Saturn seem to
be held in place by many tiny moons, called Shepherding moons, which use their
gravity to shape and redistribute the ring material. It is still not clear how the rings were made, or how old
they are, but it is probable that the ring material needs to be replenished or
the rings will fade over millions of years. The new material could come from the dozens of moons in
SaturnÕs family, when collisions or meteorite impacts throw clouds of rock and
ice into space.
Find
Out More
2009 is International Year
of Astronomy, chosen to commemorate the 400th anniversary of
GalileoÕs discoveries with the telescope.
Find out what else is happening by visiting these web sites:
The World site for International Year of
Astronomy.
The United States national site for
International Year of Astronomy.
NASAÕs International Year of Astronomy
website.
For more information on the
Cassini Mission, go to:
http://saturn.jpl.nasa.gov/home/index.cfm/
For more information on the
planets of the Solar System, go to:
http://solarsystem.nasa.gov/planets/index.cfm
The space probes that have
visited Saturn are Pioneer 11 (1979), Voyager 1 (1980), Voyager 2 (1981) and
Cassini-Huygens (2004). To read
about all NASAÕs missions, go to http://www.nasa.gov/missions/index.html
Take
a look at the full list of objects in MicroObservatoryÕs Galileo activity,
and see how our understanding has evolved over the last four centuries.