- Saturn has the most extensive ring system in the solar system, consisting of ice and dust particles orbiting the planet. It has several moons within its rings. - Titan is Saturn's largest moon, composed of ice and rock. It is the only known moon with a dense nitrogen-rich atmosphere and contains lakes of liquid methane and ethane. - Cassini's radar images provided the first evidence of liquid on Titan's surface in the form of large lakes, suggesting weather patterns similar to Earth's.

2.  Saturn has 12 rings and 2 divisions. It has the
most extensive ring system of any planet in
our solar system. These rings consist of
countless small particles, ranging in size from
micrometers to meters that form clumps
orbiting the planet. The ring particles are
made almost entirely of water ice that is
contaminated with dust and chemicals.
Saturn has several moons that are within the
rings.

3.  The Giant
Titan is the fifteenth of Saturn's moons
and is the largest. It is also the second
largest moon in the Solar System. Titan
was names after the ancient race of
giants in Greek Mythology. They were
the children of Uranus and Gaia, who
sought to rule the heavens but were
overthrown by the family of Zeus.

4.  Titan is the only known moon with a fully developed, planet-like atmosphere. Unfortunately, this thick
atmosphere prevented us from learning much about its surface features during the Voyager missions. What we
do know is that it appears to be composed of about half water ice and half rocky material. It is believed to be
similar in composition to many of Saturn's other moons, but is much denser because of its large size and higher
gravity. Titan's atmosphere is believed to have two cloud layers at about 125 miles (200 km) and 186 miles (300
km) above the surface.
 Titan has no known magnetic field, and sometimes orbits outside Saturn's magnetosphere. This exposes it
directly to the solar wind, which may ionize and remove particles from the atmosphere. In 2004, the Cassini
probe arrived at Saturn and dropped a probe called Huygens into Titan's atmosphere. It landed and sent back
images of the surface as well as measurements of Titan's atmosphere. Cassini was then able to map Titan's
surface using radar, as was done on the Magellan mission to Venus. As amazing as these images were, they only
posed more questions than answers. But thanks to Cassini, we have now witnessed some of the most detailed
images yet of the ringed planet and her moons.
 Liquid Lakes
 Because Titan has a thick atmosphere containing hydrocarbons, scientists had long theorized that there could be
lakes of liquid methane and ethane on its surface. When the Voyager spacecraft encountered Titan in 1980 and
1981, they were unable to see beneath the moon's thick layer of clouds. NASA's Cassini spacecraft arrived at
Saturn in 2005 armed with radar. The radar instruments were able to see through the clouds and map the moon's
surface. Radar images taken in 2006 proved the existence of liquid lakes on Titan. These are the first liquid lakes
seen anywhere in the Solar System besides Earth. The largest of these newly discovered lakes is larger than the
Great Lakes on Earth. In addition to the lakes, channels resembling rivers were observed. This provided strong
evidence of liquid rain. Scientists believe that rain composed of liquid methane and ethane regularly falls across
Titan's surface. In fact, the weather on Titan may be very similar to weather patterns on Earth.

5.  Statistics for Titan
 Discovered by
 Year of Discovery
 Diameter
 Mean Distance from Saturn
 Rotational Period
 Orbital Period
 Orbital Eccentricity
 Orbital Inclination
 Mean Surface Temperature
 Main Atmospheric Component
 Atmospheric Pressure
 Apparent Magnitude
 Christiaan Huygens
 1655
 3,200.6 miles (5,151 km)
 759,067 miles (1,221,850 km)
 15.9 days
 15.9 days
 0.0292
 0.33 degrees
 -289° F (-178° C)
 Nitrogen
 1.5 bars
 8.28

7.  The eight planet in distance from he sun,
fourth largest planet in diameter and third
largest mass in solar system.
 Has 4 rings and 13 known moons. The planet
named after the sea of god Neptune on
Roman Mythology.

9.  It was named after the Greek god Triton, who
was the son of Poseidon (Neptune). He is
usually portrayed as having the head and
body of a man and the tail of a fish. This
moon of Neptune was discovered by the
British astronomer William Lassell in 1846.
Since then it has been visited by only one
spacecraft, Voyager 2, in 1989.

10.  Triton orbits Neptune in what is known as a retrograde orbit. This
means that it orbits Neptune a direction opposite the planet's
rotation. It is the only large moon in the Solar System to do this.
Astronomers are not quite sure of the reason for this retrograde
orbit. Some believe that it condensed this way from the original
material of the early solar system. Others think that Triton may
have been formed elsewhere and then captured by Neptune's
gravity. In fact, many astronomers have noticed that the surface
features of Triton, as well as its size, are very similar to what they
believe the planet Pluto to look like. Some even wonder if there is
some connection between Triton's features and the fact that Pluto
actually crosses Neptune's orbit from time to time. Just what that
connection might be is anyone's guess at this point.

12.  Triton is the coldest known object in the Solar System. Its surface
temperature averages only -391° F (-235° C). This is caused by the
moon's high albedo. Very little sunlight is absorbed by the surface.
Triton's axis of rotation is tilted 157 degrees with respect to Neptune's
axis. This causes the moon's polar and equatorial regions to be
alternately pointed towards the Sun. This causes extreme seasonal
changes as Triton's orientation changes. This uneven heating and
cooling could account for some of the moon's curious surface features.
Triton has an extremely thin atmosphere composed mainly of nitrogen
and methane. There are very few craters visible on the surface,
indicating that the moon is very young and probably highly active.
There are high ridges and deep valleys all over the moon's surface.
Perhaps the most interesting discovery to be made by Voyager 2 was
Triton's ice volcanoes. Voyager photographed a plume of frozen
material being ejected from the moon's surface. Astronomers believe
this material to be composed of liquid nitrogen or methane.

13.  Statistics for Triton
 Discovered by
 Year of Discovery
 Diameter
 Mean Distance from Neptune
 Rotational Period
 Orbital Period
 Orbital Eccentricity
 Orbital Inclination
 Mean Surface Temperature
 Main Atmospheric
Component
 Apparent Magnitude
 William Lassell
 1846
 1,677 miles (2,700 km)
 220,405 miles (354,800 km)
 5.87 days
 5.87 days
 0
 157.4 degrees
 -391° F (-235° C)
 Nitrogen
 13.47

14.  This is Earth's moon, and it is the planet's only natural satellite.
Although we call it simply "the Moon", it is associated with the
Roman goddess Luna, who was goddess of the hunt and of the
Moon. It is the sixth largest moon in theSolar System, and has
been Earth's partner for most of the planet's known history.
Although it has been lighting our dark nights for so long, its
origins are mostly unknown. Some believe it was formed when a
gigantic asteroid smashed into the Earth. The resulting impact
flung molten material far out into space where it cooled and
formed the Moon we see today. Others believe it was a
wandering planetoid captured by the Earth's gravitational pull.
Wherever it came from, it has fascinated mankind for centuries.
The Moon is the only planetary body whose surface can be seen
from Earth with the naked eye.

16.  Perhaps the most prominent features of the Moon are its
numerous craters. Its surface has been bombarded continually throughout
its history. Since the Moon has no measurable atmosphere and no liquid
water, there is no erosion taking place. This has preserved the many
thousands of craters on its surface.
 Another prominent feature on the Moon are the smooth areas
called maria. The maria are believed to have been formed by more recent
lava flows which have covered over the older craters. There are also many
mountain ranges and rift valleys on the Moon's surface. All of these
features have combined to form a unique facial feature known as the "Man
in the Moon" that can be seen if one knows what to look for. This feature is
visible every night of the year because the Moon always keeps its same
face towards the Earth. This is because its period of rotation and revolution
are the same; 29 days, 12 hours and 44 minutes.
 This cycle is known as the lunar month As the Moon orbits the Earth, it
appears to change shape as more or less of its sunlit side is visible. When
the Moon is on the opposite side of the Earth as the Sun, it appears as a full
moon. When it is on the same side, it is invisible, also known as a new
moon. Since it is so close to the Earth, the Moon's gravity pulls on our
oceans and creates the tides.

17.  Diameter
 Mean Distance from Earth
 Rotational Period
 Orbital Period
 Orbital Eccentricity
 Orbital Inclination
 Inclination of Axis
 Mean Surface Temperature
 Main Atmospheric
Component
 Atmospheric Depth
 Apparent Magnitude
 2,160 miles (3,476 km)
 238,800 miles (384,400 km)
 27.32 days
 27.32 days
 0.05
 5.14 degrees
 1.53 degrees
 0° F (-17° C)
 Hydrogen
 negligible
 -12.74

18.  The moon has a very heavily cratered surface, which tells the tale of solar system.
Earth would be the same way if it had no atmosphere nor plate tectonics. Without
an atmosphere or water to erode the craters, the lunar landscape has remained
relatively constant for billions of years.
 It is through these craters that we can actually tell some of the solar system's
history. Through dating the craters, planetary scientists have been able to
determine that most of the craters were made in the early days of the solar
system, approximately 3.8-4.5 billion years ago. This means that early in the solar
system, there was a period of heavy asteroid bombardment. This is most likely
due to all of the extra material left over from the solar system's formation. After
approximately 1.2 billion years, most of the material had formed into the Asteroid
Belt, been ejected from the solar system, or hit the planets and moons.
 If you look at the moon closely, you can see dark patches. After the period of
heavy asteroid bombardment, the moon's surface cracked in many places. The
lowlands of the moon filled with volcanic material, which then cooled. This lasted
for approximately 750 million years. They are called maria(singular is mare) due to
their resemblance to dark oceans.