Transcript Saturn
Saturn
Presentation by: Heather DeRoy
Basic Facts
6th Planet from the Sun
2nd Largest Planet in the Solar System
7 thin, flat rings
62 Moons
Ancient Observations
Farthest planet prehistoric astronomers knew
Used in mythology
Planet can be seen by Earth with the naked
eye, but the rings cannot
Saturn the Name
Roman god of agriculture and
harvest
Father of Ceres, Jupiter, Pluto,
and Neptune
Ruled during the Golden Age of
Men
Saturn represents limits of
control as it was thought to be
the limit of the Solar System
Unlucky Saturn
In Astrology, Saturn is blamed for all
things sad, unfortunate, and terrible
Size of Saturn
2nd largest planet in the
Solar System
95 Earth masses
“Gas Giant” along with
Jupiter, Uranus and
Neptune
Diameter 120,540km
(10x Earth)
Density
Lowest of all the planets
1/10 the density of Earth
2/3 dense as water
Saturn would float in water!
Saturn’s Orbit
Aphelion ~ 10.1 AU ; Perihelion ~ 9.0 AU
Period of Orbit – 29.46 Earth years
Axis tilt of 27 degrees
Eccentricity of .056
Rotation is 2nd fastest of known planets
Saturn rotates ~ 10 hours 39 minutes
Shape of Saturn
Rapid rotation causes the planet to bulge
Oblate spheroid – flattened at poles and
bulges at equator
Rings
Saturn’s Rings
Discovered by Galileo (1600s)
Rings tilt at same angle as
equator
~20m thick
93% water ice composition,
7% amorphous carbon
7 rings made up of thousands
of ringlets, made up of billions
of ice particles
Particles range in size from
dust to a car
2 Main Ring Theories
Theory 1
Remnants
of destroyed moon of Saturn
Theory 2
Rings
left over from original nebular material that
formed Saturn
Some ice comes from the moon
Enceladus’ ice volcanoes
Saturn’s Surface
Saturn is a giant ball of gas
Believed to have no solid surface
Inner core of iron and rocky material
Outer core of ammonia, methane, and
water
Liquid metallic hydrogen surrounds outer
core
Hydrogen and helium in a viscous form
Saturn’s Atmosphere
The surface and
atmosphere merge
(hydrogen and helium)
Dense clouds cover
Saturn
Difference in temperature
and altitude cause
patterns and color
differences in cloud tops
Hexagon clouds at North
Pole
Temperature
Tilt of axis causes
seasons on Saturn
Each season = 7.5 Earth
years (Saturn takes 29x
longer than Earth to
revolve)
Top of clouds is -175
degrees C (-285 F)
Below clouds is hot –
planet gives off 2.5x the
heat it receives from the
Sun
Moons
62 Moons
Largest, Titan (diameter 5,150km) is larger
than Mercury and Pluto and contains an
atmosphere
Discovery
Galileo discovered rings 1610, though
believed they were moons on either side
Christian Huygens first coined “Rings”
1665
Exploration
1973, Pioneer-Saturn launched by
U.S.
Flew
within 20,900km of Saturn
Sent close-up pictures
Discovery of 2 outer rings
Found a magnetic field 1000 times
stronger than the Earth’s
Pioneer 11 Photos (1970s)
Exploration
1977, Voyager 1 and Voyager 2
existence of 7th ring
Discovered planet’s rings are made of ringlets
Discovery of 9 satellites
Atmosphere of Titan is nitrogen
Confirmed
Photos from Voyager 1
Saturn
Haze over Titan
F Ring
Photos from Voyager 2
Saturn
Iapetus
Enceladus
Titan
Exploration
1997 Cassini probe
Began
orbiting Saturn in 2004
Studying Saturn, its rings, and its satellites
First spacecraft to orbit Saturn (between F and G
rings)
Cassini Probe
New Moons Daphnis and Phoebe
Titan
Eclipse
Saturn Mysteries?
Much to learn about the rings
Strange features
Clean ice suggests only few hundred million
years old?
Hexagon clouds at North Pole
Rotation impossible to pinpoint
(approximate day calculated)
References
Spinrad, Hyron. "Saturn." World Book
Online Reference Center. 2004. World
Book, Inc.
http://www.worldbookonline.com/wb/Article
?id=ar492440.
http://en.wikipedia.org/wiki/Saturn#Planeta
ry_rings