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Can you name all nine planets? |
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Mercury is the planet closest to our Sun, and it
is the eighth largest of the nine planets. Mercury is a small, rocky planet
- much like our Moon. It is covered with craters and has changed very
little from when it was first formed. |
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It rotates around the sun in about 88 days. The
same side always faces the sun so it doesn’t see the light of day. The dark
side is extremely cold. |
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One of Mercury's largest features is called the Caloris
Basin. It is about 1300 km across! It was probably created by a very large
crash early in the history of the Solar System. |
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Venus is the second planet from the Sun, and the
sixth largest of all the nine planets. |
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Venus' hot temperature is due to what we call
"the Greenhouse Effect." The large amount of carbon dioxide in
Venus' atmosphere acts like a blanket. The heat gets trapped underneath the
thick layer of clouds. Because the heat has nowhere to go, Venus gets
hotter and stays hot. |
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This is an artists idea of what the surface of
Venus might be like. |
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No one has actually ever been to Venus but NASA
has sent probes to study the planet. |
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The Earth is a small, rocky planet which
supports a variety of life. As far as we know, Earth is unique from all
other planets in this respect. |
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The Earth moves around the sun, taking one year
to go around once. The moon goes around the Earth. It is smaller than the
sun, but it looks as big as the sun because it is much closer to us. |
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The moon is roughly one sixth the size of Earth.
It rotates around Earth every twenty-seven days, seven hours, and
forty-three minutes. However, we only see one side of it because the other
side never faces the Earth. |
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Several Americans have walked on the moon as
part of the Apollo space program. This is a look at the liftoff of Apollo
12 on November 14, 1969. |
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This picture shows you how the size of the earth
compares to the size of the moon. |
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Mars is a small, rocky planet. There are no seas
and it is always very cold. The air
is so thin that we could not breath it. It is smaller than the Earth,
though bigger than our moon. |
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Mars has permanent ice caps at both poles made
up mostly of solid carbon dioxide. We know this as "dry ice."
Very strong winds and vast dust storms sometimes blow through the entire
planet for months! |
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Mars has two tiny moons which orbit very close
to the surface. Their names are Phobos and Deimos. |
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Jupiter is the fifth planet from the Sun and by
far the largest of all nine planets. |
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Jupiter is not like Earth. It is made up of gases, so we could never land
a rocket there. |
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Jupiter's most outstanding and interesting
feature is called "The Great Red Spot", which is a huge storm in
Jupiter's gas. |
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Jupiter has sixteen moons. Four of them are big. One of them, called Io, has active
volcanoes on it. |
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You can see these four moons with any telescope. |
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Jupiter has faint rings like Saturn's, but much
smaller. Unlike Saturn's, Jupiter's rings are dark . They're
probably composed of very small grains of rocky material. |
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This is the huge storm that has been going for
decades. |
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This is Jupiter’s moon Io. |
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The bright light on the left of the picture is
an erupting volcano. |
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Io is the most volcanically active place in the
solar system. |
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Jupiter has very faint rings. They are much more difficult to see than
the rings of Saturn. |
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Saturn is the sixth planet from the Sun, and the
second largest of the nine planets. Like Jupiter, Saturn has a surface made
up of gas. |
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Saturn has rings around it, which are made of
little bits of ice moving around Saturn. Saturn has eighteen moons
that we know of. |
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Uranus is a cold, giant gas planet which is made
up of mostly rock and various ices. Uranus has a faint ring system and 21
known moons. |
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Uranus is a very odd planet. It sits on its side
with the north and south poles sticking out the sides. |
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This picture shows Uranus with four of its
moons. |
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Neptune is a cold, giant gas planet which is
made up of mostly rock and various ices. Neptune is about half as big as
Saturn and has eight known moons; seven small ones and a large moon called Triton. |
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Neptune is usually the eighth planet from the
Sun but occasionally the ninth planet Pluto crosses Neptune's orbit and
becomes the "eighth planet".
Its bluish color comes from its atmosphere of methane gas. |
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Pluto is the farthest planet from the Sun
(usually) and by far the smallest of the nine planets. |
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Discovered in 1930, Pluto has always appeared as
nothing more than a dot of light in even the largest earth-based
telescopes. The Hubble Space
Telescope is able to get better images of this distant planet. |
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Pluto is 2/3 the size of Earth's Moon but 1,200
times farther away. Viewing surface detail is as difficult as trying to
read the printing on a golf ball located thirty-three miles away! |
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This shows Pluto on the left and its moon Chiron
on the right. By comparing them to
the map of the United States, you can see how small they are. |
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About 4 billion years ago, a 100 kilometer-wide asteroid
struck Mercury creating an impact crater that is 1300 kilometers wide. The Caloris
Basin, as the crater is called, could hold the entire state of Texas! |
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The greenhouse effect is the term used to
describe the way a planet’s atmosphere traps heat and warms a planet. |
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The sun’s
energy passes through the atmosphere and heats up the surface of the
planet. Some of that heat is
trapped by gasses in the air such as carbon dioxide. |
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Average Distance From Sun |
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Kilometers: 57,000,000 |
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Miles: 36,000,000 |
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Astronomical Units: 0.387 |
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Length of Year: 87.97 days |
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Length of Day: 58 days 15 hours 30 minutes |
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Average Orbital Speed |
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Kilometers/Second: 47.89 |
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Miles/Second: 29.76 |
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Equatorial Diameter |
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Kilometers: 4,878 |
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Miles: 3,031 |
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Earth=1: 0.382 |
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Mass (Earth=1): 0.056 |
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Volume (Earth=1): 0.056 |
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Number of Known Satellites: 0 |
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Average Distance From Sun |
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Kilometers: 108,200,000 |
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Miles: 67,000,000 |
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Astronomical Units: 0.723 |
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Length of Year: 224.7 days |
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Length of Day: 243 days 0 hours 25 minutes
(Retrograde) |
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Average Orbital Speed |
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Kilometers/Second: 35.03 |
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Miles/Second: 21.77 |
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Equatorial Diameter |
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Kilometers: 12,100 |
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Miles: 7,518 |
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Earth=1: 0.949 |
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Mass (Earth=1): 0.815 |
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Volume (Earth=1): 0.855 |
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Number of Known Satellites: 0 |
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Average Distance From Sun |
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Kilometers: 149,600,000 |
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Miles: 93,000,000 |
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Astronomical Units: 1.000 |
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Length of Year: 365.26 days |
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Length of Day: 23 hours 56 minutes 4 seconds |
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Average Orbital Speed |
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Kilometers/Second: 29.79 |
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Miles/Second: 18.51 |
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Equatorial Diameter |
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Kilometers: 12,756 |
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Miles: 7,926 |
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Earth=1: 1.000 |
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Mass (Earth=1): 1.000 |
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Volume (Earth=1): 1.000 |
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Number of Known Satellites: 1 |
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Average Distance From Earth |
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Kilometers: 384,500 |
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Miles: 238,900 |
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Astronomical Units: 0.0026 |
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Length of Year (To Orbit Earth): 27.32 days |
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Length of Day: 27 days 7 hours 43 minutes |
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Average Orbital Speed |
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Kilometers/Second: 1.023 |
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Miles/Second: 0.636 |
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Equatorial Diameter |
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Kilometers: 3,476 |
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Miles: 2,160 |
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Earth=1: 0.24 |
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Mass (Earth=1): 0.012 |
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Volume (Earth=1): 0.020 |
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Average Distance From Sun |
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Kilometers: 227,900,000 |
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Miles: 141,600,000 |
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Astronomical Units: 1.524 |
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Length of Year: 1.88 years |
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Length of Day: 24 hours 37 minutes 12 seconds |
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Average Orbital Speed |
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Kilometers/Second: 24.13 |
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Miles/Second: 14.99 |
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Equatorial Diameter |
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Kilometers: 6,796 |
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Miles: 4,223 |
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Earth=1: 0.532 |
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Mass (Earth=1): 0.107 |
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Volume (Earth=1): 0.151 |
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Number of Known Satellites: 2 |
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Average Distance From Sun |
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Kilometers: 778,300,000 |
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Miles: 483,600,000 |
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Astronomical Units: 5.203 |
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Length of Year: 11.86 years |
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Length of Day: 9 hours 50 minutes 33 seconds (at
equator) |
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Average Orbital Speed |
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Kilometers/Second: 13.06 |
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Miles/Second: 8.12 |
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Equatorial Diameter |
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Kilometers: 143,000 |
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Miles: 89,353 |
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Earth=1: 11.27 |
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Mass (Earth=1): 317.89 |
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Volume (Earth=1): 1,403 |
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Number of Known Satellites: 27 (plus rings) |
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Average Distance From Sun |
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Kilometers: 1,427,000,000 |
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Miles: 886,700,000 |
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Astronomical Units: 9.539 |
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Length of Year: 29.46 years |
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Length of Day: 10 hours 39 minutes 24 seconds
(at equator) |
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Average Orbital Speed |
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Kilometers/Seconds: 9.64 |
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Miles/Second: 5.99 |
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Equatorial Diameter |
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Kilometers: 120,000 |
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Miles: 74,565 |
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Earth=1: 9.44 |
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Mass (Earth=1): 95.15 |
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Volume (Earth=1): 833 |
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Number of Known Satellites: 22 (plus rings) |
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Average Distance From Sun |
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Kilometers: 2,870,000,000 |
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Miles: 1,783,000,000 |
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Astronomical Units: 19.18 |
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Length of Year: 84.01 years |
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Length of Day: 17 hours 14 minutes ? seconds
(Retrograde) |
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Average Orbital Speed |
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Kilometers: 6.81 |
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Miles: 4.23 |
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Equatorial Diameter |
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Kilometers: 50,800 |
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Miles: 31,600 |
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Earth=1: 4.10 |
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Mass (Earth=1): 14.54 |
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Volume (Earth=1): 63.0 |
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Number of Known Satellites: 21 (plus rings) |
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Average Distance From Sun |
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Kilometers: 4,497,000,000 |
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Miles: 2,794,000,000 |
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Astronomical Units: 30.06 |
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Length of Year: 164.8 years |
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Length of Day: 18 hours 25 minutes 55 seconds |
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Average Orbital Speed |
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Kilometers/Second: 5.43 |
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Miles/Second: 3.37 |
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Equatorial Diameter |
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Kilometers: 49,500 |
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Miles: 30,758 |
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Earth=1: 3.88 |
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Mass (Earth=1): 17.23 |
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Volume (Earth=1): 55.3 |
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Number of Known Satellites: 8 (rings) |
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Average Distance From Sun |
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Kilometers: 5,913,520,000 |
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Miles: 3,666,000,000 |
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Astronomical Units: 39.44 |
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Length of Year: 248.54 years |
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Length of Day: 6 days 9 hours 17 minutes |
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Average Orbital Velocity |
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Kilometers/Second: 4.74 |
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Miles/Second: 2.95 |
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Equatorial Diameter |
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Kilometers: 2,294 |
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Miles: 1,425 |
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Earth=1: 0.18 |
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Mass (Earth=1): 0.0022 |
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Volume (Earth=1): 0.013? |
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Number of Known Satellites: 1 |
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Facts Slides: |
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Bell , Richard S. . "The Solar
System." Stargazer Online.
<http://my.voyager.net/stargazer/solar_system.html>. |
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Text: |
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Smith, Gail . "The Planets." The
Planets of Our Solar System.
<http://scils.rutgers.edu/~gails/planets.html>. |
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Windows to the Universe. University Corporation
for Atmospheric Research. <http://www.windows.ucar.edu/>. |
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All pictures are believed to by public domain. |
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