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Jupiter is one of the most interesting planets in the solar
system. It is a gas giant with storms that are larger than
the planet Earth, a thick poisonous atmosphere, a diverse system
of moons, and even thin, faint rings. It is a great
telescope target. Jupiter rotates about every 10 hours, so
from night to night, it looks different. Most of the
visible clouds on Jupiter are made of ammonia. Strong east
and west winds form the bands that are easily viewable in most
telescopes. Water has been detected on the planet.
Due to its thick atmosphere, we have not been able to peer at
its core, but it is suspected to contain a small rocky core,
possible the size of earth (which is miniscule compared to the
overall size of Jupiter).

Jupiter Cloud Motion
Jupiter has storm called the Great Red Spot (GRS) which is also
visible in most telescopes. the GRS has been raging for
over 300 years. It is about 3 times the size of Earth.
The Great Red Spot changes color from dark red to white to a
dark pink. The Great Red Spot is far from the only storm
on Mars. It just so happens to be the largest and most
dynamic.

Great Red Spot in Motion
Jupiter has an enormous magnetic field that is 20,000 times
larger than that of Earth. It extends almost 1 million
miles toward the Sun. The solar wind "pushes" most of the
the magnetic field away from the sun and causes it to extend 1
billion miles behind Jupiter, reaching all the way to Saturn.
Jupiter also has a thin, faint ring system. The rings were
discovered by Voyager 1 in 1979. The rings are only
visible when the are lit from the back by the Sun, so they are
only visible when you are on the other side of Jupiter relative
to the Earth. Thus, no Earth based telescopes can see the
rings.
Jupiter has been visited by Pioneer 10, Pioneer 11, Galileo,
Voyager 1, Voyager 2, Cassini, and most recently the New
Horizons Spacecraft flew by on its way to Pluto. Jupiter
missions present a real challenge for spacecraft engineers due
to the intense radiation it gives off.
Jupiter is almost a solar system unto itself. Various
spacecraft to have visited Jupiter have located a total of 49
moons! The outer moons are most likely asteroids that got
caught up in Jupiter's gravity and entered its orbit. From ground based telescopes, we can see the four
largest moons, Io, Ganymede, Europa, and Callisto. They
revolve around Jupiter rather fast and you can see them change
position throughout the night. Sky & Telescope has a
great
tool to determine
the positions of these four moons for any date
and time.
Jupiter's moon Io is the most volcanically active body in the
solar system. Jupiter's intense gravity tugs and pulls Io
causing it to deform, heating up its core and causing volcanoes
to spew throughout the moon. The surface is a yellow color
due to deposits of sulfur.
Europa is a moon that is thought to be a large body of water
(twice as much water as on Earth) encapsulated by a thin layer
of ice. The liquid water underneath the surface does not
freeze because there is some heat source inside. We can
surmise that there is liquid water underneath the ice because of
the cracks in the surface with water that flows up and freezes
over creating new surface ice. Astrobiologists are excited
about the prospect of liquid water that may support life.
Life has been found in thermal vents on the bottom of the ocean
on Earth, which may be similar to the conditions on Europa.
Ganymede is actually larger than Mercury and is the largest
known moon of an any planet. Ganymede is thought to have a
rocky core surrounded by a large amount of ice and topped off
with a thin layer ice and rock mixed together.
Callisto's surface is littered with ancient craters. There
are no real defined layers on Callisto. The moon is
thought to be one big mixture of ice and rock. A fine dust
covers the surface of Callisto, including its craters.
| Mass (kg)
| 1.90 x 1027
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| Diameter (km)
| 142,800
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| Mean density (kg/m3)
| 1314
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| Escape velocity (m/s)
| 59500
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| Average distance from Sun
| 5.203 AU (778,412,020 km)
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| Rotation period (length of day in Earth days)
| 0.41 (9.8 Earth hours)
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| Revolution period (length of year in Earth years)
| 11.86
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| Obliquity (tilt of axis degrees)
| 3.08
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| Orbit inclination (degrees)
| 1.3
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| Orbit eccentricity (deviation from circular)
| 0.048
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| Mean surface temperature (K)
| 120 (cloud tops)
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| Visual geometric albedo (reflectivity)
| 0.44
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| Atmospheric components
| 90% hydrogen,
10% helium,
.07% methane
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| Rings
| Faint ring.
Infrared spectra imply dark rock fragments.
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Image of
The Planet Jupiter

Photograph of
Jupiter's Moon Callisto

Picture of the
Surface of Europa

Picture of
Jupiter's
Moon
Ganymede

Image of
Jupiter's Moon Io
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