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Jupiter
The Bringer of Jollity Jupiter is the fifth planet from the Sun,
the largest in the solar system.
Orbit: 778,330,000 km (483,654,262 miles) or (5.20
AU) from Sun
Diameter: 142,984 km (88850 miles)
Mass: 1.900 x 1027 kg
(3.838 x 1027 lbs)
In mythology, Jupiter (also known as Jove or Zeus) was
the King of the Gods, the ruler of Olympus and the patron of the Roman
state. Zeus was the son of Cronus (Saturn).
If Jupiter were hollow, more than one thousand Earths
could fit inside. It also contains more matter than all of the other
planets combined. It has a mass of 1.9 x 1027 kg and is 142,800 kilometers
(88,736 miles) across the equator. Jupiter possesses 16 satellites,
four of which - Callisto, Europa, Ganymede and Io - were observed by
Galileo as long ago as 1610. There is a ring system, but it is very
faint and totally invisible from the Earth. (The ring was discovered
in 1979 by Voyager 1.)
The atmosphere is very deep, perhaps comprising the whole
planet, and is somewhat like the Sun. It is composed mainly of hydrogen
and helium, with small amounts of methane, ammonia, water vapor and
other compounds. Deep within Jupiter, the pressure is so great that
the hydrogen atoms are broken up and the electrons are freed so that
the resulting atoms consist of bare protons. This produces a state in
which the hydrogen becomes metallic.
Jupiter
was first visited by Pioneer 10 in 1973 and later by Pioneer 11, Voyager
1, Voyager 2 and Ulysses. The spacecraft Galileo is currently in orbit
around Jupiter and will be sending back data for at least the next two
years.
Colorful latitudinal bands, atmospheric clouds and storms
illustrate Jupiter's dynamic weather systems. The cloud patterns change
within hours or days. The Great Red Spot is a complex storm moving in
a counter-clockwise direction. At the outer edge, material appears to
rotate in four to six days; near the center, motions are small and nearly
random in direction. An array of other smaller storms and eddies can
be found throughout the banded clouds.
Auroral emissions, similar to Earth's northern lights,
were observed in the polar regions of Jupiter. The auroral emissions
appear to be related to material from Io that spirals along magnetic
field lines to fall into Jupiter's atmosphere. Cloud-top lightning bolts,
similar to superbolts in Earth's high atmosphere, were also observed.
In July 1994, Comet Shoemaker-Levy 9 collided with Jupiter
with spectacular results. The effects were clearly visible even with
amateur telescopes. The debris from the collision was visible for nearly
a year afterward with HST. Jupiter's Ring Unlike Saturn's intricate
and complex ring patterns, Jupiter has a single ring that is almost
uniform in its structure. It is probably composed of dust particles
less than 10 microns in diameter-about the size of cigarette smoke particles.
It extends to an outer edge of about 129,000 kilometers (80,161 miles)
from the center of the planet and inward to about 30,000 kilometers
(18,642 miles). The origin of the ring is probably from micrometeorite
bombardment of the tiny moons orbiting within the ring.
Jupiter's ring and moons exist within an intense radiation
belt of electrons and ions trapped in the planet's magnetic field. These
particles and fields comprise the jovian magnetosphere or magnetic environment,
which extends 3 to 7 million kilometers (1.9 to 4.3 million miles) toward
the Sun, and stretches in a windsock shape at least as far as Saturn's
orbit-a distance of 750 million kilometers (466 million miles).
The Galileo atmospheric probe discovered a new intense
radiation belt between Jupiter's ring and the uppermost atmospheric
layers. This new belt is approximately 10 times as strong as Earth's
Van Allen radiation belts. Surprisingly, this new belt was also found
to contain high energy helium ions of unknown origin.
Values for the smaller moons are approximate.
| Jupiter's Ring |
Distance(km) |
Width(km) |
Mass (kg) |
| Halo |
100000 |
22800 |
? |
| Main |
122800 |
64000 |
le13 |
| Gossamer |
120200 |
850000 |
? |
Jupiter's satellites are named for other figures in mythology.
| Satellite |
Distanct (000km) |
Radius (km) |
Mass (kg) |
Discoverer |
Date |
| Metis |
128 |
20 |
9.57e16 |
Synott |
1979 |
| Adrastea |
129 |
10 |
1.91e16 |
Jewitt |
1979 |
| Amalthea |
181 |
98 |
7.17e18 |
Barnard |
1982 |
| Thebe |
222 |
50 |
7.77e17 |
Synott |
1979 |
| Io |
422 |
1815 |
8.94e22 |
Galileo |
1610 |
| Europa |
671 |
1569 |
4.80e22 |
Galileo |
1610 |
| Ganymede |
1070 |
2631 |
1.48e23 |
Galileo |
1610 |
| Callisto |
1883 |
2400 |
1.08e23 |
Galileo |
1610 |
| Leda |
11094 |
8 |
5.68e15 |
Kowal |
1964 |
| Himalia |
11480 |
93 |
9.56e18 |
Perrine |
1904 |
| Lysithea |
11720 |
18 |
7.77e16 |
Nicholson |
1938 |
| Elara |
11737 |
38 |
7.77e17 |
Perrine |
1905 |
| Ananke |
21200 |
15 |
3.82e16 |
Nicholson |
1951 |
| Carme |
22600 |
20 |
9.56e16 |
Nicholson |
1938 |
| Pasiphae |
23500 |
25 |
1.91e17 |
Melotte |
1908 |
| Sinope |
23700 |
18 |
7.77e16 |
Nicholson |
1914 |

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