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Jupiter

Voyager 1 photo of Jupiter  Voyager 2 close-up of Jupiter cloud features Cassini mosaic image of Jupiter
Voyager 1 photo of Jupiter (NASA/JPL) Voyager 2 close-up of Jupiter cloud features (NASA/JPL) Cassini mosaic image of Jupiter (NASA/JPL/Space Science Institute)




King of the Gods

As we enter the Jovian system, we are presented with a truly awesome sight. It is a gaseous planet of enormous proportions. This is the planet Jupiter. It is the fifth planet from the Sun and is the largest. In fact, Jupiter is almost twice the size of all of the other planets combined. Over one thousand Earths could fit inside if it were hollow. Because of its gigantic size, Jupiter was named after the king of the gods in Roman mythology. In Greek mythology, he was known as Zeus, and was famous for hurling lightning bolts at earthbound mortals. Jupiter is the fourth brightest object in the sky, so it has been known to exist since prehistoric times. But it was Galileo who discovered Jupiter's four largest moons, Callisto, Europa, Ganymede, and Io, in 1610. We now know of 63 moons in orbit around Jupiter, ranging in size from just a few miles across to nearly Earth-sized. The Jovian system is like a miniature solar system within a solar system. With so many satellites tugging on Jupiter with their tidal forces, these moons are actually causing Jupiter's rotation to slow down. These same tidal forces are also pushing the moons farther away from the massive planet.


Voyager 2 closeup of Jupiter's famous red spot Galileo image of Jipiter's moon Io Voyager 1 close-up of Jupiter's cloud details
Voyager 2 closeup of Jupiter's famous red spot (NASA/JPL) Galileo image of Jipiter's moon Io
(NASA/JPL/University of Arizona)
Voyager 1 close-up of Jupiter's cloud details (NASA/JPL)


The Famous Red Spot

One of the most famous features of Jupiter is the giant red spot. This spot is actually a gigantic storm system. It is a high-pressure region where the winds blow in a counter-clockwise direction at over 250 miles (402 km) per hour. The cloud tops are much higher and colder than the surrounding clouds. This accounts for the spot's darker color. With a diameter of more than 16,000 miles (25,000 km), this storm is twice the size of the Earth!  Many spots and colorful bands appear and disappear in Jupiter's turbulent atmosphere, but the great red spot has been know to exist for more than 300 years. Astronomers do not yet know what forces have kept this storm together for so long. And nobody knows just how much longer it will last. Spots of a different kind were seen in 1994 when a comet named Shoemaker-Levy 9 smashed into the planet. The comet had broken into 21 separate fragments as a result of a close encounter with Jupiter's massive gravitational forces. On July 16 1994, for seven days, these fragments bombarded the giant planet. The impacts left monstrous black scars on the Jupiter's surface. Explosive plumes several times the size of Earth were observed, and the dark scars remained visible on the planet for nearly a year. It was one of the most watched astronomical events in history, and it proved once and for all that comets do hit planets.


Features of Jupiter

Jupiter has amazed and intrigued astronomers for centuries. It has been visited by a total of six spacecraft, including the current Galileo mission. In 1995, Galileo dropped a probe into Jupiter's atmosphere. The probe took measurements and gave us our first clues as to what was inside Jupiter's thick atmosphere. With this data, and data collected on previous missions, we now know that Jupiter is essentially a gigantic ball of gas. The planet is composed mainly of hydrogen, with helium and traces amounts of other gases. One surprising find was that there is much less water in Jupiter's atmosphere than previously expected. Astronomers believe that Jupiter has no solid surface. Instead the gases get thicker and denser as they get closer to the planet's center. The extreme pressure at Jupiter's core compresses the hydrogen into a rare liquid metallic state. The planet may also have a small, rocky core about 10 times the size of Earth. Jupiter's outer atmosphere is extremely dynamic. Colorful bands and spots can be see rotating and changing regularly. The colors in the bands are believed to be the result of chemical reactions in the atmosphere. The Galileo probe measured wind speeds exceeding 400 miles (643 km) per hour. A big surprise revealed by the Voyager 1 spacecraft was that Jupiter has rings, much like Saturn. But unlike Saturn's rings, Jupiter's rings are very delicate and simple. These rings are divided into three main segments, and were not known to exist prior to Voyager's discovery because they are too thin to be seen from Earth. One other item in Jupiter's long list of oddities is its magnetic field. It is so strong that is actually extends past the orbit of Saturn. In fact, it is 4000 times stronger than Earth's magnetic field. Even stranger still is the fact that Jupiter's rotation is so fast - only 9.8 Earth hours - that the planet actually bulges out in the center. A close examination of any Jupiter photo will reveal that the planet is more oval shaped than round.

 

Statistics for Jupiter
Diameter...... 88,823 miles (142,984 km)
Number of Natural Satellites...... 16
Mean Distance from the Sun...... 482,546,000 miles (778,330,000 km)
Rotational Period...... 9.84 hours
Orbital Period...... 4333 days
Orbital Eccentricity...... 0.0483
Orbital Inclination...... 1.308 degrees
Inclination of Axis...... 3.12 degrees
Mean Cloud Temperature...... -185° F (-121° C)
Main Atmospheric Component...... Hydrogen
Atmospheric Pressure...... 0.7 bars
Atmospheric Depth...... 100 miles (161 km)
Apparent Magnitude...... -2.7

 

The Moons of Jupiter
Listed in order of distance from Jupiter
Click on linked names for more information
Name   Diameter (km)    Distance (km)   Year
   Discovered  
Metis 44 128,100 1979
Adrastea 16 128,900 1979
Amalthea 168 181,400 1892
Thebe 98 221,900 1979
Io 3643 421,800 1610
Europa 3122 671,100 1610
Ganymede 5262 1,070,400 1610
Callisto 4821 1,882,700 1610
Themisto 9 7,507,000 2000
Leda 18 11,165,000 1974
Himalia 184 11,461,000 1904
Lysithea 38 11,717,000 1938
Elara 78 11,741,000 1905
S/2000 J11 4 12,555,000 2000
Carpo 3 17,144,900 2003
S/2003 J12 1 17,739,600 2003
Euporie 2 19,302,000 2001
S/2003 J3 2 19,621,800 2003
S/2003 J18 2 19.812.600 2003
Thelxinoe 2 20,453,800 2004
Euanthe 3  20,464,800 2002
Helike 4 20,540,300 2003
Orthosie 2  20,568,000 2002
Locaste 5 20,722,600 2001
S/2003 J16 2 20,743,800 2003
Praxidike 7  20,824,000 2001
Harpalyke 4  21,063,900 2001 
Mneme 2 21,129,800 2003
Hermippe 4  21,182,100 2002
Thyone 4  21,405,600 2002
Ananke 28 21,455,000 1951
S/2003 J17 2 22,134,400 2003
Aitne 3  22,285,200 2002
Kale 2  22,409,200 2002
Taygete 5 22,438,700 2001
S/2003 J19 2 22,709,000 2003
Chaldene 4 22,713,400 2001
S/2003 J15 2 22,721,000 2003
S/2003 J10 2 22,730,800 2003
S/2003 J23 2 22,739,700 2003
Erinome 3 22,986,300 2001
Aoede 4 23,044,200 2003
Kallichore 2 23,111,800 2003
Kalyke 5 23,180,800 2001
Carme 46 23,404,000 1938
Callirrhoe 9 23,215,000 2000
Eurydome 3 23,230,900 2002
Pasithee 2 23,307,300 2002
Cyllene 2 23,396,300 2003
Eukelade 4 23,483,700 2003
S/2003 J4 2 23,570,800 2003
Pasiphae 60 23,624,000 1908
Hegemone 3 23,702,500 2003
Arche 3 23,717,000 2002
Isonoe 4 23,800,600 2001
S/2003 J9 1 23,857,800 2003
S/2003 J5 4 23,973,900 2003
Sinope 38 23,939,000 1914
Sponde 2 24,252,400 2002
Autonoe 4 24,264,400 2002
Kore 2 23,345,000 2003
Megaclite 5 24,687,200 2001
S/2003 J2 2 30,290,800 2003

 

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