Jupiter's Statistics

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Michael Ammar
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 Mass (kg) 1.900e+27 
 Mass (Earth = 1) 3.1794e+02 
 Equatorial radius (km) 71,492 
 Equatorial radius (Earth = 1) 1.1209e+01 
 Mean density (gm/cm^3) 1.33 
 Mean distance from the Sun (km) 778,330,000 
 Mean distance from the Sun (Earth = 1) 5.2028 
 Rotational period (days) 0.41354 
 Orbital period (days) 4332.71 
 Mean orbital velocity (km/sec) 13.07 
 Orbital eccentricity 0.0483 
 Tilt of axis (degrees) 3.13 
 Orbital inclination (degrees) 1.308 
 Equatorial surface gravity (m/sec^2) 22.88 
 Equatorial escape velocity (km/sec) 59.56 
 Visual geometric albedo 0.52 
 Magnitude (Vo) -2.70 
 Mean cloud temperature -121�C 
 Atmospheric pressure (bars) 0.7 
 Atmospheric composition
Hydrogen
Helium

90% 
10% 

 

Jupiter's Rings

 
Name Distance* Width Thickness Mass Albedo
Halo 92,000 km 30,500 km 20,000 km ? 0.05
Main 122,500 km 6,440 km < 30 km 1 x 10^13 kg 0.05
Inner Gossamer 128,940 km 52,060 km ? ? 0.05
Outer Gossamer 181,000 km 40,000 km ? ? 0.05

 

Jupiter's Moon Summary

 

Nearly four centuries ago Galileo Galilei turned his homemade telescope towards the heavens and discovered three points of light, which at first he thought to be stars, hugging the planet Jupiter. These stars were arranged in a straight line with Jupiter. Sparking his interest, Galileo observed the stars and found that they moved the wrong way. Four days later another star appeared. After observing the stars over the next few weeks, Galileo concluded that they were not stars but planetary bodies in orbit around Jupiter. These four stars have come to be know as the Galilean satellites.

Over the course of the following centuries another 12 moons were discovered bringing the total to 16. Finally in 1979, the strangeness of these frozen new worlds was brought to light by the Voyager spacecrafts as they swept past the Jovian system. Again in 1996, the exploration of these worlds took a large step forward as the Galileo spacecraft began its long term mission of observing Jupiter and its moons.

Twelve of Jupiter's moons are relatively small and seem to have been more likely captured than to have been formed in orbit around Jupiter. The four large Galilean moons, Io, Europa, Ganymede and Callisto, are believed to have accreted as part of the process by which Jupiter itself formed. The following table summarizes the radius, mass, distance from the planet center, discoverer and the date of discovery of each of the moons of Jupiter:

 

Moon # Radius
(km)
Mass
(kg)
Distance
(km)
Discoverer Date
 Metis XVI 20 9.56e+16 127,969 S. Synnott 1979
 Adrastea XV 12.5x10x7.5 1.91e+16 128,971 Jewitt-Danielson 1979
 Amalthea V 135x84x75 7.17e+18 181,300 E. Barnard 1892
 Thebe XIV 55x45 7.77e+17 221,895 S. Synnott 1979
 Io I 1,815 8.94e+22 421,600 Marius-Galileo 1610
 Europa II 1,569 4.80e+22 670,900 Marius-Galileo 1610
 Ganymede III 2,631 1.48e+23 1,070,000 Marius-Galileo 1610
 Callisto IV 2,400 1.08e+23 1,883,000 Marius-Galileo 1610
 Leda XIII 8 5.68e+15 11,094,000 C. Kowal 1974
 Himalia VI 93 9.56e+18 11,480,000 C. Perrine 1904
 Lysithea X 18 7.77e+16 11,720,000 S. Nicholson 1938
 Elara VII 38 7.77e+17 11,737,000 C. Perrine 1905
 Ananke XII 15 3.82e+16 21,200,000 S. Nicholson 1951
 Carme XI 20 9.56e+16 22,600,000 S. Nicholson 1938
 Pasiphae VIII 25 1.91e+17 23,500,000 P. Melotte 1908
 Sinope IX 18 7.77e+16 23,700,000 S. Nicholson 1914

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Copyright � 1998 Michael Ammar.