Tidbit: Jupiter contains a majority (about 2/3) of the planetary mass in the solar system.
Distance Radius Mass Satellite (000 km) (km) (kg) Discoverer Date --------- -------- ------ ------- ---------- ----- Metis 128 20 9.56e16 Synnott 1979 Adrastea 129 10 1.91e16 Jewitt 1979 Amalthea 181 98 7.17e18 Barnard 1892 Thebe 222 50 7.77e17 Synnott 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 1974 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
Values for the smaller moons are approximate. Many more small moons are not listed here.
Another tidbit: the four Galilean moons (Io, Europa, Ganymede, and Callisto) are tidally locked to Jupiter; just like the Earth's moon, they always have one side facing their parent planet. This is also the case for some of the other moons, but not all. Plus we still don't know the orbital periods for several of the smaller moons.
Jupiter's moons orbit as close as 80,000 miles (within the main ring!) in the case of Metis, and as far away as 16,500,000 miles in the case of Sinope!