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natural satellite comparison table
Subject is part of has diameter has orbital period has inclination is an instance of has rotation period has mean density has eccentricity has dicoverer has albedo has crust thickness has radiu has mean distance from Earth has obliquity has surface composition has mean radiu has synodic period has core temperature has sidereal period has center of mass location has period has diameter about has atmosphere composition has surface gravity has orbital velocity has discoverer has rotational period is a kind of has eccetricity has V< i>esc has mass has dicovery date has inclination of orbital plane to ecliptic has mantle thickness has synonym has definition has discovery date
AmaltheaJupiter140 km0.498 daysi = 0°.4natural satellite  e = 0.0028                 Barnard        Barnard's satelliteThe innermost satellite of Jupiter.1892
ArielUranus1600 km  natural satellite               2.52 days    Lassell         Second satellite of Uranus.1851
DeimosMars P = 1.26 days1°.6natural satellite  e = 0.003 0.06 12 × 13 km             A. Hall         The outer satellite of Mars. Mariner 9 has shown that both Phobos and Deimos are locked in synchronous rotation with Mars.1897
DemeterJupiter P = 259.2 daysi = 29°natural satellite  e = 0.12                 Nicholson         Unofficial name for Jupiter X.1938
DioneSaturn P = 4.5 days natural satellite      440 km             Cassini         Fifth satellite of Saturn1684
EnceladusSaturn500 km1.37 days natural satellite                    Herschel         Third satellite of Saturn1789
Galilean satelliteJupiter                        Galileo natural satellite       The largest satellites of Jupiter - Io, Europa, Ganymede, and Callisto. All are locked in synchronous rotation with Jupiter.1610
HadesJupiter P = 758 days retrogradei = 156°natural satellite  e = 0.28                 Nicholson        Jupiter IXAn unofficial name for Jupiter IX, the outermost satellite of Jupiter.1914
HeraJupiter P = 259.65 daysi = 28°natural satellite  e = 0.21                 Perrine        Jupiter VIIUnofficial name for Jupiter VII.1905
HestiaJupiter P = 250 daysi = 29°natural satellite  e = 0.16                 Perrine        Jupiter VIUnofficial name for Jupiter VI.1904
HyperionSaturn160 kmP = 21d6h38m natural satellite                    Bond         Eighth satellite of Saturn1848.
IapetusSaturn  inclination 14°.7 to Saturn's orbital planenatural satellite      850±100 km        79d7h55m       e = 0.028      The ninth satellite of Saturn. It has the most extreme variation in albedo of any satellite in the solar system (0.04 for the leading side, 0.28 for the trailing side). Discovered by Cassini in 1671. 
JanusSaturn  i ≈ 0natural satellite  e ≈ 0   R = 175 km        P = 0.75 days    Dollfus         The innermost satellite of Saturn, just outside Saturn's rings. Named Janus for the first and the last.1966
MimasSaturn P = 0d.94 natural satellite    0.49 R ≈ 250 km             Herschel     1789   The second innermost satellite of Saturn. The perturbations of Mimas and Janus produce the divisions in Saturn's rings. 
MirandaUranus500 kmP = 1d10h natural satellite                    Kuiper         The innermost satellite of Uranus.1948
MoonEarth   natural satellite 3.34 g cm-3e = 0.0549 0.0760 km 384404.377 ± 0.001 km (1.28 lt-sec)6°41' 1738 km29d12h44m2s.91500 K27d7h43m11sdisplaced about 2 km from geometrical center towards the direction of Earth   162.2 cm s-2 = 0.165 Earth'sVorb = 1.02 km s-1    2.38 km s-17.35 × 1025 g = 0.0123 MEarth 5°8'43"1000 km Natural satellite of Earth. Studies of lunar rocks have shown that melting and separation must have begun at least 4.5 × 109 years ago,so the crust of the Moon was beginning to form a very short time after the solar system itself. It would have taken only 107 years to slow the Moon's rotation into its present lock with its orbital period. The Moon's orbit is always concave toward the Sun. 
NereidNeptune about 360 days direct natural satellite  e = 0.76   150-250 km             Kuiper         The outer satellite of Neptune. It has the most eccentric orbit of any natural satellite.1950
OberonUranus P = 13.46 days natural satellite      R ≥ 500 km             Herschel13.46 days        Outermost satellite of Uranus.1787
PanJupiter P = 692di = 163°natural satellite  e = 0.2Nicholson                         Jupiter XIUnofficial name for Jupiter XI.1938
PhobosMars 7h39m14si = 1°.1natural satellite7h39m14s e = 0.021 0.06 about 18 × 22 km  dust (from Infrared observations)          A. Hall         The potato-shaped inner satellite of Mars. Phobos lies just outside the Martian Roche limit.1877
PhoebeSaturn 550 days natural satellite      100 km             Pickering         The outermost satellite of Saturn. Has retrograde orbit.1898
PoseidonJupiter P = 737di = 147°natural satellite  e = 0.4                 Melotte        Jupiter VIIIUnofficial name for J VIII, the next outermost satellite of Jupiter.1908
RheaSaturn   natural satellite4d12h25m   0.57           1500 km   Cassini         Sixth satellite of Saturn1672
TethysSaturn1000 kmP = 1.87 days natural satellite                    Cassini         Fourth satellite of Saturn1684
ThemisSaturn   natural satellite                              A satellite of Saturn discovered by Pickering in 1900, but since lost. 
TitanSaturn 15d22h41m natural satellite15d22h41m   0.21 R ≈ 2900 km          H2 and CH4  Huyghens        S VISeventh (known) moon out from Saturn, its largest and brightest. It is possibly also the largest satellite in the Solar System.1655
TitaniaUranus P = 8d17h natural satellite      R ≈ 850 km             Herschel         Fourth satellite of Uranus.1787
TritonNeptune   natural satellite                              The inner satellite of Neptune, discovered by Lassell in 1846. It is larger than the Moon (R ≈ 2900 km), with an almost circular retrograde orbit of 5 days 21 hours. 
UmbrielUranus 4.1 days natural satellite      200 km             Lassell         A satellite of Uranus.1851

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