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 |
Amalthea | Jupiter | 140 km | 0.498 days | i = 0°.4 | natural satellite | | | e = 0.0028 | | | | | | | | | | | | | | | | | | Barnard | | | | | | | | | Barnard's satellite | The innermost satellite of Jupiter. | 1892 |
Ariel | Uranus | 1600 km | | | natural satellite | | | | | | | | | | | | | | | | 2.52 days | | | | | Lassell | | | | | | | | | | Second satellite of Uranus. | 1851 |
Deimos | Mars | | P = 1.26 days | 1°.6 | natural 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 |
Demeter | Jupiter | | P = 259.2 days | i = 29° | natural satellite | | | e = 0.12 | | | | | | | | | | | | | | | | | | Nicholson | | | | | | | | | | Unofficial name for Jupiter X. | 1938 |
Dione | Saturn | | P = 4.5 days | | natural satellite | | | | | | | 440 km | | | | | | | | | | | | | | Cassini | | | | | | | | | | Fifth satellite of Saturn | 1684 |
Enceladus | Saturn | 500 km | 1.37 days | | natural satellite | | | | | | | | | | | | | | | | | | | | | Herschel | | | | | | | | | | Third satellite of Saturn | 1789 |
Galilean satellite | Jupiter | | | | | | | | | | | | | | | | | | | | | | | | | Galileo | | natural satellite | | | | | | | | The largest satellites of Jupiter - Io, Europa, Ganymede, and Callisto. All are locked in synchronous rotation with Jupiter. | 1610 |
Hades | Jupiter | | P = 758 days retrograde | i = 156° | natural satellite | | | e = 0.28 | | | | | | | | | | | | | | | | | | Nicholson | | | | | | | | | Jupiter IX | An unofficial name for Jupiter IX, the outermost satellite of Jupiter. | 1914 |
Hera | Jupiter | | P = 259.65 days | i = 28° | natural satellite | | | e = 0.21 | | | | | | | | | | | | | | | | | | Perrine | | | | | | | | | Jupiter VII | Unofficial name for Jupiter VII. | 1905 |
Hestia | Jupiter | | P = 250 days | i = 29° | natural satellite | | | e = 0.16 | | | | | | | | | | | | | | | | | | Perrine | | | | | | | | | Jupiter VI | Unofficial name for Jupiter VI. | 1904 |
Hyperion | Saturn | 160 km | P = 21d6h38m | | natural satellite | | | | | | | | | | | | | | | | | | | | | Bond | | | | | | | | | | Eighth satellite of Saturn | 1848. |
Iapetus | Saturn | | | inclination 14°.7 to Saturn's orbital plane | natural 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. | |
Janus | Saturn | | | i ≈ 0 | natural 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 |
Mimas | Saturn | | 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. | |
Miranda | Uranus | 500 km | P = 1d10h | | natural satellite | | | | | | | | | | | | | | | | | | | | | Kuiper | | | | | | | | | | The innermost satellite of Uranus. | 1948 |
Moon | Earth | | | | natural satellite | | 3.34 g cm-3 | e = 0.0549 | | 0.07 | 60 km | | 384404.377 ± 0.001 km (1.28 lt-sec) | 6°41' | | 1738 km | 29d12h44m2s.9 | 1500 K | 27d7h43m11s | displaced about 2 km from geometrical center towards the direction of Earth | | | | 162.2 cm s-2 = 0.165 Earth's | Vorb = 1.02 km s-1 | | | | | 2.38 km s-1 | 7.35 × 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. | |
Nereid | Neptune | | 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 |
Oberon | Uranus | | P = 13.46 days | | natural satellite | | | | | | | R ≥ 500 km | | | | | | | | | | | | | | Herschel | 13.46 days | | | | | | | | | Outermost satellite of Uranus. | 1787 |
Pan | Jupiter | | P = 692d | i = 163° | natural satellite | | | e = 0.2 | Nicholson | | | | | | | | | | | | | | | | | | | | | | | | | | Jupiter XI | Unofficial name for Jupiter XI. | 1938 |
Phobos | Mars | | 7h39m14s | i = 1°.1 | natural satellite | 7h39m14s | | 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 |
Phoebe | Saturn | | 550 days | | natural satellite | | | | | | | 100 km | | | | | | | | | | | | | | Pickering | | | | | | | | | | The outermost satellite of Saturn. Has retrograde orbit. | 1898 |
Poseidon | Jupiter | | P = 737d | i = 147° | natural satellite | | | e = 0.4 | | | | | | | | | | | | | | | | | | Melotte | | | | | | | | | Jupiter VIII | Unofficial name for J VIII, the next outermost satellite of Jupiter. | 1908 |
Rhea | Saturn | | | | natural satellite | 4d12h25m | | | | 0.57 | | | | | | | | | | | | 1500 km | | | | Cassini | | | | | | | | | | Sixth satellite of Saturn | 1672 |
Tethys | Saturn | 1000 km | P = 1.87 days | | natural satellite | | | | | | | | | | | | | | | | | | | | | Cassini | | | | | | | | | | Fourth satellite of Saturn | 1684 |
Themis | Saturn | | | | natural satellite | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | A satellite of Saturn discovered by Pickering in 1900, but since lost. | |
Titan | Saturn | | 15d22h41m | | natural satellite | 15d22h41m | | | | 0.21 | | R ≈ 2900 km | | | | | | | | | | | H2 and CH4 | | | Huyghens | | | | | | | | | S VI | Seventh (known) moon out from Saturn, its largest and brightest. It is possibly also the largest satellite in the Solar System. | 1655 |
Titania | Uranus | | P = 8d17h | | natural satellite | | | | | | | R ≈ 850 km | | | | | | | | | | | | | | Herschel | | | | | | | | | | Fourth satellite of Uranus. | 1787 |
Triton | Neptune | | | | 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. | |
Umbriel | Uranus | | 4.1 days | | natural satellite | | | | | | | 200 km | | | | | | | | | | | | | | Lassell | | | | | | | | | | A satellite of Uranus. | 1851 |