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A 'natural satellite' is an object that orbits a planet or other body larger than itself and which is not man-made. Such objects are often called 'moons'. Technically, the term could also refer to a planet orbiting a star, or even to a star orbiting a galactic center, but these uses are rare. Instead, the term is normally used to identify non-artificial satellites of planets, dwarf planets, or minor planets.
There are 240 known moons within the Solar System, including 165 orbiting the planets,^[1] 4 orbiting dwarf planets, and dozens more orbiting small solar system bodies. Other stars and their planets also have natural satellites.
The large gas giants have extensive systems of natural satellites, including half a dozen comparable in size to Earth's moon. Of the inner planets, Mercury and Venus have no moons at all; Earth has one large moon (the Moon); and Mars has two tiny moons, Phobos and Deimos. Among the dwarf planets, Ceres has no moons (though many objects in the asteroid belt do), Eris has one, Dysnomia, and Pluto has three known satellites, Nix, Hydra, and a large companion called Charon. The Pluto-Charon system is unusual in that the center of mass lies in open space between the two, a characteristic of a double planet system.

Contents

Origin

Orbital characteristics

Tidal locking

Satellites of satellites

Trojan satellites

Asteroid satellites

Natural satellites of the Solar System

Terminology

The definition of a moon

See also

Natural satellites of planets and dwarf planets

Natural satellites of small Solar System bodies

Notes and references

External links

Jupiter's moons

Saturn's moons

Neptune's moons

All moons

Origin

The natural satellites orbiting relatively close to the planet on prograde orbits (''regular'' satellites) are generally believed to have been formed out of the same collapsing region of the protoplanetary disk that gave rise to its primary. In contrast, irregular satellites (generally orbiting on distant, inclined, eccentric and/or retrograde orbits) are thought to be captured asteroids possibly further fragmented by collisions. The Earth-Moon^[2] and possibly Pluto-Charon systems^[3] are exceptions among large bodies in that they are believed to have originated by the collision of two large proto-planetary objects (see the giant impact hypothesis). The material that would have been placed in orbit around the central body is predicted to have reaccreted to form one or more orbiting moons. As opposed to planetary-sized bodies, asteroid moons are thought to commonly form by this process.

Orbital characteristics

Tidal locking

Most regular natural satellites in the solar system are tidally locked to their primaries, meaning that one side of the moon is always turned toward the planet. Exceptions include Saturn's moon Hyperion, which rotates chaotically because of a variety of external influences.
In contrast, the outer moons of the gas giants (irregular satellites) are too far away to become 'locked'. For example, Jupiter's moon Himalia, Saturn's moon Phoebe and Neptune's moon Nereid have rotation period in the range of 10 hours compared with their orbital periods of hundreds of days.

Satellites of satellites

No "moons of moons" (natural satellites that orbit the natural satellite of another body) are known. It is uncertain whether such objects can be stable in the long term. In most cases, the tidal effects of their primaries make such a system unstable; the gravity from other nearby objects (most notably the primary) would perturb the orbit of the moon's moon until it broke away or impacted its primary. In theory, a secondary satellite could exist in a primary satellite's Hill sphere, outside of which it would be lost because of the greater gravitational pull of the planet (or other object) that the primary satellite orbits. For example, the Moon orbits Earth because the Moon is 370,000 km from Earth, well within Earth's Hill sphere, which has a radius of 1.5 million km (0.01 AU or 235 Earth radii). If a Moon-sized object were to orbit Earth outside its Hill sphere, it would soon be captured by the Sun and become a dwarf planet in a near-Earth orbit.

Trojan satellites

Two moons are known to have small companions at their L₄ and L₅ Lagrangian points, which are about sixty degrees ahead of and behind the body in its orbit. These companions are called Trojan moons, because their positions are comparable to the positions of the Trojan asteroids relative to Jupiter. Such objects are Telesto and Calypso, which are the leading and following companions respectively of Tethys; and Helene and Polydeuces, which are the leading and following companions of Dione.

Asteroid satellites

The discovery of 243 Ida's moon Dactyl in the early 1990s confirms that some asteroids also have moons. Some, like 90 Antiope, are double asteroids with two equal-sized components. The asteroid 87 Sylvia has two moons. See asteroid moon for further information.

Natural satellites of the Solar System

The largest natural satellites in the Solar System (those bigger than about 3000 km across) are Earth's moon, Jupiter's Galilean moons (Io, Europa, Ganymede, and Callisto), Saturn's moon Titan, and Neptune's captured moon Triton. For smaller moons see the articles on the appropriate planet. In addition to the moons of the various planets there are also over 80 known moons of the dwarf planets, asteroids and other small solar system bodies. Some studies estimate that up to 15% of all trans-Neptunian objects could have satellites.
The following is a comparative table classifying the moons of the solar system by diameter. The column on the right includes some notable planets, dwarf planets, asteroids, and Trans-Neptunian Objects for comparison.
It is normal for natural satellites to be named after mythological figures, (predominately Greek), however Uranus's moons are named after Shakespearean characters.

Mean diameter (km)	Satellites of planets						Dwarf planet satellites		Satellites of SSSBs[4]	Non-satellites for comparison
	Earth	Mars	Jupiter	Saturn	Uranus	Neptune	Pluto	Eris
6000-7000										Mars
5000-6000			Ganymede	Titan
4000-5000			Callisto							Mercury
3000-4000	The Moon[5]		Io Europa
2000-3000						Triton				Eris Pluto
1500-2000				Rhea	Titania Oberon					90377 Sedna
1000-1500				Iapetus Dione Tethys	Umbriel Ariel		Charon			90482 Orcus 50000 Quaoar
500-1000				Enceladus						Ceres 20000 Varuna 28978 Ixion 2 Pallas, 4 Vesta many more TNOs
250-500				Mimas Hyperion	Miranda	Proteus Nereid		Dysnomia	S/2005 () 1 S/2005 (79360) 1	10 Hygiea 511 Davida 704 Interamnia and many others
100-250			Amalthea Himalia Thebe	Phoebe Janus Epimetheus	Sycorax Puck Portia	Larissa Galatea Despina			S/2005 () 2 many more TNOs	many
50-100			Elara Pasiphaë	Prometheus Pandora	Caliban Juliet Belinda Cressida Rosalind Desdemona Bianca	Thalassa Halimede Neso Naiad	Nix[6] Hydra		Menoetius[7] S/2000 (90) 1 many more TNOs	many
10-50		Phobos	Carme Metis Sinope Lysithea Ananke Leda Adrastea	Siarnaq Helene Albiorix Atlas Pan Telesto Paaliaq Calypso Ymir Kiviuq Tarvos Ijiraq Erriapo	Ophelia Cordelia Setebos Prospero Perdita Mab Stephano Cupid Francisco Ferdinand Margaret Trinculo	Sao Laomedeia Psamathe			Linus[8] S/2000 (762) 1 S/2002 (121) 1 Romulus[9] Petit-Prince[10] S/2003 (283) 1 S/2004 (1313) 1 and many TNOs	many
less than 10		Deimos	at least 47	at least 21					many	many

Terminology

The first known natural satellite was the Moon (''luna'' in Latin). Until the discovery of the Galilean satellites in 1610, however, there was no opportunity for referring to such objects as a class. Galileo chose to refer to his discoveries as ''Planetæ'' ("planets"), but later discoverers chose other terms to distinguish them from the objects they orbited.
Christiaan Huygens, the discoverer of Titan, was the first to use the term ''moon'' for such objects, calling Titan ''Luna Saturni'' or ''Luna Saturnia'' – "Saturn's moon" or "The Saturnian moon", because it stood in the same relation to Saturn as the Moon did to the Earth.
As additional moons of Saturn were discovered, however, this term was abandoned. Giovanni Domenico Cassini sometimes referred to his discoveries as ''planètes'' in French, but more often as ''satellites'', using a term derived from the Latin ''satelles'', meaning "guard", "attendant", or "companion", because the ''satellites'' accompanied their primary planet in their journey through the heavens.
The term ''satellite'' thus became the normal one for referring to an object orbiting a planet, as it avoided the ambiguity of "moon". In 1957, however, the launching of the artificial object Sputnik created a need for new terminology. The terms ''man-made satellite'' or ''artificial moon'' were very quickly abandoned in favor of the simpler ''satellite'', and as a consequence, the term has come to be linked primarily with artificial objects flown in space – including, sometimes, even those which are not in orbit around a planet.
As a consequence of this shift in meaning, the term ''moon'', which had continued to be used in a generic sense in works of popular science and in fiction, has regained respectability and is now used interchangeably with ''satellite'', even in scientific articles. When it is necessary to avoid both the ambiguity of confusion with the Earth's moon on the one hand, and artificial satellites on the other, the term ''natural satellite'' (using "natural" in a sense opposed to "artificial") is used.

The definition of a moon

There has been some debate about the precise definition of a moon. This debate has been caused by the presence of orbital systems where the difference in mass between the larger body and its satellite is not as pronounced as in more typical systems. Two examples are the Pluto-Charon system and the Earth-Moon System. The presence of these systems has caused a debate about where to precisely draw the line between a double body system, and a main body-satellite system. The most common definition rests upon whether the barycentre is below the surface of the larger body, though this is unofficial and somewhat arbitrary. At the other end of the spectrum there are many ice/rock clumps that form ring systems around the Solar System's gas giants, and there is no set point to define when one of these clumps is large enough to be classified as a moon. The term "moonlet" is sometimes used to refer to extremely small objects in orbit around a larger body, but again there is no official definition.

See also

★ Asteroid moon

★ Co-orbital moon

★ Extrasolar moon

★ Inner satellite

★ Irregular satellite

★ List of natural satellites

★ List of natural satellites by diameter

★ Naming of natural satellites

★ Quasi-satellite

★ Timeline of discovery of Solar System planets and their natural satellites

★ Trojan moon

Natural satellites of planets and dwarf planets

★ Earth's natural satellite; see Moon

★ Mars' natural satellites

★ Jupiter's natural satellites

★ Saturn's natural satellites

★ Uranus' natural satellites

★ Neptune's natural satellites

★ Pluto's natural satellites

★ Eris' natural satellite; see Dysnomia

Natural satellites of small Solar System bodies

★ 2003 EL61's natural satellites

Notes and references

1. List of natural satellites orbiting the planets.
2. Origin of the Moon in a giant impact near the end of the Earth's formation, , , R. Canup and E. Asphaug, Nature,
3. A giant impact origin for Pluto's small moons and satellite multiplicity in the Kuiper belt, , , S. Stern, H. Weaver, A. Steffl, M. Mutchler, W. Merline, M. Buie, E. Young,
L. Young, and J. Spencer, Nature,
4. This column lists objects that are moons of small solar system bodies, not small solar system bodies themselves.
5. Sometimes referred to as "Luna".
6. Diameters of the new Plutonian satellites are still very poorly known, but they are estimated to lie between 44 and 130 km.
7. (617) Patroclus I Menoetius
8. (22) Kalliope I Linus
9. (87) Sylvia I Romulus
10. (45) Eugenia I Petit-Prince

External links

Jupiter's moons

★ Data on Jupiter's satellites

★ Jupiter's new moons (discovered in 2000)

★ Jupiter's new moons (discovered in 2002)

★ Jupiter's new moons (discovered in 2003)

Saturn's moons

★ Saturn's new moons (discovered in 2000)

★ Saturn's new moon (discovered in 2003)

Neptune's moons

★ Neptune's new moons (discovered in 2003)

All moons

★ Natural Satellite Physical Parameters (JPL-NASA, with refs)

★ Moons of the Solar System (The Planetary Society)

★ Scott Sheppard's page

★ Major moons in order from the Sun

★ JPL's Solar System Dynamics page

★ Moon of an Object? First Photo of Satellite Beyond the Solar System

★ USGS list of named moons

★ Upper size limit for moons explained

★ Asteroids with Satellites