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Natural satellite

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Moons of the Solar System scaled to Earth's Moon

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 or minor planets.

There are 240 known moons within the Solar system, including 162 orbiting the planets, 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 moons, 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" or "Luna"); 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. Charon is also unusual in that it does not orbit Pluto, but rather both bodies orbit a barycenter in empty space, making Pluto-Charon a binary system.

Origin

Moons orbiting relatively close to the planet on prograde orbits (regular satellites) are believed to have been formed out of the same collapsing region of protoplanetary disk that gave rise to its primary. Most irregular satellites (orbiting on distant, inclined, eccentric often retrograde orbits) are thought to be captured asteroids possibly further fragmented by collisions. Many special scenarios exist, including origin in a break-up of the planet. For example, in the case of Earth's Moon, a portion of the planet itself might have been blasted into orbit by a large impact. A very different scenario required to explain the origin of the large Neptunian satellites: circular but retrograde orbit of Triton and extremely eccentric but prograde orbit of Nereid.

Orbital characteristics

Tidal locking

Most regular moons 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 Nereid have rotation period in the range of 10 hours to compare with their orbital periods of hundreds of days.

Satellites of satellites

No "moons of moons" (natural satellites that orbit the natural satelite 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 due to the greater gravitational pull of the planet (or other object) that the primary satellite orbits. For example, the Moon orbits the 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 the 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

However, two moons are known have small companions in their L4 and L5 Lagrangian points of their orbits, about sixty degrees ahead of and behind their positions. These companions are called Trojan moons, because their positions are comparable to the positions of the Trojan asteroids relative to Jupiter. They are Telesto and Calypso, the leading and following companions respectively of Tethys; and Helene and Polydeuces, the leading and following companions of Dione).

Asteroid satellites

The recent discovery of 243 Ida's moon Dactyl 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.

Moons of the Solar system

The largest moons 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, Neptune's captured moon Triton and Button Moon. 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.

Mean diameter
(km)
Satellites of planets Dwarf planet satellites Satellites of
SSSBs
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 Moon


Io
Europa
2000-3000


Triton Eris
Pluto
1000-2000 Rhea
Iapetus
Dione
Tethys
Titania
Oberon
Umbriel
Ariel
Charon (136472) 2005 FY9
(136108) 2003 EL61
90377 Sedna
90482 Orcus
50000 Quaoar
500-1000 Enceladus Ceres
20000 Varuna
28978 Ixion
2 Pallas4 Vesta
many more TNOs
250-500 Mimas
Hyperion
Miranda Proteus
Nereid
Dysnomia S/2005 (2003 EL61) 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 (2003 EL61) 2
many more TNOs
many
50-100 Elara
Pasiphaë
Prometheus
Pandora
Caliban
Juliet
Belinda
Cressida
Rosalind
Desdemona
Bianca
Thalassa
S/2002 N 1
S/2002 N 4
Naiad
Nix
Hydra
Menoetius
S/2000 (90) 1
many more TNOs
many
10-50 Phobos
Deimos
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
S/2002 N 2
S/2002 N 3
Psamathe
Linus
S/2000 (762) 1
S/2002 (121) 1
Romulus
Petit-Prince
S/2003 (283) 1
S/2004 (1313) 1
and many TNOs
many
less than 10 at least 47 at least 21 many many


The definition of a moon

Comparison of Earth and Luna (The Moon)
File:Plutoncharon1.jpg
Comparison of Pluto and Charon
Comparison of Jupiter's Great Red Spot and Jupiter's 4 largest moons. Compared to Earth/Luna and Pluto/Charon there is a much greater difference in mass

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, are not as pronounced as in normal systems (a commonly accepted defining point is where the satellite is larger than 1/40th the mass of the larger body) . Two examples include the Pluto-Charon system, and the Earth-Luna 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 commonly agreed upon definition is whether the barycentre is below the surface of the larger body, though this is not official. Another definition is whether the Sun or the larger body in the system has the most gravitational influence over the satellite in question. At the other end of the spectrum there are many ice/rock clumps that form the ring systems on 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, though the term moonlet may be sometimes used to refer to extremely small objects in orbit around a larger body, there is again no official definition.

See also

Natural satellites of planets and dwarf planets

Notes and references

  1. List of natural satellites orbiting the planets.
  2. This column lists objects that are moons of small solar system bodies, not small solar system bodies themselves.
  3. Also known as "Luna".
  4. ^ Diameters of the new Plutonian satellites are still very poorly known, but they are estimated to lie between 44 and 130 km.
  5. (617) Patroclus I Menoetius
  6. (22) Kalliope I Linus
  7. (87) Sylvia I Romulus
  8. (45) Eugenia I Petit-Prince

External links

Jupiter's moons

Saturn's moons

Neptune's moons

All moons

Natural satellites of the Solar System
Moons of terrestrial planets and asteroids
EarthMarsAsteroid moons
Moons of Jupiter
Listed in increasing approximate distance from Jupiter
Inner moons
Galilean moons
Themisto
Himalia group (9)
Carpo group (2)
Valetudo
Ananke group (26)
Carme group (30)
Pasiphae group (18)
See also
Moons of Saturn
Listed in approximate increasing distance from Saturn
Ring moonlets
Ring shepherds
Other inner moons
Alkyonides
Large moons
(with trojans)
Inuit group (13)
Kiviuq subgroup
Paaliaq subgroup
Siarnaq subgroup
Gallic group (7)
Norse group (100)
Phoebe subgroup
Outlier prograde
irregular moons
  • S/2006 S 12
  • S/2004 S 24
  • Moons of Uranus
    • Listed in approximately increasing distance from Uranus
    Inner
    Major (spheroid)
    Outer (irregular)
    Prograde
    Retrograde
    Geological features
    Moons of Neptune
    Listed in approximately increasing distance from Neptune
    Regular (inner)
    Irregular
    Triton
    Prograde
    Retrograde
    See also
    Moons of likely dwarf planets
    PlutoHaumeaErisMakemakeGonggong
    QuaoarOrcusSalaciaVarda2013 FY27
    Natural satellites of the Solar System
    Planetary
    satellites
    of


    Dwarf planet
    satellites
    of
    Minor-planet
    moons
    Near-Earth
    Florence
    Didymos
    Dimorphos
    Moshup
    Squannit
    1994 CC
    2001 SN263
    Main belt
    Kalliope
    Linus
    Euphrosyne
    Daphne
    Peneius
    Eugenia
    Petit-Prince
    Sylvia
    Romulus
    Remus
    Minerva
    Aegis
    Gorgoneion
    Camilla
    Elektra
    Kleopatra
    Alexhelios
    Cleoselene
    Ida
    Dactyl
    Roxane
    Olympias
    Pulcova
    Balam
    Dinkinesh (Selam)
    Jupiter trojans
    Patroclus
    Menoetius
    Hektor
    Skamandrios
    Eurybates
    Queta
    TNOs
    Lempo
    Hiisi
    Paha
    2002 UX25
    Sila–Nunam
    Salacia
    Actaea
    Varda
    Ilmarë
    Gǃkúnǁʼhòmdímà
    Gǃòʼé ǃHú
    2013 FY27
    Ranked
    by size
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