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Revision as of 00:53, 26 October 2006 by 64.12.116.65 (talk) (→Moons of the Solar system)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)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.
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, 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
- Asteroid moon
- Extrasolar moon
- Inner satellite
- Irregular satellite
- 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
Notes and references
- List of natural satellites orbiting the planets.
- This column lists objects that are moons of small solar system bodies, not small solar system bodies themselves.
- Also known as "Luna".
- ^ Diameters of the new Plutonian satellites are still very poorly known, but they are estimated to lie between 44 and 130 km.
- (617) Patroclus I Menoetius
- (22) Kalliope I Linus
- (87) Sylvia I Romulus
- (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
Neptune's moons
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
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