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24: Series 5
In association with Amazon.co.uk £26.97 |
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Contents
Origin
Orbital characteristics
Moons of the Solar system
Origin - Contents
Most moons are assumed to have been formed out of the same collapsing region of protoplanetary disk that gave rise to its primary. However, there are many exceptions and variations to this standard model of moon formation that are known or theorized. Several moons are thought to be captured asteroids; others may be fragments of larger moons shattered by impacts, or (in the case of Earth's Moon) a portion of the planet itself blasted into orbit by a large impact. As most moons are known only through a few observations via probes or telescopes, most theories about their origins are still uncertain.
Orbital characteristics - Contents
Most 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 are Saturn's moon Hyperion, which rotates chaotically due to a variety of external influences, and the outermost moons of the gas giants, which are too far away to become 'locked' (an example is Saturn's moon Phoebe).It is not possible for a moon to have moons of its own: the tidal effects of their primaries would make such a system unstable. However, several moons have small companions in the Lagrangian points of their orbits (e.g., Saturn's moons Tethys and Dione).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 - Contents
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, and Neptune's captured moon Triton. For smaller moons see the articles on the appropriate planet.The following is a comparative table classifying the moons of the solar system by diameter. The column on the right includes some notable planets, asteroids and Kuiper belt objects for comparison.
Diameter (km) |
Earth |
Mars |
Jupiter |
Saturn |
Uranus |
Neptune |
Pluto |
Other objects |
5000-6000 |
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Ganymede |
Titan |
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4000-5000 |
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Callisto |
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Mercury |
3000-4000 |
Moon |
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Io
Europa |
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2000-3000 |
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Triton |
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2003 UB313 Pluto |
1000-2000 |
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Rhea
Iapetus
Dione
Tethys |
Titania
Oberon
Umbriel
Ariel |
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Charon |
2005 FY9
2003 EL61
90377 Sedna
90482 Orcus
50000 Quaoar |
500-1000 |
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Enceladus |
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1 Ceres
20000 Varuna
28978 Ixion
2 Pallas
4 Vesta (and many others) |
250-500 |
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Mimas
Hyperion |
Miranda |
Proteus
Nereid |
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10 Hygiea
511 Davida
704 Interamnia
3 Juno S/2005 (2003 UB313) 1
S/2005 (2003 EL61) 1 (and many others) |
100-250 |
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Amalthea
Himalia |
Phoebe
Janus
Epimetheus
Prometheus |
Sycorax
Puck
Portia |
Larissa
Galatea
Despina |
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S/2005 (2003 EL61) 2 (too many to list) |
50-100 |
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Thebe
Elara
Pasiphaë |
Pandora |
Caliban
Juliet
Belinda
Cressida
Rosalind
Desdemona
Bianca |
Thalassa
Naiad
S/2002 N 4 |
S/2005 P 12
S/2005 P 22 |
(too many to list) |
10-50 |
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Phobos
Deimos |
Carme
Metis
Sinope
Lysithea
Ananke
Leda
Adrastea |
Siarnaq
Atlas
Helene
Albiorix
Telesto
Pan
Paaliaq
Calypso
Ymir
Kiviuq
Tarvos
Ijiraq |
Ophelia
Cordelia
Setebos
Prospero
Stephano
Perdita
Ferdinand
Francisco
Margaret
Trinculo
Mab
Cupid |
S/2002 N 1
S/2002 N 2
S/2002 N 3
Psamathe |
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(too many to list) |
less than 10 |
Cruithne1 |
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At least 47, see Jupiter's natural satellites. |
At least 22, see Saturn's natural satellites. |
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(too many to list) |
1) Cruithne is not a real moon; it is mainly placed here for comparison's sake. 2) Diameters of the new Plutonian satellites are still very poorly known, but they are estimated to lie between 44 and 130 km. In addition to the moons of the various planets there are also over 80 known moons of the asteroids and other minor planets. |
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