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In the case of the Sun, Jupiter, and Saturn, the volumetric mean radius is used. For mostly spherical objects ( oblate) such as planets and large planetoids, the equatorial radius is used. For irregular objects, the radii along three axes are given.
The ordering is not the same as the order of a list of solar system objects by mass because some objects are denser than others. For instance Uranus is bigger than Neptune but less massive, and although Ganymede and Titan are larger than Mercury, they have less than half its mass.
The list is incomplete because the radii of many asteroids are not accurately known, or even well-defined in the case of irregular objects.
| Sun | 696,000 km |
| Jupiter | 69,911 |
| Saturn | 58,232 |
| Uranus | 25,559 |
| Neptune | 24,764 |
| Earth | 6,378 |
| Venus | 6,052 |
| MarsMars is the fourth planet from the Sun in the solar system, named after the Roman god of war (the counterpart of the Greek Ares), on account of its blood red color as viewed in the night sky. Mars has two small moons, Phobos and Deimos, both small and odd | 3,397 |
| Ganymede | 2,631 |
| Titan | 2,575 |
| Mercury | 2,440 |
| CallistoCallisto is a moon of the planet Jupiter, discovered in 1610 by Galileo Galilei. It is the third-largest moon in the solar system, about the same size as the planet Mercury. It is named after Callisto, one of Zeus's many love interests in Greek mythology. | 2,410 |
| IoIo is the innermost of the four Galilean moons of Jupiter. It is named after the Greek mythological figure Io, one of the many lovers of Zeus (who is also known as Jupiter in the Roman mythology). Although the name "Io" was suggested by Simon Marius soon | 1,822 |
| MoonFor other moons in the solar system see natural satellite. For other uses see Moon (disambiguation). The Moon is the only natural satellite of Earth. It has no formal name other than "The Moon" although it is occasionally called Luna ( Latin for moon to d | 1,738 |
| Europa | 1,561 |
| Triton | 1,353 |
| Pluto | 1,195 |
| 90377 Sedna | <800 |
| Orcus | 800 |
| Titania | 789 |
| Rhea | 764 |
| Oberon | 761 |
| Iapetus | 718 |
| Quaoar | ~600 |
| Charon | 593 |
| Umbriel | 585 |
| Ariel | 581 × 578 × 578 |
| Dione | 560 |
| Ixion | 532 |
| Tethys | 536 × 528 × 526 |
| 20000 Varuna | ~500 |
| 1 Ceres | 485 |
| ... | |
| 2 Pallas | 285 |
| ... | |
| 45 Eugenia | 113 |
| ... | |
| 2060 Chiron | 90 |
| ... |
The rankings of some remaining natural satellites are shown below. There are various asteroids larger than many of these, but the exact sizes of many asteroids are not known precisely enough although asteroid diameters can sometimes be determined by timing stellar occultations. In any case many asteroids are known to be highly irregular in shape—some are not even approximately spherical—making any comparison of radii infeasible even if exact figures are known.
| Enceladus | 256 × 247 × 245 |
| Miranda | 240 × 234 × 233 |
| Proteus | 220 × 208 × 202 |
| Mimas | 209 × 196 × 191 |
| Hyperion | 185 × 140 × 113 |
| Nereid | 170 |
| Amalthea | 131 × 73 × 67 |
| Phoebe | 115 × 110 × 105 |
| Larissa | 108 × 102 × 84 |
| Galatea | 102 × 92 × 72 |
| Janus | 97 × 95 × 77 |
| Sycorax | 95 |
| Despina | 90 × 74 × 64 |
| Himalia | 85 |
| Puck | 81 |
| Portia | 68 |
| Prometheus | 74 × 50 × 34 |
| Epimetheus | 69 × 55 × 55 |
| Thebe | 55 × 45 |
| Pandora | 55 × 44 × 31 |
| Thalassa | 54 × 50 × 26 |
| Caliban | 48 |
| Naiad | 48 × 30 × 26 |
| Juliet | 47 |
| Belinda | 40 |
| Cressida | 40 |
| Elara | 40 |
| Rosalind | 36 |
| Desdemona | 32 |
| Bianca | 27 |
| Ophelia | 21 |
| Cordelia | 20 |
| Metis | 20 |
| Pasiphaë | 18 |
| Carme | 15 |
| Sinope | 14 |
| Lysithea | 12 |
| Adrastea | 13 × 10 × 8 |
| Phobos | 13.4 × 11.2 × 9.2 |
| Ananke | 10 |
| Pan | 10 |
| Deimos | 7.5 × 6.1 × 5.2 |