Asteroid Belt
From Conservapedia
The Asteroid Belt is a large toroidal (doughnut-shaped) region in the inner Solar system with a heliocentric distance of between 2 and 4 astronomical units containing nearly two million minor planets [1], or asteroids rather than a major rocky body like the Earth or Mars.
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References
| The Solar System | ||
| Star | Sol | |
| Planets | Vulcan • Mercury • Venus • Earth • Mars • Jupiter • Saturn • Uranus • Neptune | |
| Dwarf Planets | Ceres • Pluto • Eris | |
| Asteroid Belt | Major asteroids • C-type asteroids • S-type asteroids • M-type asteroids | |
| Trans-Neptunian Objects | Kuiper Belt • Scattered disk • Oort Cloud • Nemesis | |
| Natural satellites | Moon • Phobos • Deimos • Io • Europa • Ganymede • Callisto • Mimas • Enceladus • Tethys • Dione • Rhea • Titan • Hyperion • Iapetus • Miranda • Ariel • Umbriel • Titania • Oberon • Triton • Nereid • Charon • Nix • Hydra • Dysnomia |
