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| | Planetary orbit Summary |
 | | Geostationary orbit is also known as a Clarke orbit, after science fiction writer Arthur C. Clarke, who first proposed the concept in 1945. |
 | | An open orbit has the shape of a hyperbola (or in the limiting case, a parabola); the bodies approach each other for a while, curve around each other around the time of their closest approach, and then separate again forever. |
 | | There are also specific terms for orbits around particular bodies; things orbiting the Sun have a perihelion and aphelion, things orbiting the Earth have a perigee and apogee, and things orbiting the Moon have a perilune and apolune (or, synonymously, periselene and aposelene). |
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