The closest distance a body in orbit about a mass M reaches is called the periapsis and is denoted . The distance from M is then given by
where a is the semimajor axis Eric Weisstein's World of Math, e is the eccentricity, and is the orbital angle. At periapsis, , so
Apoapsis, Perigee, Eric Weisstein's World of Astronomy Perihelion Eric Weisstein's World of Astronomy
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