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Kepler Orbit
CHF 61.55
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M681SE6FFM1
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Geliefert zwischen Di., 25.11.2025 und Mi., 26.11.2025
Details
High Quality Content by WIKIPEDIA articles! In celestial mechanics, a Kepler orbit describes the motion of an orbiting body as an ellipse, parabola, or hyperbola, which forms a two-dimensional orbital plane in three-dimensional space. (A Kepler orbit can also form a straight line.) It considers only the gravitational attraction of two bodies, neglecting perturbations due to gravitational interactions with other objects, atmospheric drag, solar radiation pressure, a non-spherical central body, and so on. It is thus said to be a solution of a special case of the two-body problem, known as the Kepler problem. As a theory in classical mechanics, it also does not take into account the effects of general relativity. Keplerian orbits can be parametrized into six orbital elements in various ways. In most applications, there is a large central body, the center of mass of which is assumed to be the center of mass of the entire system. By decomposition, the orbits of two objects of similar mass can be described as Kepler orbits around their common center of mass, their barycenter.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786130241445
- Editor Frederic P. Miller, Agnes F. Vandome, John McBrewster
- Sprache Englisch
- Genre Physik & Astronomie
- Größe H220mm x B150mm x T9mm
- Jahr 2009
- EAN 9786130241445
- Format Kartonierter Einband
- ISBN 978-613-0-24144-5
- Titel Kepler Orbit
- Untertitel Orbital elements, Celestial mechanics, Ellipse, Parabola, Hyperbola, Line (geometry), Drag (physics), Sphere, Two-body problem, Kepler problem, Classical mechanics, General relativity
- Gewicht 249g
- Herausgeber Alphascript Publishing
- Anzahl Seiten 156
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