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In stellar dynamics a box orbit refers to a particular type of orbit which can be seen in triaxial systems, that is, systems which do not possess a symmetry around any of its axes. They contrast with the loop orbits which are observed in spherically symmetric or axisymmetric systems.
In a box orbit, the star oscillates independently along the three different axes as it moves through the system. As a result of this motion, it fills in a (roughly) box-shaped region of space. Unlike loop orbits, the stars on box orbits can come arbitrarily close to the center of the system. As a special case, if the frequencies of oscillations in different axes are exact multiples of each other, the orbit will be closed.
Examples of box orbits (in 2 dimensions)
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| Beginning of a box orbit
| Many cycles of a box orbit
| A closed box orbit
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References
See also
v • d • e Orbits |
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| Orbital parameters |
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Classical orbital elements
Inclination
Longitude of the ascending node
Eccentricity
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Argument of periapsis
Semi-major axis
Mean anomaly at epoch
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Other parameters
True anomaly
Semi-minor axis
Linear eccentricity
Eccentric anomaly
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Mean longitude
True longitude
Orbital period
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| Types | |
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| Maneuvers | Bi-elliptic transfer · Geostationary transfer · Gravity assist · Hohmann transfer · Inclination change · Phasing · Rendezvous |
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| Related topics | Apsis · Celestial coordinate system · Delta-v budget · Epoch · Ephemeris · Equatorial coordinate system · Gravity turn · Ground track · Interplanetary Transport Network · Kepler\'s laws of planetary motion · Lagrangian point · n-body problem · Oberth effect · Orbit equation · Orbital state vectors · Perturbation · Retrograde and direct motion · Specific orbital energy · Specific relative angular momentum |
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| List of orbits |
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