Orbit classification in exoplanetary systems

The circular version of the restricted three-body problem, along with the method of grid classification are used to determine the character of the trajectories of a test particle, which move in a binary exoplanetary system. The binary system can be either a parent star-exoplanet or an exoplanet–exop...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2020-02, Vol.634, p.A60
Hauptverfasser:	Zotos, Euaggelos E., Érdi, Bálint, Saeed, Tareq, Alhodaly, Mohammed Sh
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Classification Coordinates Extrasolar moons Extrasolar planets Planetary orbits Planetary systems Rotating bodies Stellar systems Three body problem
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