Anisotropy of Long-period Comets Explained by Their Formation Process

Long-period comets coming from the Oort cloud are thought to be planetesimals formed in the planetary region on the ecliptic plane. We have investigated the orbital evolution of these bodies due to the Galactic tide. We extended our previous work and derived analytical solutions to the Galactic long...

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Veröffentlicht in:	The Astronomical journal 2020-09, Vol.160 (3), p.134
1. Verfasser:	Higuchi, Arika
Format:	Artikel
Sprache:	eng
Schlagworte:	Anisotropy Anomalies Astronomy Comets Ecliptic Evolution Exact solutions Galactic evolution Galactic rotation Long period comets Numerical integration Oort cloud Orbital mechanics Planet formation Planetary evolution
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