Long-term stability of horseshoe orbits

Author:

Ćuk Matija1,Hamilton Douglas P.2,Holman Matthew J.3

Affiliation:

1. Carl Sagan Center; SETI Institute; Mountain View; CA; 94043; USA

2. Department of Astronomy; University of Maryland; College Park; MD; 20742; USA

3. Smithsonian Astrophysical Observatory; Cambridge; MA; 02138; USA

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 57 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. When the horseshoe fits: Characterizing 2023 FY3 with the 10.4 m Gran Telescopio Canarias and the Two-meter Twin Telescope;Astronomy & Astrophysics;2023-12-20

2. Asteroids co-orbital motion classification based on Machine Learning;Monthly Notices of the Royal Astronomical Society;2023-11-22

3. Photometric Survey of Neptune's Trojan Asteroids. I. The Color Distribution;The Planetary Science Journal;2023-08-01

4. Survival and dynamics of rings of co-orbital planets under perturbations;Monthly Notices of the Royal Astronomical Society;2023-04-29

5. A semi-analytical model for coorbital motion;Monthly Notices of the Royal Astronomical Society;2023-04-11

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