Constellations of co-orbital planets: horseshoe dynamics, long-term stability, transit timing variations, and potential as SETI beacons. Issue 2 (2nd March 2023)

• Record Type: Journal Article
• Authors: Raymond, Sean N; Veras, Dimitri; Clement, Matthew S; Izidoro, Andre; Kipping, David; Meadows, Victoria
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 521:Issue 2(2023)
• Page Start: 2002
• Page End: 2011
• Publication Date: 2023-03-02
• Subjects: extraterrestrial intelligence -- astrobiology -- planets and satellites: dynamical evolution and stability -- stars: evolution; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stad643
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: Co-orbital systems contain two or more bodies sharing the same orbit around a planet or star. The best-known flavours of co-orbital systems are tadpoles (in which two bodies' angular separations oscillate about the L4/L5 Lagrange points 60° apart) and horseshoes (with two bodies periodically exchanging orbital energy to trace out a horseshoe shape in a co-rotating frame). Here, we use N -body simulations to explore the parameter space of many-planet horseshoe systems. We show that up to 24 equal-mass, Earth-mass planets can share the same orbit at 1 au, following a complex pattern in which neighbouring planets undergo horseshoe oscillations. We explore the dynamics of horseshoe constellations, and show that they can remain stable for billions of years and even persist through their stars' post-main sequence evolution. With sufficient observations, they can be identified through their large-amplitude, correlated transit timing variations. Given their longevity and exotic orbital architectures, horseshoe constellations may represent potential SETI beacons.