Planet Swaps
Posted: Sat Feb 22, 2020 1:24 pm
GIANT PLANET SWAPS DURING CLOSE STELLAR ENCOUNTERS
ABSTRACT
The discovery of planetary systems outside of the solar system has challenged some of the tenets of planetary
formation. Among the difficult-to-explain observations, are systems with a giant planet orbiting a very-low mass
star, such as the recently discovered GJ 3512b planetary system, where a Jupiter-like planet orbits an M-star in
a tight and eccentric orbit. Systems such as this one are not predicted by the core accretion theory of planet
formation. Here we suggest a novel mechanism, in which the giant planet is born around a more typical Sunlike star (M∗,1), but is subsequently exchanged during a dynamical interaction with a flyby low-mass star (M∗,2).
We perform state-of-the-art N-body simulations with M∗,1 = 1M and M∗,2 = 0.1M to study the statistical
outcomes of this interaction, and show that exchanges result in high eccentricities for the new orbit around the
low-mass star, while about half of the outcomes result in tighter orbits than the planet had around its birth star.
We numerically compute the cross section for planet exchange, and show that an upper limit for the probability
per planetary system to have undergone such an event is ...
https://arxiv.org/pdf/2002.08366.pdf
Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY
ABSTRACT
The discovery of planetary systems outside of the solar system has challenged some of the tenets of planetary
formation. Among the difficult-to-explain observations, are systems with a giant planet orbiting a very-low mass
star, such as the recently discovered GJ 3512b planetary system, where a Jupiter-like planet orbits an M-star in
a tight and eccentric orbit. Systems such as this one are not predicted by the core accretion theory of planet
formation. Here we suggest a novel mechanism, in which the giant planet is born around a more typical Sunlike star (M∗,1), but is subsequently exchanged during a dynamical interaction with a flyby low-mass star (M∗,2).
We perform state-of-the-art N-body simulations with M∗,1 = 1M and M∗,2 = 0.1M to study the statistical
outcomes of this interaction, and show that exchanges result in high eccentricities for the new orbit around the
low-mass star, while about half of the outcomes result in tighter orbits than the planet had around its birth star.
We numerically compute the cross section for planet exchange, and show that an upper limit for the probability
per planetary system to have undergone such an event is ...
https://arxiv.org/pdf/2002.08366.pdf
Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY