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Extreme secular excitation of eccentricity inside mean motion resonance
2017
Astronomy and Astrophysics
It is well known that asteroids and comets fall into the Sun. Metal pollution of white dwarfs and transient spectroscopic signatures of young stars like β-Pic provide growing evidence that extra solar planetesimals can attain extreme orbital eccentricities and fall onto their parent stars. We aim to develop a general, practically implementable, semi-analytical theory of secular eccentricity excitation of small bodies in mean motion resonances with an eccentric planet valid for arbitrary values
doi:10.1051/0004-6361/201730936
fatcat:oq35znn4qrcczar7arg4ke6y6e