Exomoons as Sources of White Dwarf Pollution

نویسندگان

چکیده

Polluted white dwarfs offer a unique way to study the bulk compositions of exoplanetary material, but it is not always clear if this material originates from comets, asteroids, moons, or planets. We combine N-body simulations with an analytical model assess prevalence extrasolar moons as dwarf (WD) polluters. Using sample observed polluted we find that extrapolated parent body masses polluters are often more consistent those many solar system rather than solar-like asteroids. provide framework for estimating fraction currently undergoing observable moon accretion based on results simulated planetary and systems. Focusing three-planet Super-Earth Neptune-mass bodies, could expect about one percent such systems be accretions opposed asteroid accretion.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2022

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/ac86d5