The dynamical evolution of multiplanet systems in open clusters

W. Hao*, M. B.N. Kouwenhoven, R. Spurzem

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

67 Citations (Scopus)

Abstract

The majority of stars form in star clusters and many are thought to have planetary companions. We demonstrate that multiplanet systems are prone to instabilities as a result of frequent stellaren counters in these star clusters much more than single-planet systems. The cumulative effect of close and distant encounters on these planetary systems are investigated using Monte Carlos cattering experiments. We consider two types of planetary configurations orbiting Sun-likestars: (i) five Jupiter-mass planets in the semi major axis range 1-42 au orbiting a Solar massstar, with orbits that are initially coplanar, circular and separated by 10 mutual Hill radii and (ii)the four gas giants of our Solar system. We find that in the equal-mass planet model, 70 per centof the planets with initial semimajor axes a > 40 au are either ejected or have collided with the central star or another planet within the lifetime of a typical cluster, and that more than50 per cent of all planets with a < 10 au remain bound to the system. Planets with short orbitalperiods are not directly affected by encountering stars. However, secular evolution of perturbedsystems may result in the ejection of the innermost planets or in physical collisions of theinnermost planets with the host star, up to many thousands of years after a stellar encounter. The simulations of the Solar system-like systems indicate that Saturn, Uranus and Neptune are affected by both direct interactions with encountering stars, as well as planet-planet scattering. Jupiter, on the other hand, is almost only affected by direct encounters with neighbouring stars, as its mass is too large to be substantially perturbed by the other three planets. Our resultsindicate that stellar encounters can account for the apparent scarcity of exoplanets in star clusters, not only for those on wide-orbit that are directly affected by stellar encounters, but also planets close to the star which can disappear long after a stellar encounter has perturbed the planetary system.

Original languageEnglish
Pages (from-to)867-877
Number of pages11
JournalMonthly Notices of the Royal Astronomical Society
Volume433
Issue number1
DOIs
Publication statusPublished - Jul 2013
Externally publishedYes

Keywords

  • Planetary systems
  • Planets and satellites: Dynamical evolution and stability

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