Is our Sun a singleton?

Research output: Contribution to journalArticle

Abstract

All stars are formed in some form of cluster or association. These environments can have a much higher number density of stars than the field of the galaxy. Such crowded places are hostile environments: a large fraction of initially single stars will undergo close encounters with other stars or exchange into binaries. We describe how such close encounters and exchange encounters will affect the properties of a planetary system around a single star. We define singletons as single stars which have never suffered close encounters with other stars or spent time within a binary system. It may be that planetary systems similar to our own solar system can only survive around singletons. Close encounters or the presence of a stellar companion will perturb the planetary system, leading to strong planet-planet interactions, often leaving planets on tighter and more eccentric orbits. Thus, planetary systems which initially resembled our own solar system may later more closely resemble the observed exoplanetary systems.

Details

Authors
  • Melvyn B Davies
  • Daniel Malmberg
  • J. E. Chambers
  • R P Church
  • F. De Angeli
  • D. Mackey
  • M. I. Wilkinson
Organisations
Research areas and keywords

Subject classification (UKÄ) – MANDATORY

  • Astronomy, Astrophysics and Cosmology
Original languageEnglish
Article number014030
JournalPhysica Scripta
VolumeT130
Publication statusPublished - 2008
Publication categoryResearch
Peer-reviewedYes