On the enlargement of habitable zones around binary stars in hostile environments

Nikolaos Georgakarakos, Siegfried Eggl

Research output: Contribution to journalArticlepeer-review

Abstract

We investigate the hypothesis that the size of the habitable zone around hardened binaries in dense star-forming regions increases. Our results indicate that this hypothesis is essentially incorrect. Although certain binary star configurations permit extended habitable zones, such set-ups typically require all orbits in a system to be near-circular. In all other cases, planets can only remain habitable if they display an extraordinarily high climate inertia.

Original languageEnglish (US)
Pages (from-to)L58-L60
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume487
Issue number1
DOIs
StatePublished - Jul 1 2019
Externally publishedYes

Keywords

  • (stars:) binaries: general
  • (stars:) planetary systems
  • astrobiology
  • planets and satellites: atmospheres
  • planets and satellites: dynamical evolution and stability
  • planets and satellites: terrestrial planets

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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