Abstract
We present a study on S-type planets in binary star systems with separations a < 100 AU. For systems with at least one detected giant planet we determine the location of (linear) secular resonances with that planet by means of a semi-analytical method. We demonstrate that under some conditions, e.g. when the secondary star is at about 20 AU, the habitable zone can be perturbed or completely destabilized in these systems.
Original language | English |
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Article number | ESPC2015-449 |
Journal | Abstracts of the EPSC-DPS |
Volume | 10 |
Publication status | Published - Oct 2015 |
Event | European Planetary Science Congress 2015 - Nantes, France Duration: 27 Sep 2015 → 2 Oct 2015 |
Austrian Fields of Science 2012
- 103003 Astronomy
- 103004 Astrophysics