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dc.contributor.authorForgan, Duncan
dc.date.accessioned2017-03-28T15:30:12Z
dc.date.available2017-03-28T15:30:12Z
dc.date.issued2016-08-20
dc.identifier.citationForgan , D 2016 , ' Milankovitch cycles of terrestrial planets in binary star systems ' , Monthly Notices of the Royal Astronomical Society , vol. 463 , no. 3 , pp. 2768-2780 . https://doi.org/10.1093/mnras/stw2098en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 249488826
dc.identifier.otherPURE UUID: ebf9be4d-5278-44d1-9401-bb7db227075f
dc.identifier.otherScopus: 85015058757
dc.identifier.otherWOS: 000393566000039
dc.identifier.urihttp://hdl.handle.net/10023/10546
dc.descriptionDHF gratefully acknowledges support from the ECOGAL project, grant agreement 291227, funded by the European Research Council under ERC-2011-ADG.en
dc.description.abstractThe habitability of planets in binary star systems depends not only on the radiation environment created by the two stars, but also on the perturbations to planetary orbits and rotation produced by the gravitational field of the binary and neighbouring planets. Habitable planets in binaries may therefore experience significant perturbations in orbit and spin. The direct effects of orbital resonances and secular evolution on the climate of binary planets remain largely unconsidered. We present latitudinal energy balance modelling of exoplanet climates with direct coupling to an N-Body integrator and an obliquity evolution model. This allows us to simultaneously investigate the thermal and dynamical evolution of planets orbiting binary stars, and discover gravito-climatic oscillations on dynamical and secular time-scales. We investigate the Kepler-47 and Alpha Centauri systems as archetypes of P- and S-type binary systems, respectively. In the first case, Earth-like planets would experience rapid Milankovitch cycles (of order 1000 yr) in eccentricity, obliquity and precession, inducing temperature oscillations of similar periods (modulated by other planets in the system). These secular temperature variations have amplitudes similar to those induced on the much shorter time-scale of the binary period. In the Alpha Centauri system, the influence of the secondary produces eccentricity variations on 15 000 yr time-scales. This produces climate oscillations of similar strength to the variation on the orbital time-scale of the binary. Phase drifts between eccentricity and obliquity oscillations creates further cycles that are of order 100 000 yr in duration, which are further modulated by neighbouring planets.
dc.format.extent13
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2016 The Author. Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://dx.doi.org/10.1093/mnras/stw2098en
dc.subjectAstrobiologyen
dc.subjectMethods: numericalen
dc.subjectPlanets and satellites: generalen
dc.subjectAstronomy and Astrophysicsen
dc.subjectSpace and Planetary Scienceen
dc.subjectDASen
dc.titleMilankovitch cycles of terrestrial planets in binary star systemsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stw2098
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/1608.05592en


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