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Is our Sun a singleton?

Davies, M B; Malmberg, D; Chambers, J E; Church, R P; De Angeli, F; Mackey, Alasdair; Wilkinson, Mark, I.

Description

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...[Show more]

dc.contributor.authorDavies, M B
dc.contributor.authorMalmberg, D
dc.contributor.authorChambers, J E
dc.contributor.authorChurch, R P
dc.contributor.authorDe Angeli, F
dc.contributor.authorMackey, Alasdair
dc.contributor.authorWilkinson, Mark, I.
dc.date.accessioned2015-12-10T22:16:25Z
dc.identifier.issn0031-8949
dc.identifier.urihttp://hdl.handle.net/1885/50936
dc.description.abstractAll 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. � 2008 The Royal Swedish Academy of Sciences.
dc.publisherRoyal Swedish Academy of Sciences
dc.sourcePhysica Scripta
dc.subjectKeywords: Solar equipment; Solar system; Stars; Binary systems; Eccentric orbits; Hostile environments; Number densities; Planetary systems; Astronomy
dc.titleIs our Sun a singleton?
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolumeT130
dc.date.issued2008
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4630950xPUB213
local.type.statusPublished Version
local.contributor.affiliationDavies, M B, Lund Observatory
local.contributor.affiliationMalmberg, D, Lund University
local.contributor.affiliationChambers, J E, Carnegie Institution of Washington
local.contributor.affiliationChurch, R P, Lund University
local.contributor.affiliationDe Angeli, F, University of Cambridge
local.contributor.affiliationMackey, Alasdair, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWilkinson, Mark, I. , University of Leicester
local.description.embargo2037-12-31
local.bibliographicCitation.startpage041030
local.identifier.doi10.1088/0031-8949/2008/T130/014030
dc.date.updated2015-12-09T08:23:59Z
local.identifier.scopusID2-s2.0-53349144353
CollectionsANU Research Publications

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