Effect of Planetary Mass on the Orbit of Star-Planet Systems

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dc.authoridOzturk, Oguz/0000-0002-9135-9865
dc.contributor.authorOzturk, O.
dc.contributor.authorErdem, A.
dc.date.accessioned2025-01-27T21:07:13Z
dc.date.available2025-01-27T21:07:13Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description32nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEY
dc.description.abstractTwo main parameters, which determine the radial velocity semi-amplitude of the host star in a star-planet system, are the planet mass and the orbital period. In order to examine the effect of planet mass on the radial velocity semi-amplitude, we firstly select sensitive data of spectroscopic orbital solutions of 737 systems, given in the database of exoplanet.org. The selected systems are then categorized into 31 groups according to their orbital periods. For each group, an empirical relation between the radial velocity semi amplitude and the planet mass is obtained. In order to check the accuracy of these empirical relations, the measured and expected values of planet masses are compared.
dc.description.sponsorshipTurkish Phys Soc
dc.description.sponsorshipTUBITAK (Scientific and Technological Research Council of Turkey) [113F353]; TUBITAK
dc.description.sponsorshipThis research has been supported by TUBITAK (Scientific and Technological Research Council of Turkey) under Grant No. 113F353. This work was partly supported by TUBITAK for a Doctoral Fellowship Award. This paper is part of the PhD thesis of Oguz OZTURK.
dc.identifier.doi10.1063/1.4976450
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85016035640
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976450
dc.identifier.urihttps://hdl.handle.net/20.500.12428/27931
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100106
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofProceedings of The Turkish Physical Society 32nd International Physics Congress (Tps32)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.titleEffect of Planetary Mass on the Orbit of Star-Planet Systems
dc.typeConference Object

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