Abstract:
We present a self-consistent modelling of the available light curve and radial velocity data of WASP-47 that takes into account the gravitational interactions between all known bodies in the system. The joint analysis of light curve and radial velocity data in a multi-planetary system allows deriving absolute densities, radii, and masses without the use of theoretical stellar models. For WASP-47 the precision is limited by the reduced dynamical information that is due to the short time span of the K2 light curve. We achieve a precision of around 22% for the radii of the star and the transiting planets, between 40% and 60% for their masses, and between 1.5% and 38% for their densities. All values agree with previously reported measurements. When theoretical stellar models are included, the system parameters are determined with a precision that exceeds that achieved by previous studies, thanks to the self-consistent modelling of light curve and radial velocity data. © 2016 ESO.
Registro:
Documento: |
Artículo
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Título: | Absolute densities, masses, and radii of the WASP-47 system determined dynamically |
Autor: | Almenara, J.M.; Diáz, R.F.; Bonfils, X.; Udry, S. |
Filiación: | Observatoire de Genève, Département d'Astronomie, Université de Genève, Chemin des Maillettes 51, Versoix, 1290, Switzerland Univ. Grenoble Alpes, CNRS, IPAG, Grenoble, 38000, France Aix Marseille Université, CNRS, Laboratoire d'Astrophysique de Marseille, Marseille, 13388, France Instituto de Astronomiá y Física Del Espacio, Sucursal 28, Buenos Aires, C1428EHA, Argentina
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Palabras clave: | Planetary systems; Stars: individual: WASP-47; Techniques: photometric; Techniques: radial velocities; Stars; Velocity; Absolute density; Gravitational interaction; Joint analysis; Planetary system; Radial velocity datum; Stars: individual; Techniques: photometric; Techniques: radial velocities; Gravitation |
Año: | 2016
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Volumen: | 595
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DOI: |
http://dx.doi.org/10.1051/0004-6361/201629770 |
Título revista: | Astronomy and Astrophysics
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Título revista abreviado: | Astron. Astrophys.
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ISSN: | 00046361
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CODEN: | AAEJA
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Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v595_n_p_Almenara |
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Citas:
---------- APA ----------
Almenara, J.M., Diáz, R.F., Bonfils, X. & Udry, S.
(2016)
. Absolute densities, masses, and radii of the WASP-47 system determined dynamically. Astronomy and Astrophysics, 595.
http://dx.doi.org/10.1051/0004-6361/201629770---------- CHICAGO ----------
Almenara, J.M., Diáz, R.F., Bonfils, X., Udry, S.
"Absolute densities, masses, and radii of the WASP-47 system determined dynamically"
. Astronomy and Astrophysics 595
(2016).
http://dx.doi.org/10.1051/0004-6361/201629770---------- MLA ----------
Almenara, J.M., Diáz, R.F., Bonfils, X., Udry, S.
"Absolute densities, masses, and radii of the WASP-47 system determined dynamically"
. Astronomy and Astrophysics, vol. 595, 2016.
http://dx.doi.org/10.1051/0004-6361/201629770---------- VANCOUVER ----------
Almenara, J.M., Diáz, R.F., Bonfils, X., Udry, S. Absolute densities, masses, and radii of the WASP-47 system determined dynamically. Astron. Astrophys. 2016;595.
http://dx.doi.org/10.1051/0004-6361/201629770