CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM

There have been previous hints that the transiting planet WASP-3b is accompanied by a second planet in a nearby orbit, based on small deviations from strict periodicity of the observed transits. Here we present 17 precise radial velocity (RV) measurements and 32 transit light curves that were acquir...

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Main Authors: Winn, Joshua Nathan, McKnight, Laura A.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: IOP Publishing 2014
Online Access:http://hdl.handle.net/1721.1/88681
https://orcid.org/0000-0002-4265-047X
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author Winn, Joshua Nathan
McKnight, Laura A.
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Winn, Joshua Nathan
McKnight, Laura A.
author_sort Winn, Joshua Nathan
collection MIT
description There have been previous hints that the transiting planet WASP-3b is accompanied by a second planet in a nearby orbit, based on small deviations from strict periodicity of the observed transits. Here we present 17 precise radial velocity (RV) measurements and 32 transit light curves that were acquired between 2009 and 2011. These data were used to refine the parameters of the host star and transiting planet. This has resulted in reduced uncertainties for the radii and masses of the star and planet. The RV data and the transit times show no evidence for an additional planet in the system. Therefore, we have determined the upper limit on the mass of any hypothetical second planet, as a function of its orbital period.
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spelling mit-1721.1/886812022-10-01T03:25:18Z CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM Winn, Joshua Nathan McKnight, Laura A. Massachusetts Institute of Technology. Department of Physics Winn, Joshua Nathan McKnight, Laura A. There have been previous hints that the transiting planet WASP-3b is accompanied by a second planet in a nearby orbit, based on small deviations from strict periodicity of the observed transits. Here we present 17 precise radial velocity (RV) measurements and 32 transit light curves that were acquired between 2009 and 2011. These data were used to refine the parameters of the host star and transiting planet. This has resulted in reduced uncertainties for the radii and masses of the star and planet. The RV data and the transit times show no evidence for an additional planet in the system. Therefore, we have determined the upper limit on the mass of any hypothetical second planet, as a function of its orbital period. United States. National Aeronautics and Space Administration (Origins program) Massachusetts Institute of Technology. Undergraduate Research Opportunities Program 2014-08-11T19:07:15Z 2014-08-11T19:07:15Z 2013-10 2013-08 Article http://purl.org/eprint/type/JournalArticle 0004-6256 1538-3881 http://hdl.handle.net/1721.1/88681 Maciejewski, G., et al. "CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM." The Astronomical Journal 146(6): 147. https://orcid.org/0000-0002-4265-047X en_US http://dx.doi.org/10.1088/0004-6256/146/6/147 The Astronomical Journal Creative Commons Attribution-Noncommercial-Share Alike http://creativecommons.org/licenses/by-nc-sa/4.0/ application/pdf IOP Publishing arXiv
spellingShingle Winn, Joshua Nathan
McKnight, Laura A.
CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
title CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
title_full CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
title_fullStr CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
title_full_unstemmed CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
title_short CONSTRAINTS ON A SECOND PLANET IN THE WASP-3 SYSTEM
title_sort constraints on a second planet in the wasp 3 system
url http://hdl.handle.net/1721.1/88681
https://orcid.org/0000-0002-4265-047X
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