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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IOP Publishing
2014
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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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format | Article |
id | mit-1721.1/88681 |
institution | Massachusetts Institute of Technology |
language | en_US |
last_indexed | 2024-09-23T11:24:45Z |
publishDate | 2014 |
publisher | IOP Publishing |
record_format | dspace |
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 |
work_keys_str_mv | AT winnjoshuanathan constraintsonasecondplanetinthewasp3system AT mcknightlauraa constraintsonasecondplanetinthewasp3system |