Kepler constraints on planets near hot Jupiters
Creators
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1.
Fermilab
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2.
Harvard-Smithsonian Center for Astrophysics
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3.
University of California, Santa Cruz
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4.
University of Florida
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5.
Ames Research Center
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6.
San Diego State University
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7.
National Aeronautics and Space Administration
Abstract
We present the results of a search for planetary companions orbiting near hot Jupiter planet candidates (Jupiter-size candidates with orbital periods near 3 d) identified in the Kepler data through its sixth quarter of science operations. Special emphasis is given to companions between the 2∶1 interior and exterior mean-motion resonances. A photometric transit search excludes companions with sizes ranging from roughly two-thirds to five times the size of the Earth, depending upon the noise properties of the target star. A search for dynamically induced deviations from a constant period (transit timing variations) also shows no significant signals. In contrast, comparison studies of warm Jupiters (with slightly larger orbits) and hot Neptune-size candidates do exhibit signatures of additional companions with these same tests. These differences between hot Jupiters and other planetary systems denote a distinctly different formation or dynamical history.
Additional Information
© 2012 National Academy of Sciences. Edited by Neta A. Bahcall, Princeton University, Princeton, NJ, and approved March 23, 2012 (received for review December 19, 2011). Funding for the Kepler mission is provided by the National Aeronautics and Space Administration's (NASA) Science Mission Directorate. We thank the Kepler team for their many years of hard work. J.H.S acknowledges support from NASA under Grant NNX08AR04G under the Kepler Participating Scientist Program. D.C.F. and J.A.C. acknowledge support from NASA through Hubble Fellowship Grants HF-51272.01-A and HF-51267.01-A awarded by the Space Telescope Science Institute, operated by the Association of Universities for Research in Astronomy, Inc., under Contract NAS 5-26555. Author contributions: J.H.S. and M.J.H. designed research; D.R., D.C.F., E.B.F., W.F.W., W.J.B., A.P.B., D.R.C., and S.N.Q. performed research; J.A.C. and J.F.R. analyzed data; and J.H.S. wrote the paper.Attached Files
Published - Steffen2012p18426P_Natl_Acad_Sci_Usa.pdf
Files
Steffen2012p18426P_Natl_Acad_Sci_Usa.pdf
Additional details
Identifiers
- PMCID
- PMC3361435
- Eprint ID
- 31894
- Resolver ID
- CaltechAUTHORS:20120613-132754013
Funding
- NASA
- NNX08AR04G
- NASA Hubble Fellowship
- HF-51272.01-A
- NASA Hubble Fellowship
- HF-51267.01-A
- Space Telescope Science Institute
Dates
- Created
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2012-06-14Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field