CaltechAUTHORS
  A Caltech Library Service

The California-Kepler Survey. V. Peas in a Pod: Planets in a Kepler Multi-planet System Are Similar in Size and Regularly Spaced

Weiss, Lauren M. and Marcy, Geoffrey W. and Petigura, Erik A. and Fulton, Benjamin J. and Howard, Andrew W. and Winn, Joshua N. and Isaacson, Howard T. and Morton, Timothy D. and Hirsch, Lea A. and Sinukoff, Evan J. and Cumming, Andrew and Hebb, Leslie and Cargile, Phillip A. (2018) The California-Kepler Survey. V. Peas in a Pod: Planets in a Kepler Multi-planet System Are Similar in Size and Regularly Spaced. Astronomical Journal, 155 (1). Art. No. 48. ISSN 0004-6256. https://resolver.caltech.edu/CaltechAUTHORS:20180103-112110390

[img] PDF - Published Version
See Usage Policy.

1575Kb
[img] PDF - Submitted Version
See Usage Policy.

1154Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20180103-112110390

Abstract

We have established precise planet radii, semimajor axes, incident stellar fluxes, and stellar masses for 909 planets in 355 multi-planet systems discovered by Kepler. In this sample, we find that planets within a single multi-planet system have correlated sizes: each planet is more likely to be the size of its neighbor than a size drawn at random from the distribution of observed planet sizes. In systems with three or more planets, the planets tend to have a regular spacing: the orbital period ratios of adjacent pairs of planets are correlated. Furthermore, the orbital period ratios are smaller in systems with smaller planets, suggesting that the patterns in planet sizes and spacing are linked through formation and/or subsequent orbital dynamics. Yet, we find that essentially no planets have orbital period ratios smaller than 1.2, regardless of planet size. Using empirical mass–radius relationships, we estimate the mutual Hill separations of planet pairs. We find that 93% of the planet pairs are at least 10 mutual Hill radii apart, and that a spacing of ~20 mutual Hill radii is most common. We also find that when comparing planet sizes, the outer planet is larger in 65% ± 0.4% of cases, and the typical ratio of the outer to inner planet size is positively correlated with the temperature difference between the planets. This could be the result of photo-evaporation.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/1538-3881/aa9ff6DOIArticle
http://iopscience.iop.org/article/10.3847/1538-3881/aa9ff6PublisherArticle
https://arxiv.org/abs/1706.06204arXivDiscussion Paper
ORCID:
AuthorORCID
Weiss, Lauren M.0000-0002-3725-3058
Marcy, Geoffrey W.0000-0002-2909-0113
Petigura, Erik A.0000-0003-0967-2893
Fulton, Benjamin J.0000-0003-3504-5316
Howard, Andrew W.0000-0001-8638-0320
Winn, Joshua N.0000-0002-4265-047X
Isaacson, Howard T.0000-0002-0531-1073
Morton, Timothy D.0000-0002-8537-5711
Hirsch, Lea A.0000-0001-8058-7443
Sinukoff, Evan J.0000-0002-5658-0601
Cumming, Andrew0000-0002-6335-0169
Hebb, Leslie0000-0003-1263-8637
Additional Information:© 2018. The American Astronomical Society. Received 2017 June 18; revised 2017 December 4; accepted 2017 December 4; published 2018 January 3. The CKS project was conceived, planned, and initiated by A.W.H., G.W.M., J.A.J., H.T.I., and T.D.M. Keck time for the CKS multis project was acquired by G.W.M., with assistance from L.M.W. The observations were coordinated by H.T.I. and A.W.H. and carried out by A.W.H., H.T.I., G.W.M., J.A.J., T.D.M., B.J.F., L.M.W., E.A.P., E.S., and L.A.H. A.W.H. secured CKS project funding. SpecMatch was developed and run by E.A.P., and SME@XSEDE was developed and run by L.H. and P.A.C. Downstream data products were developed by E.A.P., H.T.I., and B.J.F. Results from the two pipelines were consolidated and the integrity of the parameters were verified by A.W.H., H.T.I., E.A.P., G.W.M., with assistance from B.J.F., L.M.W., E.S., L.A.H., and I.J.M.C. E.A.P. computed derived planetary and stellar properties with assistance from B.J.F. L.M.W. performed the analysis in this paper, with assistance from G.W.M., J.W., and A.C. This manuscript was largely written by L.M.W. with assistance from J.W. and G.W.M. We thank John Asher Johnson, a PI and originator of the magnitude-limited CKS survey. Conversations with Rebekah Dawson, Daniel Fabrycky, Eve Lee, Doug Lin, Jack Lissauer, Jason Rowe, and Scott Tremaine influenced this paper. We thank the referee for a thorough and insightful discussion. The results presented herein were made possible by observations at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA. We are grateful to the time assignment committees of the University of Hawaii, the University of California, the California Institute of Technology, and NASA for their generous allocations of observing time that enabled this large project. Kepler was competitively selected as the tenth NASA Discovery mission. Funding for this mission is provided by the NASA Science Mission Directorate. L.M.W. acknowledges support from Gloria and Ken Levy and from the Trottier Family Foundation. E.A.P. acknowledges support from Hubble Fellowship grant HST-HF2-51365.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc. for NASA under contract NAS 5-26555. B.J.F. acknowledges National Science Foundation Graduate Research Fellowship under grant No. 2014184874. A.W.H. acknowledges NASA grant NNX12AJ23. G.T.D.M. acknowledges NASA grant NNX14AE11G. P.A.C. acknowledges National Science Foundation grant AST-1109612. L.H. acknowledges National Science Foundation grant AST-1009810. E.S. is supported by a post-graduate scholarship from the Natural Sciences and Engineering Research Council of Canada. Finally, the authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Facilities: Keck:I (HIRES) - KECK I Telescope, Kepler - The Kepler Mission.
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
W. M. Keck FoundationUNSPECIFIED
NASANAS 5-26555
Gloria and Ken LevyUNSPECIFIED
Trottier Family FoundationUNSPECIFIED
NASA Hubble FellowshipHST-HF2-51365.001-A
NSF Graduate Research Fellowship2014184874
NASANNX12AJ23G
NASANNX14AE11G
NSFAST-1109612
NSFAST-1009810
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Subject Keywords:catalogs; planetary systems; stars: fundamental parameters; surveys
Issue or Number:1
Record Number:CaltechAUTHORS:20180103-112110390
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180103-112110390
Official Citation:Lauren M. Weiss et al 2018 AJ 155 48
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:84055
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:03 Jan 2018 20:48
Last Modified:03 Nov 2019 19:49

Repository Staff Only: item control page