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Two Transiting Low Density Sub-Saturns from K2

Petigura, Erik A. and Howard, Andrew W. and Lopez, Eric D. and Deck, Katherine M. and Fulton, Benjamin J. and Crossfield, Ian J. M. and Ciardi, David R. and Chiang, Eugene and Lee, Eve J. and Isaacson, Howard and Beichman, Charles A. and Hansen, Brad M. S. and Schlieder, Joshua E. and Sinukoff, Evan (2016) Two Transiting Low Density Sub-Saturns from K2. Astrophysical Journal, 818 (1). Art. No. 36. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20160311-123435885

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Abstract

We report the discovery and confirmation of K2-24 b and c, two sub-Saturn planets orbiting a bright (V = 11.3), metal-rich ([Fe/H] = 0.42 ± 0.04 dex) G3 dwarf in the K2 Campaign 2 field. The planets are 5.68 ± 0.56 R_⊕ and 7.82 ± 0.72 R_⊕ and have orbital periods of 20.8851 ± 0.0003 days and 42.3633 ± 0.0006 days, near the 2:1 mean-motion resonance. We obtained 32 radial velocities with Keck/HIRES and detected the reflex motion due to K2-24 b and c. These planets have masses of 21.0 ± 5.4 M_⊕ and 27.0 ± 6.9 M_⊕, respectively. With low densities of 0.63 ± 0.25 g cm^(−3) and 0.31 ± 0.12 g cm^(−3), respectively, the planets require thick envelopes of H/He to explain their large sizes and low masses. Interior structure models predict that the planets have fairly massive cores of 17.6 ± 4.3 M_⊕ and 16.1 ± 4.2 M_⊕, respectively. They may have formed exterior to their present locations, accreted their H/He envelopes at large orbital distances, and migrated in as a resonant pair. The proximity to resonance, large transit depths, and host star brightness offers rich opportunities for TTV follow-up. Finally, the low surface gravities of the K2-24 planets make them favorable targets for transmission spectroscopy by Hubble Space Telescope, Spitzer, and James Webb Space Telescope.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.3847/0004-637X/818/1/36UNSPECIFIEDArticle
http://iopscience.iop.org/article/10.3847/0004-637X/818/1/36UNSPECIFIEDArticle
http://arxiv.org/abs/1511.04497arXivDiscussion Paper
ORCID:
AuthorORCID
Petigura, Erik A.0000-0003-0967-2893
Howard, Andrew W.0000-0001-8638-0320
Fulton, Benjamin J.0000-0003-3504-5316
Crossfield, Ian J. M.0000-0002-1835-1891
Ciardi, David R.0000-0002-5741-3047
Chiang, Eugene0000-0002-6246-2310
Lee, Eve J.0000-0002-1228-9820
Isaacson, Howard0000-0002-0531-1073
Beichman, Charles A.0000-0002-5627-5471
Hansen, Brad M. S.0000-0001-7840-3502
Schlieder, Joshua E.0000-0001-5347-7062
Sinukoff, Evan0000-0002-5658-0601
Additional Information:© 2016 American Astronomical Society. Received 2015 November 13; accepted 2015 December 26; published 2016 February 4. We thank Geoffrey Marcy, Konstantin Batygin, and Leslie Rogers for helpful discussions. We thank an anonymous referee for valuable comments. E. A. P. acknowledges support from a 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. A. W. H. acknowledges support for our K2 team through a NASA Astrophysics Data Analysis Program grant. A. W. H. and I. J. M. C. acknowledge support from the K2 Guest Observer Program. E. D. L. received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement number 313014 (ETAEARTH). B. J. F. acknowledges support from a National Science Foundation Graduate Research Fellowship under grant No. 2014184874. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. This work made use of the SIMBAD database (operated at CDS, Strasbourg, France), NASA's Astrophysics Data System Bibliographic Services, and data products from the Two Micron All Sky Survey (2MASS), the APASS database, the SDSS-III project, and the Digitized Sky Survey. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. Some of the data presented herein were obtained at the W. M. Keck Observatory (which is operated as a scientific partnership among Caltech, UC, and NASA). 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. Facility: Kepler - , Keck: I - (HIRES - ), Keck: II - (NIRC2 - ).
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASA Hubble FellowshipHST-HF2-51365.001-A
NASANAS 5-26555
European Research Council (ERC)313014 (ETAEARTH)
NSF Graduate Research Fellowship2014184874
Department of Energy (DOE)DE-AC02-05CH11231
NASANNX09AF08G
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:planets and satellites: detection; stars: individual (EPIC-203771098) ; techniques: photometric; techniques: spectroscopic
Issue or Number:1
Record Number:CaltechAUTHORS:20160311-123435885
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160311-123435885
Official Citation:Erik A. Petigura et al 2016 ApJ 818 36
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:65302
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:11 Mar 2016 22:01
Last Modified:14 Oct 2019 21:33

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