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TOI-1338 : TESS' first transiting circumbinary planet

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Kostov_2020_AJ_159_253.pdf (2.607Mb)
Date
06/2020
Author
Kostov, Veselin B.
Orosz, Jerome A.
Feinstein, Adina D.
Welsh, William F.
Cukier, Wolf
Haghighipour, Nader
Quarles, Billy
Martin, David V.
Montet, Benjamin T.
Torres, Guillermo
Triaud, Amaury H. M. J.
Barclay, Thomas
Boyd, Patricia
Briceno, Cesar
Cameron, Andrew Collier
Correia, Alexandre C. M.
Gilbert, Emily A.
Gill, Samuel
Gillon, Michaël
Haqq-Misra, Jacob
Hellier, Coel
Dressing, Courtney
Fabrycky, Daniel C.
Furesz, Gabor
Jenkins, Jon M.
Kane, Stephen R.
Kopparapu, Ravi
Hodžić, Vedad Kunovac
Latham, David W.
Law, Nicholas
Levine, Alan M.
Li, Gongjie
Lintott, Chris
Lissauer, Jack J.
Mann, Andrew W.
Mazeh, Tsevi
Mardling, Rosemary
Maxted, Pierre F. L.
Eisner, Nora
Pepe, Francesco
Pepper, Joshua
Pollacco, Don
Quinn, Samuel N.
Quintana, Elisa V.
Rowe, Jason F.
Ricker, George
Rose, Mark E.
Seager, S.
Santerne, Alexandre
Ségransan, Damien
Short, Donald R.
Smith, Jeffrey C.
Standing, Matthew R.
Tokovinin, Andrei
Trifonov, Trifon
Turner, Oliver
Twicken, Joseph D.
Udry, Stéphane
Vanderspek, Roland
Winn, Joshua N.
Wolf, Eric T.
Ziegler, Carl
Ansorge, Peter
Barnet, Frank
Bergeron, Joel
Huten, Marc
Pappa, Giuseppe
van der Straeten, Timo
Funder
Science & Technology Facilities Council
Grant ID
ST/R00824/1
Keywords
Exoplanet astronony
Eclipsing binary stars
QB Astronomy
QC Physics
3rd-DAS
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Abstract
We report the detection of the first circumbinary planet (CBP) found by Transiting Exoplanet Survey Satellite (TESS). The target, a known eclipsing binary, was observed in sectors 1 through 12 at 30 minute cadence and in sectors 4 through 12 at 2 minute cadence. It consists of two stars with masses of 1.1 M⊙ and 0.3 M⊙ on a slightly eccentric (0.16), 14.6 day orbit, producing prominent primary eclipses and shallow secondary eclipses. The planet has a radius of ∼6.9 R⊕ and was observed to make three transits across the primary star of roughly equal depths (∼0.2%) but different durations—a common signature of transiting CBPs. Its orbit is nearly circular (e ≍ 0.09) with an orbital period of 95.2 days. The orbital planes of the binary and the planet are aligned to within ∼1°. To obtain a complete solution for the system, we combined the TESS photometry with existing ground-based radial-velocity observations in a numerical photometric-dynamical model. The system demonstrates the discovery potential of TESS for CBPs and provides further understanding of the formation and evolution of planets orbiting close binary stars.
Citation
Kostov , V B , Orosz , J A , Feinstein , A D , Welsh , W F , Cukier , W , Haghighipour , N , Quarles , B , Martin , D V , Montet , B T , Torres , G , Triaud , A H M J , Barclay , T , Boyd , P , Briceno , C , Cameron , A C , Correia , A C M , Gilbert , E A , Gill , S , Gillon , M , Haqq-Misra , J , Hellier , C , Dressing , C , Fabrycky , D C , Furesz , G , Jenkins , J M , Kane , S R , Kopparapu , R , Hodžić , V K , Latham , D W , Law , N , Levine , A M , Li , G , Lintott , C , Lissauer , J J , Mann , A W , Mazeh , T , Mardling , R , Maxted , P F L , Eisner , N , Pepe , F , Pepper , J , Pollacco , D , Quinn , S N , Quintana , E V , Rowe , J F , Ricker , G , Rose , M E , Seager , S , Santerne , A , Ségransan , D , Short , D R , Smith , J C , Standing , M R , Tokovinin , A , Trifonov , T , Turner , O , Twicken , J D , Udry , S , Vanderspek , R , Winn , J N , Wolf , E T , Ziegler , C , Ansorge , P , Barnet , F , Bergeron , J , Huten , M , Pappa , G & van der Straeten , T 2020 , ' TOI-1338 : TESS' first transiting circumbinary planet ' , Astronomical Journal , vol. 159 , no. 6 , 253 . https://doi.org/10.3847/1538-3881/ab8a48
Publication
Astronomical Journal
Status
Peer reviewed
DOI
https://doi.org/10.3847/1538-3881/ab8a48
ISSN
0004-6256
Type
Journal article
Rights
Copyright © 2020 American Astronomical Society. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.3847/1538-3881/ab8a48
Description
Funding: Funding for the DPAC has been provided by national institutions, in particular, the institutions participating in the Gaia Multilateral Agreement. W.F.W. and J.A.O.thank John Hood Jr. for his generous support of exoplanet research at SDSU. Support was also provided and acknowledged through NASA Habitable Worlds grant 80NSSC17K0741 and NASA XRP grant 80NSSC18K0519. This work is partly supported by NASA Habitable Worlds grant 80NSSC17K0741. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship Program under grant No.(DGE-1746045). A.H.M.J.T. has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 803193/BEBOP) and from a Leverhulme Trust Research Project grant No. RPG-2018-418. A.C. acknowledges support by CFisUC strategic project (UID/FIS/04564/2019).
Collections
  • University of St Andrews Research
URL
http://adsabs.harvard.edu/abs/2020AJ....159..253K
URI
http://hdl.handle.net/10023/20067

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