Ares Osborn
TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet
Osborn, Ares; Armstrong, David J; Cale, Bryson; Brahm, Rafael; Wittenmyer, Robert A; Dai, Fei; Crossfield, Ian J M; Bryant, Edward M; Adibekyan, Vardan; Cloutier, Ryan; Collins, Karen A; Mena, E Delgado; Fridlund, Malcolm; Hellier, Coel; Howell, Steve B; King, George W; Lillo-Box, Jorge; Otegi, Jon; Sousa, S; Stassun, Keivan G; Matthews, Elisabeth C; Ziegler, Carl; Ricker, George; Vanderspek, Roland; Latham, David W; Seager, S; Winn, Joshua N; Jenkins, Jon M; Acton, Jack S; Addison, Brett C; Anderson, David R; Ballard, Sarah; Barrado, David; Barros, Susana C C; Batalha, Natalie; Bayliss, Daniel; Barclay, Thomas; Benneke, Björn; Berberian Jr., John; Bouchy, Francois; Bowler, Brendan P; Briceño, César; Burke, Christopher J; Burleigh, Matthew R; Casewell, Sarah L; Ciardi, David; Collins, Kevin I; Cooke, Benjamin F; Demangeon, Olivier D S; Díaz, Rodrigo F; Dorn, C; Dragomir, Diana; Dressing, Courtney; Dumusque, Xavier; Espinoza, Néstor; Figueira, P; Fulton, Benjamin; Furlan, E; Gaidos, E;...
Authors
David J Armstrong
Bryson Cale
Rafael Brahm
Robert A Wittenmyer
Fei Dai
Ian J M Crossfield
Edward M Bryant
Vardan Adibekyan
Ryan Cloutier
Karen A Collins
E Delgado Mena
Malcolm Fridlund
Coel Hellier c.hellier@keele.ac.uk
Steve B Howell
George W King
Jorge Lillo-Box
Jon Otegi
S Sousa
Keivan G Stassun
Elisabeth C Matthews
Carl Ziegler
George Ricker
Roland Vanderspek
David W Latham
S Seager
Joshua N Winn
Jon M Jenkins
Jack S Acton
Brett C Addison
David R Anderson
Sarah Ballard
David Barrado
Susana C C Barros
Natalie Batalha
Daniel Bayliss
Thomas Barclay
Björn Benneke
John Berberian Jr.
Francois Bouchy
Brendan P Bowler
César Briceño
Christopher J Burke
Matthew R Burleigh
Sarah L Casewell
David Ciardi
Kevin I Collins
Benjamin F Cooke
Olivier D S Demangeon
Rodrigo F Díaz
C Dorn
Diana Dragomir
Courtney Dressing
Xavier Dumusque
Néstor Espinoza
P Figueira
Benjamin Fulton
E Furlan
E Gaidos
C Geneser
Samuel Gill
Michael R Goad
Erica J Gonzales
Varoujan Gorjian
Maximilian N Günther
Ravit Helled
Beth A Henderson
Thomas Henning
Aleisha Hogan
Saeed Hojjatpanah
Jonathan Horner
Andrew W Howard
Sergio Hoyer
Dan Huber
Howard Isaacson
James S Jenkins
Eric L N Jensen
Andrés Jordán
Stephen R Kane
Richard C Kidwell Jr.
John Kielkopf
Nicholas Law
Monika Lendl
M Lund
Rachel A Matson
Andrew W Mann
James McCormac
Matthew W Mengel
Farisa Y Morales
Louise D Nielsen
Jack Okumura
Hugh P Osborn
Erik A Petigura
Peter Plavchan
Don Pollacco
Elisa V Quintana
Liam Raynard
Paul Robertson
Mark E Rose
Arpita Roy
Michael Reefe
Alexandre Santerne
Nuno C Santos
Paula Sarkis
J Schlieder
Richard P Schwarz
Nicholas J Scott
Avi Shporer
A M S Smith
C Stibbard
Chris Stockdale
Paul A Strøm
Joseph D Twicken
Thiam-Guan Tan
A Tanner
J Teske
Rosanna H Tilbrook
C G Tinney
Stephane Udry
Jesus Noel Villaseñor
Jose I Vines
Sharon X Wang
Lauren M Weiss
Richard G West
Peter J Wheatley
Duncan J Wright
Hui Zhang
F Zohrabi
Abstract
We present the bright (Vmag = 9.12), multiplanet system TOI-431, characterized with photometry and radial velocities (RVs). We estimate the stellar rotation period to be 30.5 ± 0.7 d using archival photometry and RVs. Transiting Exoplanet Survey Satellite (TESS) objects of Interest (TOI)-431?b is a super-Earth with a period of 0.49 d, a radius of 1.28 ± 0.04 R?, a mass of 3.07 ± 0.35 M?, and a density of 8.0 ± 1.0 g cm-3; TOI-431 d is a sub-Neptune with a period of 12.46 d, a radius of 3.29 ± 0.09 R?, a mass of 9.90+1.53-1.49 M?, and a density of 1.36 ± 0.25 g cm-3. We find a third planet, TOI-431?c, in the High Accuracy Radial velocity Planet Searcher RV data, but it is not seen to transit in the TESS light curves. It has an Msin i of 2.83+0.41-0.34 M?, and a period of 4.85 d. TOI-431?d likely has an extended atmosphere and is one of the most well-suited TESS discoveries for atmospheric characterization, while the super-Earth TOI-431?b may be a stripped core. These planets straddle the radius gap, presenting an interesting case-study for atmospheric evolution, and TOI-431?b is a prime TESS discovery for the study of rocky planet phase curves.
Citation
Osborn, A., Armstrong, D. J., Cale, B., Brahm, R., Wittenmyer, R. A., Dai, F., …Zohrabi, F. (2021). TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet. Monthly Notices of the Royal Astronomical Society, 507(2), 2782 - 2803. https://doi.org/10.1093/mnras/stab2313
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 3, 2021 |
Online Publication Date | Aug 11, 2021 |
Publication Date | 2021-10 |
Publicly Available Date | May 30, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 507 |
Issue | 2 |
Pages | 2782 - 2803 |
DOI | https://doi.org/10.1093/mnras/stab2313 |
Keywords | Space and Planetary Science, Astronomy and Astrophysics |
Publisher URL | https://academic.oup.com/mnras/article-abstract/507/2/2782/6348103?redirectedFrom=fulltext |
Files
stab2313.pdf
(4 Mb)
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Publisher Licence URL
https://creativecommons.org/licenses/by-nc/4.0/
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