TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite

Rafael Brahm; Louise D. Nielsen; Robert A. Wittenmyer; Songhu Wang; Joseph E. Rodriguez; Néstor Espinoza; Matías I. Jones; Andrés Jordán; Thomas Henning; Melissa Hobson; Diana Kossakowski; Felipe Rojas; Paula Sarkis; Martin Schlecker; Trifon Trifonov; Sahar Shahaf; George Ricker; Roland Vanderspek; David W. Latham; Sara Seager; Joshua N. Winn; Jon M. Jenkins; Brett C. Addison; Gáspár Bakos; Waqas Bhatti; Daniel Bayliss; Perry Berlind; Allyson Bieryla; Francois Bouchy; Brendan P. Bowler; César Brice&ntilde;o; Timothy M. Brown; Edward M. Bryant; Douglas A. Caldwell; David Charbonneau; Karen A. Collins; Allen B. Davis; Gilbert A. Esquerdo; Benjamin J. Fulton; Natalia M. Guerrero; Christopher E. Henze; Aleisha Hogan; Jonathan Horner; Chelsea X. Huang; Jonathan Irwin; Stephen R. Kane; John Kielkopf; Andrew W. Mann; Tsevi Mazeh; James McCormac; Curtis McCully; Matthew W. Mengel; Ismael Mireles; Jack Okumura; Peter Plavchan; Samuel N. Quinn; Markus Rabus; Sophie Saesen; Joshua E. Schlieder; Damien Segransan; Bernie Shiao; Avi Shporer; Robert J. Siverd; Keivan G. Stassun; Vincent Suc; Thiam Guan Tan; Pascal Torres; Chris G. Tinney; Stephane Udry; Leonardo Vanzi; Michael Vezie; Jose I. Vines; Maja Vuckovic; Duncan J. Wright; Daniel A. Yahalomi; Abner Zapata; Hui Zhang; Carl Ziegler

doi:10.3847/1538-3881/abba3b

TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite

Rafael Brahm
, Louise D. Nielsen
, Robert A. Wittenmyer
, Songhu Wang
, Joseph E. Rodriguez
, Néstor Espinoza
, Matías I. Jones
, Andrés Jordán
, Thomas Henning
, Melissa Hobson
, Diana Kossakowski
, Felipe Rojas
, Paula Sarkis
, Martin Schlecker
, Trifon Trifonov
, Sahar Shahaf
, George Ricker
, Roland Vanderspek
, David W. Latham
, Sara Seager

Joshua N. Winn, Jon M. Jenkins, Brett C. Addison, Gáspár Bakos, Waqas Bhatti, Daniel Bayliss, Perry Berlind, Allyson Bieryla, Francois Bouchy, Brendan P. Bowler, César Briceño, Timothy M. Brown, Edward M. Bryant, Douglas A. Caldwell, David Charbonneau, Karen A. Collins, Allen B. Davis, Gilbert A. Esquerdo, Benjamin J. Fulton, Natalia M. Guerrero, Christopher E. Henze, Aleisha Hogan, Jonathan Horner, Chelsea X. Huang, Jonathan Irwin, Stephen R. Kane, John Kielkopf, Andrew W. Mann, Tsevi Mazeh, James McCormac, Curtis McCully, Matthew W. Mengel, Ismael Mireles, Jack Okumura, Peter Plavchan, Samuel N. Quinn, Markus Rabus, Sophie Saesen, Joshua E. Schlieder, Damien Segransan, Bernie Shiao, Avi Shporer, Robert J. Siverd, Keivan G. Stassun, Vincent Suc, Thiam Guan Tan, Pascal Torres, Chris G. Tinney, Stephane Udry, Leonardo Vanzi, Michael Vezie, Jose I. Vines, Maja Vuckovic, Duncan J. Wright, Daniel A. Yahalomi, Abner Zapata, Hui Zhang, Carl Ziegler

Research output: Contribution to journal › Article › peer-review

38 Scopus citations

Abstract

We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have similar radii (0.99 0.01 and 1.07 0.02, respectively), and orbital periods (10.3311 days and 10.6266 days, respectively), but significantly different masses (1.53 0.03, respectively). Both planets orbit metal-rich stars ( = dex and = for TOI-481 and TOI-892, respectively) but at different evolutionary stages. TOI-481 is a = 1.14 0.02 = 1.66 0.02 G-type star (=K), that with an age of 6.7 Gyr, is in the turn-off point of the main sequence. TOI-892 on the other hand, is a F-type dwarf star (=K), which has a mass of = 1.28 0.03 and a radius of = 1.39 0.02. TOI-481 b and TOI-892 b join the scarcely populated region of transiting gas giants with orbital periods longer than 10 days, which is important to constrain theories of the formation and structure of hot Jupiters.

Original language	English
Article number	235
Journal	Astronomical Journal
Volume	160
Issue number	5
DOIs	https://doi.org/10.3847/1538-3881/abba3b
State	Published - Nov 2020
Externally published	Yes

Access to Document

10.3847/1538-3881/abba3b

Cite this

Brahm, R., Nielsen, L. D., Wittenmyer, R. A., Wang, S., Rodriguez, J. E., Espinoza, N., Jones, M. I., Jordán, A., Henning, T., Hobson, M., Kossakowski, D., Rojas, F., Sarkis, P., Schlecker, M., Trifonov, T., Shahaf, S., Ricker, G., Vanderspek, R., Latham, D. W., ... Ziegler, C. (2020). TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite. Astronomical Journal, 160(5), Article 235. https://doi.org/10.3847/1538-3881/abba3b

@article{ab84b11f22644d8d8b222fd47e10371d,

title = "TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite",

abstract = "We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have similar radii (0.99 0.01 and 1.07 0.02, respectively), and orbital periods (10.3311 days and 10.6266 days, respectively), but significantly different masses (1.53 0.03, respectively). Both planets orbit metal-rich stars ( = dex and = for TOI-481 and TOI-892, respectively) but at different evolutionary stages. TOI-481 is a = 1.14 0.02 = 1.66 0.02 G-type star (=K), that with an age of 6.7 Gyr, is in the turn-off point of the main sequence. TOI-892 on the other hand, is a F-type dwarf star (=K), which has a mass of = 1.28 0.03 and a radius of = 1.39 0.02. TOI-481 b and TOI-892 b join the scarcely populated region of transiting gas giants with orbital periods longer than 10 days, which is important to constrain theories of the formation and structure of hot Jupiters.",

author = "Rafael Brahm and Nielsen, \{Louise D.\} and Wittenmyer, \{Robert A.\} and Songhu Wang and Rodriguez, \{Joseph E.\} and N{\'e}stor Espinoza and Jones, \{Mat{\'i}as I.\} and Andr{\'e}s Jord{\'a}n and Thomas Henning and Melissa Hobson and Diana Kossakowski and Felipe Rojas and Paula Sarkis and Martin Schlecker and Trifon Trifonov and Sahar Shahaf and George Ricker and Roland Vanderspek and Latham, \{David W.\} and Sara Seager and Winn, \{Joshua N.\} and Jenkins, \{Jon M.\} and Addison, \{Brett C.\} and G{\'a}sp{\'a}r Bakos and Waqas Bhatti and Daniel Bayliss and Perry Berlind and Allyson Bieryla and Francois Bouchy and Bowler, \{Brendan P.\} and C{\'e}sar Brice\ño and Brown, \{Timothy M.\} and Bryant, \{Edward M.\} and Caldwell, \{Douglas A.\} and David Charbonneau and Collins, \{Karen A.\} and Davis, \{Allen B.\} and Esquerdo, \{Gilbert A.\} and Fulton, \{Benjamin J.\} and Guerrero, \{Natalia M.\} and Henze, \{Christopher E.\} and Aleisha Hogan and Jonathan Horner and Huang, \{Chelsea X.\} and Jonathan Irwin and Kane, \{Stephen R.\} and John Kielkopf and Mann, \{Andrew W.\} and Tsevi Mazeh and James McCormac and Curtis McCully and Mengel, \{Matthew W.\} and Ismael Mireles and Jack Okumura and Peter Plavchan and Quinn, \{Samuel N.\} and Markus Rabus and Sophie Saesen and Schlieder, \{Joshua E.\} and Damien Segransan and Bernie Shiao and Avi Shporer and Siverd, \{Robert J.\} and Stassun, \{Keivan G.\} and Vincent Suc and Tan, \{Thiam Guan\} and Pascal Torres and Tinney, \{Chris G.\} and Stephane Udry and Leonardo Vanzi and Michael Vezie and Vines, \{Jose I.\} and Maja Vuckovic and Wright, \{Duncan J.\} and Yahalomi, \{Daniel A.\} and Abner Zapata and Hui Zhang and Carl Ziegler",

year = "2020",

month = nov,

doi = "10.3847/1538-3881/abba3b",

language = "English",

volume = "160",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "5",

}

Brahm, R, Nielsen, LD, Wittenmyer, RA, Wang, S, Rodriguez, JE, Espinoza, N, Jones, MI, Jordán, A, Henning, T, Hobson, M, Kossakowski, D, Rojas, F, Sarkis, P, Schlecker, M, Trifonov, T, Shahaf, S, Ricker, G, Vanderspek, R, Latham, DW, Seager, S, Winn, JN, Jenkins, JM, Addison, BC, Bakos, G, Bhatti, W, Bayliss, D, Berlind, P, Bieryla, A, Bouchy, F, Bowler, BP, Briceño, C, Brown, TM, Bryant, EM, Caldwell, DA, Charbonneau, D, Collins, KA, Davis, AB, Esquerdo, GA, Fulton, BJ, Guerrero, NM, Henze, CE, Hogan, A, Horner, J, Huang, CX, Irwin, J, Kane, SR, Kielkopf, J, Mann, AW, Mazeh, T, McCormac, J, McCully, C, Mengel, MW, Mireles, I, Okumura, J, Plavchan, P, Quinn, SN, Rabus, M, Saesen, S, Schlieder, JE, Segransan, D, Shiao, B, Shporer, A, Siverd, RJ, Stassun, KG, Suc, V, Tan, TG, Torres, P, Tinney, CG, Udry, S, Vanzi, L, Vezie, M, Vines, JI, Vuckovic, M, Wright, DJ, Yahalomi, DA, Zapata, A, Zhang, H & Ziegler, C 2020, 'TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite', Astronomical Journal, vol. 160, no. 5, 235. https://doi.org/10.3847/1538-3881/abba3b

TY - JOUR

T1 - TOI-481 b and TOI-892 b

T2 - Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite

AU - Brahm, Rafael

AU - Nielsen, Louise D.

AU - Wittenmyer, Robert A.

AU - Wang, Songhu

AU - Rodriguez, Joseph E.

AU - Espinoza, Néstor

AU - Jones, Matías I.

AU - Jordán, Andrés

AU - Henning, Thomas

AU - Hobson, Melissa

AU - Kossakowski, Diana

AU - Rojas, Felipe

AU - Sarkis, Paula

AU - Schlecker, Martin

AU - Trifonov, Trifon

AU - Shahaf, Sahar

AU - Ricker, George

AU - Vanderspek, Roland

AU - Latham, David W.

AU - Seager, Sara

AU - Winn, Joshua N.

AU - Jenkins, Jon M.

AU - Addison, Brett C.

AU - Bakos, Gáspár

AU - Bhatti, Waqas

AU - Bayliss, Daniel

AU - Berlind, Perry

AU - Bieryla, Allyson

AU - Bouchy, Francois

AU - Bowler, Brendan P.

AU - Briceño, César

AU - Brown, Timothy M.

AU - Bryant, Edward M.

AU - Caldwell, Douglas A.

AU - Charbonneau, David

AU - Collins, Karen A.

AU - Davis, Allen B.

AU - Esquerdo, Gilbert A.

AU - Fulton, Benjamin J.

AU - Guerrero, Natalia M.

AU - Henze, Christopher E.

AU - Hogan, Aleisha

AU - Horner, Jonathan

AU - Huang, Chelsea X.

AU - Irwin, Jonathan

AU - Kane, Stephen R.

AU - Kielkopf, John

AU - Mann, Andrew W.

AU - Mazeh, Tsevi

AU - McCormac, James

AU - McCully, Curtis

AU - Mengel, Matthew W.

AU - Mireles, Ismael

AU - Okumura, Jack

AU - Plavchan, Peter

AU - Quinn, Samuel N.

AU - Rabus, Markus

AU - Saesen, Sophie

AU - Schlieder, Joshua E.

AU - Segransan, Damien

AU - Shiao, Bernie

AU - Shporer, Avi

AU - Siverd, Robert J.

AU - Stassun, Keivan G.

AU - Suc, Vincent

AU - Tan, Thiam Guan

AU - Torres, Pascal

AU - Tinney, Chris G.

AU - Udry, Stephane

AU - Vanzi, Leonardo

AU - Vezie, Michael

AU - Vines, Jose I.

AU - Vuckovic, Maja

AU - Wright, Duncan J.

AU - Yahalomi, Daniel A.

AU - Zapata, Abner

AU - Zhang, Hui

AU - Ziegler, Carl

PY - 2020/11

Y1 - 2020/11

N2 - We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have similar radii (0.99 0.01 and 1.07 0.02, respectively), and orbital periods (10.3311 days and 10.6266 days, respectively), but significantly different masses (1.53 0.03, respectively). Both planets orbit metal-rich stars ( = dex and = for TOI-481 and TOI-892, respectively) but at different evolutionary stages. TOI-481 is a = 1.14 0.02 = 1.66 0.02 G-type star (=K), that with an age of 6.7 Gyr, is in the turn-off point of the main sequence. TOI-892 on the other hand, is a F-type dwarf star (=K), which has a mass of = 1.28 0.03 and a radius of = 1.39 0.02. TOI-481 b and TOI-892 b join the scarcely populated region of transiting gas giants with orbital periods longer than 10 days, which is important to constrain theories of the formation and structure of hot Jupiters.

AB - We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have similar radii (0.99 0.01 and 1.07 0.02, respectively), and orbital periods (10.3311 days and 10.6266 days, respectively), but significantly different masses (1.53 0.03, respectively). Both planets orbit metal-rich stars ( = dex and = for TOI-481 and TOI-892, respectively) but at different evolutionary stages. TOI-481 is a = 1.14 0.02 = 1.66 0.02 G-type star (=K), that with an age of 6.7 Gyr, is in the turn-off point of the main sequence. TOI-892 on the other hand, is a F-type dwarf star (=K), which has a mass of = 1.28 0.03 and a radius of = 1.39 0.02. TOI-481 b and TOI-892 b join the scarcely populated region of transiting gas giants with orbital periods longer than 10 days, which is important to constrain theories of the formation and structure of hot Jupiters.

UR - https://www.scopus.com/pages/publications/85095767062

U2 - 10.3847/1538-3881/abba3b

DO - 10.3847/1538-3881/abba3b

M3 - Article

AN - SCOPUS:85095767062

SN - 0004-6256

VL - 160

JO - Astronomical Journal

JF - Astronomical Journal

IS - 5

M1 - 235

ER -

TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite

Abstract

Access to Document

Fingerprint

Cite this