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Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii

Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Wheatley, P. J.; Busuttil, R.; Liebig, C.; Anderson, D. R.; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Delrez, L.; Enoch, B.; Fumel, A.; Haswell, C. A.; Hébrard, G.; Hellier, C.; Holmes, S.; Jehin, E.; Kolb, U.; Maxted, P. F. L.; McCormac, J.; Miller, G. R. M.; Norton, A. J.; Pepe, F.; Queloz, D.; Rodríguez, J.; Ségransan, D.; Skillen, I.; Stassun, K. G.; Udry, S.; Watson, C.

Authors

Y. Gómez Maqueo Chew

F. Faedi

D. Pollacco

D. J. A. Brown

A. P. Doyle

A. Collier Cameron

M. Gillon

M. Lendl

A. H. M. J. Triaud

R. G. West

P. J. Wheatley

R. Busuttil

C. Liebig

D. R. Anderson

D. J. Armstrong

S. C. C. Barros

J. Bento

J. Bochinski

V. Burwitz

L. Delrez

B. Enoch

A. Fumel

C. A. Haswell

G. Hébrard

S. Holmes

E. Jehin

U. Kolb

J. McCormac

G. R. M. Miller

A. J. Norton

F. Pepe

D. Queloz

J. Rodríguez

D. Ségransan

I. Skillen

K. G. Stassun

S. Udry

C. Watson



Abstract

We report the discovery of two transiting hot Jupiters, WASP-65b (Mpl = 1.55 ± 0.16 MJ; Rpl = 1.11 ± 0.06 RJ), and WASP-75b (Mpl = 1.07 ± 0.05 MJ; Rpl = 1.27 ± 0.05 RJ). They orbit their host star every ~2.311, and ~2.484 days, respectively. The planet host WASP-65 is a G6 star (Teff = 5600 K, [Fe/H] = −0.07 ± 0.07, age ≳8 Gyr); WASP-75 is an F9 star (Teff = 6100 K, [Fe/H] = 0.07 ± 0.09, age ~ 3 Gyr). WASP-65b is one of the densest known exoplanets in the mass range 0.1 and 2.0 MJ (ρpl = 1.13 ± 0.08 ρJ), a mass range where a large fraction of planets are found to be inflated with respect to theoretical planet models. WASP-65b is one of only a handful of planets with masses of ~1.5 MJ, a mass regime surprisingly underrepresented among the currently known hot Jupiters. The radius of WASP-75b is slightly inflated (≲10%) as compared to theoretical planet models with no core, and has a density similar to that of Saturn (ρpl = 0.52 ± 0.06 ρJ).

Citation

Gómez Maqueo Chew, Y., Faedi, F., Pollacco, D., Brown, D. J. A., Doyle, A. P., Collier Cameron, A., …Watson, C. (2013). Discovery of WASP-65b and WASP-75b: Two hot Jupiters without highly inflated radii. Astronomy & Astrophysics, 559, Article A36. https://doi.org/10.1051/0004-6361/201322314

Journal Article Type Article
Acceptance Date Sep 27, 2013
Online Publication Date Nov 1, 2013
Publication Date 2013-11
Deposit Date Jun 15, 2023
Journal Astronomy & Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 559
Article Number A36
DOI https://doi.org/10.1051/0004-6361/201322314
Keywords Space and Planetary Science; Astronomy and Astrophysics