Bibcode
Cooke, Benjamin F.; Pollacco, Don; Almleaky, Y.; Barkaoui, K.; Benkhaldoun, Z.; Blake, James A.; Bouchy, François; Boumis, Panos; Brown, D. J. A.; Bruni, Ivan; Burdanov, A.; Cameron, Andrew Collier; Chote, Paul; Daassou, A.; D'ago, Giuseppe; Dalal, Shweta; Damasso, Mario; Delrez, L.; Doyle, A. P.; Ducrot, E.; Gillon, M.; Hébrard, G.; Hellier, C.; Henning, Thomas; Jehin, E.; Kiefer, Flavien; King, George W.; Liakos, Alexios; Lopez, Théo; Mancini, Luigi; Mardling, Rosemary; Maxted, P. F. L.; McCormac, James; Murray, C.; Nielsen, Louise D.; Osborn, Hugh; Palle, E.; Pepe, Francesco; Pozuelos, F. J.; Prieto-Arranz, J.; Queloz, D.; Schanche, Nicole; Ségransan, Damien; Smalley, Barry; Southworth, John; Thompson, S.; Turner, Oliver; Udry, Stéphane; Velasco, S.; West, Richard; Wheatley, Pete
Bibliographical reference
The Astronomical Journal
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6
2020
Citations
6
Refereed citations
5
Description
We report the discovery of two transiting exoplanets from the WASP survey, WASP-150b and WASP-176b. WASP-150b is an eccentric (e = 0.38) hot Jupiter on a 5.6 day orbit around a V = 12.03, F8 main-sequence host. The host star has a mass and radius of 1.4 ${M}_{\odot }$ and 1.7 ${R}_{\odot }$ respectively. WASP-150b has a mass and radius of 8.5 ${M}_{{\rm{J}}}$ and 1.1 RJ, leading to a large planetary bulk density of 6.4 ρJ. WASP-150b is found to be ∼3 Gyr old, well below its circularization timescale, supporting the eccentric nature of the planet. WASP-176b is a hot Jupiter planet on a 3.9 day orbit around a V = 12.01, F9 sub-giant host. The host star has a mass and radius of 1.3 M☉ and 1.9 R☉. WASP-176b has a mass and radius of 0.86 MJ and 1.5 RJ, respectively, leading to a planetary bulk density of 0.23 ρJ.
Related projects
Exoplanets and Astrobiology
The search for life in the universe has been driven by recent discoveries of planets around other stars (known as exoplanets), becoming one of the most active fields in modern astrophysics. The growing number of new exoplanets discovered in recent years and the recent advance on the study of their atmospheres are not only providing new valuable
Enric
Pallé Bago