Results 121 to 130 of about 624,657 (195)

The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201

The Astrophysical Journal Letters
Measuring the obliquities of stars hosting giant planets may shed light on the dynamical history of planetary systems. Significant efforts have been made to measure the obliquities of FGK stars with hot Jupiters, mainly based on observations of the ...
Tianjun Gan, Sharon X. Wang, Fei Dai, Joshua N. Winn, Shude Mao, Siyi Xu, Enric Pallé, Jacob L. Bean, Madison Brady, Nina Brown, Cicero Lu, Rafael Luque, Teo Mocnik, Andreas Seifahrt, Guđmundur K. Stefánsson   +14 more
doaj   +1 more source

Are Hot Jupiters Tidally Disrupted During Stellar Main Sequence?

The Astronomical Journal
Once hot Jupiters (HJs) reach their very close orbits, they are expected to experience orbital decay due to tidal interactions with their host star. However, the strength of tidal dissipation is highly uncertain, and it remains an open question whether ...
Qingru Hu, Wei Zhu, Yang Huang, Bowen Zhang   +3 more
doaj   +1 more source

A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b. [PDF]

Nature, 2023
Coulombe LP, Benneke B, Challener R, Piette AAA, Wiser LS, Mansfield M, MacDonald RJ, Beltz H, Feinstein AD, Radica M, Savel AB, Dos Santos LA, Bean JL, Parmentier V, Wong I, Rauscher E, Komacek TD, Kempton EM, Tan X, Hammond M, Lewis NT, Line MR, Lee EKH, Shivkumar H, Crossfield IJM, Nixon MC, Rackham BV, Wakeford HR, Welbanks L, Zhang X, Batalha NM, Berta-Thompson ZK, Changeat Q, Désert JM, Espinoza N, Goyal JM, Harrington J, Knutson HA, Kreidberg L, López-Morales M, Shporer A, Sing DK, Stevenson KB, Aggarwal K, Ahrer EM, Alam MK, Bell TJ, Blecic J, Caceres C, Carter AL, Casewell SL, Crouzet N, Cubillos PE, Decin L, Fortney JJ, Gibson NP, Heng K, Henning T, Iro N, Kendrew S, Lagage PO, Leconte J, Lendl M, Lothringer JD, Mancini L, Mikal-Evans T, Molaverdikhani K, Nikolov NK, Ohno K, Palle E, Piaulet C, Redfield S, Roy PA, Tsai SM, Venot O, Wheatley PJ.   +75 more
europepmc   +1 more source

Planetary population synthesis and the emergence of four classes of planetary system architectures. [PDF]

Eur Phys J Plus, 2023
Emsenhuber A, Mordasini C, Burn R.
europepmc   +1 more source

CHEMICAL CONSEQUENCES OF THE C/O RATIO ON HOT JUPITERS: EXAMPLES FROM WASP-12b, COROT-2b, XO-1b, AND HD 189733b. [PDF]

Astrophys J, 2012
Moses JI, Madhusudhan N, Visscher C, Freedman RS.   +3 more
europepmc   +1 more source

CHES: An astrometry mission searching for nearby habitable planets. [PDF]

Innovation (Camb), 2022
Ji J, Wang S, Li H, Fang L, Li D.
europepmc   +1 more source

Stellar clustering shapes the architecture of planetary systems. [PDF]

Nature, 2020
Winter AJ, Kruijssen JMD, Longmore SN, Chevance M.   +3 more
europepmc   +1 more source

Are hot Neptunes partially evaporated hot Jupiters?

, 2011
International audienceThe detection of short period planets (hot Jupiters and their lower mass counterparts, hot Neptunes and super-Earths) still defies the models of planet formation and evolution. Several possibilities have been proposed to explain the
Santos, Nuno C., Boué, Gwenaël, Figueira, P., Correia, Alexandre C. M.   +3 more
core  

Exploring exoplanet dynamics with JWST: Tides, rotation, rings, and moons. [PDF]

Proc Natl Acad Sci U S A
Millholland SC, Winn JN.
europepmc   +1 more source

The rotational and divergent components of atmospheric circulation on tidally locked planets. [PDF]

Proc Natl Acad Sci U S A, 2021
Hammond M, Lewis NT.
europepmc   +1 more source