Results 151 to 160 of about 2,143 (179)

Formation, habitability, and detection of extrasolar moons. [PDF]

Astrobiology, 2014
Heller R, Williams D, Kipping D, Limbach MA, Turner E, Greenberg R, Sasaki T, Bolmont E, Grasset O, Lewis K, Barnes R, Zuluaga JI.   +11 more
europepmc   +1 more source

Extended main sequences in star clusters. [PDF]

Fundam Res
Li C, Milone AP, Sun W, de Grijs R.
europepmc   +1 more source

Habitable planets around white and brown dwarfs: the perils of a cooling primary. [PDF]

Astrobiology, 2013
Barnes R, Heller R.
europepmc   +1 more source

COMPOSITIONAL DIVERSITY IN THE ATMOSPHERES OF HOT NEPTUNES, WITH APPLICATION TO GJ 436b. [PDF]

Astrophys J, 2013
Moses JI, Line MR, Visscher C, Richardson MR, Nettelmann N, Fortney JJ, Barman TS, Stevenson KB, Madhusudhan N.   +8 more
europepmc   +1 more source

Could CoRoT-7b and Kepler-10b be remnants of evaporated gas or ice giants?

Planet Space Sci, 2011
Leitzinger M, Odert P, Kulikov YN, Kulikov YN, Lammer H, Wuchterl G, Penz T, Guarcello MG, Micela G, Khodachenko ML, Weingrill J, Hanslmeier A, Biernat HK, Schneider J.   +13 more
europepmc   +1 more source

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Atmospheric Thermal Tides of Exoplanets

Gravitational interactions between a planet and its host star may have important effects on the orbit and rotation rates of the two bodies. Gravitational tides, through tidal friction, change the rotation period of a planet, ultimately synchronizing it with its orbital period and tidally locking it when the orbit is nearly circular. While the theory of
openaire   +1 more source

Effects of tides on the infrared light curve of rocky exoplanets

2011
Short-period exoplanets undergo strong tidal interactions that affect their orbital and spin evolution and their internal structure via tidal heating. Tidal models are, however, limited by uncertainties on key processes such as the dissipation rate. We show here that infrared photometric monitoring of eccentric rocky exoplanets can be used to determine
Maurin, A. S., Selsis, Franck, Hersant, F., Raymond, Sean N., Leconte, J., Delbo, M.   +5 more
openaire   +1 more source

Studying network of symmetric periodic orbit families of the Hill problem via symplectic invariants, Extension of the creep tide theory to exoplanet systems with high stellar obliquity

Studying network of symmetric periodic orbit families of the Hill problem via symplectic invariants In the framework of the spatial circular Hill three-body problem we illustrate the application of symplectic invariants to analyze the network structure of symmetric periodic orbits families.
openaire   +1 more source

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H

Nature, 2023
Lili Alderson, Hannah R Wakeford, Munazza K Alam   +2 more
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