Results 121 to 130 of about 2,563,330 (219)
, 2014 A unique short-period (P = 0.65356(1) d) Mercury-size Kepler exoplanet candidate KIC012557548b has been discovered recently by Rappaport et al. (2012).
Zhou, Guyin (George) +6 more
core +1 more source
Unexpected Near-Resonant and Metastable States of Young Multiplanet Systems
The Astrophysical JournalRecent observations suggest that the incidence of near-resonant planets declines as planetary systems age, making young planetary systems key signposts of early dynamical evolution.
Zhecheng Hu +6 more
doaj +1 more source
The Astronomical JournalAtmospheric escape’s potential to shape the exoplanet population motivates detailed observations of systems actively undergoing escape. AU Mic is a young and active M dwarf hosting two close-in transiting sub- to Neptune-sized planets. Atmospheric escape
Keighley E. Rockcliffe +10 more
doaj +1 more source
A key piece in the exoplanet puzzle
, 2018 The detection of a low-mass exoplanet on a relatively wide orbit has implications for models of planetary formation and evolution, and could open the door to a new era of exoplanet characterization.Fil: Diaz, Rodrigo Fernando.
Rodrigo F. Díaz, Diaz, Rodrigo Fernando
core +1 more source
Simulation of the Spin Evolution of Some Selected Exoplanets and Inferences on Their Climate
UniverseIn this work, using the simulator VPLanet, we analyze the spin evolution of some selected exoplanets due to the tidal interaction with their host star. For a rocky planet, two spin “conditions” are possible, the “trapped” rotation and the “fast” rotation, referring to the cases of achieved and non-achieved tidal trapping, respectively.
Salvatore Camposeo +4 more
openaire +3 more sources
OrbDot: A Python package for studying the secular evolution of exoplanet orbits
Journal of Open Source SoftwareOrbDot is a Python package for studying the secular (long-term) evolution of exoplanet orbits from observational data. It employs nested sampling algorithms to fit evolutionary models to any combination of transit and eclipse mid-times, radial velocities, and transit durations.
Simone R. Hagey, Aaron C. Boley
openaire +3 more sources
Not All Sub-Neptune Exoplanets Have Magma Oceans
The Astrophysical Journal LettersThe evolution and structure of sub-Neptunes may be strongly influenced by interactions between the outer gaseous envelope of the planet and a surface magma ocean.
Bodie Breza +2 more
doaj +1 more source
dfm/exoplanet: exoplanet v0.1.5
, 2019 <ul> <li>Improves contact point solver using companion matrix to solve quadratic</li> <li>Improves reliability of <code>Angle</code> distribution when the value of the angle is well constrained</li> </ul ...
Dan Foreman-Mackey +2 more
core +1 more source
No Strong Associations between Eccentricity and Orbital Architecture in Kepler Compact Multis
The Astronomical JournalThe dynamical history of a planetary system is recorded in the present day architecture of its constituent planets’ sizes, orbital periods, and eccentricities.
Gregory J. Gilbert +2 more
doaj +1 more source
dfm/exoplanet: exoplanet v0.1.4
, 2019 <ul> <li>Improves the reliability of the PyMC3Sampler</li> <li>Adds a new <code>optimize</code> function since the <code>find_MAP</code> method in PyMC3 is deprecated</li> <li>Adds cronjob ...
Dan Foreman-Mackey +2 more
core +1 more source