Results 141 to 150 of about 2,941,415 (239)
EUCLID : Dark Universe Probe and Microlensing planet Hunter
There is a remarkable synergy between requirements for Dark Energy probes by cosmic shear measurements and planet hunting by microlensing. Employing weak and strong gravitational lensing to trace and detect the distribution of matter on cosmic and ...
Batista, V +15 more
core
No Strong Associations between Eccentricity and Orbital Architecture in Kepler Compact Multis
The 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
OrbDot: A Python package for studying the secular evolution of exoplanet orbits
OrbDot 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 +2 more sources
WASP-69b’s Escaping Envelope Is Confined to a Tail Extending at Least 7 Rp
Studying the escaping atmospheres of highly irradiated exoplanets is critical for understanding the physical mechanisms that shape the demographics of close-in planets.
Dakotah Tyler +3 more
doaj +1 more source
The distribution of period ratios for 580 known two-planet systems is apparently nonuniform, with several sharp peaks and troughs. In particular, the vicinity of the 2:1 commensurability seems to have a deficit of systems.
Valeri Makarov +2 more
doaj +1 more source
We report the discovery of a hot Jupiter candidate orbiting HS Psc, a K7 (≈0.7 M _⊙ ) member of the ≈130 Myr AB Doradus moving group. Using radial velocities over 4 yr from the Habitable-zone Planet Finder spectrograph at the Hobby–Eberly Telescope, we ...
Quang H. Tran +8 more
doaj +1 more source
Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b
GJ 486b is a close-in planet orbiting an M dwarf and is therefore expected to have undergone strong atmospheric escape. Motivated by theoretical and observational studies on the constraints of its water and atmosphere, we investigate which combinations ...
Junda Zhou +3 more
doaj +1 more source
The degree of alignment between a star’s spin axis and the orbital plane of its planets (the stellar obliquity) is related to interesting and poorly understood processes that occur during planet formation and evolution.
Nicholas Saunders +55 more
doaj +1 more source
Water Evolution and Inventories of Super-Earths Orbiting Late M Dwarfs
Super-Earths orbiting M dwarf stars may be the most common habitable planets in the Universe. However, their habitability is threatened by intense irradiation from their host stars, which drives the escape of water to space and can lead to surface ...
Keavin Moore +3 more
doaj +1 more source
Magma Ocean Interactions Can Explain JWST Observations of the Sub-Neptune TOI-270 d
Sub-Neptunes with substantial atmospheres may possess magma oceans in contact with the overlying gas, with chemical interactions between the atmosphere and magma playing an important role in shaping atmospheric composition.
Matthew C. Nixon +11 more
doaj +1 more source

