Results 141 to 150 of about 4,598,556 (263)
Binarity of Transit Host Stars - Implications on Planetary Parameters
Straight-forward derivation of planetary parameters can only be achieved in transiting planetary systems. However, planetary attributes such as radius and mass strongly depend on stellar host parameters.
Bakos+37 more
core +2 more sources
It has been suggested that β Pic b has a supersolar metallicity and subsolar C/O ratio. Assuming solar carbon and oxygen abundances for the star β Pic and therefore the planet’s parent protoplanetary disk, β Pic b’s C/O ratio suggests that it formed via ...
Henrique Reggiani+7 more
doaj +1 more source
Investigating Planet Formation and Evolutionary Processes with Short-Period Exoplanets
White Paper submitted to National Academy of Sciences Exoplanet Science Strategy ...
Jackson, B.+3 more
openaire +3 more sources
Imaging Cool Giant Planets in Reflected Light: Science Investigations and Synergy with Habitable Planets [PDF]
Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photometry and spectroscopy of cool extrasolar giant planets.
Arney, Giada+40 more
core +1 more source
The K2 Mission: Characterization and Early results
The K2 mission will make use of the Kepler spacecraft and its assets to expand upon Kepler's groundbreaking discoveries in the fields of exoplanets and astrophysics through new and exciting observations.
Aigrain, Suzanne+18 more
core +1 more source
Are WASP-107-like Systems Consistent with High-eccentricity Migration?
WASP-107 b seems to be a poster child of the long-suspected high-eccentricity migration scenario. It is on a 5.7 day, polar orbit. The planet is Jupiter-like in radius but Neptune-like in mass with exceptionally low density.
Hang Yu, Fei Dai
doaj +1 more source
Formation of stars, substellar objects and exoplanets : Observations of multiplicity
Many nearby stars are part of a binary or multiple system. Details about their history are preserved in their multiplicity characteristics, and observations of binary/multiple star systems provide a way to measure fundamental physical properties of the stars as well as clues to their formation and evolution.
openaire +2 more sources
Cloud formation in exoplanet atmospheres : nucleation of small molecular clusters
It has been inferred that many exoplanets host clouds in their atmospheres. Understanding the processes through which these clouds form, and being able to model them is essential for our understanding of their climate and to explain our observations.
openaire +3 more sources
Directly Imaging Rocky Planets from the Ground [PDF]
Over the past three decades instruments on the ground and in space have discovered thousands of planets outside the solar system. These observations have given rise to an astonishingly detailed picture of the demographics of short-period planets, but are
Artigau, É.+62 more
core +1 more source
Strong Fractionation of Deuterium and Helium in Sub-Neptune Atmospheres along the Radius Valley
We simulate atmospheric fractionation in escaping planetary atmospheres using IsoFATE , a new open-source numerical model. We expand the parameter space studied previously to planets with tenuous atmospheres that exhibit the greatest helium and deuterium
Collin Cherubim+3 more
doaj +1 more source