Planet Migration in Protoplanetary Disks with Rims
Complex structures, including sharp edges, rings, and gaps, have been commonly observed in protoplanetary disks with or without planetary candidates. Here we consider the possibility that they are the intrinsic consequences of angular momentum transfer ...
Zhuoya Cao +3 more
doaj +1 more source
Introduction-First Billion Years: Habitability. [PDF]
Rivera-Valentín EG +6 more
europepmc +1 more source
Characterizing the atmospheric compositions of exoplanets, along with determining properties such as their mass, mean density, and orbital configuration, are thought to be an effective means for differentiating between various formation and evolution ...
Alan P. Boss
doaj +1 more source
On the implementation of novel RKARMS(4,4) algorithm to study the structures of initial extrasolar giant protoplanets. [PDF]
Chandra Paul G +2 more
europepmc +1 more source
Confirmation of the Low-eccentricity Warm Jupiter HD 278555 b with NEID
The study of warm Jupiters is crucial to understanding the processes that govern giant-planet formation and migration. These planets sit at the boundary between cold giant planets and hot Jupiters, and studying their orbital properties, including period,
James Ball +20 more
doaj +1 more source
Production of diamond using intense heavy ion beams at the FAIR facility and application to planetary physics. [PDF]
Tahir NA +4 more
europepmc +1 more source
A comprehensive investigation of the Galilean moon, Io, by tracing mass and energy flows. [PDF]
Thomas N.
europepmc +1 more source
Identification of carbon dioxide in an exoplanet atmosphere. [PDF]
JWST Transiting Exoplanet Community Early Release Science Team.
europepmc +1 more source
Detection of Four Cold Jupiters through Combined Analyses of Radial Velocity and Astrometry Data
Cold Jupiters play a crucial role in planet formation and dynamical evolution. Since their initial discovery around 47 UMa, they have attracted significant interest; however, their formation mechanisms remain uncertain, underscoring the need to expand ...
Yiyun Wu +21 more
doaj +1 more source
Semianalytical Accretion-tracer Emission: Forming Planets Are Intrinsically Faint
Direct-imaging surveys have looked for accreting planets through their accretion tracers such as H α but have been less fruitful than expected.
Gabriel-Dominique Marleau
doaj +1 more source

