Results 41 to 50 of about 226 (101)

Free-floating Planets, Survivor Planets, Captured Planets, and Binary Planets from Stellar Flybys

open access: yesThe Astrophysical Journal
In star clusters, close stellar encounters can strongly impact the architecture of a planetary system or even destroy it. We present a systematic study of the effects of stellar flybys on two-planet systems.
Fangyuan Yu, Dong Lai
doaj   +1 more source

Large planets may not form fractionally large moons. [PDF]

open access: yesNat Commun, 2022
Nakajima M, Genda H, Asphaug E, Ida S.
europepmc   +1 more source

Probing the Outskirts of M Dwarf Planetary Systems with a Cycle 1 JWST NIRCam Coronagraphy Survey

open access: yesThe Astronomical Journal
The population of giant planets on wide orbits around low-mass M dwarf stars is poorly understood, but the unprecedented sensitivity of JWST NIRCam coronagraphic imaging now provides direct access to planets significantly less massive than Jupiter beyond
Ellis Bogat   +20 more
doaj   +1 more source

Revising the Giant Planet Mass–Metallicity Relation: Deciphering the Formation Sequence of Giant Planets

open access: yesThe Astrophysical Journal
The rate at which giant planets accumulate solids and gas is a critical component of planet formation models, yet it is extremely challenging to predict from first principles.
Yayaati Chachan   +4 more
doaj   +1 more source

Planet population synthesis: the role of stellar encounters. [PDF]

open access: yesMon Not R Astron Soc, 2022
Ndugu N, Abedigamba OP, Andama G.
europepmc   +1 more source

The Nature and Origins of Sub-Neptune Size Planets. [PDF]

open access: yesJ Geophys Res Planets, 2021
Bean JL, Raymond SN, Owen JE.
europepmc   +1 more source

JWST-TST High Contrast: Living on the Wedge, or, NIRCam Bar Coronagraphy Reveals CO2 in the HR 8799 and 51 Eri Exoplanets’ Atmospheres

open access: yesThe Astronomical Journal
High-contrast observations with JWST can reveal key composition and vertical mixing dependent absorption features in the spectra of directly imaged planets across the 3–5 μ m wavelength range.
William O. Balmer   +21 more
doaj   +1 more source

Exploring the link between star and planet formation with Ariel. [PDF]

open access: yesExp Astron (Dordr), 2022
Turrini D   +24 more
europepmc   +1 more source

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