Results 111 to 120 of about 45,387 (213)

TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence

open access: yesThe Astronomical Journal
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

Insight into the Formation of β Pic b through the Composition of Its Parent Protoplanetary Disk as Revealed by the β Pic Moving Group Member HD 181327

open access: yesThe Astronomical Journal
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

Separating Super-puffs versus Hot Jupiters among Young Puffy Planets

open access: yesThe Astrophysical Journal
Discoveries of close-in young puffy ( R _p ≳ 6 R _⊕ ) planets raise the question of whether they are bona fide hot Jupiters or puffed-up Neptunes, potentially placing constraints on the formation location and timescale of hot Jupiters.
Amalia Karalis   +2 more
doaj   +1 more source

Early Release Science of the exoplanet WASP-39b with JWST NIRCam. [PDF]

open access: yesNature, 2023
Ahrer EM   +98 more
europepmc   +1 more source

Fully fluorinated non-carbon compounds NF3 and SF6 as ideal technosignature gases. [PDF]

open access: yesSci Rep, 2023
Seager S   +5 more
europepmc   +1 more source

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H. [PDF]

open access: yesNature, 2023
Alderson L   +91 more
europepmc   +1 more source

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