Results 91 to 100 of about 269 (181)

Transiting Jupiters around M Dwarfs Have Similar Masses to FGK Warm Jupiters

open access: yesThe Astrophysical Journal
This paper presents a comparative analysis of the bulk properties (mass and radius) of transiting giant planets (≳8 R _⊕ ) orbiting FGKM stars. Our findings suggest that the average mass of M-dwarf Jupiters is lower than that of their solar-type ...
Shubham Kanodia
doaj   +1 more source

Formation of Giant Planets by Gas Disk Gravitational Instability on Wide Orbits around Protostars with Varied Masses. II. Quadrupled Spatial Resolution and Beta Cooling

open access: yesThe Astrophysical Journal
Exoplanet demographics are sufficiently advanced to provide important constraints on theories of planet formation. While core and pebble accretion are preferred for rocky and icy planets, there appears to be a need for gas disk gravitational instability (
Alan P. Boss
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

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

Searching for GEMS: TOI-5688 A b, a Low-density Giant Orbiting a High-metallicity Early M-dwarf

open access: yesThe Astronomical Journal
We present the discovery of a low-density planet orbiting the high-metallicity early M-dwarf TOI-5688 A b. This planet was characterized as part of the search for transiting giant planets ( R  ≳ 8 R _⊕ ) through the Searching for Giant Exoplanets around ...
Varghese Reji   +33 more
doaj   +1 more source

Searching for GEMS: Characterizing Six Giant Planets Around Cool Dwarfs

open access: yesThe Astronomical Journal
Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an increasingly large number of them to enable statistical surveys like the Searching ...
Shubham Kanodia   +44 more
doaj   +1 more source

Jupiter Science Enabled by ESA's Jupiter Icy Moons Explorer. [PDF]

open access: yesSpace Sci Rev, 2023
Fletcher LN   +49 more
europepmc   +1 more source

Characterisation of hot Jupiter atmospheres with phase-resolved emission spectra

open access: yes
Hot Jupiters are gaseous giant planets with orbital periods of less than ten days. They are currently the only class of exoplanets that can be characterised with high-quality spectroscopic observations over multiple orbital phases owing to their large ...
Yang, Jingxuan
core   +1 more source

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