Results 91 to 100 of about 269 (181)
Transiting Jupiters around M Dwarfs Have Similar Masses to FGK Warm Jupiters
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
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]
Nakajima M, Genda H, Asphaug E, Ida S.
europepmc +1 more source
Exploring the link between star and planet formation with Ariel. [PDF]
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
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
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Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds. [PDF]
Mansfield M.
europepmc +1 more source
Igneous processes in the small bodies of the Solar System I. Asteroids and comets. [PDF]
Leone G, Tanaka HKM.
europepmc +1 more source
Searching for GEMS: Characterizing Six Giant Planets Around Cool Dwarfs
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]
Fletcher LN +49 more
europepmc +1 more source
Characterisation of hot Jupiter atmospheres with phase-resolved emission spectra
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

