Results 111 to 120 of about 828 (196)
Breaking Giant Chains: Early-stage Instabilities in Long-period Giant Planet Systems
Orbital evolution is a critical process that sculpts planetary systems, particularly during their early stages where planet–disk interactions are expected to lead to the formation of resonant chains.
Vighnesh Nagpal +2 more
doaj +1 more source
The GAPS programme at TNG. LXI. Atmospheric parameters and elemental abundances of TESS young exoplanet host stars [PDF]
The study of exoplanets at different evolutionary stages can shed light on their formation, migration, and evolution. The determination of exoplanet properties depends on the properties of their host stars.
R. Cosentino +75 more
core +1 more source
The observed census of resonant extrasolar planets spans a tantalizing display of orbital architectures, ranging from familiar 2:1 and 3:2 mean-motion commensurabilities to nearly coorbital configurations characterized by period ratios close to unity ...
Konstantin Batygin +1 more
doaj +1 more source
86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Unified Formation Channel of Hot and Warm Jupiters via Planet–Planet Scattering
Recent observations show distinct orbital architectures for hot and warm Jupiters: hot Jupiters span a wide range of stellar obliquities and tend to host distant companions without close-by companions, whereas warm Jupiters are often aligned and ...
Julia Esposito, Gongjie Li, Songhu Wang
doaj +1 more source
The evolution of hot Jupiters revealed by the age distribution of their host stars. [PDF]
Chen DC +13 more
europepmc +1 more source
TOI-2494 c and TOI-5143 c: A Hot Saturn and a Hot Jupiter with Interior Planetary Companions
We present the TESS-based discoveries of planetary systems orbiting the late G dwarfs TOI-2494 and TOI-5143, each of which harbors a hot giant planet and a smaller interior planet. TOI-2494 hosts a transiting mini-Neptune ( P = 2.41 days, $\,{R}_{{\rm{P}}
Samuel N. Quinn +71 more
doaj +1 more source
Study of Exoplanet Migration Mechanisms with the Direct Imaging Method
学位の種別:課程博士 審査委員会委員 : (主査)東京大学教授 小久保 英一郎, 東京大学准教授 宮田 隆志, 東京大学准教授 片坐 宏一, 東京大学准教授 生駒 大洋, 大阪大学教授 芝井 ...
openaire
The influence of hypothetical exomoons on planetary thermal phase curves
Context. More than 200 moons exist in our Solar System, yet no exomoon has been confirmed to date. While the innermost two planets of the Solar System lack natural satellites and most studies favour the existence of exomoons around long-period planets ...
Song Xinyi, Yang Jun, Ouyang Yueyun
doaj +1 more source

