Warm giant exoplanet characterisation: current state, challenges and outlook
The characterisation of giant exoplanets is crucial to constrain giant planet formation and evolution theory and for putting the solar-system’s giant planets in perspective. Typically, mass-radius (M-R) measurements of moderately irradiated warm Jupiters are used to estimate the planetary bulk compo...
Main Authors: | Simon Müller, Ravit Helled |
---|---|
Format: | Article |
Language: | English |
Published: |
Frontiers Media S.A.
2023-05-01
|
Series: | Frontiers in Astronomy and Space Sciences |
Subjects: | |
Online Access: | https://www.frontiersin.org/articles/10.3389/fspas.2023.1179000/full |
Similar Items
-
Interior and Evolution of the Giant Planets
by: Yamila Miguel, et al.
Published: (2023-01-01) -
TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars
by: Samuel K. Grunblatt, et al.
Published: (2023-01-01) -
Age Distribution of Exoplanet Host Stars: Chemical and Kinematic Age Proxies from GAIA DR3
by: C. Swastik, et al.
Published: (2023-01-01) -
Small Planets around Cool Dwarfs: Enhanced Formation Efficiency of Super-Earths around M Dwarfs
by: Yayaati Chachan, et al.
Published: (2023-01-01) -
TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey
by: Judah Van Zandt, et al.
Published: (2023-01-01)