Inner Habitable Zone Boundary for Eccentric Exoplanets
The climate of a planet can be strongly affected by its eccentricity due to variations in the stellar flux. There are two limits for the dependence of the inner habitable zone boundary (IHZ) on eccentricity: (1) the mean stellar flux approximation ( ${S}_{{\rm{IHZ}}}\propto \sqrt{1-{e}^{2}}$ ), in w...
Main Authors: | Xuan Ji, Nora Bailey, Daniel Fabrycky, Edwin S. Kite, Jonathan H. Jiang, Dorian S. Abbot |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal Letters |
Subjects: | |
Online Access: | https://doi.org/10.3847/2041-8213/acaf62 |
Similar Items
-
A Catalog of Habitable Zone Exoplanets
by: Michelle L. Hill, et al.
Published: (2023-01-01) -
Implications of Atmospheric Nondetections for Trappist-1 Inner Planets on Atmospheric Retention Prospects for Outer Planets
by: Joshua Krissansen-Totton
Published: (2023-01-01) -
Prospects for the characterization of habitable planets
by: Mazevet, Stephane, et al.
Published: (2023-08-01) -
The Abundance of Belatedly Habitable Planets and Ambiguities in Definitions of the Continuously Habitable Zone
by: Noah W. Tuchow, et al.
Published: (2023-01-01) -
Eccentricity Distribution beyond the Snow Line and Implications for Planetary Habitability
by: Stephen R. Kane, et al.
Published: (2024-01-01)