Grain Alignment and Rotational Disruption by Radiative Torques in Exoplanet Atmospheres
Dust clouds are ubiquitous in the atmospheres of hot Jupiters and affect their observable properties. The alignment of dust grains in the clouds and resulting dust polarization provide a promising way to study the magnetic fields of exoplanets. Moreover, the grain size distribution plays an importan...
Main Authors: | Thiem Hoang, Alex Lazarian |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2023-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/acc9a6 |
Similar Items
-
Haze Optical Depth in Exoplanet Atmospheres Varies with Rotation Rate: Implications for Observations
by: Maureen Cohen, et al.
Published: (2024-01-01) -
On the Application of Bayesian Leave-one-out Cross-validation to Exoplanet Atmospheric Analysis
by: Luis Welbanks, et al.
Published: (2023-01-01) -
Patchy Forsterite Clouds in the Atmospheres of Two Highly Variable Exoplanet Analogs
by: Johanna M. Vos, et al.
Published: (2023-01-01) -
High-resolution Transmission Spectroscopy of the Terrestrial Exoplanet GJ 486b
by: Andrew Ridden-Harper, et al.
Published: (2023-01-01) -
Earth as a Transiting Exoplanet: A Validation of Transmission Spectroscopy and Atmospheric Retrieval Methodologies for Terrestrial Exoplanets
by: Jacob Lustig-Yaeger, et al.
Published: (2023-01-01)