The Influence of General Relativity on the Spins of Celestial Bodies in Inclined Orbits
Through the Rossiter–McLaughlin effect, several hot Jupiters have been found to exhibit spin–orbit misalignment and even retrograde orbits. The high obliquity observed in these planets can be attributed to two primary formation mechanisms, as summarized in the existing literature. First, the host st...
Saved in:
Main Authors: | Huan-Rong Yuan, Ying Wang, Xin Wu, Ji-Wei Xie, Hui-Gen Liu, Ji-Lin Zhou, Wei Sun |
---|---|
Format: | Article |
Language: | English |
Published: |
IOP Publishing
2025-01-01
|
Series: | The Astrophysical Journal |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4357/ada5fc |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Eight New Candidate Multiplanet Systems among TESS Objects of Interest
by: Mohamed Jassim Munavar Hussain, et al.
Published: (2025-01-01) -
True Mass and Atmospheric Composition of the Nontransiting Hot Jupiter HD 143105 b
by: Luke Finnerty, et al.
Published: (2025-01-01) -
Most High-density Exoplanets Are Unlikely to Be Remnant Giant Planet's Cores
by: Zifan Lin, et al.
Published: (2025-01-01) -
JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum
by: Dana R. Louie, et al.
Published: (2025-01-01) -
The Hottest Neptunes Orbit Metal-rich Stars
by: Shreyas Vissapragada, et al.
Published: (2025-01-01)