Detecting Planetary Oblateness in the Era of JWST: A Case Study of Kepler-167e
Planets may be rotationally flattened, and their oblateness thus provides useful information on their formation and evolution. Here, we develop a new algorithm that can compute the transit light curve due to an oblate planet very efficiently and use it to study the detectability of planet oblateness...
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| Principais autores: | , , , , , , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2025-01-01
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| coleção: | The Astronomical Journal |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/1538-3881/ad9b8c |
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