A New Spectral Library for Modeling the Surfaces of Hot, Rocky Exoplanets
JWST’s MIRI LRS provides the first opportunity to spectroscopically characterize the surface compositions of close-in terrestrial exoplanets. Models for the bare-rock spectra of these planets often utilize a spectral library from R. Hu et al., which is based on room-temperature reflectance measureme...
| Autores principales: | , , , , , , , , , |
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| Formato: | Artículo |
| Lenguaje: | English |
| Publicado: |
IOP Publishing
2025-01-01
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| Colección: | The Astrophysical Journal |
| Materias: | |
| Acceso en línea: | https://doi.org/10.3847/1538-4357/ada9eb |