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...
| Main Authors: | , , , , , , , , , |
|---|---|
| 格式: | 文件 |
| 语言: | English |
| 出版: |
IOP Publishing
2025-01-01
|
| 丛编: | The Astrophysical Journal |
| 主题: | |
| 在线阅读: | https://doi.org/10.3847/1538-4357/ada9eb |