A New Spectral Library for Modeling the Surfaces of Hot, Rocky Exoplanets

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...

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Bibliographic Details
Main Authors: Kimberly Paragas, Heather A. Knutson, Renyu Hu, Bethany L. Ehlmann, Giulia Alemanno, Jörn Helbert, Alessandro Maturilli, Michael Zhang, Aishwarya Iyer, George Rossman
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Exoplanet surface composition
Exoplanet surface characteristics
Exoplanet surfaces
Exoplanets
Extrasolar rocky planets
Super Earths
Online Access:https://doi.org/10.3847/1538-4357/ada9eb
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https://doi.org/10.3847/1538-4357/ada9eb

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