Potassium Bromide Glass: Simulating Exoplanet Settings for Infrared Spectroscopy

Abstract Potassium bromide (KBr) glasses are widely used in infrared spectroscopy for their optical transparency and ability to produce high-fidelity molecular spectra. They are used in astronomical studies to characterize molecular vibrations; however, their use in simulating exoplanetary conditions in laboratory settings remains underexplored. This Research Note emphasizes KBr glasses as a practical tool to study refractory molecules including polycyclic aromatic hydrocarbons under controlled chemical, pressure, and temperature conditions. These simulations can yield high-resolution reference spectra relevant to exoplanetary environments, supporting the interpretation of IR data from space telescopes such as the James Webb Space Telescope, and bridging laboratory spectroscopy to astrophysical observation.

Authors

Publication Details

Journal
Research Notes of the AAS
Published
2025-05-14
DOI
https://doi.org/10.3847/2515-5172/add72c
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00
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article

Potassium Bromide Glass: Simulating Exoplanet Settings for Infrared Spectroscopy

Paul Shapshak, Jean Schneider
Research Notes of the AAS
Stellar, planetary, and galactic studies
article

Potassium Bromide Glass: Simulating Exoplanet Settings for Infrared Spectroscopy

Paul Shapshak, Jean Schneider
article en

Abstract

Abstract Potassium bromide (KBr) glasses are widely used in infrared spectroscopy for their optical transparency and ability to produce high-fidelity molecular spectra. They are used in astronomical studies to characterize molecular vibrations; however, their use in simulating exoplanetary conditions in laboratory settings remains underexplored. This Research Note emphasizes KBr glasses as a practical tool to study refractory molecules including polycyclic aromatic hydrocarbons under controlled chemical, pressure, and temperature conditions. These simulations can yield high-resolution reference spectra relevant to exoplanetary environments, supporting the interpretation of IR data from space telescopes such as the James Webb Space Telescope, and bridging laboratory spectroscopy to astrophysical observation.

Research Notes of the AASVol. 9(5)
Openalex Percentile: Top 93%
Stellar, planetary, and galactic studies
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