A Systematic Study on the Absorption Features of Interstellar Ices in Presence of Impurities

TL;DR

This study investigates how impurities like CO, CO2, CH3OH, H2CO, HCOOH, and NH3 affect the vibrational absorption features of water ice, combining theoretical calculations with infrared spectroscopy experiments to improve interpretation of interstellar ice observations.

Contribution

It provides a comprehensive analysis of impurity effects on water ice vibrational modes, supported by both computational and experimental data, aiding future space observations.

Findings

Impurities significantly alter water ice vibrational band strengths and profiles.

Bulk stretching mode is most affected by impurities, bending least affected.

HCOOH and NH3 notably influence specific vibrational modes, with NH3 causing the disappearance of free-OH band at high concentrations.

Abstract

Spectroscopic studies play a key role in the identification and analysis of interstellar ices and their structure. Some molecules have been identified within the interstellar ices either as pure, mixed, or even as layered structures. Absorption band features of water ice can significantly change with the presence of different types of impurities (CO, CO2, CH3OH, H2CO, etc.). In this work, we carried out a theoretical investigation to understand the behavior of water band frequency, and strength in the presence of impurities. The computational study has been supported and complemented by some infrared spectroscopy experiments aimed at verifying the effect of HCOOH, NH3 , and CH3 OH on the band profiles of pure H2O ice. Specifically, we explored the effect on the band strength of libration, bending, bulk stretching, and free-OH stretching modes. Computed band strength profiles have been compared with our new and existing experimental results, thus pointing out that vibrational modes of H2O and their intensities can change considerably in the presence of impurities at different concentrations. In most cases, the bulk stretching mode is the most affected vibration, while the bending is the least affected mode. HCOOH was found to have a strong influence on the libration, bending, and bulk stretching band profiles. In the case of NH3, the free-OH stretching band disappears when the impurity concentration becomes 50%. This work will ultimately aid a correct interpretation of future detailed spaceborne observations of interstellar ices by means of the upcoming JWST mission.