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

Gorai, Prasanta; Sil, Milan; Das, Ankan; Sivaraman, Bhalamurugan; Chakrabarti, Sandip K.; Ioppolo, Sergio; Puzzarini, Cristina; Kanuchova, Zuzana; Dawes, Anita; Mendolicchio, Marco; Mancini, Giordano; Barone, Vicenzo; Nakatani, Naoki; Shimonishi, Takashi and Mason, Nigel (2020). Systematic Study on the Absorption Features of Interstellar Ices in the Presence of Impurities. ACS Earth and Space Chemistry, 4(6) pp. 920–946.

DOI: https://doi.org/10.1021/acsearthspacechem.0c00098

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 the 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 CH₃OH 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.

Viewing alternatives

Metrics

Item Actions

Export

You can export this page using these formats Digital Object Identifier - DOI

About

• Item ORO ID
• 70918
• Item Type
• Journal Item
• ISSN
• 2472-3452
• Project Funding Details

• Funded Project Name	Project ID	Funding Body
  Not Set	ISRO/RES/2/402/16-17	ISRO
  Not Set	Not Set	Royal Society
  COST Action TD1308 − ORIGINS	Not Set	Not Set

• Keywords
• astrochemistry; spectra; ISM: molecules; methods: numerical; experimental; infrared: band strength; interstellar ice
• Academic Unit or School
• Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
  Faculty of Science, Technology, Engineering and Mathematics (STEM)
• Research Group
• Astronomy
  Physics
• Copyright Holders
• © 2020 American Chemical Society
• Related URLs
• • https://arxiv.org/abs/2005.12867
• SWORD Depositor
• Jisc Publications-Router
• Depositing User
• Jisc Publications-Router