Skip to main content
Go to the home page of the European Commission (opens in new window)
English en
CORDIS - EU research results
CORDIS

Interstellar Chemical Evolution: Probing HCN and HNC Formation and Destruction on Icy Surfaces with Computational Chemistry

Project description

Exploring the chemistry of star-forming ices

Dense gas regions in galaxies, where stars and planets form, are rich in molecules that hold clues about cosmic chemistry. Two such molecules, hydrogen cyanide and hydrogen isocyanide, are key tracers of temperature and gas density. They are also vital precursors to prebiotic compounds like amino acids and nucleotides. While their formation in the gas phase is well understood, how they form and break apart on icy surfaces in space remains unknown. With the support of the Marie Skłodowska-Curie Actions programme, the ICE-CN project will study the interaction of CN radicals with water and CO ices. Using advanced computational tools and astrochemical models, the project investigates these processes, shedding light on the role of surface chemistry in star-forming regions.

Objective

HCN and HNC are routinely used by astronomers to trace temperature and dense gas regions in galaxies, where stars and planetary systems form. They are key precursors of complex species, including prebiotic molecules like amino acids and nucleotides. While their gas-phase formation and evolution are well understood, their formation and destruction paths on interstellar ices remains largely unchartered territory.

The aim of this proposal is to remedy this knowledge gap by investigating the formation of HCN and HNC through CN radical hydrogenation on interstellar water and CO ices, as well as their destruction paths using state-of-the-art computational chemistry and astrochemical modelling. Including, in all cases, their deuterated counterparts. It also presents an opportunity to study the interaction of CN radicals with ice surfaces, which can occur either through physisorption or hemibonding on both types of ices. The four primary objectives of this proposal are: (i) to explore the CN to water and CO ice binding energy distribution as well as the dominant binding modes, (ii) to quantify the hydrogenation reactions of CN with atomic and molecular hydrogen forming HCN and HNC, as well as other possible hydrogenation products due to the hemibonding interactions, (iii) to investigate the destruction of the products in the previous point resulting from further hydrogenation reactions, and finally, (iv) to calculate the rate constants, including quantum tunnelling, and implement these in the UCLCHEM astrochemical model to assess the importance of surface chemistry in two specific cases: the shocked region L1157-B1 and the NGC1068 galaxy.

The novelty of this proposal lies in the combination of computational chemistry and astrochemical modelling to unveil the ice-surface formation and evolution of HCN and HNC and their deuterated counterparts for the first time, encompassing a comprehensive characterization of the CN to water and CO hemibonding interaction.

Fields of science (EuroSciVoc)

Keywords

Programme(s)

Topic(s)

Funding Scheme

HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

See all projects funded under this funding scheme

Call for proposal

(opens in new window) HORIZON-MSCA-2023-PF-01

See all projects funded under this call

Coordinator

UNIVERSITEIT LEIDEN
Net EU contribution
€ 187 624,32
Address
RAPENBURG 70
2311 EZ Leiden
Netherlands
Activity type
Higher or Secondary Education Establishments
Links
Total cost
No data