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Updated: Jul 17, 2026

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Chemical processing in the coma as the source of cometary HNC
W M Irvine1, E A Bergin, J E Dickens
1Five College Radio Astronomy Observatory, University of Massachusetts, Amherst 01003, USA. irvine@fcrao1.phast.umass.edu
Hydrogen isocyanide (HNC) in comets likely forms via chemical reactions in the coma, not from preserved interstellar material. This finding impacts how we interpret cometary composition and early Solar System conditions.
Area of Science:
- Astrochemistry
- Cometary Science
- Planetary Science
Background:
- Discovery of hydrogen isocyanide (HNC) in comet Hyakutake, with abundance similar to interstellar clouds, suggested it might be surviving interstellar material.
- Preserved interstellar material in comets could constrain early Solar System processes.
- Alternatively, HNC could be photochemically produced in the coma, limiting its use as a direct indicator of early Solar System conditions.
Purpose of the Study:
- To investigate the origin of HNC in comets.
- To determine if HNC represents preserved interstellar material or is produced in the cometary coma.
- To assess the implications for understanding early Solar System composition.
Main Methods:
- Analysis of the HNC/HCN ratio in comet Hale-Bopp.
- Comparison of observed HNC/HCN ratios with predictions from chemical models.
- Distinguishing between cometary nucleus origin versus in-situ coma production.
Main Results:
- The HNC/HCN ratio in comet Hale-Bopp showed a variation with heliocentric distance.
- This observed variation aligns with models of gas-phase chemical production of HNC within the coma.
- The data does not support HNC originating directly from the comet's nucleus.
Conclusions:
- HNC is primarily formed through chemical reactions occurring within the cometary coma.
- Photochemical processes in the coma are the dominant source of observed HNC.
- Cometary HNC abundance should not be directly interpreted as preserved interstellar material; cometary chemistry must be considered.
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