Hydrogen Cyanide at the Onset of Prebiotic Chemical Reactivity
Doctoral thesis, 2026

Hydrogen Cyanide (HCN) is a central molecule in prebiotic chemistry, serving as a key precursor for the synthesis of essential building blocks of life. This simple yet highly energetic nitrile is commonly found in the universe, from the interstellar medium and cometary coma, to the atmospheres of several planets and moons. One notable setting is Saturn’s moon Titan, where \HCN is also found in the solid state, forming clouds. However, the very reactivity that makes HCN such an interesting prebiotic molecule also renders its self-reaction chemistry difficult to unravel, as it is prone to yielding intractable polymers. Furthermore, its peculiar solid-state properties remain largely undiscovered, warranting further investigation. In this thesis, I use quantum chemical methods to investigate HCN's complex reactivity and the unique behavior of its solid phase.

The first part of this thesis focuses on HCN reactivity. Exploration of the thermodynamic landscape derived from its self reaction reveal that while most products are thermodynamically favorable, several proposed polymerization pathways are endergonic. Among the most favored products are highly-conjugated polymers and the nucleobase adenine. In a subsequent study, I perform a thorough investigation of proposed base-catalyzed pathways to adenine in a HCN-rich environment, proposing a new pathway and clarifying key missing steps. This work helps explain the kinetic bottlenecks that limit adenine yields in experiments.

In the second part, I study the HCN crystal structure and surface properties in cryogenic environments, with particular focus on Titan. I find that HCN forms needle-shaped crystals, whose tips comprise of high-energy polar surfaces that are predicted to exert strong electric fields. These surfaces might assist chemical transformations at low temperatures, such as the isomerization of HCN to HNC. Furthermore, the electronic structure of HCN polar surfaces shows the emergence of localized metallic surface states. This metallicity is transferred to chemisorbed water molecules, suggesting enhanced reactivity at the interface.

HCN-derived products

Diaminomaleonitrile

Titan

Adenine

Hydrogen Cyanide

Computational Chemistry

Origin of Life

FB salen, Fysik huset
Opponent: Prof. Thanja Lamberts, Leiden University, Leiden, Netherlands

Author

Marco Cappelletti

Chalmers, Chemistry and Chemical Engineering, Chemistry and Biochemistry

A Thermodynamic Landscape of Hydrogen Cyanide-Derived Molecules and Polymers

ACS Earth and Space Chemistry,;Vol. 8(2024)p. 1272-1280

Journal article

Cappelletti, M., Rahm, M., How Does Adenine Form from Hydrogen Cyanide?

Electric Fields Can Assist Prebiotic Reactivity on Hydrogen Cyanide Surfaces

ACS CENTRAL SCIENCE,;Vol. In Press(2026)

Journal article

Cappelletti, M., Rahm, M., Hydrogen Cyanide Surfaces Can Turn Water Metallic

How did life emerge from non-living matter? This is the central puzzle of prebiotic chemistry, the study of the chemistry that led to life. At the heart of this mystery lies Hydrogen Cyanide (HCN), a molecule that is paradoxically a deadly poison to modern life, yet a central precursor to its origins. Uncovering its role in the origin of life is, however, difficult: not only is HCN highly toxic, but it also creates an unmanageable black "tar" that challenges experimental analysis. Thankfully, modern computer simulations allow us to bypass these problems. In this thesis, I use these computational tools to safely explore the reactions at the onset of prebiotic chemistry. I reveal how HCN can successfully form adenine, an essential letter in our genetic alphabet. Furthermore, I show that in cold environments HCN crystallizes into needle-shaped structures that generate intense electric fields capable of catalyzing chemical reactions. These findings are particularly relevant for cold worlds like Saturn’s moon Titan, suggesting that prebiotic chemistry can also take place in cold, alien environments.

Predicting Prebiotic Origins of Polypeptides and Solid-State Chemistry on Titan

Swedish Research Council (VR) (2024-05049), 2025-01-01 -- 2028-12-31.

Computational Astrobiology: The Rise of Macromolecules

Swedish Research Council (VR) (2020-04305), 2021-01-01 -- 2024-12-31.

Subject Categories (SSIF 2025)

Theoretical Chemistry

Physical Chemistry

DOI

10.63959/chalmers.dt/5822

ISBN

978-91-8103-365-6

Doktorsavhandlingar vid Chalmers tekniska högskola. Ny serie: 5822

Publisher

Chalmers

FB salen, Fysik huset

Opponent: Prof. Thanja Lamberts, Leiden University, Leiden, Netherlands

More information

Latest update

1/23/2026