Journal article icon

Journal article

Shadow of a Shadow: Ferrocyanide and Nitroprusside as Sunscreens for Photosensitive Prebiotic Molecules

Abstract:
Stellar irradiation is thought to be a significant contributor to the origin of life. Ultraviolet (UV) light interacting with iron cyanide complexes may play an important role in prebiotic chemistry. The UV-Visible (UV-Vis) spectra of these iron cyanide complexes can be measured by the same source that drives the chemistry, providing a real-time in situ quantitative analysis of prebiotically relevant, UV-driven photochemistry. We measure the UV-Vis absorbances of ferrocyanide and nitroprusside, and relate these absorbances to known concentrations. We show that these absorbances can be combined to accurately predict the concentrations of ferrocyanide-nitroprusside mixtures that could be generated from ferrocyanide and nitroxyl salts irradiated by ultraviolet light. The ferrocyanide molar attenuation coefficients were found to be maximal at the following: εferrocyanide(340nm)=(2.2±0.4)×103dm2mol-1. Nitroprusside peaks show the following values: εnitroprusside(340nm)=(4.1±0.3)×102dm2mol-1, εnitroprusside(400nm)=(1.71±0.05)×102dm2mol-1, and εnitroprusside(500nm)=62.1±1.7dm2mol-1. With the help of our measured absorbances, we consider ferrocyanide and nitroprusside to function as sunscreens. In the absence of continuous ferrocyanide sources, UV-sensitive compounds could be protected on timescales of months. This would allow for compounds like nicotinamide adenine dinucleotide, NADH, to survive for over a year at depths of 5 m, compared to a lifetime of 6 months when unprotected. Our toy model constrains the photochemical survival of compounds of interest to the origin of life community across a comprehensive spectral range and can be used to constrain the survival using different exoplanetary irradiative conditions; thus, we are able to explore the UV environment with the presence of ferrocyanide and nitroprusside and contribute to the wider discussion surrounding the prevalence of the origin of life in the Universe.
Publication status:
Published
Peer review status:
Peer reviewed

Actions

Access Document

Files:
Publisher copy:
10.3390/life16050856

Authors

More by this author
Role:
Author
ORCID:
0009-0000-8665-2453
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Physics - Central
Role:
Author
ORCID:
0009-0007-6871-0008
More by this author
Role:
Author
ORCID:
0000-0002-8039-194X
More by this author
Role:
Author
ORCID:
0000-0002-7180-081X


Publisher:
MDPI
Journal:
Life More from this journal
Volume:
16
Issue:
5
Pages:
856
Publication date:
2026-05-21
Acceptance date:
2026-05-11
DOI:
EISSN:
2075-1729
ISSN:
2075-1729
Pmid:
42195411


Language:
English
Keywords:
Source identifiers:
4117387
Deposit date:
2026-06-05
ARK identifier:
This ORA record was generated from metadata provided by an external service. It has not been edited by the ORA Team.

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP