Photostability of gas- and solid-phase biomolecules within dense molecular clouds due to soft X-rays
S. Pilling (UNIVAP), D. P. P. Andrade (UNIVAP), E. M. do Nascimento, (UFBA), R. R. T. Marinho (UFBA), H. M. Boechat-Roberty (UFRJ), L. H. de, Coutinho (UFRJ), G. G. B. de Souza (UFRJ), R. B. de Castilho (UFRJ), R. L., Cavasso-Filho (UFABC), A. F. Lago (UFABC)

TL;DR
This study investigates the stability of key biomolecules like amino acids and nucleobases under soft X-ray irradiation in space-like environments, revealing nucleobases are significantly more resistant than amino acids, with implications for astrobiology.
Contribution
The paper provides experimental data on the photostability of biomolecules in gas and solid phases under soft X-ray conditions relevant to space environments, highlighting differences in their resistance.
Findings
Solid-phase amino acids have half-lives of at least 3E5 to 3E8 years in molecular clouds and disks.
Gas-phase amino acids have longer half-lives than solid-phase, by about an order of magnitude.
Nucleobases are 2-3 orders of magnitude more resistant to radiation than amino acids.
Abstract
An experimental photochemistry study involving gas- and solid-phase amino acids (glycine, DL-valine, DL-proline) and nucleobases (adenine and uracil) under soft X-rays was performed. The aim was to test the molecular stabilities of essential biomolecules against ionizing photon fields inside dense molecular clouds and protostellar disks analogs. In these environments, the main energy sources are the cosmic rays and soft X-rays. The measurements were taken at the Brazilian Synchrotron Light Laboratory (LNLS), employing 150 eV photons. In-situ sample analysis was performed by Time-of-flight mass spectrometer (TOF-MS) and Fourier transform infrared (FTIR) spectrometer, for gas- and solid- phase analysis, respectively. The half-life of solid phase amino acids, assumed to be present at grain mantles, is at least 3E5 years and 3E8 years inside dense molecular clouds and protoplanetary disks,…
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