4.1 Article

Degradation of microbial fluorescence biosignatures by solar ultraviolet radiation on Mars

Journal

INTERNATIONAL JOURNAL OF ASTROBIOLOGY
Volume 13, Issue 2, Pages 112-123

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/S1473550413000335

Keywords

life detection; extremophile; ultraviolet radiation; spectroscopy; fluorescence; Mars; biosignatures

Funding

  1. UCL Institute of Origins
  2. Science and Technology Facilities Council (STFC)
  3. Science and Technology Facilities Council [PP/E007740/1, ST/I001964/1] Funding Source: researchfish
  4. STFC [ST/I001964/1] Funding Source: UKRI

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Recent and proposed robotic missions to Mars are equipped with implements to expose or excavate fresh material from beneath the immediate surface. Once brought into the open, any organic molecules or potential biosignatures of present or past life will be exposed to the unfiltered solar ultraviolet (UV) radiation and face photolytic degradation over short time courses. The key question, then, is what is the window of opportunity for detection of recently exposed samples during robotic operations? Detection of autofluorescence has been proposed as a simple method for surveying or triaging samples for organic molecules. Using a Mars simulation chamber we conduct UV exposures on thin frozen layers of two model microorganisms, the radiation-resistant polyextremophile Deinococcus radiodurans and the cyanobacterium Synechocystis sp. PCC 6803. Excitation-emission matrices (EEMs) are generated of the full fluorescence response to quantify the change in signal of different cellular fluorophores over Martian equivalent time. Fluorescence of Deinococcus cells, protected by a high concentration of carotenoid pigments, was found to be relatively stable over 32h of Martian UV irradiation, with around 90% of the initial signal remaining. By comparison, fluorescence from protein-bound tryptophan in Synechocystis is much more sensitive to UV photodegradation, declining to 50% after 64h exposure. The signal most readily degraded by UV irradiation is fluorescence of the photosynthetic pigments - diminished to only 35% after 64h. This sensitivity may be expected as the biological function of chlorophyll and phycocyanin is to optimize the harvesting of light energy and so they are readily photobleached. A significant increase in a similar to 450nm emission feature is interpreted as accumulation of fluorescent cellular degradation products from photolysis. Accounting for diurnal variation in Martian sunlight, this study calculates that frozen cellular biosignatures would remain detectable by fluorescence for at least several sols; offering a sufficient window for robotic exploration operations.

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