Pigmentation as a survival strategy for ancient and modern photosynthetic microbes under high ultraviolet stress on planetary surfaces
By D. Wynn-Williams, H. Edwards, E. M. Newton, J. M. Holder. International Journal of Astrobiology, 2002
112 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology, Ecology, Evolution, Behavior and Systematics
View Paper: https://www.semanticscholar.org/paper/cc3171a8035a0c5e0709f89d3698a7af8c3447b8
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Citations in the corpus
- Viability of the lichen Xanthoria elegans and its symbionts after 18 months of space exposure and simulated Mars conditions on the ISS (2014, background): “The UV and blue light screening abilities of the secondary metabolite parietin have been discussed by several authors, mainly with respect to UV-B irradiation (e.g. Solhaug & Gauslaa 1996; Wynn-Williams et al. 2002; Nybakken et al. 2004).”
- Development of a laser Raman spectrometer for deep-ocean science (2004, background): “It has been reported that Raman spectroscopy can “characterize in situ the molecular components of pigments and other significant organic and inorganic constituents of a microbial community within its lithic habitat” (Wynn-Williams et al., 2002), although achieving this goal on the ocean floor would”
- The potential of the lichen symbiosis to cope with extreme conditions of outer space – I. Influence of UV radiation and space vacuum on the vitality of lichen symbiosis and germination capacity (2002, background): “Both species possess a densely structured upper cortex containing high concentrations of UV-absorbing compounds (Wynn-Williams et al. 2002) with the potential to protect them against the intense UV radiation governing their habitat.”