scholarly journals Implications of a 3.472–3.333 Gyr-old subaerial microbial mat from the Barberton greenstone belt, South Africa for the UV environmental conditions on the early Earth

2006 ◽  
Vol 361 (1474) ◽  
pp. 1857-1876 ◽  
Author(s):  
Frances Westall ◽  
Cornel E.J de Ronde ◽  
Gordon Southam ◽  
Nathalie Grassineau ◽  
Maggy Colas ◽  
...  

Modelling suggests that the UV radiation environment of the early Earth, with DNA weighted irradiances of about three orders of magnitude greater than those at present, was hostile to life forms at the surface, unless they lived in specific protected habitats. However, we present empirical evidence that challenges this commonly held view. We describe a well-developed microbial mat that formed on the surface of volcanic littoral sediments in an evaporitic environment in a 3.5–3.3 Ga-old formation from the Barberton greenstone belt. Using a multiscale, multidisciplinary approach designed to strongly test the biogenicity of potential microbial structures, we show that the mat was constructed under flowing water by 0.25 μm filaments that produced copious quantities of extracellular polymeric substances, representing probably anoxygenic photosynthesizers. Associated with the mat is a small colony of rods–vibroids that probably represent sulphur-reducing bacteria. An embedded suite of evaporite minerals and desiccation cracks in the surface of the mat demonstrates that it was periodically exposed to the air in an evaporitic environment. We conclude that DNA-damaging UV radiation fluxes at the surface of the Earth at this period must either have been low (absorbed by CO 2 , H 2 O, a thin organic haze from photo-dissociated CH 4 , or SO 2 from volcanic outgassing; scattered by volcanic, and periodically, meteorite dust, as well as by the upper layers of the microbial mat) and/or that the micro-organisms exhibited efficient gene repair/survival strategies.

Author(s):  
Charles S Cockell ◽  
John A Raven

The trace gas ozone, produced in the present-day stratosphere, acts as a screen for UV radiation between 195 and approximately 290 nm, depending on its column abundance. On the anoxic Archaean Earth, such an ozone screen would not have existed. Although the presence of other screens, such as an organic haze, might have ameliorated the UV radiation flux, even assuming the worst-case scenario (no UV screen), it can be shown that early land masses and the photic zone of the oceans could have been colonized, suggesting that: (i) high UV radiation would not have prevented the colonization of land and (ii) it is unlikely that the fossil record can be used to constrain estimates of the UV radiation environment of the early Earth (although geochemical approaches and the study of extrasolar planetary atmospheres are likely to provide empirical constraints on the early photobiological environment).


2021 ◽  
Vol 567 ◽  
pp. 116999
Author(s):  
Roger R. Fu ◽  
Nadja Drabon ◽  
Michael Wiedenbeck ◽  
Alec R. Brenner ◽  
Donald R. Lowe ◽  
...  

2015 ◽  
Vol 267 ◽  
pp. 311-322 ◽  
Author(s):  
Alice Montinaro ◽  
Harald Strauss ◽  
Paul R.D. Mason ◽  
Desiree Roerdink ◽  
Carsten Münker ◽  
...  

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