School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife, UK.
Astrobiology. 2012 Feb;12(2):115-24. doi: 10.1089/ast.2011.0678. Epub 2012 Jan 27.
The potential for Earth-like planets within binary/multiple-star systems to host photosynthetic life was evaluated by modeling the levels of photosynthetically active radiation (PAR) such planets receive. Combinations of M and G stars in (i) close-binary systems; (ii) wide-binary systems, and (iii) three-star systems were investigated, and a range of stable radiation environments were found to be possible. These environmental conditions allow for the possibility of familiar, but also more exotic, forms of photosynthetic life, such as IR photosynthesizers and organisms that are specialized for specific spectral niches.
通过模拟类地行星接收到的光合有效辐射 (PAR) 水平,评估了双星/多星系统中存在光合生命的可能性。研究了 M 型星和 G 型星的组合:(i) 近双星系统;(ii) 宽双星系统;和 (iii) 三星系统,并发现了一系列可能的稳定辐射环境。这些环境条件不仅允许存在熟悉的光合作用形式,还允许存在更奇特的光合作用形式,例如红外光合生物和专门适应特定光谱生态位的生物。