Yeung Laurence Y, Li Shuning, Kohl Issaku E, Haslun Joshua A, Ostrom Nathaniel E, Hu Huanting, Fischer Tobias P, Schauble Edwin A, Young Edward D
Department of Earth, Environmental and Planetary Sciences, Rice University, Houston, TX 77005, USA.
Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, CA 90089, USA.
Sci Adv. 2017 Nov 17;3(11):eaao6741. doi: 10.1126/sciadv.aao6741. eCollection 2017 Nov.
Molecular nitrogen (N) comprises three-quarters of Earth's atmosphere and significant portions of other planetary atmospheres. We report a 19 per mil (‰) excess of NN in air relative to a random distribution of nitrogen isotopes, an enrichment that is 10 times larger than what isotopic equilibration in the atmosphere allows. Biological experiments show that the main sources and sinks of N yield much smaller proportions of NN in N. Electrical discharge experiments, however, establish NN excesses of up to +23‰. We argue that NN accumulates in the atmosphere because of gas-phase chemistry in the thermosphere (>100 km altitude) on time scales comparable to those of biological cycling. The atmospheric NN excess therefore reflects a planetary-scale balance of biogeochemical and atmospheric nitrogen chemistry, one that may also exist on other planets.
分子氮(N)占地球大气的四分之三,在其他行星的大气中也占相当大的比例。我们报告称,相对于氮同位素的随机分布,空气中的N₂有19‰的过量,这种富集程度比大气中同位素平衡所允许的程度大10倍。生物学实验表明,氮的主要来源和汇在氮中产生的N₂比例要小得多。然而,放电实验确定N₂的过量高达+23‰。我们认为,由于热层(海拔>100公里)中的气相化学作用,在与生物循环相当的时间尺度上,N₂在大气中积累。因此,大气中N₂的过量反映了生物地球化学和大气氮化学在行星尺度上的平衡,这种平衡可能也存在于其他行星上。