Broadley Michael W, Barry Peter H, Tyne Rebecca L, Bekaert David V, Karolyte Ruta, Hudak Michael R, McPaul Katelyn, Ramirez Carlos J, Curtice J, Lloyd Karen G, Ballentine Christopher J, Marty Bernard, Young Edward D, Seltzer Alan M
Department of Earth and Environmental Science, University of Manchester, Manchester M13 9PL, U.K.
Marine Chemistry and Geochemistry, Woods Hole Oceanographic Institution, Woods Hole 02543, United States.
ACS Earth Space Chem. 2025 Mar 24;9(6):1310-1321. doi: 10.1021/acsearthspacechem.4c00349. eCollection 2025 Jun 19.
Nitrogen plays a critical role in maintaining Earth's hospitable surface environment over geological time. Despite our atmosphere being dominated by nitrogen, our understanding of how nitrogen was delivered to Earth and how subsequent planetary processes modified Earth's nitrogen budget through time is currently lacking. Here, we report measurements of isotopologues of N (Δ), along with ultrahigh precision measurements of Ar, Kr, and Xe isotopes, of hydrothermal gas samples from Yellowstone National Park. We show that δN variations are correlated with nonradiogenic Ar, Kr, and Xe isotope ratios, indicating that groundwater-derived nitrogen and noble gases in hydrothermal samples are fractionated by the same process as they diffuse through a rising column of magmatic CO. Notably, a similar correlation exists regardless of the degree of atmospheric contamination, suggesting that the δN of the Yellowstone mantle source is similar to the atmosphere (i.e., ∼0‰). Two component mixing models between Δ and noble gases demonstrate that N/Ar (5.3 ± 0.7 × 10) and Ar/Xe (1611 ± 212) in the Yellowstone mantle source are lower and greater than the MORB mantle source, respectively, suggesting that contrary to previous findings, the plume mantle source has not been more efficiently overprinted by the addition of N- and Xe-rich recycled material. Conversely, we suggest that the similarity in δN and N/Ar between the Yellowstone mantle source and chondritic meteorites indicates that nitrogen and noble gases in the deep mantle reflect the composition of the material that initially formed Earth.
在地质时期,氮在维持地球宜居的表面环境方面发挥着关键作用。尽管我们的大气以氮为主,但目前我们仍缺乏对氮如何输送到地球以及随后的行星过程如何随时间改变地球氮预算的了解。在此,我们报告了来自黄石国家公园热液气体样本中氮的同位素变体(Δ)的测量结果,以及氩、氪和氙同位素的超高精度测量结果。我们表明,δN变化与非放射性氩、氪和氙同位素比率相关,这表明热液样本中源自地下水的氮和惰性气体在通过上升的岩浆CO柱扩散时,是通过相同过程进行分馏的。值得注意的是,无论大气污染程度如何,都存在类似的相关性,这表明黄石地幔源的δN与大气相似(即约0‰)。Δ与惰性气体之间的双组分混合模型表明,黄石地幔源中的N/Ar(5.3±0.7×10)和Ar/Xe(1611±212)分别低于和高于洋中脊玄武岩地幔源,这表明与先前的研究结果相反,羽状体地幔源并没有因添加富含氮和氙的再循环物质而更有效地被覆盖。相反,我们认为黄石地幔源与球粒陨石之间δN和N/Ar的相似性表明,深部地幔中的氮和惰性气体反映了最初形成地球的物质的组成。