2002
DOI: 10.1007/bf02932205
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Extraterrestrial3 He in marine polymetallic nodules: A potential method for measuring growth rate of nodules

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Cited by 4 publications
(6 citation statements)
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“…Previous studies on deep-sea sediments [15][16][17][18][19] and nodules [41,43,44] and seamount crusts [46,47,50,69] in the open oceans suggested that the extremely high 3 He/ 4 He ratio reflects extraterrestrial inputs, such as IDPs. Helium isotope characteristics of individual IDPs collected in the stratosphere were analyzed, yielded 3 He/ 4 He ratios of mainly 2.4 × 10 −4 (172R A ) and the 3 He content of 1.9 × 10 −5 cm 3 ·STP·g −1 [70].…”
Section: Extraterrestrial Sourcementioning
confidence: 99%
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“…Previous studies on deep-sea sediments [15][16][17][18][19] and nodules [41,43,44] and seamount crusts [46,47,50,69] in the open oceans suggested that the extremely high 3 He/ 4 He ratio reflects extraterrestrial inputs, such as IDPs. Helium isotope characteristics of individual IDPs collected in the stratosphere were analyzed, yielded 3 He/ 4 He ratios of mainly 2.4 × 10 −4 (172R A ) and the 3 He content of 1.9 × 10 −5 cm 3 ·STP·g −1 [70].…”
Section: Extraterrestrial Sourcementioning
confidence: 99%
“…Sano et al [41] first studied the He and Ar isotopes of the deep-sea nodules from the Ogasawara Islands and Mariana Trough and suggested that extremely high 3 He/ 4 He ratios are caused by the input of extraterrestrial material. Subsequently, the He isotopes of the deep-sea nodules from the Pacific Clarion-Clipperton Fracture Zone (CCFZ) were studied [42][43][44][45]. These researches founded that the deep-sea nodules have high 3 He contents and 3 He/ 4 He ratios (5-54 R A [42,45]) and that the sediments around the deep-sea nodules also have the high 3 He/ 4 He ratios [44].…”
mentioning
confidence: 99%
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“…All the results of helium are given in forms of 3 He/ 4 He ratio and R/Ra ratio, where R is the 3 He/ 4 He ratio of the sample and Ra is that of air. The blank level of 4 He is 2 × 11 −11 cm 3 STP and the blanking 3 He/ 4 He ratio is 1 × 10 −6 (Li et al , 2002). The analytical precision of the standard gas is 1% and that of samples is included in Table 3.…”
Section: Isotope Geochemistrymentioning
confidence: 99%