2011
DOI: 10.1016/j.gca.2011.01.005
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Spherules with pure iron cores from Myanmar jadeitite: Type-I deep-sea spherules?

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Cited by 18 publications
(9 citation statements)
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“…However, this principle lacks any proven evidence through scienti c studies on spherules, as per our knowledge. Also, the discovery of cosmic spherules from Myanmar jadeitite, a rock type from subduction zone forming at high pressure (> 1 GPa) and relatively low temperatures of about ~ 250-370°C, indicates that the cosmic spherules can withstand such alteration conditions 7 . Though the spherules from Myanmar jadeitite consist of higher Mn (up to 2 wt.%) in the cortex, they also consist of Ni and pure iron cores 7 .…”
Section: Genetic Constraints On the Origin Of Spherules: Mn Hypothesismentioning
confidence: 99%
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“…However, this principle lacks any proven evidence through scienti c studies on spherules, as per our knowledge. Also, the discovery of cosmic spherules from Myanmar jadeitite, a rock type from subduction zone forming at high pressure (> 1 GPa) and relatively low temperatures of about ~ 250-370°C, indicates that the cosmic spherules can withstand such alteration conditions 7 . Though the spherules from Myanmar jadeitite consist of higher Mn (up to 2 wt.%) in the cortex, they also consist of Ni and pure iron cores 7 .…”
Section: Genetic Constraints On the Origin Of Spherules: Mn Hypothesismentioning
confidence: 99%
“…Among these, Fe-rich spherules of extraterrestrial origin are widely investigated to establish the ux of extraterrestrial dust to Earth (Prasad et al 8 and references therein). Earlier studies on cosmic spherules have suggested three types: the chondritic stony spherules (type-S), the glass spherules with dendritic magnetite (type-G), and the nonchondritic iron spherules (type-I) 7,11 . Several criteria have been proposed for the identi cation of the type-I cosmic spherules: (1) morphological features like spherical shape, dendritic phases, and void spaces; (2) chemical signatures like Ni-bearing wustite/magnetite, FeNi metal, and particles of MET, OXMET, and OX type 3 .…”
Section: Introductionmentioning
confidence: 99%
“…The highly depleted mantle Hf isotope signatures of zircons in jadeitites suggest that the fluids were derived from the dehydration of altered oceanic mafic crust (Qiu et al, ; Shi et al, ). However, the presence of Ba‐rich minerals, deep‐sea spherules, and CH 4 ‐rich fluid inclusions in the Myanmar jadeitites suggests that subducted sediments were also incorporated into the jadeite‐forming fluids (Shi et al, , , ). In addition, Mg‐Cr‐rich jadeite rims in jadeitites reflect a minor addition of serpentinite‐derived fluid into the jadeite‐forming fluids (Sorensen et al, ).…”
Section: Geological Setting and Samplesmentioning
confidence: 99%
“…The jadeites in the white jadeitites commonly exhibit rhythmic zoning in Ca and Mg (Figure 3b), suggesting that they were most likely precipitated from Na-Al-Si-rich fluids (Figure 7; Shi et al, 2003Shi et al, , 2012Sorensen et al, 2006). Such fluids were mainly derived from subducted AOC and sediments (e.g., Harlow et al, 2015;Qiu et al, 2009;Shi et al, 2010Shi et al, , 2011. Minor locally serpentinite-derived fluids might also contribute to the jadeitite-forming fluids (Sorensen et al, 2006); however, no direct mineral evidence for serpentinite dehydration was observed.…”
Section: Fluid Sources Along the Subduction Interfacementioning
confidence: 99%
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