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Interplanetary dust particles accrete on the Earth at a rate of ∼40 ktons yr −1 . Some 90% of this material evaporates in the atmosphere, producing a bioavailable iron flux of 3×10 −7 mol Fe m −2 yr −1 . This extraterrestrial Fe flux is 30–300% of the eolian flux of bioavailable iron transported from terrestrial sources in remote marine regions and ∼20% of the upwelled Fe flux in the Southern Ocean. Extraterrestrial Fe may play an important role in regulating the marine carbon cycle in these regions.
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Kenneth S. Johnson (2001) studied this question.
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