Impact of plant photosystems in the remediation of benzo[a]pyrene and pyrene spiked soils

The phytoremediation potential of 14 different plant species belonging to C3 and C4 carbon fixation pathway for soils spiked with polycyclic aromatic hydrocarbons (PAHs) such as benzo[a]pyrene (B[a]P) and pyrene (PYR) was investigated. A glasshouse experiment was conducted to measure the changes in...

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Published inChemosphere (Oxford) Vol. 193; pp. 625 - 634
Main Authors Sivaram, Anithadevi Kenday, Logeshwaran, Panneerselvan, Lockington, Robin, Naidu, Ravi, Megharaj, Mallavarapu
Format Journal Article
LanguageEnglish
Published England Elsevier Ltd 01.02.2018
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Summary:The phytoremediation potential of 14 different plant species belonging to C3 and C4 carbon fixation pathway for soils spiked with polycyclic aromatic hydrocarbons (PAHs) such as benzo[a]pyrene (B[a]P) and pyrene (PYR) was investigated. A glasshouse experiment was conducted to measure the changes in morphological, physiological, biochemical parameters and the bioaccumulation and biodegradation ability of the plants in soils spiked with 48 and 194 mg kg−1 of B[a]P and PYR, respectively. The per cent removal efficacy of B[a]P and PYR by the tested plant species over a period of 50 days was from 6 to 26% and 14 to 40% respectively. The maximum removal of both B[a]P and PYR was observed in Sudan grass (C4), vetiver (C4), maize (C4), and sunflower (C3). In terms of accumulation in root and shoot, the concentration of PYR was higher in both C3 and C4 plant species when compared to B[a]P. Overall the results indicated that C4 plants were more efficient than their C3 counterparts in terms of morphological, physiological, biochemical and degradation ability of PAHs. •Plants tolerant to B[a]P and pyrene were identified.•C4 plants outperformed C3 plants in remediation of PAH contaminated soils.•The efficiency of plants in dissipating pyrene from soil was higher than B[a]P.•Residual B[a]P & pyrene significantly differed between unplanted & planted soils.
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ISSN:0045-6535
1879-1298
DOI:10.1016/j.chemosphere.2017.11.081