Classifying the metal dependence of uncharacterized nitrogenases
Abstract
Nitrogenase enzymes have evolved complex iron–sulfur (Fe–S) containing cofactors that most commonly contain molybdenum (MoFe, Nif) as a heterometal but also exist as vanadium (VFe, Vnf) and heterometal-independent (Fe-only, Anf) forms. All three varieties are capable of the reduction of dinitrogen (N_2) to ammonia (NH_3) but exhibit differences in catalytic rates and substrate specificity unique to metal type. Recently, N_2 reduction activity was observed in archaeal methanotrophs and methanogens that encode for nitrogenase homologs which do not cluster phylogenetically with previously characterized nitrogenases. To gain insight into the metal cofactors of these uncharacterized nitrogenase homologs, predicted three-dimensional structures of the nitrogenase active site metal-cofactor binding subunits NifD, VnfD, and AnfD were generated and compared. Dendrograms based on structural similarity indicate nitrogenase homologs cluster based on heterometal content and that uncharacterized nitrogenase D homologs cluster with NifD, providing evidence that the structure of the enzyme has evolved in response to metal utilization. Characterization of the structural environment of the nitrogenase active site revealed amino acid variations that are unique to each class of nitrogenase as defined by heterometal cofactor content; uncharacterized nitrogenases contain amino acids near the active site most similar to NifD. Together, these results suggest that uncharacterized nitrogenase homologs present in numerous anaerobic methanogens, archaeal methanotrophs, and firmicutes bind FeMo-co in their active site, and add to growing evidence that diversification of metal utilization likely occurred in an anoxic habitat.
Additional Information
© 2013 McGlynn, Boyd, Peters and Orphan. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in other forums, provided the original authors and source are credited and subject to any copyright notices concerning any third-party graphics etc. Received: 09 October 2012; Paper pending published: 02 November 2012; Accepted: 20 November 2012; Published online: 30 January 2013. Shawn E. McGlynn is an Agouron Geobiology Option postdoctoral fellow in the Division of Geological and Planetary Sciences at Caltech and is grateful for support provided by the Agouron Institute. Additional support for this work was provided by the Department of Energy Grant DE-SC0004949 (to Victoria J Orphan) and the NASA Astrobiology Institute (NAI) NNA08C-N85A (to John W. Peters and Eric S. Boyd). Eric S. Boyd also wishes to acknowledge support from the National Science Foundation (EAR-1123689 and PIRE-0968421). The authors are grateful for comments from Aaron D. Goldman, Joshua A. Steele, Wolfgang Nitschke, and members of the laboratory of Victoria Orphan.Attached Files
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Additional details
- PMCID
- PMC3578447
- Eprint ID
- 37576
- Resolver ID
- CaltechAUTHORS:20130320-133744148
- Agouron Institute
- Department of Energy (DOE)
- DE-SC0004949
- NASA
- NNA08C-N85A
- NSF
- EAR-1123689
- NSF
- PIRE-0968421
- Created
-
2013-03-25Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)