INTRODUCTION
Iron cycling is a key biogeochemical process in rice paddies that plays important roles in the growth and quality of rice crops. Fe(II) oxidation leads to the production of Fe(III) oxyhydroxides (ferrihydrite, goethite, and lepidocrocite), which are strong sorbents of organic carbon, phosphate, and metal(oid)s such as As and Cd (
1–5); Fe(III) reduction dissolves the oxyhydroxides and releases sorbed nutrients and toxins (
6). Of particular interest are iron oxyhydroxide coatings (plaques) that develop on the surface of rice roots (rhizoplane), as well as in the rhizosphere (satellite plaque). Fe(II)-oxidizing and Fe(III)-reducing bacteria (FeOB and FeRB) have been documented in association with a variety of wetland plants (
7,
8). Because plaque is closely associated with rice roots, its formation and dissolution may limit or drive plant uptake of oxyhydroxide-sorbed chemicals (
9–12), motivating us to study the mechanisms of rice root plaque formation. FeOB can catalyze the formation of Fe(III) oxyhydroxides via their metabolism. FeOB have been detected in paddy soil (
11,
13,
14), making them a potential mechanism for iron plaque formation in conditions in which they can outcompete abiotic Fe(II) oxidation.
The rice rhizoplane is in fact an ideal niche for microaerophilic FeOB, which gain energy by coupling Fe(II) oxidation to oxygen reduction, and thus grow best where Fe(II) and O
2 fluxes are high. Although Fe(II) oxidation coupled to nitrate reduction is possible in theory, it is unlikely to be a significant process because N is a limiting nutrient throughout most of the rice growing season (
15–18). Rice paddy soil is rich in Fe(II) formed by microbial Fe(III) reduction; thus, plaque formation is partially dependent on the activities of FeRB. Rice root aerenchyma is a conduit of O
2, which diffuses from roots into saturated soil rich in Fe(II), providing both electron donor and acceptor for FeOB. Aerobic FeOB must compete with abiotic oxidation, and kinetics studies showed they become the dominant mechanism of iron oxidation as oxygen concentrations decrease (
19,
20). Different neutrophilic FeOB can thrive at O
2 concentrations < 1–100 µM (
21–24), concentrations that coincide with ranges typically found at the surface of rice roots (few micromolar to tens of micromolar O
2) (
25,
26). Thus, it is plausible that a significant proportion of plaque iron oxidation is microbial.
Indeed, studies have increasingly documented FeOB in rice paddy soil, thus increasing recognition that microbes can contribute to iron oxidation in this environment. FeOB can be documented by culturing, 16S rRNA gene analyses, and metagenomic studies, which give different evidence of potential contributions. Numerous studies have shown that FeOB can be cultured from rice paddy soil, with a range of taxa represented (
13,
24,
27–31). While culturing demonstrates microbial iron oxidation activity, it only proves that soil-derived organisms are capable of iron oxidation, but cannot show that these FeOB represent the major active organisms
in situ. Studies using 16S rRNA genes give a broader view of soil microbial communities, but it is often unclear which organisms are FeOB, or identification is equivocal due to the metabolic flexibility of putative FeOB. The exceptions are taxa specifically known for iron oxidation, like Gallionellaceae iron-oxidizing genera, including
Gallionella,
Ferrigenium, and
Sideroxydans (
28,
32,
33). As their primary metabolism is iron oxidation, detection of Gallionellaceae FeOB in field samples is a strong indication of microbial iron oxidation in the environment.
Gallionellaceae FeOB have been cultured from paddy soil, including the isolates
Gallionella/Ferrigenium kumadai An22 (
28,
34) and
Sideroxydans sp. (
24). While the isolate An22 was named
Ferrigenium based on 16S rRNA gene dissimilarity from
Gallionella, subsequent full-genome analyses showed that it is a
Gallionella (
35). Gallionellaceae have also been identified using 16S rRNA gene analyses including universal and taxa-specific primers in paddy soil and the rice rhizosphere (
31,
36–39). Their abundance has been shown to correspond to iron oxidation in paddy soil and soil incubations (
30,
40).
Gallionella have been detected in rhizoplane samples by qRT-PCR (
41). However, it has not been shown whether Gallionellaceae are specifically enriched in abundance at the rhizoplane (vs soil) and associated with plaque oxyhydroxides. Schmidt and Eickhorst (
36) used CARD-FISH to show Betaproteobacteria (which includes Gallionellaceae) on root surfaces, and suggested that these may represent Gallionellaceae detected via 16S rRNA sequences (
42). In all, there is strong evidence for the existence of these FeOB in paddy soil, but it is still unclear if Gallionellaceae are specifically associated with plaque and therefore contribute to iron oxyhydroxide formation. If FeOB are in fact associated with plaque, this close association with the root could cause them to compete with the plant for nutrients like N, or alternatively, FeOB may provide fixed N and other nutrients to help promote plant growth. To understand the biogeochemical cycling in the rice root rhizosphere, we need to determine the dynamics and functions of plaque microorganisms, and their interactions with the rice plant.
In this study, we investigated the spatial and temporal dynamics of rice-associated FeOB and FeRB in rice paddies over a growing season, using 16S rRNA gene analyses of bulk soil, rhizosphere, and plaque samples. This was coupled to plaque Fe analyses as well as examination of metagenomic-assembled genomes of FeOB to more specifically identify metabolic capabilities and niches. Taken together, this allowed us to identify the major FeOB enriched in iron plaque and give insight into how microbes contribute to plaque formation over the life cycle of field-grown rice.
ACKNOWLEDGMENTS
The authors thank the Joint Genome Institute for funding and performing sequencing. We thank our field sampling team: Patrick Wise, Kristy Northrup, Weida Wu, Ayofela Dare, Kendall McCoach, Fred Teasley, Douglas Amaral, Ruifang Hu, Alesia Hunter, Julia O’Brien, and Heather Eby. The authors thank Olushola Awoyemi for help with genome analyses.
This work was supported by the National Science Foundation Grant nos. 1350580 and 1833525, USDA NIFA Grant no. 2016-67013-24846, the DENIN Environmental Fellows Program, the University of Delaware Doctoral and Dissertation Fellowships, and the Preston C. Townsend Biotechnology Fellowship. Sequencing for this project was completed by the Joint Genome Institute for project ID 503349. Use of the Stanford Synchrotron Radiation Lightsource, SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract no. DE-AC02-76SF00515.
This work is not a product of the United States Government or the United States Environmental Protection Agency. The author/editor is not doing this work in any governmental capacity. The views expressed are his/her own and do not necessarily represent those of the United States or the US EPA.