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Applied and Environmental Microbiology, January 2008, p. 61-66, Vol. 74, No. 1
0099-2240/08/$08.00+0 doi:10.1128/AEM.01199-07
Copyright © 2008, American Society for Microbiology. All Rights Reserved.

Department of Biological Sciences, University of Wisconsin—Milwaukee, Milwaukee, Wisconsin
Received 29 May 2007/ Accepted 24 October 2007
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For more than a century, bacterial bioluminescence has called attention to itself by its obvious visual phenotype. It is only since the advent of molecular probing techniques that we have become aware of the potentially widespread occurrence of non-visibly luminous strains (19, 27, 29). Palmer and Colwell (27) found a wide range of luminescence intensity levels among natural Vibrio cholerae isolates and discovered that a significant fraction of "visually non-luminescent" isolates contained a luxA gene. Lee and Ruby (19) took advantage of molecular probing to demonstrate that near-shore Hawaiian seawater contains a large number of non-visibly luminous Vibrio fischeri strains, consistent with the phenotype of the light organ symbionts of the bobtail squid Euprymna scolopes, which do not visibly glow under typical laboratory culture conditions but glow brightly in the squid. Using a V. harveyi luxA gene probe, Ramaiah et al. (29) found that an average of 1.7% of their Chesapeake Bay isolates had luxA but were not visibly bioluminescent. They suggested that either lux genes were not being expressed or that alterations or deletions had occurred in lux genes. The molecular basis of these dark phenotypes in natural populations has been, until now, unexplored.
Our work shows that natural populations of vibrios in Boca Ciega Bay, Florida, also include dark strains that contain lux genes. Additionally, we have discovered the molecular basis for the dark phenotypes of our isolates. In this paper, we report the detection of mutations in the lux operon of dark strains of Vibrio species. Screening of over 600 environmental Vibrio isolates from Boca Ciega Bay, Florida, revealed three dark genotypes. Sequence analysis of lux operons from the dark mutants reveals that one strain has an IS10 insertion sequence in luxA, a mutated luxE stop codon, and a truncated luxH gene. A second mutant has a deletion in luxC, while a third mutant has a frameshift in luxC. To our knowledge, this is the first molecular characterization of natural dark mutants.
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TABLE 1. Bacterial strains used in this study
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TABLE 2. Oligonucleotide primer and probe sequences used in this study
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-32P]dCTP (Perkin-Elmer Life Sciences, Wellesley, MA) using the Prime-A-Gene system purchased from Promega (Madison, WI). For initial luxA hybridizations, environmental Vibrio strains were inoculated individually onto gridded circular nylon transfer membranes (Osmonics) on SWC agar plates. The SWC plates were incubated for 16 h at room temperature, after which membranes were removed from SWC plates using sterile forceps, and colonies were lysed according to Sambrook et al. (32). For screening of genomic libraries, colonies were transferred to membranes by colony lift. Membranes were prehybridized and hybridized using standard protocols (32).
DNA extraction and fingerprint analysis.
Genomic DNA was isolated from SWC broth cultures using the cetyltrimethylammonium bromide procedure (1). Bacteria were genotyped by repetitive extragenic palindromic PCR genomic fingerprinting using a BOX primer, as described by Rademaker and deBruijn (28). Gel images were digitally captured using a Gel Logic 100 Kodak Imaging System and examined visually for differences in genomic profiles of different strains.
Screening environmental clones for luminescence.
Environmental isolates showing positive luxA hybridization were stabbed onto SWC plates and grown overnight at room temperature. Colonies were then taken into a dark room and visually examined for bioluminescence. Environmental isolates that appeared to be visually dark were then stabbed onto a single SWC plate, placed on X-ray film in a light-protected box, and exposed overnight.
Genomic cloning of strains BCB440, BCB451, and BCB494.
Total genomic DNA was subjected to either partial Sau3A digestion (BCB451) or total Xba1 digestion (BCB440 and BCB494), followed by size selection of 10-kb fragments on 0.75% agarose gels. DNA was eluted from gels using Qiaex II (Qiagen) and ligated into pGEM3Z cloning vector (Promega, Madison, WI). Ligated plasmids were then moved into Escherichia coli strain XL10-Gold (Stratagene) by transformation. The transformed cells were plated on LB plates containing 100 µg/ml ampicillin, 50 µl of X-Gal (5-bromo-4-chloro-3-indolyl-β-D-galactopyranoside; 50 mg/ml), and 50 µl of 100 mM IPTG for blue/white screening.
Plasmid isolation and DNA sequencing.
Plasmids were isolated using a QIAprep Spin Miniprep Kit (Qiagen, Inc.) and insertion ends were sequenced using primers specific to the T7 and SP6 promoter regions. Automated sequencing was done by the Cancer Research Center DNA Sequencing Facility at the University of Chicago. Internal lux operon sequences were generated using primers based on V. harveyi strain B392. Flanking regions were sequenced using primers based on the previous sequence runs (i.e., primer walking). To identify protein coding genes, DNA sequences were subjected to BLASTX analysis (12; http://www.ncbi.nlm.nih.gov) using the default parameters.
Genomic cloning of the V. harveyi B392 lux operon for complementation.
The lux operon from V. harveyi strain B392 (ATCC 33843) including regulatory elements was cloned into a KpnI-digested Vibrio shuttle vector, pVSV105 (8) (gift of Erik Stabb), which contains a chloramphenicol resistance cassette. The shuttle vector with insert was designated pEOG. pEOG was transformed into E. coli strain DH5
pir (Erik Stabb, Active Motif, Carlsbad, CA) and plated on LB plates containing 25 mg/ml chloramphenicol, 50 µl of X-Gal (50 mg/ml), and 50 µl of isopropyl-β-D-thiogalactopyranoside (100 mM) allowing for blue/white screening.
Conjugation.
Triparental matings were carried out using E. coli DH5
pir containing the pEOG as the donor, E. coli CC118
pir containing the conjugation helper plasmid pEVS104, and, in separate conjugations, BCB440, BCB451, or BCB494 as the recipients. Three empty vector controls, BCB440/pVSV105, BCB451/pVSV105, and BCB494/pVSV105, were also generated using triparental mating.
Light and turbidity measurements.
Strains BCB440/pEOG, BCB451/pEOG, BCB494/pEOG, BCB440/pVSV105, BCB451/pVSV105, BCB494/pVSV105, BCB440, BCB451, and BCB494 were inoculated and grown for 16 h at room temperature. After 16 h, samples were diluted 1:100, and luminescence and optical density readings were taken every hour over an 8-h time period. Luminescence was measured using a Lumac/3m Biocounter M2010 luminometer. Optical density at 600 nm was measured in all strains prior to light measurements on a Versamax Spectrophotometer plate reader.
Nucleotide sequence accession numbers.
The following sequences obtained in this study for the lux operon and flankers of the indicated strains were deposited in the GenBank database (accession numbers are in parentheses): BCB440 (EU192082), BCB451 (EU192083), and BCB494 (EU192084).
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FIG. 1. Autoradiogram indicating the Vibrio isolates positive for luxA. Thirty of 610 isolates hybridized with a V. harveyi luxA gene probe. Control strains are shown at the bottom right.
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FIG. 2. Amplified PCR products obtained using luxA primers 127 F and 1007 R (left) and luxC primers VhluxC F1 and VhluxC R1 (right) from dark mutants and V. harveyi B392 (ATCC).
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FIG. 3. Gene map of BCB451 (A), BCB494 (B), and BCB440 (C) lux operons. The genes, insertion elements, and deletions are drawn to scale and positioned in the direction in which they are transcribed. Positions of point mutations in strains BCB451 and BCB440 are indicated. UTR, untranslated region.
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FIG. 4. Direct and inverted repeats of BCB451. (A) Schematic of the positions of direct and inverted repeats flanking IS10. (B) Sequence of direct repeats. (C) Alignment of BCB451 and S. flexneri inverted repeats.
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FIG. 5. (A) Translated sequence of BCB494 truncated IS3 insertion sequence aligned with insertion sequences of V. parahaemolyticus (Vp) and V. vulnificus (Vv). (B) IS22 insertion sequence aligned with that of Pseudomonas aeruginosa.
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Although the mutations described above are sufficient to account for the dark phenotypes observed in strains BCB440, BCB451, and BCB494, the entire lux operon of each mutant was cloned and sequenced to determine whether additional debilitating mutations can be detected. No additional lesions were found in BCB494 and BCB440, but there were two additional mutations in BCB451. The luxE stop codon of BCB451 has mutated to TCA, and the luxH gene is truncated by 203 bp (Fig. 3A).
Complementation of dark mutants.
The identification and nature of the mutations in the three dark mutants raised the question as to whether genetic complementation would rescue the light phenotype. To test this, the entire lux operon of V. harveyi strain B392 was cloned and introduced into each of the three dark mutants by conjugation. As shown in Fig. 6, complementation with a functional lux operon restored light production in all three mutants. In addition, the rescued light-producing phenotype displayed the cell density dependence typical of quorum sensing.
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FIG. 6. (A-C) Luminescence measurements of dark mutants complemented with the lux operon and upstream regulatory region. (A) BCB440/pEOG (circles), BCB440/pVSV105 (triangles), and BCB440 (squares). (B)BCB451/pEOG (circles), BCB451/pVSV105 (triangles), and BCB451 (squares). (C) BCB494/pEOG (circles), BCB494/pVSV105 (triangles), and BCB494 (squares). (D-F) Quorum-sensing-regulated luminescence. Specific luminescence was calculated by dividing luminescence by the absorbance for each time point of strains BCB440/pEOG (D), BCB451/pEOG (E), and BCB494/pEOG (F).
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Consistent with the abnormally large luxA PCR product of strain BCB451, we find that its luxA gene has been invaded by an IS10 insertion sequence. Although the BCB451 insertion has the signature inverted repeats of IS10, there is an additional 19-bp insertion within the inverted repeat on the 5' end of the transposase gene. Whether this impairs the function of the IS10 is unknown. It is possible that the insertion within this inverted repeat happened subsequent to transposition, and the insertion element is now immovably trapped in the luxA gene. In BCB494, the first 396 bp of luxC are deleted. The sequences adjacent to the luxC deletion are homologous to the known bacterial insertion elements IS3 and IS222. However, these insertion sequences have themselves suffered catastrophic deletions and are unlikely to be functional. Unlike strains BCB451 and BCB494, which immediately showed PCR anomalies that led us to discover their respective lesions, PCR analysis of BCB440 showed no obvious abnormalities. When we sequenced the operon, the only lesion we found was a single base pair frameshift in luxC. Complementation of all three dark mutants restored cell density-dependent light production, indicating that the lesions in their lux operons solely account for the dark phenotype of these strains. Had the complementation not restored light production, other physiological or regulatory processes might have been implicated, in addition to the structural mutations.
There is a precedent for insertion sequence invasion of lux genes in a recent report of transposase disruption of the luxF gene in a Photobacterium mandapamensis strain (14). Although the P. mandapamensis insertion does not knock out luminescence (since luxF is not essential for bioluminescence), there are, nevertheless, indications that the insertion might affect the intensity of light emission in that strain. Since the P. mandapamensis strain carrying this insertion in luxF was isolated as a light organ symbiont, this knockout is a natural experiment in selection on the light-producing phenotype.
Because the operon functions as an integrated system, erosion of other lux genes in these dark mutants might be expected. Only BCB451 shows noticeable deterioration of the operon, which occurs in two additional places. The mutated luxE stop codon of BCB451 would result in a frameshifted fusion of luxE and luxG. An additional abnormality in BCB451 is a truncated luxH gene. However, luxH is a homolog of the ubiquitous ribB, which would provide the compensatory function in the riboflavin synthesis pathway which is required for luminescence. We have no way of knowing whether these additional mutations occurred before or after the IS10 insertion in luxA.
Dark variants have long been known in the bacterial bioluminescence field (15, 22, 33). Such variants occur most often in old cultures, especially in broth. However, such variants generally arise as a subset of luminous populations and are often unstable and prone to reversion, implying a mechanism akin to phase variation. In contrast, our mutants were dark as primary colonies and have remained so in all subsequent cultures derived from them. The luxA hybridization assays were performed after one transfer, and DNA was isolated for PCR and cloning from the same colonies as the hybridization assays. For these reasons, we are confident that the mutations did not arise in the laboratory. Further evidence to support a natural origin of our mutants includes the following: (i) we encountered the BCB494 genotype twice (BCB584 has the same genotype), in separate samples from separate locations in Boca Ciega Bay; (ii) BCB451 has three different types of mutations within the lux operon, a circumstance that would be highly unlikely to occur simultaneously in the primary colony; and (iii) in BCB440, the single point mutation leading to a frameshift would have to have occurred in the single cell that gave rise to the primary dark colony (i.e., in the seawater sample itself).
It is generally assumed that the preservation of gene sequences is the result of positive selection, but selection in the lux operon has long been the subject of debate (2, 4, 5, 23, 34). Several Vibrio and Photobacterium strains trade light for nutrients while participating in symbiotic relationships with various fish and/or squid species (7, 23, 30, 31). The selective advantage for light production is obvious in these cases. However, the vast majority of luminous bacterial isolates (including ours) are planktonic. At any time of the year, Boca Ciega Bay water yields dozens of luminous isolates per milliliter, most of which have different genotypes (16, 17). By sheer number and diversity, it is clear that planktonic bioluminescent strains are very common, yet the selective pressure that maintains this process is not obvious. It has been suggested (15; discussed in reference 34) that dark mutants would out-compete otherwise isogenic bright strains, simply because of the cost of light production. However, expression of the lux operon in the planktonic state should normally be low (and therefore inexpensive), because it is under quorum-sensing regulation (23). Quorum sensing requires high population density, which should be very rare in planktonic forms (however, see references 18, 21, and 26). This regulatory requirement argues that under typical environmental conditions, the lux operon would be all but superfluous in planktonic forms, so its loss should not be disadvantageous. However, although our data show that dark mutants are not uncommon, they are in the minority of the strains that possess lux genes. This argues against the idea that bioluminescence is an expensive remnant that is on its way to extinction in all but the symbiotic forms or an unnecessary vestige that can be lost with no disadvantage.
To our knowledge, the deletions we have found in BCB494 luxC and BCB451 luxH represent the first report of incomplete lux operons in natural isolates. We predict that there are many more. It is likely that we are underestimating the number of dark mutants in our sample group, since our initial screening used only luxA as a probe. It would not be surprising to find other mutants that lack luxA but possess other lux genes or that have lost the lux operon entirely. Such strains have thus far escaped detection, simply because we have not yet looked for them. We are almost certainly seeing a snapshot of a very dynamic process.
Published ahead of print on 2 November 2007. ![]()
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