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Infection and Immunity, April 2000, p. 2344-2348, Vol. 68, No. 4
Mikrobielle Genetik, Universität
Tübingen, D-72076 Tübingen,
Germany,1 and ZENECA
Pharmaceuticals, Macclesfield, Cheshire SK10 4TG,
England2
Received 25 October 1999/Returned for modification 18 November
1999/Accepted 13 December 1999
The Staphylococcus aureus repeat (STAR) element is a
sequence identified in two intergenic regions in S. aureus.
The element is found in 13 to 21 copies in individual S. aureus strains, and elements in the homologous intergenic
location are variable in length. The element sequence consists of
several small and unusually GC-rich direct repeats with recurring
intervening sequences. In addition, STAR-like elements may be present
in related staphylococcal species.
Nosocomial Staphylococcus
aureus infections require rapid identification and source
recognition so that further spread, particularly of multiply resistant
or unusually pathogenic strains, can be controlled. A number of methods
to identify and distinguish bacterial strains have been developed.
More-traditional phenotypic characterization has been gradually
replaced by DNA sequence-based technology. PCR amplification has been
particularly useful for strain typing in a clinical setting because it
is rapid, relatively easy to automate, and less labor-intensive
(14) than methods such as pulsed-field gel electrophoresis
or Southern blotting (12). As DNA sequencing technology
becomes increasingly more available in a clinical setting,
nucleotide-level analysis is likely to be used more often, perhaps in
combination with PCR fingerprinting, for strain identification.
A strategy currently used for strain typing of S. aureus
relies on the amplification of defined tandemly repeated DNA sequences, often within surface-associated proteins, that are present in a
variable number of copies in different strain isolates (for reviews,
see references 7 and 13). This
technique usually requires the analysis of several marker loci to
differentiate strains that may by chance alone be identical at one locus.
Here, we describe a DNA sequence that is highly variable among S. aureus strains and that is found in many copies throughout the
genome. An analysis of PCR products whose sizes may differ by only a
few nucleotides and/or nucleotide sequence analysis at several loci
would allow the rapid identification and detailed differentiation of
clinical isolates.
Methods.
The primers listed in Fig.
1A lie within the uvrA and
hprK coding regions and were used to amplify the
uvrA-hprK intergenic sequence for sizing as well as
subcloning and sequencing. The primers shown in Fig. 1B lie just
downstream of the icaC and geh coding sequences
and were used for fragment sizing. The following two primers within the
coding region of each gene were used to amplify a slightly larger
fragment from each strain for subcloning and sequencing: SA18,
5'-GTATAGGTGTCGGCATGATATTGCGTG; SA19,
5'-T GAAAACTGAAAAGCTGACTGATACTAAGC. Primers were
obtained from MWG-Biotech (Ebersberg, Germany). Fragments were
amplified using Taq (AGS, Heidelberg, Germany) or Vent (New
England Biolabs GmbH, Schwalbach, Germany) polymerase and annealing
temperatures of 62 (uvrA-hprK) or 52°C
(icaC-geh). PCR products were blunt-end ligated into vector pUC18 using the SureClone ligation kit (Amersham Pharmacia Biotech, Braunschweig, Germany) and sequenced on both strands by MWG-Biotech, with the following exceptions. The uvrA-hprK intergenic
sequence from strain 601055 (Zeneca Pharmaceuticals strain collection) was obtained using Pathoseq S. aureus contig sequence
information available from Incyte Pharmaceuticals (Palo Alto, Calif.)
and contained on contig Sau1c0627. The icaC-geh intergenic
sequence from strain ATCC 35556 was previously published by our group
and was not resequenced for this work (2). Computer sequence
analysis was performed using Multalin, version 3.5.5 (1),
with manual adjustments. Preliminary S. aureus sequence data
were obtained from The Institute for Genomic Research at
http://www.tigr.org and the S. aureus Genome Sequencing
Project (University of Oklahoma) at http://www.genome.ou.edu.
Southern blots were hybridized and washed (0.1× SSC [1× SSC is 0.15 M NaCl plus 0.015 M sodium citrate]-0.1% sodium dodecyl sulfate) at
55°C and detected using the DIG DNA labeling and detection kit from
Boehringer (Mannheim, Germany).
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Copyright © 2000, American Society for Microbiology. All rights reserved.
Identification of a New Repetitive Element in
Staphylococcus aureus
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FIG. 1.
Intraspecies diversity in STAR element size. The
intergenic sequences between uvrA-hprK (A) and
icaC-geh (B) in 12 S. aureus strains, listed
below each agarose gel, were amplified by PCR. The fragments were
grouped into size classes (I to VI and I to V, respectively), and a
representative from each class was sequenced. A schematic
representation of the chromosomal organization in each region is shown
beneath each agarose gel. The primers used for PCR amplification are
listed at the bottom.
Identification of the STAR element. A comparison of the hprK sequence from Staphylococcus xylosus (3a) with the S. aureus sequence available from a commercial provider (Incyte Pharmaceuticals) identified a noncoding intervening sequence in the region between uvrA and the hprK promoter that was not present in S. xylosus. The sequence contained two large and several smaller direct repeats that were unusually GC rich, including several copies of the sequence GGGGCCCC. The presence of multiple copies of this sequence, which contains the recognition site for restriction enzyme ApaI (GGGCC^C), in close proximity is highly improbable in these AT-rich organisms.
Public database searches identified a Tn557 attachment site (6) and significant similarity to a noncoding sequence included in a database entry for the S. aureus lipase (geh) (9). Other work with the neighboring S. aureus intercellular adhesion (ica) genes identified the same database entry and led to a closer examination of the intergenic sequences at the two loci (2). In the meantime, public databases show a third example of what we have called the S. aureus repeat (STAR) element near the trxB gene in S. aureus (accession no. AJ223781.1). From these dispersed representatives, we concluded that STAR is a repetitive element present in multiple copies in the S. aureus genome.Size variability. Initial sequence comparisons revealed that the intergenic regions between icaC and geh in strain ATCC 35556 and strain U500 in the database were not identical, the latter being smaller by a 58-bp directly repeated sequence. This led to a size analysis of the icaC-geh intergenic sequences by PCR amplification of a number of different S. aureus strains, which revealed that the sequence showed significant size variability. A similar PCR analysis, which also showed size variability among strains, was carried out at the uvrA-hprK locus. Figure 1A shows six different size classes ranging from 573 to 1,127 bp among representative strains in which the intergenic region between uvrA and hprK was examined. Five size classes (380 to 577 bp) were discernible among the same strains when the intergenic region between icaC and geh was investigated (Fig. 1B). In addition, a sixth size class (520 bp) is represented by the icaC-geh intergenic sequence of strain U500 (9), not shown here.
Sequence comparison.
The sizes of each sequenced fragment and
the corresponding STAR element are listed in Table
1, along with the database nomenclature. A sequence comparison of the STAR elements, including part of each
intergenic region, is shown in Fig. 2.
The alignment is structured around the largest STAR element, star01,
from the uvrA-hprK intergenic region of strain 601055. Figure 3 graphically depicts the
structure of the star01 sequence, including the sequences flanking the
STAR element.
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Abundance of the STAR element in S. aureus.
Due to the
presence of two STAR elements in different and apparently unrelated
chromosomal locations, it seemed reasonable to assume that there were
more STAR elements elsewhere in the S. aureus genome.
Chromosomal DNA from the strains shown in Fig. 1 was digested with
restriction enzyme HindIII, blotted, and hybridized with
the uvrA-hprK intergenic region from strain 601005, the
largest STAR sequence from the two loci we investigated in detail. We expected that a single hybridizing band would be specific for the
fragment containing the uvrA-hprK region used as the probe and that any other bands would represent other STAR elements. The
Southern blot shown in Fig. 4 reveals 13 to 21 cross-hybridizing bands, depending on the strain. The number of
cross-hybridizing bands may be an underestimate, however, because each
band could contain more than one STAR element, but it is clear that the
STAR element is present in tens but not thousands of copies in the S. aureus genome.
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Presence and abundance of the STAR element in other staphylococci. Cross-species staphylococcal DNA hybridization was also performed, using the same S. aureus uvrA-hprK STAR element as a probe. No signal was detected with DNA from S. carnosus, S. hyicus, S. saprophyticus, S. simulans, or S. xylosus; however, cross-hybridization with the STAR probe was observed with DNA from S. epidermidis (6 bands), S. haemolyticus (16 bands), S. hominis (1 band), S. intermedius (1 band), S. lentus (18 bands), S. sciuri (10 bands), and S. warneri (15 bands) (data not shown).
Hybridization to S. aureus chromosomal DNA was at least 10 times stronger than hybridization to that of the other species, although approximately one-third as much S. aureus DNA was loaded on the gel. The single band in S. hominis and S. intermedius may represent cross-hybridization with uvrA-hprK homologues. The probe contained the Tn557 attachment site; however these data suggest that portions of the STAR element may also be present in other members of this genus. Database searches of all the publicly available finished and unfinished genome projects failed to reveal evidence of this element in any organism other than S. aureus.Concluding remarks. With the ever-expanding number of microbial genome sequences available, it is likely that more small multicopy sequences will be identified. The Bacillus subtilis genome project has produced one such 190-bp sequence, present in 10 nonidentical copies in the strain sequenced (8). The genome of Mycobacterium leprae also contains 28 copies of a sequence that shows strain-to-strain variability (3, 15).
We have no evidence for the function of the GC-rich STAR element in S. aureus; however, its ubiquity suggests that it has (or had) an important function in microbial life. The element does not have a defined short sequence that is tandemly repeated a variable number of times, as is the case with many repeating-unit sequences that are currently used for strain identification, nor does it show similarity to known insertion elements. The diversity of sequences at the same locus among S. aureus strains suggests that the element changes quite rapidly in evolutionary terms and might thus be useful as a typing marker for the identification and pedigree analysis of clinical isolates. The presence of multiple STAR loci would greatly expand the specificity and accuracy of any strain analysis.Nucleotide sequence accession numbers. The sequences determined in this study have been submitted to the EMBL, GenBank, and DDBJ nucleotide sequence data libraries under the accession numbers listed in Table 1.
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ACKNOWLEDGMENTS |
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We thank Phuong Lan Huynh and Ulrike Pfitzner for technical assistance.
S.E.C. was supported by NRSA Postdoctoral Fellowship AI09626 from the National Institute of Allergy and Infectious Diseases. This project was supported by the German Bundesministerium für Bildung, Wissenschaft, Forschung und Technologie (DLR: 01KI9751/1) and by the Deutsche Forschungsgemeinschaft (BR 947/3-1).
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FOOTNOTES |
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* Corresponding author. Mailing address: Mikrobielle Genetik, Auf der Morgenstelle 28, Universität Tübingen, D-72076 Tübingen, Germany. Phone: 49 7071 297 4635. Fax: 49 7071 29 46 34. E-mail: sarah.cramton{at}uni-tuebingen.de.
Editor: E. I. Tuomanen
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