MBE Advance Access originally published online on September 21, 2005
Molecular Biology and Evolution 2006 23(1):189-202; doi:10.1093/molbev/msj022
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Research Article |
Molecular Evolution of Minisatellites in Hemiascomycetous Yeasts
Unité de Génétique Moléculaire des Levures, Université Pierre et Marie Curie, Institut Pasteur, 75724 Paris Cedex 15, France
E-mail: gfrichar{at}pasteur.fr.
| Abstract |
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Minisatellites are DNA tandem repeats exhibiting size polymorphism among individuals of a population. This polymorphism is generated by two different mechanisms, both in human and yeast cells, "replication slippage" during S-phase DNA synthesis and "repair slippage" associated to meiotic gene conversion. The Saccharomyces cerevisiae genome contains numerous natural minisatellites. They are located on all chromosomes without any obvious distribution bias. Minisatellites found in protein-coding genes have longer repeat units and on the average more repeat units than minisatellites in noncoding regions. They show an excess of cytosines on the coding strand, as compared to guanines (negative GC skew). They are always multiples of three, encode serine- and threonine-rich amino acid repeats, and are found preferably within genes encoding cell wall proteins, suggesting that they are positively selected in this particular class of genes. Genome-wide, there is no statistically significant association between minisatellites and meiotic recombination hot spots. In addition, minisatellites that are located in the vicinity of a meiotic hot spot are not more polymorphic than minisatellites located far from any hot spot. This suggests that minisatellites, in S. cerevisiae, evolve probably by strand slippage during replication or mitotic recombination. Finally, evolution of minisatellites among hemiascomycetous yeasts shows that even though many minisatellite-containing genes are conserved, most of the time the minisatellite itself is not conserved. The diversity of minisatellite sequences found in orthologous genes of different species suggests that minisatellites are differentially acquired and lost during evolution of hemiascomycetous yeasts at a pace faster than the genes containing them.
Key Words: minisatellite replication slippage meiotic hot spot GC skew yeast
| Introduction |
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Repetitive elements are a common feature of all prokaryotic and eukaryotic genomes. They can be classified in two categories: dispersed repeat elements (transposons, tRNAs, paralogous protein encoding genes, etc.) and tandem repeat elements. Micro- and minisatellites are tandem repeat arrays whose unit sizes range from a few nucleotides for the former to more than 10 bp for the latter (Charlesworth, Sniegowski, and Stephan 1994
One of the most intriguing question concerning tandem repeat sequences in general and minisatellites in particular is their very origin. Are minisatellites initially created by S-phase replication slippage or by homologous recombination when located by chance near a meiotic hot spot? To address this question, we performed an in silico analysis of the completely sequenced S. cerevisiae genome, looking for minisatellites. To our surprise, we found a large number of such elements, most of them never described before in the literature. Most of the time, they are located within genes exhibiting a negative GC skew (more cytosines than guanines on the coding strand) and are themselves more skewed than their containing genes. Very often, short flanking repeats are found upstream and downstream of minisatellites. No positive correlation was found between the location of minisatellites and the distribution of meiotic hot spots in the yeast genome. Altogether, these data suggest that, in S. cerevisiae, natural minisatellites are acquired and lost by a molecular mechanism independent of meiotic recombination, and probably involving replication slippage between short flanking sequences, in genes exhibiting a strong bias for cytosines on the coding strand.
| Materials and Methods |
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Analysis of the S. cerevisiae Genome
We ran the program MREPS (Kolpakov, Bana, and Kucherov 2003
In addition, some minisatellites, corresponding in fact to imperfect microsatellites (Richard and Dujon 1996
), were detected by the program but not taken into account thereafter. Using this approach, MREPS detected 257 repeats fulfilling the required criteria. After careful examination, some of the repeats found by the program were partially overlapping or were part of the same minisatellite, resulting in a final number of 84 minisatellites used for the present analysis.
GC skews were calculated as (G C/G + C), using DNA Strider 1.4f6 (Marck 1988
). Windows of 100 bp were used for the calculation. Both GC content and GC skew of minisatellite-containing genes were calculated on the gene DNA sequence without the minisatellite. Functional annotations are based on Gene Ontology annotations retrieved from the Saccharomyces Genome Database.
Search for Orthologues in Hemiascomycetous Yeasts
The Saccharomyces paradoxus orthologues of S. cerevisiae genes were retrieved from the Saccharomyces Genome Database (ftp://genome-ftp.stanford.edu/yeast/data_download/sequence/fungal_genomes/S_paradoxus/). For Candida glabrata, Kluyveromyces lactis, Debaryomyces hansenii, and Yarrowia lipolytica, we started from protein families built from sequence similarities during Génolevures 2 (Dujon et al. 2004
). For families containing only one gene per sequenced species (1:1:1:1:1 relationship), we considered that this gene was the direct orthologue of the S. cerevisiae gene. For other gene families, when orthologues could not be chosen among paralogues based on sequence similarity, synteny conservation was used, whenever possible, to determine the correct orthologue. Most of the time, synteny did not help to find the correct orthologue, and these genes were, therefore, tagged as "family" ("fam." in table 5). Finally, for S. cerevisiae genes without orthologues by the former approach, we performed BlastP searches, using as a query the S. cerevisiae gene, in the Génolevures database (http://cbi.labri.fr/Genolevures). The best match was in turn used as a query in a BlastP search against the S. cerevisiae genome. Positive bidirectional best hits were validated as real S. cerevisiae orthologues (22 orthologues found using this approach).
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Polymerase Chain Reaction Analysis of Minisatellite Polymorphism
Specific primers were designed to amplify polymerase chain reaction (PCR) fragments of 212 bp (SNF11), 254 bp (PRY2), 315 bp (BUD27), 209 bp (DSN1), 192 bp (SCW11), 292 bp (YKL105c), 321 bp (YOL155c), or 148 bp (NIS1). Primer sequences are available on request. The PCR program used was 95°C for 15 s, 60°C for 1 min, 72°C for 30 s (30 cycles), and a final extension step at 72°C for 10 min. A sample was loaded on a 3% Metaphor agarose gel (TEBU, Le Perray en Yvelines Cedex, France) with 100-bp ladder as a size marker (Eurogentec, Seraing, Belgium). The gel was run overnight at 1 V/cm in 1x TBE. Origin of the different yeast strains used can be found in Richard and Dujon (1996)
| Results |
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Distribution of Minisatellites in the S. cerevisiae Genome
We performed a systematic search of minisatellites in the S. cerevisiae genome using the MREPS sofware (Kolpakov, Bana, and Kucherov 2003
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Interestingly, minisatellite-containing genes tend to show, on the average, a higher GC content (44 ± 0.5%) than other yeast genes (ca. 39%, Dujon 1996
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Human minisatellites are not perfect tandem repeats but a succession of variant repeats, differing from each other by one or more nucleotides. This polymorphism was used to rapidly determine their exact sequence by minisatellite variant repeats mapping (Jeffreys, Neumann, and Wilson 1990
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Minisatellites located in the subtelomeric Y' elements are made of a 36-bp repeat unit, as previously described (Horowitz and Haber 1984
Among the 49 minisatellite-containing genes, it is striking to note that half of them (25 out of 49) are involved in cell wall organization. Among them, a majority encode proteins that are covalently associated to cell wall polysaccharides (FLO9, FLO1, TIP1, TIR1, FLO5, FLO11, PIR2, DAN1, PIR1, and PIR3). A few others are involved in processes such as cell division, budding, transcription, or RNA processing (table 3). Some of these proteins were known to contain internal amino acid repeats (Klis et al. 2002
). However, at the DNA level, they do not necessarily contain a recognizable minisatellite. For example, the PIR family (for protein with internal repeats) contains four members (PIR14), but only PIR1, PIR2, and PIR3 contain a minisatellite and the fourth member, PIR4, contains a degenerate repeat that does not fulfill our criteria (see Materials and Methods). Among the 25 cell wall genes, 19 are known or predicted to encode a glycosyl-phosphatidylinositol domain (GPI), involved in anchoring the protein to the plasma membrane (Caro et al. 1997
; Hagen et al. 2004
). GPIs are always located very close to the C-terminal part of the protein (except in the case of FLO9). Minisatellite location is apparently less constrained and corresponds to the first two-thirds of the protein. The average distance of the GPI from the 3' part of the gene (if one excludes FLO9) is 69 ± 1 bp, whereas the average distance of the minisatellite from the 3' part of the gene is 1417 ± 291 bp.
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Among amino acids encoded by minisatellites, serine and threonine are the most abundant, representing together 42% of the total (table 4). Among them, minisatellite-containing genes encoding cell wall proteins contain more Ser and Thr residues than other proteins. On the average, cell wall protein repeats contain 59% of Ser + Thr residues, whereas other classes of minisatellite-containing proteins contain from 13% to 26% of Ser + Thr. The second most frequent amino acids encoded by minisatellites are alanine (9%), glutamic acid (7%), and valine (7%). Each of the other amino acids is found only one to five percent of the time. This is very different from what was observed for genes encoding trinucleotide repeats (a particular class of microsatellites) in which glutamine, asparagine, glutamic acid, and aspartic acid are the four most common amino acids encoded by these repeats, and genes containing these repeats are mostly transcription factors (Richard and Dujon 1996
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Note that some repeat sequences are similar (FLO1, FLO5, and FLO9 or PIR1 and PIR2) and may have arisen by gene conversion.
Meiotic Hot Spots and Minisatellites
It was previously shown in man and yeast that minisatellites located near a meiotic hot spot expand and contract at a high frequency during meiosis (Appelgren, Cederberg, and Rannug 1997
; Jeffreys, Murray, and Neumann 1998
; Debrauwère et al. 1999
). We asked whether minisatellites were close to meiotic hot spots, defined from whole-genome analyses of meiotic DSB sites (Gerton et al. 2000
; Borde et al. 2004
). In S. cerevisiae, meiotic gene conversion tracts are rather limited in size (12 kb) (reviewed in Pâques and Haber 1999
). We found two minisatellites within 2 kb from a meiotic hot spot (SNF11 and PRY2; fig. 1) and four others within 5 kb of a hot spot (FLO9, RPL34B, DSN1, BBC1; fig. 1). Given the numbers of hot spots and minisatellites in the yeast genome, a random distribution would generate, respectively, two minisatellites within 2 kb of a hot spot and five within 5 kb, which is not different from what we found. We therefore rejected the hypothesis that minisatellites are associated to meiotic hot spots more often than randomly expected.
Minisatellite Size Polymorphism Among Different Yeast Strains
We previously demonstrated microsatellite size polymorphism among laboratory or industrial yeast strains or strains isolated from infected patients (Richard and Dujon 1996
; Hennequin et al. 2001
). This size polymorphism was used to classify the strains studied and could be used as a typing method to find their origin. In order to determine to what extent natural yeast minisatellites were also polymorphic, we selected eight independent laboratory haploid yeast strains, based on the uniqueness of their microsatellite haplotype (Richard and Dujon 1996
) and studied eight minisatellite loci. Four were chosen within 2 or 5 kb of a meiotic hot spot (SNF11, BUD27, PRY2, and DSN1; fig. 1). The other four were selected so that their unit size and unit number were as similar to the first four as possible and so that they were not close to a hot spot. Unique primers were designed to PCR amplify the eight minisatellites in each strain, strain FYBL1-8B (a derivative of the S288C sequenced strain) being used as the reference. Six out of the eight minisatellites exhibited size polymorphism (only SCW11 and PRY2 minisatellites did not) (fig. 5). We were able to assign each strain to a specific unique haplotype because we did not find two strains with the same haplotype. Interestingly, the HC9-7 strain exhibited three different bands at the NIS1 locus, on chromosome XIV. In the other strains, amplification of this minisatellite was very specific because it amplified only one band. The HC9-7 strain also showed two different alleles of a microsatellite located on chromosome XI in a former study (Richard and Dujon 1996
). Therefore, there must be some aneuploidy (or segmental duplications) in this particular strain.
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We did not find any difference in the degree of polymorphism of minisatellites located near meiotic hot spots or far from them. In both cases, three minisatellites out of four showed some level of polyphormism (fig. 5). The number of different alleles for a given minisatellite is not correlated to the presence of a hot spot either. We therefore concluded that minisatellite stability in these different laboratory strains did not depend on the presence of a near meiotic hot spot.
Conservation of Minisatellites in Hemiascomycetous Yeasts
In order to estimate minisatellite conservation during evolution, we investigated other hemiascomycetous yeast genomes (fig. 6). Saccharomyces paradoxus is a Saccharomyces sensu stricto, very close to S. cerevisiae. Candida glabrata is a pathogenic yeast, a causative agent of human candidiasis (Bennett, Izumikawa, and Marr 2004
). Kluyveromyces lactis is also related to S. cerevisiae and has been used for genetic studies or industrial applications (Bolotin-Fukuhara et al. 2000
). Debaryomyces hansenii is a halotolerant yeast, phylogenetically close to the pathogen Candida albicans (Lépingle et al. 2000
). Yarrowia lipolytica is a more distantly related yeast, able to grow as individual cells or as a mycelium (Casarégola et al. 2000
). The evolutionary distance between S. cerevisiae and Y. lipolytica, measured as the amino acid divergence between orthologous proteins, is larger than the entire phylum of Chordates (Dujon et al. 2004
).
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In the closest species, S. paradoxus, we found one orthologue for each of the 49 S. cerevisiae minisatellite-containing genes. In 73% of the cases (36 out of 55 minisatellites), a minisatellite was also found in the S. paradoxus gene (table 5). Except in 8 cases out of 36, the motif unit has the same size as in S. cerevisiae. In one case (MF(alpha)1), the minisatellite is not detectable at the DNA level anymore, although the protein repeat is still present. We called it a "minisatellite relic" as a reminiscence of the term "gene relic" used to describe very degenerate genes found in the genomes of hemiascomycetous yeasts (Lafontaine et al. 2004
We subsequently looked for minisatellite conservation in the four other species. Finding orthologues of S. cerevisiae genes was more challenging, even in the second closest species, C. glabrata, because many of the minisatellite-containing genes belong to gene families containing from 2 to 65 paralogous members (table 5). Most of the time, we could not use the synteny data to choose among several homologues because synteny breakpoints are frequent in regions containing dispersed repeated elements, like retrotransposons or gene families (Fischer et al. 2000
, 2001
). As expected, minisatellite-containing genes were easier to identify in C. glabrata and K. lactis, as compared to the more distant D. hansenii and Y. lipolytica. However, we more often found a minisatellite in Y. lipolytica (8 minisatellites out of 17 conserved genes, chi-square test: P = 0.05) than in C. glabrata, K. lactis, or D. hansenii (table 5). Also, three minisatellite relics are found in C. glabrata, K. lactis, and D. hanseni and none in Y. lipolytica. When minisatellite sequences were compared, most of the time their sequence was found to be different between S. cerevisiae and the other hemiascomycetous yeast species. Sequence alignments showed that in 25% of the cases accumulation of point mutations "erased" the minisatellite, in 25% there was a complete deletion of the minisatellite although the protein sequence is conserved upstream and downstream of it, and in the remaining cases (50%) a mix of point mutations and small deletions led to the loss of the minisatellite. The kind of mutational events encountered is reminiscent of what was observed for microsatellites in different yeast species (Malpertuy, Dujon, and Richard 2003
). In S. paradoxus, 23 minisatellite sequences are conserved, whereas in other species, only 2 sequences in C. glabrata, K. lactis, and D. hansenii and 1 sequence in Y. lipolytica are conserved. Note that the only minisatellite whose repeat motif is conserved in all species in which it is found is the RPO21 minisatellite. This minisatellite is split in two minisatellites in baker's yeast, separated by only 9 nt, whereas in the other species there is only one minisatellite covering the same region of the gene.
In conclusion, when a minisatellite is found in a yeast species, its sequence is most of the time different from the S. cerevisiae sequence, although it is located at the same position within the gene. A striking example is the case of the PRY2 minisatellite, present in three species and only found as a relic in D. hansenii (fig. 6A). Protein sequence alignment shows that the repeat unit is different in the four species in which it is found (fig. 6B). This raises the intriguing question of the origin of this minisatellite. Either there was a minisatellite in the common ancestor of the PRY2 gene and it diverged rapidly in all species or each species acquired independently a different minisatellite in the same gene, suggesting that some genes might be preferential targets for minisatellite formation.
| Discussion |
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In the present work, we report the first comprehensive analysis of minisatellites in the genome of a completely sequenced organism. To the best of our knowledge, although numerous papers describing microsatellites in eukaryotic and prokaryotic genomes have been published (Richard and Dujon 1997
It was surprising to find a strong negative GC skew in minisatellites and in their associated genes. We investigated whether it was linked to amino acid composition and/or to codon usage bias because it was shown that biased base composition in CAG repeat containing genes in human and mouse were due to their unusual amino acid content (Hancock, Worthey, and Santibañez-Koref 2001
). Among the six possible serine codons, TCT is overrepresented and AGT underrepresented, and among the four possible threonine codons, ACT and ACC are overrepresented and ACA and ACG are underrepresented in minisatellites. This could be the basis for the GC skew observed in some cases but not all because 5 minisatellites exhibit a (Ser + Thr) composition higher than 50% and no skew (DAN1, FLO10, CTS1, YMR317w, and TIR4; tables 1 and 4), whereas 10 minisatellites exhibit a (Ser + Thr) composition lower than 50% and a negative GC skew (FLO9, FLO1, FLO5, PAN1, BBC1, PIR1, PIR3, DDR48 [both repeats], and FIT3; tables 1 and 4). Many circular bacterial chromosomes exhibit a strong GC skew with guanines more abundant on the leading strand of DNA replication, on each side of the replication origin (Lobry 1996
). In addition, an opposite GC skew (cytosines > guanines) was recently described around the transcription start site of Arabidopsis thaliana and Oryza sativa (rice) genes. Some fungal genomes (but not S. cerevisiae) show the same bias around their transcription initiation regions (Fujimori, Washio, and Tomita 2005
). But so far, no such compositional bias was described in S. cerevisiae. No other significant skew was found in the minisatellites described here, so it is specifically an overrepresentation of cytosines in the gene-coding strand. No obvious correlation was found between minisatellite locations and replication profiles of yeast chromosomes (Raghuraman et al. 2001
) because out of 33 minisatellites exhibiting a negative GC skew (table 1), 18 are predicted to be replicated on the leading strand and 15 on the lagging strand during S-phase replication. Finally, no significant association of minisatellites with replication origins was found.
Possible Molecular Mechanisms Propagating Minisatellites
Despite earlier observations of minisatellite instability due to the presence of a nearby meiotic hot spot, we found no preferential association of minisatellites with them and no greater polymorphism for those near a hot spot, suggesting that in S. cerevisiae, minisatellites mainly evolve independently of such hot spots. However, it was recently shown that meiotic hot spots are, for their most part, not conserved between humans and chimpanzees, despite 99% conservation of the DNA sequence between these two species (Winckler et al. 2005
). Therefore, we cannot rule out that the minisatellites we found, originally arose near ancient meiotic hot spots that have since disappeared. A possible mechanism to explain minisatellite origin in yeast was proposed by Haber and Louis (1998)
. They observed that the Y' minisatellite, a Saccharomyces carlbergensis minisatellite, and several human minisatellites are flanked by two short identical sequences. They speculated that an initial duplication event, resulting from replication slippage between these two short sequences, was responsible for the birth of the minisatellite, followed in next generations by unequal crossing-over between sister chromatids or again, replication slippage leading to minisatellite expansion. Examination of sequences flanking the 55 S. cerevisiae minisatellites found in genes confirm and extend this finding. We found such short identical sequences for 49 minisatellites; we could not detect such sequences only for NUM1, DSN1, CTS1, CHS5, and one of the two minisatellites in RPO21 and FLO11 (table 6). The average size between the end of the minisatellite and the downstream short sequence is 27 ± 6 nt (fig. 4). These flanking repeats are trimers (3 cases out of 49), tetramers (15 cases), pentamers (20 cases), hexamers (4 cases), or heptamers or more (7 cases). Pentamers were also found flanking the 18 occurences of the Y' minisatellite. The reason why pentamers are more frequent, as compared to other repeat sizes, is unknown.
Rapid Evolution of Minisatellites
In a former study, it was shown that microsatellites evolved rapidly among several hemiascomycetous yeast genomes (Malpertuy, Dujon, and Richard 2003
). We come to the same conclusion for minisatellites. Although a minisatellite-containing gene is conserved, its minisatellite is not necessarily conserved, and most of the time its sequence is divergent from the S. cerevisiae sequence (table 5 and fig. 6). Analysis of the completely sequenced genomes of the hemiascomycetes studied here, using criteria similar to the present study, shows that they all contain numerous minisatellites, in proportions comparable to what was found in S. cerevisiae (data not shown). This observation implies that each species contains minisatellites that are absent from the S. cerevisiae genome, suggesting that each species has a specific subset of minisatellites that are not shared by the others. Hence, there must be molecular mechanisms responsible for de novo creation of minisatellites, as suggested before for microsatellites (Malpertuy, Dujon, and Richard 2003
).
Birth, Life, and Death of Minisatellites: A Model
We propose that initial formation of a minisatellite requires a negatively GC-skewed DNA region; hence, it has more chance to occur in genes that naturally exhibit this negative skew. Birth requires slippage (probably occuring during DNA replication) between two short repeats flanking the region that will be duplicated, as originally proposed by Haber and Louis (1998)
. After the initial duplication event, the minisatellite can be amplified by different mechanisms, including slippage during replication, mitotic recombination, or meiotic gene conversion. Replication errors can introduce point mutations into a given unit that will eventually lead to correction or propagation of the mutation by gene conversion. If too many mutations accumulate in a minisatellite, repeat size change cannot occur anymore because the repeat units are too divergent to promote slippage during replication or recombination (Pâques, Richard, and Haber 2001
). From then on, the minisatellite will accumulate more point mutations, eventually erasing the repeats.
Toward a Biological Definition of Tandem Repeat Sequences
Finally, we want to point out that the frontier between micro- and minisatellites varies a lot in the literature, depending on authors. The present work allows us to propose a biological definition of these two genetic objects. In S. cerevisiae, mono- to hexanucleotide repeats are found (Richard et al. 1999
), and trinucleotide repeats (a particular class of microsatellites) are mainly found in nuclear genes, often encoding transcription factors (Richard and Dujon 1996
; Alba, Santibañez-Koref, and Hancock 1999
; Young, Sloan, and Van Riper 2000
; Malpertuy, Dujon, and Richard 2003
), whereas minisatellites are mainly found in cell wall genes, as shown by the present study. The shortest repeat size of a minisatellite found in S. cerevisiae was 12 nt long, but 9-nt-long repeat units were found in S. paradoxus (PAN1 and BBC1). We therefore propose that the frontier between micro- and minisatellites be set at 9 nt, defining two classes of tandem repeat sequences, short tandem repeats found in transcription factors and longer ones in cell wall genes.
| Note Added in Proof |
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A recent work by G. Fink and colleagues also show that minisatellites are frequently found in cell wall genes (Verstrepen et al. 2005
| Acknowledgements |
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We thank our colleagues, especially C. Fairhead, B. Llorente, and J.-P. Latgé, for fruitful discussions and advices, H. Muller, C. Hennequin, and G. Fischer for sharing unpublished results, and two anonymous reviewers for helpful comments. B.D. is a member of the Institut Universitaire de France.
| Footnotes |
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Edward Holmes, Associate Editor
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