Distribution of Chromomeres As a Basis of Chromosomal Coiling
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J. Cell Sd. 80, 193-205 (1986) 193 Printed in Great Britain © The Company of Biologist! Limited 1986 DISTRIBUTION OF CHROMOMERES AS A BASIS OF CHROMOSOMAL COILING VEIKKO SORSA Department of Genetics, University of Helsinki, Finland SUMMARY Periodicity in the distribution of prominent bands was analysed from the light and electron microscopic maps of salivary gland chromosomes of Drosophila melanogaster. The data obtained indicate that a similar distribution of prominent chromomeres in an individual interphase chromatid results in a unilateral accumulation of chromatin at the chromonema stage, if the helical axis of chromonema consists of ~S-9 interchromomere + chromomere units per turn. Orientation of the largest chromomeres mainly on one lateral half and the smallest chromomeres mairrly on the opposite lateral half of the chromonema apparently bends it to form the chromosomal 'macro* coil. Thus the increase in DNA content in the chromomeric loops located at specific intervals along the chromatids may have an important role in the evolution of coiling hierarchy in the eukaryotic chromosomes. INTRODUCTION At about the same time in the last century as the helical coiling of chromosomes was first depicted by Baranetzky (1880) the polytene chromosomes were also described as striated cords in the cell nuclei of certain insects (Balbiani, 1881). Since then an abundance of reports has been published concerning both the coiling of chromosomes (see e.g. Kaufmann, 1936, 1948; Ris, 1961; Ris & Korenberg, 1979) and the banding pattern in the polytenized interphase chromosomes (see Beermann, 1962). Although chromosomal coiling has been clearly demonstrable by means of light microscopy (LM) (e.g. see Ohnuki, 1968), electron microscopy (EM) of whole mounts has often failed to uncover it, and favoured the folded fibre or radial loop models of mitotic chromosomes instead of coiling hierarchy (DuPraw, 1970; Labhart, Koller & Wunderli, 1982; Utsumi, 1982). Occasionally, coiling has also been detected in whole-mounted chromosomes by means of both transmission EM (e.g. see Colomb & Bahr, 1974; Haapala & Nokkala, 1982) and scanning EM (e.g. see Harrison, Britch, Allen & Harris, 1981; Mullinger & Johnson, 1983). EM of cross-sectioned mitotic chromosomes has strongly supported the radial loop organization of coiled chromosomes (Marsden & Laemmli, 1979; Adolph, 1980a,6) but the existence and nature of the chromosome 'scaffold' (see Earnshaw & Laemmli, 1983) are still disputable (e.g. see Okada & Comings, 1980; Hadlaczky, Praznovsky & Bisztray, 1982; Nasedkina & Slesinger, 1982). Essential contributions in favour of the side loop model of chromatid structure have been the demonstration of the Key words: chromomeres, chromosomal coiling, Drosophila. 194 V. Sorsa lampbrush type of organization in polytene chromosomes (Sorsa, Pusa, Virrankoski & Sorsa, 1970) as well as in the meiotic prophase of insect chromosomes (Keyl, 1975) and the DNA side loops in spread mitotic chromosomes (Paulson & Laemmli, 1977). Axial coiling model of chromosomes The whole light-microscopically recognizable hierarchy of coiling with minor, major and supercoils was depicted by Cleveland (1949) from the chromosomes of flagellates. Many of his drawings give an impression that the coiling hierarchy exists in the axial part of chromosomes. Accordingly, recent advances in the studies on chromosome organization indicate that the coiling of chromatids starts with the formation of an 'axial fibre' to which the chromomeric loops are laterally attached (Nokkala & Nokkala, 19856). The contraction of interchromomeric DNA pulls the adjacent chromomeres more closely together. The tight packaging of chromomeric material, particularly in the largest chromomere loops, bends the laterally located 'axial fibre' to form helical coils, which may then be stabilized by 'scaffolding' proteins (Adolph, Cheng & Laemmli, 1977; Laemmli et al. 1978; Earnshaw & Laemmli, 1983, 1984). By coiling of the axial cord all the chromomeric material is orientated radially outwards from the helical axis. This stage, which obviously corresponds to the 'minor' coil in terminology of Cleveland (1949) is called the 'chromonema' stage by Nokkala & Nokkala (19856). According to the-axial coiling model, the further condensation of chromatin compels the chromonema to form larger helical coiling. This order of coiling is called the chromosomal (macro) coil and it evidently corresponds to the 'major' coil in the terminology of Cleveland (1949). However, it is unclear what makes a coiled chromonema form a higher order of helical structure. One reason could be the unilateral accumulation of chromomeric material on one side of the chromonema, which necessitates further coiling. Apparently, distribution of large chromomeres mainly on one side of the chro- monema makes its structure bilateral and tends to bend it. Unilateral accumulation of large loops in the chromonema stage implies that they should be located at certain intervals along the axial fibre. It means that a corresponding periodicity in location of large chromomeres should be detectable already in the interphase chromatids, and this could be best studied on the polytenized interphase chromosomes. In the present study the periodicity of heavy bands has been analysed from the salivary gland chromosomes of Drosophila melanogaster in which the banding pattern has been mapped most exactly. MATERIALS AND METHODS The sites of the ~S20 most prominent bands, which are usually easily detectable in the photomicrographs of the salivary gland chromosomes 1-3 of D. melanogaster, were determined according to the revised reference maps of Bridges (see Lindsley & Grell, 1968). In the 2L chromosome and in the distal half of the X chromosome the sites of prominent marker bands were also localized with the EM maps (Sorsa, 1982, 1984; Sorsa, Saura & Heino, 1983). The average Chromomeres and chromosomal coiling 195 intervals between the marker bands (or doublets or band complexes) were determined as inter- band + band units. Presuming that the intervals of prominent bands in polytenized interphase chromosomes also represent the intervals of prominent chromomeres in the individual interphase chromatids, the results were tested against the concept of axial coiling hierarchy of chromosomes. The axial coiling model of chromosomes has been strongly supported by the recent results of Nokkala & Nokkala (1985a,6). RESULTS AND DISCUSSION When compiling the reference maps of the salivary gland chromosomes of D. melanogaster, C. B. Bridges already noticed that there are more prominent bands at certain rather regular intervals along the polytene chromosomes. Bridges (1935) utilized this special distribution of distinct bands by using them as border-lines of divisions and subdivisions in his guide maps of the salivary gland chromosomes of D. melanogaster. The distribution of heavy bands is also clear in the photographic maps of Lefevre (1976). A comparison of the photo map of Lefevre with the revised camera lucida maps of Bridges (Lindsley & Grell, 1968) and with the electron microscopic maps (Sorsa, 1982, 1984) shows that many of the heavy bands in the photo maps are actually formed by groups of closely adjacent bands. In terms of the polyteny hypothesis this implies that also in every individual interphase chromatid the large chromomeres and groups of them are located at similar intervals as shown by the banding pattern in the polytenized interphase chromosomes. To study the distribution of prominent bands shown by the photomicrographs of salivary gland chromosomes of D. melanogaster, the sites of those bands were marked on the revised reference maps of Bridges and on the EM maps. The average distances of marker bands were determined as interband (+band) units (i.b. units). Distribution of prominent bands in the polytene chromosomes of D. melanogaster The total axial length of the salivary gland chromosomes X, 2 and 3 of D. melanogaster is ~2173 ^m according to the revised reference maps of Bridges. This length is approximately 4*5 % of the total DNA length of the D. melanogaster genome, which is estimated to be ~47-6mm (Laird, 1971). The number of prominent bands, which can usually be recognized in the light micrographs of chromosomes X, 2 and 3 is approximately 520. The total number of i.b. units in the chromosomes X, 2 and 3 is —-5010 according to the revised reference maps (see Lindsley & Grell, 1968) giving on average —9-6 i.b. units per prominent marker band. If the short interbands in between the halves of the doublet bands of Bridges are excluded, the respective numbers are —3695 and ~7 i.b. units. The number of i.b. units in regions between the marker bands varies from 2 to ~20. Correspondingly, there are in a single chromatid of polytene chromosome 2-20 interchromomere + chromomere units (i.e. units) between the same prominent markers. According to the axial coiling model a marker chromomere and its adjacent region consisting of a certain number of i.e. units correspond to a complete turn of 196 V. Sorsa Table 1. Distance of prominent light-microscopic marker bands according to the revised reference maps of Bridges given as the average number of i.b. units Average distance of Chromosome markers (i.b. units) S.D. (x) X(l) 6-9 2-08 2L 7-1 1-94 2R(2) 7-4 1-98 3L 6-8 1-98 3R(3) 7-5 1-92 Means for (1W3) 714 1-98 The regions of salivary gland chromosomes between the marker bands are proposed to correspond to chromonemal coils in mitotic chromosomes of D. melanogaster. The intervals of the prominent