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2 Department of Biological Sciences, Texas Tech University, Lubbock, Texas 79409-3131 USA; 3 Oklahoma Biological Survey and Department of Botany and Microbiology, University of Oklahoma, 770 Van Vleet Oval, Norman, Oklahoma 73019-6131 USA; and 4 Samuel Roberts Noble Microscopy Laboratory, University of Oklahoma, Norman, Oklahoma 73019-6131 USA
Received for publication November 9, 1999. Accepted for publication February 10, 2000.
| ABSTRACT |
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Key Words: cavea Compositae ektexine endexine foot layer Haplopappus internal foramina mutant pollen
| INTRODUCTION |
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As with many other Astereae, normal H. gracilis pollen has a surface of conspicuous densely packed spines, while the mutant surface is spineless, covered instead with randomly dispersed angular and globular fragments. A particular plant produces either normal or mutant pollen but not both, and the distinction between the two types is easily recognized at low power (125x) of a compound microscope. Because of the ease of phenotypic recognition and the small number of chromosomes (Jackson, 1957
), this mutation will be useful for future genetic analyses designed to locate additional markers on the two linkage groups of the species as described by Jackson (1964)
.
Our objectives were to characterize and compare normal and mutant pollen wall ultrastructural differences by scanning and transmission electron microscopy (SEM and TEM) and to determine the inheritance pattern of the mutant trait. Our results should encourage further studies of pollen wall variation within and among populations and lead to a better understanding of pollen wall evolution in the Compositae. One future question to be answered is whether different pollen wall structures within the family are due to single gene or to quantitative effects.
| MATERIALS AND METHODS |
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1015 mm long were transplanted to hot-water-expanded Jiffy-7 peat pots (Jiffy Products Ltd., Norway) in white plastic dishpans, covered with clear plastic with aeration under light for 3 d, and then grown with small amounts of water without the cover under artificial light until roots were visible. The peat pots were then transferred to 8-inch soil-filled pots and the plants grown in a greenhouse until maturity.
Mutant source
Most plants from population No. 8208 seeds had normal pollen with spines (Fig. 1), but a spineless pollen mutant (Fig. 2) was isolated, propagated by further crosses, and used in the hybridization program.
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Monohybrid crosses were made between spineless pollen plants from No. 8208 and spined pollen plants from No. 8222. F1 hybrids were intercrossed to produce 46 F2 seedlings.
Dihybrid crosses were made later between plants with spineless pollen and normal stems and those with normal (spined) pollen and fasciated stems. The fasciated gene is recessive as analyzed by Mangum (1992)
and was localized to chromosome A (linkage group 1).
Electron microscopy
Buds from mutant and wild-type plants were divided into two portions. One portion was immersed in 2.5% glutaraldehyde with 0.2 mol/L cacodylate buffer (pH 7.2). Softened anthers were then sliced open, and loose pollen was washed in cacodylate buffer to remove the glutaraldehyde. The other portion was acetolyzed (Erdtman, 1960
). Both samples were cleaned of detritus by sucrose density gradient sedimentation (Chissoe and Skvarla, 1974
). For SEM, acetolyzed and nonacetolyzed pollen grains were divided into two groups. Whole pollen grains were examined either by drying with hexamethyldisilazane (HMDS; Chissoe, Vezey, and Skvarla, 1994
), mounting on specimen stubs and sputter coating with gold; or by drying and made electrically conductive using the osmium-thiocarbohydrazide (OTOTO) method revised by Chissoe, Vezey, and Skvarla (1995)
. Other samples for SEM were frozen on an International Cryostat IEC Model CTR microtome as described elsewhere (Vezey et al., 1994
) and sectioned with a steel knife at a thickness of
20 µm, collected on SEM specimen mounts (JEOL bulk specimen mounts), and sputtered coated with gold. Examination and photography were done with a JEOL-880 SEM equipped with a lanthanum hexaboride gun at 15 kV. For TEM, acetolyzed pollen was stained in cacodylate-buffered 0.5% OsO4 for 2 h, washed in distilled water, dehydrated through ETOH and embedded in araldite-epon resins (Mollenhauer, 1964
). Ultrathin sectioning was accomplished with diamond knives, and sections were retrieved on copper grids and stained with uranyl acetate and lead citrate to improve general contrast. Sections were examined with a JEOL-2000 intermediate-voltage TEM.
Pollen terminology
The terminology used to describe Haplopappus pollen is based on Faegri (1956)
and Iversen and Troels-Smith (1950)
, as adapted to Composite pollen by Skvarla and Larson (1965)
and Skvarla et al. (1977)
. The terminology recognizes two discrete exine layers after acetolysis treatment (Erdtman, 1960
): an outer electron dense complex layer termed ektexine, composed of spines, tectum, columellae and foot layer, and an inner less electron dense single layer, termed endexine.
| RESULTS |
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Dihybrid crosses
Plants homozygous for spineless pollen and normal stems were crossed to those with spined pollen and fasciated stems. The 16 F1 hybrids analyzed had spined pollen and normal stems. Among 88 F2 progeny were 54 spined pollen and normal stems, 17 spined pollen and fasciated stems, 14 spineless pollen and normal stems; three spineless pollen and fasciated stems.
The F2 data give an acceptable fit to a 9:3:3:1 proportion expected for two unlinked traits under simple Mendelian control (
2(3) = 1.94, P = 0.58). For each trait, the F2 progeny also had acceptable fits to monohybrid expectations.
Normal (wild type) pollen
The ektexine in normal H. gracilis pollen has a surface completely ornamented with acute spines
2 µm in height (Fig. 1). Spine tips are supported by basal regions composed of short (<0.1 µm) pillars. The tectum (roof) (<0.25 µm thick) underlying the spines is the distal extension of columellae that are
0.51.5 µm in height (Figs. 14, 17). The basal parts of the columellae are united into an irregular layer ranging from
0.25 to 1.0+ µm in thickness (Figs. 7, 8, 14, 17). Columellae bases in each of the three interapertural regions of the pollen wall are separated from the remainder of the exine by a cavity, termed cavea (Blackmore, van Helvoort, and Punt, 1984
) (Figs. 7, 8, 14). Below each cavea are two exine layers joined as a band (Fig. 14). The upper layer, the foot layer, is part of the ektexine and is the only ektexine layer without internal foramina (Skvarla and Turner, 1966
). At each aperture margin the foot layer connects with columellae bases to give unity to the pollen wall (Figs. 7, 8). The foot layer is considerably narrower than the lower, less electron-dense endexine layer, which is highly lamellate, disrupted, and lacking internal foramina (Fig. 14).
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Ultrathin sections (Figs. 15, 16, 18, 19) show an endexine layer that is highly lamellate and with considerable disruptions at the lower margin. Directly overlying the endexine is a comparatively thicker and slightly more electron-dense ektexine layer that is perforated with abundant internal foramina, which appear to be several tiers in height. Frozen sections (Figs. 10, 12) further support this bilayering of ektexine and endexine. Loosely attached to the upper part of the ektexine layer are the randomly displaced fragments noted above by SEM. All fragments also contain numerous internal foramina (Figs. 15, 16, 18, 19). Internal foramina in the mutant and wild-type pollen grains appear identical (compare enlarged TEMs in Fig. 17 with Figs. 18, 19).
| DISCUSSION |
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These observations suggest that some organizing factor(s) during pollen wall formation were disrupted by the mutation, interfering with proper assembly of the ektexine. Paxson-Sowders, Owens, and Makaroff (1997)
compared pollen wall development in normal and mutant Arabidopsis thaliana pollen in order to follow development of the reticulate pollen wall. They noted that the mutant exine was not differentiated into distinct exine units (see their fig. 18, p. 61), but rather it consisted of a random deposition of unorganized sporopollenin much like that described above for Haplopappus. They suggested that specific stencil or exine receptors to organize the accumulating sporopollenin were absent.
The genetic data show the recessive nature of the spineless mutant gene and indicate a location on chromosome B (linkage group 2). However, this location is not certain because a high recombination frequency approaching 50% between the fasciated and spineless gene on paired homologous chromosomes of linkage group 1 could also yield a good fit to an expected dihybrid ratio.
The spineless mutant that causes such massive disruption of exine development in Haplopappus gracilis indicates its critical importance to pollen wall development, and sequencing its allele could lead to identification of the same gene in related species and other genera. Published data on pollen morphology show numerous fixed taxon differences that undoubtedly are under genetic control, and crosses among interfertile species with such differences could provide useful genetic data. However, population sampling within taxa will more likely provide fertile mutants that could lead to a better understanding of ontogenetic pathways in this critical life cycle stage.
| FOOTNOTES |
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| LITERATURE CITED |
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Wodehouse, R. P. 1930 Pollen grains in the identification and classification of plants V. Haplopappus and other Astereae: the origin of their furrow configuration.Bulletin of the Torrey Botanical Club 57: 2146.[CrossRef]
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