Lectin histochemistry of the hyaline layer in the asteroid,pisaster ochraceus

Synthesis and secretion of molecules exhibiting the HL1 epitope during development of the hyaline layer of the asteroid Pisaster ochraceus

A complex ECM layer called the hyaline layer (HL) surrounds embryos and larvae of the starfish Pisaster ochraceus. When preserved by freeze substitution, the HL of a bipinnaria larva consists of six sublayers. From the plasmalemma outwards these are the intervillous layer (iv), the H3, H2, H1 sublayers that make up the supporting layer, a boundary layer (b) and the coarse outer meshwork (cm). HL development begins at fertilization when exocytosis of the cortical granules releases ECM into the perivitelline space and elevates the fertilization membrane. Over the course of early development the layers are added in a sequential manner and by hatching the embryo is surrounded by a thin HL containing most if not all of the layers. The layers thicken over the next few days. By the bipinnaria stage the larvae are surrounded by a thick six-layered HL. HL1 is a monoclonal antibody that reacts against an epitope found in all regions of the HL of the bipinnaria larva except the H2 sublayer. Western blots show that it is present on several molecules during HL development. The number and pattern of the HL1-labeled molecules change during development, suggesting that either new molecules are being produced or that some molecules are precursors of others. Light (immunofluorescence) and TEM (immunogold) studies using HL1 in the early stages of development show that HL1-positive material is not present in the corticle granules and that it only begins to be manufactured and secreted in quantity in the blastula stage at 18-20 h. Following this it continues to be secreted at least as far as the bipinnaria stage. Molecules containing the HL1 antigen therefore do not appear to play a major role in early development of the HL but are necessary for later events. The results suggest that, like the sea urchin HL, the starfish HL undergoes a sequential organization of the different HL layers from ECM components, which are released into the perivitelline space.

Ultrastructural aspects of the development of the hyaline layer and extracellular matrix lining the gastrointestinal tract in embryos and larvae of the starfish Pisaster ochraceus preserved by freeze substitution

Embryos and larvae of the starfish Pisaster ochraceus are surrounded by a complex extracellular matrix (ECM) layer called the hyaline layer (HL). A similar but less well-organized ECM layer lines some regions of the larval gut. Examination of material preserved by freeze substitution shows that the HL consists of a coarse outer meshwork, a boundary layer, a supporting layer, which is divided into three sublayers, H1, H2, and H3, and an intervillus layer. The development of the HL has been studied in material preserved by freeze substitution. Development begins at fertilization when exocytosis of the cortical granules releases ECM into the perivitelline space and elevates the fertilization membrane. Shortly after, plaques of dense material with attached fibers are present on the outer surface of the egg plasmalemma. Following this, these plaques and fibers are associated with the tips of short microvilli, suggesting that they may induce microvillus formation. Next, the tips of some of the microvilli are joined by short regions of the H1 sublayer. Some of these H1 regions have short segments of boundary layer material associated with their outer surfaces while others are naked. Just prior to hatching, the H1 and boundary layers completely surround the embryo, separating the developing coarse meshwork and intervillus layers. Short segments of the H2 and H3 sublayers are also present. Posthatching, the microvilli and all HL layers increase in thickness and density, particularly the H2, boundary, and coarse outer meshwork layers. The results suggest a sequential organization of HL components from ECM that is secreted into the perivitelline space.

Localization and partial characterization of a molecule found in the plasma membrane of starfish and sea urchin embryos using a novel monoclonal antibody

A monoclonal antibody, P212, has been developed which reacts against 120 kD and 90 kD proteins, P212 antigens found in the plasma membranes of both starfish and sea urchin embryos. Immunocytochemical studies with colloidal gold tagged P212 showed that the P212 antigens are also found on the inner membranes of several different types of granules and vesicles located in the eggs and cytoplasm of embryonic cells, and in the trans region of the Golgi apparatus. One or both of the P212 antigens are also found in the cortical granules, granules which are exocytosed at fertilization. They are not found on intracellular membrane structures such as the rough endoplasmic reticulum, the nuclear membrane, or a number of deeper granular structures. The P212 antigens are probably located on the membranes of vesicles which are on the exocytosis-endocytosis pathway and may be involved in cell trafficking.

Lectin histochemistry of the hyaline layer around the larvae of Patiriella species (Asteroidea) with different developmental modes

Larvae of sea stars are surrounded by an extracellular matrix called the hyaline layer. The lectin-binding properties of this matrix were investigated in an ultrastructural study of Patiriella species having different modes of development. The planktonic bipinnaria and brachiolaria of P. regularis and the planktonic brachiolaria of P. calcar demonstrated the same labeling of the hyaline layer for three lectins: Con A, SBA, and WGA. In both species the outer coarse meshwork stained for all three lectins, whereas the intervillous layer displayed patchy labeling. In the benthic brachiolaria of P. exigua, the outer coarse meshwork displayed heavy labeling for all three lectins. The heavy labeling of the outer coarse meshwork of P. exigua compared with that of the other species suggests an increased number of lectin binding sites in the hyaline layer of this species. The similar ultrastructure and histochemistry of the hyaline layer of P. regularis and P. calcar may reflect similar requirements of their extracellular cover in their planktonic environment. Lectin labeling shows that hypertrophy of the hyaline layer of P. exigua, in particular the outer coarse meshwork, involves elaboration of the carbohydrate composition of the matrix. Modifications seen in the ultrastructure and histochemistry of the hyaline layer of P. exigua appear to be associated with the evolution of benthic development.

Basement membrane lectin binding sites are decreased in the esophageal endoderm during the arrival of presumptive muscle mesenchyme in the developing asteroid Pisaster ochraceus

Basement membranes (BMs) of vertebrates and invertebrates have been shown to contain glycoproteins and proteoglycans, which include oligosaccharides and glycosaminoglycans. Lectin binding sites were characterized in the BM of gastrulating embryos of the starfish, Pisaster ochraceus. In early and mid-gastrulae, the fluorescein isothiocyanate (FITC)-lectin conjugates of concanavalin A (Con A) and wheat germ agglutinin (WGA) reveal the presence of mannose/glucose and glucosamine/sialic acid residues in the BM of all regions of the embryos. However, in the late gastrula embryo, an apparent reduction of these components is observed over the esophageal BM. Ultrastructural studies using the lectin-gold conjugates Con A, Limax flavus agglutinin (LFA), specific for sialic acid, and Dolichos biflorus agglutinin (DBA), specific for galactosamine, demonstrate that most mannose/glucose and galactosamine-containing residues lie in the lamina densa, whereas most sialic acid residues are located over the lamina lucida. In addition, a statistical analysis of lectin binding in the late gastrula embryo reveals that the amount of labelling with both Con A and LFA is significantly reduced in the esophageal region, suggesting that mannose/glucose and sialic acid residues are reduced in this region. These results confirm the observations of the FITC-lectin studies described above. They also confirm earlier studies that demonstrated a difference in BM morphology of the esophageal region (Crawford, '88). Mesenchyme cells, some of which arise from the forming coeloms (Crawford, '90), and which may represent a distinct population, colonize exclusively on this esophageal BM, where they later differentiate into muscle. Quantitative differences in BM glycoconjugates may act to direct the presumptive muscle cells to the region of the esophagus.

Ultrastructural study of the hyaline layer of the starfish embryo, Pisaster ochraceus

The hyaline layer (HL) is a multilayered extracellular matrix (ECM) that coats the external surfaces of sea urchin and starfish embryos. It is thought to protect and lubricate the embryo, stabilize the blastomeres during morphogenesis, and regulate nutrient intake. Ultrastructural studies of chemically fixed embryos have shown the HL to consist of two to four sublayers. However, since chemical fixatives may cause collapse and alter the positions and antigenicity of the extracellular components, fixation methods that exclude chemicals may reveal a picture of the HL closer to what is present in vivo. Freeze substitution, a fixation method whereby tissues are rapidly frozen and dehydrated at low temperatures, has proved useful for fixing material rich in ECM. In this study, embryos of the starfish Pisaster ochraceus were fixed for microscopy using freeze substitution and three chemical methods in order to determine, as accurately as possible, the structure of the HL. Embryos appear to be best preserved by freeze substitution and demonstrate a HL consisting of at least six distinct sublayers. Based on staining with anionic dyes, most sublayers appear to contain glycosaminoglycans. Freeze substituted embryos, which were also stained with monoclonal antibodies raised against their ECM, revealed that some molecules are common to all six sublayers, whereas other molecules may be restricted to specific sublayers. This suggests that each sublayer could have a different function. Additional evidence suggests that microvillus associated bodies, present in other marine invertebrate embryos, may anchor the asteroid HL to the cell surface microvilli.