Abstract
AbstractIn Nerita picea the proacrosomal granule is formed basally in the early spermatid from one large cisterna of the Golgi body, with which the other Golgi‐derived vesicles fuse. After the proacrosomal granule has attached to the plasma membrane and invaginated to form a cup shape, one cisterna of endoplasmic reticulum inserts into the open end and deposits a granular secretion on the inner surface. Subsequently, the proacrosome migrates along the plasma membrane to the apex of the nucleus, but the Golgi body remains basal, as occurs in other archaeogastropods and also many polychaete annelids. However, the final shape and structure of the acrosome is similar to that of mesogastropods. The annulus attaches the distal centriole to the plasma membrane early in spermiogenesis. The production of the flagellum by the distal centriole not only expands the plasma membrane posteriorly but moves the centriolar complex to the nucleus, causing an invagination of the plasma membrane where it is bound by the annulus. During proacrosome migration, the Golgi body secretes a dense tube around the flagellum, and the mitochondria fuse into two spheres at the base of the nucleus. The nuclear plug that closes off the intranuclear canal until this stage rapidly reorganizes itself into two tubes of material inside the canal. The centrioles continue flagellar production, break away from the annulus, and move deep into the intranuclear canal where they fuse together to form the basal body of the sperm. In the maturing spermatid, the two mitochondria fuse into a single sheath that spirals around the flagellum. The annulus does not migrate posteriorly but remains anterior to the midpiece, which is unusual for a filiform sperm. Spermiogenesis in Nerita picea has features in common with both archaeogastropods and mesogastropods but also has some unique features. These observations lend credence to the idea that the Neritidae are a transitional group between Archaeogastropoda and Mesogastropoda.
Published Version
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