BACTERIA THAT INDUCE MORPHOGENESIS IN ULVA PERTUSA (CHLOROPHYTA) GROWN UNDER AXENIC CONDITIONS1

Marine foliaceous green macroalgae such as Ulva lose their typical morphology when cultured aseptically in defined synthetic media. However, after reinfection by certain marine bacteria (isolated from unialgal cultures of Ulva pertusa Kjellman), the organisms regain their typical foliaceous or tubular morphology. To investigate the morphogenesis (MG) induced in U. pertusa by bacteria, we isolated and identified bacteria with MG activity on U. pertusa and studied the distribution of such bacteria in seawater and on various marine macroalgae. We isolated 1555 bacterial strains from 18 species of marine macroalgae (six Chlorophyta, five Phaeophyta, and seven Rhodophyta), from seawater and from sediment collected at the beach at Omaezaki, Shizuoka Prefecture; Japan. Of these, 676 bacterial strains (43.5%) showed MG activity. They were classified into six bacterial groups, Flavobacterium, Vibrio, Pseudomonas, Deleya, Escherichia, and gram-positive cocci. These bacteria were ubiquitous among the samples and were not specific to U. pertusa. Several plant growth regulators had no MG activity. Filter-sterilized supernatants of culture media of MG-active bacteria strains did not induce MG. Cocultivation of Ulva with active bacterial strains is so far the only way to induce the MG effect, which suggests that for MG direct contact between Ulva and the bacterial strain is necessary.     

Effects of hypergravity on the elongation and morphology of protonemata of Adiantum capillus-veneris

Elongation growth of protonemata of Adiantum capillus-veneris , which can be controlled by light irradiation, was examined under acropetal and basipetal hypergravity conditions (from -13 to +20 g ) using a newly developed centrifugation equipment. Elongation of the protonemata under red light was inhibited by basipetal hypergravity at more than +15 g but was promoted by acropetal hypergravity from -5 to -8 g . Division of the protonemal cells that was induced by white light was inhibited under basipetal hypergravity at +20 g but was unaffected under acropetal hypergravity at -15 g . Upon exposure to continuous red light for 7 to 8 days, most of the protonemata grew as filamentous cells in the absence of a change in the normal gravitational force (control), but more than half of the protonemal cells were abnormal in terms of shape when maintained under hypergravity at +20 g .     

Pollen morphology of Gyrostemonaceae,Bataceae andKoeberlinia

Pollen morphology of Gyrostemonaceae, Bataceae, andKoeberlinia, which have been affiliated with glucosinolate-producing taxa, was examined by field emission scanning and transmission electron microscopy. Pollen grains of Gyrostemonaceae are tricolpate with scabrate-spinulate surface and have a thick, unstratified exine, while those of Bataceae are tricolporoidate with granular surface and have a thin exine with a single, outermost granular layer. Gyrostemonaceae and Bataceae, which had often been considered sister taxa based on palynological similarity and now are considered more distantly related, have a similar spongy ektexine, but differences between them are evident.Koeberlinia, which is recently considered a sister group to Bataceae+Salvadoraceae (with no spongy ektexine), has tricolporoidate pollen composed of a plesiomorphic, stratified exine with columellae. The totality of evidence indicates that, contrary to earlier observations, pollen of Gyrostemonaceae and Bataceae does not closely resemble each other, and that the spongy ektexine, which looks to be similar in TEM sections, is a homoplasy that evolved independently in the two families. Dedicated to the late Prof. Emer. Kankichi Sohma (August 28, 1926–June 26, 1995), who supervised us for our M. Sc. and D. Sc. programs at Tohoku University, Sendai. He died after his 40 years career in palynology; his wide range of interests and enthusiasm for research, and his unfailing encouragement for students are greatly missed.     

The initiation mess?

This review concerns the mechanisms which control initiation of chromosome replication in enterobacteria with respect to cell growth. Initiation control is commonly separated into positive and negative regulatory mechanisms. Four main points are advanced concerning these different aspects of initiation control. (i) The average concentration of the initiator protein DnaA is proportional to the origin concentration, i.e. the origin per cell mass ratio and, thus, inversely proportional to the very often used term of the 'initiation mass'. (ii) The time of initiation of chromosome replication in the cell cycle is set by DnaA protein accumulating to a threshold level, which in concert with a number of other factors allows for a co-operative formation of the initiation complex. (iii) The time of initiation is not determined by the interaction with these other factors or by the transient interaction between newly replicated origins ( oriC  ) and the cell surface. (iv) The aberrant initiation phenotype observed in various mutants, including dnaA (ts) mutants, might be due to a defective pre-initiation DnaA– oriC interaction or it might be due to a defect in the protection of newly initiated origins from reinitiation. Many of these points are discussed and evaluated in view of recent developments concerning the regulation of chromosome replication in Escherichia coli     

Surfactant-mediated gene transfer for animal cells

A commercially available cationic surfactant, dimethyl-dioctadecyl ammonium bromide (DDAB), was used for making lipid vesicles. DDAB easily dissolved in water at 60 °C and formed lipid vesicles at room temperature. The lipid vesicles showed very low cytotoxicity compared with other cationic surfactants. After the lipid vesicles were mixed with plasmid DNA solution, the solution was added to mammalian cells. The addition of a nonionic surfactant (Tween 80) to the cationic lipid vesicles at the weight ratio of 1:1 enhanced transfection efficiency. Adding more or less than the optimal amounts of DNA and lipid vesicles resulted in decreased transfection efficiency. With the optimal amounts of DNA (pCMVβ) and lipid vesicles, about 90–95% of CHO-K1 and BHK-21C13 cells transiently expressed β-galactosidase activity 24 h after transfection. By this procedure, stable transformants around 10⁵ cells corresponding to 10% efficiency could be obtained by one batch transfection. This revised version was published online in June 2006 with corrections to the Cover Date.     

DEVELOPMENT OF OMNIAPERTURATE POLLEN IN TRILLIUM KAMTSCHATICUM (LILIACEAE)

Ultrastructural changes during omniaperturate pollen development in Trillium kamtschaticum Pall, was examined using transmission electron microscopy. The pollen mother cells are not enveloped within a thick callosic wall. The microspores resulting from successive meiosis are divided by scanty deposition of callosic wall in the tetrad. A primexine/exine template is not recognizable within the tetrad during formation of exinous components. Preexinous globules, originating from vesicles in the callosic wall, accumulate electron-dense materials and develop into exinous globules. The preexinous globules have ca 10 nm wide contacts with tilted and invaginated plasma membrane of the microspore within the callosic wall. After dissolution of the callosic wall, the microspores separate and mitosis subsequently leads to the formation of a generative cell and vegetative cell encased in a loose aggregation of developing exinous globules. When the generative cell is at the pollen grain surface, the channeled zone is initiated at the opposite side of the microspore on the surface of the vegetative cell. Just before pollen maturity, a new layer develops under the channeled zone. Thus, development of the omniaperturate pollen grains of T. kamtschaticum involves some processes that are distinct from those of Canna and Heliconia and some that are similar.     

Life history of amphibians and gravity.

Anurans hold a unique position in vertebrate phylogeny, as they made the major transition from water to land. Through evolution they have acquired fundamental mechanisms to adapt to terrestrial gravity. Such mechanisms are now shared among other terrestrial vertebrates derived from ancestral amphibians. Space research, using amphibians as a model animal, is significant based on the following aspects: (1) Anuran amphibians show drastic changes in their living niche during their metamorphosis. Environments for tadpoles and for terrestrial life of frogs are quite different in terms of gravity and its associated factors. (2) Certain tadpoles, such as Rhacophorus viridis amamiensis, have a transparent abdominal wall. Thus visceral organs and their motion can be observed in these animals in non-invasive manner through their transparent abdominal skin. This feature enables biologists to evaluate the physiological state of these amphibians and study the autonomic control of visceral organs. It is also feasible for space biologists to examine how such autonomic regulation could be altered by microgravity and exposure to the space environment.