Modified mevalonate pathway of the archaeon Aeropyrum pernix proceeds via trans-anhydromevalonate 5-phosphate.

The modified mevalonate pathway is believed to be the upstream biosynthetic route for isoprenoids in general archaea. The partially identified pathway has been proposed to explain a mystery surrounding the lack of phosphomevalonate kinase and diphosphomevalonate decarboxylase by the discovery of a conserved enzyme, isopentenyl phosphate kinase. Phosphomevalonate decarboxylase was considered to be the missing link that would fill the vacancy in the pathway between mevalonate 5-phosphate and isopentenyl phosphate. This enzyme was recently discovered from haloarchaea and certain Chroloflexi bacteria, but their enzymes are close homologs of diphosphomevalonate decarboxylase, which are absent in most archaea. In this study, we used comparative genomic analysis to find two enzymes from a hyperthermophilic archaeon, Aeropyrum pernix, that can replace phosphomevalonate decarboxylase. One enzyme, which has been annotated as putative aconitase, catalyzes the dehydration of mevalonate 5-phosphate to form a previously unknown intermediate, trans-anhydromevalonate 5-phosphate. Then, another enzyme belonging to the UbiD-decarboxylase family, which likely requires a UbiX-like partner, converts the intermediate into isopentenyl phosphate. Their activities were confirmed by in vitro assay with recombinant enzymes and were also detected in cell-free extract from A. pernix These data distinguish the modified mevalonate pathway of A. pernix and likely, of the majority of archaea from all known mevalonate pathways, such as the eukaryote-type classical pathway, the haloarchaea-type modified pathway, and another modified pathway recently discovered from Thermoplasma acidophilum.

Identification of enzymes involved in the mevalonate pathway of Flavobacterium johnsoniae.

The mevalonate pathway is prevalent in eukaryotes, archaea, and a limited number of bacteria. This pathway yields the fundamental precursors for isoprenoid biosynthesis, i.e., isopentenyl diphosphate and dimethylally diphosphate. In the downstream part of the general eukaryote-type mevalonate pathway, mevalonate is converted into isopentenyl diphosphate by the sequential actions of mevalonate kinase, phosphomevalonate kinase, and diphosphomevalonte decarboxylase, while a partial lack of the putative genes of these enzymes is sometimes observed in archaeal and bacterial genomes. The absence of these genes has led to the recent discovery of modified mevalonate pathways. Therefore, we decided to investigate the mevalonate pathway of Flavobacterium johnsoniae, a bacterium of the phylum Bacteroidetes, which is reported to lack the genes of mevalonate kinase and phosphomevalonate kinase. This study provides proof of the existence of the general mevalonate pathway in F. johnsoniae, although the pathway involves the kinases that are distantly related to the known enzymes.

Determination of Chitin Based on the Colorimetric Assay of Glucosamine in Acidic Hydrolysate.

A colorimetric method for the glucosamine (GlcN) assay was applied for the determination of chitin, which can be hydrolyzed to produce GlcN. A 10-mg sample was mixed with 10 mL of a 5 mol/L HCl aqueous solution, and the mixture was kept at 100°C for 12 h. Under these conditions, chitin was completely depolymerized and deacetylated to produce GlcN, even when the sample was a crab shell. A 20-µL aliquot of the hydrolysate was mixed with 20 µL of a 5 mol/L NaOH aqueous solution and 200 µL of a 50 mmol/L Na2SiO3, 600 mmol/L Na2MoO4, 1.5 mol/L CH3COOH and 30% (v/v) dimethyl sulfoxide solution. The mixture was kept at 70°C for 30 min. In the mixture, GlcN reduced the Mo(VI) species to form a blue molybdosilicate anion, which gave an absorbance maximum at around 750 nm. Since N-acetylglucosamine and chitin oligosaccharides could not render the reaction mixture blue, GlcN in the hydrolysate could be assayed colorimetrically with high selectivity. When a standard chitin sample was examined, the GlcN concentration in the hydrolysate was determined to be 0.97 ± 0.02 g/L (as hydrochloride salt), indicating that the sample contained 10.0 ± 0.2 mg chitin (as an N-acetylglucosamine homopolymer). Calcium cation, amino acids, and proteins did not interfere with the GlcN assay. Thus, the proposed method was successfully applied to determine chitin in a crab shell sample.

Cold ions in the hot plasma sheet of Earth's magnetotail.

Most visible matter in the Universe exists as plasma. How this plasma is heated, and especially how the initial non-equilibrium plasma distributions relax to thermal equilibrium (as predicted by Maxwell-Boltzman statistics), is a fundamental question in studies of astrophysical and laboratory plasmas. Astrophysical plasmas are often so tenuous that binary collisions can be ignored, and it is not clear how thermal equilibrium develops for these 'collisionless' plasmas. One example of a collisionless plasma is the Earth's plasma sheet, where thermalized hot plasma with ion temperatures of about 5 x 10(7) K has been observed. Here we report direct observations of a plasma distribution function during a solar eclipse, revealing cold ions in the Earth's plasma sheet in coexistence with thermalized hot ions. This cold component cannot be detected by plasma sensors on satellites that are positively charged in sunlight, but our observations in the Earth's shadow show that the density of the cold ions is comparable to that of hot ions. This high density is difficult to explain within existing theories, as it requires a mechanism that permits half of the source plasma to remain cold upon entry into the hot turbulent plasma sheet.