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On the basis of non-covalent bond interactions in nucleic acids, we synthesized the deoxyadenosine derivatives tethering a phenyl group (X) and a naphthyl group (Z) by an amide linker, which mimic a Watson–Crick base pair. Circular dichroism spectra indicated that the duplexes containing X and Z formed a similar conformation regardless of the opposite nucleotide species (A, G, C, T and an abasic site analogue F), which was not observed for the natural duplexes. The ΔG370 values among the natural duplexes containing the A/A, A/G, A/C, A/T and A/F pairs differed by 5.2 kcal mol−1 while that among the duplexes containing X or Z in place of the adenine differed by only 1.9 or 2.8 kcal mol−1, respectively. Fluorescence quenching experiments confirmed that 2-amino purine opposite X adopted an unstacked conformation. The structural and thermodynamic analyses suggest that the aromatic hydrocarbon group of X and Z intercalates into a double helix, resulting in the opposite nucleotide base flipping into an unstacked position regardless of the nucleotide species. This observation implies that modifications at the aromatic hydrocarbon group and the amide linker may expand the application of the base pair-mimic nucleosides for molecular biology and biotechnology.

Glycosidase-promoted hydrolysis was performed in a microreaction channel. The result was compared with the reaction in a micro-test tube. Transgalactosylation on p-nitrophenyl-2-acetamide-2-deoxy-beta-D-glucopyranoside was also examined in a microreaction channel, because transglycosylation is a useful method for oligosaccharide synthesis. We examined both the forward reaction, i.e., hydrolysis, and the reverse reaction, i.e., transglycosylation, in the microreaction channel. The results showed that both hydrolysis and transglycosylation were enhanced in the microreaction channel compared with the batch reaction.

The high-precision gamma-ray spectrometer (GRS) on the lunar polar orbiter SELENE is designed to measure 200 keV-12 MeV gamma rays in order to determine elemental compositions of the lunar surface. The GRS consists of a large germanium (Ge) crystal as a main detector and a massive bismuth germanate crystal and a plastic scintillator as anticoincidence detectors. The Ge detector is cooled by a Stirling cryocooler with its compressor attached to a passive radiator facing the cold space. The cooling system maintains the Ge detector below 90 K during the observation. The flight model of the GRS has achieved an energy resolution of 3.0 keV (FWHM) at 1333 keV. Energy spectra obtained by the GRS will show sharp gamma-ray lines whose energies identify the elements and whose intensities determine the concentrations of the elements, permitting global mapping of the elemental abundances in the sub-surface of the Moon. The elemental maps obtained by the GRS with such high-energy resolution enable us to study lunar geoscience problems.

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Novel deoxyadenosine derivatives tethering a phenyl or naphthyl group by means of an amido linker have been synthesized, and these derivatives, stacking on the 5' end of a DNA duplex, provide free energy contributions equal to or greater than that of the Watson-Crick A/T base pair.

Summary: A novel semi‐interpenetrating polymer network (semi‐IPN) with photomechanical switching ability was developed by a cationic copolymerization of azobenzene‐containing vinyl ethers in a matrix of a linear polycarbonate (PC). The semi‐IPN film showed reversible deformation upon switching the UV irradiation on and off and responded with unprecedented rapidity. The photomechanical effect is attributed to a reversible change between the highly aggregated and dissociated states of the azobenzene groups.The reversible UV response of the length of the semi‐IPN film at 25 °C.magnified imageThe reversible UV response of the length of the semi‐IPN film at 25 °C.

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