ABSTRACT
We present the first direct experimental test of the complex ion structure in liquid carbon at pressures around 100 GPa, using spectrally resolved x-ray scattering from shock-compressed graphite samples. Our results confirm the structure predicted by ab initio quantum simulations and demonstrate the importance of chemical bonds at extreme conditions similar to those found in the interiors of giant planets. The evidence presented here thus provides a firmer ground for modeling the evolution and current structure of carbon-bearing icy giants like Neptune, Uranus, and a number of extrasolar planets.
ABSTRACT
cDNA for the C-terminal Ca(2+)-binding domain of rat calpain small subunit was cloned by means of the polymerase chain reaction. The encoded protein (21 kDa), which corresponds closely to the natural autolysis product of the small subunit, was produced in soluble form in Escherichia coli at a level of 20 mg/liter of cell culture. Rat calpain II large subunit (80 kDa) was produced from a cDNA clone in E. coli in soluble form at a level of approximately 1 mg/liter. The 80-kDa subunit alone had no proteinase activity, with or without Ca2+, but Ca(2+)-dependent proteinase activity was obtained following association of the two subunits, which was achieved either by co-expression of the two subunit cDNAs in E. coli, or by mixing the two partially purified subunits in the presence of 1 M NaSCN followed by dialysis. The heterodimeric (80 + 21 kDa) proteinase had a Ca2+ requirement for 50% activity of 0.35 mM and a specific activity at 2 mM Ca2+ of approximately 1 unit/microgram, values essentially identical to those of natural (80 + 30 kDa) calpain II. The results establish association and biological activity of the bacterially produced subunits and provide a system for studying structure-function relationships in calpain by means of mutagenesis.
