Dahlin S, Reinhammar B, Angström J
Department of Biochemistry and Biophysics, University of Göteborg, Sweden.
Biochemistry. 1989 Sep 5;28(18):7224-33. doi: 10.1021/bi00444a014.
1H nuclear magnetic resonance (1H NMR) experiments on Co(II)-substituted stellacyanin have been performed. Large paramagnetic hyperfine shifts are observed, the whole spectrum covering a range of 190 ppm. Experiments were mainly performed at 270 MHz from which temperature and pH* dependencies of the out-shifted resonances were reported, as well as determinations of the longitudinal (T1) and transverse (T2) relaxation times. These relaxation times are among other things, dependent on the individual proton-metal distance, and the aim of this work has been to determine these distances, by use of the Solomon-Bloembergen equations modified to include the so-called "Curie spin". The application of this method to a protein has not been reported earlier. Experiments were also performed at 100, 400, and 500 MHz in order to estimate the size of the Curie spin from the field dependence of the line widths. Furthermore, determination of the values for the rotational correlation time, tau r, and the effective magnetic moment, mu eff, was necessary for the present approach. With apostellacyanin, tau r was found to be (6.0 +/- 0.4) X 10-8 s. From the paramagnetic susceptibility of Co(II) stellacyanin, the value (4.53 +/- 0.03)beta was determined for mu eff. The proposed assignments of several paramagnetically out-shifted resonances. the proton-metal distances obtained, and the known peptide sequence of stellacyanin have allowed us to build a three-dimensional model of the metal site and its surrounding structure consistent with all the experimental data. It is revealed that both histidine ligands bind the metal with their 3-nitrogens. Also we find strong indications that a second sulfur atom is actually binding the metal, this being the long-sought-after fourth ligand. The model suggests that this sulfur belongs to Cys-59, which together with Cys-93 constitutes the disulfide bridge known to be present in the structure. A potential fifth ligand, an amide oxygen from Asn-47, is also found.
已对钴(II)取代的星蓝蛋白进行了氢核磁共振(1H NMR)实验。观察到较大的顺磁超精细位移,整个光谱范围覆盖190 ppm。实验主要在270 MHz下进行,据此报道了外移共振的温度和pH*依赖性,以及纵向(T1)和横向(T2)弛豫时间的测定。这些弛豫时间尤其取决于各个质子与金属的距离,这项工作的目的是通过使用经修改以纳入所谓“居里自旋”的所罗门-布洛姆伯根方程来确定这些距离。此前尚未报道过将此方法应用于蛋白质的情况。还在100、400和500 MHz下进行了实验,以便根据线宽的场依赖性估计居里自旋的大小。此外,对于本方法而言,确定旋转相关时间τr和有效磁矩μeff的值是必要的。对于脱辅基星蓝蛋白,发现τr为(6.0±0.4)×10-8 s。根据钴(II)星蓝蛋白的顺磁磁化率,确定μeff的值为(4.53±0.03)β。对几个顺磁外移共振的拟定归属、获得的质子-金属距离以及星蓝蛋白已知的肽序列,使我们能够构建一个与所有实验数据一致的金属位点及其周围结构的三维模型。结果表明,两个组氨酸配体均通过其3-氮原子与金属结合。我们还发现有力迹象表明,第二个硫原子实际上在与金属结合,这就是长期寻找的第四个配体。该模型表明,这个硫属于半胱氨酸-59,它与半胱氨酸-93一起构成了已知存在于该结构中的二硫键。还发现了一个潜在的第五个配体,即来自天冬酰胺-47的酰胺氧。