Sahu S C, Bhuyan A K, Majumdar A, Udgaonkar J B
Department of Chemical Sciences, Tata Institute of Fundamental Research, Mumbai, India.
Proteins. 2000 Dec 1;41(4):460-74. doi: 10.1002/1097-0134(20001201)41:4<460::aid-prot40>3.0.co;2-x.
Backbone dynamics of uniformly (15)N-labeled barstar have been studied at 32 degrees C, pH 6.7, by using (15)N relaxation data obtained from proton-detected 2D (1)H-(15)N NMR spectroscopy. (15)N spin-lattice relaxation rate constants (R(1)), spin-spin relaxation rate constants (R(2)), and steady-state heteronuclear (1)H-(15)N NOEs have been determined for 69 of the 86 (excluding two prolines and the N-terminal residue) backbone amide (15)N at a magnetic field strength of 14.1 Tesla. The primary relaxation data have been analyzed by using the model-free formalism of molecular dynamics, using both isotropic and axially symmetric diffusion of the molecule, to determine the overall rotational correlation time (tau(m)), the generalized order parameter (S(2)), the effective correlation time for internal motions (tau(e)), and NH exchange broadening contributions (R(ex)) for each residue. As per the axially symmetric diffusion, the ratio of diffusion rates about the unique and perpendicular axes (D( parallel)/D( perpendicular)) is 0.82 +/- 0.03. The two results have only marginal differences. The relaxation data have also been used to map reduced spectral densities for the NH vectors of these residues at three frequencies: 0, omega(H), and omega(N), where omega(H),(N) are proton and nitrogen Larmor frequencies. The value of tau(m) obtained from model-free analysis of the relaxation data is 5.2 ns. The reduced spectral density analysis, however, yields a value of 5.7 ns. The tau(m) determined here is different from that calculated previously from time-resolved fluorescence data (4.1 ns). The order parameter ranges from 0.68 to 0.98, with an average value of 0.85 +/- 0.02. A comparison of the order parameters with the X-ray B-factors for the backbone nitrogens of wild-type barstar does not show any considerable correlation. Model-free analysis of the relaxation data for seven residues required the inclusion of an exchange broadening term, the magnitude of which ranges from 2 to 9.1 s(-1), indicating the presence of conformational averaging motions only for a small subset of residues.
通过利用从质子检测的二维¹H-¹⁵N NMR光谱获得的¹⁵N弛豫数据,在32℃、pH 6.7条件下研究了均匀¹⁵N标记的巴司星的主链动力学。在14.1特斯拉的磁场强度下,已测定了86个(不包括两个脯氨酸和N端残基)主链酰胺¹⁵N中69个的¹⁵N自旋晶格弛豫速率常数(R₁)、自旋-自旋弛豫速率常数(R₂)以及稳态异核¹H-¹⁵N NOE。通过使用分子动力学的无模型形式体系,利用分子的各向同性和轴对称扩散,对主要弛豫数据进行了分析,以确定每个残基的整体旋转相关时间(τm)、广义序参数(S₂)、内部运动的有效相关时间(τe)以及NH交换加宽贡献(Rex)。根据轴对称扩散,围绕唯一轴和垂直轴的扩散速率之比(D平行/D垂直)为0.82±0.03。这两个结果仅有微小差异。弛豫数据还被用于绘制这些残基的NH向量在三个频率下的约化谱密度:0、ωH和ωN,其中ωH、N是质子和氮的拉莫尔频率。从弛豫数据的无模型分析获得的τm值为5.2纳秒。然而,约化谱密度分析得出的值为5.7纳秒。此处确定的τm与先前从时间分辨荧光数据计算得出的值(4.1纳秒)不同。序参数范围为0.68至0.98,平均值为0.85±0.02。将序参数与野生型巴司星主链氮的X射线B因子进行比较,未显示出任何显著相关性。对七个残基的弛豫数据进行无模型分析需要纳入一个交换加宽项,其大小范围为2至9.1 s⁻¹,表明仅一小部分残基存在构象平均运动。