秀丽隐杆线虫中心体星状体在动力学上占主导地位的组装途径是依赖γ-微管蛋白的。
The kinetically dominant assembly pathway for centrosomal asters in Caenorhabditis elegans is gamma-tubulin dependent.
作者信息
Hannak Eva, Oegema Karen, Kirkham Matthew, Gönczy Pierre, Habermann Bianca, Hyman Anthony A
机构信息
Max Planck Institute of Molecular Cell Biology and Genetics, 01307 Dresden, Germany.
出版信息
J Cell Biol. 2002 May 13;157(4):591-602. doi: 10.1083/jcb.200202047.
gamma-Tubulin-containing complexes are thought to nucleate and anchor centrosomal microtubules (MTs). Surprisingly, a recent study (Strome, S., J. Powers, M. Dunn, K. Reese, C.J. Malone, J. White, G. Seydoux, and W. Saxton. Mol. Biol. Cell. 12:1751-1764) showed that centrosomal asters form in Caenorhabditis elegans embryos depleted of gamma-tubulin by RNA-mediated interference (RNAi). Here, we investigate the nucleation and organization of centrosomal MT asters in C. elegans embryos severely compromised for gamma-tubulin function. We characterize embryos depleted of approximately 98% centrosomal gamma-tubulin by RNAi, embryos expressing a mutant form of gamma-tubulin, and embryos depleted of a gamma-tubulin-associated protein, CeGrip-1. In all cases, centrosomal asters fail to form during interphase but assemble as embryos enter mitosis. The formation of these mitotic asters does not require ZYG-9, a centrosomal MT-associated protein, or cytoplasmic dynein, a minus end-directed motor that contributes to self-organization of mitotic asters in other organisms. By kinetically monitoring MT regrowth from cold-treated mitotic centrosomes in vivo, we show that centrosomal nucleating activity is severely compromised by gamma-tubulin depletion. Thus, although unknown mechanisms can support partial assembly of mitotic centrosomal asters, gamma-tubulin is the kinetically dominant centrosomal MT nucleator.
含γ-微管蛋白的复合物被认为可成核并锚定中心体微管(MTs)。令人惊讶的是,最近一项研究(斯特罗姆,S.,J. 鲍尔斯,M. 邓恩,K. 里斯,C.J. 马龙,J. 怀特,G. 赛杜克斯,和W. 萨克斯顿。《分子生物学细胞》12:1751 - 1764)表明,在通过RNA介导的干扰(RNAi)使γ-微管蛋白缺失的秀丽隐杆线虫胚胎中会形成中心体星状体。在此,我们研究了γ-微管蛋白功能严重受损的秀丽隐杆线虫胚胎中中心体MT星状体的成核和组织情况。我们对通过RNAi使约98%的中心体γ-微管蛋白缺失的胚胎、表达γ-微管蛋白突变形式的胚胎以及缺失一种γ-微管蛋白相关蛋白CeGrip - 1的胚胎进行了表征。在所有情况下,中心体星状体在间期都无法形成,但在胚胎进入有丝分裂时会组装。这些有丝分裂星状体的形成不需要ZYG - 9(一种中心体MT相关蛋白)或胞质动力蛋白(一种向负端移动的马达蛋白,在其他生物体中有助于有丝分裂星状体的自我组织)。通过在体内动态监测冷处理的有丝分裂中心体的MT再生,我们发现γ-微管蛋白缺失会严重损害中心体的成核活性。因此,尽管未知机制可以支持有丝分裂中心体星状体的部分组装,但γ-微管蛋白是动力学上占主导地位的中心体MT成核因子。
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