Vig B K, Richards B T
Department of Biology, University of Nevada, Reno 89557-0015.
Exp Cell Res. 1992 Aug;201(2):292-8. doi: 10.1016/0014-4827(92)90276-e.
Whereas the major satellite fraction in mouse extends its domain from the centromere to the distal end of the pericentric heterochromatin, the minor satellite DNA is present specifically in the centromere or primary constriction. We hybridized the biotinylated minor satellite sequence to L929 cells of mouse origin. The sequence hybridized to all chromosomes. Whereas hybridization was detected on all active centromeres, the inactive centromeres in certain dicentrics did not show any signal. This satellite, however, was detected in all inactive centromeres in a heptacentric chromosome. The intensity of fluorescence on the inactive centromeres of the heptacentric was similar to that present on the active centromeres. Several heterochromatin blocks, which were not associated with any centromere, were also found to lack hybridization with the minor satellite. The inactive centromeres, whether carrying the minor satellite DNA fraction or not, generally do not react with the antikinetochore antibodies present in the scleroderma serum. These studies are interpreted to show that (1) the primary constriction in mouse can be formed without the participation of minor satellite, (2) heterochromatin in mouse may constitute without this fraction, (3) the major and minor satellite may not be interspersed but are joined at some defined boundary, and (4) the binding of CENP-B does not depend upon the quantity of minor satellite or the number of CENP boxes present in the inactive centromeres.
在小鼠中,主要卫星部分从着丝粒延伸至近着丝粒异染色质的远端,而次要卫星DNA则特异性地存在于着丝粒或主缢痕中。我们将生物素化的次要卫星序列与小鼠来源的L929细胞进行杂交。该序列与所有染色体均发生杂交。虽然在所有活跃着丝粒上均检测到杂交信号,但某些双着丝粒中的非活跃着丝粒未显示任何信号。然而,在一条七着丝粒染色体的所有非活跃着丝粒中均检测到了这种卫星。七着丝粒非活跃着丝粒上的荧光强度与活跃着丝粒上的相似。还发现几个与任何着丝粒均无关联的异染色质块也缺乏与次要卫星的杂交。无论是否携带次要卫星DNA部分,非活跃着丝粒通常都不会与硬皮病血清中的抗动粒抗体发生反应。这些研究被解释为表明:(1)小鼠中的主缢痕可以在没有次要卫星参与的情况下形成;(2)小鼠中的异染色质可能在没有这一部分的情况下构成;(3)主要和次要卫星可能不是相互穿插的,而是在某个确定的边界处相连;(4)CENP - B的结合不依赖于非活跃着丝粒中次要卫星的数量或CENP框的数量。