同移距离
在宇宙学中,共动距离和普通距离是两种很相关的距离测量方式,用于定义两个天体之间的距离。
普通距离就是我们平常所使用的距离衡量方式,在宇宙时的某个特定时间用一系列的测量手段测量天体到地球之前的距离,由于宇宙膨胀,这个测量出来的距离会随着时间变化。而共动距离排除了宇宙膨胀的影响,给出了不随空间膨胀的距离结果。
共动距离和普通距离被定义成在当前时间相等,其他的所有时间普通距离随时间以宇宙標度因子变化,而共动距离一直保持不变。
共动坐标
引用
外部链接
- Distance measures in cosmology(页面存档备份,存于)
- Ned Wright's cosmology tutorial (页面存档备份,存于)
- iCosmos: Cosmology Calculator (With Graph Generation )(页面存档备份,存于)
- Weinberg, Steven (1972)
- Peebles (1993)
- Davis and Lineweaver, Expanding Confusion(页面存档备份,存于)
- Ned Wright's Javascript cosmology calculator(页面存档备份,存于)
- General method, including locally inhomogeneous case(页面存档备份,存于) and Fortran 77 software
- cosmdist-0.2.0 (页面存档备份,存于) - command line and/or C or Fortran library, based on GNU Scientific Library, for as functions of z and their inverses
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.