Skip to main content
Log in

The Cosmic Time-Scale

  • Article
  • Published:

From Nature

View current issue Submit your manuscript

Abstract

IN a series of recent mathematical papers, culminating in a general review of the subject in more physical terms1, S. Chandrasekhar has laid the foundations of a statistical theory of stellar dynamics which treats the subject in a way fundamentally different from the ordinary analytical approach. Certain aspects of the theory concerning the dynamics of star clusters and the statistics of binary stars are discussed in detail by Chandrasekhar; they have interesting repercussions on current ideas concerning the time-scale of the universe, and are summarized below.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. Ann. New York Acad. Sci., 45, 131 (1943).

  2. Astrophys. J., 97, 255 (1943).

  3. Astrophys. J., 98, 54 (1943).

  4. Science, 99, 133 (1944).

    Article  ADS  CAS  Google Scholar 

  5. Nature, 137, 537 (1936).

    Article  ADS  Google Scholar 

  6. Astrophys. J., 99, 54 (1944).

  7. Nature, 149, 235 (1942).

  8. Observatory, 65, 211 (1944).

Download references

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

HUNTER, A. The Cosmic Time-Scale. Nature 154, 327–328 (1944). https://doi.org/10.1038/154327a0

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1038/154327a0

  • Springer Nature Limited

Navigation