Hostname: page-component-8448b6f56d-m8qmq Total loading time: 0 Render date: 2024-04-15T19:45:16.284Z Has data issue: false hasContentIssue false

The Use of SI Units in Astronomy

Published online by Cambridge University Press:  12 April 2016

G. A. Wilkins*
Affiliation:
Royal Greenwich Observatory

Summary

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The principal features of the International System of Units (SI) are briefly described and the advantages of its wider adoption in astronomy are discussed. The need for the continued use of a system of astronomical units for some purposes is recognised.

Type
Part I. Standards for the Presentation of Data
Copyright
Copyright © Reidel 1977

References

1. Bureau Internationale des Poids et Mesures, 1970. Le Système International d’Unités. OFFILIB, 48 rue Gay-Lussac, F 75, Paris 5, France.Google Scholar
2a. National Physical Laboratory, 1970. SI The International System of Units. Her Majesty’s Stationery Office, London, England.Google Scholar
2b. National Bureau of Standards, 1970. SI The International System of Units. NBS Special Publication 330, US Government Printing Office, Washington DC, USA.Google Scholar
3. CODATA, 1973. Guide for the presentation in the primary literature of numerical data derived from experiments. CODATA Bulletin No. 9. Available from CODATA Secretariat, 51 Boulevard de Montmorency, 75016, Paris, France.Google Scholar
4. Royal Society, 1975. Quantities, Units, and Symbols. 2nd edition. ISBN 0 85403 071 9. Royal Society, 6 Carlton House Terrace, London, SW1Y 5AG, England.Google Scholar
5. Markowitz, W M, 1973. SI, The International System of Units. Geophysical Surveys 1, 217241.CrossRefGoogle Scholar