The transit of Venus, 8 June 2004: a teachers’ guide to finding the Earth Sun distance

Details The transit of Venus, 8 June 2004: a teachers’ guide to finding the Earth Sun distance The transit of Venus, 8 June 2004: a teachers’ guide to finding the Earth Sun distance

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004phyed..39..252c&link_type=abstract

Physics Education, Volume 39, Issue 3, pp. 252-266 (2004).

Physics

Physics Education

Scientific paper

Transits of Venus have been observed since the 17th century and were soon recognized as a way of determining the distance from the Earth to the Sun. But just how can this be done? There are in fact four methods and this article examines them in turn, making clear how Venus will appear to move, what observations are required, the calculations that follow and the relative merits of each method.
JG was supported by KBN grant no 2 P03A 020 24.

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