Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-17T16:15:22.591Z Has data issue: false hasContentIssue false

Commission 34. (Solar Parallax.)

Published online by Cambridge University Press:  25 April 2016

Extract

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 President first summarized the present position of the work of determining the solar parallax as given in the Report.

In connection with the determination of the positions of the reference stars it was stated that within the next six months or so the reductions of all the series of photographs will be completed and it will then be possible to co-ordinate the results and publish a definitive list of secondary comparison stars. At the same time it has become apparent that there are appreciable errors in the positions based on the meridian observations of some of the primary stars given in Prof. Kopff’s catalogue. By co-ordinating the measures of the several series of path plates it will be possible to derive corrections to the positions of the Kopff stars, which will still keep them on the system adopted by Prof. Kopff, but will improve their homogeneity.

Type
Part III: Meetings Of Commissions
Copyright
Copyright © Cambridge University Press 1936