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Alpha Centauri, with a graphic projection of its orbit from its apparent curve
Biggs, Alfred Barrett (1887) Alpha Centauri, with a graphic projection of its orbit from its apparent curve. Papers & Proceedings of the Royal Society of Tasmania. pp. 79-82.
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Several circumstances invest the star Alpha Centauri, one of the brightest in our southern sky, with special interest. It was one of the earliest whose annual parallax (from which is deduced its distance) was approximately ascertained. It is, so far as at present known, by much the nearest of the fixed stars to our system. It is perhaps the most magnificent of double stars. And (what invests it with special interest to us) it is, from its great southern declination, invisible to the Observatories of the Northern Hemisphere. Science is therefore dependent entirely upon southern observations for all that can be known of the relative movements of its components. Its distance from the solar system is about 225,000 times that of the earth from the sun. Includes illustration
|Keywords:||Royal Society of Tasmania, Van Diemens Land, VDL, Hobart Town, natural sciences, proceedings, records|
|Journal or Publication Title:||Papers & Proceedings of the Royal Society of Tasmania|
|Page Range:||pp. 79-82|
|Collections:||Royal Society Collection > Papers & Proceedings of the Royal Society of Tasmania|
|Additional Information:||In 1843 the Horticultural and Botanical Society of Van Diemen's Land was founded and became the Royal Society of Van Diemen's Land for Horticulture, Botany, and the Advancement of Science in 1844. In 1855 its name changed to Royal Society of Tasmania for Horticulture, Botany, and the Advancement of Science. In 1911 the name was shortened to Royal Society of Tasmania.|
|Date Deposited:||02 Dec 2012 23:10|
|Last Modified:||18 Nov 2014 04:45|
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