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When Double-Star Research Began

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Double Stars

Part of the book series: Geophysics and Astrophysics Monographs ((GAAM,volume 15))

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Abstract

The first occurrence of the name ‘double star’ happened to have been — by modern definitions — a mistake: in Ptolemy’s star catalogue (2nd century AD), the two stars v1 and v2 Sagittarii — separated by 14 min arc, and independent — were called \(\delta i\pi \lambda ous\) Several of the Arab star names refer jointly to two or more neighboring stars easily separated by the naked eye. On the other hand, the well-known naked-eye pair Mizar and Alcor in the Big Dipper received separate names, probably because their difference of brightness did not make them appear as a ‘pair’ of stars.

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© 1978 D. Reidel Publishing Company, Dordrecht, Holland

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Heintz, W.D. (1978). When Double-Star Research Began. In: Double Stars. Geophysics and Astrophysics Monographs, vol 15. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9836-0_2

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  • DOI: https://doi.org/10.1007/978-94-009-9836-0_2

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-277-0886-1

  • Online ISBN: 978-94-009-9836-0

  • eBook Packages: Springer Book Archive

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