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Luminosities, Colours, Diameters, Densities, Masses of the Stars

  • Chapter
Das Sternsystem

Part of the book series: Handbuch der Astrophysik ((volume 5/2))

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Abstract

The underestimation of the distance and the dimensions of the Sun that was a dominating feature of Greek astronomy, was adopted by the astronomers of the Occident and believed until the end of the 17th century. Practically nothing was known about the physical nature of the stars until that time. The distances of the stars also were underestimated and that fact may explain why many observers thought that the stars displayed measurable diameters. It is clear that it was the irradiation and diffraction that deceived the pioneers. In order to illustrate the kind of rôle these phenomena sometimes play we quote some measurements of the “diameters” of different magnitudes.

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  1. Lund, Schweden

    Knut Lundmark

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  1. Knut Lundmark
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Heber D. Curtis B. Lindblad K. Lundmark H. Shapley

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Dieses Kapitel ist Teil des Digitalisierungsprojekts Springer Book Archives mit Publikationen, die seit den Anfängen des Verlags von 1842 erschienen sind. Der Verlag stellt mit diesem Archiv Quellen für die historische wie auch die disziplingeschichtliche Forschung zur Verfügung, die jeweils im historischen Kontext betrachtet werden müssen. Dieses Kapitel ist aus einem Buch, das in der Zeit vor 1945 erschienen ist und wird daher in seiner zeittypischen politisch-ideologischen Ausrichtung vom Verlag nicht beworben.

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Lundmark, K. (1933). Luminosities, Colours, Diameters, Densities, Masses of the Stars. In: Curtis, H.D., Lindblad, B., Lundmark, K., Shapley, H. (eds) Das Sternsystem. Handbuch der Astrophysik, vol 5/2. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-90704-3_1

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