On the Telescopic Disks of Stars: A Review and Analysis of Stellar Observations from the Early Seventeenth through the Middle Nineteenth Centuries.

Since the dawn of telescopic astronomy astronomers have observed and measured the ‘spurious’ telescopic disks of stars, generally reporting that brighter stars have larger disks than fainter stars. Early observers such as Galileo Galilei interpreted these disks as being the physical bodies of stars;...

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Publicado en:Annals of Science Vol. 68; no. 3; pp. 351 - 374
Autores principales: Graney, ChristopherM., Grayson, TimothyP.
Formato: Artículo
Publicado: Taylor & Francis Ltd Jul2011
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Acceso en línea:Ver este registro en EBSCOhost
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        10.1080/00033790.2010.507472
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        atl: On the Telescopic Disks of Stars: A Review and Analysis of Stellar Observations from the Early Seventeenth through the Middle Nineteenth Centuries.
      aug:
        au:
          Graney, ChristopherM.
          Grayson, TimothyP.
        affil:
          1000 Community College Drive, Jefferson Community & Technical College, KY 40272, Louisville, USA
          Ktech Corporation, 901 North Stuart Street, Suite 902, Arlington, VA, 22203, USA
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        Star observations
        History of astronomy
        Telescopes
        Airy, George Biddell, 1801-1892
        Galilei, Galileo, 1564-1642
        Huygens, Christiaan, 1629-1695
        Herschel, William
        Marius, Simon
        Halley, Edmond, 1656-1742
        Illusion (Philosophy)
        Wave theory of light
        Astronomical photography
        History
      sug:
        subj:
          Star observations
          History of astronomy
          Telescopes
          Airy, George Biddell, 1801-1892
          Galilei, Galileo, 1564-1642
          Huygens, Christiaan, 1629-1695
          Herschel, William
          Marius, Simon
          Halley, Edmond, 1656-1742
          Illusion (Philosophy)
          Wave theory of light
          Astronomical photography
          History
      ab: Since the dawn of telescopic astronomy astronomers have observed and measured the ‘spurious’ telescopic disks of stars, generally reporting that brighter stars have larger disks than fainter stars. Early observers such as Galileo Galilei interpreted these disks as being the physical bodies of stars; later observers such as William Herschel understood them to be spurious; some, such as Christian Huygens, argued that stars show no disks at all. In the early nineteenth-century George B. Airy produced a theoretical explanation of star images sufficient to explain all historical observations, but astronomers were slow to fully recognise this. Even today conventional wisdom concerning stars and telescopes stands at odds to both historical observations and Airy’s theory. We give a detailed analysis of both historical observations and Airy’s theory, illustrating how Airy’s theory explains the historical observations, from Galileo to Huygens to Herschel. We argue that the observations themselves appear in all cases to be valid and worth further study.
      pubtype: Academic Journal
      doctype: Article
      src: R
    language: English
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      custom: Copyright of Annals of Science is the property of Taylor & Francis Ltd and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use.
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