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How Time Served to Measure the Geographical Position Since Hellenism

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BERJAYA The Science of Time 2016

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP,volume 50))

Abstract

The orthogonal grid of latitudes and longitudes on a spherical Earth dates back to Ptolemy’s book on Geography in the second century, and the suggestion to determine the longitude of a traveller dates back to the fourth century. Nevertheless, determining one’s own position while travelling remained a problem for two millennia. The solution was technically performed by the Harrison H4 clock in the eighteenth century, but the idea to measure longitudes by time had always been considered a computing exercise. In this paper, we discuss this classical exercise and the question whether and why it had not been applied. Primarily, we recall this example given by different authors and we will recognize differences in their values. Consequently, we will ask about their sources to trace the transfer and transformation of knowledge, since we will finally have to conclude that their descriptions of the measurement were not based on observations but rather that the numerical values were constructed. We further examine the accuracy of the method, investigating if ancient data were sufficient to apply it at all. Summarizing, we can only wonder why scientists for so many centuries praised the method’s elegance without collecting the data and applying the method.

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Notes

  1. 1.

    Both quotations: Berggren et al. (2000), 1.2.1, p. 59.

  2. 2.

    Berggren et al. (2000) point out in a footnote on p. 59 that the Almagest only explains “astrolabe”, while the “meteoroskopeion” is mentioned and not explained in Geogr. 1.3. They add in another footnote that the description of this instrument by Ptolemy is lost but must have existed according to Pappus and Proclus. It was an armillary-like instrument.

  3. 3.

    The inhabited part of the world (spherical Earth) in Greek is the oikumene.

  4. 4.

    Engl. transl.: Berggren et al. (2000), 1.1.4.

  5. 5.

    In case of measuring the altitude, of course, the geographical latitude must be taken into account.

  6. 6.

    Berggren et al. (2000), p. 62, Geogr. 1.3.

  7. 7.

    Sometimes we find phrases more generally like “with eclipses” or “with solar and lunar eclipses”. The latter variant is probably ill conceived. It cannot work with solar eclipses, since those events are not absolute: Two observers at different places on Earth are hit by the shadow at different times (if they are hit at all). Seen from the Moon, they are not shadowed simultaneously.

  8. 8.

    Toomer and Ptolemaios (1984), 2.1.

  9. 9.

    Berggren et al. (2000), Geogr. 1.1.4.

  10. 10.

    Berggren et al. (2000), Geogr. 1.2.2.

  11. 11.

    Ptol., Geogr. 1.4.2.

  12. 12.

    Ptol., Geogr. 1.4.2.

  13. 13.

    Strabo and T.E.P (1960), p. 23.

  14. 14.

    Natural History II, 180 cited from Littre (1877).

  15. 15.

    http://eclipse.gsfc.nasa.gov/eclipse.html.

  16. 16.

    Strabo criticizes that in the work of Eratosthenes: Strabo, Geogr. 2.1.40.

  17. 17.

    Hunger and Sachs (1988–2014), Vol. 1, p. 176/177, No. −330, lines 2 and 3.

  18. 18.

    Usually, this term is not translated. We know that one UŠ equals one degree on the equator, equals 4 min in time. UŠ as a distance measure is half a cubit and, therefore, probably a span.

  19. 19.

    Modern computations show that totality started 2 h 41.4 min after sunset, cf. http://eclipse.gsfc.nasa.gov/eclipse.html or Huber and de Meis (2004), p. 113 or a good planetarium software. This is in the third hour of the night.

  20. 20.

    Herodotus and Godley (2016) Hdt. 1.74.6 cited from http://perseus.uchicago.edu/.

  21. 21.

    Xen., Hell. 1.6, English translation: Xenophon and Brownson (1918).

  22. 22.

    Thuc. 4.52, English translation: Thucydides et al. (1910).

  23. 23.

    Livy, History of Rome, 44.37, Engl. transl.: Livius and Roberts (1912).

  24. 24.

    cf. Alm. IV, 11.

  25. 25.

    cf. Neugebauer (1975), p. 77.

  26. 26.

    cf. Neugebauer (1975), Vol. 2, p. 780.

  27. 27.

    Although Ptolemy and all astronomers before him did not have the term “error bar”, they had a concept of errors in observations (at least since Hipparchus).

  28. 28.

    His astronomical opus is discussed in Villey (2014).

  29. 29.

    This quote is a reminiscence to Dava Sobel’s bestselling (hi)story on clock maker Harrison who devoted his life to the development of the world’s first portable clock. Such as an eternal flame, it was able to transport the time of a far place with the local observer.

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Correspondence to Susanne M. Hoffmann.

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Hoffmann, S.M. (2017). How Time Served to Measure the Geographical Position Since Hellenism. In: Arias, E., Combrinck, L., Gabor, P., Hohenkerk, C., Seidelmann, P. (eds) The Science of Time 2016. Astrophysics and Space Science Proceedings, vol 50. Springer, Cham. https://doi.org/10.1007/978-3-319-59909-0_4

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