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The Leap Second Debate and the Lessons from Timekeeping History

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Book cover The Vatican Observatory, Castel Gandolfo: 80th Anniversary Celebration

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP,volume 51))

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Abstract

Timekeeping, together with navigation, is one of the oldest missions of astronomy, originating long before the dawn of written history. The ancient and sacred task of timekeeping, linking the eternal with the everyday, stood at the origin of the Vatican Observatory. The history of timekeeping schemes throughout millennia has been a search for a balance between the practical and the symbolic. The current debate focuses on the Leap Second, a mechanism first applied in 1972. Atomic clocks, careful observations of distant quasars, etc. tell us that the Earth spins somewhat irregularly. The symbolic value of coupling civil timekeeping to the heavens is so strong, however, that the international community still requires the International Telecommunication Union to broadcast time signals following Earth’s rotation. In order to reconcile this symbolically significant requirement with the practicality of uniformly flowing atomic time, a leap second is added (or subtracted) from the otherwise perfectly regular sequence, so that every so often there is a minute with 61 (or 59) seconds. This system is currently under review, with a proposal on the table to abandon the leap second, decoupling civil timekeeping from astronomical phenomena. Social mechanisms involved in timekeeping can be studied by examining the historical evidence related to calenders. These lessons may provide a broader context for the leap-second debate and they may shed light on it. Calculated timekeeping does not actually agree with the heavens at any given moment, but this does not seem to jeopardize the general perception of its astronomical conformity since it is rightly perceived as a way of preserving it on average. The current proposal, however, clearly entails decoupling civil time from Earths rotation. If presented as a definitive solution, it would result in a direct and unprecedented breach with the principle of astronomical conformity. If presented as a temporary measure, to be applied until a better solution is found, it would preserve the principle of astronomical conformity because the latter fulfills its social function even when it is not observed perfectly considering that in the realm of symbolism what counts is the general perception, not the fact.

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Notes

  1. 1.

    The specification of conditions was added in 1997.

  2. 2.

    It has been proposed that CGPM 2018 redefine all base units in terms of the second by fixing the numerical values of the constants c, h, e, k, and NA (Mills 2010). Although CGPM 2018 might redefine the second, it is more likely to defer the decision to the following CGPM.

  3. 3.

    We shall refrain from discussing other vital components of every timekeeping system: record keeping, synchronization and time transfer.

  4. 4.

    The apparent positions in the sky at given times of the Sun, Moon, the planets, and other celestial bodies, derived from our mathematical models of their motions.

  5. 5.

    In principle it could be at the end of any month but since 1972 it has always been only June and December, months which have been designated as first preference. March and September are the second preference.

  6. 6.

    http://www.ucolick.org/˜sla/leapsecs/ (Allen 2016).

  7. 7.

    ITU = International Telecommunications Union; ITU-R = Radiocommunications Sector of ITU.

  8. 8.

    CIPM’s Comité consultatif du temps et des fréquence (Consultative Committee for Time and Frequency). CIPM = Comité internationale des poids et mesures (International Committee for Weights and Measures).

  9. 9.

    International Earth Rotation and Reference Systems Service.

  10. 10.

    Bureau international des poids et mesures (International Bureau of Weights and Measures).

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Acknowledgements

This paper is the result of the author’s participation in symposia held in Exton in 2011 (Seago et al. 2011), in Charlottesville in 2013 (Seago et al. 2013), and at Harvard in 2016 (Arias et al. 2017). It presents some material from (Gabor 2011) in a more popular form and with a different emphasis. The author is very grateful to the organizers of these meetings for their invitation and valuable discussions.

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Gabor, P. (2018). The Leap Second Debate and the Lessons from Timekeeping History. In: Gionti, S. J., G., Kikwaya Eluo, S.J., JB. (eds) The Vatican Observatory, Castel Gandolfo: 80th Anniversary Celebration. Astrophysics and Space Science Proceedings, vol 51. Springer, Cham. https://doi.org/10.1007/978-3-319-67205-2_15

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