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The Pre-Discovery Observations of Uranus

Published online by Cambridge University Press:  12 April 2016

Eric G. Forbes*
Affiliation:
University of Edinburgh

Extract

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In his Astronomisches Jahrbuch for 1784, Johann Elert Bode summarises the scanty information that had reached Berlin concerning the recent discovery on 13 March 1781 of a new heavenly body by a still-unidentified observer in England. Its easterly progress through the Milky Way during the interim six months had been parallel to the ecliptic, and thus entirely consistent with the view - hitherto based only upon its brightness and clearly-defined disc - that it was a planet and not a comet. Bode therefore asks why this sixth-magnitude object had not been previously detected, and raises the question of whether it had in fact been observed by earlier astronomers but misidentified as a star. He himself had already scanned the star-catalogues of Tycho Brahe, Johann Hevelius, John Flamsteed, and Tobias Mayer; and had come to suspect that a missing sixth magnitude star in the constellation Capricorn, observed by Tycho on 20 November 1589, might have been the planet. A second possibility which still required investigation was Mayer’s star No. 964, observed in Aquarius on 25 September 1756.

Type
History of the Discovery of Uranus
Copyright
Copyright © Cambridge University Press 1982

References

Notes

1. Astronomisches Jahrbuch für das Jahr 1784 nebst einer Sammlung der neuesten in die astronomischen Wissenschaften einschlagenden Abhandlungen, Beobachtungen und Nachrichten. Mit Genehmhaltung der KSnigl. Akademie der Wissenschaften berechnet und herausgegeben von J.E. Bode, Astronom der Akademie (Berlin, 1781). The abbreviated title of this periodical, adopted below, is Astr.Jahrb.

2. “Ueber einen im gegenwärtigen 1781sten Jahre entdeckten beweglichen Stern, den man für einen jenseits der Saturnsbahn laufenden, und bisher noch unbekannt gebliebenen Planeten halten kann”, ibid., pp.210-20. In a footnote on p.211 of this article, Bode gives the following five variants of Herschel’s surname that had appeared in the early French and English reports of the discovery: Mersthel, Hertschel, Herthel, Herrschell, and Hermstel.

3. Ibid., p.218.

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9. Astr.Jahrb. für 1785 (Berlin, 1782), p.189.

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11. Op.cit., note 7.

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13. Ibid., p.190.

14. “Aus einem Schreiben des Herrn Herschel an mien” (London, 13 August 1783), in Bode’s Astr.Jahrb. far 1786 (Berlin, 1783), p.258.

15. Méchain to Bode; Paris, 1 April 1784, in Bode’s Astr.Jahrb. für 1787 (Berlin, 1784), p.141.

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21. Op.cit., note 18, p.246.

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28. Op.cit., note 25, p.20.

29. Op.cit., note 6; vol.2, p.86.

30. Astr.Jahrb. für 1793 (Berlin, 1790), p.20.

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38. op.cit., note 34, p.412.

39. Op.cit., note 33, p.341.

40. Bessel, F.W. Fundamenta Astronomiae pro Anno MDCCIV deductaex Observationibus viri incomparabilis James Bradley in Specula Astronomica Grenovicensi per Annos 1750-1762 institutis (Regiomonti, 1818), p.283.Google Scholar Mayer’s observation of 25 September 1756 is reduced by Bessel on pp.284-5.

41. Breen, H., “On early Observations of Uranus by Bradley”, Monthly Notices of the Royal Astronomical Society 24 (1864), 1245.Google Scholar

42. These are discussed by their author in the second part of the introduction to his Tables Astronomiques publiées par le Bureau des Longitudes de France, contenant les Tables de Jupiter, de Saturne et d’Uranus, construites d’après la Théorie de la Méchanique céleste (Paris, 1821).

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45. Bessel, F.W., “Ueber die Verbindung der astronomischen Beobachtungen mit der Astronomie”, in Schumacher, H.C. (ed.), Populare Vorlesungen über wissenschaftliche GegenstSnde (Hamburg, 1848), p.452.Google Scholar

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50. ibid., p.131.

51. Le Verrier, U.-J.J., “Recherches sur les Mouvements de la Planète Herschel, dite Uranus”, Connaissance des Temps … pour l’An 1849 (Paris, 1846)Google Scholar; Additions, pp.1-254.

52. Detailed accounts of the circumstances surrounding this discovery are contained in Alexander, A.F.O’D., The Planet Uranus (London, 1965)Google Scholar and Grosser, Edward M., The Discovery of Neptune (Cambridge, Mass., 1962).Google Scholar

53. Op.cit., note 51, p.126. A table in ibid., p.129 contains the corrected mean times (based on the Paris meridian), the observed and calculated equatorial co-ordinates, and the residual differences in both these and the ecliptic coordinates.

54. This is taken from Edgar W. Woolard, “Comparison of the Observations of Uranus previous to 1781 with theoretical positions obtained by numerical integration”, The Astronomical Journal 57 (1952), 35-38. Compare his Table 1, p.36 with that in Le Verrier, op.cit., note 51, p.129.

55. Newcomb, S., “An Investigation of the Orbit of Uranus, with general Tables of its Motion”, Smithsonian Contributions to Knowledge No. 262, vol.19 (Washington [D.C.], 1874).Google Scholar

56. Safford, T.H., “On the Perturbations of Uranus and the Mass of Neptune”, Monthly Notices of the Royal Astronomical Society 22 (1862), 1424.CrossRefGoogle Scholar

57. Op.cit., note 54, p.37.

58. This can be appreciated by an inspection of the results of Newcomb’s reductions of Flamsteed’s observations; namely, for cases 1, 3, 4, 5 in Table II: -0?8, +5”; -0?1, -6”; +0?9. +2”; and -1?5, +10” respectively.

59. Rawlins, D., “A Long Lost Observation of Uranus: Flamsteed, 1714”, Publications of the Astronomical Society of the Pacific 80 (1968), 21719.CrossRefGoogle Scholar