Abstract
In a letter of 27 October 1604, David Fabricius (1564–1617) eagerly reported to Johannes Kepler (1571–1630) his observations of a brilliant new luminary in the constellation of Sagittarius. Fabricius had first observed the new luminary “near the location of the great conjunction,”1 which had occurred just 10 months earlier. His eyes had been drawn to the area by the proximity of the three superior planets when “Mars and Jupiter were conjoined and Saturn had by then returned directly to the location of the great conjunction.”2 There, Fabricius had identified “a new star, with no motion of its own,” in the outer sphere encasing the cosmos.3 The star had surpassed Jupiter “in diameter and silvery splendor,”4 and its scintillation had proven incomparably swift.
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Acknowledgements
This paper proceeds from a postdoctoral fellowship with the National Science Foundation, “The Supernova of 1604 as a Source of Scientific Debate” (no. 0749138). I would like to thank the many individuals whose comments and suggestions contributed to the improvement of it. I am especially grateful to Miguel A. Granada, Robert A. Hatch, and Lawrence M. Principe for their editorial insight.
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© 2011 Springer Science+Business Media B.V.
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Boner, P.J. (2011). Kepler’s Copernican Campaign and the New Star of 1604. In: Boner, P. (eds) Change and Continuity in Early Modern Cosmology. Archimedes, vol 27. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-0037-6_6
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DOI: https://doi.org/10.1007/978-94-007-0037-6_6
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