scholarly journals Bearing the Heavens: Tycho Brahe and the Astronomical Community of the Late Sixteenth Century

1969 ◽  
Vol 32 (3) ◽  
pp. 128-130
Author(s):  
Adam Mosley (book author) ◽  
Piers Brown (review author)
1965 ◽  
Vol 3 (2) ◽  
pp. 81-81
Author(s):  
J. L. E. Dreyer ◽  
Robert T. Lagemann

1980 ◽  
Vol 11 (2) ◽  
pp. 114-129
Author(s):  
Michel-Pierre Lerner

Taking as his starting point a passage by G. B. Riccioli (1598–1671), the author investigates those writers in the sixteenth century who postulated that the Sun rotates—that is, prior to the observational proof by Galileo. The idea of the axial rotation of the Sun was proposed in Antiquity by Plato but strongly resisted by Aristotle. It reappears in the writings of the anti-Aristotelean philosopher Bernardino Telesio (1509–88), for whom it was a necessary consequence of his conception of a Sun formed of fire. But other pre-telescopic authors, such as Cesalpino, Bruno, Campanella, and Kepler, likewise proposed the rotation of the Sun as required for one reason or another, although at the close of the sixteenth century Tycho Brahe (who of course had no telescope) rejected such a rotation as an optical illusion.


1965 ◽  
Vol 2 (4) ◽  
pp. 291-296 ◽  
Author(s):  
Christine Schofield

It has become generally accepted that the earliest geoheliocentric representation of the planets' motions in which the majority of the planets orbited about the Sun appeared in 1588. For in this year the Danish astronomer Tycho Brahe announced his discovery of a new system of the world, in which Sun and Moon moved about the Earth, and the five planets Mercury, Venus, Mars, Jupiter and Saturn performed their motions about the Sun. Yet the accompanying figure, which depicts a planetary arrangement in general identical with that of Tycho, occurs in a manuscript prepared at least a year before Tycho's publication of his system. Moreover, the author of the manuscript derived this representation of the planets' motions not from Tycho, but rather from Copernicus. The aim of this paper is to show that as a result of the work of Copernicus, a number of sixteenth-century mathematicians produced treatments of the planetary motions similar to the system proposed by Tycho in 1588.


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