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In his Chronology, Newton uses astronomical "evidence" to support its extreme rejuvenation of ancient times. These elements, having a scientific varnish, provide some credibility to the work. They have been fiercely debated for a century,…

物理学史与哲学 · 物理学 2013-11-20 Yael Naze

Ptolemy-s planetary model is an ancient geocentric astronomical model, describing the observed motion of the Sun and the planets. Ptolemy accounted for the deviations of planetary orbits from perfect circles by introducing two small and…

物理学史与哲学 · 物理学 2015-03-11 Ilia Rushkin

In late antiquity and throughout the middle ages, the positions of stars on the celestial sphere were obtained from the star catalogue of Ptolemaios. A catalogue based on new measurements appeared in 1437, with positions by Ulugh Beg, and…

天体物理仪器与方法 · 物理学 2015-06-05 Frank Verbunt , Robert H. van Gent

Four hundred years after its publication, Galileo's masterpiece Sidereus Nuncius is still a mine of useful information for historians of science and astronomy. In his short book Galileo reports a large amount of data that, despite its age,…

物理学史与哲学 · 物理学 2012-06-20 Enrico Bernieri

The celestial phenomenon have always been a source of wonder and interest to people, even as long ago as the ancient Egyptians. While the ancient Egyptians did not know all the things about astronomy that we do now, they had a good…

天体物理学 · 物理学 2011-08-23 Bojan Novakovic

The geocentric universe, in its most developed form as set out by Ptolemy, was a remarkably successful and coherent theory. It did not, however, specify the order of the planets, that is, which was closer to Earth and which farther away.…

科普物理 · 物理学 2023-05-11 Alan B. Whiting

Observational cosmology of the first decades of the Twentieth Century was dominated by two giants: Edwin Hubble and Harlow Shapley. Hubble's major contributions were to the study and classification of individual galaxies with large…

物理学史与哲学 · 物理学 2011-10-12 Sidney van den Bergh

Galileo Galilei believed that stars were distant suns whose sizes, measured via his telescope, were a direct indication of distance -- fainter stars (appearing smaller in the telescope) were farther away than brighter ones. Galileo argued…

物理学史与哲学 · 物理学 2009-07-27 Christopher M. Graney , Henry Sipes

The history of astrometry, the branch of astronomy dealing with the positions of celestial objects, is a lengthy and complex chronicle, having its origins in the earliest records of astronomical observations more than two thousand years…

物理学史与哲学 · 物理学 2015-06-11 Michael Perryman

This is a historian's view of how modern astronomy data can be used to discuss the shifting historical worldview of Late Antiquity. In this article an attemp is made to construct an approximate model of how the cycles of astronomical…

物理学史与哲学 · 物理学 2024-03-07 D. N. Starostin

One of the greatest discoveries of modern times is that of the expanding Universe, almost invariably attributed to Hubble (1929). What is not widely known is that the original treatise by Lemaitre (1927) contained a rich fusion of both…

物理学史与哲学 · 物理学 2015-05-28 David L. Block

What are the historical evidence concerning the turning of the spyglass into an astronomical instrument, the telescope? In Sidereus Nuncius and in his private correspondence Galileo tells the reader what he did with the telescope, but he…

物理学史与哲学 · 物理学 2014-04-14 Yaakov Zik , Giora Hon

The handed down latitudinal data ascribed to Eratosthenes and Hipparchus are composed and each tested for consistency by means of adjustment theory. For detected inconsistencies new explanations are given concerning the origin of the data.…

物理学史与哲学 · 物理学 2015-11-17 Christian Marx

Astrometry, the most ancient branch of astronomy, was facing extinction during much of the 20th century in the competition with astrophysics. The revival of astrometry came with the European astrometry satellite Hipparcos, approved by ESA…

天体物理仪器与方法 · 物理学 2014-08-12 Erik Høg

Edwin Hubble is famous for a number of discoveries that are well known to amateur and professional astronomers, students and the general public. The origins of these discoveries are examined and it is demonstrated that, in each case, a…

物理学史与哲学 · 物理学 2013-01-31 Michael J. Way

The current system of stellar magnitudes first introduced by Hipparchus was strictly defined by Norman Robert Pogson in 1856. He based his system on Ptolemy's star catalogue `Almagest', recorded in about 137 A.D., and defined the…

天体物理学 · 物理学 2007-05-23 Tomoko Fujiwara , Hitoshi Yamaoka

Several scholars have accorded the Tychonic System a prominent place, considering it a credible alternative to the Ptolemaic and Copernican systems. In recent years, there have even been some enthusiastic contributions in support of Brahe,…

物理学史与哲学 · 物理学 2026-05-29 Gabriele Vanin

Galileo determined distances to stars based on the assumption that stars were suns, the apparent sizes of stars as seen through his telescope, and basic geometry. However, the apparent sizes that he measured were the result of diffraction…

物理学史与哲学 · 物理学 2009-07-27 Christopher M. Graney

The principle that celestial bodies must move on circular orbits or on paths resulting from the composition of circular orbits has been assumed as a constant guide in the astronomical thougth of the peoples facing the Mediterranean sea as…

物理学史与哲学 · 物理学 2007-05-23 Dino Boccaletti

In "On the Heavens" Aristotle criticizes the Pythagorean point of view which claims the existence of a cosmic music and a cosmic sound. According to the Pythagorean argument, there exists a cosmic music produced by stars and planets. These…

物理学史与哲学 · 物理学 2017-09-20 J. C. S. Neves