{"title":"G.B.里乔利的地心说运用了本轮、椭圆和螺旋","authors":"F. Marcacci","doi":"10.1177/00218286231165331","DOIUrl":null,"url":null,"abstract":"According to Giovanni Battista Riccioli (1598–1671), planets describe orbits in a fluid heaven in a helio-geocentric model of cosmos. In his Almagestum Novum (1651) he stresses the need for a novel and rigorous geometrical explanation for the motion of heavenly bodies, which considers a separate Primum Mobile as an unnecessary hypothesis. Riccioli rejects the standard eccentric-epicycle theory as unsatisfactory and argues for what he calls “Eccentrepicyclos” or “Epicepicycles.” He takes the Keplerian elliptical theory into account and includes a variable oscillation of both the mobile eccentric center and the variation of the epicycle’s diameter. As a result, planets move along spiral orbits that have variable sizes. The inequalities, which astronomers had always tried to explain, are now justified: the spiral trajectory, obtained by means of the oscillation of the eccentric center, warrants the first inequality, about the variation of the planets’ velocity. The variable amplitude of the spirals, obtained by the variation of the epicycle’s diameter, explains the second inequality, namely the apparent retrograde or progressive planetary motion. In the later work Astronomia Reformata (1665), Riccioli uses explicitly the term “ellipse.” Riccioli’s innovations are of great interest and help to understand the complexity of the astronomical debates about the best world-system.","PeriodicalId":56280,"journal":{"name":"Journal for the History of Astronomy","volume":"54 1","pages":"171 - 192"},"PeriodicalIF":0.3000,"publicationDate":"2023-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"G.B. Riccioli’s geo-heliocentric use of Epicepicycles, ellipses and spirals\",\"authors\":\"F. Marcacci\",\"doi\":\"10.1177/00218286231165331\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"According to Giovanni Battista Riccioli (1598–1671), planets describe orbits in a fluid heaven in a helio-geocentric model of cosmos. In his Almagestum Novum (1651) he stresses the need for a novel and rigorous geometrical explanation for the motion of heavenly bodies, which considers a separate Primum Mobile as an unnecessary hypothesis. Riccioli rejects the standard eccentric-epicycle theory as unsatisfactory and argues for what he calls “Eccentrepicyclos” or “Epicepicycles.” He takes the Keplerian elliptical theory into account and includes a variable oscillation of both the mobile eccentric center and the variation of the epicycle’s diameter. As a result, planets move along spiral orbits that have variable sizes. The inequalities, which astronomers had always tried to explain, are now justified: the spiral trajectory, obtained by means of the oscillation of the eccentric center, warrants the first inequality, about the variation of the planets’ velocity. The variable amplitude of the spirals, obtained by the variation of the epicycle’s diameter, explains the second inequality, namely the apparent retrograde or progressive planetary motion. In the later work Astronomia Reformata (1665), Riccioli uses explicitly the term “ellipse.” Riccioli’s innovations are of great interest and help to understand the complexity of the astronomical debates about the best world-system.\",\"PeriodicalId\":56280,\"journal\":{\"name\":\"Journal for the History of Astronomy\",\"volume\":\"54 1\",\"pages\":\"171 - 192\"},\"PeriodicalIF\":0.3000,\"publicationDate\":\"2023-05-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal for the History of Astronomy\",\"FirstCategoryId\":\"98\",\"ListUrlMain\":\"https://doi.org/10.1177/00218286231165331\",\"RegionNum\":3,\"RegionCategory\":\"哲学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"HISTORY & PHILOSOPHY OF SCIENCE\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal for the History of Astronomy","FirstCategoryId":"98","ListUrlMain":"https://doi.org/10.1177/00218286231165331","RegionNum":3,"RegionCategory":"哲学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"HISTORY & PHILOSOPHY OF SCIENCE","Score":null,"Total":0}
G.B. Riccioli’s geo-heliocentric use of Epicepicycles, ellipses and spirals
According to Giovanni Battista Riccioli (1598–1671), planets describe orbits in a fluid heaven in a helio-geocentric model of cosmos. In his Almagestum Novum (1651) he stresses the need for a novel and rigorous geometrical explanation for the motion of heavenly bodies, which considers a separate Primum Mobile as an unnecessary hypothesis. Riccioli rejects the standard eccentric-epicycle theory as unsatisfactory and argues for what he calls “Eccentrepicyclos” or “Epicepicycles.” He takes the Keplerian elliptical theory into account and includes a variable oscillation of both the mobile eccentric center and the variation of the epicycle’s diameter. As a result, planets move along spiral orbits that have variable sizes. The inequalities, which astronomers had always tried to explain, are now justified: the spiral trajectory, obtained by means of the oscillation of the eccentric center, warrants the first inequality, about the variation of the planets’ velocity. The variable amplitude of the spirals, obtained by the variation of the epicycle’s diameter, explains the second inequality, namely the apparent retrograde or progressive planetary motion. In the later work Astronomia Reformata (1665), Riccioli uses explicitly the term “ellipse.” Riccioli’s innovations are of great interest and help to understand the complexity of the astronomical debates about the best world-system.
期刊介绍:
Science History Publications Ltd is an academic publishing company established in 1971 and based in Cambridge, England. We specialize in journals in history of science and in particular history of astronomy.