The Process and Impact of Technological and Methodological Advances in Telescopes on the Detection and Analysis of Earth's Nutation in the 18th Century

Authors

  • Lucas Vinicius Antunes Universidade Federal do Rio de Janeiro https://orcid.org/0009-0005-8317-9302
  • Gerard Emile Grimberg Universidade Federal do Rio de Janeiro

DOI:

https://doi.org/10.23925/2178-2911.2025v32p90-117

Keywords:

History of the Telescope, nutation, Astronomy in the 18th Century

Abstract

This article examines research on the phenomena of nutation and precession during the first half of the 18th century. In this period, improvements in refracting telescopes allowed for more precise observational data, while the development of Leibnizian differential calculus applied to mechanics enabled the theoretical calculation of these motions. For the first time, nutation and precession became the subject of a systematic comparison between theoretical predictions and experimental data. The study is structured into three parts: the technological evolution of telescopes, the advancement of differential calculus in mechanics, and an analysis of the first theoretical results on these phenomena, obtained by D’Alembert in 1749 in his Recherches sur la précession des équinoxes, et sur la nutation de l’axe de la Terre, dans le système Newtonien.

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Published

2025-12-26

How to Cite

Vinicius Antunes, L., & Grimberg, G. E. (2025). The Process and Impact of Technological and Methodological Advances in Telescopes on the Detection and Analysis of Earth’s Nutation in the 18th Century. História Da Ciência E Ensino: Construindo Interfaces, 32, 90–117. https://doi.org/10.23925/2178-2911.2025v32p90-117

Issue

Section

Tópicos de História da Ciência