Solar System Research

, Volume 47, Issue 6, pp 487–490

Experimental reconstruction of Lomonosov’s discovery of Venus’s atmosphere with antique refractors during the 2012 transit of Venus

Authors

  • A. Koukarine
  • I. Nesterenko
    • Budker Institute of Nuclear Physics
  • Yu. Petrunin
    • Telescope Engineering Company, Inc.
  • V. Shiltsev
    • Fermilab
Article

DOI: 10.1134/S0038094613060038

Cite this article as:
Koukarine, A., Nesterenko, I., Petrunin, Y. et al. Sol Syst Res (2013) 47: 487. doi:10.1134/S0038094613060038

Abstract

In 1761, the Russian polymath Mikhail Vasilievich Lomonosov (1711–1765) discovered the atmosphere of Venus during its transit over the Sun’s disc. In this paper we report on experimental reenactments of Lomonosov’s discovery with antique refractors during the transit of Venus June 5–6, 2012. We conclude that Lomonosov’s telescope was fully adequate to the task of detecting the arc of light around Venus off the Sun’s disc during ingress or egress provided proper experimental techniques as described by Lomonosov in his 1761 report are employed.

Copyright information

© Pleiades Publishing, Inc. 2013