Long term light variations of Io and Titan

Details Long term light variations of Io and Titan Long term light variations of Io and Titan

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..103b&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, Mar. 1977, p. 103-108.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Io, Light Curve, Secular Variations, Titan, Electrophotometry, Luminous Intensity, Perihelions, Satellite Orbits

Scientific paper

A long-term variation of the V magnitude at mean opposition of Io and
Titan is shown to be correlated with the orbital motion of Jupiter and
Saturn respectively. The amplitude of the variation is about 0.2 m for
both satellites. The maximum of brightness occurs near the perihelion of
the respective planet.

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