Faint Satellites of Outer Planets

Details Faint Satellites of Outer Planets Faint Satellites of Outer Planets

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982msngr..27...25v&link_type=abstract

The Messenger, No.27, P. 25, 1982

Astronomy and Astrophysics

Astronomy

Scientific paper

In astronomy, as in other matters, the charm 01 novelty is one of the important lactors that govern the choice 01 the observations. How many objects saw suddenly many eyes or kinds of detectors looking at them, before linding again, some months or years later, their sidereal quietness! ... However, it is often after a long time of regular observations that they confide a (small) part 01 their secrets. The laint satellites 01 planets don't transgress this fortunately approximative rule. The deliciency in observations during many consecutive years makes the determination 01 their motion very difficult, and it is olten too late to make up lor lost time. We shall try to i1lustrate this lact in the next lines using the observations of the systems of Saturn, Uranus and Neptune we made in April 1981 on the DanishESO 1.5-m reflector.

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