A tool for furnishing observations of planetary satellites with epheme
rides has been developed and is being distributed for practical use. A
new approach to obtaining ephemerides has been adopted. Instead of ta
bles with satellite coordinates, a computer program with a user-friend
ly interface has been written which displays the apparent positions of
planetary satellites in graphical and digital forms. The coordinates
are not calculated in advance to be stored; rather, the program comput
es them instantaneously for any given time. Visibility conditions for
a planet at a specified observatory, including topocentric coordinates
of the planet, Sun, Moon, and phases of the Moon are simultaneously d
etermined and displayed. Mutual occultations and eclipses of the satel
lites are automatically detected, and decline in their brightness is c
omputed during these events.