From reanalysis of 17th century and 20th century eclipse observations,
with three different models for the earth's rotation, and from the us
e of both longitude comparison and mean motion comparison, we find tha
t Io has a fractional acceleration of (4.54+/-0.95)x10(-10) yr(-1). If
Io can be considered a Keplerian oscillator, its orbital semi-major a
xis decreases by 13 cm/yr. (C) 1995 American Astronomical Society.