We present proper-motion measurements of the bipolar lobes and equatorial d
isk features ejected from eta Carinae during the last century and deduce th
eir relative ages in order to determine the likelihood of multiple ejection
events. Hubble Space Telescope Wide Field Planetary Camera 2 images taken
in 1994, 1995, and 1999 were compared, and the motions of small (similar to
1 ") patches throughout the nebula were measured. Assuming that the materia
l has not been accelerated or decelerated, the projected expansion velociti
es of both lobes and two equatorial features (the "Paddle" and regions in t
he NN Jet) indicate that the bipolar lobes and fast equatorial ejecta have
the same origin date, some 150 years ago during the Great Eruption. We also
conclude that the ejection of the partial shell of outer debris preceded t
he Great Eruption by at least several decades or possibly a century, confir
ming that the nebula surrounding eta Car represents at least two outburst e
vents and maybe more.