A very important step for the acquisition of accurate orbital information o
f near Earth asteroids (NEAs) is the recovery process. About one-third of t
he known NEAs have been observed for more than one opposition. We studied t
he circumstances of the recovery of all NEAs with atleast two oppositions a
nd found that there are several ways to find observations of a different op
position from that of the discovery. We divided all the recoveries into fou
r different classes. Following the observations at the new opposition, we c
oncluded that planning observations at the telescope is still the best way
to hope to observe NEAs at a new opposition. At the same time we reached th
e conclusion that a large number of NEA observations are still to be found
in existing archival astronomical records. (C) 2000 Elsevier Science Ltd. A
ll rights reserved.