The infrared space observatory (ISO) observed many asteroids in great detai
l., including near-Earth asteroids (NEA). Additionally, a large number of o
bserving programmes contain serendipitous observations of known and unknown
solar system objects (SSO). The ISO specific constraints, like sensitivity
, visibility and orbit parallax and their consequences for SSO extraction a
re presented. Model calculations demonstrate the efficiency and effectivene
ss of space-based infrared programmes for investigations of SSOs. Four larg
e ISO programmes have been analyzed and first results from the SSO search a
re discussed. The possibilities and limits of ISO with respect to near-Eart
h objects (NEO) are briefly mentioned. (C) 2001 Elsevier Science Ltd. All r
ights reserved.