It is argued that the term 'meteoroid' is best defined as being applic
able to any natural solid object moving in space, and having a size be
tween 100 mu m and Iom (10(-4)-10(1) m). This definition reflects mode
rn-day instrumentation limitations and recognizes the physical constra
ints that dictate the production of a meteor in the Earth's atmosphere
. Our argument also has implications for the definitions of the terms
'asteroid' (synonym 'minor planet'), 'micrometeorite', and 'interplane
tary dust.'