The evidence for resonant structure in the distribution of the semimaj
or axes of members of asteroid families and meteoroid streams is revie
wed. It is shown that, because families and streams are identified by
clustering of orbital elements, great care must be taken to distinguis
h between actual removal of objects ('real' gaps) and the failure to i
dentify members of families or streams because of resonant perturbatio
ns ('imaginary' gaps). If it can be shown that gaps are real then this
can lead to important constraints on the time-scale for the removal o
f objects. Sample variations of semimajor axis and eccentricity are ca
lculated for resonant locations in the Themis asteroid family and the
Quadrantid meteoroid stream using high-order expansions of the planeta
ry disturbing function. Evidence is presented suggesting that a promin
ent gap in the Themis family associated with the 15:7 jovian resonance
is real, whereas that associated with the 3:1 resonance in the Quadra
ntid meteors is imaginary. Recent claims concerning resonant structure
in the Perseid meteor stream are examined in a similar context.