Optical photometric observations of the blazar 3C 371 are presented as part
of an ongoing study of variations in blazars occurring on timescales of mi
nutes to hours, which has been termed microvariability. The observations pr
esented here provide further evidence of the classwide nature of this pheno
menon. Timescales as short as these provide important clues about the natur
e of blazars, and a discussion of the types of possible mechanisms responsi
ble for producing these variations is given.