IAU/IHW filter set is used to study the polarization in Comet Hyakutak
e in various molecular bands. The observations were taken on March 13.
97 and March 18.88 UT dates using 1.2 m telescope at Mount Abu Observa
tory, India. The errors in the measurement of the percent polarization
are very low (<0.5%). The phase dependence of the polarization of C-2
and CN molecular emission bands due to resonance fluorescence is in g
ood agreement with theory. However, the observed polarization in C-3 m
olecular band is found to be about 3% which is less than the predicted
value. In the case of CN molecule, significant deviation is noticed i
n the direction of polarization vector from normal to the plane of sca
ttering.