  Polytropes have long been used to model a wide variety of astrophysical
objects. A bipolytrope (composite polytrope) may be used for bodies with a
distinct core-envelope structure. In this short paper, I demonstrate that a
rotating bipolytrope is a reasonable approximation for Jovian interior. Similar
models may be used to probe rotating exoplanets to gain an intuitive
understanding of their internal structure.
