  In this work, we study the Mazur and Mottola gravastar model within the
context of Randall-Sundrum II type braneworld scenario, based on the fact that
our four dimensional space-time is a three-brane, embedded in a five
dimensional bulk. We present exact solutions of the modified field equations in
each of the three regions making up the gravastar, namely, (I) the core, (II)
the shell, and (III) the vacuum exterior. The junction conditions at each
interface are fulfilled and we further explore interesting physical properties
such as length and energy and entropy of the spherical distribution.
