  We compute the proper time Lyapunov exponent for charged Myers Perry black
hole spacetime and investigate the instability of the equatorial circular
geodesics (both timelike and null) via this exponent. We also show that for
more than four spacetime dimensions $(N \geq 3)$, there are \emph{no} Innermost
Stable Circular Orbits (ISCOs) in charged Myers Perry black hole spacetime. We
further show that among all possible circular orbits, timelike circular orbits
have \emph{longer} orbital periods than null circular orbits (photon spheres)
as measured by asymptotic observers. Thus, timelike circular orbits provide the
\emph{slowest way} to orbit around the charged Myers Perry black hole.
