  We have developed a methodology to test the age-old cosmic censorship
hypothesis in Kerr geometry. We have shown that the Kerr black hole can be
overspun by particles captured from the innermost stable circular orbit.
However, it appears that this does not happen for particles coming from
infinity. We have also observed that overspinning becomes possible only when
the black hole approaches a near-extremal limit, which approaches as we
increase the black hole's mass. Our study demonstrates that an extremal black
hole cannot be overspun. However, our methodology neglects backreaction and
self-force effects, which could affect the overspinning.
