  In this paper, we revisit the experimental constraints on the multipolar dark
matter that has derivative coupling to the visible sector mediated by the
Standard Model photon. The momentum dependent interaction enables them to be
captured efficiently within massive celestial bodies boosted by their steep
gravitational potential. This phenomena makes compact celestial bodies as an
efficient target to probe such type of dark matter candidates. We demonstrate
that a synergy of the updated direct detection results from DarkSide-50 and
LUX-ZEPLIN together with IceCube bounds on high energy solar neutrinos from
dark matter capture disfavour the viable parameter space of the dipolar dark
matter scenario. Whereas, for the anapole dark matter scenario, a narrow window
survives that lies within the reach of prospective heating signals due to the
capture of dark matter at cold neutron stars.
