  Using a yukawa type of metric we derive the kretschmann scalar for a general
static black hole of a certain mass. The scalar gives the curvature of the
space time as a function of the radial distance in the vicinity as well as
inside of the black hole. Furthermore, the kretschmann scalar helps us
understand the appearance of the black hole as a whole entity. It can be
applied in solar mass size black holes, neutron stars or super massive black
holes at the center of various galaxies. In an effort to investigate the
connection of geometry to entropy and information, the kretschmann scalar for a
solar mass yukawa schwarzschild and simple schwarzschild black holes are
derived. Moreover, the dependence of the curvature on the entropy and number of
information in nats is derived.
