  During the 2016 International Workshop on Astronomy and Relativistic
Astrophysics (IWARA), the question was raised as to if conformal gravity could
explain the timely result of McGaugh et. al. 2016 which showed a universal
nature found in the centripetal accelerations of spiral galaxies. At the time
of the conference, the McGaugh result was only published for two weeks. Since
then, the result has become known as the Radial Acceleration Relation (RAR) and
has been considered tantamount to a natural law. In this work, we summarize how
conformal gravity can explain the Radial Acceleration Rule in a fashion
consistent with the findings of the original authors without the need for dark
matter.
