  Noncommutative geometry is one of the quantum gravity theories, which various
researchers have been using to describe different physical and astrophysical
systems. However, so far, no direct observations can justify its existence, and
this theory remains a hypothesis. On the other hand, over the past two decades,
more than a dozen over-luminous type Ia supernovae have been observed, which
indirectly predict that they originate from white dwarfs with
super-Chandrasekhar masses $2.1-2.8 \rm\,M_\odot$. In this article, we discuss
that considering white dwarfs as squashed fuzzy spheres, a class of
noncommutative geometry, helps in accumulating more mass than the Chandrasekhar
mass-limit. The length-scale beyond which the effect of noncommutativity
becomes prominent is an emergent phenomenon, which depends only on the
inter-electron separations in the white dwarf.
