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The recently proved `no short hair' theorem asserts that, if aspherically-symmetric static black hole has hair, then this hair (the externalfields) must extend beyond the null circular geodesic (the "photonsphere") ofthe corresponding black-hole spacetime: $r_{\text{field}}>r_{\text{null}}$. Inthis paper we provide compelling evidence that the bound can be {\it violated}by {\it non}-spherically symmetric hairy black-hole configurations. To thatend, we analytically explore the physical properties of cloudy Kerr-Newmanblack-hole spacetimes -- charged rotating black holes which support linearizedstationary charged scalar configurations in their exterior regions.

Extremal Kerr-Newman black holes with extremely short charged scalar hair