The no-hair theorem characterizes the fundamental nature of black holes in general relativity. This theorem can be tested observationally by measuring the mass and spin of a black hole as well as its quadrupole moment. which may deviate from the expected Kerr value. Sgr A*. https://www.markymarkscott.com/product-category/classic-76-clipper-blade/
CLASSIC 76 CLIPPER BLADE
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