  Galaxy and galaxy clusters exhibit tight robust physical scaling relations
between baryons and system dynamics. One such phenomenon is mass discrepancy
with two leading solution spaces occupied by LCDM and MOND. Here, we propose an
alternative solution to this puzzling problem exclusively based on application
of the scalar virial theorem. For these dynamically equilibrated systems, we
demonstrate there is ample virially-induced kinetic energy available to modify
bulk structure dynamics in apparent violation of Newtonian law. We propose the
ubiquitous Baryonic Tully-Fisher Relation represents the preferred dynamic
configuration that best assures long-term survivability for these thermodynamic
quasi-equilibrated systems. We compare total mass estimates guided by the
empirical evidence to those obtained from NFW dark matter halo fits ranging
from small dwarf galaxies to massive galaxy clusters.
