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Gaia HyperVelocity Star (HVS) kinematic observations favor a local escapevelocity of ~700 km/s, nearly forty-percent greater than conventionalestimates. Combining HVS and dwarf galaxy satellite data reveal the globalescape velocity profile for the Galaxy smoothly traces an unbroken Kepleriandecline from the central bar to the most remote satellite galaxy. We reveal arobust upper bound in baryonic mass discrepancy (maximal relativeaccelerations) linked to the virial theorem and obtain a fundamental anduniversal mass discrepancy-acceleration relation for virialized compact cosmicobjects.

The Global Escape Velocity Profile and Virial Mass Estimate of The Milky Way Galaxy from Gaia Observations