The close-approach of the Sun by asteroid 2000 B19 provides further evidence for MOdified Newtonian Dynamics (MOND) and Asymmetric Near-Field (ASNF) gravity by observational data, which shows added acceleration along the elliptical orbit trajectory between the Sun's L1 point with the galaxy and the asteroid perihelion on November 5, 2021. This research posits that the object should increase in velocity due to MOND acceleration of 2.5 x 10-11 m/sec 2 during the approach to perihelion, which can generate an additional velocity of ~8 m/sec that is measurable as a displacement along the elliptical orbit, resulting in an early passage through perihelion. Previous research already postulated that the anomalous acceleration of asteroid 1I/2017 U1 was clearly explainable by MOND acceleration in the solar flyby of that object, without exotic speculative scenarios. Herein is included an analysis of the ephemeris data of BD19 from NASA/JPL, which we then use to predict the MOND effect in the observational data.