  Recent experimental results for the gravitational constant G from
Cavendish-type experiments were analysed in the framework of Modified Newtonian
Dynamics (MOND). MOND corrections were applied to the equation of motion of a
pendulum, under the assumption that the magnitude of the horizontal time
dependent gravitational acceleration determines the amount of MOND corrections.
The large vertical component of the local gravitational field of the earth is
fully compensated by the alignment of the torsion pendulum in accordance with
Newtons third law and therefore not considered for MOND corrections. From the
analysis of the MOND corrected equation of motion of a realistic torsion
pendulum with mixed gravitational and electromagnetic restoring torque simple
rules for meaningful MOND corrections of measured G values determined by
different operational modes of Cavendish type G experiments were derived. Based
on this analysis the reported discrepancies for G determined by static
deflection and electrostatic servo methods of the BIPM experiment by Quinn et
al. and between time-of-swing and angular acceleration feedback methods for the
HUST experiment by Li et al. could be fully resolved by MOND corrections using
one common MOND interpolation function, determined by a one parameter fit. The
MOND corrected BIPM and HUST results, along with other single method results
from G experiments by Gundlach and Merkovitz, Schlamminger et al. and Newman et
al. lead to an average G value of 6.67422x10^-11 m^3 kg^-1 s^-2 with a standard
deviation of 12.5 ppm only. The applied MOND correction procedure and the
fitted interpolation function employed for the G experiments were found to be
consistent with the most viable MOND fits to galaxy rotation curves.
