We will learn to calculate Newton’s classical force of gravity in a new quantummechanical (h-based) way. (Einstein’s general relativity obtains the same classical result as Newton.) Just 8 steps are required: 1) Calculate Newtonian classical gravity for absolutely any situation. Fgravity=Gm1m2- /r2 , where G=6.6728674 X 10-8 cm3 /gmsec2 ; m1 and m2 are the 2 masses; r is the distance between them; cm=centimeter; gm=gram; and sec=second. 2) Separately, take ANY MASS AT ALL - - m - - and set it equal to 1. 3) Set m’s de Broglie wavelength - - λ - - equal to ─1. 4) Set the time, t, taken for light to travel λ (=λ/c) equal to √−1. 5) Calculate a numerical value for the three c-g-s units via steps 2), 3) and 4) respectively. 6) Calculate G using these new unit equivalencies, resulting in a positive number result. (t2 will cancel ─1 because t = √−1]. Call this result y. 7) Recalculate step 1), REPLACING G with y, and REPLACING the c-g-s units with the new unit equivalencies, resulting in another positive number. Call it n. 8) Calculate nh/λt. This quantum-mechanical term will ALWAYS be exactly equal to the classical gravity, Gm1m2/r2 , calculated in step 1) (minus late-decimal rounding.) This will ALWAYS be true FOR ANY AND ALL m1,m2, r, m, λ and t.