TurtleMeister said:
Here's the Wikipedia page for that equation:
https://en.wikipedia.org/wiki/Free-fall_time
Thank you TurtleM for the derivation...
The usual (standard) Kepler eqn. that I was trying to reconstruct by squaring your equation is;
T^2 / R^3 = 4(pi)^2 / G(M+m) ... but apparently the factor 1/32 kept appearing..
I think this clears it up here:(from your article)...
"Note that T (orbit) in the above equation, is the time for the mass to fall in a highly eccentric orbit, make a "hairpin" turn at the central mass at nearly zero radius distance, and then returns to
R when it repeats the very sharp turn.
This orbit corresponds to nearly linear motion back and from distance R to distance 0. As noted above, this orbit has only half as long a semimajor axis (R/2) as a circular orbit with radius R (where the semimajor axis is
R), and thus the period for the shorter high-eccentricity "orbit" is that for one with an axis of
R/2 and a total orbital pathlength of only twice the infall distance. Thus, by Kepler's third law, with half the semimajor axis radius it thus takes only (1/2)3/2 = (1/8)1/2 as long a time period, as the "corresponding" circular orbit that has a constant radius the same as the maximal radius of the eccentric orbit (which goes to essentially zero radius from the primary at its other extreme).
The time to traverse half the distance R, which is the infall time from R along an eccentric orbit, is the Kepler time for a circular orbit of R/2 (not R), which is (1/32)1/2 times the period P of the circular orbit at R. For example, the time for an object in the orbit of the Earth around the Sun, to fall into the Sun if it were suddenly stopped in orbit, would be P / (sq.rt.32) where
P is one year..."
Since the first equation (Point masses) is somewhat useless, I included the free fall oscillating in a hole of a Large Mass and concluded it would be equivalent to Kepler's Orbital eqn. for uniform mass density...
They derived a similar result (there is an equivalent equation as the pt. mass eqn.) for extended mass of uniform mass distribution... if M >> m.
Quite interesting...thanks for the link.
Pet Scan