- Mon Apr 16, 2007 7:43 pm
#221319
well...just a thought...basically we have:
- a planet's gravitational pull on its periphery, a function of mass vs. size ( about 9.m/s² @ ~4000mi radius for Earth )
vs.
- centrifugal force ( Earth's rotational speed is 15deg/h, or ~1000mph @ 4000mi radius )
- external gravitational pull from other celestial bodies
For a planet to remain constant size, these factors would need to be in perfect balance...what exactly are the real chances of that?
Regarding Earth's gravity in a historical sense, I don't believe the theory asserts that Earth's mass has changed appreciably ( how could it change...lots of meteors? ), just it's diameter. Observed gravitational force would be greater at the surface of a smaller sphere of equivalent mass ( gravitational force varies inverse to the square of distance from a body of given mass ). However, this would likely be offset by a greater rotational speed...given a constant mass, as diameter increases, rotational speed would naturally decrease. Therefore, assuming his theory is correct, observed gravitational force at any point in history is most likely not possible to accurately predict, but may not necessarily be much different than it is for the current rotation/diameter.
Either way, at first glance, this interesting theory surely makes more sense to me than any I've previously heard...but I'm no scientist...
Next Limit Team