#26
by Calilasseia » Dec 11, 2011 3:14 am
As you take precise measurements at different point on the Earth's surface, you find that the value of g varies. Not by very much, but it does vary, and that variation is measurable. Moreover, that measurement is related to the basic equation for gravitational attraction, namely:
F = G Mm/r2
Where:
F is the force between the two gravitating objects
G is Newton's Universal Gravitational Constant (magnitude approximately 6.6 × 10-11)
M is the mass of one of the gravitating objects
m is the mass of the other gravitating object
r is the distance between those objects, or, more correctly, the distance between the centres of gravity of those objects.
Now, if we let M above be the mass of the Earth, and m be the mass of another object (e.g., a human being), then the force experienced by that other object is given by mg, where g is the acceleration due to gravity. Equating the two, we find that:
g = GM/r2
Since G and M are effectively constant, this leaves r as the varying parameter. Consequently, the larger the value of r, the smaller the value of g, and vice versa.
Of course, this elementary analysis neglects a range of effects, but is sufficient to establish why g is slightly greater at the poles than at the equator.
As for the matter of gravitational attraction being slightly greater at the summit of Everest than at sea level, first of all, what is meant here, is that the attraction is greater at the summit of Everest, than it is at a location on the Earth's surface at the same latitude as Everest. This is because, in effect, Everest constitutes a third gravitating body interspersed between ourselves and the rest of the planet. For once, this is a three body problem that is solvable, because all of the bodies are fixed in place, and we don't have to take the complexities of orbital mechanics into account in order to arrive at a reasonable solution. The general three-body problem is of course insoluble, at least from the standpoint of obtaining a closed form analytical solution - one can, however, obtain excellent numerical approximations, some of which are good enough to plot spacecraft trajectories for interplanetary missions. But I digress.
Of course, any precise determination of g at a given location will have to take into account a range of other quantities, such as the various dynamical form factors for Earth, and a host of other complications that I have omitted here, in order to arrive at a complete formula for any given part of the Earth's surface.
