It’s been bothering me that we’ve been neglecting, or at least glossing over, the effect of the Earth’s rotation. I get this effect to be 11.05 km at the Earth’s center at 45 degrees latitude; fully half the difference between down and the direction to the Earth’s center is due to the Earth’s rotation. Presumably, the other half comes from the Earth’s mass distribution.
For the effect of the Moon, I get less than a meter difference at the Earth’s center, and even this amount would tend to average to zero over time, so it can be neglected. Since the Moon causes the biggest tide, the other solar system masses are even more negligible.
If you’re not interested in the math, skip the rest of this message:
gmass = 980 cm/s^2 radially
grot = 3.39 cm/s^2cos(theta) away from axis of rotation (rhodially?
)
The angle gmass + grot pulls is atan(gmass sin(theta) / ((gmass+grot)cos(theta))
= atan(1.00347 tan(theta))
= 45.09927 degrees at theta = 45 degrees
So the difference of 0.09927 degrees is the effect on “down” due to the Earth’s rotation. Converting to the difference at the Earth’s center gives 6378 * tan(0.09927) = 11.05 km.
The effect of the moon’s gravity will be smaller than the effect of the Earth by the factor
(Mmoon/MEarth) * (Rearth/Dmoon)^2 * (2 * REarth / Dmoon)
where Mmoon, MEarth are the moon and Earth masses, REarth is the Earth Radius, and Dmoon is the distance to the moon. The last factor
comes from the acceleration we care about being the difference between the acceleration at the Earth center and our location on the surface. This is the worst case number.
Using Mmoon/Mearth = 0.013, Dmoon/Rearth = 60, the Moon’s acceleration relative to Earth is smaller by 1.2E-7, less than a meter difference at the Earth’s center.
It is too clear, and so it is hard to see.