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I am trying to answer this Phys.SE question but got an unreasonable answer:

In making laboratory measurements of $g$, how precise does one have to be to detect diurnal variations due to the moon's gravity? [Clarifications omitted.]

I figured I can calculate the change in GPE for a test mass

$$GPE_{earth} - GPE_{moon}$$ at apogee and perigee, and take a ratio to see how many significant figures are affected.

Where $d$ is lunar distance,

$$\frac{m(g_{earth}R_{earth}-g_{moon}d_{min})}{m(g_{earth}R_{earth}-g_{moon}d_{max})} = \frac{m_{earth}R_{earth}-m_{moon}d_{min}}{m_{earth}R_{earth}-m_{moon}d_{max}}$$

I asked Wolfram Alpha to calculate this and got a ratio of about 1.4, which seems unreasonable.

What has gone wrong?

Qmechanic
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spraff
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  • Diurnal means during a day. Has nothing to do with perigee and apogee. Terms that refers to position of Earth around the Sun anyway. 2. Your formula looks wrong. What happens with the g earth and g moon in the second half? 3. Question is about variations in g and not on potential energy.
  • – nasu Sep 26 '18 at 11:40
  • Interesting fact: you can quite easily see the effects of this in the rates of good (OK, very good) pendulum clocks. Astonishingly you can also see effects from the Earth ringing as things like volcanoes stimulate it: the primary resonance is about 8.5 cycles/day. –  Sep 26 '18 at 12:03