Clock precision as a function of temperature and height above sea level

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The discussion focuses on the effects of height and temperature on the period of a grandfather pendulum clock when moved from sea level to 200 meters above. It calculates that the period increases by approximately 2.7 seconds per day due to the change in gravitational force at the new height. Additionally, to maintain clock precision, a temperature adjustment of about -3.1 K is required, based on the pendulum's thermal expansion coefficient. There is some confusion regarding the calculations for temperature change, with one participant suggesting an alternative approach using the difference in gravitational acceleration. The thread seeks clarification on the assumptions and methods used in these calculations.
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Homework Statement



A grandfather pendulum clock is to be moved from a location at sea level to a new location approximately 200 m up in height.

We assume that the Earth's radius is 6400 km. We know Newton's gravitational law and the oscillation equation for a pendulum.

(*) How much will the period of the clock increase, expressed as seconds/day as it is moved from the old height to the new height?

(**) We also know that the pendulum's period will change with temperature. If the thermal expansion coefficient for the pendulum is α = 2.03E-5 per Kelvin, how much do we have to alter the room temperature from the usual temperature in order for the clock to be precise again? (You may assume that the pendulum has the form of a rod, and that it is suspended from one end.) [Answer ΔT ~ -(1/α)*((2h)/R) ~ -3.1 K] (The difference between these given variables h and R are not clear from the text.)

Homework Equations



Newton's grav. law: F = G*(m1*m2)/r²
Oscillation equation (I combined relations found in the book by Tipler and Mosca): T = (2π)/ω. ω = sqrt(k/m).

The Attempt at a Solution



(*) I imagined two extremely long pendulum clocks with extremely long periods:

F = G*(m_1m_2)/r² = m_1*a [m_1 is mass of pendulum]

a = G*m_2/r² [m_2 is mass of Earth]

m = m_2

T = 2π * sqrt(m_2/a) = 2πsqrt(r²/G) [G gravitational constant]

--> T_1 = 2π*(6400E3)*sqrt(1/6.67E-11) ~ 4.923760562E12, ie. seconds

T_2 = 2π*(6400E3+200)*sqrt(1/6.67E-11) ~ 4.923914429E12

Difference in period, in seconds/day:

(T_2-T_1)/T_2 * 60²*24 s/d ~ 2.7 s/d

which was also given as correct in the paper. Please give comments on this anyway if you think my assumptions / method of solution is strange etc.

(**)

I found the equation ΔL/L = αΔT <--> ΔT = ΔL/(α*L) = 200 / (6400E3 * 2.03E-5 K-1) ~ 1.539 K

The given answer is as mentioned above -3.1 K. I observe that 1.539 K * 2 ~ 3.1 K. Should I use some other relations?

Thanks for your help.

 
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Or you could just wok out the diffeence in 'g' at the two heights and use T = 2pi sqt(L/g)
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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