Question #266249

The orbital speed of the Earth around the Sun is 30 km/s. In one year, how many seconds do the clocks on the Earth lose with respect to the clocks of an inertial reference frame at rest relative to the Sun


1
Expert's answer
2021-11-16T19:20:39-0500

If we are to consider an inertial frame at rest relative to the sun, it must be the one keeping the proper time interval ∆tp. Over the course of one year, we have

tp=1  yr3.156×107  s∆t_p = 1 \; yr ≈ 3.156 \times 10^7 \;s

The observers on earth are in motion relative to the sun, and therefore they measure a dilated time

interval t=γtp∆t^* =γ∆t_p . We are asked for the difference between the two clocks after one year as measured in the sun’s inertial frame, or

difference=ttp=γtptp=(γ1)tpdifference = ∆t^* − ∆t_p = γ∆t_p − ∆t_p = (γ − 1) ∆t_p

Since in this case the relative velocity of earth is small with respect to c, v = 30 km/s = 3 × 104 s so v/c= 10−4 , we can use the second approximation given.

γ1=11v2c211+12v2c21=12v2c2difference12v2c2Δtp=12(104)2(3.156×107  s)=(5×109)(3.156×107  s)=0.16  sγ -1 = \frac{1}{\sqrt{1 -\frac{v^2}{c^2}}} -1 ≈ 1 + \frac{1}{2} \frac{v^2}{c^2} -1 = \frac{1}{2} \frac{v^2}{c^2 } \\ difference ≈ \frac{1}{2} \frac{v^2}{c^2} Δt_p \\ = \frac{1}{2} (10^{-4})^2 (3.156 \times 10^7 \;s) \\ = (5 \times 10^{-9}) (3.156 \times 10^7 \; s) \\ = 0.16 \;s


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