Question #43043

Two atomic clocks are synchronized while on Earth before one is launched (within a GPS satellite) into a medium-altitude Earth orbit. The satellite orbits the Earth at an altitude of 22,000 km, with an orbital velocity of 15,000 km/hr. After 1000 orbits, estimate the time difference between the two atomic clocks? (Assume that only special relativity effects are present.)

Expert's answer

Answer on Question #43043, Physics, Relativity

Two atomic clocks are synchronized while on Earth before one is launched (within a GPS satellite) into a medium-altitude Earth orbit. The satellite orbits the Earth at an altitude of 22,000 km, with an orbital velocity of 15,000 km/hr. After 1000 orbits, estimate the time difference between the two atomic clocks? (Assume that only special relativity effects are present.)

Solution:

Given:


h=22000 km=22106 m,v=15000 km/hr=4166.67 m/s,N=1000 orbits,δt=?\begin{array}{l} h = 22000 \text{ km} = 22 \cdot 10^{6} \text{ m}, \\ v = 15000 \text{ km/hr} = 4166.67 \text{ m/s}, \\ N = 1000 \text{ orbits}, \\ \delta t = ? \end{array}


According to special relativity, the rate of a clock is greatest according to an observer who is at rest with respect to the clock. In a frame of reference in which the clock is not at rest, the clock runs more slowly, as expressed by the Lorentz factor.

The Lorentz factor is defined as:


γ=11v2c2=11β2\gamma = \frac{1}{\sqrt{1 - \frac{v^{2}}{c^{2}}}} = \frac{1}{\sqrt{1 - \beta^{2}}}


where:

- vv is the relative velocity between inertial reference frames,

- β\beta is the ratio of vv to the speed of light cc.

- c=3108 m/sc = 3 \cdot 10^{8} \text{ m/s} is the speed of light in a vacuum.

Thus,


γ=114166.67291016=1.000000000096451\gamma = \frac{1}{\sqrt{1 - \frac{4166.67^{2}}{9 \cdot 10^{16}}}} = 1.000000000096451

Time dilation

The time (Δt)(\Delta t') between two ticks as measured in the frame in which the clock is moving, is longer than the time (Δt)(\Delta t) between these ticks as measured in the rest frame of the clock:


Δt=γΔt\Delta t' = \gamma \Delta t


For time Δt\Delta t we have:


Δt=Distancevelocity=2π(R+h)Nv\Delta t = \frac{\text{Distance}}{\text{velocity}} = \frac{2\pi(R + h)N}{v}


where R=6.371106 mR = 6.371 \cdot 10^{6} \text{ m} is the Earth's mean radius.

Thus,


Δt=2π(6.371106+22106)10004166.67=4.27824107 s\Delta t = \frac{2\pi(6.371 \cdot 10^{6} + 22 \cdot 10^{6}) \cdot 1000}{4166.67} = 4.27824 \cdot 10^{7} \text{ s}


The time difference between the two atomic clocks is


δt=ΔtΔt=γΔtΔt=Δt(γ1)\delta t = \Delta t' - \Delta t = \gamma \Delta t - \Delta t = \Delta t (\gamma - 1)


Thus,


δt=4.27824107(1.0000000000964511.0)=0.00413 s=4.13103 s\delta t = 4.27824 \cdot 10^{7}(1.000000000096451 - 1.0) = 0.00413 \text{ s} = 4.13 \cdot 10^{-3} \text{ s}


Answer. δt=4.13103 s\delta t = 4.13 \cdot 10^{-3} \text{ s}.

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