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
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
"\u2206t_p = 1 \\; yr \u2248 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 "\u2206t^* =\u03b3\u2206t_p" . We are asked for the difference between the two clocks after one year as measured in the sun’s inertial frame, or
"difference = \u2206t^* \u2212 \u2206t_p = \u03b3\u2206t_p \u2212 \u2206t_p = (\u03b3 \u2212 1) \u2206t_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.
"\u03b3 -1 = \\frac{1}{\\sqrt{1 -\\frac{v^2}{c^2}}} -1 \u2248 1 + \\frac{1}{2} \\frac{v^2}{c^2} -1 = \\frac{1}{2} \\frac{v^2}{c^2 } \\\\\n\ndifference \u2248 \\frac{1}{2} \\frac{v^2}{c^2} \u0394t_p \\\\\n\n= \\frac{1}{2} (10^{-4})^2 (3.156 \\times 10^7 \\;s) \\\\\n\n= (5 \\times 10^{-9}) (3.156 \\times 10^7 \\; s) \\\\\n\n= 0.16 \\;s"
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