A satellite orbits the earth a distance of 1.50 × 107 m above the planet's surface and takes 8.65 hours for each revolution about the earth. The earth's radius is 6.38 × 106 m. The acceleration of this satellite is closest to
The acceleration in a circular motion is defined as:
"a = \\frac{v^{2}}{r} \\;(1)"
Where a is the centripetal acceleration, v the velocity and r is the radius.
The equation of the orbital velocity is defined as
"v = \\frac{2 \\pi r}{T}\\; (2)"
Where r is the radius and T is the period
For this particular case, the radius will be the sum of the high of the satellite"(1.50 \\times 10^{7} \\;m)" and the Earth radius "(6.38 \\times 10^{6} \\;m)" :
"r = 1.50 \\times 10^{7} \\;m+6.38 \\times 10^{6} \\;m \\\\\n\nr = 21.38 \\times 10^{6} \\;m"
Then, equation 2 can be used:
"T = 8.65 \\;hrs \\times \\frac{3600 \\;s}{1\\;hrs}=31140 \\; s \\\\\n\nv = \\frac{2 \\pi (21.38 \\times 10^{6}\\;m)}{31140 \\;s} \\\\\n\nv = 4313 \\;m\/s"
Finally equation 1 can be used:
"a = \\frac{(4313 \\;m\/s)^{2}}{21.38 \\times 10^{6}m} \\\\\n\na = 0.87\\; m\/s^{2}"
Hence, the acceleration of the satellite is "0.87 \\;m\/s^{2}"
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