Let's first find the distance of the satellite from the center of the Earth from the Kepler's Third Law:
"\\frac{T^2}{R^3} = \\frac{4\\pi^2}{GM_E},"here,
"T"is the period that the satellite needs to make one revolution,
"R"is the distance of the satellite from the center of the Earth,
"G"is the universal gravitational constant and
"M_E"is the mass of the Earth.
Then, from this equation we can find the distance
of the satellite from the center of the Earth:
"R = \\sqrt[3]{\\frac{GMT^2}{4\\pi^2}}."Let's substitute the numbers:
"R = \\sqrt[3]{\\frac{6.67 \\cdot 10^{-11} \\frac{Nm^2}{kg^2} \\cdot 5.98 \\cdot 10^{24} kg \\cdot (6.0 hr \\cdot \\frac{3600 s}{1 hr})^2}{4\\pi^2}} = 1.67 \\cdot 10^7 m."We can find the height of the satellite above the Earth's surface from the formula:
"R = R_{Earth} + h,"here,
"R_{Earth}"is the radius of the Earth,
"h"is the height of the satellite above the Earth's surface.
Finally, we get:
"h = R - R_{Earth} = 1.67 \\cdot 10^7 m - 6.37 \\cdot 10^6 m = 1.03 \\cdot 10^7 m."Answer:
"h = 1.03 \\cdot 10^7 m".
Comments
Thanks. Correct answer
Leave a comment