Let's first find the distance of the satellite from the center of the Earth from the Kepler's Third Law:
R3T2=GME4π2,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
ME 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=34π2GMT2.Let's substitute the numbers:
R=34π26.67⋅10−11kg2Nm2⋅5.98⋅1024kg⋅(6.0hr⋅1hr3600s)2=1.67⋅107m.We can find the height of the satellite above the Earth's surface from the formula:
R=REarth+h,here,
REarth is the radius of the Earth,
h is the height of the satellite above the Earth's surface.
Finally, we get:
h=R−REarth=1.67⋅107m−6.37⋅106m=1.03⋅107m.Answer:
h=1.03⋅107m.
Comments
Thanks. Correct answer