a satellite revolves in an orbit close to the surface of a planet of density 6300 kg m^-3. Calculate The time period of the satellite. Take The radius of the planet as 6400 km.
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The planet is a sphere of volume 43πR343πR3, and density -
d=M43πR3d=M43πR3
Where MM and RR are the mass and Radius of the planet. Therefore −−
M=d(43πR3)M=d(43πR3) ——— eqn 1
If mm is the mass of the rotating satellite, then the acceleration it feels due to planets gravity -
g=FGmg=FGm, where FGFG is Newton's force of gravity. Thus using Newton's gravitational law -
g=1mGMmR2g=1mGMmR2
Substitute value of MM from eqn 1 here,
g=GR2d(43πR3)g=GR2d(43πR3)
g=4GdπR3g=4GdπR3
This gravitational acceleration acts as the centripetal acceleration for rotating satellite. So -
Centripetal acceleration = gg
ω2R=4GdπR3ω2R=4GdπR3
ω=4Gdπ3−−−−−√ω=4Gdπ3 — — eq 2
Here ωω is the angular velocity of the rotating satellite. Therefore the period of rotation is give as -
T=2πωT=2πω
Substitute ωω from eqn 2 here -
T=2π34Gdπ−−−−−√T=2π34Gdπ
T=3πGd−−−√T=3πGd
T=3∗3.146.67∗10−11∗6300−−−−−−−−−−−−−−−√T=3∗3.146.67∗10−11∗6300
T=9.426.67∗6.3−−−−−−−−√104T=9.426.67∗6.3104
T=0.473469∗104T=0.473469∗104 sec
T=0.473469∗10460∗60T=0.473469∗10460∗60 hours
T=1.315T=1.315 hours for satellite to complete one revolution around the planet.
d=M43πR3d=M43πR3
Where MM and RR are the mass and Radius of the planet. Therefore −−
M=d(43πR3)M=d(43πR3) ——— eqn 1
If mm is the mass of the rotating satellite, then the acceleration it feels due to planets gravity -
g=FGmg=FGm, where FGFG is Newton's force of gravity. Thus using Newton's gravitational law -
g=1mGMmR2g=1mGMmR2
Substitute value of MM from eqn 1 here,
g=GR2d(43πR3)g=GR2d(43πR3)
g=4GdπR3g=4GdπR3
This gravitational acceleration acts as the centripetal acceleration for rotating satellite. So -
Centripetal acceleration = gg
ω2R=4GdπR3ω2R=4GdπR3
ω=4Gdπ3−−−−−√ω=4Gdπ3 — — eq 2
Here ωω is the angular velocity of the rotating satellite. Therefore the period of rotation is give as -
T=2πωT=2πω
Substitute ωω from eqn 2 here -
T=2π34Gdπ−−−−−√T=2π34Gdπ
T=3πGd−−−√T=3πGd
T=3∗3.146.67∗10−11∗6300−−−−−−−−−−−−−−−√T=3∗3.146.67∗10−11∗6300
T=9.426.67∗6.3−−−−−−−−√104T=9.426.67∗6.3104
T=0.473469∗104T=0.473469∗104 sec
T=0.473469∗10460∗60T=0.473469∗10460∗60 hours
T=1.315T=1.315 hours for satellite to complete one revolution around the planet.
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