(a) We can find the energy of the satellite from the law of konservation of energy:
E s a t = K E a + P E a = K E p + P E p , E_{sat}=KE_a+PE_a=KE_p+PE_p, E s a t = K E a + P E a = K E p + P E p , E s a t = 1 2 m v a 2 − G M m r a , E_{sat}=\dfrac{1}{2}mv_a^2-\dfrac{GMm}{r_a}, E s a t = 2 1 m v a 2 − r a GM m , E s a t = 1 2 ⋅ 2500 k g ⋅ ( 6114 m s ) 2 − 6.67 ⋅ 1 0 − 11 N m 2 k g 2 ⋅ 5.97 ⋅ 1 0 24 k g ⋅ 2500 k g 9.38 ⋅ 1 0 6 m = − 5.94 ⋅ 1 0 10 J . E_{sat}=\dfrac{1}{2}\cdot 2500\ kg\cdot(6114\ \dfrac{m}{s})^2-\dfrac{6.67\cdot10^{-11}\ \dfrac{Nm^2}{kg^2}\cdot5.97\cdot10^{24}\ kg \cdot2500\ kg}{9.38\cdot10^6\ m}=-5.94\cdot10^{10}\ J. E s a t = 2 1 ⋅ 2500 k g ⋅ ( 6114 s m ) 2 − 9.38 ⋅ 1 0 6 m 6.67 ⋅ 1 0 − 11 k g 2 N m 2 ⋅ 5.97 ⋅ 1 0 24 k g ⋅ 2500 k g = − 5.94 ⋅ 1 0 10 J .
(b) We can find the angular momentum of the satellite from the formula:
L = m v a r a = m v p r p , L=mv_ar_a=mv_pr_p, L = m v a r a = m v p r p , here, m = 2500 k g m=2500\ kg m = 2500 k g is the mass of the satellite, r a = ( R E + h a ) r_a=(R_E+h_a) r a = ( R E + h a ) is the apagee distance, r p = ( R E + h p ) r_p=(R_E+h_p) r p = ( R E + h p ) is the perigee distance, R E = 6.38 ⋅ 1 0 6 m R_E=6.38\cdot10^6\ m R E = 6.38 ⋅ 1 0 6 m is the radius of the Earth, h a = 3.0 ⋅ 1 0 6 m h_a=3.0\cdot10^6\ m h a = 3.0 ⋅ 1 0 6 m is the altitude of apagee, h p = 1.0 ⋅ 1 0 6 m h_p=1.0\cdot10^6\ m h p = 1.0 ⋅ 1 0 6 m is the altitude of perigee, v a v_a v a , v p v_p v p is the speed of the satellite at apogee and perigee, respectivelly.
Let's first calculate r a r_a r a and r p r_p r p :
r a = ( 6.38 ⋅ 1 0 6 m + 3.0 ⋅ 1 0 6 m ) = 9.38 ⋅ 1 0 6 m , r_a=(6.38\cdot10^6\ m+3.0\cdot10^6\ m)=9.38\cdot10^6\ m, r a = ( 6.38 ⋅ 1 0 6 m + 3.0 ⋅ 1 0 6 m ) = 9.38 ⋅ 1 0 6 m , r p = ( 6.38 ⋅ 1 0 6 m + 1.0 ⋅ 1 0 6 m ) = 7.38 ⋅ 1 0 6 m . r_p=(6.38\cdot10^6\ m+1.0\cdot10^6\ m)=7.38\cdot10^6\ m. r p = ( 6.38 ⋅ 1 0 6 m + 1.0 ⋅ 1 0 6 m ) = 7.38 ⋅ 1 0 6 m . Let's also find semi-major axis of the satellite:
a = r a + r p 2 , a=\dfrac{r_a+r_p}{2}, a = 2 r a + r p , a = 9.38 ⋅ 1 0 6 m + 7.38 ⋅ 1 0 6 m 2 = 8.38 ⋅ 1 0 6 m . a=\dfrac{9.38\cdot10^6\ m+7.38\cdot10^6\ m}{2}=8.38\cdot10^6\ m. a = 2 9.38 ⋅ 1 0 6 m + 7.38 ⋅ 1 0 6 m = 8.38 ⋅ 1 0 6 m . Then, we can find the speed of the satellite at apogee and perigee from the vis-viva equation:
v = G M ( 2 r − 1 a ) . v=\sqrt{GM(\dfrac{2}{r}-\dfrac{1}{a})}. v = GM ( r 2 − a 1 ) . Then, the speed of the satellite at the apagee will be:
v a = 6.67 ⋅ 1 0 − 11 N m 2 k g 2 ⋅ 5.97 ⋅ 1 0 24 k g ⋅ ( 2 9.38 ⋅ 1 0 6 m − 1 8.38 ⋅ 1 0 6 m ) = 6114 m s . v_a=\sqrt{6.67\cdot10^{-11}\ \dfrac{Nm^2}{kg^2}\cdot5.97\cdot10^{24}\ kg\cdot(\dfrac{2}{9.38\cdot10^6\ m}-\dfrac{1}{8.38\cdot10^6\ m})}=6114\ \dfrac{m}{s}. v a = 6.67 ⋅ 1 0 − 11 k g 2 N m 2 ⋅ 5.97 ⋅ 1 0 24 k g ⋅ ( 9.38 ⋅ 1 0 6 m 2 − 8.38 ⋅ 1 0 6 m 1 ) = 6114 s m .
v p = 6.67 ⋅ 1 0 − 11 N m 2 k g 2 ⋅ 5.97 ⋅ 1 0 24 k g ⋅ ( 2 7.38 ⋅ 1 0 6 m − 1 8.38 ⋅ 1 0 6 m ) = 7771 m s . v_p=\sqrt{6.67\cdot10^{-11}\ \dfrac{Nm^2}{kg^2}\cdot5.97\cdot10^{24}\ kg\cdot(\dfrac{2}{7.38\cdot10^6\ m}-\dfrac{1}{8.38\cdot10^6\ m})}=7771\ \dfrac{m}{s}. v p = 6.67 ⋅ 1 0 − 11 k g 2 N m 2 ⋅ 5.97 ⋅ 1 0 24 k g ⋅ ( 7.38 ⋅ 1 0 6 m 2 − 8.38 ⋅ 1 0 6 m 1 ) = 7771 s m .
Finally, we can calculate the angular momentum of the satellite:
L = 2500 k g ⋅ 6114 m s ⋅ 9.38 ⋅ 1 0 6 m = 1.43 ⋅ 1 0 14 k g m 2 s . L=2500\ kg\cdot 6114\ \dfrac{m}{s}\cdot 9.38\cdot10^6\ m=1.43\cdot10^{14}\ \dfrac{kgm^2}{s}. L = 2500 k g ⋅ 6114 s m ⋅ 9.38 ⋅ 1 0 6 m = 1.43 ⋅ 1 0 14 s k g m 2 . Answer:
a) E s a t = − 5.94 ⋅ 1 0 10 J . E_{sat}=-5.94\cdot10^{10}\ J. E s a t = − 5.94 ⋅ 1 0 10 J .
b) L = 1.43 ⋅ 1 0 14 k g m 2 s . L=1.43\cdot10^{14}\ \dfrac{kgm^2}{s}. L = 1.43 ⋅ 1 0 14 s k g m 2 .
c) v a = 6114 m s , v p = 7771 m s . v_a=6114\ \dfrac{m}{s}, v_p=7771\ \dfrac{m}{s}. v a = 6114 s m , v p = 7771 s m .
Comments
Leave a comment