Question #66743

A satellite going around the earth in an elliptical orbit has a speed of 10 km/s at the perigee which is at a distance of 227 km from the surface of the earth. Calculate the apogee distance &its speed at that point.
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Expert's answer

2017-03-30T11:12:07-0400

Answer on Question #66743, Physics / Mechanics | Relativity

Question:

A satellite going around the earth in an elliptical orbit has a speed of 10km/s10\mathrm{km / s} at the perigee which is at a distance of 227km227\mathrm{km} from the surface of the earth. Calculate the apogee distance & its speed at that point.

Solution:

The satellite's speed at the perigee may be calculated according to this formula:

vp=GMrp(1+e)v_{p} = \sqrt{\frac{GM}{r_{p}}(1 + e)} , where GG — gravitational constant (6.674×10 11^{-11} m 3^3 kg 1^{-1} s 2^{-2} );

M - the Earth's mass (5.972×10 24^{24} kg);

rpr_p - perigee distance from the centre of the earth;

ee - eccentricity of the orbit.

Then e=vp2rpGM1=100002(6371000+227000)6.674×10115.972×10241=0.655e = \frac{v_p^2 r_p}{GM} - 1 = \frac{10000^2 \cdot (6371000 + 227000)}{6.674 \times 10^{-11} \cdot 5.972 \times 10^{24}} - 1 = 0.655

In apogee the satellite's speed:

va=GMra(1e)v_{a} = \sqrt{\frac{GM}{r_{a}}(1 - e)} , where rar_a - apogee distance from the centre of the earth.

For elliptical orbit the distances rpr_p and rar_a are related as rarp=1+e1e\frac{r_a}{r_p} = \frac{1 + e}{1 - e} , and then

ra=rp1+e1e=(6371000+227000)1+0.65510.655=31651275mr_a = r_p \frac{1 + e}{1 - e} = (6371000 + 227000) \frac{1 + 0.655}{1 - 0.655} = 31651275 \, m .

The apogee distance from the surface of the earth

da=316512756371000=25280275m25280km.d_{a} = 31651275 - 6371000 = 25280275 \, m \cong 25280 \, km.

va=6.674×10115.972×102431651275(10.655)=2084ms2.1km/sv_{a} = \sqrt{\frac{6.674\times 10^{-11}\cdot 5.972\times 10^{24}}{31651275}(1 - 0.655)} = 2084\frac{m}{s}\cong 2.1km / s

Answer:

25280 km

2.1 km/s

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