Question #65596

A satellite going around Earth in an elliptic orbit has a speed of 10 km s−1 at the perigee which is at a distance of 227 km from the surface of the earth. Calculate the apogee distance and its speed at that point
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Expert's answer

2017-02-28T12:05:06-0500

Answer on Question #65596, Physics / Mechanics | Relativity |

A satellite going around Earth in an elliptic orbit has a speed of 10kms110\,\mathrm{km\,s^{-1}} at the perigee which is at a distance of 227km227\,\mathrm{km} from the surface of the earth. Calculate the apogee distance and its speed at that point.

Solution

hp=2.27105mvp=104m/secG=6.671011m3kg1sec2 (universal gravitational constant)r=6.37106m (Earth radius)M=5.971024kg (Earth mass)va?,ha?\begin{array}{l} h_p = 2.27 \cdot 10^5\,\mathrm{m} \\ v_p = 10^4\,\mathrm{m/sec} \\ G = 6.67 \cdot 10^{-11}\,\mathrm{m^3\,kg^{-1}\,sec^{-2}} \text{ (universal gravitational constant)} \\ r = 6.37 \cdot 10^6\,\mathrm{m} \text{ (Earth radius)} \\ M = 5.97 \cdot 10^{24}\,\mathrm{kg} \text{ (Earth mass)} \\ v_a - ?, h_a - ? \end{array}


We do definitions: rp=r+hpr_p = r + h_p, ra=r+har_a = r + h_a, a=(rp+ra)/2a = (r_p + r_a)/2;

From the formula


v=GM(2/r1/a)v = \sqrt{GM(2/r - 1/a)}


we find this equality


a=GMrp2GMvp2rp.a = \frac{G M r_p}{2 G M - v_p^2 r_p}.


After the substitution of values, a=19217kma = 19\,217\,\mathrm{km}, ra=2arp=31837kmr_a = 2a - r_p = 31\,837\,\mathrm{km}, ha=rar=25467kmh_a = r_a - r = 25\,467\,\mathrm{km}.


vavp=rpra,va=rpravp.\frac{v_a}{v_p} = \frac{r_p}{r_a}, \quad v_a = \frac{r_p}{r_a} \cdot v_p.

va=0.21104m/secv_a = 0.21 \cdot 10^4\,\mathrm{m/sec}.

Answer: 25467km25\,467\,\mathrm{km}, 2.1km/sec2.1\,\mathrm{km/sec}.

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