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Question: A satellite is projected into space from a point 'P' at a distance '$r_0$' from the centre of the ea...

A satellite is projected into space from a point 'P' at a distance 'r0r_0' from the centre of the earth with an initial velocity v0=GMr0v_0 = \sqrt{\frac{GM}{r_0}} at an angle α=37\alpha = 37^\circ with the horizontal at point 'P' as shown in the figure. It is found that the satellite is propelled into an elliptical orbit. Length of semi-major axis of the ellipse is found to be ar02\frac{ar_0}{2} and eccentricity of the ellipse is e.

Answer

e = sin 37° ≈ 0.6

Explanation

Solution

  1. Energy:
    At point P,

    E=12v02GMr0=12GMr0GMr0=GM2r0.E = \frac{1}{2}v_0^2 - \frac{GM}{r_0} = \frac{1}{2}\frac{GM}{r_0} - \frac{GM}{r_0} = -\frac{GM}{2r_0}.

    Since for an elliptical orbit,

    E=GM2a,E = -\frac{GM}{2a},

    we have a=r0a = r_0. (This is consistent with the given semi‐major axis ar02\frac{ar_0}{2} if we take the constant a=2a=2.)

  2. Angular Momentum:
    The horizontal component of the velocity is

    v0x=v0cos37.v_{0x} = v_0\cos 37^\circ.

    Thus,

    L=r0v0cos37=r0GMr0cos37=GMr0cos37.L = r_0\, v_0 \cos 37^\circ = r_0\sqrt{\frac{GM}{r_0}}\, \cos 37^\circ = \sqrt{GM\,r_0}\, \cos 37^\circ.
  3. Eccentricity Calculation:
    Using the formula

    e=1+2EL2(GM)2,e = \sqrt{1+\frac{2EL^2}{(GM)^2}},

    substitute the values:

    2E=GMr0,L2=GMr0cos237.2E = -\frac{GM}{r_0}, \quad L^2 = GM\,r_0\,\cos^2 37^\circ.

    So,

    e=1+GMr0(GMr0cos237)(GM)2=1cos237=sin37.e = \sqrt{1 + \frac{-\frac{GM}{r_0}\cdot (GM\,r_0\,\cos^2 37^\circ)}{(GM)^2}} = \sqrt{1-\cos^2 37^\circ} = \sin 37^\circ.