- ✓starts moving in an elliptical orbit around the planet
- Bcontinues to move in a circular orbit
- CFalls vertically downwards towards the planet
- DEscapes from the Planet's Gravitational field.
$\mathrm{v}_{0}=\sqrt{\frac{\mathrm{GM}}{\mathrm{R}}}$
After collision, let the combined mass moves with speed $v_{1 }$
${\mathrm{mv}_{0}+\frac{\mathrm{m}}{2} \frac{\mathrm{v}_{0}}{2}=\left(\frac{3 \mathrm{m}}{2}\right) \mathrm{v}_{1}}$
${\mathrm{v}_{1}=\frac{5 \mathrm{v}_{0}}{6}}$
since after collision, the speed is not equal to orbital speed at that point. So motion cannot be circular. since velocity will remain tangential, so it cannot fall vertically towards the planet. Their speed after collision is less than escape speed $\sqrt{2} v_{0}, \quad$
so they cannot escape gravitational field. So their motion will be elliptical around the planet.
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$\left[\right.$ Take $\left.g=10 m / s ^{2}\right]$

$(A)$ $\beta=0$ when $a= g / \sqrt{2}$
$(B)$ $\beta>0$ when $a= g / \sqrt{2}$
$(C)$ $\beta=\frac{\sqrt{2}-1}{\sqrt{2}}$ when $a= g / 2$
$(D)$ $\beta=\frac{1}{\sqrt{2}}$ when $a= g / 2$