An object is thrown directly away from Earth's surface. Its initial speed is \(V_0\) and escape velocity is \(V_E\). If the object reaches a distance of \(\frac{4R}{3}\) from the centre of the Earth, then the ratio \(\frac{V_E}{V_0}\) is:
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For escape velocity type questions, always compare total mechanical energy at two radial positions using gravitational potential energy \(-\frac{GMm}{r}\).