The minimum speed required for an object to escape the gravitational field of Earth is given by the escape velocity formula: \[ v_{\text{escape}} = \sqrt{\frac{2GM}{R}} \]
where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( R \) is the distance from the center of the Earth.
However, in this case, the object is placed at a distance of \( 3R \) from the Earth’s surface.
The total distance from the center of the Earth is \( 4R \).
The escape velocity at this distance is: \[ v_{\text{escape}} = \sqrt{\frac{2GM}{4R}} = \sqrt{\frac{GM}{2R}} \]
Thus, the minimum speed with which the object must be projected is \( \sqrt{\frac{GM}{2R}} \), and the correct answer is (1).