Answer:
The kinetic energies just before touching the ground are as follows;
Case 1
![W_(1) = G* M_(E)* m * (1)/(2 * r_(2))](https://img.qammunity.org/2021/formulas/physics/college/qvavlbbe41h9l1kzy54imvwkjt69gg915l.png)
Case 2
![W_(2) = G* M_(E)* m * (2)/(3 * r_(2))](https://img.qammunity.org/2021/formulas/physics/college/vjm1kwnsmnfcjdmffrolak8esk8ztsnkwc.png)
The correct option is;
K2 = (4/3) K1
Step-by-step explanation:
The work done is given by the relation;
For case 1
![W_1 = W_(1\rightarrow 2) = G* M_(E)* m * \left ((1)/(r_(2))-(1)/(r_(1)) \right )](https://img.qammunity.org/2021/formulas/physics/college/cr0zbxul3a1yevn7wvl8qhx8xzd26wt0bd.png)
Where for case 1 we have:
G = Gravitational constant = 6.67408 × 10⁻¹¹ m³/(kg·s²)
r₂ = Radius of the Earth
r₁ = 2 × Radius of the Earth = 2 × r₂
Hence;
![W_2 = W_(1\rightarrow 2) = G* M_(E)* m * \left ( (1)/(r_(2)) - (1)/(2* r_(2)) \right )](https://img.qammunity.org/2021/formulas/physics/college/3kwuycpa52kz50nrtw7j3pfy60tzgu6lu3.png)
![W_(1\rightarrow 2) = G* M_(E)* m * (1)/(2 * r_(2))](https://img.qammunity.org/2021/formulas/physics/college/4njbcanrrhn6ga1fjvet9wxr0h20r8f9qa.png)
For case 2 we have:
G = Gravitational constant = 6.67408 × 10⁻¹¹ m³/(kg·s²)
r₂ = Radius of the Earth
r₁ = 3 × Radius of the Earth = 2 × r₂
Hence;
![W_(1\rightarrow 2) = G* M_(E)* m * \left ( (1)/(r_(2)) - (1)/(3* r_(2)) \right )](https://img.qammunity.org/2021/formulas/physics/college/23jty66hal3ic3pi3eja4umb1d94r0dfs0.png)
![W_(1\rightarrow 2) = G* M_(E)* m * (2)/(3 * r_(2))](https://img.qammunity.org/2021/formulas/physics/college/muw8b9g1ei4dm01gb6llho8nv1xnnhrrnx.png)
Therefore;
![(\Delta K2)/(\Delta K1) = (W_(2))/(W_(1)) = (G* M_(E)* m * (2)/(3 * r_(2)))/(G* M_(E)* m * (1)/(2* r_(2))) = (4)/(3)](https://img.qammunity.org/2021/formulas/physics/college/zpabvhldld3qx77zz3uzr06vzc5pyic4bf.png)
Hence;
K2 = (4/3) × K1.