4 v
v
2 v
3 v
To solve this problem, we need to understand the concept of escape velocity and how it changes with variations in planetary characteristics.
The escape velocity \(v_e\) from the surface of a planet can be determined by the formula:
\(v_e = \sqrt{\frac{2GM}{R}}\)
Here:
Given in the problem, the new planet has a radius four times that of Earth (i.e., \(R' = 4R_{E}\)) and the same mass density as Earth. To find out the new mass \(M'\) based on density concepts:
\(\text{Density} = \frac{\text{Mass}}{\text{Volume}}\)
The volume \(V\) of a sphere is given by:
\(V = \frac{4}{3} \pi R^3\)
If the density remains constant and the radius increases to four times:
\(\text{New Mass }, M' = \text{Density} \times \text{New Volume} = \text{Density} \times \left(\frac{4}{3} \pi (4R_{E})^3\right)\)
Therefore, \(M' = 64 \times \text{Mass of Earth }, M_{E}\), because \((4R_{E})^3 = 64R_{E}^3\)
Substitute \(M'\) and \(R'\) into the escape velocity formula:
\(v_e' = \sqrt{\frac{2G(64M_E)}{4R_E}}\)
Simplifying:
\(v_e' = \sqrt{\frac{128GM_E}{4R_E}} = \sqrt{32} \, \times \sqrt{\frac{2GM_E}{R_E}} = 4 \, \times v\)
This means the escape velocity from the surface of the new planet is four times that of Earth.
Therefore, the correct answer is 4 v.
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)