Step 1: Formula for Escape Velocity.
The escape velocity \( v_e \) is given by the formula:
\[
v_e = \sqrt{\frac{2GM}{R}}
\]
where:
- \( G \) is the gravitational constant,
- \( M \) is the mass of the planet, and
- \( R \) is the radius of the planet.
Step 2: Understand the Given Data.
We are told that:
- The radius of the new planet is double that of Earth, so \( R_{\text{new}} = 2R_{\text{earth}} \).
- The density of the new planet is the same as Earth, meaning the mass of the new planet \( M_{\text{new}} \) will be 8 times the mass of Earth.
This is because the mass of a planet depends on its volume, and volume scales with the cube of the radius. Therefore, if the radius is doubled, the volume (and thus the mass) increases by a factor of \( 2^3 = 8 \).
Step 3: Relation for New Planet.
The escape velocity \( v_e \) depends on both the mass \( M \) and the radius \( R \) of the planet. The formula for the escape velocity can be written for the new planet as:
\[
v_{e,\text{new}} = \sqrt{\frac{2GM_{\text{new}}}{R_{\text{new}}}}
\]
Substitute \( M_{\text{new}} = 8M_{\text{earth}} \) and \( R_{\text{new}} = 2R_{\text{earth}} \) into the equation:
\[
v_{e,\text{new}} = \sqrt{\frac{2G(8M_{\text{earth}})}{2R_{\text{earth}}}}
\]
Step 4: Simplifying the Expression.
Now simplify the expression:
\[
v_{e,\text{new}} = \sqrt{\frac{8GM_{\text{earth}}}{2R_{\text{earth}}}}
\]
\[
v_{e,\text{new}} = \sqrt{4 \cdot \frac{2GM_{\text{earth}}}{R_{\text{earth}}}}
\]
Step 5: Compare with Escape Velocity from Earth.
We know that the escape velocity from Earth is:
\[
v_{e,\text{earth}} = \sqrt{\frac{2GM_{\text{earth}}}{R_{\text{earth}}}} = 11 \, \text{km/s}
\]
Thus, we can write:
\[
v_{e,\text{new}} = 2 \cdot v_{e,\text{earth}} = 2 \cdot 11 \, \text{km/s} = 22 \, \text{km/s}
\]
Step 6: Conclusion.
Therefore, the escape velocity from the new planet is \( 22 \, \text{km/s} \).