Step 1: Understanding the Question:
We need to find the escape velocity of a planet given its mass and radius in terms of Earth's mass and radius.
Step 2: Key Formula or Approach:
The escape velocity \( v_e \) from the surface of a spherical body of mass \( M \) and radius \( R \) is given by:
\[
v_e = \sqrt{\frac{2GM}{R}}
\]
where \( G \) is the universal gravitational constant.
Step 3: Detailed Explanation:
Let the escape velocity of Earth be:
\[
v_E = \sqrt{\frac{2GM_E}{R_E}}
\]
For the given planet, mass \( M_P = 81 M_E \) and radius \( R_P = 9 R_E \).
The escape velocity from this planet is:
\[
v_P = \sqrt{\frac{2GM_P}{R_P}}
\]
Substitute the values of \( M_P \) and \( R_P \):
\[
v_P = \sqrt{\frac{2G(81M_E)}{9R_E}}
\]
\[
v_P = \sqrt{9 \times \frac{2GM_E}{R_E}}
\]
\[
v_P = 3 \sqrt{\frac{2GM_E}{R_E}} = 3 v_E
\]
Thus, the escape velocity from the planet is 3 times the escape velocity of Earth.
Step 4: Final Answer:
(B) 3 times Earth's escape velocity