Step 1: Use the Formula for Acceleration Due to Gravity
The formula for acceleration due to gravity is:
$$ g = \frac{G M}{R^2} $$
Where:
G = Gravitational constant
M = Mass of the planet
R = Radius of the planet
Step 2: Express the Planet’s Mass and Radius in Terms of Earth’s
Let Earth’s mass and radius be:
\( M_e \) = Earth's mass
\( R_e \) = Earth's radius
For the given planet:
$$ M_p = \frac{M_e}{10}, \quad R_p = \frac{R_e}{2} $$
Step 3: Substitute Values into the Formula
Using the gravitational formula for the planet:
$$ g_p = \frac{G M_p}{R_p^2} $$
Substituting the values:
$$ g_p = \frac{G \cdot \frac{M_e}{10}}{\left(\frac{R_e}{2}\right)^2} $$
Rewriting the denominator:
$$ g_p = \frac{G \cdot \frac{M_e}{10}}{\frac{R_e^2}{4}} $$
Since division by a fraction is multiplication by its reciprocal:
$$ g_p = G \cdot M_e \cdot \frac{4}{10 R_e^2} $$
Since we know that:
$$ g_e = \frac{G M_e}{R_e^2} = 9.8 \text{ m/s}^2 $$
We substitute \( g_e \) into the equation:
$$ g_p = \frac{4}{10} \cdot 9.8 $$
Solving:
$$ g_p = 3.92 \text{ m/s}^2 $$
Conclusion
The acceleration due to gravity on the given planet is 3.92 m/s².
The following diagram shown restriction sites in E. coli cloning vector pBR322. Find the role of ‘X’ and ‘Y’gens :