Step 1: Apply the Acceleration Due to Gravity Formula
The formula for acceleration due to gravity is:
$$ g = \frac{G M}{R^2} $$
Where:
G = Gravitational constant
M = Mass of the celestial body
R = Radius of the celestial body
Step 2: Express the Celestial Body’s Mass and Radius Relative to Earth’s
Let Earth’s mass and radius be denoted as:
\( M_e \) = Earth's mass
\( R_e \) = Earth's radius
For the specified celestial body:
$$ M_p = \frac{M_e}{10}, \quad R_p = \frac{R_e}{2} $$
Step 3: Substitute Values into the Formula
Using the gravitational formula for the celestial body:
$$ g_p = \frac{G M_p}{R_p^2} $$
Substituting the defined values:
$$ g_p = \frac{G \cdot \frac{M_e}{10}}{\left(\frac{R_e}{2}\right)^2} $$
Simplifying the denominator:
$$ g_p = \frac{G \cdot \frac{M_e}{10}}{\frac{R_e^2}{4}} $$
Multiplying by the reciprocal of the denominator:
$$ g_p = G \cdot M_e \cdot \frac{4}{10 R_e^2} $$
Given that:
$$ g_e = \frac{G M_e}{R_e^2} = 9.8 \text{ m/s}^2 $$
Substitute \( g_e \) into the equation:
$$ g_p = \frac{4}{10} \cdot 9.8 $$
Calculation yields:
$$ g_p = 3.92 \text{ m/s}^2 $$
Conclusion
The acceleration due to gravity on the specified celestial body is 3.92 m/s².