To find the center of gravity of a rod whose mass per unit length is directly proportional to its distance from one end, we can use the following approach:
Step 1: Define the mass distribution.
Let the rod be placed along the x-axis from x = 0 to x = 3 \, \text{m}. Assume the mass per unit length (linear mass density) at a distance x from one end is given by \lambda(x) = kx, where k is a constant of proportionality.
Step 2: Express total mass of the rod.
The total mass M of the rod is the integral of the linear density along the length of the rod:
M = \int_0^3 \lambda(x) \, dx = \int_0^3 kx \, dxM = \left[ \frac{kx^2}{2} \right]_0^3 = \frac{k(3)^2}{2} = \frac{9k}{2}
Step 3: Find the center of gravity.
The center of gravity (x_{\text{cg}}) is given by:
x_{\text{cg}} = \frac{\int_0^3 x \lambda(x) \, dx}{M} = \frac{\int_0^3 x (kx) \, dx}{M}x_{\text{cg}} = \frac{\int_0^3 kx^2 \, dx}{\frac{9k}{2}} = \frac{k \left[ \frac{x^3}{3} \right]_0^3}{\frac{9k}{2}}
= \frac{k \cdot \frac{27}{3}}{\frac{9k}{2}} = \frac{9k}{\frac{9k}{2}} = 2 \, \text{m}
Thus, the center of gravity from the given end of the rod will be 2 m.
The center of mass of a thin rectangular plate (fig - x) with sides of length \( a \) and \( b \), whose mass per unit area (\( \sigma \)) varies as \( \sigma = \sigma_0 \frac{x}{ab} \) (where \( \sigma_0 \) is a constant), would be 