Step 1: The number of radial nodes for any orbital is given by the formula: $\text{Radial Nodes} = n - l - 1$.
Step 2: For a 3s orbital, the principal quantum number $n = 3$ and the azimuthal quantum number $l = 0$.
Step 3: Substitute the values: $\text{Radial Nodes} = 3 - 0 - 1 = 2$.
Step 4: A radial distribution function plot ($4\pi r^2 \psi^2$ vs $r$) for a 3s orbital will touch the x-axis (zero probability) exactly at two points before reaching the final peak.