Density of nuclear matter is independent of mass number, so the required ratio is 1: 1.
Alternative
$A_{1}: A_{2}=1: 3$
Their radii will be in the ratio
$R_{0} A_{1}^{1 / 3}: R_{0} A_{2}^{1 / 3}$
$=1: 3^{1 / 3}$
Density $=\frac{A}{\frac{4}{3} \pi R^{3}}$
$\therefore \rho_{A_{1}}: \rho_{A_{2}}=\frac{1}{\frac{4}{3} \pi R_{0}^{3} \cdot 1^{3}}$
$=\frac{4}{3} \pi R_{0}^{3}\left(3^{1 / 3}\right)^{3}$
Their nuclear densities will be the same.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of