Step 1: Start from the volume expansion instead of quoting the density-change shortcut.
Heating a fixed mass $m$ of mercury lets its volume grow as $V_2 = V_1(1+\beta\Delta T)$, since $\beta$ is defined as the fractional change in volume per unit rise in temperature.
Step 2: Write the density before and after in terms of this.
\[
\rho_1 = \frac{m}{V_1}, \qquad \rho_2 = \frac{m}{V_1(1+\beta\Delta T)} = \frac{\rho_1}{1+\beta\Delta T}
\]
Step 3: Since $\beta\Delta T$ is tiny, use $\dfrac{1}{1+\beta\Delta T}\approx 1-\beta\Delta T$, giving the fractional drop in density directly.
\[
\frac{\rho_1-\rho_2}{\rho_1} \approx \beta\Delta T
\]
Step 4: Substitute $\beta = 18.2\times10^{-5}\ \text{K}^{-1}$ and $\Delta T = 60-10 = 50$ K.
\[
\frac{\Delta\rho}{\rho} \approx 18.2\times10^{-5}\times50 = 9.1\times10^{-3}
\]
Step 5: Convert to a percentage.
\[
9.1\times10^{-3}\times100\% = 0.91\%
\]
Step 6: Conclusion.
\[
\boxed{0.91\%}
\]