Mercury remains liquid at room temperature due to its unique electronic structure and low binding energy relative to other metals. It has a fully filled 6s2 valence subshell, which contributes to its inertness and low boiling point of -39°C. The valence electrons in mercury are tightly bound to the nucleus, with poor screening from the diffuse 4f electrons, resulting in a higher effective nuclear charge. Additionally, the large atomic size of mercury leads to relativistic effects that lower the energy state of its valence electrons. These factors collectively explain why mercury is an exception among transition metals, maintaining a liquid state under standard conditions.