Solar radiation is the primary driver of thermal expansion in ocean water. When sunlight strikes the ocean surface, energy is absorbed by water molecules, causing them to vibrate faster and move farther apart. This increase in molecular motion results in a decrease in density and an increase in volume—thermal expansion.
This process is a fundamental engine of global ocean circulation. As surface waters warm and expand, they become lighter and tend to stay near the surface, while cooler, denser water sinks. This density-driven movement, combined with wind and the Earth's rotation, powers the great ocean currents that redistribute heat around the globe, regulating climate and weather patterns.
Thermal expansion is also a major contributor to sea-level rise. As the oceans absorb over 90% of the excess heat trapped by greenhouse gases, the water itself expands, raising sea levels even without melting ice sheets.