Solar Type Stars

Solar-type stars are stars similar to our Sun in size, temperature, and brightness. They belong to a category called "G-type main-sequence stars," where they generate energy through nuclear fusion of hydrogen in their cores. These stars typically have surface temperatures around 5,500 to 6,000°C and are stable over billions of years. They serve as key examples for understanding stellar life cycles and are often the stars around which planets—potentially habitable ones—may orbit. In essence, solar-type stars are common, well-studied stars that help us learn about stellar behavior and the potential for life beyond Earth.