
The fraction of incident light that a surface reflects, here describing a planet's brightness.Reflectivity, also called albedo, is the fraction of incident light that a surface reflects. For planets, it determines how much sunlight is bounced back into space versus absorbed, directly influencing surface temperature and climate. A high-reflectivity planet stays cooler, while a low-reflectivity one absorbs more heat. This property is key for understanding planetary atmospheres, detecting exoplanets, and studying dark matter interactions that might heat a planet's interior.
The concept of albedo was formalized by Johann Heinrich Lambert in the 18th century, and later extended by August Beer and others for planetary studies.
Reflectivity depends on the surface material, roughness, and wavelength of light. For a planet, it is measured as the ratio of reflected to incident radiation across the spectrum. Ice and clouds have high reflectivity, while oceans and dark rock have low reflectivity. The balance between absorbed and reflected energy drives the planet's energy budget.
Reflectivity measurements are used in climate modeling, satellite remote sensing, and the search for habitable exoplanets by analyzing their reflected light.
The Earth's albedo is about 0.3, meaning it reflects 30% of incoming sunlight, but this varies with cloud cover and snow extent.




