Moonlight Brightness Calculator
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Lux Reference Scale
The Science of Moonlight
How do we calculate the brightness of a rock 238,000 miles away? This tool utilizes the Krisciunas-Schaefer Photometry Model to simulate lunar luminance based on four critical physical variables.
Phase Angle
As the moon wanes, shadows lengthen inside craters, hiding bright soil. This causes brightness to drop non-linearly. A 50% lit moon is only 10% as bright as a full moon.
Atmospheric Extinction
Light scatters as it travels through air. When the moon is low on the horizon, its light passes through a thicker Air Mass, significantly reducing Lux intensity.
Opposition Surge
The "Retro-Reflection" effect. When the Sun is directly behind Earth (Full Moon), the moon's porous surface reflects light straight back, creating a 40% spike in brightness.
Orbital Distance
The moon's orbit is elliptical. During Perigee (Supermoon), it is ~30,000 miles closer than Apogee, making the moonlight up to 30% more intense.
