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Moonlight consists of mostly sunlight (with little earthlight) reflected from the parts of the Moon's surface where the Sun's light strikes. The ancient Greek philosopher Anaxagoras was aware that "the sun provides the moon with its brightness". The intensity of moonlight varies greatly depending on the lunar phase, but even the full moon typically provides only about 0.05–0.1 lux illumination. When a full Moon around perigee (a "supermoon") is viewed around upper culmination from the tropics, the illuminance can reach up to 0.32 lux. From Earth, the apparent magnitude of the full Moon is only about that of the Sun. The color of moonlight, particularly around full moon, appears bluish to the human eye compared to other, brighter light sources due to the Purkinje effect. The blue or silver appearance of the light is an illusion. The Moon's bond albedo averages 0.136, meaning only 13.6% of incident sunlight is reflected from the lunar surface. Moonlight takes approximately 1.26 seconds to reach Earth's surface. Scattered in Earth's atmosphere, moonlight generally increases the brightness of the night sky, reducing contrast between dimmer stars and the background. For this reason, many astronomers usually avoid observing sessions around a full moon. File:ISS-44 Moon - Goodnight Earth.jpg|Moonlight onto Earth's cloud cover from space File:Sunrise over the VLT.jpg|Moonlight shines on the [[Very Large Telescope]]. File:Tonsvatnet, tåke og måne.JPG|Moonlight illuminates a lake and surroundings. File:Giftedtypist - red moon (by).jpg|During a [[lunar eclipse]], the Moon is colored red by indirect [[sunlight]], which [[Earth's atmosphere]] has [[light scattering|scattered]] and [[atmospheric refraction|refracted]]. File:Earthshine Moon.jpg|[[earthlight (astronomy)|Earthlight]] (indirect sunlight reflected from Earth) illuminates the dim side of the Moon, while direct sunlight the bright side. File:High ISO with long exposure.jpg|With manual [[exposure (photography)|exposure]] settings, photographs taken in moonlight do not appear much different from those taken in [[daylight]].

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Starlight

Starlight is the light emitted by stars. It typically refers to visible electromagnetic radiation from stars other than the Sun, observable from Earth at night, although a component of starlight is observable from Earth during daytime. Sunlight is the term used for the Sun's starlight observed during daytime. During nighttime, albedo describes solar reflections from other Solar System objects, including moonlight, planetshine, and zodiacal light.

Night sky

The night sky is the nighttime appearance of celestial objects like stars, planets, and the Moon, which are visible in a clear sky between sunset and sunrise, when the Sun is below the horizon. Natural light sources in a night sky include moonlight, starlight, and airglow, depending on location and timing. Aurorae light up the skies above the polar circles. Occasionally, a large coronal mass ejection from the Sun or simply high levels of solar wind may extend the phenomenon toward the Equator.

Lux

The lux (symbol: lx) is the unit of illuminance, or luminous flux per unit area, in the International System of Units (SI). It is equal to one lumen per square metre. In photometry, this is used as a measure of the intensity, as perceived by the human eye, of light that hits or passes through a surface. It is analogous to the radiometric unit watt per square metre, but with the power at each wavelength weighted according to the luminosity function, a model of human visual brightness perception, standardized by the CIE and ISO.

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