Starlight is the light emitted by stars. It typically refers to visible electromagnetic radiation from stars other than the Sun observable from Earth during the nighttime although a component of starlight is observable from the Earth during the daytime.
Observation and measurement of starlight through telescopes is the basis for many fields of astronomy, including photometry and stellar spectroscopy. Starlight is also a notable part of personal experience and human culture, impacting a diverse range of pursuits including poetry, astronomy, and military strategy.
The U.S. Army spent millions of dollars in the 1950s and onward to develop a starlight scope, that could amplify starlight, moonlight filtered by clouds, and the fluorescence of rotting vegetation about 50,000 times to allow a person to see in the night. In contrast to previously developed active infrared system such as sniperscope, it was a passive device and did not require additional light emission to see.
The average color of starlight in the universe is a shade of yellowish-white that has been given the name Cosmic Latte.
Starlight spectroscopy, examination of the stellar spectra, was pioneered by Joseph Fraunhofer in 1814. Starlight can be understood to be composed of three main spectra types, continuous spectrum, emission spectrum, and absorption spectrum.
- Keith Robinson - Starlight: An Introduction to Stellar Physics for Amateurs (2009) - Page 38-40 (Google Books Link)
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