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Emission Spectrum

/ɪˈmɪʃən ˈspɛktrəm/noun
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An emission spectrum is the distinctive series of colored lines or bands of light emitted by atoms or molecules when they release energy from an excited state, acting as a unique identifier for elements like a cosmic barcode. In today's technology, it's essential for applications such as environmental monitoring and forensic analysis, where it reveals hidden details about materials or pollutants that aren't visible to the naked eye.

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The emission spectrum of the sun revealed the existence of helium in 1868, discovered by astronomers Pierre Janssen and Norman Lockyer during a solar eclipse, making it the only element first identified outside Earth. This breakthrough not only expanded the periodic table but also paved the way for modern astrophysics, as over 90% of the universe's atoms are hydrogen and helium, elements whose spectra help map distant galaxies.

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