Bolometric luminosity

/ˌboʊləˈmɛtrɪk ˌlumɪˈnɑsəti/ noun

The total energy output of a star across all wavelengths of electromagnetic radiation. This is different from visual luminosity, which only measures light visible to human eyes.

From Greek 'bole' (ray of light) + 'metron' (measure) + Latin 'luminositas' (brightness). The term developed in the early 20th century as astronomers realized stars emit energy across the entire electromagnetic spectrum.

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