KnowraKirchhoff's laws of spectroscopyLinked fromLinked fromThe 11 pages that link to Kirchhoff's laws of spectroscopy, each with the reason it gives.All 11Broader topic 1Related 9Compared with 1Stellar spectroscopyRelated: They explain why stars show absorption lines while surrounding hot gas can produce emission lines.Astronomical spectroscopyRelated: They connected observed line patterns with the sources and gases producing them.Atomic spectrumRelated: They explain why the same element can create bright or dark lines in different settings.Robert BunsenRelated: These laws supplied the physical basis for interpreting the lines Bunsen observed.Atomic spectroscopyRelated: They established how spectral lines can identify elements in hot sources and cooler intervening gas.Fraunhofer linesRelated: The solar lines helped connect dark spectral features to cooler absorbing gas.Solar spectrumRelated: They explain why cooler solar gas imprints dark lines on brighter continuous light.Joseph von FraunhoferRelated: These laws explained why dark lines appear in sunlight and connected them to elemental absorption.Heinrich KayserRelated: These laws explained why laboratory spectra could identify elements in stars.