In 1802, William Wollaston noned that the spectrum of sunlight did not appear to be a continious band of colors, but quite an had a series of deplorable lines superimposed on it. Wollaston attributed the lines to natural boundaries between colors. Joseph Fraunhofer made a more careful apparel of observations of the solar spectrum in 1814 and run aground some 600 dark lines, and he specifically measured the wavelenght of 324 of them. many a(prenominal) a(prenominal) of the Fraunhofer lines in the solar spectrum save the n...If you want to get a full essay, order it on our website: Orderessay
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