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Chemistry of heavenly bodies in 1878 illustration
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French chemist Eugene Chevreuls Colours of the solar spectrum showing colours from the solar spectrum produced by a carbon disulfide prism Solid
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Fraunhofers solar spectrum illustration
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Fraunhofers solar spectrum illustration
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Solar spectrum
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Joseph von Fraunhofers (1787-1826) diagram of the lines of the solar spectrum and above it a curve showing the intensity of sunlight in different pa
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William Hyde Wollaston (1766-1828) English chemist born at East Dereham Norfolk England Wollaston discovered Palladium (1804) Rhodium (1805) a
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Spectroscope 1872 Instrument of the type developed by Robert Bunsen (1811-1899) and Robert Kirchhoff (1824-1887) during the 1850s Their work provid
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Spectroscope 1872 Instrument of the type developed by Robert Bunsen (1811-1899) and Robert Kirchhoff (1824-1887) during the 1850s Their work provi
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Spectroscope 1872 Instrument of the type developed by Robert Bunsen (1811-1899) and Robert Kirchhoff (1824-1887) during the 1850s Their work provi
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Spectrum of visible light emitted from the sub-giant star Procyon (Alpha Canis Minoris) At bottom left is the shortest wavelength visible around 400
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William Hyde Wollaston (1766-1828) Caricature of the English chemist and physicist William Hyde Wollaston Wollaston is best known for developing the
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Prism and spectrum
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Fraunhofer lines Illustration of the Suns spectrum showing a set of dark absorption lines known as Fraunhofer lines These are named after the Germ
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Fraunhofer lines Illustration of the Suns spectrum showing a set of dark absorption lines known as Fraunhofer lines These are named after the Germ
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Continuous spectrum with Fraunhofer lines top and comparison spectra Chromolithogrpah 1892
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Joseph von Fraunhofers (1787-1826) diagram of the lines of the solar spectrum and above it a curve showing the intensity of sunlight in different pa
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Joseph von Fraunhofer (1787-1826) German physicist Developed the spectrum and mapped the lines of the solar spectrum (Fraunhofer lines) Engraving
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William Hyde Wollaston (1766-1828) English chemist born at East Dereham Norfolk England Wollaston discovered Palladium (1804) Rhodium (1805) an
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Continuous spectrum with Fraunhofer lines top and comparison spectra Chromolithogrpah 1892
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Fraunhofer lines Illustration of the Suns spectrum showing a set of dark absorption lines known as Fraunhofer lines These are named after the Germ
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Fraunhofer lines Illustration of the Suns spectrum showing a set of dark absorption lines known as Fraunhofer lines These are named after the Germ
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Star spectra Diagram of the spectra of stars showing a set of dark absorption lines known as Fraunhofer lines The spectrum is shown ranging from bl
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Fraunhofer lines Diagram of the Suns spectrum showing a set of dark absorption lines known as Fraunhofer lines These are named after the German ph
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Sirius emission spectrum This multicoloured band is obtained by recording what wavelengths of light (each seen as a different colour) are emitted by
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Joseph von Fraunhofer (1787-1826) German physicist Developed the spectrum and mapped the lines of the solar spectrum (Fraunhofer lines) Engraving
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William Hyde Wollaston (1766-1828) English chemist born at East Dereham Norfolk England Wollaston discovered Palladium (1804) Rhodium (1805) a
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Joseph von Fraunhofers (1787-1826) diagram of the lines of the solar spectrum and above it a curve showing the intensity of sunlight in different pa
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Joseph von Fraunhofer (1787-1826) German physicist Developed the spectrum and mapped the lines of the solar spectrum (Fraunhofer lines) Engraving
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Portrait of the German physicist and optician Josef von Fraunhofer 1787-1826 Fraunhofer was apprenticed as a mirror-maker and lens polisher in Munic
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Omicron Ceti emission spectrum This multicoloured band is obtained by recording what wavelengths of light (each seen as a different colour) are emitt
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Betelgeuse emission spectrum This multicoloured band is obtained by recording what wavelengths of light (each seen as a different colour) are emitted
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Aldebaran emission spectrum This multicoloured band is obtained by recording what wavelengths of light (each seen as a different colour) are emitted
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Pleiades emission spectra These multicoloured bands are obtained by recording what wavelengths of light (each seen as a different colour) are emitted
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THIS PICTURE MAY NOT BE USED TO STATE OR IMPLY NOAO ENDORSEMENT OF ANY COMPANY OR PRODUCT Solar spectrum This shows the range of visible lig
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BTHIS PICTURE MAY NOT BE USED TO STATE OR IMPLY THE BENDORSEMENT BY NOAO OF ANY COMPANY OR PRODUCT THIS PICTURE MAY NOT BE USED TO STATE OR IMP
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THIS PICTURE MAY NOT BE USED TO STATE OR IMPLY NOAO ENDORSEMENT OF ANY COMPANY OR PRODUCT Solar spectrum This shows the range of visible lig
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BTHIS PICTURE MAY NOT BE USED TO STATE OR IMPLY THE BENDORSEMENT BY NOAO OF ANY COMPANY OR PRODUCT THIS PICTURE MAY NOT BE USED TO STATE OR IMP
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