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Hermann Carl Vogel (Leipzig, 3 de abril de 1841 – 13 de agosto de 1907) fue un astrónomo alemán, [1] uno de los pioneros en el uso del espectroscopio en astronomía. Con este instrumento analizó la atmósfera de los planetas del Sistema Solar , siendo el primero en determinar el periodo de rotación del Sol usando el desplazamiento Doppler .
- Johann Carl Christoph Vogel
Hermann Carl Vogel ( / ˈfoʊɡəl /; German: [ˈfoːɡl̩]; 3 April 1841 – 13 August 1907) was a German astrophysicist. He was born in Leipzig, Kingdom of Saxony. From 1882 to 1907 he was director of the Astrophysical Observatory, Potsdam. He made extensive discoveries using spectral analysis of the stars.
Hermann Carl Vogel fue un astrónomo alemán, uno de los pioneros en el uso del espectroscopio en astronomía. Con este instrumento analizó la atmósfera de los planetas del Sistema Solar, siendo el primero en determinar el periodo de rotación del Sol usando el desplazamiento Doppler.
3 de abr. de 2019 · Hermann Carl Vogel, a German astronomer, was born Apr. 3, 1841. Vogel was a pioneer in applying the new science of spectroscopy to analyzing the motion of celestial bodies. Johann Doppler had discovered his famous Doppler effect back in the 1840s, revealing that the wavelengths of sound are lengthened or shortened, depending on ...
Vogel was a pioneer in the use of astronomical spectroscopy and photography. He measured the solar rotation and showed that the solar photosphere shared the rotational motion inferred from sunspots observations. He also carried out some of the first spectroscopic studies of other planets in the solar system.
Vogel made spectroscopic analyses of stars, planets, comets, and the sun. He was the first to demonstrate the sun’s rotation by measuring Doppler shifts of its receding and approaching limbs. He made detailed tables of the solar spectrum and attempted spectral classification of stars.
16 de abr. de 2024 · Hermann Karl Vogel was a German astronomer who discovered spectroscopic binaries—double-star systems that are too close for the individual stars to be discerned by any telescope but, through the analysis of their light, have been found to be two individual stars rapidly revolving around one.
