Friedrich Georg Wilhelm von Struve (Russian:Василий Яковлевич Струве, trans.Vasily Yakovlevich Struve; 15 April 1793 – 23 November [O.S. 11 November] 1864) was aBaltic Germanastronomer andgeodesist. He is best known for studyingdouble stars and initiating a triangulation survey later namedStruve Geodetic Arc in his honor.
In 1808 he entered theUniversity of Tartu (Dorpat), where he first studiedphilology, but soon turned his attention toastronomy. From 1813 to 1820, he taught at the university and collected data at theTartu Observatory, and in 1820 became a full professor and director of the observatory. His teachings have had a strong effect that is still felt at the university.[3][4][5]
Struve's name is best known for his observations ofdouble stars, which he carried on for many years. Although double stars had been studied earlier byWilliam Herschel,John Herschel andSir James South, Struve outdid any previous efforts. While at Dorpat he obtained in 1824 a refracting telescope with an aperture of 23 cm (about 9 inches) made byJoseph von Fraunhofer, said to be a masterpiece of optical and mechanical quality.[10] With this telescope Struve discovered a very large number of double stars. In 1827 published his double star catalogueCatalogus novus stellarum duplicium.[5] Stars of his catalogue are sometimes indicated by the Greek letter sigma, Σ. Thus, 61 Cygni is also designated as Σ2758.
Since mostdouble stars are truebinary stars rather than mereoptical doubles (as William Herschel had been the first to discover), they orbit around their commonbarycenter and slowly change position over the years. Thus Struve made micrometric measurements of 2714 double stars from 1824 to 1837 and published these in his workStellarum duplicium et multiplicium mensurae micrometricae.[5]
Struve carefully measured the "constant ofaberration" in 1843. He was also the first to measure theparallax of the starVega, althoughFriedrich Bessel had been the first to measure the parallax of a star (61 Cygni).[5]
In an 1847 work,Etudes d'Astronomie Stellaire: Sur la voie lactee et sur la distance des etoiles fixes, Struve was one of the first astronomers to identify the effects ofinterstellar extinction (though he provided no mechanism to explain the effect). His estimate of the average rate of visual extinction, 1 mag per kpc, is remarkably close to modern estimates (0.7–1.0 mag per kpc).[5]
Struve was the second of a dynasty of astronomers through five generations. He was the great-grandfather ofOtto Struve and the father ofOtto Wilhelm von Struve. He was also the grandfather ofHermann von Struve, who was Otto Struve's uncle.
^abcdefghiA. H. Batten (1977). "The Struves of Pulkovo – A Family of Astronomers".Journal of the Royal Astronomical Society of Canada.71: 345.Bibcode:1977JRASC..71..345B.