Jan Hendrik Oort

Oort, Jan Hendrik


Born Apr. 28, 1900, in Franeker. Dutch astronomer. Professor at the University of Leiden (1935).

In 1924, Oort began working at the Leiden Observatory, and from 1945 to 1970 he was its director. He is primarily involved in the study of stellar motion. In 1927 he proposed formulas for the detection of the differential rotation of the Milky Way Galaxy by observing the radial velocities and proper motions of the stars; applying his formulas, he demonstrated the rotation of the galaxy. In 1938 he proposed a method for determining the spatial density distribution of the stars. He also worked on problems involving the structure of the interstellar medium and the Milky Way Galaxy using cosmic radio-emission data. From 1935 to 1948 he was secretary-general and from 1958 to 1961 president of the International Astronomical Union. He is a foreign member of the Academy of Sciences of the USSR (1966).


“Investigations Concerning the Rotational Motion of the Galactic System.” Bulletin of the Astronomical Institutes of the Netherlands, 1927, vol. 4.
“Dynamics of the Galactic System in the Vicinity of the Sun.” Ibid., 1928, vol. 4.
“Absorption and Density Distribution in the Galactic System.” Ibid., 1938, vol. 8.
References in periodicals archive ?
Las siguientes detecciones podran confirmar otra teoria, la del origen de los co metas, propuesta por Jan Hendrik Oort, quien planteo que esos cuerpos se forman a partir de una nube de material planetario residual.
Incidentally, Franeker was also the birthplace of the great Dutch astronomer Jan Hendrik Oort, who died in November 1992.
It seemed to the Dutch astronomer Jan Hendrik Oort (b.
El astronomo holandes Jan Hendrik Oort propuso que los cometas se forman a partir de una nube de material planetario residual, es decir de restos de la materia con la que se crearon todos los planetas.