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Biography. Honours. Lectures. Awards. Named after him. Works. References. External links. Herbert Hall Turner FRS (13 August 1861 – 20 August 1930) was a British astronomer and seismologist . Biography. Herbert Hall Turner was educated at the Leeds Modern School, Clifton College, [1] Bristol and Trinity College, Cambridge. [2] .
- Bruce Medal (1927)
- 20 August 1930 (aged 69), Stockholm, Sweden
- 13 August 1861, Leeds, England
Leeds Modern School. Ocupação. astronomia, sismólogo. Prêmios. Medalha Bruce (1927) Empregador (a) Universidade de Oxford. [ edite no Wikidata] Herbert Hall Turner ( Leeds, 13 de agosto de 1861 — Estocolmo, 20 de agosto de 1930) foi um astrônomo e sismólogo britânico.
- Reino Unido
12 de abr. de 2024 · Herbert Hall Turner (born Aug. 13, 1861, Leeds, Yorkshire, Eng.—died Aug. 20, 1930, Stockholm, Sweden) was an English astronomer who pioneered many of the procedures now universally employed in determining stellar positions from astronomical photographs.
- The Editors of Encyclopaedia Britannica
After serving as chief assistant at the Royal Greenwich Observatory for nine years, he spent most of his career as Savilian professor of astronomy at the University of Oxford. One of the leaders in the worldwide effort to produce an astrographic chart of the sky, he developed improved methods.
Turner, Herbert Hall (updated) Born Leeds, England, 13 August 1861. Died Stockholm, Sweden, 20 August 1930. Besides making fundamental contributions to the disciplines of astronomy and seismology, Herbert Turner was a leading advocate of international cooperation in science. He was the eldest son of John and Isabella Turner.
Herbert Hall Turner ( Leeds, 13 de agosto de 1861 — Estocolmo, 20 de agosto de 1930) foi um astrônomo e sismólogo britânico. Factos rápidos. Fechar. Biografia. Herbert Hall Turner foi educado na Leeds Modern School, Clifton College, Bristol e Trinity College, Cambridge.
Creator: Herbert Hall Turner Reference number: RR/15/226 Referee's report by Herbert Hall Turner, on a paper 'The distribution of blue and violet light in the corona on August 30, 1905, as derived from photographs taken at Kalaa-es-Senam, Tunisia' by L Becker
