Yusuke Hagihara
Hagihara in 1954
Born28 March 1897
Osaka, Japan
Died29 January 1979
Tokyo, Japan
Alma materTokyo Imperial University (BSc 1921)
University of Tokyo (D.Sc. 1930)
Scientific career
Fields
  • Astronomy
  • Celestial mechanics
InstitutionsUniversity of Tokyo
Tokyo Astronomical Observatory
Japan Academy
Notable studentsYoshio Fujita

Yusuke Hagihara (萩原 雄祐, Hagihara Yūsuke, 28 March 1897 in Osaka – 29 January 1979 in Tokyo) was a Japanese astronomer noted for his contributions to celestial mechanics.[1]

Life and work

Hagihara graduated from Tokyo Imperial University with a degree in astronomy in 1921 and became an assistant professor of astronomy there two years later.[2] In 1923 the Japanese government sent him abroad as a traveling scholar. Hagihara went to Cambridge University in England to study differential equations under the mathematician Henry Frederick Baker[2] and relativity alongside Paul Dirac under the astrophysicist Sir Arthur Stanley Eddington.[1][3] He was a visiting scholar in France, Germany, and the United States.[1]

He returned to Japan in 1925 but left for the United States three years later to study the topology of dynamical systems at Harvard University under George David Birkhoff on a Rockefeller Foundation Fellowship.[3]

Hagihara finished his studies at Harvard in 1929 and returned again to the University of Tokyo, where, in 1930, he completed a D.Sc. dissertation on the stability of satellite systems.[2] In 1935, he published a paper showing that the trajectory of a test particle in the Schwarzschild metric can be expressed in terms of elliptic functions.[3] For more than a decade after 1937, he investigated the distribution of electron velocities in planetary nebulae.[3]

He was promoted to full professor at the University of Tokyo in 1935.[2] From 1945 to 1957 he was the director of the Tokyo Astronomical Observatory and subsequently was a professor at Tohoku University (1957–1960) and president of Utsunomiya University (1961–1967).[3] In 1961 he was elected vice-president of the International Astronomical Union and president of the IAU's commission on celestial mechanics.[2]

He retired from all of his official duties, except for the Japan Academy, in 1967 and devoted himself to writing his comprehensive five volume work, Celestial Mechanics, which was based on his lecture notes.[2]

Hagihara was regarded as a quiet and cultured gentleman, an excellent teacher and a capable administrator.[1][2]

He has pointed out the importance of the post-Newton models for celestial mechanics, namely that developed by Georgi Manev.[citation needed]

Honors

Works

See also

References

  1. ^ a b c d Herget, Paul (1979). "Yusuke Hagihara". Physics Today. 32 (6): 71. Bibcode:1979PhT....32f..71H. doi:10.1063/1.2995600.
  2. ^ a b c d e f g Kozai, Yoshihide (1979). "Yusuke Hagihara". Quart. Jour. Royal Astron. Soc. 20 (3): 325–8.
  3. ^ a b c d e Kozai, Yoshihide (1998). "Development of Celestial Mechanics in Japan". Planet. Space Sci. 46 (8): 1031–36. Bibcode:1998P&SS...46.1031K. doi:10.1016/s0032-0633(98)00033-6.
  4. ^ Schmadel, Lutz D. (2007). "(1971) Hagihara". Dictionary of Minor Planet Names – (1971) Hagihara. Springer Berlin Heidelberg. p. 159. doi:10.1007/978-3-540-29925-7_1972. ISBN 978-3-540-00238-3.
  • Greene, Jay E., ed. (1980). McGraw-Hill Modern Scientists and Engineers. 3 vols. New York: McGraw-Hill.
Categories