Takeshi Oka

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Takeshi Oka
岡 武史
Born1932
NationalityJapanese
CitizenshipJapan
Alma materUniversity of Tokyo
Known forDiscover the Trihydrogen cation (H3+)
Hydronium
Methanium
AwardsEarle K. Plyler Prize (1982)
William F. Meggers Award (1997)
Ellis R. Lippincott Award (1998)
E. Bright Wilson Award in Spectroscopy (2002)
Davy Medal (2004)
Scientific career
FieldsAstrochemistry
InstitutionsUniversity of Tokyo
Herzberg Institute of Astrophysics
University of Chicago
Academic advisorsGerhard Herzberg[1]
Doctoral studentsMoungi G. Bawendi
Benjamin J. McCall
Christopher M. Lindsay
Christopher G. Tarsitano
Jennifer L. Gottfried
Christopher P. Morong
Christopher F. Neese[1]
Other notable studentsMitchio Okumura[1]

Takeshi Oka (岡 武史, Oka Takeshi, born 1932), FRS FRSC, is a Japanese-American chemist and astronomer specializing in the field of galactic astronomy, known as the pioneer of astrochemistry and the discoverer of extraterrestrial trihydrogen cation (H+
3
).[3]

He is now R.A. Milliken Distinguished Service Emeritus Professor, Departments of Astronomy and Astrophysics, Chemistry; Enrico Fermi Institute; and the College of University of Chicago.[4]

Education

Oka was born in Tokyo, Japan, on 1932. He received his BS and PhD degree in 1955 and 1960, respectively, from the University of Tokyo.[2]

Career

In 1963, Oka working as a postdoctoral fellow with Harry Kroto at Gerhard Herzberg's laboratory,[5] National Research Council of Canada. Among them, Kroto and Herzberg have won the Nobel Prize in Chemistry, furthermore, the Nobel laureate Robert Curl was also Oka's colleague.[6]

From 1960 to 1963, Oka appointed a fellow at JSPS, the University of Tokyo. Afterward, he was successively worked at Herzberg Institute of Astrophysics (1963-1981), and the University of Chicago (1981-).[2]

In 1980, Oka discovered the infrared spectrum of H+
3
, and revealed that "molecular clouds" are the birthplace of stars and that the chemical evolution of the clouds is a crucial step in star formation.[3]

Currently, Oka group's studies specializing in the field of the quantum mechanics and dynamics of fundamental molecular ions and their behavior in astronomical objects.[2]

Honors and awards[2]

Oka was on the list of ChemBank's prediction for the 2015 Nobel Prize in Chemistry.[7]

Awards

Titles

  • 2004 - Wei Lun Visiting Professorship.
  • 2004 - Honorary DSc from the University College London.
  • 2003 - Earl W. McDaniel Lecture Georgia Institute of Technology.
  • 2001 - Honoris caua, University of Waterloo.
  • 2000 - George Pimentel Memorial Lecture, University of California, Berkeley.
  • 1998 - Medaili Jana Marca Marci.
  • 1997 - Distinguished JILA Visitor.
  • 1995 - Golden Jubilee Lecture, Tata Institute of Fundamental Research.
  • 1992 - Special Issue, Journal of Molecular Spectroscopy, Vol. 153.
  • 1992 - Lecturer, International School of Physics, "Enrico Fermi".
  • 1992 - Lord Lecturer, Massachusetts Institute of Technology.
  • 1989 - McDowell Lecturer, University of British Columbia.
  • 1985-1986 - Chancellor's Distinguished Lecturer, University of California, Berkeley.
  • 1981-1982 - Centenary Lecturer, Royal Society.

Membership in learned societies

Publications[2]

  • Near-infrared electronic spectrum of CH2+. J. Chem. Phys., 121, 11527 (2004).
  • High-resolution spectroscopy of the 22Πu←Χ4Σg- forbidden transitions of C2+. J. Chem. Phys., 121, 6290 (2004)
  • Atomic and molecular emission lines from the Red Rectangle. Astrophys. J., 615, 947 (2004)
  • The non-thermal rotational distribution of H3+. Astrophys. J., 613, 349 (2004).
  • Nuclear spin selection rules in chemical reactions by angular momentum algebra. J. Mol. Spectroscc., 228, 635 (2004).
  • Near-infrared spectroscopy of H3+ above the barrier to linearity. J. Chem. Phys., 118, 10890 (2003).
  • Observations of C3 in translucent sightlines. Astrophys. J., 582, 823 (2003).
  • Absorption line survey of H3+ toward the Galactic center sources I. GCS 3-2 and GC IRS2. Publ. Astron. Soc. Japan,, 54, 951 (2002).
  • Observation of H3+ in the diffuse interstellar medium. Astrophys. J., 567, 391 (2002).
  • Sharp Spectral Lines Observed in γ-Ray Ionized Parahydrogen Crystals. Phys. Rev. Lett. 86, 4795 (2001).
  • CH5+:The Infrared Spectrum Observed. Science, 284, 135 (1999).

See also

References

  1. ^ a b c Chemistry Tree - Takeshi Oka Details
  2. ^ a b c d e f "University Webpage". University of Chicago. Retrieved July 14, 2016.
  3. ^ a b Jian Tang and Takeshi Oka (1999). "Infrared spectroscopy of H
    3
    O+
    : the v1 fundamental band". J. Mol. Spectrosc. 196 (1): 120–130. Bibcode:1999JMoSp.196..120T. doi:10.1006/jmsp.1999.7844. PMID 10361062.
  4. ^ The Department of Astronomy and Astrophysics | Takeshi Oka
  5. ^ Sir Harold Kroto - Biographical
  6. ^ Robert F. Curl Jr. - Biographical
  7. ^ Nobel Predictions | ChemBark

External links