Harold Kroto
Encyclopedia : H : HA : HAR : Harold Kroto
Sir Harold Walter Kroto KBE , FRS , Ph.D (born 7 October, 1939) is an English chemist and one of the winners of the 1996 Nobel Prize in Chemistry.
He spent a large part of his working career at the University of Sussex, and is currently on faculty at Florida State University.
Early life
He was born, christened Harold Krotoschiner in Wisbech, Cambridgeshire, England with his unusual name being of Silesian origin. His father's family came from Bojanowo, Poland, and his mother's from Berlin, Germany.Both his parents were born in Berlin but came to Great Britain in the 1930s as refugees from the Nazis because his father was Jewish.
He was raised in Bolton, Lancashire, England, where he attended Bolton School, where he was a contemporary of the highly acclaimed actor Sir Ian McKellen. In 1955 the family name was shortened to Kroto.
As a child, he became fascinated by a Meccano set. Kroto credits Meccano — amongst other things — with developing skills useful in scientific research. He was raised Jewish, but the religion never made any sense to him.
He now claims to have four "religions": humanism, atheism, amnesty-internationalism and humourism. He developed an interest in chemistry, physics, and mathematics in secondary school, and because his sixth form chemistry teacher (Harry Heaney - who subsequently became a University Professor) felt that the University of Sheffield had the best chemistry department in the United Kingdom, he went to Sheffield.
In 1963 he married the former Margaret Henrietta Hunter (now Margaret, Lady Kroto).
Early work
In 1961 he took a first class B. Sc. honours degree in chemistry at the University of Sheffield, followed in 1964 by a Ph. D. at the same institution. His doctoral research involved high-resolution electronic spectra of free radicals produced by flash photolysis (breaking of chemical bonds by light).Among other things such as making the first phosphaalkenes (compounds with carbon phosphorus double bonds), his doctoral studies included some unpublished research on carbon suboxide, O=C=C=C=O, and this led to a general interest in molecules containing chains of carbon atoms with numerous multiple bonds. He started his work with an interest in organic chemistry, but when he learned about spectroscopy it inclined him to quantum chemistry.
After postdoctoral research at the National Research Council in Canada and Bell Laboratories in the USA he began teaching and research at the University of Sussex in England in 1967. He became a full professor in 1985, and a Royal Society Research Professor from 1991 – 2001.
Subsequent work
In the 1970s he launched a research programme at Sussex to look for carbon chains in interstellar space. Earlier studies had detected the molecule cyanoacetylene, H-C≡C-C≡N. Kroto's group searched for spectral evidence of longer similar molecules such as cyanobutadiyne, H-C≡C-C≡C-C≡N and cyanohexatriyne, H-C≡C-C≡C-C≡C-C≡N, and found them from 1975–1978.Trying to explain them led to the discovery of the C60 molecule. (See buckminsterfullerene.) He heard of laser spectroscopy work being done by Richard Smalley and Robert Curl at Rice University in Texas. He suggested that they should use the Rice apparatus to simulate the carbon chemistry that occurs in the atmosphere of a carbon star.
The experiment carried out in September 1985 not only proved that carbon stars could produce the chains but revealed an amazing, serendipitous result - the totally unexpected existence of the C60 species. The three scientists carried out the work with graduate students Jim Heath (now a full Professor at Cal. Tech.), Sean O'Brien (now at Texas Instruments), and Yuan Liu (now at Oak Ridge). The Nobel Prize in Chemistry was shared by Curl, Kroto and Smalley in 1996.
In 1995 he jointly set up the Vega Science Trust a UK educational charity (see [www.vega.org.uk]) to create high quality science films for TV and Internet Broadcast. Vega has produced some 92 programmes of which 50 have been broadcast on BBC TV in the late-night slots all programmes stream for free from the Vega website. Viewing figures vary from 600,000 to 300,000.
He presently carries out research in Nanoscience and Nanotechnology.
Awards and Honours
Kroto was elected a Fellow of the Royal Society in 1990, and was awarded a knighthood (becoming Sir Harold Kroto) in 1996. Later that year he received the Nobel Prize in Chemistry.His alma mater, the University of Sheffield, awarded him an honorary doctorate in 1995 at the undergraduate degree congregation.
On 29 November, 2004, Kroto announced he was to return his honorary degree from the University of Exeter, in protest over the closure of their Department of Chemistry.
He was awarded the 2004 Copley Medal of the Royal Society.
On 17 June, 2005, the University of Surrey conferred an honorary doctorate on him at an undergraduate degree ceremony. (see [link]) University of Surrey Press Release.
External links
- [Harry Kroto autobiography from Nobel foundation]
- [Sir Harry Kroto FRS - Chemical architecture] from the Royal Society
- [Harry Kroto homepage at the University of Sussex]
- [Professor Harry Kroto]
- [Vega Science Trust]
- [Harry Kroto personal website]
- [Florida State University page]
| width="" align="" valign="" style="padding-left:;"| 1901: van 't Hoff
1902: E.Fischer
1903: Arrhenius
1904: Ramsay
1905: von Baeyer
1906: Moissan
1907: Buchner
1908: Rutherford
1909: Ostwald
1910: Wallach
1911: Curie
1912: Grignard, Sabatier
1913: Werner
1914: Richards
1915: Willstätter
1918: Haber
1920: Nernst
1921: Soddy
1922: Aston
1923: Pregl
1925: Zsigmondy
1926: Svedberg
1927: Wieland
1928: Windaus
1929: Harden, von Euler‑Chelpin
1930: H.Fischer
1931: Bosch, Bergius
1932: Langmuir
1934: Urey
1935: F.Joliot‑Curie, I.Joliot‑Curie
1936: Debye
1937: Haworth, Karrer
1938: Kuhn
| width="" align="" valign="" style="padding-left:;"| 1939: Butenandt, Ružička
1943: de Hevesy
1944: Hahn
1945: Virtanen
1946: Sumner, Northrop, Stanley
1947: Robinson
1948: Tiselius
1949: Giauque
1950: Diels, Alder
1951: McMillan, Seaborg
1952: Martin, Synge
1953: Staudinger
1954: Pauling
1955: du Vigneaud
1956: Hinshelwood, Semyonov
1957: Todd
1958: Sanger
1959: Heyrovský
1960: Libby
1961: Calvin
1962: Perutz, Kendrew
1963: Ziegler, Natta
1964: Hodgkin
1965: Woodward
1966: Mulliken
1967: Eigen, Norrish, Porter
1968: Onsager
1969: Barton, Hassel
1970: Leloir
1971: Herzberg
1972: Anfinsen, Moore, Stein
1973: E.O.Fischer, Wilkinson
| width="" align="" valign="" style="padding-left:;"| 1974: Flory
1975: Cornforth, Prelog
1976: Lipscomb
1977: Prigogine
1978: Mitchell
1979: Brown, Wittig
1980: Berg, Gilbert, Sanger
1981: Fukui, Hoffmann
1982: Klug
1983: Taube
1984: Merrifield
1985: Hauptman, Karle
1986: Herschbach, Lee, Polanyi
1987: Cram, Lehn, Pedersen
1988: Deisenhofer, Huber, Michel
1989: Altman, Cech
1990: Corey
1991: Ernst
1992: Marcus
1993: Mullis, Smith
1994: Olah
1995: Crutzen, Molina, Rowland
1996: Curl, Kroto, Smalley
1997: Boyer, Walker, Skou
1998: Kohn, Pople
1999: Zewail
2000: Heeger, MacDiarmid, Shirakawa
2001: Knowles, Noyori, Sharpless
2002: Fenn, Tanaka, Wüthrich
2003: Agre, MacKinnon
2004: Ciechanover, Hershko, Rose
2005: Grubbs, Schrock, Chauvin
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