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Hugh P. Taylor Jr.

Hugh P. Taylor Jr.
Born27 December 1932 Edit this on Wikidata
Holbrook Edit this on Wikidata
Died26 October 2021 Edit this on Wikidata (aged 88)
Alma mater
Employer
Awards

Hugh Pettingill Taylor Jr. (December 27, 1932, Holbrook, Arizona – October 26, 2021) was an American geochemist.

Biography

Hugh P. Taylor Jr. and his (non-identical) twin brother lived in Arizona and New Mexico until 1943 when they moved with their parents to Los Angeles County, California. The family struggled financially. He and his brother attended South Gate High School. Their parents divorced in 1944. In 1949 Hugh P. Taylor Jr. scored the highest on a state-wide chemistry exam and won a scholarship from the American Chemical Society, enabling him to attend California Institute of Technology (Caltech). There he played varsity football, under head coach Bert LaBrucherie, and was inspired to study geology by a course taught by Professor Robert P. Sharp with the teaching assistants Clarence Allen and Leon Silver. Taylor graduated in 1954 with a B.S. in geochemistry.[1] He was one of the first two graduating geochemistry majors in Caltech's history.[2] From 1954 to 1955 Taylor was a graduate student at Harvard University, where he graduated with an M.S. in geology.[3] In 1955 he returned to Caltech as a graduate student in geochemistry. He spent the summers of 1955 and 1956 working for the U.S. Steel Corporation to explore for iron ores in southeastern Alaska.[1] His 1959 Ph.D. thesis O¹⁸/0¹⁶ Ratios in Coexisting Minerals of Igneous and Metamorphic Rocks[4] was supervised by Samuel Epstein.[2] Taylor married his first wife in 1959.[1]

Taylor had a temporary teaching position at Caltech until the end of 1960. From January 1961 until the summer of 1961 he held an appointment as an assistant professor at Pennsylvania State University.[1] At Caltech he was an assistant professor from 1962 to 1964, an associate professor from 1964 to 1969, and a full professor 1969 to 2002, when he retired as professor emeritus. From 1981 he held an appointment as Robert P. Sharp Professor of Geology. From 1987 to 1994 Taylor served as Caltech's executive officer for geology.[2]

Taylor was in the autumn semester of 1979 a Crosby Visiting professor at M.I.T.[1] He was in the academic year 1980–1981 a geologist the U.S. Geological Survey in Saudi Arabia and in the academic year 1981–1982 a visiting professor at Stanford University[3] (shortly after divorcing his first wife).[1] He served as editor for Chemical Geology and as an associate editor for Geochimica et Cosmochimica Acta.[3]

Taylor's Ph.D. research on oxygen isotopes formed the basis of much his scientific career over decades. He gained a reputation as a leading expert on stable isotopes in geochemistry. He studied rocks in terms of isotope variations of oxygen, hydrogen, carbon, silicon, and other elements.[2] In the 1960s Epstein and Taylor did research on oxygen isotope variation in tektites.[5][6][7] In the 1970s Epstein and Taylor analyzed isotopic compositions of samples of lunar rocks and minerals, returned from 6 Apollo missions — Apollo 11, 12, & 14 to 17.[8][9][10] Epstein and Taylor also analyzed samples returned by Soviet Union's Luna 20 mission.[11]

Taylor was the author or co-author of more than 150 scientific articles.[3] He was a co-editor, with John W. Valley and James R. O'Neil, of the 1986 book Stable Isotopes in High Temperature Geological Processes[12] He did research with Bruno Turi on igneous rocks in Italy.[13][14][15] Taylor and his colleagues did research on the interactions of the oceans with the underlying igneous crust, the hydrothermal circulation cells that form around intrusive igneous rocks, the geochemical origins of ore deposits[2] (such as the Comstock Lode),[16] and oxygen isotope analyses of minerals in stony meteorites.[17]

In 1981 Taylor was elected a member of the National Academy of Sciences[18] and also a fellow of the American Academy of Arts and Sciences.[19] He was awarded in 1993 the Arthur L. Day Medal and in 1995 the Urey Medal. He delivered the 30th William Smith Lecture to the Geological Society of London.[3][20]

Upon his death in 2021, Hugh P. Taylor was survived by his second wife and his son.[2]

Selected publications

References

  1. ^ a b c d e f "Taylor, Hugh P. Interview by Shirley K. Cohen. Pasadena, California, June-July, 2002". Oral History Project, California Institute of Technology Archives. August 2006.
  2. ^ a b c d e f "Caltech Mourns the Passing of Geology Professor Hugh Taylor (BS '54, PhD '59)". Caltech. January 7, 2022.
  3. ^ a b c d e Gates, Alexander E. (2009). A to Z of Earth Scientists. Infobase. p. 259. ISBN 9781438109190.
  4. ^ Taylor, Hugh Pettingill (1959). O¹⁸/0¹⁶ Ratios in Coexisting Minerals of Igneous and Metamorphic Rocks. Dissertation (Ph.D.) (phd). California Institute of Technology. doi:10.7907/1M8V-DM23.
  5. ^ Taylor, Hugh P.; Epstein, Samuel (1962). "Oxygen isotope studies on the origin of tektites". Journal of Geophysical Research. 67 (11): 4485–4490. Bibcode:1962JGR....67.4485T. doi:10.1029/JZ067i011p04485.
  6. ^ Taylor, Hugh P.; Epstein, Samue (1966). "Oxygen Isotope Studies of Ivory Coast Tektites and Impactite Glass from the Bosumtwi Crater, Ghana". Science. 153 (3732): 173–175. Bibcode:1966Sci...153..173T. doi:10.1126/science.153.3732.173. PMID 17831505. S2CID 34730477.
  7. ^ Taylor, Hugh P.; Epstein, Samuel (1969). "Correlations between O18/O16ratios and chemical compositions of tektites". Journal of Geophysical Research. 74 (27): 6834–6844. Bibcode:1969JGR....74.6834T. doi:10.1029/JB074i027p06834.
  8. ^ Epstein, S.; Taylor Jr., H. P. (1970). "The concentration and isotopic composition of hydrogen, carbon and silicon in Apollo 11 lunar rocks and minerals". In Levinson, Alfred Abraham (ed.). Geochimica et Cosmochimica Acta Supplement, Proceedings of the Apollo 11 Lunar Science Conference held 5-8 January, 1970 in Houston, TX. Volume 2: Chemical and Isotope Analyses. Vol. 1. New York: Pergammon Press. pp. 1085–1096. Bibcode:1970GeCAS...1.1085E.
  9. ^ Epstein, S. A.; Taylor Jr, H. P. (1971). "O18/O16, Si30/Si28, D/H and C13/C12 ratios in lunar samples". Proceedings of the Second Lunar Science Conference. Vol. 2. M.I.T. Press. pp. 1421–1441. Bibcode:1971LPSC....2.1421E.
  10. ^ Epstein, S.; Taylor Jr., H.P. (1973). "The isotopic composition and concentration of water, hydrogen, and carbon in some Apollo 15 and 16 soils and in the Apollo 17 orange soil". Geochimica et Cosmochimica Acta Supplement vol. 4, Proceedings of the Fourth Lunar Science Conference, vol. 2. Vol. 4. pp. 1559–1575. Bibcode:1973LPSC....4.1559E.
  11. ^ Taylor, Hugh P.; Epstein, Samuel (1973). "Oxygen and silicon isotope ratios of the Luna 20 soil". Geochimica et Cosmochimica Acta. 37 (4): 1107–1109. Bibcode:1973GeCoA..37.1107T. doi:10.1016/0016-7037(73)90204-4.
  12. ^ Valley, John W.; Taylor, Hugh P.; O'Neil, James R., eds. (June 1986). Stable Isotopes in High Temperature Geological Processes. Reviews in Mineralogy, Vol. 16. Mineralogical Society of America. ISBN 978-0939950201; pbk; vii+570 pages{{cite book}}: CS1 maint: postscript (link) ; description & table of contents, Mineralogical Society of America (minsocam.org)
  13. ^ Taylor, Hugh P.; Gregory, Robert T.; Turi, Bruno (1987). "18O/16O Evidence for Fluid-Rock Interaction in the Upper Mantle: Data from Ultramafic Nodules and K-Rich Volcanic Rocks in Italy". Chemical Transport in Metasomatic Processes. pp. 1–37. doi:10.1007/978-94-009-4013-0_1. ISBN 978-94-010-8280-8.
  14. ^ Turi, Bruno; Taylor, Hugh P. (1976). "Oxygen isotope studies of potassic volcanic rocks of the Roman Province, Central Italy". Contributions to Mineralogy and Petrology. 55 (1): 1–31. Bibcode:1976CoMP...55....1T. doi:10.1007/BF00372752. S2CID 128622001.
  15. ^ Taylor, Hugh P.; Giannetti, Bernardino; Turi, Bruno (1979). "Oxygen isotope geochemistry of the potassic igneous rocks from the Roccamonfina volcano, Roman comagmatic region, Italy". Earth and Planetary Science Letters. 46 (1): 81–106. Bibcode:1979E&PSL..46...81T. doi:10.1016/0012-821X(79)90067-0.
  16. ^ Taylor, H. P. (1973). "O18/O16 evidence for meteoric-hydrothermal alteration and ore deposition in the Tonopah, Comstock Lode, and Goldfield mining districts, Nevada". Economic Geology. 68 (6): 747–764. Bibcode:1973EcGeo..68..747T. doi:10.2113/gsecongeo.68.6.747.
  17. ^ Taylor, Hugh P.; Duke, Michael B.; Silver, Leon T.; Epstein, Samuel (1965). "Oxygen isotope studies of minerals in stony meteorites". Geochimica et Cosmochimica Acta. 29 (5): 489–512. Bibcode:1965GeCoA..29..489T. doi:10.1016/0016-7037(65)90043-8.
  18. ^ "Hugh P. Taylor". Member Directory, National Academy of Sciences.
  19. ^ "Professor Hugh Pettingill Taylor". American Academy of Arts and Sciences.
  20. ^ Taylor, H. P. (1977). "Water/Rock interactions and the origin of H2O in granitic batholiths". Journal of the Geological Society. 133 (6): 509–558. Bibcode:1977JGSoc.133..509T. doi:10.1144/gsjgs.133.6.0509. S2CID 131292784.
Quelle: https://en.wikipedia.org/wiki/Hugh_P._Taylor_Jr.