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• W2552174157 abstract "Joe Goldstein, who passed away on June 27, was an extraordinarily accomplished researcher and much loved professor and colleague. Joe was born in Syracuse, New York, and received his bachelor's, master's, and doctorate degrees in metallurgy from the Massachusetts Institute of Technology in 1960, 1962, and 1964, respectively. At MIT, he was introduced to the electron microprobe and to meteorites by his advisor, Robert Ogilvie. After working from 1964 to 1968 at the NASA Goddard Space Flight Center in Greenbelt, Maryland, Joe became a professor of Metallurgy and Material Sciences at Lehigh University and developed a worldwide reputation for his work on microanalysis and on extraterrestrial materials. He was a pioneer in scanning electron microscopy and X-ray microanalysis and generously shared his expertise organizing short courses and writing and editing several books, most notably the best-selling textbook Scanning Electron Microscopy and X-ray Microanalysis, which was published in 1981 and updated in 1992 and 2003. The Lehigh Microscopy School, which Joe founded, has educated thousands of analysts in electron microscopy and microanalysis during the past 45 years. Joe Goldstein was a skilled and accomplished university administrator. At Lehigh University, he served as Vice-President for Research for seven years, from 1983 to 1990. He became Dean of the College of Engineering at the University of Massachusetts, Amherst in 1993, a position he held for 11 years while maintaining an active research lab. In 2003, Joe was named a Distinguished Professor at Amherst in recognition of his remarkable academic achievements and his extraordinary level of productivity. He continued as a faculty member of the Department of Mechanical and Industrial Engineering at Amherst until he retired in 2014. After his retirement, he continued to work on research papers until he passed away from amyotrophic lateral sclerosis. Joe Goldstein was a rare scientist who excelled in two very different fields. To his faculty colleagues, he was a materials scientist who used electron microscopy and electron microprobe analysis to characterize alloys and oxides at the nano-scale level to solve practical problems in materials science and engineering. He used the data obtained by electron microscopy to derive solid-state diffusion rates and compositional data for phase diagrams. In addition, he investigated diffusion-controlled phase transformations, spinodal decomposition, and order-disorder reactions using computer simulations. To his cosmochemical colleagues, Joe Goldstein was the acknowledged expert in characterizing the chemical composition and structure of Fe-Ni metal at the micrometer and nanometer scale in diverse kinds of extraterrestrial materials to elucidate their origin and thermal history. He and his students are best known for their work on deriving cooling rates at 650–400 °C for iron meteorites from the chemical zoning in taenite grains. In a long series of papers, Goldstein and his students and post-docs studied subsolidus phase equilibria in the Fe-Ni, Fe-Ni-P, Fe-Ni-Co, Fe-Ni-C, and Fe-Ni-S system and diffusion rates in the Fe-Ni-P system so that thermal histories of metal in meteorites could be refined using computer modeling. Joe collaborated with many colleagues in studying metal grains in a variety of meteorites to help understand their origin. Metallic Fe-Ni, phosphides, and carbides in Apollo rocks and soils were analyzed to help understand their origin and elucidate the role of impacts in the lunar regolith. Metallic spherules from the Barringer Meteorite Crater were studied to help elucidate the origin and cooling rate of lunar metallic spherules formed by impact melting. Joe studied metal in pallasites and mesosiderites to constrain their cooling rates and showed that they cooled slower than iron meteorites. He used diverse metallographic techniques to constrain the thermal history of shocked and heated ordinary chondrites. In addition, Joe studied metal grains in CB chondrites and was invited to help study metal grains returned from comet Wild 2. One of his important scientific legacies is a wonderful tool-kit of techniques for petrologists who study metal-bearing extraterrestrial materials and want to elucidate their origin and impact history. Joe Goldstein belonged to many scientific societies but the one he enjoyed most was the Meteoritical Society. In an oral history recorded by Derek Sears, he said, “I really enjoyed the people, the accomplishments, being in a society where people really care” (Sears 2012). Joe served the Society as Councilor (1975–1978), Annual Meeting Organizer (1976), Treasurer (1995–1998), and President (2007–2008). He was also a very active member of the Investments and the Endowment Committee for many years, and was instrumental in establishing the Society's Legacy Program. Joe Goldstein received many awards for his leadership in science and his service to his colleagues and students during his career. In 1965, he was awarded the Nininger Meteorite Award by Arizona State University for his graduate research on the growth of the Widmanstätten pattern. In 1999, he received the Henry Clifton Sorby Award from the International Metallographic Society in recognition of his lifetime achievements in metallurgy. This award to Joe was very appropriate for several reasons. Sorby was not only the “father of metallography” but he was also a pioneer in petrography who invented the polarizing microscope for studying rocks in thin section, and was the first to describe chondrules in thin section in 1864. Joe's work on iron meteorites epitomized Sorby's belief that great conclusions could be derived from the study of minute objects (Sorby 1858; Young 2003). The 5–10 km wide asteroid 4989 was named Joegoldstein in his honor in 2000 by Schelte J. Bus, who discovered the asteroid at the Anglo-Australian Telescope. In 2005 Joe received the Leonard Medal from the Meteoritical Society for his work on metal, phosphide, carbide, and sulfide in meteorites and lunar rocks; the formation of the Widmanstätten pattern and the determination of cooling rates in irons, stony-irons, and chondrites; the nature of plessite and martensite formation; and determinations of phase diagrams for the Fe-Ni, Fe-Ni-P, Fe-Ni-Co, Fe-Ni-C, and Fe-Ni-S systems. I was very fortunate to work closely with Joe over many years. I met him first in 1970 at Lehigh University when I was a graduate student on my first visit to the United States. He very kindly invited me to stay with him and his wife, Barbara, and went out of his way to help and advise me with my research. In the past 10 years, I have been especially fortunate and honored to work closely with Joe on a series of papers with his colleague, Jijin Yang, on the thermal and impact histories of irons and stony-iron meteorites. We had a lot of fun and made some exciting discoveries. Two more papers are still in the pipeline. How fortunate we have been to have such a wise, generous, and considerate colleague who cared deeply about meteorites, planetary science, and his friends. Joe Goldstein set us a wonderful example of how we should pursue excellence as scientists and conduct ourselves honorably while enjoying life to the fullest. Joe was loved and revered by his students and colleagues and will be deeply missed. In recognition of Joe Goldstein's exceptional work in training many generations of students in microanalytical techniques, the Microanalysis Society and the Meteoritical Society have jointly established the Joseph Goldstein Scholar Award to help train young scientists in microanalytical techniques and advance their careers either by attending a microanalysis course or by visiting a microanalysis facility to make measurements." @default.
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