Rhian H. Jones (born 1960) [1] is a British planetary scientist whose research focuses on chondrites and the evidence they provide on how the Solar System formed. She is Reader in Isotope Geo- and Cosmochemistry in the Department of Earth and Environmental Sciences at the University of Manchester. [2]
Jones read chemistry at the University of Oxford, earning a bachelor's degree there in 1983. She completed a PhD in geology at the University of Manchester in 1986. [3]
She went to the University of New Mexico for postdoctoral research, beginning her lifelong work on meteorites, and remained at the university as a faculty member for many years, [2] also becoming curator of meteorites for the university's Institute of Meteoritics. [4] In 2015, she retired from the University of New Mexico as a professor emerita, [5] [6] and returned to the University of Manchester as a reader. [2]
Jones is the 2023 winner of the Price Medal of the Royal Astronomical Society, "in recognition of her outstanding contributions in a series of closely-linked investigations using chondritic meteorites to understand the composition and formation of the first planetary bodies in the Solar System". [7]
Asteroid 5366 Rhianjones is named for her. [1] [7]
Cosmochemistry or chemical cosmology is the study of the chemical composition of matter in the universe and the processes that led to those compositions. This is done primarily through the study of the chemical composition of meteorites and other physical samples. Given that the asteroid parent bodies of meteorites were some of the first solid material to condense from the early solar nebula, cosmochemists are generally, but not exclusively, concerned with the objects contained within the Solar System.
Grenville Turner is a research professor at the University of Manchester. He is one of the pioneers of cosmochemistry.
Meteoritics is the science that deals with meteors, meteorites, and meteoroids. It is closely connected to cosmochemistry, mineralogy and geochemistry. A specialist who studies meteoritics is known as a meteoriticist.
George Wetherill was a physicist and geologist and the Director Emeritus of the Department of Terrestrial Magnetism at the Carnegie Institution of Washington, DC, USA.
The Meteoritical Society is a non-profit scholarly organization founded in 1933 to promote research and education in planetary science with emphasis on studies of meteorites and other extraterrestrial materials that further our understanding of the origin and history of the Solar System.
Dante S. Lauretta is a professor of planetary science and cosmochemistry at the University of Arizona's Lunar and Planetary Laboratory. He is currently serving as the principal investigator on NASA's OSIRIS-REx mission.
Harry "Hap" Y. McSween is Chancellor's Professor Emeritus of Planetary Geoscience at the University of Tennessee at Knoxville. He has published papers and popular books about meteorites and planetary exploration, and textbooks on geochemistry and cosmochemistry.
The Allende meteorite is the largest carbonaceous chondrite ever found on Earth. The fireball was witnessed at 01:05 on February 8, 1969, falling over the Mexican state of Chihuahua. After it broke up in the atmosphere, an extensive search for pieces was conducted and over 2 tonnes were recovered. The availability of large quantities of samples of the scientifically-important chondrite class has enabled numerous investigations by many scientists; it is often described as "the best-studied meteorite in history." The Allende meteorite has abundant, large calcium–aluminium-rich inclusions (CAI), which are among the oldest objects formed in the Solar System.
Extraterrestrial material refers to natural objects now on Earth that originated in outer space. Such materials include cosmic dust and meteorites, as well as samples brought to Earth by sample return missions from the Moon, asteroids and comets, as well as solar wind particles.
Gerald J. Wasserburg was an American geologist. At the time of his death, he was the John D. MacArthur Professor of Geology and Geophysics, Emeritus, at the California Institute of Technology. He was known for his work in the fields of isotope geochemistry, cosmochemistry, meteoritics, and astrophysics.
Christian Köberl is a professor of impact research and planetary geology at the University of Vienna, Austria. From June 2010 to May 2020 he was director general of the Natural History Museum in Vienna. He is best known for his research on meteorite impact craters.
Laurie Leshin is an American scientist and academic administrator serving as the 10th Director of the NASA Jet Propulsion Laboratory and as Vice President and Bren Professor of Geochemistry and Planetary Science at California Institute of Technology. Leshin's research has focused on geochemistry and space science. Leshin previously served as the 16th president of Worcester Polytechnic Institute.
Planetary science is the scientific study of planets, celestial bodies and planetary systems and the processes of their formation. It studies objects ranging in size from micrometeoroids to gas giants, aiming to determine their composition, dynamics, formation, interrelations and history. It is a strongly interdisciplinary field, which originally grew from astronomy and Earth science, and now incorporates many disciplines, including planetary geology, cosmochemistry, atmospheric science, physics, oceanography, hydrology, theoretical planetary science, glaciology, and exoplanetology. Allied disciplines include space physics, when concerned with the effects of the Sun on the bodies of the Solar System, and astrobiology.
Robert Norman Clayton was a Canadian-American chemist and academic. He was the Enrico Fermi Distinguished Service Professor Emeritus of Chemistry at the University of Chicago. Clayton studied cosmochemistry and held a joint appointment in the university's geophysical sciences department. He was a member of the National Academy of Sciences and was named a fellow of several academic societies, including the Royal Society.
Anat Shahar is a staff scientist at the Earth and Planets Laboratory, Carnegie Institution of Washington and adjunct Professor at the University of Maryland. Her work uses high-pressure, high-temperature experiments and stable isotope geochemistry to understand the formation of planets in the solar system.
Toshiko K. Mayeda was a Japanese American chemist who worked at the Enrico Fermi Institute in the University of Chicago. She worked on climate science and meteorites from 1958 to 2004.
The Department of Earth and Environmental Sciences at The University of Manchester is one of the oldest earth and environmental science departments in the UK. The Department takes roughly 100 new undergraduates and 140 postgraduates each year, and employs 90 members of academic staff, 41 postdoctoral researchers, 27 technical staff and 20 administrative staff.
Hiroko Nagahara is a Japanese cosmochemist and astromineralogist whose research studies the chemical composition and formation of chondrules, the molten mineral droplets that accrete to form asteroids and meteoroids. She is a fellow of the Earth–Life Science Institute of the Tokyo Institute of Technology, a professor emerita of Tokyo University, and a former president of the Meteoritical Society.
Katharina Lodders is a German-American planetary scientist and cosmochemist who works as a research professor in the Department of Earth and Planetary Sciences at Washington University in St. Louis, where she co-directs the Planetary Chemistry Laboratory. Her research concerns the chemical composition of solar and stellar environments, including the atmospheres of planets, exoplanets, and brown dwarfs, and the study of the temperatures at which elements condense in stellar environments.
Nicolas Dauphas is a French-American planetary scientist and isotope geochemist. He is the Louis Block professor of geochemistry and cosmochemistry in the Department of the Geophysical Sciences and Enrico Fermi Institute at the University of Chicago. His research focuses on isotope geochemistry and cosmochemistry. He studies the origin and evolution of planets and other objects in the solar system by analyzing the natural distributions of elements and their isotopes using mass spectrometers.