Barringer Medal | |
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Awarded for | Outstanding work in the field of impact cratering |
Sponsored by | Barringer Crater Company |
Presented by | Meteoritical Society |
Reward(s) | Medal |
First awarded | 1984 |
Website | www.meteoriticalsociety.org |
The Barringer Medal recognizes outstanding work in the field of impact cratering and/or work that has led to a better understanding of impact phenomena. [1] The Barringer Medal and Award were established to honor the memory of D. Moreau Barringer Sr. and his son D. Moreau Barringer Jr. and are sponsored by the Barringer Crater Company. The medal is awarded by the Meteoritical Society. The senior Barringer was the first to seriously propose an impact origin for the crater that now bears his name.
The first recipient, Eugene Shoemaker, co-discovered Comet Shoemaker–Levy 9 and was the first to offer accepted proof of Barringer Crater’s meteoritic origin. [2]
Year | Name [3] |
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1984 | Eugene M. Shoemaker |
1985 | Robert S. Dietz |
1986 | Donald E. Gault |
1987 | Wolf J. von Engelhardt |
1988 | Michael R. Dence |
1989 | Virgil E. Barnes |
1990 | Richard A. F. Grieve |
1991 | Victor L. Masaitis |
1992 | Edward C. T. Chao |
1993 | Dieter Stöffler |
1994 | D. W. Roddy |
1995 | William A. Cassidy |
1996 | F. Hörz |
1997 | T. Ahrens |
1998 | B. A. Ivanov |
1999 | H. Jay Melosh |
2000 | Ralph Belknap Baldwin |
2001 | Alexander T. Basilevsky |
2002 | Bevan M. French |
2003 | Graham Ryder |
2004 | Peter H. Schultz |
2005 | Billy P. Glass |
2006 | Robert M. Schmidt |
2007 | Christian Koeberl |
2008 | Frank T. Kyte |
2009 | Wolf Uwe Reimold |
2010 | William K. Hartmann |
2011 | Bruce F. Bohor |
2012 | Jan Smit |
2013 | Walter Alvarez |
2014 | Alex Deutsch |
2015 | Natalia Artemieva |
2016 | Keith Holsapple |
2017 | Akira Fujiwara |
2018 | Thomas Kenkmann |
2019 | Mark Cintala |
2020 | Joanna Morgan [4] |
2021 | Gordon Osinski |
2022 | Gareth Collins and Kai Wünnemann |
2023 | Birger Schmitz |
2023 | John Spray |
An impact crater is a circular depression in the surface of a solid astronomical object formed by the hypervelocity impact of a smaller object. In contrast to volcanic craters, which result from explosion or internal collapse, impact craters typically have raised rims and floors that are lower in elevation than the surrounding terrain. Lunar impact craters range from microscopic craters on lunar rocks returned by the Apollo program and small, simple, bowl-shaped depressions in the lunar regolith to large, complex, multi-ringed impact basins. Meteor Crater is a well-known example of a small impact crater on Earth.
A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the atmosphere to reach the surface of a planet or moon. When the original object enters the atmosphere, various factors such as friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate energy. It then becomes a meteor and forms a fireball, also known as a shooting star; astronomers call the brightest examples "bolides". Once it settles on the larger body's surface, the meteor becomes a meteorite. Meteorites vary greatly in size. For geologists, a bolide is a meteorite large enough to create an impact crater.
Meteor Crater or Barringer Crater is a meteorite impact crater about 37 mi (60 km) east of Flagstaff and 18 mi (29 km) west of Winslow in the desert of northern Arizona, United States. The site had several earlier names, and fragments of the meteorite are officially called the Canyon Diablo Meteorite, after the adjacent Canyon Diablo.
An impact event is a collision between astronomical objects causing measurable effects. Impact events have physical consequences and have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, though atmospheres mitigate many surface impacts through atmospheric entry. Impact craters and structures are dominant landforms on many of the Solar System's solid objects and present the strongest empirical evidence for their frequency and scale.
Eugene Merle Shoemaker was an American geologist. He co-discovered Comet Shoemaker–Levy 9 with his wife Carolyn S. Shoemaker and David H. Levy. This comet hit Jupiter in July 1994: the impact was televised around the world. Shoemaker also studied terrestrial craters, such as Barringer Meteor Crater in Arizona, and along with Edward Chao provided the first conclusive evidence of its origin as an impact crater. He was also the first director of the United States Geological Survey's Astrogeology Research Program.
Carolyn Jean Spellmann Shoemaker was an American astronomer and a co-discoverer of Comet Shoemaker–Levy 9. She discovered 32 comets and more than 500 asteroids.
Daniel Barringer was a geologist best known as the first person to prove the existence of an impact crater on the Earth, Meteor Crater in Arizona. The site has been renamed the Barringer Crater in his honor, which is the preferred name used in the scientific community. A small lunar crater on the far side of the Moon is also named after him.
Veevers crater is an impact crater located on a flat desert plain between the Great Sandy and Gibson Deserts in the centre of the state of Western Australia.
Grove Karl Gilbert, known by the abbreviated name G. K. Gilbert in academic literature, was an American geologist.
Barringer is a surname. Notable people with the surname include:
The Canyon Diablo meteorite refers to the many fragments of the asteroid that created Meteor Crater, Arizona, United States. Meteorites have been found around the crater rim, and are named for nearby Canyon Diablo, which lies about three to four miles west of the crater.
Lunar craters are impact craters on Earth's Moon. The Moon's surface has many craters, all of which were formed by impacts. The International Astronomical Union currently recognizes 9,137 craters, of which 1,675 have been dated.
Graham Ryder was an English geologist and lunar scientist.
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.
H. Jay Melosh was an American geophysicist specialising in impact cratering. He earned a degree in physics from Princeton University and a doctoral degree in physics and geology from Caltech in 1972. His PhD thesis concerned quarks. Melosh's research interests include impact craters, planetary tectonics, and the physics of earthquakes and landslides. His recent research includes studies of the giant impact origin of the Moon, the Chicxulub impact that is thought to have extinguished most dinosaurs, and studies of ejection of rocks from their parent bodies. He was active in astrobiological studies that relate chiefly to the exchange of microorganisms between the terrestrial planets.
Edward Ching-Te Chao was one of the founders of the field of impact metamorphism, the study of the effects of meteorite impacts on the Earth's crust.
Peter H. Schultz is Professor of Geological Sciences at Brown University specializing in the study of planetary geology, impact cratering on the Earth and other objects in the Solar System, and volcanic modifications of planetary surfaces. He was co-investigator to the NASA Science Mission Directorate spacecraft Deep Impact and the Lunar Crater Observation and Sensing Satellite (LCROSS). He was awarded the Barringer Medal of the Meteoritical Society in 2004 for his theoretical and experimental studies of impact craters.
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.
Victor A. Gostin is an Australian geologist, who discovered in the Flinders Ranges of South Australia, a deposit of volcanic material that was ejected from the 300-kilometre distant Acraman crater when the impact was created by a meteorite some 580 million years ago. He is an associate professor at the University of Adelaide, Department of Earth Sciences, School of Physical Sciences.
Ludovic Ferrière is a geologist and curator of the meteorite collection and of the impactite collection at the Natural History Museum, Vienna, Austria. He is known for his research on meteorite impact craters.