|Author:||Harold J. Abrahams|
|Publisher:||Fairleigh Dickinson Univ Pr; illustrated edition edition (April 1, 1983)|
|Other formats:||rtf lit mbr doc|
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Arizona: Selected Correspondence between Daniel Moreau Barringer and Elihu Thomson. Barringer, B. (1964) Daniel Moreau Barringer (1860-1929) and his crater (The beginning of the Crater Branch of Meteoritics). Meteoritics, v. 2, pp. 183-199.
1983) Heroic Efforts at Meteor Crater, Arizona: Selected Correspondence between Daniel Moreau Barringer and Elihu Thomson. Associated University Press, East Brunswick, 322 p. Ackermann, . 1966) P-wave velocity and attenuation summary, FY-66. (1967) Historical notes on the Odessa Meteorite Crater.
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Daniel Barringer (May 25, 1860 – November 30, 1929) 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, owned privately by Barringer and now by his family, has been renamed the Barringer Crater in his honor, although this name is mainly used in the scientific community.
by. Barringer, Daniel Moreau.
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Author Barringer, Daniel Moreau, 1860-1929. Categories: Nonfiction. 7/10 2. Books by Barringer, Daniel Moreau, 1860-1929: Meteor Crater (Formerly Called Coon Mountain Or Coon Butte) in Northern Central Arizona.
Daniel Moreau Barringer (July 30, 1806 – September 1, 1873) was a Whig . Congressman from North Carolina between 1843 and 1849. He joined the Democratic Party by the early 1870s. Born near Concord, North Carolina, in 1806 to Elizabeth Brandon and Paul Barringer, Daniel had nine siblings, including at least two brothers. His middle name is from French Huguenot ancestors, who came as refugees to North Carolina. The Barringer sons were likely tutored at home in their early studies.
The differences between deformation at Meteor Crater and Lonar Crater may reflect the same disparities seen in. .
The differences between deformation at Meteor Crater and Lonar Crater may reflect the same disparities seen in simple craters produced in different target lithologies on Mars and other planetary surfaces. Atomic absorption analyses of 25 metallic spheroids from Barringer Meteorite Crater have been carried out for Fe, Ni, Co and Cu. In addition, electron microprobe analyses of 58 impactite metallic particles have been carried out for Fe, Ni and Co from four different impactite samples. The normalized Ni, Co and Cu contents of the spheroids were from 13–22 per cent, . –1. 3 per cent and 260–430 μg/g, respectively.
Barringer Crater, also known as Meteor Crater, Arizona, or Canyon Diablo Crater, is one of the world's youngest, most extensively studied, and best preserved meteorite impact craters. The location has been extensively developed as an educational and interpretive facility. Buildings, parking, and trails have been put in place both to protect the crater and to maximize the visitor's opportunity to view and learn about the structure. Barringer Crater is located at the end of a clearly marked paved road, a few miles south of Interstate 40, between Winslow and Flagstaff, Arizona