Meteorites

For thousands of years, people living in Egypt, China, Greece, Rome, and other parts of the world have been fascinated by shooting stars, which are the light and sound phenomena commonly associated with meteorite impacts. The earliest written record of a meteorite fall is logged by Chinese chronicle...

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Main Authors: Wang, Kun, Korotev, Randy
Format: Book Part
Language:English
Published: Oxford University Press 2019
Subjects:
Online Access:http://dx.doi.org/10.1093/acrefore/9780190647926.013.16
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spelling croxfordunivpr:10.1093/acrefore/9780190647926.013.16 2024-10-13T14:03:12+00:00 Meteorites Wang, Kun Korotev, Randy 2019 http://dx.doi.org/10.1093/acrefore/9780190647926.013.16 en eng Oxford University Press Oxford Research Encyclopedia of Planetary Science ISBN 9780190647926 reference-entry 2019 croxfordunivpr https://doi.org/10.1093/acrefore/9780190647926.013.16 2024-09-17T04:31:38Z For thousands of years, people living in Egypt, China, Greece, Rome, and other parts of the world have been fascinated by shooting stars, which are the light and sound phenomena commonly associated with meteorite impacts. The earliest written record of a meteorite fall is logged by Chinese chroniclers in 687 <sc>bce</sc>. However, centuries before that, Egyptians had been using “heavenly iron” to make their first iron tools, including a dagger found in King Tutankhamun’s tomb that dates back to the 14th century <sc>bce</sc>. Even though human beings have a long history of observing meteors and utilizing meteorites, we did not start to recognize their true celestial origin until the Age of Enlightenment. In 1794 German physicist and musician Ernst Chladni was the first to summarize the scientific evidence and to demonstrate that these unique objects are indeed from outside of the Earth. After more than two centuries of joint efforts by countless keen amateur, academic, institutional, and commercial collectors, more than 60,000 meteorites have been catalogued and classified in the Meteoritical Bulletin Database. This number is continually growing, and meteorites are found all over the world, especially in dry and sparsely populated regions such as Antarctica and the Sahara Desert. Although there are thousands of individual meteorites, they can be handily classified into three broad groups by simple examinations of the specimens. The most common type is stony meteorite, which is made of mostly silicate rocks. Iron meteorites are the easiest to be preserved for thousands (or even millions) of years on the Earth’s surface environments, and they are composed of iron and nickel metals. The stony-irons contain roughly the same amount of metals and silicates, and these spectacular meteorites are the favorites of many collectors and museums. After 200 years, meteoritics (the science of meteorites) has grown out of its infancy and become a vibrant area of research today. The general directions of ... Book Part Antarc* Antarctica Oxford University Press
institution Open Polar
collection Oxford University Press
op_collection_id croxfordunivpr
language English
description For thousands of years, people living in Egypt, China, Greece, Rome, and other parts of the world have been fascinated by shooting stars, which are the light and sound phenomena commonly associated with meteorite impacts. The earliest written record of a meteorite fall is logged by Chinese chroniclers in 687 <sc>bce</sc>. However, centuries before that, Egyptians had been using “heavenly iron” to make their first iron tools, including a dagger found in King Tutankhamun’s tomb that dates back to the 14th century <sc>bce</sc>. Even though human beings have a long history of observing meteors and utilizing meteorites, we did not start to recognize their true celestial origin until the Age of Enlightenment. In 1794 German physicist and musician Ernst Chladni was the first to summarize the scientific evidence and to demonstrate that these unique objects are indeed from outside of the Earth. After more than two centuries of joint efforts by countless keen amateur, academic, institutional, and commercial collectors, more than 60,000 meteorites have been catalogued and classified in the Meteoritical Bulletin Database. This number is continually growing, and meteorites are found all over the world, especially in dry and sparsely populated regions such as Antarctica and the Sahara Desert. Although there are thousands of individual meteorites, they can be handily classified into three broad groups by simple examinations of the specimens. The most common type is stony meteorite, which is made of mostly silicate rocks. Iron meteorites are the easiest to be preserved for thousands (or even millions) of years on the Earth’s surface environments, and they are composed of iron and nickel metals. The stony-irons contain roughly the same amount of metals and silicates, and these spectacular meteorites are the favorites of many collectors and museums. After 200 years, meteoritics (the science of meteorites) has grown out of its infancy and become a vibrant area of research today. The general directions of ...
format Book Part
author Wang, Kun
Korotev, Randy
spellingShingle Wang, Kun
Korotev, Randy
Meteorites
author_facet Wang, Kun
Korotev, Randy
author_sort Wang, Kun
title Meteorites
title_short Meteorites
title_full Meteorites
title_fullStr Meteorites
title_full_unstemmed Meteorites
title_sort meteorites
publisher Oxford University Press
publishDate 2019
url http://dx.doi.org/10.1093/acrefore/9780190647926.013.16
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Oxford Research Encyclopedia of Planetary Science
ISBN 9780190647926
op_doi https://doi.org/10.1093/acrefore/9780190647926.013.16
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