A meteorite is a space rock that survives its passage through Earth's atmosphere and lands on the surface. Entering the atmosphere, it becomes a meteor, creating a bright streak of light or fireball. Very bright meteors are called bolides. Meteorites vary in size, and large ones can create impact craters. Studying meteorites provides valuable insights into the solar system's composition and history, as they are remnants of asteroids, planets, or even moons.
A meteor was spotted over Houston, leading to potential meteorite landings in Harris and Montgomery Counties. NASA has created a map indicating possible strewn fields. Residents were alerted to the increased likelihood of finding meteorites.
Between 1912 and 1964, a few meteorites were found in Antarctica.
In 1915, a 61-kilogram iron meteorite was found in a Sinagua burial cyst near Camp Verde, Arizona, respectfully wrapped in a feather cloth, indicating that some Native Americans treated meteorites as ceremonial objects.
In 1959, the Příbram meteorite fell in Czechoslovakia (now the Czech Republic). Two cameras captured images of the fireball, which were used to determine the location of the stones and calculate an accurate orbit for the recovered meteorite. This was the first time such a calculation was performed for a recovered meteorite.
In 1963, the Smithsonian Astrophysical Observatory operated the Prairie Network in the midwestern US to study infalling meteorites.
Between 1912 and 1964, a few meteorites were found in Antarctica.
In 1967, after the discovery of a few meteorites in Roosevelt County, New Mexico, a public awareness campaign resulted in the finding of nearly 100 new specimens in the next few years.
In 1969, the 10th Japanese Antarctic Research Expedition found nine meteorites on a blue ice field near the Yamato Mountains, leading to the realization that ice sheets might concentrate meteorites.
In 1971, the Meteorite Observation and Recovery Project (MORP) began in Canada to study meteorite falls.
Systematic searches for meteorites in Australia began around 1971 in the Nullarbor Plain region of Western Australia and South Australia.
In 1973, a dozen other specimens were found in the same place as the 1969 discovery in Antarctica, prompting a dedicated expedition in 1974.
In 1974, a Japanese expedition was launched dedicated to the search for meteorites in Antarctica. This team recovered nearly 700 meteorites.
Since 1974, the combined efforts of expeditions have produced more than 23,000 classified meteorite specimens, with thousands more unclassified.
In 1975, the Prairie Network, operated by the Smithsonian Astrophysical Observatory, ended its operation in the midwestern US after observing meteorite falls since 1963.
In 1977, the Meteorite Observation and Recovery Project (MORP) in Canada recovered a single meteorite, Innisfree.
In 1985, the Meteorite Observation and Recovery Project (MORP) ended in Canada, after recovering a single meteorite, Innisfree.
In 1986, a German team discovered about 65 meteorites on a flat desert plain in Libya while installing a network of seismic stations for oil prospecting.
In 1989, a desert enthusiast recovered about 100 meteorites from several distinct locations in Libya and Algeria after seeing photographs of meteorites in Antarctica.
Starting in the 1990/91 season, European teams, beginning with a consortium called "EUROMET", conducted systematic searches for Antarctic meteorites.
In 1999, meteorite hunters discovered that the desert in southern and central Oman were also favorable for the collection of many specimens.
Since 2000, the Antarctic Scientific Exploration of China has conducted successful meteorite searches.
In 2002, observations by the European Fireball Network led to the discovery and orbit calculations for the Neuschwanstein meteorite.
For more information about meteorite expeditions see the article by Harvey published in 2003.
In May 2006, the first discovery of a stony meteorite found in association with a large impact crater, the Morokweng impact structure in South Africa, was reported.
In 2007, a Korean program (KOREAMET) was launched and collected a few meteorites.
In 2007, a review paper by Krot et al. summarized the modern classification and taxonomy of meteorites, which include stony meteorites (chondrites and achondrites), iron meteorites, and stony-iron meteorites.
As of mid-2009, the gravel plains in the Dhofar and Al Wusta regions of Oman had yielded about 5,000 meteorites.
In 2015, NASA scientists reported that complex organic compounds found in DNA and RNA, including uracil, cytosine, and thymine, could be formed in the laboratory under outer space conditions, using starting chemicals, such as pyrimidine, found in meteorites.
In 2018, researchers discovered that 4.5 billion-year-old meteorites found on Earth contained liquid water along with prebiotic complex organic substances, potentially the ingredients for life.
As of January 2019, the Meteoritical Bulletin Database listed 1,180 confirmed meteorite falls.
In 2019, scientists reported detecting sugar molecules, including ribose, in meteorites for the first time, suggesting that chemical processes on asteroids can produce some organic compounds fundamental to life.
In July 2024, a meteorite was recorded by security footage crashing into a residential property in Marshfield, Prince Edward Island. It is believed to be the first time such an event has been captured on camera and the sound of the crash recorded. It was subsequently registered as the Charlottetown meteorite, named after the city near to where it landed.
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