Chladni became interested in meteoritics following a conversation he had with
Georg Christoph Lichtenberg about a fireball that Lichtenberg supposedly saw in the
Gӧttingen sky in November 1791. Inspired by this report, Chladni researched reports of similar phenomena as well as reports of other falling masses across Europe and North America within the last century. Based on the uniformity among these sightings, he concluded that the phenomena of fireballs and falling masses must be genuine. This led him to publish
Über den Ursprung der von Pallas gefundenen und anderer ihr ähnlicher Eisenmassen und über einige damit in Verbindung stehende Naturerscheinungen ("On the Origin of the Iron Masses Found by
Pallas and Others Similar to it, and on Some Associated Natural Phenomena") in 1794. In this book he proposed that
meteorites have an
extraterrestrial origin. He argued that this would explain the high speeds of the falling masses as well as linking the masses to the fireballs; they glow intensely bright as they enter the Earth's atmosphere. He hypothesized that these meteorites were chunks of material that had either never been consolidated in the formation of larger masses or were debris from the formation and destruction of
planets. This was a controversial statement at the time, since meteorites were thought to be of volcanic origin. Additionally, his claims challenged the established belief that nothing existed beyond the Moon except for other stars and planets. Indeed, this supposed emptiness of space had fascinated Chladni as a child when he learned about the relatively large distance between Mars and Jupiter, where the
Asteroid Belt is now known to exist. This observation factored into his account for the origins of meteorites. Chladni's book was initially ridiculed by contemporary physicists, including Lichtenberg. Still, his writings sparked a curiosity that eventually led to more researchers supporting his theory. In 1795, a large
stony meteorite was observed during its fall to Earth at a cottage near
Wold Newton in
Yorkshire,
England and a piece of it, known as the
Wold Cottage meteorite, was given to the
British chemist Edward Howard who, along with
French mineralogist
Jacques de Bournon, carefully analyzed its composition and concluded that an extraterrestrial origin was likely, noting that the sample bore a strong resemblance to a sample of a meteorite from an early meteor shower in
Siena, Italy. Although that event had been attributed to an eruption of
Mount Vesuvius a few hundred kilometers away, no similar volcanoes exists within the same range of Wold Newton, with the closest being
Hekla in
Iceland. In 1803, the physicist and
astronomer Jean Baptiste Biot was commissioned by the
French Minister of the Interior to investigate
a meteor shower over L'Aigle in northern France that had peppered the town with thousands of meteorite fragments. Unlike Chladni's book and the scientific publication by Howard and de Bournon, Biot's lively report became popular and persuaded more people to take Chladni's insights seriously. Chladni's insights have led some in the field to call him the "father of meteoritics" while others have been more conservative with their appraisal of Chladni's contributions to the field. Chladni continued to develop his record of meteorite sightings throughout the next several decades as well as amassing a collection of meteorite samples. He donated this collection to the Mineralogical Museum of Berlin University in 1827 and it now resides in the Museum of Natural History at Humboldt University of Berlin. A mineral, first described in 1993 from the Carlton (IIICD) iron meteorite, was named in his honor. == Other work ==