English English | Deutsch Deutsch

Map Campo del Cielo meteorite
Campo del Cielo

The Campo del Cielo iron meteorite fell 4200 - 4700 years ago, about 1000 km northwest of Buenos Aires in Argentina. More than 100 tons of material has been recovered so far. The largest single meteorite found in the Campo del Cielo strewnfield is called 'Gancedo' and weighs 30.8 tons. It is the second largest known meteorite on the earth's surface after the Hoba meteorite. During impact more than 20 craters were formed in a large area of many square kilometres; the largest crater is about 100 metres in diameter. These craters have various forms; some of them were created when a part of the meteorite hit the ground at such an acute angle that the meteorite bounced back up again, leaving a shallow crater behind. The main body of the meteorite - which had a diameter of at least 5 metres before it entered Earth's atmosphere - broke into pieces after atmospheric entry. Due to the high velocity of the meteorite of several km/s (ten thousand miles per hour) the surfaces of the pieces heated up and melted. Some Campo del Cielo specimens have nice regmaglypts attesting to the enormous heat and speeds to which the fragments were exposed during their atmospheric flight.

Campo del Cielo 9000 g
Campo del Cielo 9000 g
Campo del Cielo was discovered in 1576 by members of the Spanish military, but the site was already well known to the local Indians before this and they probably used parts of the iron for their weapons. In the following centuries several expeditions were made and recovered most of the meteorites. Analysis of the strewn field shows that the meteorite came from the south-west at a very flat angle of just 9°. As with most meteorites, Campo del Cielo originated in the asteroid belt. A collision with another asteroid belt object created the meteoroid and sent it into a new, elliptical orbit. The orbit's closest distance to the Sun lay inside the Earth's orbit, so Campo del Cielo became a so-called Apollo asteroid.

Fragments of Campo del Cielo come in a wide range of sizes from small specimens of just a few grams to much rarer big pieces of tens, and sometimes even hundreds, of kilograms. A few specimens - mainly still domiciled in Argentina - have masses exceeding 1 tonne. Many of the small ones, often sold as 'crystals', were once bigger specimens that were cooled down with liquid nitrogen and then shattered into smaller pieces. The pieces shatter along their octahedral planes; this way the crystalline structure is revealed. Sometimes they have flat surfaces where the natural crystal faces used to be. Anyhow, the surfaces of these pieces are not formed during atmospheric flight.

This is an overview of the known pieces with masses > 200 kg:

Name Weight Year of discovery
Current location
Gancedo 30.8 tons 2016 Gancedo, Chaco, Argentina. Gancedo is the second heaviest meteorite on Earth.
El Chaco 28.8 tons 1980 Gancedo, Chaco, Argentina. El Chaco is the third heaviest meteorite on Earth.
Mesón de Fierro 15 tons 1576 Lost. This was the first specimen discovered by the Spanish military.
La Sorpresa 15 tons 2005 Chaco, Argentina
NO NAME 10 tons 1997 Near its find site, Chaco, Argentina
El Toba 4210 kg 1923 MACN, Buenos Aires city, Argentina
La Perdida (2) 3370 kg 1965 Still in the crater.
El Taco 1998 kg 1962 Main mass at National Museum of Natural History, Smithsonian Institution, Washington, DC; USA; 600 kg at Planetarium of Buenos Aires city, Argentina
La Perdida (1) 1625 kg 1965 Planetarium, Buenos Aires city, Argentina
El Mataco 998 kg 1937 Museo Provincial, Rosario, Santa Fe, Argentina
El Tonocote 850 kg 1931 Planetarium, Buenos Aires city, Argentina
Runa Pocito 750 kg 1803 British Museum, London, United Kingdom
El Mocoví 732 kg 1925 MACN, Buenos Aires city, Argentina
El Avipón 460 kg 1936 Museo Argentino de Ciencias Naturales, (MACN), Buenos Aires City, Argentina
El Patio 350 kg before 1960 Estancia El Taco, Chaco, Argentina

See our iron meteorites for sale.

All text and articles published by Sun.org are licensed under a Creative Commons Attribution-ShareAlike 4.0 International License.

Creative Commons License
Published by Published or last modified on 2016-09-22