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Münster (upm/anb).
A find from the “Ribbeck” meteorite.<address>© Dennis Harries</address>
A find from the “Ribbeck” meteorite.
© Dennis Harries

Ribbeck meteorite from the Havelland is 4.5 billion years old

Researchers from the University of Münster analysed 202 fragments

At the beginning of this year, on 21 January, a huge fireball was visible over the German state of Brandenburg. It was the result of a small celestial body entering the Earth’s atmosphere, bursting and falling to the ground in numerous fragments near Ribbeck in the Havelland. After hundreds of people set out in the days that ensued to search for the remains of the crashed body, researchers led by Professor Dr Addi Bischoff and Dr Markus Patzek from the Institute of Planetology at the University of Münster were able to examine the finds. The two scientists and nearly 30 other colleagues from five countries have published their findings in the journal Meteoritics & Planetary Science under the title “Cosmic pears from the Havelland (Germany): Ribbeck, the twelfth recorded aubrite fall in history”. The “cosmic pears” allude to the famous poem “Herr von Ribbeck auf Ribbeck im Havelland” by Theodor Fontane and the pears that the eponymous character distributes.

Map view of the debris field at Ribbeck, Berge and Lietzow. The arrows mark the artefacts that the scientists examined.<address>© Andreas Möller</address>
Map view of the debris field at Ribbeck, Berge and Lietzow. The arrows mark the artefacts that the scientists examined.
© Andreas Möller
In their publication, the authors report that 202 fragments of the meteorite were found, with a total weight of 1.8 kilograms. The scatter field covered an area of 1.5 by 10 kilometres near the villages of Ribbeck, Berge and Lietzow. Thanks to the unusually quick and successful search, the team was able to begin their investigation just a few days after the crash. However, without realising it at the time, the searchers were presented with a special challenge. “When searching for meteorites, you usually look for black rocks. However, due to their mineralogy and composition, the Ribbeck fragments did not have a consistently dark fusion crust. This is probably why numerous fragments were missed in the first days of the search, until this peculiarity was recognised,” explains Addi Bischoff, first author of the publication.

Addi Bischoff (left) and Markus Patzek examine the artefacts using a scanning electron microscope.<address>© Uni MS - Institut für Planetologie</address>
Addi Bischoff (left) and Markus Patzek examine the artefacts using a scanning electron microscope.
© Uni MS - Institut für Planetologie
During the analysis, the scientists determined that the “Ribbeck” meteorite belongs to the rather rare meteorite class of aubrites. This class is named after the Aubres meteorite, which fell on France in 1936 and of which there are only twelve cases in the world. Aubrites are rich in magnesium and silicon. The “Ribbeck” meteorite, for its part, occupies a special position within its class, as the rock has an exceptionally high proportion of feldspar – a mineral belonging to the silicate group.

This image clearly shows the so-called brecciation of the “Ribbeck” meteorite with its solidified debris fragments.<address>© Markus Patzek</address>
This image clearly shows the so-called brecciation of the “Ribbeck” meteorite with its solidified debris fragments.
© Markus Patzek
The researchers estimate that the parent body of the “Ribbeck” meteorite is around 4.5 billion years old and originates from the asteroid belt between the orbits of the planets Mars and Jupiter. “The intense brecciation of the rock indicates a turbulent past with devastating impacts on the parent body,” explains Markus Patzek. Breccias are debris rocks that were formed by impacts on the parent body and whose debris, i.e. fragments, were solidified again by another impact. Small areas of melting within the fine-grained debris indicate that the “Ribbeck” meteorite underwent at least one subsequent impact process, which took place after the main fragmentation events and breccia formation.

When the meteorite fragments were found, they had an intense odour of hydrogen sulphide – similar to the smell of rotten eggs. Although the individual fragments had only been exposed to the damp environment of snow and subsequent thaw for a few days, chemical reactions between the mineral phases and the moisture took place immediately after the fall, causing the odour and altering the original mineralogy of the rock. Certain mineral phases in the meteorite cannot form under terrestrial conditions and are unstable, i.e. they react with the terrestrial moisture and water and disintegrate.

 

Original publication

Bischoff, Patzek et al., 2024: Cosmic pears from the Havelland (Germany): Ribbeck, the twelfth recorded aubrite fall in history. Meteoritics & Planetary Science; DOI: 10.1111/maps.14245.

The open access provision of the article is made possible by the DEAL project of the University of Münster and Wiley.

 

Further information