Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
6430093 | Earth and Planetary Science Letters | 2013 | 12 Pages |
â¢Studying Precambrian impact spherules can elucidate Earthʼs early impact history.â¢A Late Archaean impact formed unique spherules in Western Australia and South Africa.â¢These Paraburdoo and Reivilo spherules show remarkable textural preservation.â¢Ni-rich spinels and exceptionally high contents of meteoritic material are present.â¢Meteoritic component carrier phases (likely metallic alloys) can be traced.
Deciphering Earthʼs impact history before â¼2 Ga relies heavily on the lunar record and terrestrial spherule layers, which are distal ejecta from large impacts. This study focuses on the Paraburdoo and Reivilo spherule layers in Western Australia and South Africa respectively, that were probably formed by one impact around 2.57 Ga. Both layers contain an aggregate thickness of â¼2 cm of spherules, known as microkrystites. These spherules are up to â¼0.6 mm in diameter and crystallized during flight, but were diagenetically replaced by K-feldspar and phlogopite with remarkable textural retention. Unlike any other Archaean layer, except for the 3.2 Ga S3 layer in the Barberton greenstone belt, the Paraburdoo and Reivilo spherules contain Ni-rich spinel crystals and high concentrations of meteoritic material (up to 357 ng gâ1 Ir for bulk samples of several gram). These exceptional characteristics shed new light on the distribution of the meteoritic component carrier phases (metallic alloys dispersed in the pristine glass) and the processes involved in impact spherule formation and secondary alteration.