TY - JOUR
T1 - Origin of a late Eocene to pre-Miocene buried crater and breccia lens at Fohn-1, North Bonaparte basin, Timor Sea
T2 - A probable extraterrestrial connection
AU - Gorter, John D.
AU - Glikson, Andrew Y.
PY - 2000/3
Y1 - 2000/3
N2 - Seismic reflection data and an at least 350 m thick, PGE-rich carbonate breccia lens intersected by the Fohn-1 exploration well in the Timor Sea off northern Australia, are interpreted in terms of a buried 4.8 km-diameter impact crater of late Eocene to pre-Miocene age. The crater displays the classic elements of impact structures, including a central uplift, ring syncline, and upraised rims. The presence in the breccia of redeposited Campanian and Maastrichtian microfossils suggests rebound of strata from levels deeper than 1250 m below the pre-Miocene unconformity. Morphometric modelling suggests an original crater at least 1400 m deep, which is consistent with the excavation of Cretaceous strata. Stratigraphic and palaeontological evidence suggests that the impact occurred between 36 and 24.6 Ma. The breccia contains a pseudotachylite component enriched in the inert Pt group elements (PGE) (Ir, Ru) by factors of 5-12 above the values of common sediments. The more mobile PGE (Os, Pt, Pd) show a wide scatter and terrestrial-type values. Opposite geochemical/stratigraphic trends pertain to different PGE species-the relatively inert Ir-Ru group shows an overall concentration at the base of the section, whereas the more mobile Os shows peaks at median levels of the section-suggesting upward diagenetic leaching. The near-chondritic PGE patterns at the base of the breccia pile are accompanied by near-chondritic Ni/Cr, Co/Cr, Ni/Ir, Ni/Pt, and Cu/Pd ratios. Departure from these values related to alteration at higher levels in the breccia pile is accompanied with high S levels (~1%).
AB - Seismic reflection data and an at least 350 m thick, PGE-rich carbonate breccia lens intersected by the Fohn-1 exploration well in the Timor Sea off northern Australia, are interpreted in terms of a buried 4.8 km-diameter impact crater of late Eocene to pre-Miocene age. The crater displays the classic elements of impact structures, including a central uplift, ring syncline, and upraised rims. The presence in the breccia of redeposited Campanian and Maastrichtian microfossils suggests rebound of strata from levels deeper than 1250 m below the pre-Miocene unconformity. Morphometric modelling suggests an original crater at least 1400 m deep, which is consistent with the excavation of Cretaceous strata. Stratigraphic and palaeontological evidence suggests that the impact occurred between 36 and 24.6 Ma. The breccia contains a pseudotachylite component enriched in the inert Pt group elements (PGE) (Ir, Ru) by factors of 5-12 above the values of common sediments. The more mobile PGE (Os, Pt, Pd) show a wide scatter and terrestrial-type values. Opposite geochemical/stratigraphic trends pertain to different PGE species-the relatively inert Ir-Ru group shows an overall concentration at the base of the section, whereas the more mobile Os shows peaks at median levels of the section-suggesting upward diagenetic leaching. The near-chondritic PGE patterns at the base of the breccia pile are accompanied by near-chondritic Ni/Cr, Co/Cr, Ni/Ir, Ni/Pt, and Cu/Pd ratios. Departure from these values related to alteration at higher levels in the breccia pile is accompanied with high S levels (~1%).
UR - http://www.scopus.com/inward/record.url?scp=0034162989&partnerID=8YFLogxK
U2 - 10.1111/j.1945-5100.2000.tb01784.x
DO - 10.1111/j.1945-5100.2000.tb01784.x
M3 - Article
SN - 1086-9379
VL - 35
SP - 381
EP - 392
JO - Meteoritics and Planetary Science
JF - Meteoritics and Planetary Science
IS - 2
ER -