The Sariçiçek howardite fall in Turkey: Source crater of HED meteorites on Vesta and impact risk of Vestoids
Authors: Unsalan Ozan , Jenniskens Peter , Yin Qing‐Zhu , Kaygisiz Ersin , Albers Jim , Clark David L. , Granvik Mikael , Demirkol Iskender , Erdogan Ibrahim Y. , Bengu Aydin S. , Özel Mehmet E. , Terzioglu Zahide , Gi Nayeob , Brown Peter , Yalcinkaya Esref , Temel Tuğba , Prabhu Dinesh K. , Robertson Darrel K. , Boslough Mark , Ostrowski Daniel R. , Kimberley Jamie , Er Selman , Rowland Douglas J. , Bryson Kathryn L. , Altunayar‐Unsalan Cisem , Ranguelov Bogdan , Karamanov Alexander , Tatchev Dragomir , Kocahan Özlem , Oshtrakh Michael I. , Maksimova Alevtina A. , Karabanalov Maxim S. , Verosub Kenneth L. , Levin Emily , Uysal Ibrahim , Hoffmann Viktor , Hiroi Takahiro , Reddy Vishnu , Ildiz Gulce O. , Bolukbasi Olcay , Zolensky Michael E. , Hochleitner Rupert , Kaliwoda Melanie , Öngen Sinan , Fausto Rui , Nogueira Bernardo A. , Chukin Andrey V. , Karashanova Daniela , Semionkin Vladimir A. , Yeşiltaş Mehmet , Glotch Timothy , Yilmaz Ayberk , Friedrich Jon M. , Sanborn Matthew E. , Huyskens Magdalena , Ziegler Karen , Williams Curtis D. , Schönbächler Maria , Bauer Kerstin , Meier Matthias M. M. , Maden Colin , Busemann Henner , Welten Kees C. , Caffee Marc W. , Laubenstein Matthias , Zhou Qin , Li Qiu‐Li , Li Xian‐Hua , Liu Yu , Tang Guo‐Qiang , Sears Derek W. G. , Mclain Hannah L. , Dworkin Jason P. , Elsila Jamie E. , Glavin Daniel P. , Schmitt‐Kopplin Philippe , Ruf Alexander , Le Corre Lucille , Schmedemann Nico ,   (The Sariçiçek Meteorite Consortium)
Published: March 2019

AbstractThe Sariçiçek howardite meteorite shower consisting of 343 documented stones occurred on September 2, 2015 in Turkey and is the first documented howardite fall. Cosmogenic isotopes show that Sariçiçek experienced a complex cosmic‐ray exposure history, exposed during ~12–14 Ma in a regolith near the surface of a parent asteroid, and that an ~1 m sized meteoroid was launched by an impact 22 ± 2 Ma ago to Earth (as did one‐third of all HED meteorites). SIMS dating of zircon and baddeleyite yielded 4550.4 ± 2.5 Ma and 4553 ± 8.8 Ma crystallization ages for the basaltic magma clasts. The apatite U‐Pb age of 4525 ± 17 Ma, K‐Ar age of ~3.9 Ga, and the U,Th‐He ages of 1.8 ± 0.7 and 2.6 ± 0.3 Ga are interpreted to represent thermal metamorphic and impact‐related resetting ages, respectively. Petrographic; geochemical; and O‐, Cr‐, and Ti‐isotopic studies confirm that Sariçiçek belongs to the normal clan of HED meteorites. Petrographic observations and analysis of organic material indicate a small portion of carbonaceous chondrite material in the Sariçiçek regolith and organic contamination of the meteorite after a few days on soil. Video observations of the fall show an atmospheric entry at 17.3 ± 0.8 km s−1 from NW; fragmentations at 37, 33, 31, and 27 km altitude; and provide a pre‐atmospheric orbit that is the first dynamical link between the normal HED meteorite clan and the inner Main Belt. Spectral data indicate the similarity of Sariçiçek with the Vesta asteroid family (V‐class) spectra, a group of asteroids stretching to delivery resonances, which includes (4) Vesta. Dynamical modeling of meteoroid delivery to Earth shows that the complete disruption of a ~1 km sized Vesta family asteroid or a ~10 km sized impact crater on Vesta is required to provide sufficient meteoroids ≤4 m in size to account for the influx of meteorites from this HED clan. The 16.7 km diameter Antionia impact crater on Vesta was formed on terrain of the same age as given by the 4He retention age of Sariçiçek. Lunar scaling for crater production to crater counts of its ejecta blanket show it was formed ~22 Ma ago.