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  The Sariçiçek howardite fall in Turkey: Source crater of HED meteorites on Vesta and impact risk of Vestoids

Unsalan, O., Jenniskens, P., Yin, Q., Kaygisiz, E., Albers, J., Clark, D. L., et al. (2019). The Sariçiçek howardite fall in Turkey: Source crater of HED meteorites on Vesta and impact risk of Vestoids. Meteoritics and Planetary Science, 54(5), 953-1008. doi:10.1111/maps.13258.

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Other : The Saricicek howardite fall in Turkey: Source crater of HED meteorites on Vesta and impact risk of Vestoids


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Unsalan, Ozan, Author
Jenniskens, Peter, Author
Yin, Qing‐Zhu, Author
Kaygisiz, Ersin, Author
Albers, Jim, Author
Clark, David L., Author
Granvik, Mikael, Author
Demirkol, Iskender, Author
Erdogan, Ibrahim Y., Author
Bengu, Aydin S., Author
Özel, Mehmet E., Author
Terzioglu, Zahide, Author
Gi, Nayeob, Author
Brown, Peter, Author
Yalcinkaya, Esref, Author
Temel, Tuğba, Author
Prabhu, Dinesh K., Author
Robertson, Darrel K., Author
Boslough, Mark, Author
Ostrowski, Daniel R., Author
Kimberley, Jamie, AuthorEr, Selman, AuthorRowland, Douglas J., AuthorBryson, Kathryn L., AuthorAltunayar‐Unsalan, Cisem, AuthorRanguelov, Bogdan, AuthorKaramanov, Alexander, AuthorTatchev, Dragomir, AuthorKocahan, Özlem, AuthorOshtrakh, Michael I., AuthorMaksimova, Alevtina A., AuthorKarabanalov, Maxim S., AuthorVerosub, Kenneth L., AuthorLevin, Emily, AuthorUysal, Ibrahim, AuthorHoffmann, Viktor, AuthorHiroi, Takahiro, AuthorReddy, Vishnu, AuthorIldiz, Gulce O., AuthorBolukbasi, Olcay, AuthorZolensky, Michael E., AuthorHochleitner, Rupert, AuthorKaliwoda, Melanie, AuthorÖngen, Sinan, AuthorFausto, Rui, AuthorNogueira, Bernardo A., AuthorChukin, Andrey V., AuthorKarashanova, Daniela, AuthorSemionkin, Vladimir A., AuthorYeşiltaş, Mehmet, AuthorGlotch, Timothy, AuthorYilmaz, Ayberk, AuthorFriedrich, Jon M., AuthorSanborn, Matthew E., AuthorHuyskens, Magdalena, AuthorZiegler, Karen, AuthorWilliams, Curtis D., AuthorSchönbächler, Maria, AuthorBauer, Kerstin, AuthorMeier, Matthias M. M., AuthorMaden, Colin, AuthorBusemann, Henner, AuthorWelten, Kees C., AuthorCaffee, Marc W., AuthorLaubenstein, Matthias, AuthorZhou, Qin, AuthorLi, Qiu‐Li, AuthorLi, Xian‐Hua, AuthorLiu, Yu, AuthorTang, Guo‐Qiang, AuthorSears, Derek W. G., AuthorMclain, Hannah L., AuthorDworkin, Jason P., AuthorElsila, Jamie E., AuthorGlavin, Daniel P., AuthorSchmitt‐Kopplin, Philippe, AuthorRuf, Alexander, AuthorLe Corre, Lucille, AuthorSchmedemann, Nico1, Author              The Sariçiçek Meteorite Consortium, Author               more..
1Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              


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 Abstract: The 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.


Language(s): eng - English
 Dates: 2019
 Publication Status: Published in print
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1111/maps.13258
 Degree: -



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Title: Meteoritics and Planetary Science
Source Genre: Journal
Publ. Info: Fayetteville, AR : Meteoritical Society at the University of Arkansas, Dept. of Chemistry and Biochemistry
Pages: - Volume / Issue: 54 (5) Sequence Number: - Start / End Page: 953 - 1008 Identifier: ISSN: 1086-9379
CoNE: https://pure.mpg.de/cone/journals/resource/954925424162