The Sariçiçek Howardite Fall in Turkey: Source Crater of HED Meteorites on Vesta and Impact Risk of Vestoids

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...

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Published inMeteoritics & planetary science Vol. 54; no. 5; pp. 953 - 1008
Main 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., Ozel, Mehmet E., Terzioglu, Zahide, Gi, Nayeob, Brown, Peter, Yalcinkaya, Esref, Temel, Tu_Gba, 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, Ozlem, 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, Ongen, Sinan, Fausto, Rui, Nogueira, Bernardo A., Chukin, Andrey V., Karashanova, Daniela, Semionkin, Vladimir A., Yes_Iltas, Mehmet, Glotch, Timothy, Yilmaz, Ayberk, Friedrich, Jon M., Sanborn, Matthew E., Huyskens, Magdalena, Ziegler, Karen, Williams, Curtis D., Schonbachler, 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, Corre, Lucille Le, Schmedemann, Nico
Format Journal Article
LanguageEnglish
Published Goddard Space Flight Center Wiley 01.05.2019
Wiley Subscription Services, Inc
Subjects
Age
Apatite
Asteroids
Atmospheric entry
Atmospheric models
Carbonaceous chondrites
Contamination
Craters
Crystallization
Disruption
Ejecta
Isotopes
Magma
Meteorites
Meteoroids
Meteors & meteorites
Onboard Space Systems
Orbital resonances (celestial mechanics)
Radiometric dating
Regolith
Rymdtekniska system
Soil contamination
Space Sciences (General)
Vesta asteroid
Zircon
Turkey
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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 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 blanketshow it was formed ~22 Ma ago.
AbstractList 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 4 He retention age of Sariçiçek. Lunar scaling for crater production to crater counts of its ejecta blanket show it was formed ~22 Ma ago.
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 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 blanketshow it was formed ~22 Ma ago.
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.
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 4 He retention age of Sariçiçek. Lunar scaling for crater production to crater counts of its ejecta blanket show it was formed ~22 Ma ago.
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.
Audience PUBLIC
Author Maden, Colin
Glavin, Daniel P.
Temel, Tu_Gba
Karabanalov, Maxim S.
Er, Selman
Maksimova, Alevtina A.
Semionkin, Vladimir A.
Laubenstein, Matthias
Levin, Emily
Caffee, Marc W.
Hochleitner, Rupert
Welten, Kees C.
Kocahan, Ozlem
Tang, Guo- Qiang
Elsila, Jamie E.
Ozel, Mehmet E.
Schonbachler, Maria
Mclain, Hannah L.
Terzioglu, Zahide
Rowland, Douglas J.
Karamanov, Alexander
Schmedemann, Nico
Albers, Jim
Prabhu, Dinesh K.
Demirkol, Iskender
Bryson, Kathryn L.
Liu, Yu
Hiroi, Takahiro
Ziegler, Karen
Meier, Matthias M. M.
Nogueira, Bernardo A.
Kaygisiz, Ersin
Li, Qiu-Li
Erdogan, Ibrahim Y.
Yes_Iltas, Mehmet
Ildiz, Gulce O.
Ongen, Sinan
Chukin, Andrey V.
Dworkin, Jason P.
Ruf, Alexander
Tatchev, Dragomir
Gi, Nayeob
Robertson, Darrel K.
Karashanova, Daniela
Jenniskens, Peter
Yin, Qing-Zhu
Busemann, Henner
Schmitt-Kopplin, Philippe
Friedrich, Jon M.
Sears, Derek W. G.
Sanborn, Matthew E.
Kaliwoda, Melanie
Reddy, Vishnu
Corre, Lucille Le
Altunayar-Unsalan, Cisem
Ranguelov, Bogdan
Uysal, Ibrahim
Granvik, Mikael
Unsalan, Ozan
Glotch, Timothy
Li, Xian-Hua
Baue
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  organization: İstanbul Üniversitesi
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  organization: İstanbul Üniversitesi
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  organization: California Univ
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  givenname: Kathryn L.
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  organization: NASA Ames Research Center
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  givenname: Cisem
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  organization: Ege Üniversitesi
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  givenname: Bogdan
  surname: Ranguelov
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  organization: Bulgarian Academy of Sciences
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  givenname: Alexander
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  organization: Bulgarian Academy of Sciences
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  givenname: Dragomir
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  organization: Bulgarian Academy of Sciences
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  givenname: Ozlem
  surname: Kocahan
  fullname: Kocahan, Ozlem
  organization: Tekirdağ Namık Kemal Üniversitesi
– sequence: 30
  givenname: Michael I.
  surname: Oshtrakh
  fullname: Oshtrakh, Michael I.
  organization: URALKABEL
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  givenname: Alevtina A.
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  organization: URALKABEL
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  givenname: Kenneth L.
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  givenname: Emily
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  fullname: Levin, Emily
  organization: California Univ
– sequence: 35
  givenname: Ibrahim
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  organization: Ludwig-Maximilians-Universität München
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  surname: Hiroi
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  organization: Brown Univ
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  organization: Planetary Science Inst
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  organization: Istanbul Kültür University
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  organization: İstanbul Üniversitesi
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  surname: Chukin
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  givenname: Mehmet
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– sequence: 51
  givenname: Timothy
  surname: Glotch
  fullname: Glotch, Timothy
  organization: Stony Brook Univ
– sequence: 52
  givenname: Ayberk
  surname: Yilmaz
  fullname: Yilmaz, Ayberk
  organization: İstanbul Üniversitesi
– sequence: 53
  givenname: Jon M.
  surname: Friedrich
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  organization: Fordham Univ
– sequence: 54
  givenname: Matthew E.
  surname: Sanborn
  fullname: Sanborn, Matthew E.
  organization: California Univ
– sequence: 55
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  organization: California Univ
– sequence: 56
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  fullname: Ziegler, Karen
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– sequence: 57
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  fullname: Williams, Curtis D.
  organization: California Univ
– sequence: 58
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  givenname: Kees C.
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  organization: California Univ
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  surname: Caffee
  fullname: Caffee, Marc W.
  organization: Purdue Univ
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  givenname: Matthias
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– sequence: 66
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  organization: Chinese Academy of Sciences
– sequence: 67
  givenname: Qiu-Li
  surname: Li
  fullname: Li, Qiu-Li
  organization: Chinese Academy of Sciences
– sequence: 68
  givenname: Xian-Hua
  surname: Li
  fullname: Li, Xian-Hua
  organization: Chinese Academy of Sciences
– sequence: 69
  givenname: Yu
  surname: Liu
  fullname: Liu, Yu
  organization: Chinese Academy of Sciences
– sequence: 70
  givenname: Guo- Qiang
  surname: Tang
  fullname: Tang, Guo- Qiang
  organization: Chinese Academy of Sciences
– sequence: 71
  givenname: Derek W. G.
  surname: Sears
  fullname: Sears, Derek W. G.
  organization: Bay Area Environmental Research Inst
– sequence: 72
  givenname: Hannah L.
  surname: Mclain
  fullname: Mclain, Hannah L.
  organization: Catholic Univ. of America
– sequence: 73
  givenname: Jason P.
  surname: Dworkin
  fullname: Dworkin, Jason P.
  organization: NASA Goddard Space Flight Center
– sequence: 74
  givenname: Jamie E.
  surname: Elsila
  fullname: Elsila, Jamie E.
  organization: NASA Goddard Space Flight Center
– sequence: 75
  givenname: Daniel P.
  surname: Glavin
  fullname: Glavin, Daniel P.
  organization: NASA Goddard Space Flight Center
– sequence: 76
  givenname: Philippe
  surname: Schmitt-Kopplin
  fullname: Schmitt-Kopplin, Philippe
  organization: Helmholtz Zentrum Munchen
– sequence: 77
  givenname: Alexander
  surname: Ruf
  fullname: Ruf, Alexander
  organization: Helmholtz Zentrum Munchen
– sequence: 78
  givenname: Lucille Le
  surname: Corre
  fullname: Corre, Lucille Le
  organization: Planetary Science Inst
– sequence: 79
  givenname: Nico
  surname: Schmedemann
  fullname: Schmedemann, Nico
  organization: Freie Universität Berlin
BackLink https://urn.kb.se/resolve?urn=urn:nbn:se:ltu:diva-73497$$DView record from Swedish Publication Index
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Correction added on 29 April, 2019, after first online publication: author list had Lucille's last name partially capitalized: it is “Le Corre”, not “LE Corre”
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Snippet The Sariçiçek howardite meteorite shower consisting of 343 documented stones occurred on September 2, 2015 in Turkey and is the first documented howardite...
Abstract The Sariçiçek howardite meteorite shower consisting of 343 documented stones occurred on September 2, 2015 in Turkey and is the first documented...
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StartPage 953
SubjectTerms Age
Apatite
Asteroids
Atmospheric entry
Atmospheric models
Carbonaceous chondrites
Contamination
Craters
Crystallization
Disruption
Ejecta
Isotopes
Magma
Meteorites
Meteoroids
Meteors & meteorites
Onboard Space Systems
Orbital resonances (celestial mechanics)
Radiometric dating
Regolith
Rymdtekniska system
Soil contamination
Space Sciences (General)
Vesta asteroid
Zircon
Title The Sariçiçek Howardite Fall in Turkey: Source Crater of HED Meteorites on Vesta and Impact Risk of Vestoids
URI https://ntrs.nasa.gov/citations/20190002383
https://onlinelibrary.wiley.com/doi/abs/10.1111%2Fmaps.13258
https://www.proquest.com/docview/2210806374/abstract/
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Volume 54
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