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The impact and recovery of asteroid 2018 LA

  • Peter Jenniskens
  • , Mohutsiwa Gabadirwe
  • , Qing Zhu Yin
  • , Alexander Proyer
  • , Oliver Moses
  • , Tomas Kohout
  • , Fulvio Franchi
  • , Roger L. Gibson
  • , Richard Kowalski
  • , Eric J. Christensen
  • , Alex R. Gibbs
  • , Aren Heinze
  • , Larry Denneau
  • , Davide Farnocchia
  • , Paul W. Chodas
  • , William Gray
  • , Marco Micheli
  • , Nick Moskovitz
  • , Christopher A. Onken
  • , Christian Wolf
  • Hadrien A.R. Devillepoix, Quanzhi Ye, Darrel K. Robertson, Peter Brown, Esko Lyytinen, Jarmo Moilanen, Jim Albers, Tim Cooper, Jelle Assink, Läslo Evers, Panu Lahtinen, Lesedi Seitshiro, Matthias Laubenstein, Nggie Wantlo, Phemo Moleje, Joseph Maritinkole, Heikki Suhonen, Michael E. Zolensky, Lewis Ashwal, Takahiro Hiroi, Derek W. Sears, Alexander Sehlke, Alessandro Maturilli, Matthew E. Sanborn, Magdalena H. Huyskens, Supratim Dey, Karen Ziegler, Henner Busemann, My E.I. Riebe, Matthias M.M. Meier, Kees C. Welten, Marc W. Caffee, Qin Zhou, Qiu Li Li, Xian Hua Li, Yu Liu, Guo Qiang Tang, Hannah L. McLain, Jason P. Dworkin, Daniel P. Glavin, Philippe Schmitt-Kopplin, Hassan Sabbah, Christine Joblin, Mikael Granvik, Babutsi Mosarwa, Koketso Botepe
  • The SETI Institute
  • NASA Ames Research Center
  • Botswana Geoscience Institute
  • University of California, Davis
  • Botswana International University of Science and Technology
  • University of Botswana
  • University of Helsinki
  • Ursa Finnish Fireball Network
  • University of the Witwatersrand, Johannesburg
  • University of Arizona
  • University of Hawaii
  • Jet Propulsion Laboratory
  • Project Pluto
  • European Space Agency (ESA)
  • Lowell Observatory
  • Australian Natl Univ
  • Curtin University
  • University of Maryland
  • California Institute of Technology
  • Western University
  • Astronomical Society of Southern Africa
  • Royal Netherlands Meteorological Institute
  • Department of Geoscience and Engineering, Faculty of Civil Engineering and Geosciences, Delft University of Technology
  • Laboratori Nazionali del Gran Sasso
  • SN4 NASA-Johnson Space Center
  • Brown University
  • Deutsches Zentrum für Luft- und Raumfahrt (DLR)
  • University of New Mexico
  • ETH Zurich
  • Naturmuseum St. Gallen
  • Space Sciences Laboratory at UC Berkeley
  • Purdue University
  • National Astronomical Observatories Chinese Academy of Sciences
  • Chinese Academy of Sciences
  • Catholic University of America
  • NASA Goddard Space Flight Center
  • Helmholtz Zentrum München German Research Center for Environmental Health
  • UPS)
  • Luleå University of Technology
  • Botswana National Museum

Research output: Contribution to journalArticlepeer-review

48 Scopus citations

Abstract

The June 2, 2018 impact of asteroid 2018 LA over Botswana is only the second asteroid detected in space prior to impacting over land. Here, we report on the successful recovery of meteorites. Additional astrometric data refine the approach orbit and define the spin period and shape of the asteroid. Video observations of the fireball constrain the asteroid's position in its orbit and were used to triangulate the location of the fireball's main flare over the Central Kalahari Game Reserve. Twenty-three meteorites were recovered. A consortium study of eight of these classifies Motopi Pan as an HED polymict breccia derived from howardite, cumulate and basaltic eucrite, and diogenite lithologies. Before impact, 2018 LA was a solid rock of ~156 cm diameter with high bulk density ~2.85 g cm−3, a relatively low albedo pV ~ 0.25, no significant opposition effect on the asteroid brightness, and an impact kinetic energy of ~0.2 kt. The orbit of 2018 LA is consistent with an origin at Vesta (or its Vestoids) and delivery into an Earth-impacting orbit via the ν6 resonance. The impact that ejected 2018 LA in an orbit toward Earth occurred 22.8 ± 3.8 Ma ago. Zircons record a concordant U-Pb age of 4563 ± 11 Ma and a consistent 207Pb/206Pb age of 4563 ± 6 Ma. A much younger Pb-Pb phosphate resetting age of 4234 ± 41 Ma was found. From this impact chronology, we discuss what is the possible source crater of Motopi Pan and the age of Vesta's Veneneia impact basin.

Original languageEnglish
Pages (from-to)844-893
Number of pages50
JournalMeteoritics and Planetary Science
Volume56
Issue number4
DOIs
StatePublished - Apr 2021

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