| Literature DB >> 34295141 |
Peter Jenniskens1,2, Mohutsiwa Gabadirwe3, Qing-Zhu Yin4, Alexander Proyer5, Oliver Moses6, Tomas Kohout7,8, Fulvio Franchi5, Roger L Gibson9, Richard Kowalski10, Eric J Christensen10, Alex R Gibbs10, Aren Heinze11, Larry Denneau11, Davide Farnocchia12, Paul W Chodas12, William Gray13, Marco Micheli14, Nick Moskovitz15, Christopher A Onken16, Christian Wolf16, Hadrien A R Devillepoix17, Quanzhi Ye18,19, Darrel K Robertson20, Peter Brown21, Esko Lyytinen8, Jarmo Moilanen8, Jim Albers1, Tim Cooper22, Jelle Assink23, Läslo Evers23,24, Panu Lahtinen8, Lesedi Seitshiro5, Matthias Laubenstein25, Nggie Wantlo3, Phemo Moleje3, Joseph Maritinkole3, Heikki Suhonen26, Michael E Zolensky27, Lewis Ashwal9, Takahiro Hiroi28, Derek W Sears29, Alexander Sehlke29, Alessandro Maturilli30, Matthew E Sanborn4, Magdalena H Huyskens4, Supratim Dey4, Karen Ziegler31, Henner Busemann32, My E I Riebe32, Matthias M M Meier33, Kees C Welten34, Marc W Caffee35, Qin Zhou36, Qiu-Li Li36, Xian-Hua Li37, Yu Liu37, Guo-Qiang Tang37, Hannah L McLain38,39, Jason P Dworkin39, Daniel P Glavin39, Philippe Schmitt-Kopplin40,41, Hassan Sabbah42, Christine Joblin43, Mikael Granvik26,44, Babutsi Mosarwa43, Koketso Botepe3.
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. 23 meteorites were recovered. A consortium study of eight of these classifies Motopi Pan as a 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/cm3, 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 v6 resonance. The impact that ejected 2018 LA in an orbit towards 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.Entities:
Keywords: Asteroid 2018 LA; Howardites; Motopi Pan; Vesta
Year: 2021 PMID: 34295141 PMCID: PMC7611328 DOI: 10.1111/maps.13653
Source DB: PubMed Journal: Meteorit Planet Sci ISSN: 1086-9379 Impact factor: 2.487