The Dingle Dell meteorite: A Halloween treat from the Main Belt
dc.contributor.author | Devillepoix, Hadrien | |
dc.contributor.author | Sansom, Eleanor | |
dc.contributor.author | Bland, Phil | |
dc.contributor.author | Towner, Martin | |
dc.contributor.author | Cupák, M. | |
dc.contributor.author | Howie, Robert | |
dc.contributor.author | Jansen-Sturgeon, T. | |
dc.contributor.author | Cox, M. | |
dc.contributor.author | Hartig, Benjamin | |
dc.contributor.author | Benedix, Gretchen | |
dc.contributor.author | Paxman, Jonathan | |
dc.date.accessioned | 2018-12-13T09:16:39Z | |
dc.date.available | 2018-12-13T09:16:39Z | |
dc.date.created | 2018-12-12T02:46:37Z | |
dc.date.issued | 2018 | |
dc.identifier.citation | Devillepoix, H. and Sansom, E. and Bland, P. and Towner, M. and Cupák, M. and Howie, R. and Jansen-Sturgeon, T. et al. 2018. The Dingle Dell meteorite: A Halloween treat from the Main Belt. Meteoritics and Planetary Science. 53 (10): pp. 2212-2227. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/73472 | |
dc.identifier.doi | 10.1111/maps.13142 | |
dc.description.abstract |
We describe the fall of the Dingle Dell (L/LL 5) meteorite near Morawa in Western Australia on October 31, 2016. The fireball was observed by six observatories of the Desert Fireball Network (DFN), a continental-scale facility optimized to recover meteorites and calculate their pre-entry orbits. The 30 cm meteoroid entered at 15.44 km s-1, followed a moderately steep trajectory of 51° to the horizon from 81 km down to 19 km altitude, where the luminous flight ended at a speed of 3.2 km s-1. Deceleration data indicated one large fragment had made it to the ground. The four person search team recovered a 1.15 kg meteorite within 130 m of the predicted fall line, after 8 h of searching, 6 days after the fall. Dingle Dell is the fourth meteorite recovered by the DFN in Australia, but the first before any rain had contaminated the sample. By numerical integration over 1 Ma, we show that Dingle Dell was most likely ejected from the Main Belt by the 3:1 mean motion resonance with Jupiter, with only a marginal chance that it came from the ?6 resonance. This makes the connection of Dingle Dell to the Flora family (currently thought to be the origin of LL chondrites) unlikely. | |
dc.publisher | John Wiley & Sons, Inc. | |
dc.title | The Dingle Dell meteorite: A Halloween treat from the Main Belt | |
dc.type | Journal Article | |
dcterms.source.volume | 53 | |
dcterms.source.number | 10 | |
dcterms.source.startPage | 2212 | |
dcterms.source.endPage | 2227 | |
dcterms.source.issn | 1086-9379 | |
dcterms.source.title | Meteoritics and Planetary Science | |
curtin.department | School of Earth and Planetary Sciences (EPS) | |
curtin.accessStatus | Fulltext not available |
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