Impact origin for the Hummeln structure ...
Document type :
Article dans une revue scientifique: Article original
DOI :
Permalink :
Title :
Impact origin for the Hummeln structure (Sweden) and its link to the Ordovician disruption of the L chondrite parent body
Author(s) :
Alwmark, C. [Auteur]
Department of Geology [Lund]
Ferriere, L. [Auteur]
Natural History Museum [Vienna] [NHM]
Ormo, J. [Auteur]
Instituto Nacional de Técnica Aeroespacial [INTA]
Leroux, Hugues [Auteur]
Unité Matériaux et Transformations - UMR 8207 [UMET]
Sturkell, E. [Auteur]
Department of Earth Sciences [Gothenburg]
Department of Geology [Lund]
Ferriere, L. [Auteur]
Natural History Museum [Vienna] [NHM]
Ormo, J. [Auteur]
Instituto Nacional de Técnica Aeroespacial [INTA]
Leroux, Hugues [Auteur]
Unité Matériaux et Transformations - UMR 8207 [UMET]
Sturkell, E. [Auteur]
Department of Earth Sciences [Gothenburg]
Journal title :
Geology
Volume number :
43
Pages :
279-282
Publication date :
2015
HAL domain(s) :
Planète et Univers [physics]/Astrophysique [astro-ph]
Physique [physics]/Matière Condensée [cond-mat]/Science des matériaux [cond-mat.mtrl-sci]
Physique [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Sciences de la Terre
Chimie/Matériaux
Physique [physics]/Physique [physics]/Géophysique [physics.geo-ph]
Physique [physics]/Matière Condensée [cond-mat]/Science des matériaux [cond-mat.mtrl-sci]
Physique [physics]/Astrophysique [astro-ph]
Planète et Univers [physics]/Sciences de la Terre
Chimie/Matériaux
Physique [physics]/Physique [physics]/Géophysique [physics.geo-ph]
English abstract : [en]
Several studies of meteorites show that a large disruption of an asteroid occurred ca. 470 Ma in our solar system’s asteroid belt. As a consequence, a large number of meteorite impacts occurred on Earth during the following ...
Show more >Several studies of meteorites show that a large disruption of an asteroid occurred ca. 470 Ma in our solar system’s asteroid belt. As a consequence, a large number of meteorite impacts occurred on Earth during the following few million years. The finding and characterization, for the first time, of planar deformation features in quartz grains from rocks collected at the Middle Ordovician Hummeln structure (Sweden) prove the hypervelocity impact origin of the structure. The unambiguous shock features allow us to close an ∼200-yr-old discussion about its origin, and further the hypothesis of enhanced asteroid bombardment during the Middle Ordovician, adding an impact crater to the increasing number confirmed and properly dated from this period. Despite its relatively small size (∼1.2 km in diameter), similar to the young Meteor Crater (Arizona, USA), and its old age, the Hummeln structure is remarkably well preserved, contradicting the general assumption that small craters are not preserved on Earth for more than a few tens of thousands to a couple of million years.Show less >
Show more >Several studies of meteorites show that a large disruption of an asteroid occurred ca. 470 Ma in our solar system’s asteroid belt. As a consequence, a large number of meteorite impacts occurred on Earth during the following few million years. The finding and characterization, for the first time, of planar deformation features in quartz grains from rocks collected at the Middle Ordovician Hummeln structure (Sweden) prove the hypervelocity impact origin of the structure. The unambiguous shock features allow us to close an ∼200-yr-old discussion about its origin, and further the hypothesis of enhanced asteroid bombardment during the Middle Ordovician, adding an impact crater to the increasing number confirmed and properly dated from this period. Despite its relatively small size (∼1.2 km in diameter), similar to the young Meteor Crater (Arizona, USA), and its old age, the Hummeln structure is remarkably well preserved, contradicting the general assumption that small craters are not preserved on Earth for more than a few tens of thousands to a couple of million years.Show less >
Language :
Anglais
Peer reviewed article :
Oui
Audience :
Internationale
Popular science :
Non
Administrative institution(s) :
Université de Lille
ENSCL
CNRS
INRA
ENSCL
CNRS
INRA
Collections :
Research team(s) :
Matériaux Terrestres et Planétaires
Submission date :
2019-05-16T16:45:24Z
2021-02-16T09:12:30Z
2021-02-16T09:12:30Z