Abstract:The well-documented, well-preserved, and well-exposed Lockne crater is a reference crater for marine-target impact on Earth. To date, it has been subjected to 11 short core drillings and over 5000 outcrop descriptions, as well as several geophysical surveys. The rich data allows detailed analysis of the cratering and modification processes. A unique feature with Lockne is its pristine ejecta layer. The ejecta differs, however, from the typical text book example of a land target crater in that it, to great exte… Show more
“…The other two cores mentioned here, LOC10 and LOC11, were retrieved for this study with the use of the same type of equipment as for LOC08 and LOC09. The core log descriptions presented here are in line with the aim of the study, that is, to determine the thickness and main lithological composition of the ejecta and do, thus, not provide all additional information that would be possible to obtain from the material (e.g., Lindgren et al, 2007;Melero-Asensio et al, 2014). The LOC08 core hole was located at the center of a large solitary ejecta body that occupies the outer reach of the Tandsbyn gap.…”
Section: Core Drillingmentioning
confidence: 80%
“…Closer to the crater, remnant mud and clay are impacted by the basement crater ejecta and blend in as matrix around the clasts in a transition zone between ejecta and basement (cf. LOC9 drill core, Melero-Asensio et al, 2014. For location, see Figure 1). The Cambrian clay squeezes up between major coherent ejecta masses ("mega blocks"), and/or slumps down into the basement crater (cf.…”
Section: Discussionmentioning
confidence: 99%
“…In two instances, we use drill cores (i.e., LOC08 and LOC09) that were retrieved already in 2004 as the subject of those drillings also was to investigate the thickness and properties of the crystalline ejecta deposits. Only LOC09, however, has so far been described in publications (i.e., Lindgren et al., 2007; Melero‐Asensio et al., 2014). The other two cores mentioned here, LOC10 and LOC11, were retrieved for this study with the use of the same type of equipment as for LOC08 and LOC09.…”
Section: Methodsmentioning
confidence: 99%
“…The crystalline target within the crater damage zone shows a span from being completely brecciated to only slightly fractured. The impact breccia in the crystalline rock, the Tandsbyn Breccia, forms instantly at impact and has even been observed to have been ejected as coherent large (tens of meters) bodies of breccia (e.g., Melero‐Asensio et al., 2014). Similar bodies of Tandsbyn Breccia, albeit much smaller, are also seen as part of the resurge breccia, thus creating a “breccia in breccia” (Lindström et al., 1996).…”
Section: Geological Settingmentioning
confidence: 99%
“…The height refers to the elevation of the surfaces at the site. The result of the LOC09 drilling is given inMelero-Asensio et al (2014). The drillings were performed by the company Drillcon Core AB stationed in Nora, Sweden.…”
Except for some impact structures on low-gravity cosmic bodies, essentially all fresh impact structures are surrounded by ejecta from the crater interior (Melosh, 1989, p. 89). The geological activity on Earth does not favor the preservation of ejecta deposits. The preservation varies considerably. The best-preserved exposed ejecta deposits according to Osinski et al. (2011) are the Mauritanian Tenoumer structure (1.9 km diameter, 0.0214 Ma) and Pingualuit (New Quebec) in Canada (3.4 km diameter, 1.4 Ma). In Table 1 in Osinski et al. (2011), nine additional structures with preserved ejecta deposits are listed. Several other structures are completely buried and can only be observed with drilling and for these, the precise extent of the ejecta deposits is difficult to estimate. Also, there are ejecta deposits without a known impact structure. In this aspect, the Lockne structure offers a unique opportunity to study and explore the proximal ejecta (the ejecta blanket) around a marine target impact. The preservation of the crater and its proximal ejecta is favored by a combination of a relatively young age and large magnitude of the event (making a large impact crater), as well as that it occurred
“…The other two cores mentioned here, LOC10 and LOC11, were retrieved for this study with the use of the same type of equipment as for LOC08 and LOC09. The core log descriptions presented here are in line with the aim of the study, that is, to determine the thickness and main lithological composition of the ejecta and do, thus, not provide all additional information that would be possible to obtain from the material (e.g., Lindgren et al, 2007;Melero-Asensio et al, 2014). The LOC08 core hole was located at the center of a large solitary ejecta body that occupies the outer reach of the Tandsbyn gap.…”
Section: Core Drillingmentioning
confidence: 80%
“…Closer to the crater, remnant mud and clay are impacted by the basement crater ejecta and blend in as matrix around the clasts in a transition zone between ejecta and basement (cf. LOC9 drill core, Melero-Asensio et al, 2014. For location, see Figure 1). The Cambrian clay squeezes up between major coherent ejecta masses ("mega blocks"), and/or slumps down into the basement crater (cf.…”
Section: Discussionmentioning
confidence: 99%
“…In two instances, we use drill cores (i.e., LOC08 and LOC09) that were retrieved already in 2004 as the subject of those drillings also was to investigate the thickness and properties of the crystalline ejecta deposits. Only LOC09, however, has so far been described in publications (i.e., Lindgren et al., 2007; Melero‐Asensio et al., 2014). The other two cores mentioned here, LOC10 and LOC11, were retrieved for this study with the use of the same type of equipment as for LOC08 and LOC09.…”
Section: Methodsmentioning
confidence: 99%
“…The crystalline target within the crater damage zone shows a span from being completely brecciated to only slightly fractured. The impact breccia in the crystalline rock, the Tandsbyn Breccia, forms instantly at impact and has even been observed to have been ejected as coherent large (tens of meters) bodies of breccia (e.g., Melero‐Asensio et al., 2014). Similar bodies of Tandsbyn Breccia, albeit much smaller, are also seen as part of the resurge breccia, thus creating a “breccia in breccia” (Lindström et al., 1996).…”
Section: Geological Settingmentioning
confidence: 99%
“…The height refers to the elevation of the surfaces at the site. The result of the LOC09 drilling is given inMelero-Asensio et al (2014). The drillings were performed by the company Drillcon Core AB stationed in Nora, Sweden.…”
Except for some impact structures on low-gravity cosmic bodies, essentially all fresh impact structures are surrounded by ejecta from the crater interior (Melosh, 1989, p. 89). The geological activity on Earth does not favor the preservation of ejecta deposits. The preservation varies considerably. The best-preserved exposed ejecta deposits according to Osinski et al. (2011) are the Mauritanian Tenoumer structure (1.9 km diameter, 0.0214 Ma) and Pingualuit (New Quebec) in Canada (3.4 km diameter, 1.4 Ma). In Table 1 in Osinski et al. (2011), nine additional structures with preserved ejecta deposits are listed. Several other structures are completely buried and can only be observed with drilling and for these, the precise extent of the ejecta deposits is difficult to estimate. Also, there are ejecta deposits without a known impact structure. In this aspect, the Lockne structure offers a unique opportunity to study and explore the proximal ejecta (the ejecta blanket) around a marine target impact. The preservation of the crater and its proximal ejecta is favored by a combination of a relatively young age and large magnitude of the event (making a large impact crater), as well as that it occurred
Målingen is the 0.7 km wide minor crater associated to the 10 times larger Lockne crater in the unique Lockne–Målingen doublet. The craters formed at 458 Ma by the impact of a binary asteroid related to the well‐known 470 Ma Main Belt breakup event responsible for a large number of Ordovician craters and fossil meteorites. The binary asteroid struck a target sequence including ~500 m of sea water, ~80 m of limestone, ~30 m of dark mud, and a peneplainized Precambrian crystalline basement. Although the Lockne crater has been extensively studied by core drillings and geophysics, little is known about the subsurface morphology of Målingen. We performed magnetic susceptibility and remanence, as well as density, measurements combined with gravity, and magnetic field surveys over the crater and its close vicinity as a base for forward magnetic and gravity modeling. The interior of the crater shows a general magnetic low of 90–100 nT broken by a clustered set of high‐amplitude, short wavelength anomalies caused by bodies of mafic rock in the target below the crater and as allogenic blocks in the crater infill. The gravity shows a general −1.4 mgal anomaly over the crater caused by low‐density breccia infill and fractured crystalline rocks below the crater floor. The modeling also revealed a slightly asymmetrical shape of the crater that together with the irregular ejecta distribution supports an oblique impact from the east, which is consistent with the direction of impact suggested for the Lockne crater.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.