New Early Jurassic paleomagnetic age based on paleomagnetic and diagenetic study of the Kentland impact structure, Indiana

IF 3.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Meteoritics & Planetary Science Pub Date : 2026-07-12 Epub Date: 2026-05-11 DOI:10.1111/maps.70139
Christina Hamilton, Shannon Dulin, John Weber, R. Douglas Elmore
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Abstract

A paleomagnetic and petrographic study of host carbonate rocks and impact breccias at the Kentland impact structure was conducted to better constrain the timing of the impact and to test for alteration by hydrothermal fluids. The Ordovician-Silurian target rocks sampled are fossiliferous wackestone/packstones with minor dolomite. Polymict impact breccias, also sampled, occur as dikes/sills and contain clasts of dolomite, host carbonate, sandstone, sphalerite, and rare coated grains which contain clays, dolomite, calcite, and hexagonal silica resembling tridymite. The host carbonates contain brecciated zones near the polymict breccias that display flow textures of aligned and elongated clasts and minerals. Authigenic minerals present include sylvite, apatite, gypsum, magnetite, and hematite. These observations suggest alteration by hydrothermal fluids, which probably had an estimated duration of ~7500 yrs after impact. Alternating field (AF) and thermal demagnetization of impact breccia and host carbonate specimens removed two post-tilting magnetic components: one with southerly declinations and moderate negative inclinations and the other with northerly declinations and positive inclinations. Demagnetization results suggest the magnetizations primarily reside in magnetite as well as hematite and possibly pyrrhotite. Petrographic and rock magnetic results are consistent with this interpretation. These magnetizations are interpreted as chemical remanent magnetizations acquired through a reversal, which formed from alteration by hydrothermal fluids generated after the impact. The paleomagnetic poles (mean pole, 75.7° N, 98.4° W) fall near the Early Jurassic part of the apparent polar wander path, which suggests the alteration in the breccias, and likely the impact, occurred in the Early Jurassic (175–185 Ma).

基于肯特兰撞击构造古地磁和成岩研究的早侏罗世新古地磁年龄
通过对Kentland撞击构造中寄主碳酸盐岩和撞击角砾岩的古地磁和岩石学研究,更好地确定了撞击时间,并测试了热液流体的蚀变作用。取样的奥陶系—志留系靶岩为含少量白云岩的石化尾岩/包岩。多晶冲击角砾岩,也被取样,以岩脉/岩壁的形式出现,含有白云岩、寄主碳酸盐、砂岩、闪锌矿的碎屑,以及含有粘土、白云岩、方解石和六方硅石的稀有包覆颗粒。寄主碳酸盐岩在多晶角砾岩附近含有角砾岩带,显示出排列和拉长的碎屑和矿物的流动结构。自生矿物包括钾盐、磷灰石、石膏、磁铁矿和赤铁矿。这些观测结果表明,热液流体的改变可能在撞击后持续了约7500年。对撞击角砾岩和寄主碳酸盐样品进行交变磁场(AF)和热消磁,消除了两种倾斜后的磁性成分:一种是偏南纬和中等负倾角,另一种是偏北纬和正倾角。退磁结果表明,磁化主要存在于磁铁矿、赤铁矿和磁黄铁矿中。岩石学和岩石磁学结果与这一解释一致。这些磁化被解释为通过反转获得的化学残余磁化,这是由撞击后产生的热液流体的蚀变形成的。古地磁极(平均极75.7°N, 98.4°W)落在明显极移路径的早侏罗世附近,表明角砾岩的蚀变可能发生在早侏罗世(175 ~ 185 Ma)。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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