Heterogeneous cooling subsidence of oceanic lithosphere controlled by spreading rate

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Earth and Planetary Science Letters Pub Date : 2024-10-08 DOI:10.1016/j.epsl.2024.119017
Irina M. Artemieva
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Abstract

Ocean age-dependent cooling subsidence with seafloor deepening is traditionally described by models of thermo-chemical buoyancy of oceanic plates with globally constant parameters, that specify a linear correlation between square-root of seafloor age, sqrt(age), and bathymetry. Here I present a worldwide analysis of the ocean floor split into 94 segments, delineated by wide-offset transform faults and mid-ocean ridges, to demonstrate a strong heterogeneity of sediment-corrected isostatic cooling subsidence both between and within normal oceans. Anomalous oceans are identified from bathymetry deviation from age-dependent predictions during data processing. Subsidence parameters for individual ocean segments significantly deviate from global constants in conventional models and show a large variability of subsidence rate (270–535 m/Ma1/2) and zero-age depth (−1.30 to −3.03 km) with plate thickness estimated between 50 and 160 km for cooling models with constant mantle properties.
Statistically strong correlations (R2=0.80–0.94) between major characteristics of cooling subsidence and spreading rate indicate that ocean evolution is essentially controlled by spreading rate, despite this factor is not included in conventional models of ocean subsidence. Normal oceans with slower spreading rate have, statistically, higher subsidence rate which implies faster gravitational collapse caused by faster plate cooling with moderate-to-low mantle temperatures at mid-ocean ridges. Fast-spreading oceans have the opposite characteristics. The ultraslow SW Indian and the fast-spreading Central Pacific Oceans are the end-members in ocean cooling subsidence trends, with the Atlantic/NW Indian Oceans tending towards the ultraslow end, and the Pacific/SE Indian Oceans being closer to the fast-spreading end. The Arctic Ocean and the Atlantics north of the Charlie-Gibbs Fracture Zone with an atypical subsidence behavior often deviate from the global trends. Strong correlation between spreading rate, ocean half-width and the type of ocean margins implies that ridge-push dominates tectonic forces in slower-spreading, narrower oceans with passive margins, while slab-pull at active margins is a dominant tectonic force in faster-spreading oceans with half-width exceeding 4250 km.
The age of bathymetry departure from cooling subsidence, controlled by distribution of hotspots on ocean floor, correlates (R2=0.76) with spreading rate, and thus is not fully random. Slower-spreading oceans follow normal cooling subsidence to older ages (7.5–9.5 Ma1/2) than faster-spreading oceans (5–7 Ma1/2). Recognition that spreading rate controls ocean evolution with formation of active or passive ocean margins dominated by slab-pull or ridge-push contributes to advances in understanding driving forces in geodynamics.

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受扩张速率控制的海洋岩石圈异质冷却沉降
传统上,海洋随年龄变化的冷却沉降与海底加深是通过具有全球恒定参数的大洋板块热化学浮力模型来描述的,该模型规定了海底年龄平方根、sqrt(年龄)与水深之间的线性相关关系。在这里,我介绍了一项全球范围的分析,将海底分成 94 个区段,由宽偏移转换断层和大洋中脊划定,以证明正常大洋之间和内部沉积物校正等静力冷却沉降的强烈异质性。在数据处理过程中,根据水深测量与年龄相关预测的偏差确定了异常海洋。单个海段的沉降参数明显偏离常规模型中的全球常数,并显示出沉降速率(270-535 m/Ma1/2)和零年龄深度(-1.30 至-3.03 千米)的巨大变异性,在地幔属性不变的冷却模型中,板块厚度估计在 50 至 160 千米之间。据统计,扩张速度较慢的正常海洋具有较高的沉降速度,这意味着板块冷却速度较快导致重力塌陷速度加快,洋中脊地幔温度处于中低水平。快速扩张的大洋则具有相反的特征。超慢速的西南印度洋和快速扩张的中太平洋是海洋冷却下沉趋势的末端成员,大西洋/西北印度洋趋向于超慢速的一端,而太平洋/东南印度洋更接近于快速扩张的一端。北冰洋和查理-吉布斯断裂带以北的亚特兰蒂斯海域的非典型下沉行为往往偏离全球趋势。扩张速度、海洋半宽和海洋边缘类型之间的强相关性意味着,在扩张速度较慢、海洋半宽较窄且具有被动边缘的海洋中,海脊推动力是主要的构造力,而在扩张速度较快、海洋半宽超过 4250 公里的海洋中,活动边缘的板块拉力是主要的构造力。由海底热点分布控制的水深偏离冷却下沉的年龄与扩张速度相关(R2=0.76),因此并非完全随机。与扩张速度较快的海洋(5-7 Ma1/2)相比,扩张速度较慢的海洋按照正常的冷却下沉速度扩张到较老的年龄(7.5-9.5 Ma1/2)。认识到扩张速率控制海洋演化,形成以板块拉动或海岭推动为主的主动或被动洋缘,有助于进一步了解地球动力学的驱动力。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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