Three-dimensional magnetic stripes require slow cooling in fast-spread lower ocean crust

Sarah M. Maher (), Jeffrey S. Gee, Michael J. Cheadle and Barbara E. John
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Sarah M. Maher: University of California, San Diego
Jeffrey S. Gee: University of California, San Diego
Michael J. Cheadle: University of Wyoming
Barbara E. John: University of Wyoming

Nature, 2021, vol. 597, issue 7877, 511-515

Abstract: Abstract Earth’s magnetic field is recorded as oceanic crust cools, generating lineated magnetic anomalies that provide the pattern of polarity reversals for the past 160 million years1. In the lower (gabbroic) crust, polarity interval boundaries are proxies for isotherms that constrain cooling and hence crustal accretion. Seismic observations2–4, geospeedometry5–7 and thermal modelling8–10 of fast-spread crust yield conflicting interpretations of where and how heat is lost near the ridge, a sensitive indicator of processes of melt transport and crystallization within the crust. Here we show that the magnetic structure of magmatically robust fast-spread crust requires that crustal temperatures near the dike–gabbro transition remain at approximately 500 degrees Celsius for 0.1 million years. Near-bottom magnetization solutions over two areas, separated by approximately 8 kilometres, highlight subhorizontal polarity boundaries within 200 metres of the dike–gabbro transition that extend 7–8 kilometres off-axis. Oriented samples with multiple polarity components provide direct confirmation of a corresponding horizontal polarity boundary across an area approximately one kilometre wide, and indicate slow cooling over three polarity intervals. Our results are incompatible with deep hydrothermal cooling within a few kilometres of the axis2,7 and instead suggest a broad, hot axial zone that extends roughly 8 kilometres off-axis in magmatically robust fast-spread ocean crust.

Date: 2021
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DOI: 10.1038/s41586-021-03831-6

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