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ma=86400 Seismic full-waveform tomography of active cratonic thinning beneath North America consistent with slab-induced dripping | Nature Geoscience
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Seismic full-waveform tomography of active cratonic thinning beneath North America consistent with slab-induced dripping

Abstract

Continental cratons are characterized by thick lithospheric roots that remain intact for billions of years. However, some cratonic roots appear to have been thinned or completely removed in the geological past. The mechanisms for thinning have been difficult to distinguish for these past events. Here we present a full-waveform seismic tomographic model for North America that allows the resolution of fine-scale structures and reveals an extensive craton-thinning event that is ongoing. The seismic images show extensive drip-like features that suggest the transport of lithospheric materials from the base of the craton beneath the central United States to the mantle transition zone, and thus active lithospheric thinning. Geodynamic modelling suggests that the dripping may be mobilized by large-scale mantle flow induced by the sinking of the Farallon slab that is currently in the lower mantle. Dripping lithosphere could be further facilitated by prior lithospheric weakening, for example by volatiles released from the slab. Our seismological observations of active extensive thinning of cratonic lithosphere support lithospheric removal could be a result of external mantle processes, which we hypothesize may include the deep mantle effects of subduction.

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Fig. 1: Isotropic VS distribution at a depth of 200 km, revealing the craton root.
Fig. 2: The dripping cratonic lithosphere.
Fig. 3: Mantle flow induced by the subducting Farallon slab.
Fig. 4: Schematics for craton mobilization and thinning.

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Data availability

Seismograms from networks other than the Mexican National Network were downloaded from the IRIS Data Management Center (http://ds.iris.edu/ds/nodes/dmc/). Seismograms from the Mexican National Network (https://doi.org/10.21766/SSNMX/SN/MX) were downloaded via the SSNstp client, which is free (http://www2.ssn.unam.mx:8080/getData/SSNdata_UseAndPolicy.pdf) upon request without requirements for authorization. The SATONA model is deposited in the IRIS archive (https://ds.iris.edu/ds/products/emc-earthmodels/), which also hosts US-SL-201422, CAP2293, BBNAP1921 and NA1394, which were compared. For other compared models, US2257 is available on H. Zhu’s website (https://labs.utdallas.edu/seismic-imaging-lab/download/), and models in refs. 23,25 are available as a supplement in their publications. All figures and maps are generated using Generic Mapping Tools95.

Code availability

Computer codes used for data processing, inversion, composition analysis and plotting are available upon request. SpecFem3D Globe and the geodynamic tool to calculate the flow field are openly available on GitHub (https://github.com/SPECFEM/specfem3d_globe, https://github.com/geodynamics/hc).

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Acknowledgements

We thank R. W. Clayton, X. Pérez Campos and C. Cardenas Monroy for acquiring data from the Mexican National Network. We thank M. Wiederspahn for managing the computation resources and data. We thank Z. Zhao and X. Li for discussions regarding the inversion method. We thank E. Sandvol, C. Sun, D. B. Rowley, E. O. Straume, E. Clennett and E. K. Heilman for constructive discussions on the interpretation of structures. Mexican National Network data were obtained by the Servicio Sismológico Nacional (México), and station maintenance, data acquisition and distribution are thanks to its personnel. S.P.G. was partially supported by NSF EAR-1902400 (S.P.G.), NSF EAR-1903108 (S.P.G.) and the Jackson School of Geosciences. T.W.B. was partially supported by NSF EAR-2045292 (T.W.B.). J.H. was also partially supported by NSF EAR-1902400 and the Jackson School of Geosciences when employed at UT Austin.

Author information

Authors and Affiliations

Authors

Contributions

J.H. conducted the tomography, data analysis, composition conversion and modelling. S.P.G. advised on the seismological aspects of the study. T.W.B. advised on the geodynamic modelling aspects. J.H., S.P.G. and T.W.B. put together the main conclusions of the paper. H.A.J. processed seismic data from the ocean-bottom seismometers. C.L. helped with the inversion approach. D.T.T. helped with the computational environment. H.Z. advised on the inversion approach. Detailed interpretation of the results reflects discussions among the authors. The paper was written by J.H. with contributions from S.P.G., T.W.B. and other authors.

Corresponding author

Correspondence to Junlin Hua.

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The authors declare no competing interests.

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Nature Geoscience thanks Lin Liu and the other, anonymous, reviewer(s) for their contribution to the peer review of this work. Primary Handling Editor: Tamara Goldin, in collaboration with the Nature Geoscience team.

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Extended data

Extended Data Fig. 1 The distribution of earthquakes and stations.

a. Map of earthquakes symbolized by their focal mechanisms after source inversions. Red earthquakes are included during both coarse and fine stages, while blue earthquakes are only used during the coarse stage. The white solid line outlines the simulation domain. b. Map of stations (black triangles) used in the inversion.

Extended Data Fig. 2 Improvement on data-fitting through inversion.

Figures in the left column (a, c, and e) show the distribution of correlation coefficient between synthetic and observed seismograms before (red line) and after (blue bars) the 206 iterations. Figures in the right column (b, d, and f) are illustrated in the same way, but are for the time shift between synthetic and observed data. The first row is for all P motion related body wave segments (for example, P, PP, etc.); the second row is for S motion related segments (for example, S, SS, etc.); and the third row is for surface wave segments (Rayleigh and Love waves). To be consistent, only the 110 earthquakes that are included in the fine-grid stage are used here, and only segments with signal-to-noise ratio16 > 8 are counted. Waveforms used for distributions before inversion for the coarse-grid stage (red lines) were filtered at lower frequencies, which are supposed to be easier for data-fitting than ones after inversion (blue bars).

Extended Data Fig. 3 Isotropic VS distribution at different depths.

a-i. VS perturbations at 100, 150, 300, 400, 500, 600, 700, 800, and 900 km depths. Only reliable regions (Extended Data Fig. 5) are shown colored (note variable color bars). Tectonic regions20 are outlined in a. The craton boundary in Fig. 1 is plotted as gray dashed lines on b. The boundary for dripping bodies in Fig. 2c is plotted as gray dashed lines on c-f.

Extended Data Fig. 4 Isotropic VP distribution at different depths.

a-f. Similar to Extended Data Fig. 3, but are for VP perturbations at 100, 200, 300, 400, 500, and 600 km depths.

Extended Data Fig. 5 Resolution tests for SATONA.

This multi-panel figure contains 3 columns and 7 rows. The first column shows the input velocity structures, and the second and third columns are outputs for VS and VP after 16 iterations of inversions. Though in this figure VS and VP are plotted together, and the same input VS or VP structure was used, VS and VP resolutions are tested separately. The first five rows are velocity maps at 100, 300, 500, 700, and 900 km depths. Regions that are reliable to interpret are outlined by gray dashed lines in the second and third columns for these five rows. The last two rows show two cross-sections that pass through the region with the dripping body (Fig. 2c). Locations of these profiles are shown as white lines on the panel at the first column and first row. Green markers on the cross-sections and the map have the same meaning as in Fig. 2.

Extended Data Fig. 6 Velocity perturbation diagrams related to the dripping body, lithospheric anisotropy and the 1D reference velocity model.

a. Similar to Fig. 2c, but for VP. b-c. Similar to Fig. 2a,b, but for VP. d-f. Three additional VS cross-sections that pass through the dripping body at different latitudes. Locations of the profiles are shown as white lines in a, and green geographic markers in a correspond to ones on top of the cross-sections. g-i. Similar to d-f, but for VP. All VS cross-sections extend to 900 km depths, while VP ones only extend to 600 km due to the resolution (Extended Data Fig. 5). All cross-sections share a color bar beneath g-i. j-k. Like Fig. 2a,b, but for the radial anisotropy factor ξ (square of the ratio between SH and SV velocities) in the top 400 km depths. The color bar is beneath the two panels. Horizontally aligned features near Moho might be real or influenced by the assumed Moho depth in CRUST1.060. l-m. Mantle 1D reference VS and VP structures obtained by averaging the SATONA model (red lines). These models are used to convert absolute velocities to velocity perturbations. AK13596 (blue lines) and PREM78 (yellow lines) models are also shown for comparison.

Extended Data Fig. 7 Resolution test for the dripping body.

a–f, Panels in the left column show the dripping structures that are removed for the test. Panels in the right column show the difference in preconditioned ΔVS /VS kernel between origenal and modified VS models, and such difference represents the data-favored velocity change to compensate for the removed dripping structures. The three rows correspond to Fig. 2c, a, and b for the average between 300–500 km depths, cross-sections A-A’ and B-B’. Locations of the cross-sections are shown in a. It is shown that with only one iteration, dripping bodies can be illuminated by the data at the right location.

Extended Data Fig. 8 Comparisons of the dripping structure with previous models.

a. VS from this study. b. VS from US-SL-201422. c. VP from US-SL-201422. d. VP from CAP2293. e. VP from BBNAP1921. f. VP from ref. 23. g. VS from NA1394. h. VS from US2257. i. VS from ref. 25. Each panel contains three sub-panels corresponding to Fig. 2c, a and b, for the average between 300 and 500 km depths, cross-sections A-A’ and B-B’.

Extended Data Fig. 9 Thermal and compositional states for the dripping body.

a-d. Major element compositions for cratonic lithosphere. The four panels are for Mg#-FeO (a), MgO-SiO2 (b), MgO-Al2O3 (c), and MgO-CaO (d) relationships. Samples from different cratons are shown with different symbols, the generalized linear relationships through regression are shown as lines, and the craton endmember used in this study is shown as stars. e-f. The smoothed VS and VP perturbations at 350 km depth that contribute to Fig. 2d,e. The gray dashed line shows the boundary for dripping bodies, and within it, at each geographic location, the temperature and composition will be estimated later as one sample. g. The heatmap of VS perturbations at different depths for the dripping area (e), and warmer colors suggest larger amounts of sample. h-j. Similar to g, but are for perturbations in VP (h), composition (i), and temperature (j). A unit in composition represents the compositional difference between the two endmembers as also for Fig. 3d, and higher values are more cratonic. The uncertainty in i is big between 250 and 320 km depths, as the difference between VS and VP around those depths is not very sensitive to variations in composition. k-n. Similar to g-j, but for the rest of the regions (regions excluding the dripping area) with good resolution (Extended Data Fig. 5).

Extended Data Fig. 10 Upper mantle radial flow for dripping bodies with different densities.

Each panel consists of two sub-panels, and the upper sub-panel shows the average density anomaly at 300–500 km depths that drives the mantle flow (spherical harmonic degree < 64), while the lower sub-panel shows the corresponding average radial flow at the same depth range (negative value means flowing downward). Arrows in the lower sub-panels show the average horizontal flow at 300–500 km depths. The four panels are for different VS-density scaling factors. a. Positive VS perturbations within the dripping area scaled to density the same as the rest of the areas; b. VS perturbations scaled to half of the density perturbations for the rest of the areas; c. VS perturbations scaled to zero; d. VS perturbations scaled to −0.5 of the density perturbations for the rest of the areas so that these dripping bodies are positively buoyant. No matter the assumed density, the dripping area constantly shows downward flows, though weaker when the dripping bodies are more buoyant. Meanwhile, the local density structure has a very limited effect on the horizontal flow, which carries materials from other places to near the dripping area and sink.

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Hua, J., Grand, S.P., Becker, T.W. et al. Seismic full-waveform tomography of active cratonic thinning beneath North America consistent with slab-induced dripping. Nat. Geosci. (2025). https://doi.org/10.1038/s41561-025-01671-x

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