Induced shear failure is key for enhancing hot dry rock (HDR) resource exploitation, aiming to creating an extensive fracture network. Although the macroscopic shear behavior of HDR has been extensively investigated, its microscopic shear failure mechanisms remain unclear. In this study, microscale mode II shear fracture experiments were performed for the first time under various thermal cycling. Micro-scale double-edge notched cube specimens were fabricated from primary minerals and interfaces using micro-machining and subjected to in situ shear tests under a scanning electron microscope. The microscopic shear failure mechanisms and fracture parameters of the minerals and interfaces were investigated. The results showed that multiple thermal cycles reduced macroscopic shear strength by initiating thermal cracks rather than by reducing the strength of the microscale minerals. All three minerals exhibited L-shaped crack propagation below 300°C, with shear initiation and tensile failure. Biotite failed progressively, whereas feldspar and quartz failed catastrophically. High temperatures and multiple thermal cycles caused thermal voids and complex crack paths in feldspar and quartz, whereas biotite exhibited fiber-like plastic slip bands without thermal cracking. The orientation and strength of the mineral interfaces affected crack deflection and branching. Energy was dissipated by interlayer plastic slip in biotite and by micro-crack friction and slip in quartz and feldspar. The microscopic mode II fracture toughness and critical energy release rate were 0.5–3.3 MPa·m0.5 and 0.01–0.11 kJ/m2, respectively. This research provides novel insights into the microscale shear failure of HDR and a critical micromechanical basis for multiscale fracture modeling and macroscopic shear failure analysis.
{"title":"In Situ Microscale Shear Failure Mechanism in Hot Dry Rock Under Thermal Cycling","authors":"Bowen Liu, Cunbao Li, Shixin Zhang, Jianjun Hu, Jie Liu, Biao Li, Heping Xie","doi":"10.1029/2025JB033304","DOIUrl":"10.1029/2025JB033304","url":null,"abstract":"<p>Induced shear failure is key for enhancing hot dry rock (HDR) resource exploitation, aiming to creating an extensive fracture network. Although the macroscopic shear behavior of HDR has been extensively investigated, its microscopic shear failure mechanisms remain unclear. In this study, microscale mode II shear fracture experiments were performed for the first time under various thermal cycling. Micro-scale double-edge notched cube specimens were fabricated from primary minerals and interfaces using micro-machining and subjected to in situ shear tests under a scanning electron microscope. The microscopic shear failure mechanisms and fracture parameters of the minerals and interfaces were investigated. The results showed that multiple thermal cycles reduced macroscopic shear strength by initiating thermal cracks rather than by reducing the strength of the microscale minerals. All three minerals exhibited L-shaped crack propagation below 300°C, with shear initiation and tensile failure. Biotite failed progressively, whereas feldspar and quartz failed catastrophically. High temperatures and multiple thermal cycles caused thermal voids and complex crack paths in feldspar and quartz, whereas biotite exhibited fiber-like plastic slip bands without thermal cracking. The orientation and strength of the mineral interfaces affected crack deflection and branching. Energy was dissipated by interlayer plastic slip in biotite and by micro-crack friction and slip in quartz and feldspar. The microscopic mode II fracture toughness and critical energy release rate were 0.5–3.3 MPa·m<sup>0.5</sup> and 0.01–0.11 kJ/m<sup>2</sup>, respectively. This research provides novel insights into the microscale shear failure of HDR and a critical micromechanical basis for multiscale fracture modeling and macroscopic shear failure analysis.</p>","PeriodicalId":15864,"journal":{"name":"Journal of Geophysical Research: Solid Earth","volume":"131 1","pages":""},"PeriodicalIF":4.1,"publicationDate":"2026-01-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JB033304","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145993348","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Fluid transport properties at the base of the seismogenic zone exert a critical control on fault strength, slip behavior, and fluid circulation. However, quantitative constraints on permeability in deep fault rocks remain limited. We present new laboratory measurements of permeability, porosity, and specific storage on cataclasite- and pseudotachylyte-bearing mylonitic rocks along the Red River Fault (RRF), China. Experiments conducted at effective pressures up to 165 MPa reveal systematically low permeabilities, with mylonitized cataclasites and pseudotachylyte-bearing rocks exhibiting the lowest values (10−22–10−21 m2), while mylonites display relatively higher permeabilities, up to 10−19 m2. A key finding is the pronounced permeability anisotropy, where permeability parallel to foliation is up to two orders of magnitude greater than perpendicular values. This anisotropy reflects the microstructural alignment of phyllosilicate minerals and cavitation bands, which provides interconnected flow pathways along foliation while impeding cross-foliation transport. The hydraulic architecture of the RRF at the base of the seismogenic zone is thus characterized by overall low permeabilities with fluid flow facilitated along mylonitic foliation. Such fabric-controlled anisotropy persists even under mid-crustal pressure conditions, indicating that fault zones at the base of seismogenic depths can retain directional fluid pathways despite overall low permeabilities. Our results provide critical constraints on the hydraulic architecture of the RRF and offer broader insights into the role of anisotropy in controlling fluid flow and deformation at the base of the seismogenic zone.
{"title":"Permeability Architecture at the Base of the Seismogenic Zone: Experimental Studies on Cataclasite- and Pseudotachylyte-Bearing Mylonitic Rocks Along the Red River Fault, China","authors":"Debao Liang, Qingbao Duan, Jianye Chen, Jinyu Chen","doi":"10.1029/2025JB031958","DOIUrl":"10.1029/2025JB031958","url":null,"abstract":"<p>Fluid transport properties at the base of the seismogenic zone exert a critical control on fault strength, slip behavior, and fluid circulation. However, quantitative constraints on permeability in deep fault rocks remain limited. We present new laboratory measurements of permeability, porosity, and specific storage on cataclasite- and pseudotachylyte-bearing mylonitic rocks along the Red River Fault (RRF), China. Experiments conducted at effective pressures up to 165 MPa reveal systematically low permeabilities, with mylonitized cataclasites and pseudotachylyte-bearing rocks exhibiting the lowest values (10<sup>−22</sup>–10<sup>−21</sup> m<sup>2</sup>), while mylonites display relatively higher permeabilities, up to 10<sup>−19</sup> m<sup>2</sup>. A key finding is the pronounced permeability anisotropy, where permeability parallel to foliation is up to two orders of magnitude greater than perpendicular values. This anisotropy reflects the microstructural alignment of phyllosilicate minerals and cavitation bands, which provides interconnected flow pathways along foliation while impeding cross-foliation transport. The hydraulic architecture of the RRF at the base of the seismogenic zone is thus characterized by overall low permeabilities with fluid flow facilitated along mylonitic foliation. Such fabric-controlled anisotropy persists even under mid-crustal pressure conditions, indicating that fault zones at the base of seismogenic depths can retain directional fluid pathways despite overall low permeabilities. Our results provide critical constraints on the hydraulic architecture of the RRF and offer broader insights into the role of anisotropy in controlling fluid flow and deformation at the base of the seismogenic zone.</p>","PeriodicalId":15864,"journal":{"name":"Journal of Geophysical Research: Solid Earth","volume":"131 1","pages":""},"PeriodicalIF":4.1,"publicationDate":"2026-01-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"145993349","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
J. Pablo Canales, Lucky Moffat, Kebabonye Laletsang, Daniel Lizarralde, Steven Harder, Galen Kaip, Estella A. Atekwana, Motsoptse P. Modisi
The Okavango Rift Zone (ORZ) is an incipient continental rift in Botswana at the terminus of the Southwestern Branch of the East African Rift System. The lack of syn-rift magmatism and tectonic processes overprinting pre-rift structures provide an opportunity to investigate incipient-stage rift processes and the role of pre-existing structures in rift initiation and strain localization. We present SEISORZ, a ∼450-km-long wide-angle seismic transect across the ORZ and neighboring tectonic terranes. A 2.5-D VP tomographic inversion reveals crustal thinning within a ∼130-km-wide section of the Damara Belt hosting the ORZ where Moho depth is 38.7 ± 3.4 km, shallower than in other Damara Belt terranes (46.3 ± 1.4 km) and the Kalahari Craton (45.6 ± 2.0 km). Mantle VP is consistent with ultramafic lithologies without evidence for metasomatism, partial melt, or elevated temperatures. Crustal VP is variable but consistent with geological information and with lower-crustal mafic lithologies. However, beneath the rifting region, the model shows low crustal velocities (ΔVP = −0.26 ± 0.05 km/s) that we interpret as damage from rift-related faulting and deformation, and to a lesser extent elevated temperatures possibly from excess radiogenic heat production. Upper crustal heterogeneity correlates with known and newly detected intra-rift faults, suggesting that pre-existing structures promoted strain localization and establishment of the rift border fault system. Collectively, all these factors point to a rheologically weak section in the Ghanzi-Chobe zone which is more susceptible to deformation in response to far-field stresses than neighboring terranes, explaining why incipient rifting is localizing there and not across any other of the terranes that compose the Damara Belt.
{"title":"Crustal Structure Across the Okavango Rift, Botswana: The SEISORZ Wide-Angle Seismic Experiment","authors":"J. Pablo Canales, Lucky Moffat, Kebabonye Laletsang, Daniel Lizarralde, Steven Harder, Galen Kaip, Estella A. Atekwana, Motsoptse P. Modisi","doi":"10.1029/2025JB032322","DOIUrl":"10.1029/2025JB032322","url":null,"abstract":"<p>The Okavango Rift Zone (ORZ) is an incipient continental rift in Botswana at the terminus of the Southwestern Branch of the East African Rift System. The lack of syn-rift magmatism and tectonic processes overprinting pre-rift structures provide an opportunity to investigate incipient-stage rift processes and the role of pre-existing structures in rift initiation and strain localization. We present SEISORZ, a ∼450-km-long wide-angle seismic transect across the ORZ and neighboring tectonic terranes. A 2.5-D <i>V</i><sub><i>P</i></sub> tomographic inversion reveals crustal thinning within a ∼130-km-wide section of the Damara Belt hosting the ORZ where Moho depth is 38.7 ± 3.4 km, shallower than in other Damara Belt terranes (46.3 ± 1.4 km) and the Kalahari Craton (45.6 ± 2.0 km). Mantle <i>V</i><sub><i>P</i></sub> is consistent with ultramafic lithologies without evidence for metasomatism, partial melt, or elevated temperatures. Crustal <i>V</i><sub><i>P</i></sub> is variable but consistent with geological information and with lower-crustal mafic lithologies. However, beneath the rifting region, the model shows low crustal velocities (Δ<i>V</i><sub><i>P</i></sub> = −0.26 ± 0.05 km/s) that we interpret as damage from rift-related faulting and deformation, and to a lesser extent elevated temperatures possibly from excess radiogenic heat production. Upper crustal heterogeneity correlates with known and newly detected intra-rift faults, suggesting that pre-existing structures promoted strain localization and establishment of the rift border fault system. Collectively, all these factors point to a rheologically weak section in the Ghanzi-Chobe zone which is more susceptible to deformation in response to far-field stresses than neighboring terranes, explaining why incipient rifting is localizing there and not across any other of the terranes that compose the Damara Belt.</p>","PeriodicalId":15864,"journal":{"name":"Journal of Geophysical Research: Solid Earth","volume":"131 1","pages":""},"PeriodicalIF":4.1,"publicationDate":"2026-01-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2025JB032322","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"146001102","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Hélène Le Mével, Nathan L. Andersen, Annika E. Dechert, Josef Dufek
<p>From 2019 to 2024, gravity surveys were conducted at the Three Sisters volcanic cluster (TSVC), measuring 246 gravity sites using a spring relative gravimeter. We calculated the residual Bouguer anomaly and identified three main zones with negative anomalies, ranging from −4 to −8 mGal, located southwest and west of South Sister, within an area that has been uplifting for the past two decades. After inversion, we obtain a 3D density model of the subsurface and identify low-density bodies extending from the surface down to 3 km. We estimate a total of 15 k<span></span><math>