- 1School of Earth Sciences and Resources, China University of Geosciences, Beijing, China
- 2Institute of Earth Sciences, China University of Geosciences, Beijing, China
- 3Department of Earth Sciences and Engineering, Taiyuan University of Technology, Taiyuan, China
The North Himalayan Gneiss Domes, which are essential parts of the Cenozoic extensional structures in Southern Tibet, record the thermal and tectonic processes that occurred after the India-Asian collision and are thought to be effective structures regulating post-collision intracontinental deformation. However, it is still unclear how these domes are formed and how they contribute to the regulation process. Here, we performed detailed geological mapping, elevation transect sampling, low-temperature thermochronological testing, and 3D modeling on the Kangmar dome, which is located west of the N‒S treading Yadong-Gulu rift, and its core-cover contact fault is suspected to be the northern continuation of the South Tibetan Detachment System (STDS). Our analysis revealed a discrepancy in the deformation histories of the dome’s northern and southern portions. We proposed a model in which the core-cover contact fault of the Kangmar dome was a part of the South Tibetan Detachment System and the doming event that occurred at ∼12.2 Ma was dominated by thrust stacking of the southward mid-crustal channel flow. The rapid cooling following the middle Miocene was possibly influenced by the N‒S Trending Yadong-Gulu rift activity. The present landscape was shaped by the incision of the Nianchu River, which was accompanied by increased glacial activity during the Pleistocene. Our findings enhance the intracontinental deformation patterns following collisions and shed light on the numerous domes in Himalayas and other orogenic belts.
1 Introduction
The North Himalayan Gneiss Domes (NHGDs) are ubiquitous structures within the Himalaya orogen belt, which, together with the N‒S trending normal faults and the Southern Tibetan detachment systems, compose the typical postcollision extensional structures in northern Himalaya (Zhang et al., 2012). These well-exposed middle-lower crustal rocks are archives of the crustal thickening, metamorphism, melting, deformation, and exhumation processes that occurred throughout the convergence of India and Eurasia (e.g., Schärer et al., 1986; Lee et al., 2000; Lee et al., 2006; Quigley et al., 2008; Zeng et al., 2009; Gao and Zeng., 2014). Various formation mechanisms and the geological evolution of the domes have been hypothesized (Le Fort et al., 1987; Chen et al., 1990; Lee et al., 2000; Larson et al., 2010). Particular domes have been studied via limited research methods, the evolutionary history of gneiss domes has been intensely debated. This has also led to a lack of clarity regarding the interconnection of Cenozoic extensional structures in southern Tibet.
Eskola (1949) initially stated that a mantled gneiss dome was composed of a metamorphic-plutonic complex core that was overlain by supracrustal strata. After the discovery of extensional detachment faults (Coney et al., 1980), a number of classic gneiss domes (e.g., Simplon metamorphic terrane in the Alps; gneiss domes in the Variscan belt) have been construed as extensional metamorphic core complexes (Mattauer et al., 1988; Mancktelow and Pavlis., 1994; Wawrzyniec et al., 2001). The high-strain detachment faults of gneiss dome systems usually form core-cover contact faults, which separate the dome cores from their overlying strata (Jessup et al., 2019). The difference in perception of the core-cover contact fault is also reflected in a controversy over the last few decades regarding the formation mechanisms of the typical gneiss domes found throughout the globe, which has led to three main mechanisms: 1) diapirism (Ramberg, 1980), 2) crustal shortening (e.g., Brun, 2003; Ramsay, 1967), and 3) crustal extension (e.g., Miller et al., 1992). Jessup et al. (2019) classified the kinematic models that were derived from these mechanisms and applied to the NHGD into three inconsistent groups: 1) diapirism and/or buoyancy-driven models (e.g., Le Fort et al., 1987); 2) metamorphic core complex models (e.g., Chen et al., 1990); and 3) out-of-sequence thrusting and/or folding models (Lee et al., 2000; Larson et al., 2010). Predictably, apart from the activity of the core-cover contact fault, which to some extent influences the exhumation history of the dome, it is conceivable that the precise definition of the kinematic property, activity processes, and affiliation of the dome plays a decisive part in exploring the domes’ formation mechanism and geotectonic evolution.
Although the gneiss core and overlying strata of the Kangmar dome have been dated sufficiently by prior studies (Debon, 1980; Xu and Jin, 1986; Liu et al., 2004; Wang et al., 2018), the spatiotemporal evolution history has not been elucidated. As a distinct extensional structure, the exhumation of the gneiss core and the timing and intensity of the detachment fault are crucial for understanding the doming process, which remains ambiguous. This study aims to address the cooling histories between the southern and northern portions of the dome through detailed geochronological investigations and via the thermochronological dating of samples collected along elevation transects. We apply multiple-scenario thermokinematic modeling to clarify the evolutionary history of the core-cover contact fault, the rock uplift, and the river incision that occurred following the doming event to create a bridge between dome formation and regional structural activities. Coupled with the morphological analyses of the Nianchu River and the explanation of the rapid cooling events, we shed additional light on how the Kangmar dome formed and was exhumed. Our results suggest that the hanging wall of the core-cover contact fault has an overall northward movement, and the doming event occurred first in its southern portion ∼12.2 Ma, which was much earlier than that in the northern portion. The second rapid cooling in the Pleistocene was mainly due to glaciation intensified by global cooling.
2 Geological background
2.1 Regional geological setting
The Himalayan orogenic belt was formed by the continuous convergence of the Indian and Eurasian continents after their initial collision during the early Cenozoic (Molnar and Tapponnier, 1975; Yin and Harrison, 2000; Li et al., 2012; Meng et al., 2012). Crustal shortening and extension are two deformational styles in the Himalayan orogenic belt (Li et al., 2015), forming the thrust structures of the Main Frontal Thrust (MFT), the Main Boundary Thrust (MBT), and the Main Central Thrust (MCT) from the south and the extensional South Tibetan Detachment System (STDS) to the north. These structures divide the Himalayan orogenic belt into four parts from south to north: the Sub-Himalayan Sequence (SHS), the Lesser Himalayan Sequence (LHS), the Greater Himalayan Crystalline Complex (GHC) and the Tethyan Himalayan Sequence (THS) (Figure 1A).
FIGURE 1. (A) Simplified geologic map of the Himalayan orogenic belt, southern Tibet, showing locations of the North Himalayan Gneiss Dome (modified after Wang et al., 2022). (B) Simplified geologic map of the Yarlung Tsangpo catchment, showing the relative locations of the NGHD, Nianchu River and Yalung Tsangpo River. MBT, Main Boundary thrust; MCT, Main Central thrust; MFT, Main Frontal thrust; STDS, South Tibetan detachment system; IYSZ, Indus-Yarlung suture zone; THS, Tethys Himalaya Sequence; GHS, Grater Himalaya sequence; LHS, lesser Himalaya sequence; SH, sub-Himalaya; NHGD, North Himalayan Gneiss Dome.
The Tethys Himalayan Sequence is bounded by the Indus-Yarlung suture zone (IYTZ) to the north and the STDS to the south, which represent the remnants of the stratigraphic sequence deposited along the India passive margin toward the Neotethys Ocean (Sciunnach and Garzanti, 2012). This area is separated into southern and northern sections by the Gyirong-Kangmar thrust (GKT) (Ratschbacher et al., 1994). The N‒S Trending Rifts (NSTR) (Figure 2A) and NHGD are located within these sedimentary strata and, together with the STDS, form a typical postcollisional extensional structure in the northern Himalayas. The NHGD is exposed within the THS (Figure 1A). It consists of more than ten discontinuous, subparallel latitudinal band-spreading domes, including from west to east the Malashan, Lhagoi Kangri, Mabja, Kampa, Kangmar, Ramba, Yardoi, and Cuonadong gneiss domes (e.g., Zhang et al., 2004; Aikman et al., 2008; King et al., 2011; Zeng et al., 2011; Liu et al., 2014). With an average peak elevation of over 5,000 m, the dome belt trail is consistent with the partial drainage divide of the Yarlung Tsangpo River (Figure 1B).
FIGURE 2. (A) Regional channel steepness in parts of the Nianchu catchment. See Figure 1 for location. Two black boxes mark the locations of the Kangmar and Ramba domes. The dark red frames mark the regional segments of the Yadong-Gulu rift. (B) Swath profile [corresponding to the purple rectangular box in (A)] along the Nianchu River, showing the undulating topography along the Nianchu River.
Numerous previous studies on leucogranite rocks within the NHGD have documented a series of crystallization and emplacement ages ranging from 47 to 7 Ma (e.g., Lee et al., 2004; Zeng et al., 2011; Gao et al., 2012; Liu et al., 2014; Ji et al., 2020; Chen et al., 2022) and cooling ages that range from 22 to 6 Ma (e.g., Lee et al., 2000; Lee et al., 2004; Guo et al., 2008). With deformation and metamorphic characteristics almost identical to the GHS, it was proposed that the NHGD domes were part of a laterally continuous plane with the GHS at the onset of Himalayan orogenesis (Harrison et al., 1997; Beaumont et al., 2001; Beaumont et al., 2004; Lee et al., 2006; Ding et al., 2016), and combined with the fact that the cores of these domes are always subducted beneath the THS, their core-cover contact faults are therefore widely recognized as continuous parts of the STDS (Chen et al., 1990; Hauck et al., 1998; Liu et al., 2014). The current research consensus on elevation histories is that two major ductile deformation events were recorded in those domes: an older N–S shortening and vertical thickening episode and a younger N–S extensional and vertical thinning episode, which were bracketed in age between late Eocene-early Oligocene to middle Miocene (Chen, 1997; Lee et al., 2000; Zhang et al., 2004; Aoya et al., 2005; Aoya et al., 2006; Quigley et al., 2006; Kawakami et al., 2007; Quigley et al., 2008).
Topographically, the Yarlung Tsangpo catchment and the Ganges catchment area are bordered in southern Tibet, and their dividing line roughly coincides with the NHGD uplift belt (Figure 1B), to the south of which most of the rivers drain southward into the Ganges, except the Nianchu River. As one of the largest tributaries of the Yarlung Tsangpo, the Nianchu River originates from the Greater Himalaya (Chongbayong Co., 28.22°N, 89.64°E, 4,575 m above sea level) and drains the THS with a total length of 190 km (Figure 2A). The Kangmar dome is deeply incised by the Nianchu River, which preserves the high-steepness of the stream-valley landscape.
2.2 Geology of the Kangmar dome
The Kangmar dome (Figure 3A), located in the eastern segment of the NHGD, contains a gneiss core that is mantled by Precambrian basement metasedimentary rocks and overlain by the low-grade metamorphic to non-metamorphic THS. The core-cover contact fault is fully exposed in the stream valley formed by the Nianchu River and is characterized as a low-angle ductile shear belt (Figure 3A). Above the contact is the hanging wall unit, which is composed of Ordovician to Cretaceous rocks that range from metamorphosed schist rocks at the base to unmetamorphosed sedimentary rocks at the top. Apart from the valley landscape, there are several glacial relics represented by glacial valleys (Figure 3B), resulting in the intermittent presence of tributaries of the Nianchu River.
FIGURE 3. (A) Simplified geologic map of the Kangmar gneiss dome. (B) Satellite image of the Kangmar dome area, marking the glacial remains represented by the ice erosion valley. (C) Composite structure-age diagram of the Kangmar dome. The locations of cross-section lines are shown in (A), and ages are cited from Lee et al. (2000) and show an increasing trend from south to north.
Additional U‒Pb dating of the gneiss core has revealed crystallization ages of 520–478 Ma (Schärer et al., 1986; Lee et al., 2000; Xia et al., 2008; Gao et al., 2019). A combination of 40Ar/39Ar thermochronology ages obtained from the core or from the ductile shear belt has shown two phases of cooling for the Kangmar dome at ∼20 and ∼13 Ma (Chen., 1979; Lee et al., 2000; Liu et al., 2004; Wang et al., 2015). These cooling ages were interpreted as partial thermal events or responses to fault activity. There is a general trend of younger values from south to north (Figure 3C).
3 Approach and methods
3.1 Geological mapping and sample processing
The outcropping of strata in the Kangmar dome and adjacent regions resulted in widespread exposure of typical internal structures, which are ideal features to explore the deformation characteristics of the dome. The geological mapping of the Kangmar dome includes measurements of stretching lineations preserved within the gneiss core and observations of the complex deformation structures within the core-cover contact fault shear zone and cover strata. Compared to the abundant thermochronology results from samples distributed from the incoming horizontal elevation (e.g., Chen., 1979; Lee et al., 2000; Liu et al., 2016; Wang et al., 2015), there are few data points from the age-elevation transects that could be used to calculate exhumation rates, assuming temporally and spatially invariant horizontal isotherms (Wagner and Reimer, 1972). To understand the evolution history, we collected samples from two subvertical transects along two ridges on the gneiss core, located in the northern and southern portions of the dome (Figure 3A). The two transects were sampled over a relief of ∼720 m (southern transect) and ∼860 m (northern transect) along the ranges and both within a limited horizontal distance. The rocks sampled are all gneiss with a sampling interval of ∼100 m.
3.2 Low-temperature thermochronology
Low-temperature thermochronometry is a technique that reconstructs the thermal evolution of the upper crust (<5 km) (Wagner and Van den Haute, 2012) for examining the cooling history of footwall samples exhumed via normal fault exhumation mechanisms that include time-varying rock uplift and landscape evolution (Reiners and Shuster, 2009; Ault et al., 2019). We use apatite fission track (AFT), zircon (U-Th)/He (ZHe) and zircon fission track (ZFT) dating for this study, which covers a large scale of annealing and retention and ranges from ambient temperatures to ∼190°C (Reiners, 2005; Ketcham et al., 2007; Tamer and Ketcham, 2020). Here, we present 14 AFT, 6 ZHe, and 5 ZFT samples (Table 1).
AFT and ZFT analyses for the two transects were performed at Apatite Technology Co., Ltd., whereas ZHe analyses were performed at The University of Melbourne. Details of the experimental procedure are in Supplementary Text S1.
3.3 Morphometry analysis of the Nianchu River
The morphological study of the rivers in the region is also included in our work, as we assume that a precise sequencing of fluvial formation and tectonic activity are essential prerequisites for a rational exploration of cooling history. The bedrock channel response to differential rock uplift could be measured by the channel-steepness index ksn (Whipple and Tucker, 1999; Kirby et al., 2003), which is based on the power-law relationship: S = ksA−θ (S: local channel slope; A: contributing drainage area; θ: concavity index; Flint, 1974). We adopted the principle to measure the local channel slope (S) for the change in upstream drainage area (A) along the length of the channel profiles and then calculated a normalized channel steepness (ksn) using a fixed reference concavity θ = 0.45, as shown by Liang et al. (2020). Channel steepness values are color coded for the river channels shown in Figure 2A to highlight the changes in channel morphology along with their channel profiles. A high-relief landscape area was also defined that encompassed the region in which the main channel or tributaries of the Nianchu River had relatively high Ksn values. The distribution of N‒S trending Yadong-Gulu rifts was also superimposed to visually represent the possible response of the river to fault activity.
4 Results
4.1 Deformation characteristics of the dome
The gneiss core contains a well-developed stretching lineation, which is defined by aligned biotites and weakly flattened quartz grains (Figure 4B). Measurements of stretching lineations were spread over the entire gneiss core and resulted in an approximately N‒S treading (Figure 3A). Meanwhile, mesostructures observed within the ductile shear belt of the core-cover-contact fault show a nearly identical kinematic stress direction of N‒S (Figure 4E). The kinematic stress structures observed over the contact began to exhibit an additional progressively more pronounced E‒W extension, composed of K-feldspar porphyroblasts to S-C fabric (Figures 4C, D), which indicates E‒W shearing in direction and magnitude with the gneiss core. The lower Permian slate layer (Figure 5A), located in the southern position of the covering low-grade metamorphic rock, retains large-scale shear-type boudinage structures (Figure 5B), indicating vertical thinning due to top-to-the-N shearing. The kink band (Figure 5C) superposed on preexisting asymmetrical folds also shows top-to-the-N shearing.
FIGURE 4. (A) Composite diagram illustrating the three-dimensional structure of the Kangmar dome. The locations of the cross-section lines and legend are shown in Figure 3A. (B–E): Summary of kinematic structures in different positions of the Kangmar dome.
FIGURE 5. (A) Structural observation within the lower Permian slate layer, (B) large-scale shear-type boudinage representing near top-to-the-N shearing and vertical thinning, and kink band structure (C) in the structural lower level representing the northward movement of the upper strata.
The circular shape indicating the exposed core-cover contact fault was recognized as a normal fault on both the southern and northern portions of the dome (Figure 6). The dip of the core-cover contact fault differs and the southern part shows a greater inclination (25°) than the northern portion (15°) (Figure 4A). The cover of both dome portions is consistent in terms of lithological succession but differs in thickness, with the southern portion displaying significantly thicker than the northern portion. This is especially the case in the Precambrian crystallization basement, which shows an apparent thickness of ∼620 m in the southern portion (Figure 6A) and only ∼380 m in the northern portion (Figure 6B).
FIGURE 6. Field relationships in the Kangmar dome. (A) East-looking view of the south portion, and (B) south-looking view of the north portion. Photographs taken from the location and orientation indicated by white boxes in Figure 3 show that the strata sequence was continuous, but the distance between the “core-cover contact” and marker-bed marble belt in the Precambrian basement was significantly different.
4.2 Low-temperature thermochronology ages
The AFT ages of fourteen gneiss samples range from 2.7 ± 0.5 to 8.9 ± 3.9 Ma (Tables 1, 2). The Southern transect ages range from 2.7 to 5.9 Ma, whereas the northern transect ages range from 2.7 to 8.9 Ma (Table 2). The AFT dating of the southern transect included eight samples, all of which passed the χ2 test, representing a single age population (Galbraith and Laslett, 1993), which suggests that these samples experienced full annealing for their AFT ages. The AFT dating of the northern transect included six samples. Samples D0701, D0707, and D0708 yield AFT ages of 8.9 ± 3.9, 5.8 ± 0.8 and 4.1 ± 0.7 Ma, respectively (Supplementary Figure S1), which did not pass the χ2 tests, suggesting multiple age populations (Galbraith and Laslett, 1993). The two transects both show clear age-elevation relationships (Figures 7D, E). Six samples (D0812, D0820, D0703, D0705, D0707, and D0708) from the two transects have relatively consistent and short unprojected mean horizontal confined track lengths, with negative skewness (Supplementary Figure S1; Table 2), which range from 10.98 to 13.40 μm. This suggests that these samples had a relatively short stay at the partial annealing zone and represent metamorphic rocks that cooled fast as they neared the surface (Wang et al., 2018; Bi et al., 2022).
FIGURE 7. (A) Location of the two elevation transects (Refer to Figure 3A legend for details); (B) Exhumation scenario and (C) Fault-exhumation scenario setup for the 3-D thermokinematic modeling (parameters are given in Supplementary Table S1). Measured and modeled age-elevation relationship of the southern (D) and northern (E) transects in Exhumation scenario, (F) northern transect in Fault-exhumation scenario.
Twenty-two single-grain ZHe dates from six samples have been reported (Table 3). Generally, the ZHe ages offer a narrow range of ∼9 Ma. For the two transects, the ages of samples are mostly reproducible, and the plots of the ZHe ages versus grain size or effective Uranium [(eU) = (U) + 0.235 × (Th)] content show no clear relationship (Supplementary Figure S2); hence, radiation damage does not appear to influence the age distribution (Guenthner et al., 2013).
The ZFT ages of the five gneiss samples range from 14.7 ± 0.6 to 17.3 ± 0.9 Ma (Tables 1, 4). All samples failed to pass the χ2 test (Supplementary Figure S3), perhaps because of the poor quality of zircons; therefore, the central zircon fission track ages were preferred, which ranged from 13.6 ± 0.6 to 17.3 ± 0.9 Ma in the southern transect and 14.7 ± 0.6 to 16.8 ± 0.8 Ma in the northern transect. Neither of the two transects had enough confined track lengths to determine their cooling modes.
All the low-temperature thermochronology ages are younger than their corresponding zircon U‒Pb ages of 520–478 Ma (Schärer et al., 1986; Lee et al., 2000; Xia et al., 2008; Gao et al., 2019), suggesting that these ages were generated by monotonic cooling after magma emplacement and crystallization (Gleadow et al., 1986).
4.3 Channel steepness index of the Nianchu River
The morphology of the Nianchu drainage is generally inhomogeneous, even though the channel steepness of the Nianchu mainstream remains within a limited range for the majority of stream segments. Its tributaries in the upper and lower reaches have similar Ksn values of <40, which were smaller than those in the middle reaches (40-64) within the Kangmar dome region. Although some tributaries were not identified in our fieldwork, these tributaries identified by GIS within the Kangmar dome area could perhaps be regarded as intermittent rivers, and their ksn values can also be used to characterize the steepness of the river valley in this region. These rivers with high ksn values (>40) are circled by the white line in Figure 2A and represent high-relief geomorphology, which suggests that the Nianchu River has undergone a low-relief to high-relief landscape transition during its upper-middle reaches and trends toward a low-relief landscape in its middle-lower reaches. The Kangmar dome is basically located in the center of the defined high-relief landscape area.
5 Thermokinematic modeling (Pecube)
The Pecube modeling process considers landscape evolution (topography, relief), the crustal thermal regime, tectonic setting (fault configurations, surface uplift or subsidence) and the isostasy to quantify thermal histories for rock particles at depth during exhumation or burial contexts (Braun, 2003; Braun et al., 2012). The Pecube thermokinematic program allows the testing of multiple tectonic scenarios and predicts the geographic distribution of thermochronological ages for individual samples. As part of this process, it solves the 3D heat equation in the crust and takes into account exhumation through lateral and vertical rock kinetics, as well as relief evolution. By reducing the misfit function between predictions and observations, we employed Pecube v3.0 (Braun et al., 2012) in inverse modes (neighborhood algorithm; Sambridge, 1999a; Sambridge, 1999b) to establish optimal value ranges for the tested parameters.
5.1 Model setup
In the Pecube modeling, geological scenarios accommodate temporal fluctuations in vertical exhumation rates and fault slip rates, either separately or in combination. Exhumation or topographic changes between different phases can be defined by different transition times (Ou et al., 2021). We defined an “exhumation scenario” that considers exclusively vertical exhumation rates that change geographically and temporally to maintain the present topography over time. Our new AFT ages are similar in age results to Lee et al. (2000) but show an opposite increase in the trends of different ages within the same tectonic layer (Figures 3C, 7D, E). Coupled with the difference in geological observations and dating ages between the southern and northern transects of the Kangmar dome, it is reasonable to propose that the two portions have different cooling rates; therefore, we modeled the two portions separately in the “exhumation scenario” (Supplementary Table S2). Models were started at 20 Ma to encompass the history recorded by most of our measured data. We have divided the timeline into many phases to give maximum freedom to the free parameters in the inversion. These resulting transition times are not geologically meaningful, and those transition times will be determined by the differences in rates before and after the transitions. To control for variables, the two models differed only in their age code but were similar in the area and the ranges of the free parameters (Figure 7B). The initial topographic elevation, which represents the elevation before uplift, is set within a parameter space between 3,450 and 4,570 m, consistent with the highest and lowest elevations of the current Nianchu River, and we use the results to test the rationality of the two models. Details of the thermal and mechanical parameter values used in the inverse models are detailed in Supplementary Table S1.
In an additional simulation of the northern portion, we define a “fault-exhumation scenario” as a scenario that more comprehensively considers the activities of the fault in consideration of our field geological investigations, which showed that the northern and southern portions of the dome were subject to N‒S shearing, possibly due to fault activity. The inclination of the set fault in that model was consistent with the present day inclination, and the remaining cooling was decoupled to the vertical direction and was expressed by setting a subvertical fault (Figure 7C). In contrast, the initial topographic elevation and transition times of this scenario will adopt the best-fit parameter of the northern “exhumation scenario” to control the number of unknowns (Supplementary Table S2), while other parameters are the same as the first scenario (Supplementary Table S1).
The calculation was supported by the Advanced Computing East China Subcenter. Each inversion procedure contained 19,000 Pecube forward models, and 60 iterations, with 300 sample sizes per iteration and a 33% resampling rate, were applied. The calculation of the misfit function is related to the measured-predicted relationship for each sample.
5.2 Numerical thermo(-kinematic) modeling results
The inversion results from the three models for the two scenarios are listed in Supplementary Table S2. The two models for the exhumation scenario have misfit values of 0.21 and 0.19, and the fault-exhumation scenario has a misfit value of 0.18. As mentioned before, the simulation results from the two models for the initial topo are 4,560 and 4,539 m, respectively, which are similar to the present day topographic elevation differences. Given that their models are based on different parameter settings, this similarity for the common free parameters indicates that the model settings are logical and provides a basis for a joint discussion of the two models (Figure 7B). The lowest-misfit model produces an excellent fit between the predicted and measured ages of the AFT, ZHe and ZFT thermochronometers (Figures 7D–F), and the biotite 40Ar/39Ar ages are distributed in a narrow range of 14–15 Ma, which is consistent with the result reported by Lee et al. (2000). Subsequently, we recalculate the depth-time paths generated from the temperature‒time path in the forward model, combined with the average annual temperature of the Earth’s surface (8°C) and the geostrophic gradient of 30°C/km.
6 Discussion
We identified inconsistent cooling histories between the northern and southern portions of the Kangmar dome. The modeling directly reveals the cooling histories of the two transects, the velocity of the fault activity and the vertical cooling. However, the interpretation of experimental and modeling results, coupled with geological evidence, is premised on a discussion of the properties of the Nianchu River since the modeled vertical cooling rates do not directly represent the surface uplift rates. Additionally, the flexural response to surface changes should also be considered. However, we believe that the Nianchu River is an antecedent stream river, which is indicated by the Ksn analysis results. Under such a premise, the incision of the Nianchu River will always be accompanied by surface uplift, and its rate will increase with increasing surface uplift rate. Then, in the absence of regionally significant climate change, we think that the obtained cooling rates are a positive function of surface uplift or river incision. From this, the results of the modeling scenarios can be used to develop the following discussion.
6.1 Geologic affiliation of the core-cover contact fault
Alternatively, the “core–cover contact” fault of the Kangmar dome was defined as follows: 1) the fault is part of a thrust duplex, which was based on observations of tight to isoclinal folds in the top metasedimentary carapace that converged to the south, the reorientation of fold axes to N‒S in the lower carapace, and how the shear strain rose with structural depth (Burg et al., 1984); 2) the fault represents the response of a metamorphic core complex-type detachment fault to the gravitational collapse of the Himalayan topographic front (Chen et al., 1990); 3) the fault is a non-conformity with no or minimal displacement (Lee et al., 2000); or 4) the fault indicates a normal-sense (top-to-the-N) brittle‒ductile shear zone, equivalent to the STDS (Wagner et al., 2010).
The most remarkable result of our geological analysis is the N‒S movement of the fault hanging wall, as reflected by stretching lineation, which distinguishes the Kangmar dome from the diapirism mechanisms of typical domes, such as the Yardoi dome (Zhang et al., 2007) that is located at the easternmost end of the NHGD. The stretching lineation of its core is oriented in a spreading direction to the periphery and extends downward. In the inversion result of the exhumation scenario, the southern portion of the dome experienced its first rapid cooling before 17.7 Ma (Supplementary Table S2; Figure 8A), and the depth contour lines based on depth‒time paths reflect that the southern portion was uplifted earlier before the northern portion since ∼17.7 Ma and located at a shallower depth until ∼5 Ma (Figure 9). Since the activity of the fault somehow affects the kinematic features of the gneiss core, the significant variation in uplift histories of the two portions in such a limited area is, we believe, related to the differential properties of the core-cover contact fault at each side. Furthermore, the intersection depth of the biotite 40Ar/39Ar isotherm in the northern portion is deeper than it is in reality. In comparison, the biotite intersection depth in the south portion is shallower (Figure 9), suggesting that the isotherm within the south portion has shifted upward at this stage. These differences could be explained by the thrust-sense faulting of the hanging wall in the south portion, which is consistent with the geological evidence that the southern strata are thicker (Figure 6) and the present day structures indicating top-to-the-N shearing (Figure 5). Thus, the northward movement of the cover strata caused the first rapid cooling in the southern portion, and this rapid cooling event started earlier than the starting time of our simulation models at 20 Ma.
FIGURE 8. Graphical representation of the best-fit inversion result of the cooling rate from the exhumation scenario (A) and/or velocity from fault-exhumation scenario (B); (C) the chemical index of alteration (CIA) data from Ocean Drilling Program (ODP) Hole 885A, North Pacific Ocean (Zhang., et, al. 2019), the sea surface temperature data from Ocean Drilling Program (ODP) Hole 722 in Arabian Sea and 1021 in North Pacific Ocean (Herbert and Lawrence, 2016); (D) Tectonic activities in the Kangmar-Yadong area, southern Tibet. Timing of the STDS (Webb et al., 2017; Dong et al., 2021) and E‒W extension (Dong et al., 2021; Bian et al., 2022; Wang et al., 2022).
FIGURE 9. Topographic profiles, averaged equilibrium line altitudes (ELAs), and exhumation patterns (depth isochrones) along a south‒north swath across the Kangmar dome. The swath is part of Figure 2B. The curves in the green box represent the depth‒time path of the two transects generated from their best-fit model, note that the blue dotted line represents the isotherms (assuming that the south portion takes the B-Ar value of ∼14 Ma, the north ∼12 Ma), GGD, Geothermal-Gradient Depth. The orange lines represent the depth isochrones generated from the depth‒time path.
In the exhumation scenario, the first rapid cooling of the northern portion began at ∼12.2 Ma, and after the inversion of the fault-exhumation scenario, we detailed the effects of vertical cooling or cooling along the fault and the results show that rapid cooling began at ∼12.2 Ma and was oriented mainly along the fault (Figure 8B). Although this timing is consistent with the 40Ar/39Ar age of ∼13.23 Ma, which was derived from the analysis of syn-deformation muscovite from the mylonitic garnet two-mica schist within the fault shear zone and was interpreted as the initial detaching time of the core-cover contact fault (Wang et al., 2015), we do not consider that this phase of rapid cooling was controlled by fault activity, but instead, we believe that the doming event of the north portion was the direct cause of cooling. The doming of the gneiss core increases the dip of the fault, which leads to the emergence of cooling velocities along the fault. According to the forward-modeled depth isochrons (Figure 9), the northern transect started to dramatically uplift after 12 Ma, and the doming event first occurred in the northern portion at 12.2 Ma, much later than it did in the south. Since the core-cover contact fault of the Kangmar dome was a continuous interface exposed from north to south without interruption, it is reasonable to infer that the cover strata of the northern portion also had a consistent northward movement history before its doming event.
Our simulations showed that the cover strata above the Kangmar gneiss core had the same northward movement as the STDS in the Miocene and were consistent with the geological evidence characterized by the extensive distribution of stress formations in both the gneiss core and cover (Figure 3A), which revealed a N‒S movement of the cover strata. As discussed below, considering that the onset time of the dome and its location is coincident with the STDS, we concur with the suggestion of Chen et al. (1990), Hauck et al. (1998), and Liu et al. (2016) that this fault is the northern continuation of the STDS and is an exposed portion of the Tethyan Himalayan sedimentary sequence.
6.2 Rapid cooling history of the dome
6.2.1 Post-middle Miocene rapid cooling
In our simulations, the timing of the doming event in the southern portion precedes that in the northern portion, and the core of the Kangmar dome has been experiencing rapid cooling since the Miocene and the northern portion had a higher cooling rate from 12.2 to 9.1 Ma and a more consistent cooling rate after 9.1 Ma and before 1.8 Ma. We believe that the core-cover contact fault of the Kangmar dome is subordinate to the STDS. The rapid cooling of the northern portion of the Kangmar dome at ∼12 Ma, which accompanied doming during this period, was caused by the northward sliding of the STDS. However, present day studies suggest that the more short-lived southern STDS ended prior to 11 Ma (Dong, et al., 2021; Figure 8D). The northward movement of the upper strata could not cause the rapid cooling of the southern portion. Since there are many E‒W extensional structures above the dome (e.g., Figures 4C, D), we take the N‒S trending rift’s impact on dome cooling. Wang et al. (2022) concluded from fault gouge studies that the Pari-Duoqingcuo graben (Figure 2A) was active earlier than 9 Ma and that the activity of the Yadong-Gulu Rift was consistent and continuous. Bian et al. (2022) further inverted the thermochronological data of the Yadong area and concluded that the onset of rifting occurred at 12 Ma (Figure 8D), which coincides with our modeled results for the rapid cooling of the northern portion. It is plausible that the E‒W extension of the Yadong-Gulu Rift may have triggered the uplift of the dome core by vertically thinning the cover strata, thereby causing this phase of rapid cooling. However, this explanation still needs more geological evidence and discussion.
6.2.2 Pleistocene rapid cooling
If the northward sliding of the STDS and the tectonic action of vertical thinning of the THS due to the E‒W extension of the Yadong-Gulu rift are plausible explanations for the Miocene rapid cooling of the Kangmar dome, the activity in the Yadong-Gulu Rift, which was not significantly accelerated in the Pleistocene, would not have caused the rapid cooling event starting after ∼1.8 Ma. The extensive present day pale glacial remains and very low modern glacial cover of the Kangmar dome prevent us from ignoring glacial activity over the geological-historical period within its region. At this stage, climatic events on the Tibetan Plateau coincided with global climatic events (Ji et al., 2013), and sea surface temperature changes reflected in boreholes from the North Pacific (ODP1021) and Indian Ocean (ODP722) (Herbert and Laerence, 2016) show that the Earth’s climate changed markedly during the Pliocene (Figure 8C), with a general trend of variable cooling over time. According to our simulations, the Pleistocene rapid cooling of the gneiss core is temporally similar to this rapid global cooling of sea surface temperature. Zhang et al. (2019) revealed the enhanced chemical alteration in the Asian hinterlands through the changes in the chemical index of alteration (CIA) of the core sediments from ODP885A in the North Pacific Ocean and attributed it to the increased surface exhumation caused by increased inland glaciation (Figure 8C). We suggest that the enhanced glacial activity of the Kangmar dome region in the context of this phase of rapid global cooling during the Pleistocene may have directly intensified surface exhumation, and at the same time, the increase in glacial melt water further strengthened the incision of the Nianchu River. This joint action may have caused rapid cooling since ∼1.8.
6.3 Evolution of the dome and its implications
After the doming event occurred in the Miocene, our modeling results revealed a northward movement along the STDS, which differed significantly from the “gravitational collapse” model in terms of fault movement properties. However, Chen et al. (1990) argued that the dome developed via mechanisms similar to the metamorphic core complexes (MCC) in Cordilleran regions. Our fault-modeling results agree with this fault affiliation. With an absence of essential components, e.g., detachment systems, hanging-wall extension faults, and basins, the mechanism based on simple linkage with typical MCC is seemingly unreasonable.
In light of an “inverted” pattern in which the mica cooling ages increased toward deeper structural levels and decreased northward at the same level, Lee et al. (2000) proposed that the doming event resulted from the thrusting of the hanging wall mid-crustal rocks along the north-dipping Gyirong-Kangmar thrust fault (GKT) (Figure 3C). Wang et al. (2022) modified the movement nature of the core-cover contact and tested a mid-crustal “channel-flow” model that solved its dynamic origin. However, the mechanism of “thrust along the GKT” does not fit our measured age based on a lower closure temperature that shows an increasing trend from south to north (Figures 7D, E), nor could it adequately explain the various slipping histories of the core-cover contact fault between the southern and northern portions. The core-cover contact fault around the Kangmar dome has been imaged as continuous and high-amplitude reflection events at relatively shallow depths along the INDEPTH seismic reflection profile (Nelson et al., 1996; Zhao et al., 1993). Liu et al. (2006) confirmed that the dip angle of the mid-crustal reflection formed by the Main Himalayan Thrust (MHT) increases progressively with its northward extension and that the MHT continues north of the Kangmar dome. The thrust stacking above the MHT detected by the most recent regional N‒S trending seismic profile (Li et al., 2021) between the Mabja dome and Kampa dome was interpreted as the cause of the doming event. However, the GKT was not observed at the corresponding depth in either seismic profile, and the STDS was identified at a depth of 3–3.5 km as a continuous interface overlying the high-velocity body and extending northward for a considerable distance (Figure 10D). Although the profile is located in a rift between the Mabja dome and the Kampa dome, where the STDS is not yet exposed, it is reasonable to assume that the crustal morphology it reflects is intermediate in the evolution of other domes. The “thrust stacks” at depths of 11–20 km, which are considered to control the formation of the Mabja dome, could also be transplanted to explain the cause of the Kangmar doming event (Figure 10B), and with the latest sensible application of channel flow reported by Chen et al. (2022), we further infer that the “thrust stack” in the lower-middle crust is related to the southward flowing channel flow.
FIGURE 10. Proposed model for the evolution of the Kangmar dome. (A) Top-down-to-N sliding related to the detachment of the STDS and the southward extrusion of the GHC; (B) doming expressed from local crustal thickening caused by stacked thrusts and the associated incision of the Nianchu River. Note that the detachment of the STDS persisted, and the YGR became active at some approximate later time. (C) Continued fast cooling due to glacier activity; (D) interpretation of the deep seismic reflection profile image by Li et al. (2021). R1-R5 are relatively high reflections. R1, R2, and R3 are parts of a thrust decollement, possibly the MCT. R4 represents the consequent doming, and R5 is interpreted to be the STDS shear zone. MCT, Main Central thrust; STDS, Southern Tibetan detachment system; THS, Tethys Himalaya Sequence; GHS, Grater Himalaya sequence; YGR, Yadong-Gulu rift.
Overall, the northward sliding of the THS related to the detachment of the STDS since ∼20 Ma resulted in the N-S-trending stretching lineation of the gneiss core and dominated the earlier uplift of the southern portion (Figure 10A). Note that the incision of the Nianchu River was always accompanied by the surface uplift of the dome. The doming event that occurred at ∼12.2 Ma was caused by the thrust stack, which was related to the southward flowing channel flow. Since the activities of the STDS located south of the Kangmar dome ceased before 11 Ma, the following uplifting of the dome might be associated with the N‒S trending Yadong-Gulu rift and its associated persistent thinning in the upper crust (Figure 10B), which caused the existence of E‒W extensional structures. The Pleistocene rapid cooling was attributed to enhanced glacial activity, and the incision of the Nianchu River formed the present Kangmar dome landscape (Figure 10C).
7 Conclusion
We present new (U-Th)/He and fission track data from two elevation transects across the Kangmar dome. Based on geological mapping and our new numerical modeling results, we demonstrate distinct cooling histories within the different portions of the Kangmar dome. We suggest that the core-cover contact fault was the northern continuation of the STDS exposed in the THS. We argue that the two phases of rapid cooling events during the Miocene and the Pleistocene resulted from regional extension structures and enhanced glacial activity, respectively. Combined with previous studies, we proposed a new model in which the development of the Kangmar dome was dominated by a thrust stack associated with the southward flowing channel flow, which challenges the previous models of southward thrusting along the GKT.
Data availability statement
The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding author.
Author contributions
ZM, ZH, and YL designed this study. ZM, ZH, and TX discussed. ZM, TX, and WZ contributed to the modeling. XH performed the channel steepness index analysis. ZM and ZH interpreted the data and wrote the manuscript. ZH, WB, and WZ contributed to sampling and testing. All authors contributed to the revision of the text.
Funding
This work was supported by the National Natural Science Foundation of China (Grant No. 42121002), the Second Tibetan Plateau Scientific Expedition and Research Program (STEP) (Grant No. 2019QZKK0204), the China Geological Survey (Grant No. DD20190057), and the Fundamental Research Funds for the Central Universities (Grant No. 35732020069).
Conflict of interest
The authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.
Publisher’s note
All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.
Supplementary material
The Supplementary Material for this article can be found online at: https://www.frontiersin.org/articles/10.3389/feart.2023.1186901/full#supplementary-material
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Keywords: southern Tibet, exhumation, low-temperature thermochronology, Pecube, Kangmar dome
Citation: Ma Z, Han Z, Li Y, Xu T, Han X, Bi W and Zhang W (2023) Late Cenozoic cooling and evolution history of the Kangmar dome in southern Tibet: Insights from inverse thermal modeling. Front. Earth Sci. 11:1186901. doi: 10.3389/feart.2023.1186901
Received: 15 March 2023; Accepted: 10 April 2023;
Published: 21 April 2023.
Edited by:
Xiaoming Shen, Ministry of Emergency Management, ChinaReviewed by:
Gaoyuan Sun, Hohai University, ChinaHanwen Dong, Chinese Academy of Geological Sciences (CAGS), China
Copyright © 2023 Ma, Han, Li, Xu, Han, Bi and Zhang. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
*Correspondence: Zhongpeng Han, hanzp@cugb.edu.cn