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[Display omitted] • The Taga area of the Tethyan Himalaya was located at 54.7° ± 12.0°S at ca. 147–140 Ma. • The eruption periods of the Comei igneous rocks are similar to the Bunbury basalt. • The paleolatitudes of the Comei-Bunbury LIP are similar to the Kerguelen mantle plume. • The Comei-Bunbury LIP originated from the Kerguelen mantle plume. The causal link between the Comei-Bunbury large igneous province (CBLIP) and the Kerguelen mantle plume (KMP) remains a topic of debate. Here, a new paleomagnetic study was conducted on the Zhela Formation basalts and sandstones (ca. 147–140 Ma) in the Taga area of the eastern Tethyan Himalaya (TH). The sandstone specimens had erratic demagnetization patterns, and reliable characteristic remanent magnetization (ChRM) directions could not be isolated. Positive fold and reversal tests indicate that the ChRM directions of the Zhela Formation basalts should be the primary magnetization. The tilt-corrected site-mean direction from 18 sites is D/I = 87.8°/70.0° (α 95 = 6.8°), yielded a paleopole of 21.6°N/130.2°E (A 95 = 12.0°) and a paleolatitude of 54.7° ± 12.0°S for the study area (28.4°N, 91.8°E). Comparison with robust latest Jurassic and Early Cretaceous paleomagnetic, geochemical, and geochronological data from the eastern TH, northeastern Indian craton, and southwestern Australia reveal that (1) the eruption periods of the Comei igneous rocks are similar to the Bunbury basalt (and the Naturaliste Plateau volcanic rocks); (2) the original erupted positions of the Comei-Bunbury (CB) igneous rocks were in agreement with the reconstructed KMP; and (3) the CBLIP originated from the KMP. [ABSTRACT FROM AUTHOR]

The paleogeography of the Tethyan Himalaya (TH) during the Mesozoic is vital to constrain the evolutionary history of the Neo‐Tethys Ocean, but reliable paleomagnetic data from Jurassic rocks in this area are scarce. Here, we report the first high‐quality paleomagnetic results from the Middle Jurassic (∼175–173 Ma) Lanongla Formation limestones in the Nyalam area of the TH. For most specimens, stepwise thermal or hybrid demagnetization reveals two well‐defined magnetization components. A low‐temperature component, which is isolated between natural remanent magnetization and 200–300°C, is consistent with the present geomagnetic field direction. A high‐temperature component, which is isolated between 300–350°C/10–25 mT and 500–580°C/60–120 mT, passes fold tests at the 95% and 99% confidence level, indicating a prefolding primary magnetization. The tilt‐corrected site‐mean direction for 28 paleomagnetic sites is Ds = 331.0° and Is = −49.9° with α95 = 2.7°, which provides a Fisherian site‐mean paleopole at 23.7°N, 292.9°E with A95 = 2.8° and a paleolatitude of 31.7 ± 2.8°S for the Nyalam study area (28.6°N, 86.1°E). A comparison between the reliable Middle Jurassic‐Early Cretaceous poles obtained from the TH and those observed from the Lhasa terrane reveals that the Neo‐Tethys Ocean for the reference point (29.1°N, 86.1°E) had a latitudinal width of 3,500 ± 1,000 km at ∼174 Ma, reached its greatest width of 7,000 ± 1,000 km at ∼137 Ma, and had an average latitudinal spreading rate of ∼10.4 cm/year during ∼174–137 Ma. Plain Language Summary: The Neo‐Tethys Ocean here refers to the prehistoric ocean that existed between the Lhasa terrane to the north and the Indian plate to the south during the much of the Mesozoic and early Cenozoic. Knowledge of the development of the Neo‐Tethys Ocean is crucial to understanding the evolution of the Himalayas and Tibetan Plateau. However, the opening of the Neo‐Tethys Ocean remains controversial. In this work, we report what we consider is the first high‐quality Middle Jurassic age paleopole from the Tethyan Himalaya, which shows that the Nyalam area was located at 31.7 ± 2.8°S at ∼174 Ma and that the Neo‐Tethys Ocean was at least ∼3,500 km wide in a N–S direction at that time. Key Points: The Nyalam area of the Tethyan Himalaya (TH) was located at 31.7 ± 2.8°S at ∼174 MaThe Neo‐Tethys Ocean opened a latitudinal width of ∼3,500 km at ∼174 Ma and reached its greatest width of ∼7,000 km at ∼137 MaThe Neo‐Tethys Ocean had an average latitudinal spreading rate of ∼10.4 cm/year during ∼174–137 Ma [ABSTRACT FROM AUTHOR]

The timing and location India–Asia collision is crucial to understanding the evolution of the Himalayan–Tibetan orogen and global climate change; however, estimates of the timing of the India–Asia collision and the size of Greater India remain highly controversial. We report here the first reliable early Eocene paleomagnetic results from the Zhepure Formation limestone in the Tethyan Himalaya (TH). Both positive fold and reversal tests indicate a primary origin. The tilt‐corrected site‐mean direction is Ds = 332.6°, Is = 20.1°, ks = 90.9, α95 = 2.8° (N = 30). The site‐mean inclination increased from 20.1° to 27.5° after inclination shallowing correction, yielding a paleopole at 61.2°N, 337.3°E, A95 = 2.6° and a corresponding paleolatitude of 15.2° ± 2.6°N for the reference point (29.5°N, 91.0°E). Our new paleomagnetic results, together with the reliable Cretaceous to Paleogene paleomagnetic results from the TH, Lhasa terrane and Indian craton, suggest that there was ∼900–1,140 km north‐south crustal shortening occurred between the TH and the Indian craton, and that India collided with Asia at no later than ∼51–49.5 Ma. Plain Language Summary: The India–Asia collision is among the most intriguing topics in earth sciences because of its influence on global climate and Cenozoic topography. However, several questions still remain unanswered, such as: how big was Greater India? When, where, and how did the India collide with Asia? We report the first reliable early Eocene paleopole from the TH and assess the timing of the India–Asia collision and the size of Greater India. Our results suggest a relatively small Greater India, and that India collided with Asia at no later than ∼51–49.5 Ma. The constraints on the India–Asia collision indicated by our data provide new boundary conditions for the history of the Himalayan–Tibetan orogen and global climate change. Key Points: The Tethyan Himalaya (TH) was located at 15.2° ± 2.6°N at ∼51–49.5 MaThere was ∼900–1,140 km north‐south crustal shortening occurred between the TH and the Indian cratonIndia collided with Asia at no later than ∼51–49.5 Ma [ABSTRACT FROM AUTHOR]

In this manuscript, we checked all the pieces of evidence separately and conclude that the evidence Zhao et al. (2021, https://doi.org/10.1029/2020TC006520) provided cannot be regarded as arguments supporting their points. Our observations show that (i) sampling units and depositional environment support that the Jingzhushan Formation red beds could be affected by the syntectonic sedimentation, (ii) characteristic remanent magnetization directions observed from the Jingzhushan Formation red beds represent primary magnetization acquired during the syntectonic sedimentation, not secondary remagnetization due to strain reorientation of remanence, and (iii) inclination discrepancy of the Jingzhushan Formation red beds could be attributed to syntectonic sedimentation. Therefore, the paleomagnetic results obtained from the Jingzhushan Formation red beds are reliable for paleogeographic reconstructions. Key Points: Characteristic remanent magnetization directions observed from the Jingzhushan Formation red beds represent primary magnetizationPaleomagnetic data obtained from two limbs of the folded Jingzhushan Formation red beds are reliable for paleogeographic reconstructionsSyntectonic sedimentation is a reasonable interpretation for the inclination discrepancy of the Jingzhushan Formation red beds [ABSTRACT FROM AUTHOR]

The precollisional locations and geometries of the Lhasa terrane (LT) are critical to constrain the India‐Asia collision. However, the inclinations of the Cretaceous paleomagnetic data obtained from the northern limb of folds are obviously lower than those obtained from the southern limb, which cause large discrepant paleolatitudes of the LT prior to India‐Asia collision. Here, we carried out a new paleomagnetic investigation on the Late Cretaceous Jingzhushan Formation red beds in the far western LT. The tilt‐corrected site mean direction yielded a palaeopole at 74.4°N, 226.0°E with A95 = 3.8° (N = 54). This paleomagnetic data set passes fold tests and indicates that the studied area was located at 19.6° ± 3.8°N during the Late Cretaceous. However, the mean inclination calculated from the northern limb of folds (Is = 19.0°) is significantly lower than that of the southern limb of folds (Is = 51.8°). This inclination discrepancy of the Jingzhushan Formation red beds may be attributed to the syntectonic sedimentation. Nevertheless, the site mean direction obtained from both limbs of folds is generally consistent with the site mean direction after syntectonic‐sedimentation correction. Our new paleomagnetic results, combined with the reliable Cretaceous paleomagnetic results from the LT showed that the southern margin of Asia had a present‐day relatively east‐west alignment prior to India‐Asia collision. Key Points: A new paleopole (74.4°N, 226.0°E with A95 = 3.8°) was obtained from the Jingzhushan Formation red beds in the far western Lhasa terraneInclination discrepancy of the Jingzhushan Formation red beds may be attributed to the syntectonic sedimentationThe southern margin of Asia had a present‐day relatively east‐west alignment prior to India‐Asia collision [ABSTRACT FROM AUTHOR]

The precollisional paleolatitude of the Tethyan Himalaya is essential to constrain the India‐Asia collision, the size of Greater India, and the Neotethyan paleogeography. However, reliable Late Cretaceous‐Paleocene paleomagnetic datasets are still scarce because of serious remagnetization. Here we report the first redbed‐based paleomagnetic results from the Paleocene (60‐58 Ma) redbeds in the Saga area of the northern Tethyan Himalaya. The tilt‐corrected site‐mean direction obtained from 36 paleomagnetic sites is D=178.7°, I=9.5° with ɑ95=5.4°, corresponding to a paleopole at 55.9°N, 267.6°E with dp/dm=2.8°/5.5° and a paleolatitude of 4.8°±2.8°S for the study area (29.3°N, 85.3°E). The site‐mean inclination increased from 9.5 to 14.9° after the anisotropy‐based inclination shallowing correction, leading to corresponding paleolatitudes increasing from 4.8 to 7.6°S. This reliable paleomagnetic dataset passes positive fold tests and supports that the northern Tethyan Himalaya was located at 6.3±4.3°S during 60‐58 Ma. Comparison with the coeval paleolatitudes expected from the Indian craton indicates that a north‐south crustal shortening of 3.1±5.5° (340±610 km) occurred between the Indian craton and the northern Tethyan Himalaya after 59 Ma, and no wide ocean extended between them after the Latest Jurassic. Our new Paleocene results together with reliable Cretaceous paleomagnetic results from the Lhasa terrane show that the India‐Asia collision occurred at 47.1±4.5 Ma. Key Points: The Saga area of the northern Tethyan Himalaya at ~59 Ma lay at 6.3°±4.3°SNeither wide Ocean extension nor >1,000 km crustal shortening occurred between Indian craton and Tethyan Himalaya after the latest JurassicThe India‐Asia collision occurred at 47.1±4.5 Ma [ABSTRACT FROM AUTHOR]

The breakup of eastern Gondwana is among the hottest topics in the Earth sciences because of its effect on global climate during the Jurassic‐Cretaceous, its influence on the evolution of life, and its importance to paleogeographic reconstruction. To better constrain the Jurassic and Cretaceous paleogeographic position of the Tethyan Himalaya and the breakup of eastern Gondwana, a combined paleomagnetic and geochronological study was performed on the Zhela and Weimei Formations lava flows, dated at ~138–135 Ma, in the Luozha area of the eastern Tethyan Himalaya. Both positive fold and reversal tests together with a maximum grouping at 100% unfolding indicate that the characteristic remanent magnetization directions are primary magnetizations acquired before folding. The tilt‐corrected directions yielded a paleopole at 0.9°N, 293.4°E with A95 = 7.0° and a corresponding paleolatitude of 53.5°S ± 7.0°S for the Luozha sampling area (28.9°N, 91.3°E), validating that the original erupted position of the Zhela and Weimei Formations lava flows was located in the center of the Kerguelen mantle plume. Our new results, together with the published paleomagnetic, geochronological, and geochemical results, demonstrate that the Comei‐Bunbury large igneous province originated from the Kerguelen mantle plume. The temporal and spatial relationships between the Comei‐Bunbury large igneous province and the Kerguelen mantle plume indicate that eastern Gondwana initially rifted at ~147 Ma and that the Indian Plate fully separated from the Australian‐Antarctic Plate before ~124 Ma. Key Points: The Luozha sampling area was located at ~53.5 degrees south plus‐minus 7.0 degrees south at ~138‐135 MaThe Comei‐Bunbury large igneous province (LIP) originated from the Kerguelen mantle plumeEastern Gondwana initially rifted at ~147 Ma, and the Indian Plate fully separated from the Australian‐Antarctic Plate before ~124 Ma [ABSTRACT FROM AUTHOR]

The timing of the north‐south collision between two terranes can be determined by the overlap of their paleolatitudes or the change of their convergence rate. For example, the overlapping paleolatitudes of the Lhasa terrane and Tethyan Himalaya and the dramatic decrease in the velocity of the Indian plate are usually ascribed to the India‐Asia collision at ~55 Ma. However, little is known about the paleolatitudinal evolution and velocity change of the Lhasa terrane resulting from the Lhasa‐Qiangtang collision during the Jurassic‐Cretaceous period. To better constrain the velocity change of the Lhasa terrane during this period, to constrain when and where the Lhasa‐Qiangtang collision occurred, and to assess the distribution of land and sea in the Tethyan realm, we provide a high‐quality Cretaceous paleomagnetic pole obtained from the limestone from the western part of the Lhasa terrane, which yields a paleolatitude of ~16.8° ± 1.9°N for the sampling area (32.2°N, 80.8°E) during the time interval of ~113–72 Ma. We compile existing paleomagnetic results from the Lhasa terrane, Qiangtang terrane, Tethyan Himalaya, and India and reveal that the Lhasa‐Qiangtang collision most likely occurred at or near the J/K boundary at ~19°N for the reference point at (32°N, 88°E) and that the Neo‐Tethys reached its maximum width (≥~7450 km) during this period. Key Points: The Shiquanhe sampling area was located at ~16.8° ± 1.9°N at ~113‐72 MaThe Lhasa‐Qiangtang collision most likely occurred at ~19°N at or near the J/K boundaryThe Neo‐Tethys reached its maximum width (≥~7450 km) during this period [ABSTRACT FROM AUTHOR]

This work presents zircon U-Pb age and whole-rock geochemical data for the volcanic rocks from the Lakang Formation in the southeastern Tethyan Himalaya and represents the initial activity of the Kerguelen mantle plume. SHRIMP U-Pb dating of zircons from the volcanic rocks yielded a 206Pb/238U age of 147 ± 2 Ma that reflects the time of Late Jurassic magmatism. Whole rock analyses of major and trace elements show that the volcanic rocks are characterized by high content of TiO2 (2.62 wt%-4.25 wt%) and P2O5 (0.38 wt%-0.68 wt%), highly fractionated in LREE/HREE [(La/Yb)N = 5.35-8.31] with no obvious anomaly of Eu, and HFSE enrichment with no obvious anomaly of Nb and Ta, which are similar to those of ocean island basalts and tholeiitic basaltic andesites indicating a mantle plume origin. The Kerguelen mantle plume produced a massive amount of magmatic rocks from Early Cretaceous to the present, which widely dispersed from their original localities of emplacement due to the changing motions of the Antarctic, Australian, and Indian plates. However, our new geochronological and geochemical results indicate that the Kerguelen mantle plume started from the Late Jurassic. Furthermore, we suggest that the Kerguelen mantle plume may played a significant role in the breakup of eastern Gondwanaland according to the available geochronological, geochemical and paleomagnetic data. [ABSTRACT FROM AUTHOR]

To position the Asian southern margin before the India-Asia collision, paleomagnetic and geochronologic studies were performed on the Dianzhong Formation lava flows from the Shiquanhe area of the westernmost Lhasa terrane (LT). Zircon U-Pb analyses dated the lava flows to ~69.5 ± 2.5 Ma. The characteristic remanent magnetization directions contain antipodal polarities and pass fold tests, implying that they are primary magnetizations; this interpretation is supported by rock-magnetic analyses and petrographic observations. Forty-four site-mean directions were divided into 17 statistically independent direction groups. The group-mean direction after tilt correction is Ds = 43.3°, Is = 30.3°, k = 28.0, α95 = 6.9°. The corresponding paleopole at 47.8°N, 181.4°E ( A95 = 6.4°) yields a paleolatitude of 16.6° ± 6.4°N for the Shiquanhe area of westernmost Tibet (32.34°N, 80.12°E). Consistent paleolatitudes for the southern margin of the LT calculated from the western and central part of the LT indicate that the leading edge of the LT was aligned relatively W-E. When compared with the reference pole at 70 Ma for Eurasia, this new paleopole suggests that crustal shortening between the Shiquanhe area and stable Asia was 1,500 ± 800 km. This is supported by the crustal shortening (600-1,000 km) absorbed by Cenozoic thrust and fold belts within this area, indicating that the magnitude of crustal shortening within Asia north of the India-Asia suture zone was similar in the central and western part of the plateau. [ABSTRACT FROM AUTHOR]

The evolution of the Neo-Tethys Ocean had a profound effect on global climate change and the evolution of life. To better constrain the Cretaceous paleogeographic position of the Tethyan Himalaya and evolution of the Neo-Tethys Ocean, combined paleomagnetic and detrital zircon U Pb geochronological research was performed on samples from the Gyabula Formation, constrained at ca. 117.7–94.4 Ma, in the Zhongba area of the northern Tethyan Himalaya. Both positive fold and reversal tests combined with a maximum grouping at 106% unfolding indicate that the high-temperature component directions were acquired before folding and were most likely of primary origin. The tilt-corrected directions yielded a paleopole at 29.2°N, 280.5°E with A 95 = 5.1° and a corresponding paleolatitude of −29.0° ± 5.1°N for the sampled area (29.7°N, 84.0°E). No significant inclination shallowing was identified from the sampled cherts. Comparison of the observed paleolatitude with those expected from the Indian craton indicated that an 840 ± 670 km north-south distance existed between the northern Tethyan Himalaya and the Indian craton for the reference point (29.7°N, 84.0°E). Because of the anticlockwise rotation of the Indian craton, this amounts to a crustal extent of 1130 ± 900 km at ca. 106 Ma, which represents the amount of north-south crustal shortening. Our new results, together with reliable Cretaceous paleomagnetic data obtained from the Tethyan Himalaya, indicate that no wide oceanic basin extended between the Tethyan Himalaya and Indian craton at ca. 106–75 Ma and that there was still a contiguous Indian subcontinent. • The Zhongba area of the northern Tethyan Himalaya (TH) was located at 29.0° ± 5.1°S at ca. 117.7–94.4 Ma • 1130 ± 900 km of north-south shortening occurred between the northern Tethyan Himalaya and the Indian craton • No wide oceanic basin extended between the TH and the Indian craton at ca. 106–75 Ma [ABSTRACT FROM AUTHOR]

To further constrain the India–Asia collisional process, a combined paleomagnetic and geochronologic study has been carried out on the Upper Cretaceous Jingzhushan Formation redbeds and the Lower Cretaceous Dianzhong Formation volcanic rocks dated at ~ 121–117 Ma from the Cuoqin area in the central Lhasa terrane. Stepwise thermal demagnetization successfully isolated reliable characteristic remanent magnetization (ChRM) directions that include dual polarity and pass positive fold tests at 95% and 99% confidence levels, indicating prefolding primary magnetizations. The tilt-corrected site-mean direction for 33 redbed sites is D = 316.8°, I = 30.2° with α 95 = 5.4°, corresponding to a paleopole at 49.0°N, 344.3°E with A 95 = 5.3°, and the other for 12 volcanic sites is D = 350.5°, I = 25.5° with α 95 = 7.7°, corresponding to a paleopole at 70.5°N, 292.9°E with A 95 = 7.4°. Our new paleomagnetic results, together with reliable Cretaceous paleomagnetic data obtained from the Lhasa terrane, demonstrate that the southern margin of Asia was located at ~ 15.1°N during the Cretaceous. Comparison with the apparent polar wander paths (APWP) of India and the Cretaceous–Paleocene paleopoles of the Himalayan terrane suggests that the India–Asia collision was likely a complex process, which consists of the collision of the Lhasa and Himalayan terranes at 54.0 ± 2.1 Ma, the longtime subduction of an intra-oceanic basin between the Himalayan terrane and the Indian craton from ~ 54.0 to ~ 40.4 Ma, and the collision of the Himalayan terrane and the Indian craton at 40.4 ± 4.1 Ma. Comparing with the Late Cretaceous average pole of the East Asia APWP reveals that a latitudinal convergence of 780 ± 240 km has taken place between the Lhasa terrane and East Asia (the Hexi corridor) since the India–Asia collision; the amount of latitudinal shortening deduced from paleomagnetic data is very consistent with the 600–1000 km accommodated by the Cenozoic fold and thrust belts between the Lhasa terrane and Hexi corridor. [ABSTRACT FROM AUTHOR]

To better constrain the Early Cretaceous paleogeographic position of the Tethyan Himalaya and the India–Asia collision process, a paleomagnetic study was performed on the Lakang Formation lava flows in the Cuona area in the southeastern Tethyan Himalaya. Stepwise thermal and alternating field demagnetizations successfully isolated reliable characteristic remanent magnetization (ChRM) directions that include antipodal dual polarities and pass positive fold tests at the 99% confidence level and reversal tests at 95% confidence level, indicating prefolding primary magnetizations. The distribution patterns of ChRM directions from the Lakang Formation lava flows are consistent with young lava flows at similar latitudes, suggesting that secular variation has likely been averaged out. The tilt-corrected site-mean direction for 31 sites is D = 261.6 ° , I = − 68.5 ° with α 95 = 3.6 ° , which provides a paleopole at 26.8°S, 315.2°E ( A 95 = 5.7 ° ), corresponding to a paleolatitude of 52.2 ° ± 5.7 ° S for the study area. Comparison of the paleolatitude observed from the Lakang Formation lava flows with that expected from the apparent polar wander paths of India at 130 Ma show a paleolatitude difference of ∼2.1° (∼230 km), indicating that neither a great north-south continental crustal shortening occurred between the Indian craton and the Tethyan Himalaya after 130 Ma, nor that a wide ocean separated them at that time. Comparison with reliable Cretaceous–Paleocene paleomagnetic results observed from the Tethyan Himalaya and the Lhasa terrane indicates that the latitudinal width of the Neo-Tethyan Ocean could have been up to ∼7000 km at 134–130 Ma and an extension should have existed between the Indian craton and the Tethyan Himalaya during the Late Cretaceous and Paleocene. Furthermore, reliable paleomagnetic results suggest that the India–Asia collision was a dual-collision process, consisting of a first collision of the Tethyan Himalaya with the Lhasa terrane (Asia) at 54.9 ± 2.3 Ma and a final continent–continent collision of the Indian craton with the Tethyan Himalaya at 40.0 ± 3.3 Ma . [ABSTRACT FROM AUTHOR]