An official website of the United States government
The Mongol-Okhotsk belt extends for more than 3000 km, from Mongolia to the Sea of Okhotsk in the northwest Pacific Ocean. It is the relict of the Mongol-Okhotsk ocean, a cryptic basin for which the timing, location and modes of opening and closure are still debated. One of the key components associated with the progressive closure and final collision and suturing of this ocean is the vast magmatic and volcanic record north and south of the presumed suture. Permian to Triassic magmatic and volcanic rocks are particularly abundant in the belt. They are characterized by bimodal volcanism, abundant calc-alkaline activity, secondary alkaline activity, and geochemical signatures that point to both volcanic-arc and within-plate origin as well as crustal and mantle sources. This has led to two main tectono-magmatic interpretations: (1) an Andean-style active margin modified by a mantle plume and/or affected by lithospheric delamination that evolved to a syn-and post-collisional setting, and (2) a mantle plume that recycled geochemical signatures from a long-lived active margin after the ocean was closed either by anatexis or by melting a remnant slab. These two models have first-order implications for the tectonic setting as well as for the location of the proposed mantle plume through time. We reconstruct the distribution of magmatic and volcanic provinces surrounding the Mongol-Okhotsk Suture Zone using G-Plates and the most recent paleomagnetic and mantle tomographic reconstructions to restore the position of the proposed mantle plume and the location of the slab between the Late Permian and Early Jurassic. Our reconstructions enable us to test the kinematic restoration and the viability of both the active subduction and the mantle plume models during the closure of the Mongol-Okhotsk Ocean.
more »
« less
This content will become publicly available on August 20, 2026
Oman was on the northern margin of a wide late Tonian Mozambique Ocean
Abstract The closure of the Mozambique Ocean defines the final assembly of the megacontinent Gondwana and is associated with a vast region of crustal growth in the Arabian-Nubian Shield. Despite this central paleogeographic position, there are few constraints on the position of terranes within and bounding the Mozambique Ocean. We report paleomagnetic data from ca. 726 Ma dikes exposed in southern Oman. Well-resolved magnetite magnetization is constrained to be primary by a conglomerate test on mafic clasts within overlying Cryogenian diamictite. The resulting paleomagnetic pole indicates that Oman was at a paleolatitude of 37 ± 2.5°N and was rotated ~80° counterclockwise from its present-day orientation. This position is consistent with Oman forming a contiguous plate with the India and South China cratons on the northern margin of the Mozambique Ocean in a distinct tectonic domain from Arabian-Nubian arcs to the south. This position reveals an ~5500-km-wide oceanic realm prior to subsequent closure that resulted in a major zone of Neoproterozoic crustal growth.
more »
« less
- Award ID(s):
- 2153786
- PAR ID:
- 10655578
- Publisher / Repository:
- Geological Society of America
- Date Published:
- Journal Name:
- Geology
- Volume:
- 53
- Issue:
- 11
- ISSN:
- 0091-7613
- Page Range / eLocation ID:
- 909 to 913
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
More Like this
-
-
Abstract The paleogeography of Laurentia throughout the Neoproterozoic is critical for reconstructing global paleogeography due to its central position in the supercontinent Rodinia. We develop a new paleomagnetic pole from red siltstones and fine‐grained sandstones of the early Neoproterozoic Jacobsville Formation which is now constrained to be ca. 990 Ma in age. High‐resolution thermal demagnetization experiments resolve detrital remanent magnetizations held by hematite. These directions were reoriented within siltstone intraclasts and pass intraformational conglomerate tests—giving confidence that the magnetization is detrital and primary. An inclination‐corrected mean paleomagnetic pole position for the Jacobsville Formation indicates that Laurentia's motion slowed down significantly following the onset of the Grenvillian orogeny. Prior rapid plate motion associated with closure of the Unimos Ocean between 1,110 and 1,090 Ma transitioned to slow drift of Laurentia across the equator in the late Mesoproterozoic to early Neoproterozoic. We interpret the distinct position of this well‐dated pole from those in the Grenville orogen that have been assigned a similar age to indicate that the ages of the poles associated with the Grenville Loop likely need to be revised to be younger due to prolonged exhumation.more » « less
-
ABSTRACT The ostreid genus Anomiostrea Habe & Kosuge, 1966, is monotypic for A. coralliophila Habe, 1975, which is known as a symbiont inhabiting the burrow of the ghost shrimp Neocallichirus jousseaumei (Nobili, 1904), but despite this unusual habit among oysters its phylogenetic position within the Ostreidae remained unknown. Using specimens collected from two distant localities of the Indo-Pacific, Oman and Japan, we compared shell morphology of these specimens with the holotype and assessed their phylogenetic relationships based on DNA sequence data from two mitochondrial and two nuclear genes. The genetic distance in cytochrome c oxidase subunit I between the specimens from Japan and Oman was 5.5%, indicating substantial geographic differentiation. Our molecular phylogenetic results suggest that A. coralliophila is sister to Ostrea algoensis G. B. Sowerby II, 1871, an oyster from rocky shores in South Africa, and both are closely related to other Ostrea species. This confirms assignment of Anomiostrea to Ostreinae and suggests that this burrow-wall symbiont evolved from typical rocky-shore oysters. Moreover, A. coralliophila was not monophyletic with another symbiotic ostreid Ostrea permollis G. B. Sowerby II, 1871, nor with other symbiotic oysters, indicating that the symbiotic habit evolved multiple times in the Ostreinae.more » « less
-
Abstract U–Pb ages, trace element content and oxygen isotope ratios of single zircons from five plagiogranite intrusions of the Troodos ophiolite were measured to determine their crystallization age and assess the importance of fractional crystallization versus crustal anatexis in their petrogenesis. The results indicate that oceanic magmatism in Troodos took place at 94·3 ± 0·5 Ma, about 3 Myr earlier than previously recognized. Later hydrothermal alteration has affected most of the Troodos plagiogranitic rocks, resulting in growth of new zircon and/or partial alteration of zircon domains, causing slightly younger apparent crystallization ages. The new age inferred for seafloor spreading and ocean crust accretion in Troodos nearly overlaps that of the Semail ophiolite in Oman (95–96 Ma), strengthening previous indications for simultaneous evolution of both ophiolites in similar tectonic settings. Average δ18O(Zrn) values in the Troodos plagiogranites range between 4·2 and 4·8 ‰. The lower values in this range are lower than those expected in equilibrium with mantle-derived melt (5·3 ± 0·6 ‰), indicating variable contribution from hydrothermally altered, deep-seated oceanic crust in most of the Troodos plagiogranite intrusions. The inferred substantial involvement of crustal component is consistent with the existence of a shallow axial magma chamber, typical of fast-spreading mid-ocean ridge settings, within the Troodos slow-spreading ridge environment. This apparent contradiction may be reconciled by episodically intense magmatism within an otherwise slow, magmatically deprived spreading axis.more » « less
-
Abstract Late Mesoproterozoic to Neoproterozoic sedimentary sequences within the Lake Superior region preserve critical paleogeographic records of the position of Laurentia spanning from the end of Midcontinent Rift extension through to the end of the Grenvillian Orogeny. Temporally calibrated paleomagnetic poles from these sequences are essential for resolving Laurentia's plate motion during these tectonic events. The 5 km thick ca. 1,080 to 1,045 Ma fluviolacustrine Oronto Group was deposited during thermal subsidence following rifting prior to onset of Grenvillian contractional deformation in the region. Prior paleomagnetic work has focused on the basal Freda Formation (ca. 1,075 Ma) leaving a long temporal gap in poles from that time until the ca. 990 Ma pole of the unconformably overlying Jacobsville Formation. A new U‐Pb detrital zircon maximum depositional age for the upper Freda Formation of 1,051.6 1.1 Ma indicates that Oronto Group deposition was prolonged. We have developed new inclination‐shallowing corrected paleomagnetic data from the Freda Formation that can be temporally calibrated within this improved chronostratigraphic framework. A new pole from the ca. 1,045 Ma upper Freda Formation is similar in position to that from the ca. 1,075 Ma lower Freda Formation. These data indicate that Laurentia's rapid motion of 20 cm/year from ca. 1,110 to 1,080 Ma significantly slowed to 2 cm/year following onset of the continent‐continent collision of the Grenvillian orogeny. These dynamics are what is predicted if the rapid motion was associated with differential plate tectonic motion that closed an ocean basin leading up to collisional orogenesis and the associated assembly of Rodinia.more » « less
