Abstract

The Chiron Basin extends along the southern periphery of the Siberian Craton and the western margin of the Mongol–Okhotsk Belt. Here, we present whole-rock geochemical data (major and trace elements and Sm–Nd isotopes) along with zircon U–Pb geochronology and Lu–Hf isotopic data from Paleozoic sedimentary rocks within the Chiron Basin to investigate their provenance and tectonic history. εNd(t) values of the siliciclastics rocks of the Khara–Shibir, Shazagaitui, and Zhipkhoshi formations vary from −17.8 to −6.6, with corresponding two-stage Nd model ages (tNd(C)) ranging from 2.56 to 1.65 Ga. Detrital zircon grains from these rocks are predominantly Archean, Paleoproterozoic, and Carboniferous–Devonian in age. The data suggest that the southern flank of the Siberian Craton is the only viable source area for Archean and Paleoproterozoic zircon grains with Hf model ages (tHf(C)) of >2.20 Ga. The majority of zircon grains from sandstones from the Khara–Shibir, Shazagaitui, and Zhipkhoshi formations are Devonian–Carboniferous in age. With respect to their Hf model ages, the zircon grains can be subdivided into two groups. The first group of Devonian–Carboniferous zircon grains is characterized by relatively old (mainly Paleoproterozoic) tHf(C) model ages of 2.25–1.70 Ga and the source was the southern margin of the Siberian Craton. The second group of Devonian–Carboniferous zircon grains is characterized by significantly younger (mainly Neoproterozoic) tHf(C) model ages of 1.35–0.36 Ga, which are consistent with a juvenile source, most likely eroded island arcs. Our data, show that sedimentary rocks of the Chiron Basin likely formed in a back-arc basin on the southern periphery of the Siberian Craton facing the Paleozoic Mongol–Okhotsk Ocean.

Highlights

  • The Mongol–Okhotsk Belt is one of the major structural elements of East Asia and probably represents the youngest orogenic component within the collage of Central Asian orogenic belts ([1,2,3]Minerals 2020, 10, 279; doi:10.3390/min10030279 www.mdpi.com/journal/mineralsMinerals 2020, 10, 279 and references therein)

  • Paleoproterozoic) tHf(C) model ages of 2.25–1.70 Ga and the source was the southern margin of the Siberian Craton

  • The second group of Devonian–Carboniferous zircon grains is characterized by significantly younger tHf(C) model ages of 1.35–0.36 Ga, which are consistent with a juvenile source, most likely eroded island arcs

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Summary

Introduction

The Mongol–Okhotsk Belt is one of the major structural elements of East Asia and probably represents the youngest orogenic component within the collage of Central Asian orogenic belts Minerals 2020, 10, 279 and references therein). This NE–SW-oriented belt is located in northern Mongolia and Transbaikalia (Russia) and extends for over 3000 km from central Mongolia to Uda Bay in the Okhotsk Sea (Figure 1). Numbers in circles are structures (terranes, microcontinents, cratonic blocks): (1) Anga–Talanchan; (2) Baidarik; (3) Baikal–Muya; (4) Barguzin; (5) Bayan–Khongor; (6). The Mongol–Okhotsk Belt is generally considered ([2,3,11,12,13] and references therein) to represent a remnant of the Mongol–Okhotsk Ocean, which closed owing to collision between the Siberian Craton and the Amuria Block (superterrane or microcontinent). Many aspects of the evolution of this structure from ocean to suture zone remain unresolved

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