The Tibetan Plateau is a complex amalgamation of several microcontinents that consist of, from north to south, the Kunlun-Qaidam, Songpan-Ganzi-Hoh Xil, Qiangtang, and Lhasa terranes (Figure 1a). The latter two, together with their southern Himalayas are traditionally considered to have drifted northward from Gondwana in the south and to have successively accreted to the Paleo-Asian continent in the north along the Jinsha suture zone, Bangong-Nujiang suture zone, and Indus-Yarlung Tsangpo suture zone (IYSZ), representing Paleo-, Meso-, and Neo-Tethys oceanic relicts, respectively (Kapp & DeCelles, 2019;A. Yin & Harrison, 2000). Therefore, the evolution of the Paleo-, Meso-, and Neo-Tethys oceans, especially the Neo-Tethys Ocean, whose opening, subduction, and closure accompanied the final formation of the Himalayan orogen, plays a crucial role in understanding the tectonic evolution of the Himalayan thrust belt and the southern part of the Tibetan Plateau (Gehrels et al.