Based on 230 Th-238 U disequilibrium and major element data from mid-ocean ridge basalts (MORBs) and ocean island basalts (OIBs), this study calculates mantle melting parameters, and thereby investigates the origin of 230 Th excess. ( 230 Th/ 238 U) in global MORBs shows a positive correlation with Fe 8 , P o , Na 8 , and F melt (Fe 8 and Na 8 are FeO and Na 2 O contents respectively after correction for crustal fractionation relative to MgO = 8 wt%, P o =pressure of initial melting and F melt =degree of melt), while 230 Th excess in OIBs has no obvious correlation with either initial mantle melting depth or the average degree of mantle melting. Furthermore, compared with the MORBs, higher ( 230 Th/ 238 U) in OIBs actually corresponds to a lower melting degree. This suggests that the 230 Th excess in MORBs is controlled by mantle melting conditions, while the 230 Th excess in OIBs is more likely related to the deep garnet control. The vast majority of calculated initial melting pressures of MORBs with excess 230 Th are between 1.0 and 2.5 GPa, which is consistent with the conclusion from experiments in recent years that D U >D Th for Al-clinopyroxene at pressures of >1.0 GPa. The initial melting pressure of OIBs is 2.2-3.5 GPa (around the spinel-garnet transition zone), with their low excess 226 Ra compared to MORBs also suggesting a deeper mantle source. Accordingly, excess 230 Th in MORBs and OIBs may be formed respectively in the spinel and garnet stability field. In addition, there is no obvious correlation of K 2 O/TiO 2 with ( 230 Th/ 238 U) and initial melting pressure (P o ) of MORBs, so it is proposed that the melting depth producing excess 230 Th does not tap the spinel-garnet transition zone. OIBs and MORBs in both ( 230 Th/ 238 U) vs. K 2 O/TiO 2 and ( 230 Th/ 238 U) vs. P o plots fall in two distinct areas, indicating that the mineral phases which dominate their excess 230 Th are different. Ce/Yb-Ce curves of fast and slow ridge MORBs are similar, while, in comparison, the Ce/Yb-Ce curve for OIBs shows more influence from garnet. The mechanisms generating excess 230 Th in MORBs and OIBs are significantly different, with formation of excess 230 Th in the garnet zone only being suitable for OIBs. excess 230 Th, clinopyroxene, garnet, spinel-lherzolite, mid-ocean ridge, ocean island Citation:Zhang G L, Zeng Z G. Genesis of 230 Th excess in basalts from mid-ocean ridges and ocean islands: Constraints from the global U-series isotope database and major and rare earth element geochemistry.More than 20 years of uranium-series disequilibrium studies have shown that newly formed MORBs frequently display excess 230 Th (( 230 Th/ 238 U)>1) [1, 2]. Excess 230 Th is potentially important in the studies of magma formation depth and upwelling rate [3][4][5][6][7]. However, in the international community the cause of excess 230 Th has never been satisfactorily explained [8][9][10][11]. The partition coefficients of Th and U between melt and mantle residue are affected by pressure, temperature, porosity, oxygen fu...