... The chemical composition of four Fe-Mn nodules (Si, Al, Ca, Fe, K, Mg, Mn, Na, P, Ti, Li, Be, Sc, V, Cr, Co, Ni, Cu, Zn, Ga, Ge, As, Se, Rb, Sr, Y, Zr, Nb, Mo, Ag, Cd, Sb, Cs, Ba, REE, Hf, Ta, W, Tl, Pb, Th, and U) were determined by inductively coupled plasma mass-spectrometry (ICP-MS) using Agilent 7700x (Agilent Technologies) and by inductively coupled plasma atomic emission spectroscopy with iCAP6500 Duo (ThermoScientific) in the laboratory of Far East Geological Institute in Vladivostok. Rare Earth Element and Yttrium (REY) distribution plots were used for studying Fe-Mn deposit genesis and were normalized to shale (PAAS, Post-Archean Australian Shale) [57]. The Ce anomaly was calculated as Ce* = 2Ce/(La + Pr) for PAAS-normalized values. ...