Dear All: yes, oceanic floor sediments are rich in Mn oxides, but also some basáltic flows. Usually these rocks are metamorphosed, so that the Mn-rich siliceous sediments become a Quartz-Mn-silicate rock called gondite in India. The basalt becomes Mn-rich amphibolite, but some other proceses should occur to these primary rocks in order to form deposits, such as tropical lateritization, which oxidises Mn-silicates with a low valence Mn-oxides (like braunite) to high valence oxides and hydroxides, like psilomelane and pyrolusite; this happened in the large Brazillian, Ghanan and Indian deposits. Instéad, in the huge Kalahari Manganese Fields, sedimentary Mn deposits suffered low grade metamorphism and hydrothermal alteration, and formed mixed valence oxides, like hausmannite, and hidrated silicates, like inesite. With higher metamorphism pyroxenoids like rodonite and pyroxmangite are formed, together with Mn-spinel (galaxite). In Venezuela some Archean gondites and amphibolites have formed small pyrolusite deposits, and some Proterozoic metabasalts too, Regards, Sebastián
The main process is pH- and Eh- driven. It is the process were the stability field of Mn oxy-hydrates get enlarged very much relative to the sister element bivalent Fe which is the case in alkaline conditions, e.g, on carbonate and basic rocks. Calcareous rock are poor in Mn but nevertheless they foster the separation of Fe from Mn and thereby favor the built-up of Mn depoists. In all cases Fe is too much predominating the chemical system and has a diluting effect Mn-bearing solutions.