We report the first systematic study of different textural varieties of olivine (olivine from peridotite xenoliths, macrocryst type Ol I, and phenocryst type zoned Ol II) from two diamondiferous kimberlite pipes of the Arkhangelsk diamond province (V. Grib and Pionerskaya) differing in geologic setting, geochem ical and isotopic characteristics, and diamond content. Approximately 550 olivine analyses were obtained by the EPMA technique using the precise method of Sobolev et al. (2007) adapted at the Institute of Geology of Ore Deposits, Petrography, Mineralogy, and Geochemistry (IGEM), Russian Academy of Sciences . Olivines from the V. Grib moderate Ti kimberlites, which are similar to Group I kimberlites in geochemical and Sr-Nd isotopic characteristics and rich in diamond, are dominated by high Mg# low Ti Ol I formed owing to the fractional crystallization of a carbonate rich protokimberlite melt interacting with orthopyroxene bearing peridotite material; the fraction of high Ti Ol I produced by the metasomatic alter ation of peridotite under the influence of silicate aqueous fluids is significantly lower; and xenocrysts weakly affected by metasomatic agents (melts and fluids) occur in minor amounts. Olivines from the low Ti Pioner skaya kimberlites, which are similar to Group II kimberlites in geochemical and Sr-Nd isotopic character istics and show a moderate diamond content, are dominated by high Ti Ol I, and xenocrysts weakly affected by metasomatic agents are also abundant. In the kimberlites of both pipes, the cores of Ol II crystals are usu ally composed of low Ti olivine similar in composition to Ol I; both high Ti and low Ti olivine cores occur in the Pionerskaya pipe; whereas cores corresponding to high Ti Ol I were never found in the V. Grib pipe. The outer zones of olivine and small olivine grains in the groundmass show considerable variations in minor element contents within a narrow Mg# range. It is suggested that the high Ti rims of Ol II from the V. Grib and Pionerskaya kimberlites were produced by the late crystallization of kimberlite melt, and the low Ti rims on the outer zones of Ol II in the Pionerskaya kimberlites were formed by late stage equilibration with an aqueous fluid separated from the kimberlite melt and/or possible kinetic effects. Our study revealed the diver sity of olivine origin in the kimberlites and showed that there is no single mechanism of olivine formation.