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The angular momentum of the present Earth-Moon system could be acquired atthe collision of two identical rarefied condensations with sizes of Hillspheres which total mass was about 0.1 of the mass of the Earth. Solid embryosof the Earth and the Moon could be originated as a result of contraction of thecondensation formed at the collision. Depending on eccentricities ofplanetesimals that collided with solid embryos of the Earth and the Moon, theMoon could acquire 0.04-0.3 of its mass at the stage of accumulation of solidbodies while the mass of the growing Earth increased by a factor of ten.

Formation of embryos of the Earth-Moon system as a result of a collision of two rarefied condensations