The flux of cosmic matter on the Earth is ~40 000 ± 20 000 t per year. A main fraction of the flux is present by micrometeorites that are particles <1-2 mm in size. Cosmic spherules (CSs), scoriaceous, and unmelted micrometeorites are main micrometeorite types. According to the generally accepted aerodynamic model [2][3][4], CSs are formed from micrometeoroids, which were melted during high speed entry in the Earth' atmosphere.Transmission electron microscopy (TEM) study of silicate CSs with a cryptocrystalline texture collected in the area of the Tunguska event (Tunguska collection [5]) and extracted from glacier deposits of Novaya Zemlya (Novaya Zemlya collection [6]) allowed us to obtain new data on the microtextural patterns of spherules of this type. T3 2 spherule (Tungus collec tion) with a size of 130 × 200 µm (Fig. 1) has the fol lowing bulk chemical composition (wt %): SiO 2 48.9; TiO 2 0.08; Al 2 O 3 2.17; Cr 2 O 3 0.56; FeO 16.0; MnO 0.30; NiO 0.04; MgO 30.4; CaO 1.63; P 2 O 5 0.05 [5].TEM data show that the microtexture of the T3 2 spherule is characterized by olivine (Fo 76-79 ) crystals of the same sizes (~500 × 1000 nm) regularly distrib uted in glass of the following average bulk composition (wt %): SiO 2 67; FeO 7; MgO 3; CaO 5; Al 2 O 3 18 (Fig. 2). Crystals similarly oriented in silicate glass have elongation in the [100] direction and form paral lel chains along this direction demonstrating a texture of the "stone packing" type. Ends of the crystals have a round shape. Crystal faces are strongly decorated by gaseous inclusions demonstrating the effect of corroded faces (Fig. 2). The gaseous bubbles are ~30 nm in diameter. The microtexture of the sample from the Novaya Zemlya collection is amazingly similar to the microtexture of "stone packing" type observed in the T3 2 spherule from the Tunguska collection.The NZ8 bn4 25.9 spherule with a size of 100 × 70 µm is also composed of spatially ordered euhedral olivine (Fo 77 ) crystals with a size of 1-3 × 0.7-1 µm in a glass matrix (Fig. 3) saturated with gaseous bubbles (Fig. 4). The size of gaseous bubbles is 20-50 nm. The composition of glass is the following (wt %): SiO 2 61; Al 2 O 3 19-21; FeO 8-9; MgO 4-5; CaO 6. There are no clear microtextural differences between the central and peripheral parts of the T3 2 and NZ8 bn4 25.9 spherules. The modal abundance of the olivine crystals in glass is ~74%.The microtexture of the "stone packing" type have been not described anywhere, as it is known for the authors and it is observed for the first time; the texture differs from the "macroscopic" barred texture typical of silicate CSs and olivine chondrules in meteorites. In contrast to the barred "macrotexture," "stone pack 100 µm Fig. 1. Back scattered electron image of silicate cosmic spherule T3 2 (Tunguska collection). The cryptocrystal line silicate matrix (gray) contains a droplike metallic inclusion (white).GEOCHEMISTRY