A set of four stratospheric particles was reanalysed. These particles
registered in the NASA Cosmic Dust Catalogs (CDCs) were classified in
the Houston Johnson Space Center (JSC) as the particles of cosmic orig
in (''C''). Present energy-dispersive X-ray (EDX) spectra confirmed pr
evious classification and revealed additional features in the chemical
composition of the cosmic dust particles. The particles are extremely
fine-grained aggregates with bulk chondritic composition. Somewhat hi
gher content of oxygen may indicate a presence of hydroxide containing
minerals in their phase composition.