Author/Authors :
Kohout، نويسنده , , Tom?? and Havrila، نويسنده , , Karol and T?th، نويسنده , , Juraj and Hus?rik، نويسنده , , Marek and Gritsevich، نويسنده , , Maria and Britt، نويسنده , , Daniel and Borovi?ka، نويسنده , , Ji?? and Spurn?، نويسنده , , Pavel and Igaz، نويسنده , , Antal and Svore?، نويسنده , , J?n and Korno?، نويسنده , , Leonard and Vere?، نويسنده , , Peter and Koza، نويسنده , , J?lius and Zigo، نويسنده , , Pavol and Gajdo?، نويسنده , , ?tefan and Vil?gi، نويسنده , , Jozef and ?apek، نويسنده , , David and Kri?andov?، نويسنده , , Zuzana and Tomko، نويسنده , , Du?an and ?ilha، نويسنده , , Ji?? and Schunov?، نويسنده , , Eva and Bodn?rov?، نويسنده , , Marcela and B?zov?، نويسنده , , Diana and Krej?ov?، نويسنده , , Tereza، نويسنده ,
Abstract :
Bulk and grain densities, porosities, and magnetic susceptibilities of 67 individuals of Košice H chondrite fall were measured. The mean bulk and grain densities were determined to be 3.43 g/cm3 with standard deviation (s.d.) of 0.11 g/cm3 and 3.79 g/cm3 with s.d. 0.07 g/cm3, respectively. Porosity is in the range from 4.2% to 16.1%. The logarithm of the apparent magnetic susceptibility (in 10−9 m3/kg) shows narrow distribution from 5.17 to 5.49 with mean value at 5.35 with s.d. 0.08.
results indicate that all studied Košice meteorites are of the same composition down to ~g scale without the presence of foreign (non-H) clasts and are similar to other H chondrites. Košice is thus a homogeneous meteorite fall derived from a homogeneous meteoroid.
