March, 1907. Iron Meteorites — Farrington. 



99 



size of the grains in the granular members is generally less than 0.5 

 mm., rarely 0.75 mm. No granular structure is visible, even on strong 

 magnification, in the compact members. Chesterville and Rasgata are 

 rich in rhabdite. 



[:S, 



L'ndet. 



Total. 



100.00 

 100.04 

 100.46 



99-63 



100.41 



100.81 



99.62 



99.81 



99.42 



100.81 



100.38 



98.63 



100. II 



100.71 



Sp. Gr. 



7-33-7-77 

 7-654 



.'\nalyst. 



C. U. Shepard 



O. Sjostrom 



E. A. de Schweinitz 

 O. Sjostrom 



G. E. Lichtenberger 



E. Geinitz 



E.Cohen 



O. Sjostrom 



Rivero and Boussiiigault . . . . 



F.Wohler 



O. Sjostrom 



Reference 



1849, A. J. S. (2), VII, 449 



1897, Meteoreisen-Studien, V, A. N. H., XII, 



47 



1898, Meteoreisen-Studien, VIII, A. N. H., 

 XIV, 150 



1896, A. J. S. (4), I, 208-209 



1897, Ber. Berlin Akad., 386-396 



1897. Meteoreisen-Studien, VI, A. N. H., XII, m 

 1873, Sitz. Isis. p. 4, Dresden 

 1876, Neues Jahrb., 609 



1897, Meteoreisen-Studien, V, A. N. H., XII, 



42 

 1897, Meteoreisen-Studien, VI, A. N. H., XII, 



123 

 1824, Ann. Chem. Phys., XXV, 442-443 



1852, Ann. Chem. Pharm., LXXXII, 243-248 



1808, Meteoreisen-Studien, Vlll, A. .\. H., XIII, H3 



^OUP. 



Nedagolla group, but have an essentially higher nickel-cobalt content, 

 and thus form a transition to the nickel-rich ataxites. 



