METEORITES OF NORTH AMERICA. 467 



BIBLIOGRAPHY. 



1. I860: VELASCO. Noticias estadisticas del Estado de Sonora, etc., p. 221, Mexico, 1850. 



2. 1852: LECONTE. Proc. Amer. Aasoc. Adv. Sci., Sixth meeting, held at Albany, 1851, pp. 188-189. 



3. 1852: Notice of meteoric iron in the Mexican province of Sonora. Amer. Journ. Sci., 2d ser., vol. 13, pp. 289-290. 



4. 1854: BABTLETT. Personal narrative of explorations and incidents in Texas, New Mexico, California, Sonora, and 



Chihuahua, vol. 2, pp. 297-298, New York, 1854. 



5. 1854: SHEPARD. Notice of three ponderous masses of meteoric iron at Tucson, Sonora. Amer. Journ. Sci., 2d 



ser., vol. 18, pp. 369-372. 



6. 1855: SMITH. Memoir on meteorites. A description of five new meteoric irons, with some theoretical considera- 



tions on the origin of meteorites, based on their physical and chemical characters. Amer. Joum. Sci., 2d ser., 

 vol. 19, pp. 161-163. 



7. 1855: GENTH. Analysis of the meteoric iron from Tucson, Province of Sonora, Mexico. Amer. Journ. Sci., 2d ser., 



vol. 20, pp. 119-120. 



8. 1857: MICHLER. Report of the United States and Mexican Boundary Survey, vol. 1, part 1, p. 118. 



9. 1863: BRUSH. Meteoric iron from Tucson, Arizona. Amer. Joum. Sci., 2d ser., vol. 36, pp. 152-154 and 301. 



10. 1863: WHITNEY. On meteoric iron from Arizona. Proc. Calif. Acad. Nat. Sci., vol. 3, pp. 34-35 and 49. 



11. 1863: ROSE. Meteoriten, p. 150. 



12. 1863: IRWIN and AINSA. On the great Tucson meteorite. Rept. Smithsonian Inst., 1863, pp. 85-87. 



13. 1863: HENRY. [Report regarding history of above.] Idem, pp. 55-56. 



14. 1863: WHITNEY. Remarks on the nature and distribution of the meteorites which have, up to the present time, 



been discovered on the Pacific coast and in Mexico. Proc. Calif. Acad. Nat. Sci., vol. 3, pp. 240-241. 



15. 1863: HAIDINOEH. Das Carleton-Tucson-Meteoreisen im k. k. Hof-Mineralien-Cabinete. Sitzber. Wien. Akad., 



Bd. 48, II, pp. 301-308. 



16. 1865: HENRY. Rept. Smithsonian Inst., 1865, p. 67. 



17. 1869: MEUNIER. Recherches sur la composition et la structure de meteorites. Ann. Chim. Phys., 4th ser., 



vol. 17, pp. 53 and 68. 



18. 1870: HAIDINQER. Der Ainsa-Tucson-Meteoreisenring in Washington und die Rotation der Meteoriten in ihrem 



Zuge. Sitzber. Wien. Akad., Bd. 61, II, pp. 506-511. 



19. 1873: MEUNIER. Determination mineralogique des holosideres du Museum. Comptes Rend us, Tome 76, p. 



1281. 



20. 1884: MEUNIER. Meteorites, pp. 44 and 135. 



21. 1884: WADSWORTH. Lithological Studies, p. 69. , 



22. 1885: BREZINA. Wiener Sammlung, pp. 218 and 220-221.. 



23. 1890: FLETCHER. The meteoric iron of Tucson. Mineral. Mag., vol. 9. pp. 16-36. 



24. 1893: MEUNIER. Revision des fers m^tebriques, p. 36. 



25. 1895: COHEN. Meteoreisen-Studien IV, pp. 83 and 90. 



26. 1895: BHEZINA. Wiener Sammlung, pp. 295-296. 



27. 1896: FLETCHER. Introduction, p. 11. 



28. 1900: COHEN. Die beiden Meteoreisen von Los Muchachos, Tucson, Arizona, Festschrift 27-43, Greifswald 1900 



Mitth. Naturw. ver. von Xeu-Vorpommern und Rugen, 1900, vol. 32, pp. 25-43. 



29. 1905: COHEN. Meteoreitenkunde, Heft 3, pp. 86-100. 



Tulisca. See Tomatlan. 

 Turner Mound. See Anderson. 



UNION COUNTY. 



Georgia. 



Latitude 34 48' N., longitude 84 12' W. 



Iron. Coarsest octahedrite (Ogg) of Brezina; Nelsonite (type 5) of Meunier. 



Found 1853; described 1854. 



Weight, 6.8 kgs. (15 Ibs.). 



This meteorite was first described by Shepard, 1 who states that a piece weighing 1 pound 1.75 

 ounces was brought him from a mass said to weigh about 15 pounds, found in Union County, 

 Georgia. Shepard further describes his specimen as follows: 



It appears to have formed a portion of a somewhat tabular mass about 2 inches in thickness. It is coated on three 

 sides with a thin scaly covering of brownish-black hydrated peroxide of iron. The other two sides present the appear- 

 ance of a fresh fracture but are, nevertheless, destitute of metallic luster, the surfaces being very irregular and dependent 

 in form upon the peculiar concretionary character of the mass, which is strongly analogous to that of a very coarse- 



