Sample No. 4 from the Burns Mountain long crosscut represents pyrite from the Perkins set of veins at a depth of about 275 feet beneath the surface. It was treated in exactly the same manner as No. 5. In it, however, the finenesses of the +60- and -++100-mesh gold flakes check reasonably closely, averaging about 890 parts gold per thousand. Also there is a reasonably close correspondence between the metallics and the average of five determinations of the fineness of the gold in the —100-mesh pyrite pulp of 870+30 parts per thousand. Further investigation of the variation in the fineness of the lode gold from the main Perkins vein was impossible because of the absence of reliable specimen material. That the fineness of gold from an individual vein and even from an individual stope may vary widely is reported in the Alleghany District, California, by Ferguson and Gannett.* In the Kolar goldfield in India gold fineness variations of considerable latitude, as reported by Pryor (1924, p. 110), are related to depth on the lode, gold of progressively higher fineness being obtained at deeper levels on the vein system. The variations of the lode gold from Burns Mountain do not fall into a regular pattern. They may be explained on the hypothesis either that they represent differences in the fineness of the original gold as deposited, or the hypothesis that wholly or partly they represent changes brought about by the differential solution and redeposition of gold and silver in the zone of oxidation at and near the surface outcrops of the veins. The necessary manganese for chemical reactions of this type could be supplied by the manganiferous ankerite, such as is represented by the material analysed from the Burns Mountain long crosscut (see p. 26). - Sample No. 6 is a specimen containing visible gold in rusty quartz from one of the north-north-easterly striking veins exposed at the surface on the Acme group. The gold in it has a fineness of 927.4-+-0.6 parts per thousand. Spectrochemical analyses made of samples No. 2 and No. 6 in Table II to determine if any minor elements were present in characteristic amounts did not show any sig- nificant differences between the two. The tabulated results follow :— Sample.* | SiOz. | FeoOsz. MgO. | AloOz. | Au | Ag. | Cu | Pb | He | | | | ING Ooh. et Sheesh 120.3f | 2.5 | 25.7 eS | BRIG oe een bys 52a eee Op eae et Geh INGE ate ae be ne ALOU gel cel Oldie Peas OsSiy sli ce emer 8052) eal lec6-d Ao ee carla (12.0 Ni, Ti, Cr, Bi, Sb, Co, Zn, Mn not present in either sample. * Each sample weighed 10 milligrams and 50 per cent. of the light emitted was used to produce a spectrogram. Each sample was treated for five minutes in hot 1:2 hydrochloric acid, decanted, washed, and then treated with hot 1:2 nitrie acid for five minutes. { Figures in the table are spectral line intensities and are directly proportional to the amount of metal in the sample. They are subject to an error of about 15 per cent. Undoubtedly a large part of the silica represents contamination of the sample by the quartz gangue. GEOLOGIC DISTRIBUTION OF AURIFEROUS VEINS. Quartz veins in the Stanley area are not only widely distributed areally but occur in rock-types of a considerable variety. The Foster Ledge veins in Oregon Gulch and the Perkins veins on Burns Mountain are in a series of fairly thinly bedded quartzites and argillaceous schists; the Acme group veins are in hard, fairly thickly bedded light- grey quartzites; the Cariboo Ledge veins are in sheared quartz pebble conglomerate; veins on the Eldorado claim (Lot 11350) and on Lot 1685c at the head of Olally Creek are in black argillaceous quartzite, and in Spruce Canyon there are short veins in chlorite schist. “B” veins such as these are scarce in soft, thinly fissile micaceous schist, but amongst the harder more quartzitic types it cannot be demonstrated that any one particular rock-type contains more veins than another. In this regard the area differs from the Barkerville Gold Belt, where the greatest number of veins occur in a single rock unit, the Rainbow member. * U.S. Geol. Surv., Prof. Paper 172, p. 51, 19382. 29