Publication Date:
2024-07-01
Description:
In an earlier paper by two of the authors the conclusion was reached that the 33 recognized species of oxides of Mn could be separated into 3 groups: 1) those which appeared to be persistently supergene in origin, 2) those which appeared to be persistently hypogene, and 3) those which were supergene in some localities and hypogene in other localities. When that paper was written, there were available about 250 X-ray diffraction analyses of mineral specimens, also 35 complete and about 150 partial chemical analyses. The conclusions of that paper were based upon the interpretation of the geologic conditions under which these specimens occurred. Late in the preparation of that paper, it seemed worthwhile to make numerous semiquantitative analyses of specimens, largely from 9 western [U.S.A] states, selected carefully from 5 groups of geologic environments, in the hope that the frequency and percentages of some elements might be distinctive of the several geologic groups. For this purpose, 95 specimens were selected from the 5 groups, as follows: 19 specimens interpreted as supergene oxides by the geologists who collected them, 35 specimens of hypogene vein oxides, 22 specimens of Mn-bearing hot spring aprons, 9 specimens of stratified oxides, and 10 specimens of deep-sea nodules. The spectrographic analyses here recorded indicate that a group of elements - W, Ba, Sr, Be, As, Sb, Tl, and Ge - are present more commonly, and largely in higher percentages, in the hypogene oxide than in the supergene oxides and thus serve to indicate different sources of the Mn. Also, the frequency and percentages of some of these elements indicate a genetic relation of the manganese oxides in hypogene veins, hot spring aprons, and stratified deposits. The analyses indicate a declining percentage of some elements from depth to the surface in these 3 related groups and increasing percentages of some other elements. It is concluded that some of the elements in deep-sea nodules indicate that sources other than rocks decomposed on the continents, probably vulcanism on the floors of the seas, have contributed to their formation.
Keywords:
ALB-13; ALB-173; Albatross (1882-1921); Albatross1899-1900; Albatross1904-1905; ALBTR-13; ALBTR-173; ALBTR-4662; Aluminium; Barium; Beryllium; Bismuth; Boron; Calcium; Cerium; Chromium; Cobalt; Copper; DEPTH, sediment/rock; DNWB0ABD; DOWNWIND-B1; DOWNWIND-H; Dredge; Dredge, chain bag; Dredge, rock; DRG; DRG_C; DRG_R; DWBD1; DWHD47; Elevation of event; Event label; FANB01BD; FANBD-25D; FANFARE-B; Horizon; Indian Ocean; Iron; Lanthanum; Latitude of event; Lead; LGO-BT-57 or VM14 SBT57 (SIO); Longitude of event; Magnesium; MDPC02HO-MP-025F-2; MDPC02HO-MP-033K; MIDPAC; Molybdenum; MPC-25F-2; MPC-33K; NAGA; NAGA10C; Neodymium; Nickel; Niobium; NOAA and MMS Marine Minerals Geochemical Database; NOAA-MMS; Pacific Ocean; Photo/Video; Potassium; PV; Sample ID; Scandium; Silicon; Sodium; Spectrographic analysis; Spencer F. Baird; Stranger; Strontium; Thallium; Titanium; V14; V14-57RD; Vanadium; Vema; Ytterbium; Yttrium; Zinc; Zirconium
Type:
Dataset
Format:
text/tab-separated-values, 296 data points
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