<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>A. V. Heyl</dc:contributor>
  <dc:contributor>J.P. Creel</dc:contributor>
  <dc:creator>E. Roedder</dc:creator>
  <dc:date>1968</dc:date>
  <dc:description>&lt;p&gt;&lt;span&gt;These&amp;nbsp;&lt;/span&gt;deposits&lt;span&gt;, in Pennsylvanian limestone and shale, contain barite, fluorite, low-silver galena with "J-type" lead, and quartz, and only minor amounts of other minerals. Mineralization occurs in veins, in blankets of bedded, rhythmically banded "coontail"&amp;nbsp;&lt;/span&gt;ore&lt;span&gt;, and in vuggy, coarsely crystalline open-space fillings in tectonic and solution channels in limestone adjacent to faults. Except for widespread silicification, the mineralization is very similar to that of the southern Illinois&amp;nbsp;&lt;/span&gt;deposits&lt;span&gt;. The main stages of hypogene mineralization are: 1) sphalerite, pyrite, galena and chalcopyrite; 2) five easily recognizable substages of fluorite with intermittent quartz and barite; and 3) late calcite.More than 500 primary and 2,500 pseudosecondary&amp;nbsp;&lt;/span&gt;inclusions&lt;span&gt;, mainly from fluorite, were studied on the freezing and heating microscope stages. Some primary&amp;nbsp;&lt;/span&gt;inclusions&lt;span&gt;&amp;nbsp;contain organic matter. Gross supercooling indicates slow&amp;nbsp;&lt;/span&gt;ore&lt;span&gt;-&lt;/span&gt;fluid&lt;span&gt;&amp;nbsp;movement. Recognizable planes of pseudo-secondaries (each containing 20-200&amp;nbsp;&lt;/span&gt;inclusions&lt;span&gt;) yield data essentially identical with coeval primaries, but the few planes of presumed secondaries do not.The first three substages of fluorite formed from fluids that were essentially constant in temperature&amp;nbsp;&lt;/span&gt;at&lt;span&gt;&amp;nbsp;186°-205° C (assumed pressure correction +10° C), but increased in salinity from aproximately 10 up to 15 weight percent salts. Succeeding substages formed&amp;nbsp;&lt;/span&gt;at&lt;span&gt;&amp;nbsp;gradually decreasing temperatures (to about 140° C) and increasing salinity (maximum 17%), with breaks marking several individual substages. A few&amp;nbsp;&lt;/span&gt;inclusions&lt;span&gt;&amp;nbsp;in an early barite have anomalously low homogenization temperatures. Coarse selenite has primary&amp;nbsp;&lt;/span&gt;inclusions&lt;span&gt;&amp;nbsp;full of fresh water and hence is presumed to be supergene.These data do not prove any given theory or origin for the fluids or the&amp;nbsp;&lt;/span&gt;deposits&lt;span&gt;, but they do place some limits on possible mechanisms of origin.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.2113/gsecongeo.63.4.336</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Society of Economic Geologists</dc:publisher>
  <dc:title>Environment of ore deposition at the Mex-Tex deposits, Hansonburg District, New Mexico, from studies of fluid inclusions</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>