J. R. O’Neil L.H. Adami J.D. Gleason K. Hardcastle I. Friedman 1970 <div class="panel-pane pane-highwire-panel-tabs-container article__body"><div class="pane-content"><div id="panels-ajax-tab-container-highwire_article_tabs" class="panels-ajax-tab-container" data-panels-ajax-tab-preloaded="jnl_sci_tab_art"><div class="panels-ajax-tab-wrap-jnl_sci_tab_art"><div class="panel-display panel-1col clearfix"><div class="panel-panel panel-col"><div><div class="panel-pane pane-highwire-markup"><div class="pane-content"><div class="highwire-markup"><div id="content-block-markup" data-highwire-cite-ref-tooltip-instance="highwire_reflinks_tooltip" data-highwire-glossary-tooltip-instance="highwire_reflinks_tooltip"><div class="article abstract-view "><div id="abstract-1" class="section abstract"><p id="p-1">The water content of the breccia is 150 to 455 ppm, with a δD from—580 to —870 per mil. Hydrogen gas content is 40 to 53 ppm with a δD of —830 to —970 per mil. The CO₂<span>&nbsp;</span>is 290 to 418 ppm with δ<span>&nbsp;</span>¹³C = + 2.3 to + 5.1 per mil and δ¹⁸O = 14.2 to 19.1 per mil. Non-CO₂<span>&nbsp;</span>carbon is 22 to 100 ppm, δ¹³C = —6.4 to —23.2 per mil. Lunar dust is 810 ppm H₂O (D = 80 ppm) and 188 ppm total carbon(δ¹³C = —17.6 per mil). The<span>&nbsp;</span>¹⁸O analyses of whole rocks range from 5.8 to 6.2 per mil. The temperature of crystallization of type B rocks is 1100° to 1300°C, based on the oxygen isotope fractionation between coexisting plagioclase and ilmenite.</p></div></div><span id="related-urls"></span></div></div></div></div></div></div></div></div></div></div></div> application/pdf 10.1126/science.167.3918.538 en American Association for the Advancement of Science Water, hydrogen, deuterium, carbon, carbon-13, and oxygen-18 content of selected lunar material article