D.E. Appleman J.S. Huebner J. R. Clark D. B. Stewart 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">Crystals of calcic bytownite from type B rocks have space group I1 with c ≈ 14 angstroms. Bytownite crystals from type A rocks are more sodic and have space group C1, c ≈ 7 angstroms. Cell parameters of eight bulk feldspar separates from crystalline rocks indicate that the range of angle gamma is about 23 times the standard error of measurement, and its value might be useful for estimation of composition. Cell parameters of seven ilmenites are close to those of pure FeTiO₃.</p></div></div><span id="related-urls"></span></div></div></div></div></div></div></div></div></div></div></div> application/pdf 10.1126/science.167.3918.634 en American Association for the Advancement of Science Crystallography of some lunar plagioclases article