首页> 外文期刊>The Astrophysical journal >Metastable Eutectic Condensation in a Mg-Fe-SiO-H2-O2 Vapor: Analogs to Circumstellar Dust
【24h】

Metastable Eutectic Condensation in a Mg-Fe-SiO-H2-O2 Vapor: Analogs to Circumstellar Dust

机译:Mg-Fe-SiO-H2-O2蒸气中的亚稳态共晶冷凝:类似于星尘

获取原文
获取外文期刊封面目录资料

摘要

Experimental studies of gas-to-solid condensation in a Fe-Mg-SiO-H2-O2 vapor reveal that this process yields only solids with magnesiosilica (MgO.SiO2) and ferrosilica (Fe-oxide.SiO2) compositions that coincide with metastable eutectics in the MgO-SiO2 and (FeO/Fe2O3)-SiO2 binary phase diagrams plus simple metal oxides (MgO, SiO2, and FeO or Fe2O3). No solids form with mixed Mg-Fe-O compositions during condensation nor is there evidence for the formation of ferromagnesiosilica, MgO.FeyOx.SiO2 solids. The experimental evidence demonstrates that condensation of multicomponent vapors yields only a limited number of metastable solids of well-defined composition. These results have interesting consequences for models of grain formation in circumstellar outflows, for predictions concerning the chemical and mineralogical composition of presolar silicates, and for the composition of condensates formed in protostellar systems.
机译:Fe-Mg-SiO-H2-O2蒸气中气固凝结的实验研究表明,此过程仅产生具有与亚稳共晶相符的镁硅石(MgO.SiO2)和硅铁(Fe-氧化物.SiO2)组成的固体在MgO-SiO2和(FeO / Fe2O3)-SiO2二元相图中加上简单的金属氧化物(MgO,SiO2和FeO或Fe2O3)。在缩合过程中,没有与混合的Mg-Fe-O组合物形成固体,也没有形成铁镁硅氧化物MgO.FeyOx.SiO2固体的证据。实验证据表明,多组分蒸气的冷凝仅产生有限数量的定义明确的亚稳态固体。这些结果对于在恒星外流中形成颗粒的模型,对前太阳系硅酸盐的化学和矿物组成的预测以及在原恒星系统中形成的凝结物的组成都具有有趣的结果。

著录项

获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号