Presolar grains from meteorites: Remnants from the early times of the solar system     

Katharina Lodders  Sachiko Amari 《Chemie der Erde / Geochemistry》2005,65(2):93-166

This review provides an introduction to presolar grains - preserved stardust from the interstellar molecular cloud from which our solar system formed - found in primitive meteorites. We describe the search for the presolar components, the currently known presolar mineral populations, and the chemical and isotopic characteristics of the grains and dust-forming stars to identify the grains’ most probable stellar sources.  相似文献   

黄土粒度分布中的超细粒组分及其成因^*   总被引：16，自引：10，他引：16       下载免费PDF全文

孙东怀 《第四纪研究》2006,26(6):928-936

多个剖面的粒度测量表明,黄土高原的黄土和古土壤中普遍存在超细粒组分,其平均粒径大致0.4μm,在全样中的含量大致5 ％ ~6 ％。 超细粒组分的含量在黄土中低,在古土壤中高;并且同一地层自西北至东南增加,这些特征都显示超细粒组分的形成与成壤作用强度相关。一般情况下超细粒组分的粒度在黄土中粗,在古土壤中细。黄土高原各季节的现代天然粉尘中同样存在超细粒组分,然而干旱区成壤作用较少的天然降尘中基本不存在超细粒组分。以上特征说明,黄土中的超细粒组分的形成与成壤作用有关,成壤作用中次生矿物的粒度和含量特征也支持这一解释。  相似文献   

U–Pb LA-ICP-MS geochronology of detrital zircon grains from low-grade metasedimentary rocks (Neoproterozoic – Cambrian) of the Mojotoro Range,northwest Argentina     

《Journal of South American Earth Sciences》2014

The first results of U–Pb detrital zircons were obtained in three lithostratigraphic units of the Puncoviscana Complex in NW Argentina: Chachapoyas, Alto de la Sierra and Guachos Formations. The Chachapoyas Formation has a maximum sedimentation age of 569 Ma and a minimum age of 533 Ma, based on the U–Pb age of an intrusive porphyry granitic. The Alto de la Sierra Formation, composed by sandstones and volcaniclastic rocks, has a maximum age of 543 Ma. A maximum age of 517 Ma is here reported for the deposition of the Guachos Formation, the youngest unit. The contact between the Chachapoyas and Guachos formations is by a tectonic relation, and it's probably coincident with a stratigraphic unconformity between them (unconformity Tilcara I). The Lizoite Formation is overlying by an unconformity (Tilcara II unconformity) the Puncoviscana Complex, and represents the basal unit of the Mesón Group. The provenance zircon data for that formation indicate a maximum depositional age of 513 Ma.  相似文献   

Porous and fluffy grains in the regions of anomalous extinction     

D. B. Vaidya  B. G. Anandarao  J. N. Desai  R. Gupta 《Journal of Astrophysics and Astronomy》2000,21(1-2):91-99

It has long been established that the ratio of total to selective extinction is anomalously large (>- 5) in certain regions of the interstellar medium. In these regions of anomalous extinction the dust grains are likely to be irregular in shape and fluffy in structure. Using discrete dipole approximation (DDA) we calculate the extinction for porous and fluffy grains. We apply DDA first to solid spheroidal particles assumed to be made of a certain (large) number of dipoles. Then we systematically reduce the number of dipoles to model the porous grains. The aggregates of these particles are suggested to form the fluffy grains. We study the extinction for these particles as a function of grain size, porosity and wavelength. We apply these calculations to interpret the observed extincttion data in the regions of star formation (e.g. the Orion complex).  相似文献   

Beta dose heterogeneity in sediment samples measured using a Timepix pixelated detector and its implications for optical dating of individual mineral grains     

《Quaternary Geochronology》2022

  相似文献