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The Clay Minerals Society 粘土矿物协会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.62
Haojie Cui, Lei You, Xionghan Feng, Wenfeng Tan, Guohong Qiu, Sheng Chang, Dah Tong Ray, Ming Kuang Wang, Yen Hong Shau, Yun Wei Shen, Ruey Chyong Chen, Holly A. Welsh
September is often a busy month for conferences, but this is the first year for a long time that I have not attended one. Last year I participated in two, the first here in Aberdeen and the second in Zakopane, Poland. The first was held at the Macaulay Institute as a tribute to one of its most productive researchers, V. C. Farmer, on the subject “Aluminium and Silicon in Soils and the Environment”. Colin was best known for his pioneering work on the infrared spectroscopy of minerals. The second was the highly successful Mid-European Clay Conference, at which there were many excellent presentations as well as field trips. The meeting organisers asked Joe Stucki, Editor-in-Chief of Clays and Clay Minerals, if manuscripts could be submitted for possible publication in CMS’s journal. Joe agreed and the outcome was a complete issue of Clays and Clay Minerals (August 2009) covering a range of topics. The titles of these papers can be accessed at http://ccm.geoscienceworld.org/cgi/issue_pdf/toc_pdf/57/4. Remember, CMS members with a subscription to the journal should log in at the CMS website (www.clays.org) in order to access the content.
九月通常是一个会议繁忙的月份,但今年是我很久没有参加会议的第一年。去年我参加了两次会议,第一次在阿伯丁,第二次在波兰扎科帕内。第一次会议是在麦考利研究所举行的,目的是向该研究所最有成就的研究人员之一 V. C. Farmer 致敬,会议主题是 "土壤和环境中的铝和硅"。科林因其在矿物红外光谱学方面的开创性工作而闻名于世。第二次是非常成功的中欧粘土会议,会上有许多精彩的演讲和实地考察。会议组织者询问《粘土和粘土矿物》杂志主编 Joe Stucki,是否可以提交手稿,以便在 CMS 杂志上发表。乔同意了,结果《粘土和粘土矿物》(2009 年 8 月)完整地刊载了涵盖一系列主题的论文。这些论文的标题可在 http://ccm.geoscienceworld.org/cgi/issue_pdf/toc_pdf/57/4 上查阅。请记住,已订阅该期刊的 CMS 会员应登录 CMS 网站 (www.clays.org) 以访问相关内容。
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引用次数: 0
Asteroidal Organics from the Sample Return Mission Hayabusa2 and their Implication for Understanding our Origins 隼鸟2号采样返回任务采集的小行星有机物及其对了解人类起源的意义
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.31
S. Tachibana, Nami Sakai
The C-type asteroid Ryugu samples returned by the Hayabusa2 spacecraft are the chemically most pristine material in the Solar System, as they have not been exposed to terrestrial environments. The organic matter in Ryugu records the molecular evolution from the Sun’s parent molecular cloud chemistry to asteroidal aqueous alteration. In this article, we review the results of Ryugu sample analysis and discuss the evolution of organic matter in the early Solar System by comparing these results with recent radio and infrared observations of protostars and protoplanetary disks.
隼鸟2号航天器返回的C型小行星龙宫样本是太阳系中化学性质最原始的物质,因为它们没有暴露在陆地环境中。龙宫中的有机物质记录了从太阳母分子云化学到小行星水蚀的分子演化过程。在这篇文章中,我们回顾了龙宫样本分析的结果,并通过将这些结果与最近对原初恒星和原行星盘的射电和红外观测结果进行比较,讨论了太阳系早期有机物的演化。
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引用次数: 1
Mineralogical Society of America 美国矿物学会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.52
David L. Bish, Julia A. Nord, Jeff LeClair
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引用次数: 0
Meteoritical Society 气象学会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.58
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引用次数: 0
Mineralogical Society of the UK and Ireland 英国和爱尔兰矿物学会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.48
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引用次数: 0
German Mineralogical Society 德国矿物学会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.50
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引用次数: 0
International Association on the Genesis of Ore Deposits 国际矿床成因协会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.56
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引用次数: 0
Extraterrestrial Organic Matter: An Introduction 地外有机物:导言
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.7
Mehmet Yesiltas, Yoko Kebukawa
Extraterrestrial organic matter forms in a variety of locations in space through different mechanisms. Its nature, distribution, formation mechanisms and locations are of particular interest. Some organic molecules can even be considered as key players for the emergence of life. Although new organic species are continuously detected in the interstellar media, Solar System bodies, and extraterrestrial materials, their formation and evolution are still not fully understood. Ground-based and space observations can detect organic matter in different objects with a range of complexity and diversity, while laboratory investigations of astromaterials allow detailed characterization of extraterrestrial organic matter with high precision. This issue reviews different aspects of extraterrestrial organic matter, including its origin, evolution, diversity, and delivery.
地外有机物通过不同的机制在空间的不同位置形成。它的性质、分布、形成机制和位置都特别令人感兴趣。有些有机分子甚至可以被视为生命出现的关键因素。虽然在星际介质、太阳系天体和地外物质中不断探测到新的有机物种,但对它们的形成和演化仍不完全了解。地基和空间观测可以探测到不同天体中复杂多样的有机物,而天体材料的实验室研究则可以高精度地描述地外有机物的详细特征。本期将从不同方面评述地外有机物,包括其起源、演化、多样性和输送。
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引用次数: 0
Formation and Evolution Mechanisms for Organic Matter in Space 太空有机物的形成和进化机制
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.13
Hideko Nomura, Queenie Hoi Shan Chan, Hikaru Yabuta
Organic compounds are a major component of dust in molecular clouds, alongside silicates and water ice, due to the high abundances of elements that make up these compounds in the Galaxy. The initial molecular inventory of the Solar System, inherited from the molecular cloud, was modified and new complex molecules were formed in the protoplanetary disk and planetesimals. Because astronomical observations mainly target gas, while cosmochemical evidence deals with solid phases, it is crucial to link discrepant knowledge on organic species through state-of-the-art modeling. This chapter reviews the latest understanding of surface reactions on inter-stellar dusts, gas–dust reactions in the protoplanetary disk, and alteration processes on planetesimals in the early Solar System.
有机化合物是分子云中尘埃的主要成分,此外还有硅酸盐和水冰,这是因为银河系中构成这些化合物的元素丰度很高。太阳系最初的分子清单是从分子云中继承下来的,后来发生了变化,在原行星盘和类地行星中形成了新的复杂分子。由于天文观测主要针对气体,而宇宙化学证据则涉及固相,因此通过最先进的建模将有关有机物种的差异知识联系起来至关重要。本章回顾了对星际尘埃的表面反应、原行星盘中的气体-尘埃反应以及太阳系早期行星的改变过程的最新认识。
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引用次数: 2
Mineralogical Society of Poland 波兰矿物学会
IF 4.5 2区 地球科学 Q1 Earth and Planetary Sciences Pub Date : 2024-02-01 DOI: 10.2138/gselements.20.1.61
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引用次数: 0
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