The oxygen fugacity of core segregation and the redox evolution of the mantle: constraints from iron and chromium isotopes

核心偏析的氧逸度和地幔的氧化还原演化：来自铁和铬同位素的约束

• 批准号: NE/F014295/1
• 负责人: Helen Williams
• 金额: $ 60.66万
• 依托单位: University of Oxford
• 依托单位国家: 英国
• 项目类别: Fellowship
• 财政年份: 2009
• 资助国家: 英国
• 起止时间: 2009 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=NE%2FF014295%2F1
• 关键词: oxygen; fugacity; core; segregation; redox

We know very little about the origin of our own planet, how it has evolved through time and how it came to be suitable for life. There is considerable controversy surrounding issues like climate change, and the search for new planets around stars other than the Sun and missions to planets in our own solar system and it is currently a very exciting time to be an Earth scientist. The Earth formed about 4600 million years ago, from particles of dust and rocky material present in the early solar system. Only a few million years later, the Earth underwent a massive reorganisation from an enormous mass of unsorted primitive material into a planet composed of a metal core in its centre and a surrounding rocky outer part. We still do not understand precisely how this happened, as the Earth has undergone a wide range of geological events which hide much of the evidence. One possibility is that when the Earth was still hot and molten, liquid metal separated from the rest of the planet and descended to the centre of the Earth, forming its core. During this process, most of the Earth's iron and many other elements were distributed preferentially into the metal core. This imparted a characteristic chemical signal to the outer rocky parts of the Earth, which we can sample through rocks erupted from volcanoes. However, there are many aspects of this part of Earth history that we do not understand. For example, we do not know the exact conditions of core formation and how it could have affected other aspects of the planet's chemistry, such as the amount of oxygen present in the rocky interior of the planet. This is an important question to answer if we are to understand how life originated on Earth, as it is likely that the Earth's oceans and much of the Earth's atmosphere originated from gases leaking out of planet's interior when the Earth was still very young. My project is aimed at understanding what kind of conditions the Earth's core formed under and how this affected the amount of oxygen present in the rocky interior of the Earth. It uses experiments which simulate the very high pressures and temperatures that would have been present in the Earth's interior when the core formed, combined with very precise chemical analyses of these experiments. From these results I will learn how certain chemical elements distributed themselves between the metal core and the rocky outer part of the Earth, and whether this distribution behaviour changes with different conditions and with the amount of oxygen present. By comparing the results I get from the experiments with the chemical compositions of rocks from the Earth and very primitive meteorites we will be able to understand better how the Earth's core formed, and how this may have affected the chemistry of our planet and the development of its atmosphere and oceans.

我们对地球的起源知之甚少，它是如何随着时间的推移而演变的，以及它是如何适合生命的。围绕气候变化等问题存在相当大的争议，寻找太阳以外的恒星周围的新行星，以及在我们自己的太阳系中的行星任务，目前是一个非常令人兴奋的时刻，成为一名地球科学家。地球形成于大约46亿年前，由早期太阳系中存在的尘埃和岩石物质组成。仅仅几百万年后，地球经历了一次大规模的重组，从一个巨大的未经分类的原始物质变成了一个由中心金属核心和周围岩石组成的行星。我们仍然不知道这是如何发生的，因为地球经历了广泛的地质事件，隐藏了许多证据。一种可能性是，当地球仍然炎热和熔融时，液态金属从地球的其他部分分离出来，下降到地球的中心，形成了它的核心。在这个过程中，地球上的大部分铁和许多其他元素都优先分配到金属核中。这给地球外部的岩石部分带来了一种特有的化学信号，我们可以通过火山喷发的岩石进行采样。然而，地球历史的这一部分有许多方面我们不了解。例如，我们不知道核心形成的确切条件以及它如何影响行星化学的其他方面，例如行星岩石内部的氧气量。如果我们要了解地球上的生命是如何起源的，这是一个需要回答的重要问题，因为地球的海洋和大部分地球大气层很可能起源于地球还很年轻时从地球内部泄漏出来的气体。我的项目旨在了解地核是在什么样的条件下形成的，以及这如何影响地球岩石内部的氧气量。它使用模拟地核形成时地球内部存在的非常高的压力和温度的实验，并结合对这些实验的非常精确的化学分析。从这些结果中，我将了解某些化学元素是如何在地球的金属核和岩石外层之间分布的，以及这种分布行为是否会随着不同的条件和存在的氧气量而变化。通过将我从实验中得到的结果与地球岩石和非常原始的陨石的化学成分进行比较，我们将能够更好地了解地球核心是如何形成的，以及这可能如何影响我们星球的化学成分及其大气和海洋的发展。

项目成果

Shallow forearc mantle dynamics and geochemistry: New insights from IODP Expedition 366

• DOI: 10.1016/j.lithos.2018.10.038
• 发表时间: 2019-02-01
• 期刊: LITHOS
• 影响因子: 3.5
• 作者: Debret, B.;Albers, E.;Williams, H.
• 通讯作者: Williams, H.

Silicon isotopes in meteorites and planetary core formation

• DOI: 10.1016/j.gca.2011.03.044
• 发表时间: 2011-07-01
• 期刊: GEOCHIMICA ET COSMOCHIMICA ACTA
• 影响因子: 5
• 作者: Armytage, R. M. G.;Georg, R. B.;Halliday, A. N.
• 通讯作者: Halliday, A. N.

Persistence of deeply sourced iron in the Pacific Ocean.

太平洋中深部铁的持久存在。

• DOI: 10.1073/pnas.1420188112
• 发表时间: 2015
• 期刊: Proceedings of the National Academy of Sciences of the United States of America
• 影响因子: 11.1
• 作者: Horner TJ

Iron and silicon isotope behaviour accompanying weathering in Icelandic soils, and the implications for iron export from peatlands

• DOI: 10.1016/j.gca.2017.08.033
• 发表时间: 2017-11
• 期刊: Geochimica et Cosmochimica Acta
• 影响因子: 5
• 作者: S. Opfergelt;H. Williams;J. Cornelis;R. Guicharnaud;R. B. Georg;C. Siebert;S. Gíslason;A. Halliday;K. Burton

Stable chromium isotopic composition of meteorites and metal-silicate experiments: Implications for fractionation during core formation

• DOI: 10.1016/j.epsl.2015.11.026
• 发表时间: 2016-02-01
• 期刊: EARTH AND PLANETARY SCIENCE LETTERS
• 影响因子: 5.3
• 作者: Bonnand, P.;Williams, H. M.;Halliday, A. N.
• 通讯作者: Halliday, A. N.