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Planetary Origins and Evolution at Imperial (2019-2022)

帝国理工学院的行星起源与演化（2019-2022）

基本信息

批准号：
ST/S000615/1
负责人：
Gareth Collins
金额：
$ 110.87万
依托单位：
Imperial College London
依托单位国家：
英国
项目类别：
Research Grant
财政年份：
2019
资助国家：
英国
起止时间：
2019 至无数据
项目状态：
已结题

来源：
https://gtr.ukri.org/projects?ref=ST%2FS000615%2F1
关键词：
Planetary Origins Evolution Imperial 2019

项目摘要

How do stars and planetary systems develop and is life unique to our planet? This is one of the most fundamental of questions in science and has deeply profound implications for our place in the cosmos. It is thus a key scientific challenge set by the Science and Technology Facilities Council. Our planet formed 4.5 billion years ago along with the Sun and the other planets and minor bodies in our Solar System. Only by understanding the details of how our Solar System formed can we hope to find an answer.We now know how stars and planetary systems form in general. We know that stars form by the collapse of interstellar clouds of dust and gas, and planets are constructed in disks of dust and gas surrounding these young stars. There is, however, much we don't know about how our Solar System formed. Why, for example, are all the planets so different? Why is Venus an inferno, Mars a frozen rock, and Earth a haven for life? The answer lies in events that predated the assembly of the planets. Our research program focuses on answering key outstanding questions in this early history of the Solar System.The source of presolar dust provides a context to our solar system. From what types of star was dust derived and is this mixture typical of other planetary systems? Some of this dust still remains preserved within ancient meteorites and reveals that at least 30 stars produced building blocks for our planets. We aim to sample many more stars by looking for interstellar dust preserved on the Earth's surface within sediments accumulated throughout our planet's history. This will provide a full ingredient list for planetary systems, not just our own.How planetary materials changed after the dust was assembled into larger bodies is crucial in making planets that are suitable for life. Our research will examine whether primitive planetesimals, the early forerunners of planets, melted and mixed internally by examining the evidence for early magnetic fields within meteorites. Our research will evaluate whether ancient magnetic traces already found in meteorite minerals are reliable indicators of the dynamos of metallic cores.Volatile constituents are vital to life but easily lost by heating and they differ greatly in abundance between planets in our solar system. Our research focuses on the volatile budgets of the terrestrial planets, to identify the source of the volatiles and determine when they were added. For this, the research examines the isotopes of selenium and tellurium and is made possible by technology and method advances that will be pioneered in the study. As such, the work will help us understand how planets acquire the ingredients essential to the formation life.Large quantities of volatiles, organic matter and energy, were delivered to the terrestrial planets in a prolonged period of intense bombardment in the early solar system, which likely had a profound influence on the emergence and evolution of life. Large craters that scar the Moon, Mars, Venus and large asteroids provide a record of this bombardment, but one that is challenging to decode. By simulating large crater formation using advanced numerical models, we aim to link observed crater populations to the impactors that formed them and constrain the timing and source of their delivery to the inner solar system.Finally, what constitutes a planet "suitable for life"? To date only Earth is known to have living things. Whilst the search for life on Mars continues, many believe that living organisms are more likely within the ice-covered oceans of the moons of Jupiter and Saturn. Our research will focus on recognizing the molecular signature of life within the atmospheres and outflows from icy-moons using experiments and world-leading analytical techniques. This research could provide the first convincing evidence for life beyond Earth and widen our view of the right kind of planet.

恒星和行星系统是如何发展的？生命是我们星球上独有的吗？这是科学中最基本的问题之一，对我们在宇宙中的地位有着深远的影响。因此，这是科学技术设施委员会提出的一项关键科学挑战。我们的星球与太阳以及太阳系中的其他行星和小天体一起于 45 亿年前形成。只有了解太阳系如何形成的细节，我们才有希望找到答案。我们现在知道恒星和行星系统一般是如何形成的。我们知道，恒星是由星际尘埃和气体云的塌陷形成的，而行星是在这些年轻恒星周围的尘埃和气体盘中构成的。然而，对于太阳系是如何形成的，我们还有很多不了解的地方。例如，为什么所有行星都如此不同？为什么金星是地狱，火星是冰冻岩石，而地球是生命的天堂？答案在于行星聚集之前发生的事件。我们的研究计划侧重于回答太阳系早期历史中的关键悬而未决的问题。太阳前尘埃的来源为我们的太阳系提供了背景。尘埃是从什么类型的恒星中产生的？这种混合物是其他行星系统的典型混合物吗？其中一些尘埃仍然保存在古代陨石中，表明至少有 30 颗恒星为我们的行星提供了组成部分。我们的目标是通过寻找地球历史上积累的沉积物中保存在地球表面的星际尘埃来采样更多的恒星。这将为行星系统提供完整的成分列表，而不仅仅是我们自己的系统。尘埃聚集成更大的天体后，行星材料如何变化对于形成适合生命存在的行星至关重要。我们的研究将通过检查陨石内早期磁场的证据来检验原始星子（行星的早期先驱）是否在内部熔化和混合。我们的研究将评估在陨石矿物中发现的古代磁迹是否是金属核心发电机的可靠指标。挥发性成分对生命至关重要，但很容易因加热而消失，而且太阳系中行星之间的丰度差异很大。我们的研究重点是类地行星的挥发物预算，以确定挥发物的来源并确定它们何时添加。为此，该研究检查了硒和碲的同位素，并通过该研究中开创的技术和方法的进步得以实现。因此，这项工作将帮助我们了解行星如何获得形成生命所必需的成分。在早期太阳系的长期强烈轰击中，大量的挥发物、有机物和能量被输送到类地行星，这可能对生命的出现和进化产生了深远的影响。月球、火星、金星和大型小行星上布满疤痕的大型陨石坑提供了这次轰炸的记录，但解码起来却颇具挑战性。通过使用先进的数值模型模拟大型陨石坑的形成，我们的目标是将观测到的陨石坑群与形成它们的撞击物联系起来，并限制它们输送到内太阳系的时间和来源。最后，什么构成了一颗“适合生命存在”的行星？迄今为止，只有地球已知有生物。虽然在火星上寻找生命的工作仍在继续，但许多人认为，木星和土星卫星的冰雪覆盖的海洋中更有可能存在生物体。我们的研究将侧重于利用实验和世界领先的分析技术来识别大气中生命的分子特征以及冰卫星的流出物。这项研究可以为地球以外的生命提供第一个令人信服的证据，并拓宽我们对正确类型行星的看法。