SIM-EARTH: Simulating the evolution of Earth's environment

SIM-EARTH：模拟地球环境的演变

• 批准号: EP/Y008790/1
• 负责人: Benjamin Mills
• 金额: $ 215.48万
• 依托单位: University of Leeds
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2023
• 资助国家: 英国
• 起止时间: 2023 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=EP%2FY008790%2F1
• 关键词: SIM; EARTH; Simulating; evolution; Earth

The temperature of Earth's surface and the amount of oxygen in the atmosphere and oceans has changed dramatically over our planet's history, but there is no consensus on what has driven these changes. We do not understand the relative importance of the fundamental processes that have made our planet suitable for complex life, and this is impairing our ability to understand our own evolution, to map our planet's future, and to make predictions about what type of planets might support complex life in general. A key reason for this lack of understanding is our inability to simulate the evolution of Earth's surface conditions in a realistic computer model because of the extreme billion-year timescales involved. The computational demand to do this is just far too high.SIM-EARTH will use a new computational technique that I have recently prototyped to couple plate tectonics, physical climate and global biogeochemical cycles over billions of years, creating for the first time a 3D and time-evolving model of a planetary surface environment. This model will finally allow us to integrate all of the hypothesised processes that might control Earth's environment, and opens up the ability to use rigorous model-data comparison at local and global scales to identify which processes are the most important. The outcome will help us understand what underlying properties of our planet have led to the temperate and high-oxygen environment which has allowed for the evolution of intelligent life.This project will provide a set of completely new insights into important periods of Earth's past, will inform us about how to best preserve our world for humans, and will help decide where we should look for intelligent life elsewhere in the galaxy.

地球表面的温度以及大气和海洋中的氧气量在我们星球的历史上发生了巨大变化，但是在驱动这些变化的原因方面尚无共识。我们不了解使我们的星球适合复杂生命的基本过程的相对重要性，这损害了我们了解自己的进化，绘制地球的未来，并预测哪种类型的星球可能支持复杂生活的能力。缺乏理解的一个关键原因是，由于涉及的极端时间尺度，我们无法在现实的计算机模型中模拟地球表面条件的演变。执行此操作的计算需求太高了。标准 - 地铁将使用一种新的计算技术，我最近对板块构造，物理气候和全球生物地球化学周期进行了原型，这是数十亿年来的，这是第一次创建一个行星表面环境的3D和时间变化模型。该模型最终将使我们能够整合所有可能控制地球环境的假设过程，并打开在本地和全球量表上使用严格的模型数据比较的能力，以确定哪些过程最重要。结果将有助于我们了解地球的基本特性导致了温带和高氧环境，这将允许智能生活的演变。该项目将为地球过去重要时期提供一系列全新的见解，将为我们提供如何为人类提供最好的维持世界的信息，并帮助我们在哪里为我们的其他地方提供智能的生活。