Planetary Science at Oxford Physics 2022

牛津大学物理系行星科学 2022

基本信息

  • 批准号:
    ST/W000938/1
  • 负责人:
  • 金额:
    $ 60.2万
  • 依托单位:
  • 依托单位国家:
    英国
  • 项目类别:
    Research Grant
  • 财政年份:
    2022
  • 资助国家:
    英国
  • 起止时间:
    2022 至 无数据
  • 项目状态:
    未结题

项目摘要

This proposal in planetary physics ranges from studying the atmospheres of the 'Ice Giants' giant planets through to studying the reflectance and thermal properties of airless bodies such as asteroids, which are the primary ways in which these bodies can be studied. The programme outlines a coordinated effort to: 1) measure and understand the fluid circulations, cloud condensation and photochemistry in ice giant planet atmospheres, both within the Solar System and beyond; and 2) measure and interpret the spectra of airless planetary bodies to better understand their origins, composition and regolith structure. We have four complementary main projects. Project 1: The complex, zonally banded atmospheric circulations of all of the giant planets in the Solar System appear to extend over depths that are neither very deep compared to the planetary radius, nor confined solely to a shallow 'weather layer'. This leaves unanswered a host of questions concerning the dynamical origin of their meteorology, the formation and organization of clouds and hazes and the resulting transport of heat and material tracers. In this project, we will test and evaluate possible dynamical mechanisms for energizing the principal features of the atmospheric circulations of the relatively unexplored 'Ice Giant' planets, Uranus and Neptune. Our approach will use a combination of innovative analyses of the observed wind and thermal structure from the Voyager spacecraft, ground-based observations and potentially the JWST, together with a new state-of-the-art global numerical circulation model of the deep weather layers of both planets.Project 2: Uranus and Neptune, the 'Ice Giants', are of increasing interest due to their relevance to the 'mini-Neptunes' being discovered about other stars and rapidly improving ground-based and space-based telescope observations. However, it remains unclear how clouds form in the atmospheres of these Ice Giants, how their formation is related to the overall overturning atmospheric circulation, and how bright, discrete storm cloud features are linked to atmospheric dynamics and thermal anomalies. In this project we will link near-infrared (near-IR) reflection measurements with thermal-IR emission observations taken contemporaneously to explore cloud formation in hydrogen-rich Solar System Ice Giant Planets and analyse these observations with fundamental modelling. This will ultimately benefit the understanding of clouds in both Solar System planets and exoplanets.Project 3: Primitive asteroids (usually assumed to be C- and B-type asteroids) hold important clues to the formation and evolution of the Solar System. In this project, enabled by our roles as a Co-Investigator on the mission and members of the sample analysis team, we will use data from NASA's OSIRIS-REx mission to study primitive asteroid Bennu in preparation for measurements of the sample during the grant period. As part of the mission's science team, and using our bespoke laboratory and numerical modelling capabilities, our work will place the returned sample into geologic context and also help determine Bennu's place in the wider context of the Solar System's asteroid populations. Project 4: Remote sensing measurements in the thermal infrared (TIR) can be used to determine the composition and physical properties of an airless body through spectroscopy and temperature mapping. Surface temperature datasets are being acquired by missions including NASA's Lunar Reconnaissance Orbiter (LRO) and upcoming lunar landers and orbiters, and to interpret them correctly requires new laboratory measurements. This project addresses how thermal emission varies with observation angle, surface roughness and porosity by using and upgrading a unique experimental facility, the Oxford Space Environment Goniometer, to make targeted laboratory measurements to maximise the return from these new and future datasets.
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项目成果

期刊论文数量(5)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
The bulk mineralogy, elemental composition, and water content of the Winchcombe CM chondrite fall
Winchcombe CM 球粒陨石坠落的整体矿物学、元素组成和含水量
Bidirectional reflectance distribution function measurements of the Winchcombe meteorite using the Visible Oxford Space Environment Goniometer
使用可见牛津空间环境测角仪测量温奇科姆陨石的双向反射率分布函数
Linear Modeling of Spectra of Fine Particulate Materials: Implications for Compositional Analyses of Primitive Asteroids
细颗粒材料光谱的线性模型:对原始小行星成分分析的影响
  • DOI:
    10.1029/2021ea002146
  • 发表时间:
    2022
  • 期刊:
  • 影响因子:
    3.1
  • 作者:
    Lowry V
  • 通讯作者:
    Lowry V
The Winchcombe meteorite, a unique and pristine witness from the outer solar system.
  • DOI:
    10.1126/sciadv.abq3925
  • 发表时间:
    2022-11-18
  • 期刊:
  • 影响因子:
    13.6
  • 作者:
  • 通讯作者:
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Neil Bowles其他文献

A new experimental setup for making thermal emission measurements in a simulated lunar environment.
用于在模拟月球环境中进行热发射测量的新实验装置。
  • DOI:
  • 发表时间:
    2012
  • 期刊:
  • 影响因子:
    1.6
  • 作者:
    I. Thomas;B. Greenhagen;Neil Bowles;K. D. Hanna;J. Temple;S. Calcutt
  • 通讯作者:
    S. Calcutt
The EChO payload instrument – an overview
  • DOI:
    10.1007/s10686-014-9428-8
  • 发表时间:
    2014-11-19
  • 期刊:
  • 影响因子:
    2.200
  • 作者:
    Paul Eccleston;Bruce Swinyard;Marcel Tessenyi;Giovanna Tinetti;Ingo Waldmann;Marc Ferlet;Ranah Irshad;Tanya Lim;Kevin Middleton;Tom Bradshaw;Martin Crook;Tom Hunt;Berend Winter;Ian Bryson;Naidu Bezawada;William Taylor;Neil Bowles;Enzo Pascale;Gianluca Morgante;Emanuele Pace;Alberto Adriani;Jean-Michel Reess;Marc Ollivier;Roland Ottensamer;Mirek Rataj;Gonzalo Ramos Zapata;Jan-Rutger Schrader;Avri Selig;Kate Isaak;Martin Linder;Ludovic Puig
  • 通讯作者:
    Ludovic Puig

Neil Bowles的其他文献

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{{ truncateString('Neil Bowles', 18)}}的其他基金

Planetary Science at Oxford Physics 2019
2019 年牛津物理系行星科学
  • 批准号:
    ST/S000461/1
  • 财政年份:
    2019
  • 资助金额:
    $ 60.2万
  • 项目类别:
    Research Grant
Market assessment of the potential of an IR Radiometer to detect aerosols, volcanic ash and land surface heat emissions
对红外辐射计检测气溶胶、火山灰和地表热排放潜力的市场评估
  • 批准号:
    NE/R003688/1
  • 财政年份:
    2017
  • 资助金额:
    $ 60.2万
  • 项目类别:
    Research Grant
Support for continuing Co-I Participation in NASA's OSIRIS-REx sample return mission.
支持 Co-I 继续参与 NASA 的 OSIRIS-REx 样本返回任务。
  • 批准号:
    ST/P007228/1
  • 财政年份:
    2017
  • 资助金额:
    $ 60.2万
  • 项目类别:
    Research Grant
Development of a Compact Modular Radiometer for Laboratory and Field Studies
开发用于实验室和现场研究的紧凑型模块化辐射计
  • 批准号:
    NE/H002359/1
  • 财政年份:
    2010
  • 资助金额:
    $ 60.2万
  • 项目类别:
    Research Grant

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牛津大学发现科学的跨学科研究能力。
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