Planetary Systems: from Plutos to Jupiters

行星系统:从冥王星到木星

基本信息

  • 批准号:
    261952-2012
  • 负责人:
  • 金额:
    $ 1.82万
  • 依托单位:
  • 依托单位国家:
    加拿大
  • 项目类别:
    Discovery Grants Program - Individual
  • 财政年份:
    2015
  • 资助国家:
    加拿大
  • 起止时间:
    2015-01-01 至 2016-12-31
  • 项目状态:
    已结题

项目摘要

Our solar system contains a healthy ecosystem of bodies, including a multitude of dwarf planets (like Pluto), a handful of Earth-like solid planets, and a similar number of giant planets. It is natural to wonder about the origin of all these planets. Over the past two decades, the number of planets that we can study have increased from a mere 8 to thousands. The observations of extra-solar debris disks also disclose the presence of dwarf planets around other stars. A new framework for planet formation is called for, to explain the astounding diversity as well as the emergent universality observed in these systems. We propose a theoretical research program to answer the following questions: How do a planetary system, emerging out of the gaseous disk that disappears after a few million years, manage to maintain their stability billions of years? What organize them into their observed peaceful coexistence? Orbits of our terrestial planets are chaotic, but, fortunately, with a stability lifetime comparable to the solar system lifetime. Who orders that? Is this also true for other planetary systems? Do majority of planetary systems look at all like our solar system? We will also study the Kuiper belt region to address these questions: How do Pluto and other Kuiper belt objects form in our solar system? Many stars have debris disks orders of of magnitude brighter than our own Kuiper belt. Why is ours so anemic? Are solid materials in these bright disks forming into Earth-like or even Neptune-like planets? Or is planet formation in these regions stalled by stirring by sibling giant planets? Answers to these questions provide us with important pieces to unravel the great mystery of how planets arise. Our study is a part of the human endeavour of trying to find our place in the cosmos.
我们的太阳系包含一个健康的天体生态系统,包括大量的矮行星(如冥王星),少数类地固体行星和类似数量的巨行星。想知道所有这些行星的起源是很自然的。在过去的二十年里,我们可以研究的行星数量已经从区区8个增加到数千个。对太阳系外碎片盘的观测也揭示了其他恒星周围存在矮行星。人们需要一个新的行星形成框架,来解释在这些系统中观察到的惊人的多样性和新兴的普遍性。

项目成果

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Wu, Yanqin其他文献

An Ω-3 fatty acid-deficient diet during gestation induces depressive-like behavior in rats: the role of the hypothalamo-pituitary-adrenal (HPA) system
  • DOI:
    10.1039/c7fo01714f
  • 发表时间:
    2018-06-01
  • 期刊:
  • 影响因子:
    6.1
  • 作者:
    Tang, Mimi;Liu, Yiping;Wu, Yanqin
  • 通讯作者:
    Wu, Yanqin
Identifying optimal candidates for post-TIPS patients with HCC undergoing TACE: a multicenter observational study.
  • DOI:
    10.1007/s00330-022-09249-6
  • 发表时间:
    2023-04
  • 期刊:
  • 影响因子:
    5.9
  • 作者:
    Fan, Wenzhe;Zhu, Bowen;Yue, Shufan;Zheng, Xinlin;Yuan, Guosheng;Yu, Lei;Huang, Wanchang;Huang, Shugui;Wei, Wenjiang;Li, Fuliang;Huang, Zhen;Tang, Rong;Fan, Huishuang;Li, Zhuoyong;Qiao, Liangliang;Huang, Fuxi;Cheng, Yu;Zhang, Yingqiang;Wu, Yanqin;Zou, Xinhua;Xue, Miao;Wang, Hongyu;Li, Jiaping
  • 通讯作者:
    Li, Jiaping
Prognostic Value of TP53 Mutation for Transcatheter Arterial Chemoembolization Failure/Refractoriness in HBV-Related Advanced Hepatocellular Carcinoma
TP53 突变对 HBV 相关晚期肝细胞癌经导管动脉化疗栓塞失败/难治性的预后价值
  • DOI:
    10.4143/crt.2019.533
  • 发表时间:
    2020-07-01
  • 期刊:
  • 影响因子:
    4.6
  • 作者:
    Xue, Miao;Wu, Yanqin;Li, Jiaping
  • 通讯作者:
    Li, Jiaping
KEPLER PLANETS: A TALE OF EVAPORATION
  • DOI:
    10.1088/0004-637x/775/2/105
  • 发表时间:
    2013-10-01
  • 期刊:
  • 影响因子:
    4.9
  • 作者:
    Owen, James E.;Wu, Yanqin
  • 通讯作者:
    Wu, Yanqin
Postintervention Interleukin-6 (IL-6) Level, Rather than the Pretreatment or Dynamic Changes of IL-6, as an Early Practical Marker of Tumor Response in Hepatocellular Carcinoma Treated with Transarterial Chemoembolization
  • DOI:
    10.1634/theoncologist.2018-0669
  • 发表时间:
    2019-12-01
  • 期刊:
  • 影响因子:
    5.8
  • 作者:
    Wu, Yanqin;Fan, Wenzhe;Li, Jiaping
  • 通讯作者:
    Li, Jiaping

Wu, Yanqin的其他文献

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{{ truncateString('Wu, Yanqin', 18)}}的其他基金

Tidal Processes in Planetary and Stellar Systems
行星和恒星系统中的潮汐过程
  • 批准号:
    RGPIN-2018-05886
  • 财政年份:
    2022
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Tidal Processes in Planetary and Stellar Systems
行星和恒星系统中的潮汐过程
  • 批准号:
    RGPIN-2018-05886
  • 财政年份:
    2021
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Tidal Processes in Planetary and Stellar Systems
行星和恒星系统中的潮汐过程
  • 批准号:
    RGPIN-2018-05886
  • 财政年份:
    2020
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Tidal Processes in Planetary and Stellar Systems
行星和恒星系统中的潮汐过程
  • 批准号:
    RGPIN-2018-05886
  • 财政年份:
    2019
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Tidal Processes in Planetary and Stellar Systems
行星和恒星系统中的潮汐过程
  • 批准号:
    RGPIN-2018-05886
  • 财政年份:
    2018
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Planetary Systems: from Plutos to Jupiters
行星系统:从冥王星到木星
  • 批准号:
    261952-2012
  • 财政年份:
    2016
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Planetary Systems: from Plutos to Jupiters
行星系统:从冥王星到木星
  • 批准号:
    261952-2012
  • 财政年份:
    2014
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Planetary Systems: from Plutos to Jupiters
行星系统:从冥王星到木星
  • 批准号:
    261952-2012
  • 财政年份:
    2013
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Planetary Systems: from Plutos to Jupiters
行星系统:从冥王星到木星
  • 批准号:
    261952-2012
  • 财政年份:
    2012
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual
Disks around stars and planets
恒星和行星周围的圆盘
  • 批准号:
    261952-2007
  • 财政年份:
    2011
  • 资助金额:
    $ 1.82万
  • 项目类别:
    Discovery Grants Program - Individual

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