Toward a Realistic Model of the Formation of Terrestrial Planets and Water Delivery

类地行星形成和供水的现实模型

基本信息

  • 批准号:
    2109285
  • 负责人:
  • 金额:
    $ 30.12万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Standard Grant
  • 财政年份:
    2021
  • 资助国家:
    美国
  • 起止时间:
    2021-09-15 至 2024-08-31
  • 项目状态:
    已结题

项目摘要

A team from the Planetary Science Institute will study the origin of planet Earth and its oceans by answering how Earth formed and how a large amount of water appeared on it. This project has the potential to explain how the moon formed, how many times in the past Earth was hit by asteroids, and whether it will be hit again. The origin of Earth and other small planets of our solar system, especially Mars and Venus is unknown. Revealing how these planets form will shed light on whether life existed on other planets, and whether they have the resources needed for permanent human presence. The team have developed a detailed plan on involving undergraduate and high school students in summer projects, reaching out to minorities and under-represented communities.Although many efforts have been made to determine how Earth formed, no realistic modeling yet exists. The work of the investigators will advance our knowledge of the formation of Earth and the origin of its water by presenting the most accurate pathway to the formation of the inner solar system. The investigators have developed a novel approach in which they use computer simulations to accurately create collisions between large bodies (as large as asteroids and moons) and follow the process until a complete planet has formed. The team have developed a mechanism to demonstrate how water is transferred from one object to the other during large collisions, and how it reaches the region of space where Earth forms. The team have created a unique computer code that can carry out all these processes simultaneously. They plan to perform several hundred computer simulations and study the results to identify the most viable mechanism for the formation of Earth and its water.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
来自行星科学研究所的一个小组将通过回答地球是如何形成的以及地球上大量水是如何出现的,来研究地球及其海洋的起源。这个项目有可能解释月球是如何形成的,过去地球被小行星撞击了多少次,以及它是否会再次被撞击。地球和太阳系的其他小行星,特别是火星和金星的起源是未知的。揭示这些行星是如何形成的,将揭示其他行星上是否存在生命,以及它们是否拥有人类永久存在所需的资源。该团队制定了一个详细的计划,让本科生和高中生参与暑期项目,向少数民族和代表性不足的社区伸出援手。尽管人们做出了许多努力来确定地球是如何形成的,但目前还没有一个真实的模型。研究人员的工作将通过展示太阳系内部形成的最准确途径,提高我们对地球形成及其水的起源的认识。研究人员开发了一种新颖的方法,他们使用计算机模拟来精确地制造大型物体(如小行星和卫星)之间的碰撞,并跟踪这一过程,直到一个完整的行星形成。该团队已经开发出一种机制来演示水是如何在大型碰撞中从一个物体转移到另一个物体的,以及水是如何到达地球形成的空间区域的。该团队创造了一种独特的计算机代码,可以同时执行所有这些过程。他们计划进行数百次计算机模拟,并研究结果,以确定地球及其水形成的最可行机制。该奖项反映了美国国家科学基金会的法定使命,并通过使用基金会的知识价值和更广泛的影响审查标准进行评估,被认为值得支持。

项目成果

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Nader Haghighipour其他文献

Detection of Earth-mass and super-Earth Trojan planets using transit timing variation method
  • DOI:
    10.1007/s10569-013-9510-y
  • 发表时间:
    2013-08-11
  • 期刊:
  • 影响因子:
    1.400
  • 作者:
    Nader Haghighipour;Stephanie Capen;Tobias C. Hinse
  • 通讯作者:
    Tobias C. Hinse
On the asymptotic character of electromagnetic waves in a Friedmann–Robertson–Walker universe
  • DOI:
    10.1007/s10714-005-0022-2
  • 发表时间:
    2005-02-01
  • 期刊:
  • 影响因子:
    2.800
  • 作者:
    Nader Haghighipour
  • 通讯作者:
    Nader Haghighipour
MAIN-BELT COMET P/2012 T1 (PANSTARRS)
主带彗星 P/2012 T1 (PANSTARRS)
  • DOI:
    10.1088/2041-8205/771/1/l1
  • 发表时间:
    2013
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Henry H. Hsieh;Heather M. Kaluna;Bojan Novakovic;Bin Yang;Nader Haghighipour;Marco Micheli;Larry Denneau;Alan Fitzsimmons;Robert Jedicke;Jan Kleyna;Peter Veres;Richard J. Wainscoat;Megan Ansdell;Garrett T. Elliott;Jacqueline V. Keane;Karen J. Meech;Nicholas A. Moskovitz;Timm E. Riesen;Scott S. Sheppard;Sarah Sonnett;David J. Tholen;Laurie Urban;Nick Kaiser;K. C. Chambers;William S. Burgett;Eugene A. Magnier;Jeffrey S. Morgan;Paul A. Price
  • 通讯作者:
    Paul A. Price

Nader Haghighipour的其他文献

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{{ truncateString('Nader Haghighipour', 18)}}的其他基金

A Meeting of the PIs of the NSF REU Sites in Astronomy
NSF REU 天文学站点 PI 会议
  • 批准号:
    1848922
  • 财政年份:
    2018
  • 资助金额:
    $ 30.12万
  • 项目类别:
    Standard Grant
REU Site: Astronomy in Hawai`i
REU 站点:夏威夷的天文学
  • 批准号:
    1560413
  • 财政年份:
    2016
  • 资助金额:
    $ 30.12万
  • 项目类别:
    Continuing Grant

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