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Monitoring of Venus and Mars atmosphere by time varying gravity field observation

Research Project

Project/Area Number 15K13565
Research Category

Grant-in-Aid for Challenging Exploratory Research

Allocation TypeMulti-year Fund
Research Field Solid earth and planetary physics
Research InstitutionNational Astronomical Observatory of Japan (2016-2018)
Japan Aerospace EXploration Agency (2015)

Principal Investigator

Yamamoto Keiko  国立天文台, RISE月惑星探査検討室, 特任研究員 (40452263)

Project Period (FY) 2015-04-01 – 2019-03-31
Project Status Completed (Fiscal Year 2018)
Budget Amount *help
¥2,600,000 (Direct Cost: ¥2,000,000、Indirect Cost: ¥600,000)
Fiscal Year 2017: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2016: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2015: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Keywords衛星重力観測 / 時間変動重力場 / 火星大気変動モニタリング / 衛星重力観測シミュレーション / 惑星大気
Outline of Final Research Achievements

In this study, we aimed to monitor circulation of planetary atmosphere as time-varying gravity field by satellite gravimetry. We improved the software, which was originally developed for precise estimation of the Earth-rotating satellite orbit and the earth's gravity field, so that it can be used for the orbit simulation to monitor temporal gravity field change accompanying planetary atmosphere variation. We focused on Mars atmosphere, analyzed the atmospheric circulation model for about 9 years, and extracted atmospheric surface pressure, dry ice, water ice, dust, annual, semi-annual, seasonal fluctuation components. Then these components are converted to the observed value from gravity measurement satellites. Using these data sets, we conducted simulation of the gravity field observation. Some parameters, such as measurement method, satellite's orbit and observation period, were changed and optimized in the simulation for more efficient observation.

Academic Significance and Societal Importance of the Research Achievements

本研究で実施されたシミュレーションの結果に基づき、実際に惑星大気の観測が実現された場合の、その学術的な意義は次の通りである。火星をはじめとする大気を持った惑星において、大気の循環を観測し、その運動を正しく理解することは、惑星表層の熱輸送メカニズム、気象・気候メカニズムを解明する上で重要であり、本研究で検出の対象とした質量の時間変化としての大気変動は、このメカニズムに対し、定量面での規定を与えるという役割を持つ。これは従来の気象観測では直接に得ることのできない新しい観測量であり、既存の観測、大気モデルとは独立であることから、既存の惑星大気循環モデルの検証にも役立つと予想される。

Report

(5 results)
  • 2018 Annual Research Report   Final Research Report ( PDF )
  • 2017 Research-status Report
  • 2016 Research-status Report
  • 2015 Research-status Report
  • Research Products

    (2 results)

All 2018 2016

All Presentation (2 results) (of which Int'l Joint Research: 1 results)

  • [Presentation] Simulation Study to Monitor Planetary Atmospheric Circulation by Satellite Gravimetry2018

    • Author(s)
      Keiko Yamamoto
    • Organizer
      2018 AGU Fall Meeting
    • Related Report
      2018 Annual Research Report
    • Int'l Joint Research
  • [Presentation] はやぶさ2クロスオーバー解析のシミュレーション(1)2016

    • Author(s)
      山本圭香, 松本晃治, 大坪俊通, 並木則行, はやぶさ2アストロダイナミクスチーム
    • Organizer
      日本測地学会第126回講演会
    • Place of Presentation
      奥州市文化会館(岩手県・奥州市)
    • Year and Date
      2016-10-19
    • Related Report
      2016 Research-status Report

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Published: 2015-04-16   Modified: 2020-03-30  

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