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Possibility of the evaporation of planetesimals in the protoplanetary disk

Research Project

Project/Area Number 25610133
Research Category

Grant-in-Aid for Challenging Exploratory Research

Allocation TypeMulti-year Fund
Research Field Solid earth and planetary physics
Research InstitutionKurume University (2015)
Tokyo Institute of Technology (2013-2014)

Principal Investigator

Nagasawa Makiko  久留米大学, 医学部, 准教授 (00419847)

Project Period (FY) 2013-04-01 – 2016-03-31
Project Status Completed (Fiscal Year 2015)
Budget Amount *help
¥3,510,000 (Direct Cost: ¥2,700,000、Indirect Cost: ¥810,000)
Fiscal Year 2015: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2014: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2013: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Keywords惑星起源・進化
Outline of Final Research Achievements

When the relative velocity between a planetesimal and the gas disk exceeds the speed of sound of the gas, a bow shock is produced. We find that the velocities relative to the gas disk of planetesimals a few hundred kilometers in size exceed 10 km/s in the asteroid region due to the mean-motion resonance and the secular resonance of a Jovian planet. The shock is enough strong to cause the evaporation of icy planetesimal. Our results also suggest that chondrules were produced effectively by the bow shocks.

Report

(4 results)
  • 2015 Annual Research Report   Final Research Report ( PDF )
  • 2014 Research-status Report
  • 2013 Research-status Report
  • Research Products

    (5 results)

All 2015 2014 2013 Other

All Journal Article (2 results) (of which Peer Reviewed: 2 results,  Open Access: 1 results,  Acknowledgement Compliant: 1 results) Presentation (3 results)

  • [Journal Article] REVISITING JOVIAN-RESONANCE INDUCED CHONDRULE FORMATION2014

    • Author(s)
      M. Nagasawa , K. K. Tanaka, H. Tanaka, T. Nakamoto, H. Miura, and T. Yamamoto
    • Journal Title

      The Astrophysical Journal Letters

      Volume: 794 Issue: 1 Pages: 1-5

    • DOI

      10.1088/2041-8205/794/1/l7

    • Related Report
      2014 Research-status Report
    • Peer Reviewed / Open Access / Acknowledgement Compliant
  • [Journal Article] Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse2013

    • Author(s)
      K.Masuda et al.
    • Journal Title

      The Astrophysical Journal

      Volume: 778 Issue: 2 Pages: 185-185

    • DOI

      10.1088/0004-637x/778/2/185

    • Related Report
      2013 Research-status Report
    • Peer Reviewed
  • [Presentation] 惑星散乱と潮汐相互作用2015

    • Author(s)
      長澤真樹子
    • Organizer
      日本惑星科学会2015年秋季講演会
    • Place of Presentation
      東京工業大学
    • Year and Date
      2015-10-15
    • Related Report
      2015 Annual Research Report
  • [Presentation] 木星の共鳴による微惑星の軌道進化2014

    • Author(s)
      長沢真樹子
    • Organizer
      日本惑星科学会2014年秋季講演会
    • Place of Presentation
      東北大学片平キャンパス
    • Year and Date
      2014-09-24
    • Related Report
      2014 Research-status Report
  • [Presentation] 原始惑星系円盤内で高速になる微小天体の軌道進化

    • Author(s)
      長沢真樹子
    • Organizer
      日本惑星科学会2013年秋季講演会
    • Place of Presentation
      石垣島市民会館(沖縄県)
    • Related Report
      2013 Research-status Report

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Published: 2014-07-25   Modified: 2019-07-29  

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