2009 Fiscal Year Final Research Report
Construction of a structure evolution model of small solar system bodies by numerical simulations of aggregate collisions
Project/Area Number |
20740247
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Research Category |
Grant-in-Aid for Young Scientists (B)
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Allocation Type | Single-year Grants |
Research Field |
Solid earth and planetary physics
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Research Institution | Hokkaido University |
Principal Investigator |
WADA Koji Hokkaido University, 惑星探査研究センター, 上席研究員 (10396856)
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Project Period (FY) |
2008 – 2009
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Keywords | 惑星形成・進化 / 衝突 / ダスト / 微惑星 |
Research Abstract |
Small solar system bodies, such as comets and asteroids, are considered to be remnants of planetesimals formed through collisional growth of dust aggregates consisting of submicron grains in a protoplanetary disk. We carried out numerical simulations of collisions of dust aggregates to construct a structure evolution model of planetesimals and small solar system bodies. We reveal that very low density planetesimals are inevitably formed as a result of collisional growth of dust aggregates and such process leads small solar system bodies to have low density structures we observe at present.
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[Journal Article] Collisional process on comet 9/P Tempel 1: Mass loss of its dust and ices by impacts of asteroidal objects and its collisional history2010
Author(s)
Yamamoto, S., Wada, K., Kobayashi, H., Kimura, H., Ishiguro, M., Matsui, T.
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Journal Title
Earth Planet. Space 62
Pages: 5-11
Peer Reviewed
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[Journal Article] Growth and disruption of dust aggregates by Collisions, Proceedings of Cosmic Dust2009
Author(s)
Wada, K., Tanaka, H., Suyama, T., Kimura, H., Yamamoto, T.
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Journal Title
Near & Far 2008 in Astoronomical Society of the Pacific (in press)
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[Journal Article] Comet 9P/Tempel 1: Interpretation with the Deep Impact Results2008
Author(s)
Yamamoto, S., Kimura, H., Zubko, E., Kobayashi, H., Wada, K., Ishiguro, M., Matsui, T.
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Journal Title
Astrophys. J. 673
Pages: L199-L202
Peer Reviewed
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[Presentation] Collisional Growth Possibility of Dust Aggregates: A Bouncing Problem, Lunar Planet2010
Author(s)
Wada, K., Tanaka, H., Suyama, T., Kimura, H., Yamamoto, T.
Organizer
Sci. Conf. 41th
Place of Presentation
Woodlands, TX, USA
Year and Date
20100000
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[Presentation] Numerical Simulation of Dust Aggregate Collisions: Growth and Disruption of Dust Aggregates2009
Author(s)
Wada, K., Tanaka, H., Suyama, T., Kimura, H., Yamamoto, T.
Organizer
Exoplanets and Disks: Their formation and Diversity, The 2nd Subaru International Conference
Place of Presentation
Keauhou, Hawaii, USA
Year and Date
2009-03-11
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[Presentation] Growth and disruption of dust aggregates by collisions2008
Author(s)
Wada, K., Tanaka, H., Suyama, T., Kimura, H., Yamamoto, T.
Organizer
Cosmic Dust - Near & Far
Place of Presentation
Heidelberg, Germany
Year and Date
20080000
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[Presentation] Numerical Simulation of Dust Aggregate Collisions: Compression and Disruption of 3D Aggregates2008
Author(s)
Wada, K., Tanaka, H., Suyama, T., Kimura, H., Yamamoto, T.
Organizer
Asia Oceania Geosciences Society 5th Annual Meeing
Place of Presentation
Busan, Korea
Year and Date
2008-06-18
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