Rchr
J-GLOBAL ID：200901036790346958
Update date: Aug. 28, 2020
Sekiya Minoru
セキヤ ミノル | Sekiya Minoru
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Affiliation and department：
Kyushu University Faculty of Sciences, Department of Earth and Planetary Sciences
About Kyushu University Faculty of Sciences, Department of Earth and Planetary Sciences
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Detailed information
Job title：
Professor
Homepage URL (1)：
https://jupiter.geo.kyushu-u.ac.jp/
Research field (2)：
Solid earth science
, Astronomy
Research keywords (2)：
惑星科学
, planetary science
Research theme for competitive and other funds (6)：
コンドライト隕石の形成
原始惑星系円盤の形成と進化
太陽系の起源
Formation of Chondrites
Formation and evolution of the protoplanetary disk
Origin of the solar system
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MISC (56)：
Masayuki Uesugi, Minoru Sekiya, Tomoki Nakamura. Kinetic stability of a melted iron globule during chondrule formation. I. Non-rotating model. METEORITICS & PLANETARY SCIENCE. 2008. 43. 4. 717-730
Shigeru Wakita, Minoru Sekiya. Numerical simulations of the gravitational instability in the dust layer of a protoplanetary disk using a thin disk model. ASTROPHYSICAL JOURNAL. 2008. 675. 2. 1559-1575
Fumiharu Yamoto, Minoru Sekiya. Two evolutionary paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk. ASTROPHYSICAL JOURNAL. 2006. 646. 2. L155-L158
Fumiharu Yamoto, Minoru Sekiya. Two evolutional paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk. Astrophys.J.646:L155-L158,2006. 2006
Fumiharu Yamoto, Minoru Sekiya. Two evolutionary paths of an axisymmetric gravitational instability in the dust layer of a protoplanetary disk. Astrophysical Journal. 2006. 646. L155-158
ｍore...
Books (1)：
Shear instability of the solar nebula
Primitive solar nebula and origin of planets, Terra Scientific Publishing Company 1993
Professional career (1)：
(BLANK)
Association Membership(s) (2)：
日本天文学会
, 日本惑星科学会
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