Center for Planetary Science
Hot News
- 2024-05-20 GFD Seminar, U Kenyo(University of Tokyo) "Evolution of the lunar interior caused by magmatism and mantle convection" Online by Zoom (Japanese page only) (June 6, 2024)
- 2024-05-17 GFD Seminar, OGASAWARA Koji(Kyoto University) "全球数値予報に向けた動径基底関数離散化手法" Online by Zoom (Japanese page only) (June 3, 2024)
- 2024-05-17 CPS Seminar, IWASAKI Kazunari (National Astronomical Observatory of Japan) "Dynamics near the inner Dead-zone edges in a protoplanetary disk" (June 3, 2024)
- 2024-05-17 The 14th meeting on Cosmic Dust@Nagoya University (August 5-9, 2024)
- 2023-11-16 Associate Prof. Takayuki Saitoh, who is a member of Program for Promoting Research on the Supercomputer Fugaku" (Structure and Evolution of the Universe Unraveled by Fusion of Simulation and AI) and collaborators, Junichi Baba (Kagoshima University) and Takuji Tsujimoto (NAOJ), studied the enrichment process of the primary elements in the MilkyWay galaxy and found that the Sun's birthplace would be the inner region of the Milky Way galaxy compared to its current position. This model also predicts the distribution of the elements of the planetary materials in time and space. According to this, stars in the inner part of the Milkyway galaxy is more likely to host massive planets, while those in the outer part are more likely to form water-rich planets.
(Japanese page only)
- 2023-10-24 Mr. Keiya Hirashima, who is a graduate student of the University of Tokyo and a member of Program for Promoting Research on the Supercomputer Fugaku" (Structure and Evolution of the Universe
Unraveled by Fusion of Simulation and AI) and collaborators have developed a new method to reproduce the result of the simulation of the expansion of the Supernova shell using deep learning.
- 2023-09-14 Associate Prof. Tomoaki Ishiyama (Chiba University) who are members of "Program for Promoting Researches on the Supercomputer Fugaku" (Toward a unified view of the universe: from large scale structures to planets), and collaborators have determined the relation between the mass and number of clusters of galaxies using the member galaxies of the clusters.
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