Evolution of Protoplanetary disks and Formation of Gas Giant Planets
| Project/Area Number |
19740279
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Solid earth and planetary physics
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| Research Institution | Waseda University |
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Principal Investigator |
INABA Satoshi Waseda University, 国際教養学術院, 講師 (30409718)
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| Project Period (FY) |
2007 – 2009
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| Project Status |
Completed (Fiscal Year 2009)
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| Budget Amount *help |
¥3,870,000 (Direct Cost: ¥3,300,000、Indirect Cost: ¥570,000)
Fiscal Year 2009: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2008: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2007: ¥1,400,000 (Direct Cost: ¥1,400,000)
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| Keywords | 惑星形成 / 進化 / 惑星形成・進化 / 理論天文学 / 計算物理学 |
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| Research Abstract |
We study a new mechanism to explain the formation of gas giant planets. A gas giant planet is formed while a protoplanetary disk evolves. We introduced some elementary processes (e.g., self gravity) into the numerical program to simulate the evolution of a protoplanetary disk. Using the developed numerical program, we simulated the evolution of a protoplanetary disk and found that some vortices with the mass of a gas giant planet are formed in a protoplanetary disk. The vortices are thought to evolve into a gas giant planet.
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Report
(4 results)
Research Products
(13 results)
