Search for extrasolar terrestrial planets by the microlensing follow up network
| Project/Area Number |
20340052
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| Research Category |
Grant-in-Aid for Scientific Research (B)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | Nagoya University |
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Principal Investigator |
ABE Fumio Nagoya University, 太陽地球環境研究所, 准教授 (80184224)
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| Co-Investigator(Kenkyū-buntansha) |
SUMI Takahiro 名古屋大学, 太陽地球環境研究所, 助教授 (30432214)
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| Project Period (FY) |
2008 – 2010
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| Project Status |
Completed (Fiscal Year 2010)
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| Budget Amount *help |
¥12,480,000 (Direct Cost: ¥9,600,000、Indirect Cost: ¥2,880,000)
Fiscal Year 2010: ¥3,640,000 (Direct Cost: ¥2,800,000、Indirect Cost: ¥840,000)
Fiscal Year 2009: ¥3,640,000 (Direct Cost: ¥2,800,000、Indirect Cost: ¥840,000)
Fiscal Year 2008: ¥5,200,000 (Direct Cost: ¥4,000,000、Indirect Cost: ¥1,200,000)
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| Keywords | 宇宙物理 / 光学赤外線天文学 / 惑星起源・進化 |
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| Research Abstract |
Follow up observations of microlensing events were executed by world-wide observation network to find extrasolar planets. New planets (MOA-2007-BLG-192Lb, MOA-2008-BLG-310Lb、MOA-2009-BLG-319Lb) have been discovered. From the analysis of the distribution of planets, it is concluded that cold neptunes are common. As a by-product of microlensing observation, planet search with Transit Timing Variation method was done using B&C telescope. Then, a limit on the existence of second planets was imposed for WASP-5.
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Report
(4 results)
Research Products
(85 results)
