Search for Traces of Giant Impacts of Rocky Planets with Silica Feature
Project/Area Number |
25707009
|
Research Category |
Grant-in-Aid for Young Scientists (A)
|
Allocation Type | Partial Multi-year Fund |
Research Field |
Astronomy
|
Research Institution | The University of Tokyo |
Principal Investigator |
Sako Shigeyuki 東京大学, 理学(系)研究科(研究院), 助教 (90533563)
|
Research Collaborator |
KAMIZUKA Takafumi
UCHIYAMA Masahito
YAMAGUCHI Jumpei
|
Project Period (FY) |
2013-04-01 – 2017-03-31
|
Project Status |
Completed (Fiscal Year 2016)
|
Budget Amount *help |
¥18,720,000 (Direct Cost: ¥14,400,000、Indirect Cost: ¥4,320,000)
Fiscal Year 2016: ¥4,030,000 (Direct Cost: ¥3,100,000、Indirect Cost: ¥930,000)
Fiscal Year 2015: ¥3,770,000 (Direct Cost: ¥2,900,000、Indirect Cost: ¥870,000)
Fiscal Year 2014: ¥8,060,000 (Direct Cost: ¥6,200,000、Indirect Cost: ¥1,860,000)
Fiscal Year 2013: ¥2,860,000 (Direct Cost: ¥2,200,000、Indirect Cost: ¥660,000)
|
Keywords | 系外惑星 / 中間赤外線 / 観測装置 / 監視観測 / 赤外線 / ダスト / 巨大惑星 / 巨大衝突 |
Outline of Final Research Achievements |
A rocky planet acquires mass through multiple giant impact events. We consider silica, which is produced only under a high temperature and high pressure condition, as a tracer of the giant impacts and investigate the impact events by observing a shape and time variation of silica feature in 10 microns radiated from young exo-planets with the mid-infrared instrument MIMIZUKU. MIMIZUKU can obtain spectra in the 10-micron band with high accuracy by a field stacker unit. In this study, we have developed sensor units, opto-mechanical units, and the field stacker unit of MIMIZUKU and successfully completed integrated tests after assembling them into a vacuum dewar and an optical system. We also have planned spectroscopic monitoring observations with MIMIZUKU on the Subaru telescope.
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Report
(5 results)
Research Products
(20 results)