太陽系小天體之綜合的理解; Comprehensive Understanding of Solar System Small Bodies

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/45770

Title:	太陽系小天體之綜合的理解;Comprehensive Understanding of Solar System Small Bodies
Authors:	木下大輔
Contributors:	天文學研究所
Keywords:	物理類
Date:	2008-07-01
Issue Date:	2010-12-28 15:27:42 (UTC+8)
Publisher:	行政院國家科學委員會
Abstract:	Small solar system bodies are thought to be remnants of planetesimals from which the major objects in the solar system formed. Because of their primordial characteristics, it is important to know the basic properties of the small solar system bodies, such as size distribution, spatial distribution, physical properties and chemical composition in order to understand the origin and evolution of the solar system. This program utilizes Lulin Observatory in Taiwan, Japanese space infrared telescope "Akari", and the Pan-STARRS in Hawaii to provide comprehensive understanding of small solar system bodies. The Pan-STARRS is a project to monitor the sky visible from Hawaii every week to detect transient objects. The Pan-STARRS database is used to search for comet-asteroid transition objects and young collisional family members, and to construct the phase angle dependence of the brightness of asteroids. Scientifically interesting objects are extensively followed up by 1-m and 2-m telescopes at Lulin Observatory to study the surface properties of objects. The whole-sky-survey data of space infrared telescope "Akari" is used to estimate the size and albedo of more than 5000 asteroids. This program tries to accumulate basic properties of asteroid and establish the standard database for coming decades. 研究期間：9608 ~ 9707
Relation:	財團法人國家實驗研究院科技政策研究與資訊中心
Appears in Collections:	[Graduate Institute of Astronomy] Research Project

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