• Title/Summary/Keyword: 지구근접 소행성

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Technological Trends in NEO Space Missions (NEO 우주탐사의 기술 동향)

  • Yoon, Yong-Sik;Choi, Jung-Su;Kim, Hyung-Wan
    • Current Industrial and Technological Trends in Aerospace
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    • v.9 no.1
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    • pp.102-109
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    • 2011
  • NEOs are comets and asteroids that have been nudged by the gravitational attraction of nearby planets into orbits that allow them to enter the Earth's neighborhood. When the NEOs with certain size impact in the Earth's surface, it could cause a serious disaster. However, the NEOs that are potentially the most hazardous because they can closely approach the Earth are also the objects that could bemost easily exploited for their raw materials. This paper presents the characteristics of NEOs and the technology trend of advanced countries on spacecraft missions to comets and asteroids.

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Geocentric parallax measurements of Near-Earth Asteroid using Baselines with domestic small-size observatories (국내 소형천문대 기선을 이용한 근접 소행성 지심시차 측정)

  • Jeong, Eui Oan;Sohn, Jungjoo
    • Journal of the Korean earth science society
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    • v.37 no.7
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    • pp.398-407
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    • 2016
  • We cooperated with four domestic educational astronomical observatories to construct a baseline and perform simultaneous observations to determine the geocentric parallax, distance, and motion of 1036 Ganymed, an Amor asteroid near the Earth. Observations were made on the day when simultaneous observations were possible from September to November 2011. Measured distances of 1036 Ganymed were 0.394 AU on Sept. 26, 0.365 AU on Oct. 11, and 0.340 AU on Oct. 25, respectively, which were within the error range as compared with the measured distances proposed by the US Jet Propulsion Laboratory. The 1036 Ganymed showed a tilting motion during the observation period, and the tangential angular velocities were measured at $0.037-0.052^{{\prime {\prime}}\;sec^{-1}$. Through this study, it was shown that the simultaneous observations among educational astronomical observations can obtain distance measurements with an error range of about 5% for asteroids near 0.4 AU. And it expected to be used as a research & education program emphasizing collaborative observation activities based on a network between observatories.