Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-24T18:43:09.812Z Has data issue: false hasContentIssue false
  • English
  • Français

China NEO Survey Telescope and its preliminary achievement

Published online by Cambridge University Press:  01 October 2007

H. B. Zhao ,
J. S. Yao  and
H. Lu
H. B. Zhao
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: [email protected] National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
J. S. Yao
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: [email protected] National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
H. Lu
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China email: [email protected] National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In recent years, there has been an increasing appreciation for the hazards posed by Near Earth Objects (NEOs), those asteroids and periodic comets whose motions can bring them into the Earth's neighborhood. An NEO Survey Telescope (NEOST) was built in China to be taken part in the international NEO joint survey. This telescope is a 1.0/1.2m Schmidt telescope, equipped with a 4K by 4K CCD detector with a drift-scanning function. After adjusting the telescope and test observations, in December 2006 the NEOST began its NEO survey program. We have found 188 new asteroids including an NEO – 2007 JW2 and one periodic comet –P/2007 S1 (Zhao).

Keywords

telescopesasteroidssurveysastrometry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S248: A Giant Step: from Milli- to Micro-arcsecond Astrometry , October 2007 , pp. 565 - 566
Copyright
Copyright © International Astronomical Union 2008