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NEO search telescope in China

Published online by Cambridge University Press:  01 August 2006

Yuehua Ma ,
Haibin Zhao  and
Dazhi Yao
Yuehua Ma
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China email: [email protected]
Haibin Zhao
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China email: [email protected]
Dazhi Yao
Affiliation:
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China email: [email protected]
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Abstract

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Chinese scientists have contributed many research works to the field of asteroid surveying and related topics. In the early 1960s, Purple Mountain Observatory (PMO) began observing asteroids and found over 130 new numbered asteroids during the following decades. The Schmidt CCD Asteroid Program (SCAP) of Beijing Astronomical Observatory (BAO) started in 1995 and found 575 asteroids in several years.

NEOs represent a great threat to the near-Earth environment by closely approaching Earth or even impacting with Earth. After the impact of comet SL9 on Jupiter, Chinese proposed to build a NEO Search Telescope to take part in the joint international NEO survey. It is a 1.0/1.2 m Schmidt telescope with a 4K×4K drift scanning CCD detector. Here we elaborate upon its applications to objects of scientific interest, its parameters, and its observing station.

Keywords

Surveytelescopeobservation site
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S236: Near Earth Objects, our Celestial Neighbors: Opportunity and Risk , August 2006 , pp. 381 - 384
Copyright
Copyright © International Astronomical Union 2007

References

Boattini, A. & Carusi, A. 1997, Vistas in Astronomy 41, 527CrossRefGoogle Scholar
Bottke, W. F., Morbidelli, A., Jedicke, R., Petit, J.-M., Levison, H. F., Michel, P., Metcalfe, T. S. 2002, Icarus 156, 399CrossRefGoogle Scholar
Carusi, A., Gehrels, T., Helin, E. F., Marsden, B. G., Russell, K. S., Shoemaker, C. S., Shoemaker, E. M., Steel, D. I. 1994, in: Gehrels, T. (eds.), Hazards Due to Comets and Astroids (University of Arizona Press, Tucson), p. 127Google Scholar
D'Abramo, G., Harris, A. W., Boattini, A., Werner, S. C., Harris, A. W., Valsecchi, G. B. 2001, Icarus 153, 214CrossRefGoogle Scholar
Gehrels, T. & Jedicke, R. 1995, Earth, Moon and Planets 72, 233CrossRefGoogle Scholar
Stokes, G. H., Evans, J. B., Viggh, E. M., Shelly, F. C., & Pearce, E. C. 2000, Icarus 148, 21CrossRefGoogle Scholar