DOI QR코드

DOI QR Code

Development of Adaptive Optics System for the Geochang 100 cm Telescope

  • Hyung-Chul Lim (Korea Astronomy and Space Science Institute) ;
  • Francis Bennet (Research School of Astronomy and Astrophysics, Australian National University) ;
  • Sung-Yeol Yu (Korea Astronomy and Space Science Institute) ;
  • Ian Price (Research School of Astronomy and Astrophysics, Australian National University) ;
  • Ki-Pyoung Sung (Korea Astronomy and Space Science Institute) ;
  • Mansoo Choi (Korea Astronomy and Space Science Institute)
  • Received : 2024.05.10
  • Accepted : 2024.07.23
  • Published : 2024.08.31

Abstract

Korea Astronomy and Space science Institute (KASI) partnered with the Australian National University (ANU) to develop the adaptive optics (AO) system at the Geochang observatory with a 100 cm optical telescope for multiple applications, including space geodesy, space situational awareness and Korean space missions. The AO system is designed to get high resolution images of space objects with lower magnitude than 10 by using themselves as a natural guide star, and achieve a Strehl ratio larger than 20% in the environment of good seeing with a fried parameter of 12-15 cm. It will provide the imaging of space objects up to 1,000 km as well as its information including size, shape and orientation to improve its orbit prediction precision for collision avoidance between active satellites and space debris. In this paper, we address not only the design of AO system, but also analyze the images of stellar objects. It is also demonstrated that the AO System is achievable to a near diffraction limited full width at half maximum (FWHM) by analyzing stellar images.

Keywords

Acknowledgement

This work was supported by the Korea Astronomy and Space Science Institute through the project of "Development of 30 km Long-range Free-space Quantum Key Distribution System and Core-technologies for Satellite Quantum Secure Communication" funded by the Ministry of Science and ICT (MSIT) of the Korean government.

References

  1. Kessler DJ, Cour-Palais BG, Collision frequency of artificial satellites: the creation of a debris belt, J. Geophys. Res. 83, 2637-2646 (1978). https://doi.org/10.1029/JA083iA06p02637
  2. Bennett JC, Sang J, Smith CH, Zhang K, Accurate orbit predictions for debris orbit manoeuvre using ground-based lasers, Adv. Space Res. 52, 1876-1887 (2013). https://doi.org/10.1016/j.asr.2013.08.029
  3. Sang J, Bennett JC, Achievable debris orbit prediction accuracy using laser ranging data from a single station, Adv. Space Res. 54, 119-124 (2014). https://doi.org/10.1016/j.asr.2014.03.012
  4. Sang J, Bennett JC, Smith C, Experimental results of debris orbit predictions using sparse tracking data from Mt. Stromlo, Acta Astronaut. 102, 258-268 (2014). https://doi.org/10.1016/j.actaastro.2014.06.012
  5. Bennet F, D'Orgeville C, Price I, Rigaut F, Adaptive optics for satellite imaging and space debris ranging, Proceedings of the Advanced Maui Optical and Space Surveillance Technologies Conference, Hawaii, HI, 15-18 Sep 2015.
  6. Zhang ZP, Yang FM, Zhang HF, Wu ZB, Chen JP, et al., The use of laser ranging to measure space debris, Res. Astron. Astrophys. 12, 212-218 (2012). https://doi.org/10.1088/1674-4527/12/2/009
  7. Kirchner G, Koidl F, Friederich F, Buske I, Volker U, et al., Laser measurements to space debris from Graz SLR station, Adv. Space Res. 51, 21-24 (2013). https://doi.org/10.1016/j.asr.2012.08.009
  8. Sun H, Zhang HF, Zhang ZP, Wu B, Experiment on diffuse reflection laser ranging to space debris and data analysis, Res. Astron. Astrophys. 15, 909-917 (2015). https://doi.org/10.1088/1674-4527/15/6/013
  9. Fruh C, Kelecy TM, Jah MK, Coupled orbit-attitude dynamics of high area-to-mass ratio (HAMR) objects: influence of solar radiation pressure, Earth's shadow and the visibility in light curves, Celest. Mech. Dyn. Astron. 117, 385-404 (2013). https://doi.org/10.1007/s10569-013-9516-5
  10. Mason J, Stupl J, Marshall W, Levit C, Orbital debris-debris collision avoidance, Adv. Space Res. 48, 1643-1655 (2011). https://doi.org/10.1016/j.asr.2011.08.005
  11. Rubenchik AM, Fedoruk MP, Turitsyn SK, The effect of self-focusing on laser space-debris cleaning, Light Sci. Appl. 3, e159 (2014). https://doi.org/10.1038/lsa.2014.40
  12. Bennett JC, Sang J, Smith C, Zhang K, An analysis of very short-arc orbit determination for low-Earth objects using sparse optical and laser tracking data, Adv. Space Res. 55, 617-629 (2015). https://doi.org/10.1016/j.asr.2014.10.020
  13. Bennet F, Price I, Rigaut F, Copeland M, Satellite imaging with adaptive optics on a 1 m telescope, in Advanced Maui Optical and Space Surveillance Technologies Conference, Hawaii, HI, 20-23 Sep 2016.
  14. Copeland M, Bennet F, Zovaro A, Riguat F, Piatrou P, et al., Adaptive optics for satellite and debris imaging in LEO and GEO, in Advanced Maui Optical and Space Surveillance Technologies Conference, Hawaii, HI, 20-23 Sep 2016.
  15. Grosse D, Bennet F, Copeland M, d'Orgeville C, Rigaut F, et al., Adaptive optics for satellite imaging and earth based space debris manoeuvres, in 7th European Conference on Space Debris, Darmstadt, Germany, 18-21 Apr 2017.
  16. Lim HC, Sung KP, Yu SY, Choi M, Park E, et al., Satellite laser ranging system at Geochang station, J. Astron. Space Sci. 35, 253-261 (2018). https://doi.org/10.5140/JASS.2018.35.4.253