Abstract
The space debris detectin will become greater and greater in the near future with the space debris enhancing. We introduce a theoretical approach of this problem assuming the using of a new generation large coronograph. We get some interesting — and alarming — results about the great probability to be able to observe space debris with this new ground-based large coronograph.
Similar content being viewed by others
References
Allen, C. W.: 1973,Astrophysical Quantities, 3rd ed., Athlone Press, London.
Kessler, D. J.: 1985, ‘Explorer 46 Meteoroid Bumper Experiment: Earth Orbital ‘Debris Interpreation”, inProperties and Interactions of Interplanetary Dust, Astrophysics and Space Sciences Library, Vol. 119, p. 97 (IAU Colloq. 85).
Kneizys, F. X., Shettle, E. P., Gallery, W. O., Chetwynd, J. H., Jr., Abreu, L. W., Selby, J. E. A., Clough, S. A., and Fenn, R. W.: 1983,Atmospheric Transmittance/Radiance Computer Code LOWTRAN 6, Optical Physics Division, Project 7670, Air Force Geophysics Laboratory, Hanscom Field, Mass. 01731, AFSC, USAF.
Koutchmy, S.: 1987,L'Astronomie 101, 426.
Nitschelm, C.: 1987,Etude des caractéristiques de la transparence atmosphérique et de la luminance du ciel dans le domaine ultraviolet, IAP report for the Thomson-CSF Co., IAP, Paris, France, pp. 181.
Smartt, R. N.: 1987,A Large Coronograph for High Resolution Studies, oral communication, 9th Sacramento Peak Workshop on Coronal Structure, 17–21 August.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Koutchmy, S., Nitschelm, C. Optical detection of space debris using a large achromatic coronograph. Astrophys Space Sci 143, 45–49 (1988). https://doi.org/10.1007/BF00636753
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00636753