Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-26T18:42:12.742Z Has data issue: false hasContentIssue false
  • English
  • Français

Study of Cosmic Dust Particles on Board LDEF and MIR Space Station

Published online by Cambridge University Press:  12 April 2016

J.C. Mandeville
J.C. Mandeville*
Affiliation:
ONERAICERT Space Technology Department P.O. Box 402531055 Toulouse Cedex, France

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.

Interplanetary and near-earth space contains solid objects whose size distribution continuously covers the interval from submicron sized particles to km sized asteroids or comets. Two French experiments partly devoted to the detection of cosmic dust have been flown recently in space. One on the NASA Long Duration Exposure Facility (LDEF), and one on the Soviet MIR Space Station. A variety of sensors and collecting devices will make possible the study of cosmic particles after recovery of exposed material. Flux mass distribution is expected to be derived from craters counts, with a good accuracy. Remnants of particles, suitable for chemical identification are expected to be found within stacked foil detectors. Discrimination between extraterrestrial particles and man-made orbital debris will be possible.

Type
Interplanetary Dust: Space and Earth Environment Studies
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 11 - 14
Copyright
Copyright © Kluwer 1991

References

References.

Alexander, W.M. et al. (1963) ‘Review of direct measurements of interplanetary dust from satellites and probes’, in Priester, W. (ed.), Proc. Third Intern. Space Sci.Symp., J.Wiley Publishers, p.891. Cour-Palais, B.G. (1969) ‘Meteoroid environment model’, NASA SP 8013.Google Scholar
Kessler, D.J., Reynolds, R.C. and Anz-Meador, P.D. (1989) ‘Orbital debris environment’, NASA TM 100471Google Scholar
Leinert, Ch. and Grün, E. (1990) ‘Interplanetary Dust’, in Physics and Chemistry in Space, Springer Publishers, (in press).Google Scholar
Mandeville, J-C. and McDonnell, J.A.M. (1980) ‘Micrometeoroid multiple foil penetration and particle recovery experiments on LDEF, in IAU Symposium 90 Proceedings, D. Reidel Publishers, Dordrecht.Google Scholar
Mandeville, J-C. (1984) ‘A0138-1 and A0138-2 Experiments’, in Clark, L.G. et al. (eds.), LDEF Mission 1 Experiments, NASA SP-473.Google Scholar
Mandeville, J-C. (1990) ‘Aragatz Mission Dust Collection Experiment’, Adv.Space Res. 10, pp.397–401.CrossRefGoogle Scholar
McDonnell, J.A.M. et.al. (1991) ‘Paniculate detection in the near earth space environment aboard the long duration exposure facility LDEF: Cosmic or Terrestrial’, Proc. IAU Coll. on ‘Origin and Evolution of Interplanetary Dust’, Kyoto, Japan.Google Scholar
See, T., et al. (1990). ‘Meteoroid and debris impact features documented on the Long Duration Exposure Facility’, M-D SIG, Prelim.Report.,NASA.Google Scholar
Singer, S.F. et al. (1990) ‘First spatio-temporal results from the LDEF Interplanetary dust experiment (IDE)’, Preprint XXVIII COSPAR 1990.Google Scholar
Singer, S.F. and Stanley, J.E. (1980) ‘Submicron particles in meteor streams’, in IAU Symposium 90 proceedings, D.Reidel Publishers, Dordrecht.Google Scholar
Warren, J.L. et al. (1989) ‘The detection and observation of meteoroid and space debris impact features on the Solar-Max satellite’, in Proceedings XIXth Lun.Plan.Sci.Conf., pp. 641–657.Google Scholar