Abstract The Infrared Astronomical Satellite (IRAS) was launched in 1983 for the purpose of surveying the sky in a broad area of the infrared portion of the spectrum. While the primary objects of interest of IRAS were stars and nebulae, other types of space-related objects could also be observed. These include comets, asteroids, and Earth orbiting objects. Theoretical analysis indicates that IRAS could observe objects with a diameter of 1-mm at a range of 100-km and objects with a diameter of 1-cm at a range of 1000-km, while current ground-based observations of particles in low Earth orbit are limited to objects larger than 1-cm. Thus, these data offer a unique opportunity to ascertain the number density of particles below the present observable limit. At NASA/JSC a preliminary analysis of an IRAS data set has been performed to detect and describe this population, and the results of this study are presented.


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    Titel :

    Analysis of IRAS data for orbital debris


    Beteiligte:
    Anz-Meador, P.D. (Autor:in) / Oró, D.M. (Autor:in) / Kessler, D.J. (Autor:in) / Pitts, D.E. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    1987-01-01


    Format / Umfang :

    6 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    Analysis of IRAS data for orbital debris

    Anz-Meador, P. D. / Oro, D. M. / Kessler, D. J. et al. | NTRS | 1986


    Centimetre-sized orbital debris observed with IRAS

    Van Hees, R. M. / De Jonge, A. R. W. / Wesselius, P. R. et al. | British Library Conference Proceedings | 1993


    Space debris observed by IRAS

    Wesselius, P.R. / van Hees, R. / de Jonge, A.R.W. et al. | Elsevier | 1993


    Detecting space debris above 900 km using IRAS

    DE JONGE, A. / WESSELIUS, P. | AIAA | 1990


    Orbital Debris

    Online Contents | 1993