Geo debris environment: A model to forecast the next 100 years

Advances in Space Research

Volumn 23, Issue 1, 1999, Pages 191-199

  Yasaka, T ^a   Hanada, T ^a   Hirayama, H ^a  

^a KYUSHU UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001066078     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(99)00004-6     Document Type: Article

References (5)

1. Chobotov, V., The Collision Hazard in Space, J. Astronautical Science, XXX, pp. 191-212 (1982).
2. Crowther, R., Implications of Space Debris for Constellation Survivability and Design, in Proc. First European Conference on Space Debris, ESA SD-01, pp. 565-570 (1993).
3. Klinkrad, H., J. Bendisch, H. Sdunnus, P. Wegener, and R. Westerkamp, An Introduction to the 1997 ESA MASTER Model, in Proc. Second European Conference on Space Debris, ESA SP-393, pp. 217-224 (1997).
4. Yasaka, T., and N. Ishii, Breakup in Geostationary Orbit: A Possible Creation of a Debris Ring, in Space Safety and Rescue 1991, edited by G. Heath, Vol. 82, AAS Science and Technology Series, pp. 203-216 (1993).
5. Yasaka, T., and S. Oda, Breakup, Collision and Population Growth in Geostationary Orbit, in Proc. First European Conference on Space Debris, ESASD-01, pp. 645-649 (1993).