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  • Effects of passive de-orbiting through drag and solar sails and electrodynamic tethers on the space debris environment

    Paper number

    IAC-18,A6,2,10,x45019

    Author

    Dr. Camilla Colombo, Italy, Politecnico di Milano

    Coauthor

    Dr. Alessandro Rossi, Italy, IFAC-CNR

    Coauthor

    Mr. Florio Dalla Vedova, Luxembourg, LuxSpace Sarl

    Coauthor

    Prof. Alessandro Francesconi, Italy, University of Padova - DII/CISAS

    Coauthor

    Dr. Claudio Bombardelli, Spain, Technical University of Madrid (UPM)

    Coauthor

    Mr. Mirko Trisolini, United Kingdom, University of Southampton

    Coauthor

    Dr. Juan Luis Gonzalo, Italy, Politecnico di Milano

    Coauthor

    Dr. Pierluigi Di Lizia, Italy, Politecnico di Milano

    Coauthor

    Dr. Cinzia Giacomuzzo, Italy, University of Padova, CISAS – “G. Colombo” Center of Studies and Activities for Space,

    Coauthor

    Mr. Shaker Bayajid Khan, Italy, University of Padova, CISAS – “G. Colombo” Center of Studies and Activities for Space,

    Coauthor

    Dr. Ricardo Garcia-Pelayo, Spain, Technical University of Madrid (UPM)

    Coauthor

    Dr. Vitali Braun, Germany, IMS Space Consultancy

    Coauthor

    Mr. Benjamin Bastida Virgili, Germany, European Space Agency (ESA)

    Coauthor

    Dr. Holger Krag, Germany, European Space Agency (ESA)

    Year

    2018

    Abstract
    Solar and drag sailing and electrodynamic tethers have been proposed as passive end-of-life deorbiting methods, and technological demonstrators are under development. In the drag dominated regime the required area-to-mass-ratio for deorbiting a sail spacecraft is primarily dependant on the semi-major axis, growing exponentially with increasing altitude. In the solar radiation pressure dominated regime, the required area-to-mass ratio strongly depends on both semi-major axis and inclination of the initial orbit. The deorbiting phase, at least in the first phase, is achieved on an elliptical orbit, not a circular orbit like in the case of drag sail with inward deorbiting. Another technology for end-of-life satellite deorbiting is represented by electrodynamic tethers. In general, increasing the cable length as well as its cross section increases the deorbiting force. 
    During deorbiting the satellite passes through the debris environment. The cumulative collision risk can be quantified as a function of the collisional cross-section present in orbit and the time of exposure of this cross-section to the flux of debris present in the environment. The objective of this study, funded by the European Space Agency, is to understand the net effect of using de-orbiting technologies like sails or tethers over the future debris population around the Earth. Indeed, the increased cross sectional area will decrease the deorbiting time, however they will increase the collision risk over the deorbiting phase with respect to a standard satellite. We aim at assessing the collisions risk of deorbiting satellites using these deorbiting techniques, and the consequence of such a collision in terms of global effects onto the whole debris population. To do that fragmentation models have been devised to define when a catastrophic collision will take place and to characterise the following fragments distribution. Long-term simulation of the whole space object population environment are used to evaluate the net effect of using these strategies by means of the definition of an environmental index. Finally, the effort in terms of collision avoidance manoeuvre by conventional spacecraft is assessed and methods for sails and tether to avoid small fragments with low-push manoeuvres or attitude control are investigated.
    Abstract document

    IAC-18,A6,2,10,x45019.brief.pdf

    Manuscript document

    IAC-18,A6,2,10,x45019.pdf (🔒 authorized access only).

    To get the manuscript, please contact IAF Secretariat.