Back to Search
Start Over
Optimal in-orbit repositioning of Sun-pointing Smart Dust.
- Source :
-
Acta Astronautica . Jan2019, Vol. 154, p278-285. 8p. - Publication Year :
- 2019
-
Abstract
- Abstract A Smart Dust is a femto-spacecraft with an external surface coated with electrochromic material, which exploits the solar radiation pressure to produce a propulsive acceleration. As the optical properties of the electrochromic material change upon application of a suitable electric voltage, its propulsive acceleration may be modulated, within some limits, without the use of any propellant. This paper analyzes the optimal trajectories of a Sun-pointing Smart Dust, which provides a propulsive acceleration aligned with the Sun-spacecraft direction. In particular, the paper describes the relative motion of a Smart Dust with respect to a conventional spacecraft (the Mother Ship) that covers a heliocentric circular orbit of given radius. The Smart Dust is required to vary periodically its angular position with respect to the Mother Ship using an optimal (minimum time) strategy. This problem is addressed using an indirect approach and the optimal control law is obtained in a closed-form solution. The results discussed in this paper ensure interesting improvements over existing models from the recent literature, including the possibility of obtaining a generic phasing angle of the Smart Dust and to take into account an optimal number of on-off switchings of the electrochromic control system. Highlights • The paper analyzes the phasing maneuver of a Smart Dust in a circular heliocentric orbit. • The phasing maneuver is studied by evaluating the optimal (minimum) flight time. • The optimization problem is solved using an indirect approach. • The optimal control law is obtained in an analytical form using a lin-earized dynamics. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 00945765
- Volume :
- 154
- Database :
- Academic Search Index
- Journal :
- Acta Astronautica
- Publication Type :
- Academic Journal
- Accession number :
- 133320356
- Full Text :
- https://doi.org/10.1016/j.actaastro.2018.03.036