Optimization of Solar Sailcraft Trajectory for a Comet Sample Return Mission

Master Thesis (2018)
Author(s)

A. Krishnan (TU Delft - Aerospace Engineering)

Contributor(s)

Ron Noomen – Mentor

EJO Schrama – Graduation committee member

B.T.C. Zandbergen – Graduation committee member

Faculty
Aerospace Engineering
Copyright
© 2018 Ananthakrishnan Krishnan
More Info
expand_more
Publication Year
2018
Language
English
Copyright
© 2018 Ananthakrishnan Krishnan
Graduation Date
17-12-2018
Awarding Institution
Delft University of Technology
Programme
['Aerospace Engineering | Astrodynamics & Space Missions']
Faculty
Aerospace Engineering
Reuse Rights

Other than for strictly personal use, it is not permitted to download, forward or distribute the text or part of it, without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license such as Creative Commons.

Abstract

Comets, the sporadic visitors from the outer edges of the Solar System, are considered to hold the key for understanding the formation of planets and the origin of life on Earth. Having spent the majority of time away from the radiative environment of the inner Solar System, the chemistry of the comets has remained unaltered, making them the pristine samples of the matter from the ancient Solar nebula. A mission to bring cometary particles back to Earth enables the examination of the materials in well equipped laboratories and saves the mass of the instruments to be carried on board. As conventional propulsion methods require a large quantity of propellant for this type of mission, the feasibility of using the novel propulsion technique of solar sailing is explored in this thesis. In order to return the comet samples to Earth within a reasonable time period, the orbit transfer is considered as an optimal control problem with constraints placed on the sailcraft’s position and velocity. The Differential Evolution (DE) algorithm was used to search for time-optimal trajectories that minimize the approach distance and the relative velocity with respect to the comet during sample collection. The optimal trajectory obtained predicts the solar sailcraft to reach the comet, collect the samples and return back to Earth in 6.8 years. The time of arrival at the comet was found to match with the comet's perihelion passage, enabling effective sample collection. The outcome of the trajectory analysis, thus successfully demonstrates the applicability of solar sailing to comet sample return missions in the near future.

Files

MSc_Thesis_Report_FinalReposit... (pdf)
(pdf | 3.46 Mb)
- Embargo expired in 16-06-2019
License info not available