Orbit Design for a Phobos-Deimos Cycler Mission

Author(s)
Sabitbek, Bolys
Editor(s)
Associated Organization(s)
Organizational Unit
Daniel Guggenheim School of Aerospace Engineering
The Daniel Guggenheim School of Aeronautics was established in 1931, with a name change in 1962 to the School of Aerospace Engineering
Supplementary to:
Abstract
Little is know about the Martian moons Phobos and Deimos, even though they have the potential to provide insight into the evolution of the Martian system, and could potentially serve as a staging site for a future Mars manned mission. While attempts to visit Phobos with dedicated missions have been attempted, to date none have been successful, and no dedicated mission to Deimos has been flown. As such, much of what is known about the structure and composition of either moon comes from a small collection of images. This study explores a class of stable cycler orbits that could visit both moons on a regular cadence, and can be tuned to fly-by one moon more frequently, or to vary the ground track coverage to obtain improved surface coverage. While the orbits described can be reached by a dedicated spacecraft with sufficient delta-V for a Mars insertion, the moti vation here is that the spacecraft is already in an initial insertion orbit, such as a small-satellite rideshare on an existing Mars mission. Under this assumption, the results presented illustrate that the exploration of both Phobos and Deimos can be achieved with a spacecraft with capabilities of modern nanosatellites (cubesats).
Sponsor
Date
2016-04-16
Extent
Resource Type
Text
Resource Subtype
Masters Project
Rights Statement
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