Paper
31 August 2005 Electromagnetic formation flight for the Terrestrial Planet Finder
Author Affiliations +
Abstract
Current techniques for actuating spacecraft in formation flying systems such as NASA's Terrestrial Planet Finder (TPF) use propellant-based systems. While maintaining relative orientation, propellant can become a critical consumable which can limit the mission lifetime. Additionally, propellant can cause optimal contamination, plume impingement, thermal emission, and vibration excitation. A novel technique called Electromagnetic Formation Flight (EMFF) can be used to eliminate propellant-based systems to control the relative degrees of freedom for TPF. The EMFF system consists of electromagnets in concert with reaction wheels and is used to replace the consumables. Solar energy, a renewable resource provides power for EMFF. This paper investigates the design for TPF using EMFF. The results show that EMFF is a viable option for TPF and compares favorably in terms of mass to propellant-based systems.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniel W. Kwon and David W. Miller "Electromagnetic formation flight for the Terrestrial Planet Finder", Proc. SPIE 5905, Techniques and Instrumentation for Detection of Exoplanets II, 590515 (31 August 2005); https://doi.org/10.1117/12.614556
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Cited by 1 scholarly publication.
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KEYWORDS
Space operations

Systems modeling

Electromagnetism

Magnetism

Planets

Control systems

Performance modeling

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