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Project Icarus: Optimisation of nuclear fusion propulsion for interstellar missions
Authors:KF Long  RK Obousy  A Hein
Institution:1. Department of Chemistry, University of Florida, P. O. Box 117 200, Gainesville, FL 32611, USA;2. Ghent University, Department of Chemistry, Krijgslaan 281-S12, B-9000 Ghent, Belgium;3. Department of Chemistry, University of Bari, Via Orabona 4, 70125 Bari, Italy
Abstract:The Daedalus spacecraft design was a two-stage configuration carrying 50,000 tonnes of DHe3 propellant. Daedalus was powered by electron driven Inertial Confinement Fusion (ICF) to implode the pellets at a frequency of 250 Hz. The mission was to Barnard's star 5.9 light years away in a duration of around 50 years. This paper is related to the successor Project Icarus, a theoretical engineering design study that began on 30 September 2009 and is a joint initiative between the Tau Zero Foundation and The British Interplanetary Society. In the first part of this paper, we explore ‘flyby’ variations on the Daedalus propellant utilisation for two different mission targets: Barnard's star and Epsilon Eridani, 10.7 light years away. With a fixed propellant mass a number of staged configurations (1–4) are derived for an optimal configuration but then moving to an off-optimal configuration due to the requirement for a high final science payload mass. Some comments are then made on the ICF pellet configuration compared to the typical pellets fielded at the National Ignition Facility (NIF) and those proposed for the Vista and Longshot fusion based propulsion designs. This is a working progress report, which aims to study perturbations of the Daedalus baseline design as part of a trade study. This is a submission of the Project Icarus Study Group.
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