• DocumentCode
    2098673
  • Title

    Colloid thrusters for the new millennium, ST7 DRS mission

  • Author

    Hruby, V. ; Gamero-Castaño, M. ; Spence, D. ; Gasdaska, C. ; Demmons, N. ; McCormick, R. ; Falkos, P. ; Young, J. ; Connolly, W.

  • Author_Institution
    Busek Co. Inc., Natick, MA, USA
  • Volume
    1
  • fYear
    2004
  • fDate
    6-13 March 2004
  • Abstract
    The objective of the NASA JPL Space Technology 7-Disturbance Reduction System (ST7-DRS) mission is to demonstrate: (1) test mass trajectory control that deviates from purely gravitational trajectory by less than 3×10-14m/sec2/Hz0.5 [1+(f/3 mHz)2] over a frequency range from 1 mHz to 30 mHz; and (2) spacecraft position control within 10nm/Hz0.5 over the same frequency range. To achieve these objectives, two technologies must be advanced and tightly integrated. These technologies are the gravitational reference sensors (GRS) being developed by Stanford University and the colloid micro-thruster (CMT) propulsion system in development at Busek Co. Inc. The DRS system will be integrated by JPL and fly on an ESA spacecraft called the LISA pathfinder. This work reports on the progress in the propulsion technology area. The ST7-DRS microthrusters develop thrust by emitting and electrostatically accelerating positively charged nanosized particles, generally referred to as colloids; hence these devices are known as colloid thrusters. Each colloid thruster on the DRS must produce thrust in the 2μN to 20μN range, be smoothly adjustable throughout this range with a maximum thrust increment of less than 0.1 μN and produce thrust noise at a level lower than 0.1 μN/√Hz in the 1 mHz to 30 mHz frequency interval. The DRS uses 8 colloid thrusters arranged in 2 clusters. Each thruster has an independent propellant storage and management subsystems and a power processing unit (PPU). Each cluster has a digital control and interface unit (DCIU) that receives thrust commands from the GRS computer and sends them in analog form to the appropriate thrusters within the cluster. Each cluster also has a field emission cathode based on carbon nanotubes that provides space charge neutralization for the positively charged stream of colloids. The 10:1 dynamic thrust range, the continuous thrust adjustability and noise requirements represent unique challenges that require significant advances in several technology areas, including extremely precise propellant flow control (<0.01μl/min), noise free, high voltage DC/DC converters (<10kV) and stable colloid emission (<0.1μN). We have demonst- rated that we meet the required thrust, thrust noise, and adjustability which we measured using a newly developed torsional thrust stand. We have further demonstrated the necessary functionality of the integrated system at a breadboard level. The performance, the system and the subsystem designs are described.
  • Keywords
    DC-DC power convertors; aerospace propulsion; carbon nanotubes; colloids; electric propulsion; electrostatic accelerators; space research; 1 to 30 mHz; Busek Co. Inc.; CMT propulsion system; Disturbance Reduction System; ESA spacecraft; GRS computer; Jet Propulsion Laboratory; LISA pathfinder; NASA; ST7 DRS mission; Space Technology 7; Stanford University; carbon nanotubes; colloid emission; colloid microthruster; colloid thrusters; digital control; field emission cathode; gravitational reference sensors; gravitational trajectory; high voltage DC/DC converters; interface unit; management subsystems; mass trajectory control; positively charged nanosized particles; power processing unit; propellant flow control; propellant storage; propulsion technology; space charge neutralization; spacecraft position control; thrust noise; Control systems; Frequency; Gas detectors; NASA; Position control; Propulsion; Space technology; Space vehicles; System testing; Weight control;
  • fLanguage
    English
  • Publisher
    ieee
  • Conference_Titel
    Aerospace Conference, 2004. Proceedings. 2004 IEEE
  • ISSN
    1095-323X
  • Print_ISBN
    0-7803-8155-6
  • Type

    conf

  • DOI
    10.1109/AERO.2004.1367606
  • Filename
    1367606