Space Science Reviews

, Volume 105, Issue 3, pp 535–560

The Genesis Solar-Wind Collector Materials

  • A.J.G. Jurewicz
  • D.S. Burnett
  • R.C. Wiens
  • T.A. Friedmann
  • C.C. Hays
  • R.J. Hohlfelder
  • K. Nishiizumi
  • J.A. Stone
  • D.S. Woolum
  • R. Becker
  • A.L. Butterworth
  • A.J. Campbell
  • M. Ebihara
  • I.A. Franchi
  • V. Heber
  • C.M. Hohenberg
  • M. Humayun
  • K.D. McKeegan
  • K. McNamara
  • A. Meshik
  • R.O. Pepin
  • D. Schlutter
  • R. Wieler
Article

DOI: 10.1023/A:1024469927444

Cite this article as:
Jurewicz, A., Burnett, D., Wiens, R. et al. Space Science Reviews (2003) 105: 535. doi:10.1023/A:1024469927444

Abstract

Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ultra-high purity materials will be exposed to the solar wind and then returned to Earth for laboratory analysis. There is a suite of fifteen types of ultra-pure materials distributed among several locations. Most of the materials are mounted on deployable panels (‘collector arrays’), with some as targets in the focal spot of an electrostatic mirror (the ‘concentrator’). Other materials are strategically placed on the spacecraft as additional targets of opportunity to maximize the area for solar-wind collection.

Most of the collection area consists of hexagonal collectors in the arrays; approximately half are silicon, the rest are for solar-wind components not retained and/or not easily measured in silicon. There are a variety of materials both in collector arrays and elsewhere targeted for the analyses of specific solar-wind components.

Engineering and science factors drove the selection process. Engineering required testing of physical properties such as the ability to withstand shaking on launch and thermal cycling during deployment. Science constraints included bulk purity, surface and interface cleanliness, retentiveness with respect to individual solar-wind components, and availability.

A detailed report of material parameters planned as a resource for choosing materials for study will be published on a Genesis website, and will be updated as additional information is obtained. Some material is already linked to the Genesis plasma data website (genesis.lanl.gov). Genesis should provide a reservoir of materials for allocation to the scientific community throughout the 21st Century.

Copyright information

© Kluwer Academic Publishers 2003

Authors and Affiliations

  • A.J.G. Jurewicz
    • 1
  • D.S. Burnett
    • 2
  • R.C. Wiens
    • 3
  • T.A. Friedmann
    • 4
  • C.C. Hays
    • 1
    • 2
  • R.J. Hohlfelder
    • 4
  • K. Nishiizumi
    • 5
  • J.A. Stone
    • 1
  • D.S. Woolum
    • 6
  • R. Becker
    • 7
  • A.L. Butterworth
    • 8
  • A.J. Campbell
    • 9
  • M. Ebihara
    • 10
  • I.A. Franchi
    • 8
  • V. Heber
    • 11
  • C.M. Hohenberg
    • 12
  • M. Humayun
    • 11
  • K.D. McKeegan
    • 13
  • K. McNamara
    • 14
  • A. Meshik
    • 12
  • R.O. Pepin
    • 7
  • D. Schlutter
    • 7
  • R. Wieler
    • 11
  1. 1.Jet Propulsion Laboratory/California Institute of Technology
  2. 2.California Institute of TechnologyPasadenaUSA
  3. 3.Los Alamos National LaboratoryLos AlamosUSA
  4. 4.Sandia National LabsAlbuquerqueUSA
  5. 5.Space Sciences Lab. U. CalifBerkeleyUSA
  6. 6.Dept. of PhysicsCalif. St. UFullertonUSA
  7. 7.Dept. of Physics, U. MinnesotaMinneapolisUSA
  8. 8.Planetary Science Research Institute, Open UMilton KeynesU.K
  9. 9.Dept. of Geophysical Sciences, U. of ChicagoChicagoUSA
  10. 10.Dept. of ChemistryTokyo Metropolitan UniversityUSA
  11. 11.Institute for Isotope Geology and Mineral ResourcesETH ZürichSwitserland
  12. 12.Dept. Of PhysicsWashington USt. LouisUSA
  13. 13.Dept. of Earth and Space SciencesUCLALos AngelesUSA
  14. 14.NASA Johnson Space CenterHoustonUSA

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