Hypervelocity microparticle impact studies using a novel cosmic dust mass spectrometer
Author(s) -
Austin Daniel E.,
Grimm Ronald L.,
Manning Heidi L. K.,
Bailey Carl L.,
Farnsworth James E.,
Ahrens Thomas J.,
Beauchamp J. L.
Publication year - 2003
Publication title -
journal of geophysical research: planets
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2002je001947
Subject(s) - hypervelocity , mass spectrometry , projectile , cosmic ray , physics , spectrometer , faraday cup , ion , ionization , van de graaff generator , electron ionization , materials science , nuclear physics , ion beam , optics , beam (structure) , astronomy , quantum mechanics
Micron‐sized iron and copper particles accelerated to 2–20 km/s in a 2 MV van de Graaff electrostatic accelerator were used to test the performance of our recently developed cosmic dust mass spectrometer. This compact in situ dust analyzer, known as the Dustbuster, is designed to determine the elemental composition of cosmic dust particles through impact ionization and subsequent time‐of‐flight mass spectrometry. Results from 750 laboratory impacts show high mass resolution, typically 150–350 ( m /Δ m ) for projectile components and 300–600 for the target material (tantalum). Peaks corresponding to H, C, O, Na, and K ions are also observed, consistent with previous microparticle impact experiments. Field‐induced emission of electrons immediately before impact is a possible cause of ion formation from species with high ionization potentials. The high mass resolution, large sensitive target area, and small size make the Dustbuster an ideal instrument for inclusion on a spacecraft payload.
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom