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Cometary and Interstellar Dust Analyzer for comet Wild 2
Author(s) -
Kissel J.,
Glasmachers A.,
Grün E.,
Henkel H.,
Höfner H.,
Haerendel G.,
von Hoerner H.,
Hornung K.,
Jessberger E. K.,
Krueger F. R.,
Möhlmann D.,
Greenberg J. M.,
Langevin Y.,
Silén J.,
Brownlee D.,
Clark B. C.,
Hanner M. S.,
Hoerz F.,
Sandford S.,
Sekanina Z.,
Tsou P.,
Utterback N. G.,
Zolensky M. E.,
Heiss C.
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 - 10.1029/2003je002091
Subject(s) - comet , physics , comet dust , comet nucleus , astrobiology , comet tail , spacecraft , mass spectrometry , coma (optics) , interstellar comet , cosmic dust , astronomy , astrophysics , interplanetary dust cloud , plasma , solar system , solar wind , nuclear physics , quantum mechanics
The Cometary and Interstellar Dust Analyzer (CIDA) instrument analyzes the composition of individual grains in the cometary coma. As each particle impacts a silver plate, the high‐impact energy due to the relative velocity of the spacecraft as it flies through the coma causes the elements and molecular compounds in the particle to become ionized. Using a fast time‐of‐flight mass spectrometer, a complete set of ions are detected for each impact, from a mass range of 1 (atomic hydrogen) up to a few thousand atomic mass units, encompassing all elements in the periodic table and many molecules, such as organic compounds. This experimental technique has already been applied with excellent success at Halley's comet, and the CIDA derivative instrument is flying on the Stardust mission, which will encounter comet Wild 2 in January of 2004. The data returned will give clues to the elemental and chemical composition of the dust component of this comet.

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