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Dust Measurements During Galileo's Approach to Jupiter and Io Encounter

Grün, E. (author)
Hamilton, D. P. (author)
Riemann, R. (author)
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Dermott, S. (author)
Fechtig, H. (author)
Gustafson, B. A. (author)
Hanner, M. S. (author)
Heck, A. (author)
Horanyi, M. (author)
Kissel, J. (author)
Krüger, H. (author)
Lindblad, Bertil Anders (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science
Linkert, D. (author)
Linkert, G. (author)
Mann, I. (author)
McDonnell, J. A. M. (author)
Morfill, G. E. (author)
Polanskey, C. (author)
Schwehm, G. (author)
Srama, R. (author)
Zook, H. A. (author)
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 (creator_code:org_t)
American Association for the Advancement of Science (AAAS), 1996
1996
English.
In: Science. - : American Association for the Advancement of Science (AAAS). - 1095-9203 .- 0036-8075. ; 274:5286, s. 399-401
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • About a hundred dust impacts per day were detected during the first week in December 1995 by Galileo during its approach to Jupiter. These impacts were caused by submicrometer-sized particles that were just above the detection limit. After the closest approach to Io on 7 December, impacts of these small particles ceased. This effect is expected for dust grains emitted from Io that exit the field of view of the instrument after the flyby. The impact rate of bigger micrometer-sized dust grains continued to increase toward Jupiter. These dust particles are in orbit about Jupiter or are interplanetary grains that are gravitationally concentrated near Jupiter.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

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