Author
Listed:
- G. Gloeckler
(University of Maryland
Oceanic and Space Sciences, University of Michigan)
- J. Geiss
(International Space Science Institute)
- N. A. Schwadron
(Oceanic and Space Sciences, University of Michigan)
- L. A. Fisk
(Oceanic and Space Sciences, University of Michigan)
- T. H. Zurbuchen
(Oceanic and Space Sciences, University of Michigan)
- F. M. Ipavich
(University of Maryland)
- R. von Steiger
(International Space Science Institute)
- H. Balsiger
(Physikalisches Institut, University of Bern)
- B. Wilken
(Max-Planck Institut für Aeronomie)
Abstract
Remote sensing observations1,2,3,4,5 and the direct sampling of material6,7,8 from a few comets have established the characteristic composition of cometary gas. This gas is ionized by solar ultraviolet radiation and the solar wind to form ‘pick-up’ ions9,10,11, ions in a low ionization state that retain the same compositional signatures as the original gas. The pick-up ions are carried outward by the solar wind, and they could in principle be detected far from the coma. (Sampling of pick-up ions has also been used to study interplanetary dust12,13, Venus’ tail14 and the interstellar medium15,16.) Here we report the serendipitous detection of cometary pick-up ions, most probably associated with the tail of comet Hyakutake, at a distance of 3.4 au from the nucleus. Previous observations have provided a wealth of physical and chemical information about a small sample of comets6,7,8,9, but this detection suggests that remote sampling of comet compositions, and the discovery of otherwise invisible comets, may be possible.
Suggested Citation
G. Gloeckler & J. Geiss & N. A. Schwadron & L. A. Fisk & T. H. Zurbuchen & F. M. Ipavich & R. von Steiger & H. Balsiger & B. Wilken, 2000.
"Interception of comet Hyakutake's ion tail at a distance of 500 million kilometres,"
Nature, Nature, vol. 404(6778), pages 576-578, April.
Handle:
RePEc:nat:nature:v:404:y:2000:i:6778:d:10.1038_35007015
DOI: 10.1038/35007015
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