Published February 3, 1995 | Version public
Journal Article

Metal Ions in the Atmosphere of Neptune

  • 1. ROR icon California Institute of Technology

Abstract

Microwave propagation experiments performed with Voyager 2 at Neptune revealed sharp layers of electrons in Neptune's lower ionosphere with densities of approximately 10(4) per cubic centimeter. These layers are reminiscent of the sporadic-E layers in the Earth's ionosphere, and when taken together with data from the other giant planets, these data confirm the importance of the magnetic field in layer formation. A photochemical model that incorporates species produced by meteoroid ablation predicts that singly ionized magnesium is the most likely metal to be found in the layers, although laboratory data on the kinetics of metallic atoms and ions in a reducing environment are lacking. The metal chemistry discussed here is directly relevant to the abundant metals observed at the impact site of the G fragment of comet Shoemaker Levy 9 on Jupiter.

Additional Information

© 1995 American Association for the Advancement of Science. Received 29 July 1994; accepted 1 November 1994. Discussions with G. Lindal, E. R. Kursinski, J. Connerney, Y. Yung, W. Goddard, T. Rebold, and S. Asmar are gratefully acknowledged. G. Lindal provided the electron number density profile. This work was supported by NASA grants NAGW-2362 and NAGW-1509. Contribution 5418 from the Division of Geological and Planetary Sciences, California Institute of Technology.

Additional details

Identifiers

Eprint ID
52533
Resolver ID
CaltechAUTHORS:20141210-091532590

Related works

Funding

NASA
NAGW-2362
NASA
NAGW-1509

Dates

Created
2014-12-10
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Updated
2021-11-10
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Caltech Custom Metadata

Other Numbering System Name
Caltech Division of Geological and Planetary Sciences
Other Numbering System Identifier
5418