Voyager 1 photopolarimeter experiment and the phase curve and surface microstructure of Ganymede

Voyager 1 photopolarimeter experiment and the phase curve and surface microstructure of Ganymede

Optical wavelength photometry used to determine the surface microstructure of Ganymede, shows that its surface is more porous than Callisto.

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Veröffentlicht in:Nature (London) 1979-08, Vol.280 (5725), p.804-806
Hauptverfasser: Pang, Kevin, Hord, Charles W., West, Robert A., Simmons, Karen E., Coffeen, David L., Bergstralh, Jay T., Lane, Arthur L.
Format: Artikel
Sprache:eng
Schlagworte:
Humanities and Social Sciences
multidisciplinary
news-and-views
Science
Science (multidisciplinary)
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Zusammenfassung:Optical wavelength photometry used to determine the surface microstructure of Ganymede, shows that its surface is more porous than Callisto.
ISSN:0028-0836
1476-4687
DOI:10.1038/280804a0