๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Violent silicate volcanism on Io in 1996

โœ Scribed by Stansberry, J. A.; Spencer, J. R.; Howell, R. R.; Dumas, C.; Vakil, D.


Book ID
119694627
Publisher
American Geophysical Union
Year
1997
Tongue
English
Weight
435 KB
Volume
24
Category
Article
ISSN
1944-8007

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Io: Evidence for Silicate Volcanism in 1
โœ JOHNSON, T. V.; VEEDER, G. J.; MATSON, D. L.; BROWN, R. H.; NELSON, R. M.; MORRI ๐Ÿ“‚ Article ๐Ÿ“… 1988 ๐Ÿ› American Association for the Advancement of Scienc ๐ŸŒ English โš– 985 KB
Silicate Cooling Model Fits to Galileo N
โœ Ashley Gerard Davies; Rosaly Lopes-Gautier; William D. Smythe; Robert W. Carlson ๐Ÿ“‚ Article ๐Ÿ“… 2000 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 315 KB

The Near Infrared Mapping Spectrometer (NIMS) has obtained spectra of volcanoes on the surface of the jovian satellite Io. Fits to data using a silicate cooling model allow us to constrain lava eruption rates and eruption age. The thermal signatures of the hot spots are indicative of active and cool

High-Resolution Keck Adaptive Optics Ima
โœ F. Marchis; I. de Pater; A.G. Davies; H.G. Roe; T. Fusco; D.Le Mignant; P. Desca ๐Ÿ“‚ Article ๐Ÿ“… 2002 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 367 KB

Io, the innermost Galilean satellite of Jupiter, is a fascinating world. Data taken by Voyager and Galileo instruments have established that it is by far the most volcanic body in the Solar System and suggest that the nature of this volcanism could radically differ from volcanism on Earth. We report

The role of SO2 in volcanism on Io
โœ Smith, B. A.; Shoemaker, E. M.; Kieffer, S. W.; Cook, A. F. ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 699 KB
Chemistry of Sodium, Potassium, and Chlo
โœ Bruce Fegley Jr.; Mikhail Yu. Zolotov ๐Ÿ“‚ Article ๐Ÿ“… 2000 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 274 KB

We used thermochemical equilibrium calculations in the O-S-Na-K-Cl-H system to model the speciation of volcanic gases emitted from high-temperature (1000-2000 K) silicate magmas on Io. The effects of temperature, pressure, and bulk composition of the gases are explored. The bulk compositions are bas