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High-temperature silicate volcanism on Jupiter's moon Io

Science

By:
, , , , , , , , , , , , , ,
DOI: 10.1126/science.281.5373.87

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Abstract

Infrared wavelength observations of Io by the Galileo spacecraft show that at last 12 different vents are erupting lavas that are probably hotter than the highest temperature basaltic eruptions on Earth today. In at least one case, the eruption near Pillan Patea, two independent instruments on Galileo show that the lava temperature must have exceeded 1700 kelvin and may have reached 2000 kelvin. The most likely explanation is that these lavas are ultramafic (magnesium-rich) silicates, and this idea is supported by the tentative identification of magnesium-rich orthopyroxene in lava flows associated with thse high-temperature hot spots.

Additional Publication Details

Publication type:
Article
Publication Subtype:
Journal Article
Title:
High-temperature silicate volcanism on Jupiter's moon Io
Series title:
Science
DOI:
10.1126/science.281.5373.87
Volume
281
Issue:
5373
Year Published:
1998
Language:
English
Larger Work Type:
Article
Larger Work Subtype:
Journal Article
Larger Work Title:
Science
First page:
87
Last page:
90
Number of Pages:
4