GEOLOGY AND TOPOGRAPHY OF RA PATERA, IO, IN THE VOYAGER ERA - PRELUDETO ERUPTION

Citation
Pm. Schenk et al., GEOLOGY AND TOPOGRAPHY OF RA PATERA, IO, IN THE VOYAGER ERA - PRELUDETO ERUPTION, Geophysical research letters, 24(20), 1997, pp. 2467-2470
Citations number
25
Categorie Soggetti
Geosciences, Interdisciplinary
ISSN journal
00948276
Volume
24
Issue
20
Year of publication
1997
Pages
2467 - 2470
Database
ISI
SICI code
0094-8276(1997)24:20<2467:GATORP>2.0.ZU;2-5
Abstract
Voyager era stereo images are used to map the geology and topography o f Ra Patera (a major active volcanic center and possible site of sulfu r eruptions on Io). The summit of Ra Patera reaches only similar to 1 km above the surrounding plains. pre-Voyager-era lava flows occur on s lopes of 0.1-0.3 degrees, comparable to the lunar mare. These flows we re emplaced at either low viscosities, high eruption rates, or both. A 600-km-long ridged mountain unit (rising to similar to 8 km near Cara ncho Patera) forms a 60 by 90 km wide plateau similar to 0.5 km high 5 0 km east of Ra Patera. The new lava flows observed by Galileo flowed around the southern edge of this plateau.