Voyager era stereo images are used to map the geology and topography of Ra Patera (a major active volcanic center and possible site of sulfur eruptions on Io). The summit of Ra Patera reaches only ∼1 km above the surrounding plains. Pre-Voyager-era lava flows occur on slopes of 0.1-0.3°, comparable to the lunar mare. These flows were emplaced at either low viscosities, high eruption rates, or both. A 600-km-long ridged mountain unit (rising to ∼8 km near Carancho Patera) forms a 60 by 90 km wide plateau ∼0.5 km high 50 km east of Ra Patera. The new lava flows observed by Galileo flowed around the southern edge of this plateau.
|Original language||English (US)|
|Number of pages||4|
|Journal||Geophysical Research Letters|
|Publication status||Published - 1997|
ASJC Scopus subject areas
- Earth and Planetary Sciences (miscellaneous)