Skip to main content

Kone

Caldera · Ethiopia · 1380m

The Kone volcanic complex, also known as Gariboldi, is composed of a series of silicic calderas and young basaltic scoria cones and lava flows. N is towards the lower left in this International Space Station image. The dark-colored basaltic lava flows on the caldera floor were erupted during the first half of the 19th century along a ridge between a smaller caldera to the E and a larger 5-km-wide caldera to the W. The larger young lava flow at the right was erupted from a vent on the SE flank.
The Kone volcanic complex, also known as Gariboldi, is composed of a series of silicic calderas and young basaltic scoria cones and lava flows. N is towards the lower left in this International Space Station image. The dark-colored basaltic lava flows on the caldera floor were erupted during the first half of the 19th century along a ridge between a smaller caldera to the E and a larger 5-km-wide caldera to the W. The larger young lava flow at the right was erupted from a vent on the SE flank. · Photo: NASA International Space Station image ISS001-363-9, 2001 (http://eol.jsc.nasa.gov/). · Wikimedia Commons
Type
Caldera
Country
Ethiopia
Region
Eastern Africa Volcanic Regions / Main Ethiopian Rift Volcanic Province
Elevation
1380m
Coordinates
8.810, 39.695
Last eruption
1820
Tectonic setting
Rift zone / Continental crust (> 25 km)
Landform
Caldera
Major rock type
Rhyolite
Geological summary

The Kone volcanic complex (also known as Gariboldi) is composed of a series of silicic calderas and young basaltic cinder cones and lava flows about 30 km SW of Fentale volcano in the Main Ethiopian Rift. As many as eight silicic calderas are accompanied by ignimbrite outflow sheets. Kone, the youngest caldera, is an elliptical 5 x 7.5 km structure trending E-W and oriented perpendicular to the rift. The rim rises about 100 m above the caldera floor; the eastern rim overlaps with a smaller elliptical caldera. Regional fissures trending roughly N-S cut across the caldera and its flanks. The youngest basalts were erupted during the first half of the 19th century from vents along a hinge line between the smaller eastern caldera (Korke) and the larger western one. A dark lava flow from a cone near the center of the southern caldera (Birenti), extended 12 km SW, where the caldera rim had been eroded, and surrounded older cones.

Eruption history

Summary (VEI over time)
Click a bar to see individual eruptions
1820~1820 · 1 eruptions · max VEI 118201820182118211821

Detailed timeline

  1. 1820 (±10 yrs)VEI 1Observed
    1820 – Ongoing
    East margin of Gariboldi caldera

External links

⚠ For reference only. Not for emergency response.