Logo link to homepage

Report on Ubinas (Peru) — 13 January-19 January 2016

Smithsonian / US Geological Survey Weekly Volcanic Activity Report, 13 January-19 January 2016
Managing Editor: Sally Kuhn Sennert

Please cite this report as:

Global Volcanism Program, 2016. Report on Ubinas (Peru). In: Sennert, S K (ed.), Weekly Volcanic Activity Report, 13 January-19 January 2016. Smithsonian Institution and US Geological Survey.

Volcano Profile |  Weekly Report (13 January-19 January 2016)


Ubinas

Peru

16.355°S, 70.903°W; summit elev. 5672 m

All times are local (unless otherwise noted)


Instituto Geofísico del Perú (IGP) Observatorio Volcanológico del Sur (OVS) reported that during 12-18 January the seismic network at Ubinas recorded an increase in the number and magnitude of long-period earthquakes and a decrease in volcano-tectonic events. Thermal anomalies were detected on 13 and 15 January. At 0640 on 15 January a plume rose 500 m above the crater's base. At 1253 an explosion generated an ash plume that rose 3 km above the crater's base and drifted S and SW. The report noted that this was the first explosive event since 5 November 2015.

Geologic Background. A small, 1.4-km-wide caldera cuts the top of Ubinas, Peru's most active volcano, giving it a truncated appearance. It is the northernmost of three young volcanoes located along a regional structural lineament about 50 km behind the main volcanic front of Perú. The growth and destruction of Ubinas I was followed by construction of Ubinas II beginning in the mid-Pleistocene. The upper slopes of the andesitic-to-rhyolitic Ubinas II stratovolcano are composed primarily of andesitic and trachyandesitic lava flows and steepen to nearly 45 degrees. The steep-walled, 150-m-deep summit caldera contains an ash cone with a 500-m-wide funnel-shaped vent that is 200 m deep. Debris-avalanche deposits from the collapse of the SE flank about 3700 years ago extend 10 km from the volcano. Widespread plinian pumice-fall deposits include one of Holocene age about 1000 years ago. Holocene lava flows are visible on the flanks, but historical activity, documented since the 16th century, has consisted of intermittent minor-to-moderate explosive eruptions.

Source: Instituto Geofísico del Perú (IGP)