A new eruptive phase started at Ubinas volcano, Peru on June 24, 2019, following a seismic swarm detected since June 21. This is the first activity at the volcano since March 2017.
Ash emissions mixed with gases and water vapor began at 12:18 UTC (07:18 LT), rising several hundred meters above the crater.
Un nuevo proceso eruptivo del #Ubinas comenzó hoy después de las 07:00 horas, de acuerdo a los registros sísmicos. A través de las cámaras de vigilancia volcánica, se aprecia emisiones continuas de cenizas hasta 1000 m. de altura sobre el cráter. pic.twitter.com/hRoxNIcgru— Gianfranco Argandoña (@Gianfranco_AC) June 24, 2019
As a result of this activity, the volcanic alert level has been raised from Green to Yellow.
Ash emissions rising above Ubinas volcano on June 24, 2019. Credit: NASA Terra/MODIS
A damaging lahar was produced by heavy rain falling over Ubinas volcano on February 6, 2019. This was the third lahar event at the volcano in 2019 and the largest since 2014, Ingemmet volcanologist Domingo Ramos said, adding that the event lasted for more than 1 hour.
While there were no casualties reported, the material damage was substantial, he said.
The lahar damaged agricultural fields and blocked one of the local roads, isolating many villages. In addition, power poles were destroyed, cutting off power to 80% of the villages in the Ubinas Valley.
Images courtesy Ingemmet
A small, 1.4-km-wide (0.8 miles) 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 (31 miles) behind the main volcanic front of Perú.
The growth and destruction of Ubinas I was followed by the 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 (492 feet) summit caldera contains an ash cone with a 500-m-wide (1 640 feet) funnel-shaped vent that is 200 m (656 feet) deep.
Debris-avalanche deposits from the collapse of the SE flank about 3 700 years ago extend 10 km (6.2 miles) from the volcano. Widespread plinian pumice-fall deposits include one of Holocene age about 1 000 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. (GVP)
Featured image credit: NASA Terra/MODIS
Register/become a supporter
Your support is crucial for our survival. It makes this project fully self-sustainable and keeps us independent and focused on the content we love to create and share.
You'll receive your ad-free account for 20x faster browsing experience, clean interface without any distractions, ability to post comments without prior editorial check, all our desktop and mobile applications (current and upcoming) ad-free and with the full set of features available, a direct line of communication and much more. See all options.