- Info & Contacts
The Global Volcanism Program has no activity reports for Lautaro.
The Global Volcanism Program has no Weekly Reports available for Lautaro.
The Global Volcanism Program has no Bulletin Reports available for Lautaro.
Summary of Holocene eruption dates and Volcanic Explosivity Indices (VEI).
|Start Date||Stop Date||Eruption Certainty||VEI||Evidence||Activity Area or Unit|
|1979 Mar 8 (in or before)||Unknown||Confirmed||2||Historical Observations|
|1978 Jun||Unknown||Confirmed||Historical Observations|
|1961 Oct||Unknown||Confirmed||2||Unknown||Volcano Uncertain: aerial observation; possibly Lautaro|
|1959 Dec 28||1960 Jan 20||Confirmed||2||Historical Observations|
|1945 Jan 15 ± 45 days||Unknown||Confirmed||1||Historical Observations|
|1933 Feb||Unknown||Confirmed||2||Historical Observations|
|1879||Unknown||Confirmed||Unknown||Volcano Uncertain: Between lakes San Martín and Viedma|
|[ 1878 Jan 18 ]||[ Unknown ]||Uncertain||1|
|1876 Oct||Unknown||Confirmed||2||Historical Observations|
The Global Volcanism Program has no synonyms or subfeatures listed for Lautaro.
|The northern side of Lautaro volcano rises above a sea of clouds. A 300-km gap occurs between Cerro Hudson and Lautaro, the northernmost of five volcanoes comprising the australandean volcanic zone of the southernmost Chilean Andes. Glacier-covered, 3607-m-high Lautaro volcano, the highest Chilean volcano below 40 degrees south, has a crater just below its summit on the NW side, and a 1-km-wide crater is located on the NE flank.
Photo by José Naranjo, 2002 (Servico Nacional de Geologica y Mineria).
There are no samples for Lautaro in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.
|Large Eruptions of Lautaro||Information about large Quaternary eruptions (VEI >= 4) is cataloged in the Large Magnitude Explosive Volcanic Eruptions (LaMEVE) database of the Volcano Global Risk Identification and Analysis Project (VOGRIPA).|
|WOVOdat||WOVOdat is a database of volcanic unrest; instrumentally and visually recorded changes in seismicity, ground deformation, gas emission, and other parameters from their normal baselines. It is sponsored by the World Organization of Volcano Observatories (WOVO) and presently hosted at the Earth Observatory of Singapore.|
|EarthChem||EarthChem develops and maintains databases, software, and services that support the preservation, discovery, access and analysis of geochemical data, and facilitate their integration with the broad array of other available earth science parameters. EarthChem is operated by a joint team of disciplinary scientists, data scientists, data managers and information technology developers who are part of the NSF-funded data facility Integrated Earth Data Applications (IEDA). IEDA is a collaborative effort of EarthChem and the Marine Geoscience Data System (MGDS).|
|MODVOLC - HIGP MODIS Thermal Alert System||Using infrared satellite Moderate Resolution Imaging Spectroradiometer (MODIS) data, scientists at the Hawai'i Institute of Geophysics and Planetology, University of Hawai'i, developed an automated system called MODVOLC to map thermal hot-spots in near real time. For each MODIS image, the algorithm automatically scans each 1 km pixel within it to check for high-temperature hot-spots. When one is found the date, time, location, and intensity are recorded. MODIS looks at every square km of the Earth every 48 hours, once during the day and once during the night, and the presence of two MODIS sensors in space allows at least four hot-spot observations every two days. Each day updated global maps are compiled to display the locations of all hot spots detected in the previous 24 hours. There is a drop-down list with volcano names which allow users to 'zoom-in' and examine the distribution of hot-spots at a variety of spatial scales.|
|MIROVA||Middle InfraRed Observation of Volcanic Activity (MIROVA) is a near real time volcanic hot-spot detection system based on the analysis of MODIS (Moderate Resolution Imaging Spectroradiometer) data. In particular, MIROVA uses the Middle InfraRed Radiation (MIR), measured over target volcanoes, in order to detect, locate and measure the heat radiation sourced from volcanic activity.|