- Info & Contacts
The Global Volcanism Program has no activity reports for Methana.
The Global Volcanism Program has no Weekly Reports available for Methana.
The Global Volcanism Program has no Bulletin Reports available for Methana.
This compilation of synonyms and subsidiary features may not be comprehensive. Features are organized into four major categories: Cones, Craters, Domes, and Thermal Features. Synonyms of features appear indented below the primary name. In some cases additional feature type, elevation, or location details are provided.
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
|Dome||425 m||37° 36' 54" N||23° 20' 10" E|
|Malja Glat||Dome||675 m|
|Malja Skurti||Dome||590 m|
|Sterna Gambru||Dome||625 m|
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
There is data available for 2 Holocene eruptive periods.
|Start Date||Stop Date||Eruption Certainty||VEI||Evidence||Activity Area or Unit|
|[ 1922 Aug ]||[ Unknown ]||Uncertain|
|0258 BCE ± 18 years||Unknown||Confirmed||3||Historical Observations||Kameno Vouno|
There is no Deformation History data available for Methana.
There is no Emissions History data available for Methana.
|Malja Khoriou lava dome, seen here from the SE, lies on the eastern side of the Methana Peninsula and is one of several basaltic-andesite to rhyodacitic lava domes forming the Methana volcanic complex. The peninsula extends into the Sarronian Gulf on the NE side of the Peloponnesus Peninsula. The youngest dome, Kameno Vouno, on the NW side of Methana Peninsula, was formed in the 3rd century BCE and produced a lava flow that traveled 500 m beyond the coastline.
Photo by Ichio Moriya (Kanazawa University).
The following 23 samples associated with this volcano can be found in the Smithsonian's NMNH Department of Mineral Sciences collections, and may be availble for research (contact the Rock and Ore Collections Manager). Catalog number links will open a window with more information.
|Catalog Number||Sample Description||Lava Source||Collection Date|
|NMNH 111123-855||Hornblende-Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98784||Dacite||KAMENO VOUNO||--|
|NMNH 98788||Dacite||KAMENO VOUNO||--|
|NMNH 98789||Hornblende Andesite||KAMENO VOUNO||--|
|NMNH 98790||Hornblende Andesite||KAMENO VOUNO||--|
|NMNH 98791-1||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98791-2||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98792-1||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98792-2||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98792-3||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98793||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98794||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98795||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98796||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98797||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98798||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98799||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98800||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98801||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98802||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98803||Hypersthene Andesite||KAMENO VOUNO||--|
|NMNH 98805||Dacite||KAMENO VOUNO||--|
|NMNH 98806||Hypersthene Basalt||KAMENO VOUNO||--|
|DECADE Data||The DECADE portal, still in the developmental stage, serves as an example of the proposed interoperability between The Smithsonian Institution's Global Volcanism Program, the MAGA Database, and the EarthChem Geochemical Portal. The Deep Earth Carbon Degassing (DECADE) initiative seeks to use new and established technologies to determine accurate global fluxes of volcanic CO2 to the atmosphere, but installing CO2 monitoring networks on 20 of the world's 150 most actively degassing volcanoes. The group uses related laboratory-based studies (direct gas sampling and analysis, melt inclusions) to provide new data for direct degassing of deep earth carbon to the atmosphere.|
Single Volcano View
Temporal Evolution of Unrest
Side by Side Volcanoes
|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.|
|Large Eruptions of Methana||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).|
|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.|
|MODVOLC Thermal Alerts||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.|
|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).|