- Info & Contacts
The Global Volcanism Program has no activity reports for Aragats.
The Global Volcanism Program has no Weekly Reports available for Aragats.
The Global Volcanism Program has no Bulletin Reports available for Aragats.
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.
|Aragay | Alagey | Aragatz|
|Feature Name||Feature Type||Elevation||Latitude||Longitude|
The Global Volcanism Program is not aware of any Holocene eruptions from Aragats. If this volcano has had large eruptions (VEI >= 4) prior to 10,000 years ago, information might be found on the Aragats page in the LaMEVE (Large Magnitude Explosive Volcanic Eruptions) database, a part of the Volcano Global Risk Identification and Analysis Project (VOGRIPA).
Information about Deformation periods will be available soon.
There is no Emissions History data is available for Aragats.
|The twin northern summits of Aragats volcano in NW Armenia are seen from a ridge to the south. Extensive hydrothermal alteration has modified rocks in the summit region of this large andesitic-to-dacitic stratovolcano. The 4095-m-high main edifice of Aragats is dissected by glaciers and is of Pliocene to late-Pleistocene age. Satellitic cones and fissures have produced lava flows of late-Pleistocene to possible Holocene age.
Photo by Alexander Margarian.
The following 34 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 117574-10||Andesitic Basalt||Karmratar||--|
|NMNH 117574-109||Basaltic Andesite||Astarak Flow||--|
|NMNH 117574-111||Basaltic Andesite||--||--|
|NMNH 117574-113||Andesitic Dacite||--||--|
|NMNH 117574-119||Pumice||Pokr Arteni||--|
|NMNH 117574-120||Obsidian||Pokr Arteni||--|
|NMNH 117574-121||Rhyolite||Pokr Arteni||--|
|NMNH 117574-129||Basaltic Andesite||--||--|
|NMNH 117574-130||Basaltic Andesite||--||--|
|NMNH 117574-131||Basaltic Andesite||--||--|
|NMNH 117574-132||Perlite||Pokr Arteni||--|
|NMNH 117574-14||Andesite||Menak Blur||--|
|NMNH 117574-15||Andesitic Basalt||Menak Blur||--|
|NMNH 117574-21||Andesitic Basalt||Karmratar||--|
|NMNH 117574-23||Andesitic Basalt||Karmratar||--|
|NMNH 117574-5||Basalt||Araks Cone||--|
|NMNH 117574-7||Andesitic Basalt||Shamiram||--|
|NMNH 117574-8||Andesitic Basalt||Karmratar||--|
|NMNH 117574-9||Andesitic Basalt||Blrashark||--|
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 Aragats||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).|