New research data collected from submarine volcano
Richard Arculus (2012), David Butterfield (2012), and Keener and Vailea (2012) discussed the Submarine Ring of Fire Expedition 2012 of the Research Vessel R/V Revelle during 14-15 September 2012. They conducted bathymetric profiles and submersible observations of a caldera originally called 'Volcano O' in the Tonga arc (figure 1). During this cruise, the name 'Niua Tahi' was given to this extraordinarily symmetrical, circular caldera, 15 km in diameter at 1.2 to 2 km depth, by a Senior Geological Assistant aboard from the Tonga Ministry of Lands, Environment, Climate Change and Natural Resources. According to Keener and Vailea (2012), "Volcano O, was named 'Niua Tahi' during our expedition by the Ministry, which in Tongan means 'sea', with the small cone within it being named 'Motu Tahi', or 'island in the sea'."
Niua Tahi is a giant, near-circular caldera ~15 km in diameter, with a floor at a depth of about 2 km (Arculus, 2012). A young cone (Motu Tahi) in the SE sector rises 730 m above the floor to a summit at a depth of 1,270 m depth. The volcano is in the rear arc of the Tonga system, located ~40 km W of the chain of subaerial-submarine volcanic edifices that define the volcanic front of the Tonga Arc, and 25 km E of the spreading ridge of the Northeast Lau Spreading Center. The composition of the cone and surrounding floor is predominantly dacite. Towing with sea-floor cameras over the cone and various parts of the caldera resulted in the discovery of at least three sources of hydrothermal particle venting on the cone's summit and adjacent to the inner caldera walls.
During the cruise, the remotely operated vehicle (ROV) Quest 4000 (operated by MARUM, the Center for Marine Environmental Sciences at the University of Breman, Germany) traversed from W to E over the volcano summit and around the margins of the central cone. The cone contained a shallow pit surrounding what appears to be a volcanic vent, probably the site of the most recent volcanism (figures 2a and 2b). The ROV showed that the summit of the cone was mantled with a ubiquitous sulfur-rich layer that coated rugged blocks of pillow lava, lava tubes, and ash-and-blocks deposits.
The ROV images revealed the presence of a NE-trending elongated pit crater at the cone's summit emitting a plume bearing a sulfurous particulate-rich plume. Several previous observations of the water column detected similar plumes. Hot, clear water (~105°C) welled up in numerous places through the loosely agglomerated pyroclastic materials forming both the rim of the crater and flanks of the cone. The attempt to descend the ROV into the pit for a closer look was thwarted by the dense clouds of sulfurous 'smoke.' The most recent volcanic activity was likely dominated by lava and volcaniclastic debris.
References. Arculus, R., 2012 (14 September), Crossing the cone at "Volcano O," Ocean Explorer (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/sept14/sept14.html).
Butterfield, D., 2012 (15 September), Chemistry and ecology at volcano O, Ocean Explorer (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/sept15/sept15.html).
Keener, P., and Vailea, A., 2012 (24 September), In keeping with tradition, Ocean Explorer (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/sept24/sept24.html).
Resing, J., and Embley, B., 2012, Mission summary, NOAA Ocean Explorer web site (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/summary/summary.html).
Information Contacts: Richard Arculus, Research School of Earth Sciences, The Australian National University, Canberra, Australia; Susan Merle, Oregon State University, Eugene, OR, Submarine Ring of Fire 2012 Exploration, NOAA Vents Program; Center for Marine Environmental Sciences (MARUM), University of Bremen, Bremen, Germany (URL: https://www.marum.de/); NOAA Vents Program (URL: https://www.pmel.noaa.gov/eoi/laubasin.html).
The Global Volcanism Program has no Weekly Reports available for Niuatahi.
Reports are organized chronologically and indexed below by Month/Year (Publication Volume:Number), and include a one-line summary. Click on the index link or scroll down to read the reports.
New research data collected from submarine volcano
Richard Arculus (2012), David Butterfield (2012), and Keener and Vailea (2012) discussed the Submarine Ring of Fire Expedition 2012 of the Research Vessel R/V Revelle during 14-15 September 2012. They conducted bathymetric profiles and submersible observations of a caldera originally called 'Volcano O' in the Tonga arc (figure 1). During this cruise, the name 'Niua Tahi' was given to this extraordinarily symmetrical, circular caldera, 15 km in diameter at 1.2 to 2 km depth, by a Senior Geological Assistant aboard from the Tonga Ministry of Lands, Environment, Climate Change and Natural Resources. According to Keener and Vailea (2012), "Volcano O, was named 'Niua Tahi' during our expedition by the Ministry, which in Tongan means 'sea', with the small cone within it being named 'Motu Tahi', or 'island in the sea'."
Niua Tahi is a giant, near-circular caldera ~15 km in diameter, with a floor at a depth of about 2 km (Arculus, 2012). A young cone (Motu Tahi) in the SE sector rises 730 m above the floor to a summit at a depth of 1,270 m depth. The volcano is in the rear arc of the Tonga system, located ~40 km W of the chain of subaerial-submarine volcanic edifices that define the volcanic front of the Tonga Arc, and 25 km E of the spreading ridge of the Northeast Lau Spreading Center. The composition of the cone and surrounding floor is predominantly dacite. Towing with sea-floor cameras over the cone and various parts of the caldera resulted in the discovery of at least three sources of hydrothermal particle venting on the cone's summit and adjacent to the inner caldera walls.
During the cruise, the remotely operated vehicle (ROV) Quest 4000 (operated by MARUM, the Center for Marine Environmental Sciences at the University of Breman, Germany) traversed from W to E over the volcano summit and around the margins of the central cone. The cone contained a shallow pit surrounding what appears to be a volcanic vent, probably the site of the most recent volcanism (figures 2a and 2b). The ROV showed that the summit of the cone was mantled with a ubiquitous sulfur-rich layer that coated rugged blocks of pillow lava, lava tubes, and ash-and-blocks deposits.
The ROV images revealed the presence of a NE-trending elongated pit crater at the cone's summit emitting a plume bearing a sulfurous particulate-rich plume. Several previous observations of the water column detected similar plumes. Hot, clear water (~105°C) welled up in numerous places through the loosely agglomerated pyroclastic materials forming both the rim of the crater and flanks of the cone. The attempt to descend the ROV into the pit for a closer look was thwarted by the dense clouds of sulfurous 'smoke.' The most recent volcanic activity was likely dominated by lava and volcaniclastic debris.
References. Arculus, R., 2012 (14 September), Crossing the cone at "Volcano O," Ocean Explorer (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/sept14/sept14.html).
Butterfield, D., 2012 (15 September), Chemistry and ecology at volcano O, Ocean Explorer (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/sept15/sept15.html).
Keener, P., and Vailea, A., 2012 (24 September), In keeping with tradition, Ocean Explorer (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/sept24/sept24.html).
Resing, J., and Embley, B., 2012, Mission summary, NOAA Ocean Explorer web site (URL: http://oceanexplorer.noaa.gov/explorations/12fire/logs/summary/summary.html).
Information Contacts: Richard Arculus, Research School of Earth Sciences, The Australian National University, Canberra, Australia; Susan Merle, Oregon State University, Eugene, OR, Submarine Ring of Fire 2012 Exploration, NOAA Vents Program; Center for Marine Environmental Sciences (MARUM), University of Bremen, Bremen, Germany (URL: https://www.marum.de/); NOAA Vents Program (URL: https://www.pmel.noaa.gov/eoi/laubasin.html).
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.
Synonyms |
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Volcano O | ||||
Cones |
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Feature Name | Feature Type | Elevation | Latitude | Longitude |
Motutahi | Cone | -1270 m | 15° 22' 44" S | 174° 0' 11" W |
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The Global Volcanism Program is not aware of any Holocene eruptions from Niuatahi. If this volcano has had large eruptions (VEI >= 4) prior to 12,000 years ago, information might be found on the Niuatahi page in the LaMEVE (Large Magnitude Explosive Volcanic Eruptions) database, a part of the Volcano Global Risk Identification and Analysis Project (VOGRIPA).
There is no Deformation History data available for Niuatahi.
There is no Emissions History data available for Niuatahi.
The Global Volcanism Program has no photographs available for Niuatahi.
Maps are not currently available due to technical issues.
There are no samples for Niuatahi in the Smithsonian's NMNH Department of Mineral Sciences Rock and Ore collection.
Copernicus Browser | The Copernicus Browser replaced the Sentinel Hub Playground browser in 2023, to provide access to Earth observation archives from the Copernicus Data Space Ecosystem, the main distribution platform for data from the EU Copernicus missions. |
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. |
WOVOdat
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.
GVMID Data on Volcano Monitoring Infrastructure The Global Volcano Monitoring Infrastructure Database GVMID, is aimed at documenting and improving capabilities of volcano monitoring from the ground and space. GVMID should provide a snapshot and baseline view of the techniques and instrumentation that are in place at various volcanoes, which can be use by volcano observatories as reference to setup new monitoring system or improving networks at a specific volcano. These data will allow identification of what monitoring gaps exist, which can be then targeted by remote sensing infrastructure and future instrument deployments. |
Volcanic Hazard Maps | The IAVCEI Commission on Volcanic Hazards and Risk has a Volcanic Hazard Maps database designed to serve as a resource for hazard mappers (or other interested parties) to explore how common issues in hazard map development have been addressed at different volcanoes, in different countries, for different hazards, and for different intended audiences. In addition to the comprehensive, searchable Volcanic Hazard Maps Database, this website contains information about diversity of volcanic hazard maps, illustrated using examples from the database. This site is for educational purposes related to volcanic hazard maps. Hazard maps found on this website should not be used for emergency purposes. For the most recent, official hazard map for a particular volcano, please seek out the proper institutional authorities on the matter. |
IRIS seismic stations/networks | Incorporated Research Institutions for Seismology (IRIS) Data Services map showing the location of seismic stations from all available networks (permanent or temporary) within a radius of 0.18° (about 20 km at mid-latitudes) from the given location of Niuatahi. Users can customize a variety of filters and options in the left panel. Note that if there are no stations are known the map will default to show the entire world with a "No data matched request" error notice. |
UNAVCO GPS/GNSS stations | Geodetic Data Services map from UNAVCO showing the location of GPS/GNSS stations from all available networks (permanent or temporary) within a radius of 20 km from the given location of Niuatahi. Users can customize the data search based on station or network names, location, and time window. Requires Adobe Flash Player. |
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 Mapping Gas Emissions (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. |
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). |