| Country | Mexico |
| Volcanic Region | Trans-Mexican Volcanic Arc |
| Landform | Volc Type | Composite | Stratovolcano |
| Last Known Eruption | 1270 CE |
| Coordinates | 19.7383°N, 99.7579°W |
| Elevation | 3,911 m (12,831 ft) |
| Volcano Number | 341062 |
 Google Earth Placemark with Features
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 Cite Volcano Profile
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The Global Volcanism Program has no Weekly Volcanic Activity Reports available for Jocotitlán.
The Global Volcanism Program has no Bulletin Reports available for Jocotitlán.
The Global Volcanism Program has no Weekly Reports available for Jocotitlán.
The Global Volcanism Program has no Bulletin Reports available for Jocotitlán.
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There is data available for 2 confirmed eruptive periods.
1270 ± 80 years Confirmed Eruption (Explosive / Effusive)
| Episode 1 | Eruption (Explosive / Effusive) | ||||||||||||||||||||||||
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| 1270 ± 80 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||||||
| Block-and-ash flows and pyroclastic surges from the summit traveled down the W and S flanks around 680 ± 80 years BP (Siebe et al., 1992). | ||||||||||||||||||||||||
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List of 3 Events for Episode 1
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7740 BCE ± 85 years Confirmed Eruption (Explosive / Effusive)
| Episode 1 | Eruption (Explosive / Effusive) | ||||||||||||||||||||||||||||||||||
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| 7740 BCE ± 85 years - Unknown | Evidence from Isotopic: 14C (uncalibrated) | |||||||||||||||||||||||||||||||||
| Carbon from relict tree logs in pyroclastic deposits associated with a debris avalanche on the NE flank is dated at 9,690 ± 85 years BP. The deposit is overlain by pyroclastic surge and airfall pumice deposits (Siebe et al., 1992). | ||||||||||||||||||||||||||||||||||
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List of 5 Events for Episode 1
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The Global Volcanism Program has no synonyms or subfeatures listed for Jocotitlán.
Jocotitlán rises above the Toluca basin and is seen here from the NW. This side of the edifice has a horseshoe-shaped escarpment that formed as a result of gravitational failure of the summit during the early Holocene. The conical hills of Cerro San Miguel (left) and Cerro la Cruz (center) are part of the resulting debris avalanche deposit that covers an 80 km2 area to the NE. 
The tree-covered hills in the foreground of this view of Jocotitlán from the NE are the steep lobate front of a massive debris avalanche deposit produced by partial collapse of the volcano. This catastrophic collapse was radiocarbon dated to about 9,690 years ago. The avalanche traveled a maximum distance of 12 km and covered an area of 80 km2. The 2.8 km3 avalanche deposit is overlain by pyroclastic surge and airfall pumice deposits that were erupted immediately following the collapse.
This conical hill is among many hummocks found at the NE base of Jocotitlán volcano and represents part of the edifice that collapsed in a massive volcanic debris avalanche about 9,700 years ago. The hummocks contain abundant large blocks (1-10 m in diameter) and larger mega-blocks (10-20 m in diameter). The largest are up to 200 m high and occur within 3-5 km of the volcano along with large parallel transverse ridges up to 2.7 km long. The size and height decrease towards the margins of the deposit.
The tree-covered hills in the foreground and center of this view from the summit of Jocotitlán volcano were formed during a massive debris avalanche produced by collapse of the volcano about 9,700 years ago. The debris avalanche deposit includes several conical hummocks (such as those to the lower left) and large transverse ridges up to 2.7 km long. The avalanche traveled a maximum distance of 12 km to the NE and covered an area of 80 km2.There are no samples for Jocotitlán 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. |
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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. |
| EarthScope Consortium SAGE seismic stations/networks | EarthScope Consortium operates the NSF Geodetic Facility for the Advancement of Geoscience (GAGE) and NSF Seismological Facility for the Advancement of Geoscience (SAGE). The linked map shows 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 Jocotitlán. 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. |
| Large Eruptions of Jocotitlán | 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). |
| 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). |
