- Info & Contacts
The Global Volcanism Program has no activity reports for Ubehebe Craters.
The Global Volcanism Program has no Weekly Reports available for Ubehebe Craters.
The Global Volcanism Program has no Bulletin Reports available for Ubehebe Craters.
Summary of Holocene eruption dates and Volcanic Explosivity Indices (VEI).
|Start Date||Stop Date||Eruption Certainty||VEI||Evidence||Activity Area or Unit|
|4050 BCE (?)||Unknown||Confirmed||Anthropology|
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|
|Ubehebe craters are an isolated group of maar volcanoes erupted through nonvolcanic sediments of Death Valley National Park. The craters were formed by hydrovolcanic explosions along a fault. The contact between pre-eruption yellowish- and orange-colored sedimentary rocks and overlying black ash deposits from an early stage scoria cone can be seen at the upper part of the western wall of 800-m wide, 235-m deep Ubehebe crater, the youngest and largest crater.
Photo by Lee Siebert, 1974 (Smithsonian Institution).
|Bedded pyroclastic-surge deposits from the eruptions forming Ubehebe craters can be seen in this gully south of Little Ubehebe crater. The eruption formed two clusters of explosion craters and tuff rings along a N-S line.
Photo by Lee Siebert (Smithsonian Institution).
|Erosional gullies furrow the surface of pyroclastic-surge deposits from the eruptions forming Ubehebe craters in Death Valley, California. The craters were erupted along a fault that forms the western boundary of the Tin Mountain range in the left background.
Photo by Lee Siebert (Smithsonian Institution).
|Darker-colored layers of basaltic ash drape the northern rim of Ubehebe Crater in the northern part of Death Valley National Park and spill down the crater walls. The 235-m-deep Ubehebe Crater is the largest of a series of more than a dozen overlapping maars formed by explosive eruptions through fanglomerate deposits, which form the light-colored areas below the ash layers. The Amargosa Range rises on the horizon across Death Valley to the east.
Photo by Paul Kimberly, 1997 (Smithsonian Institution).
A listing of samples from the Smithsonian collections will be available soon.
|Large Eruptions of Ubehebe Craters||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.|