Diamond Craters

Photo of this volcano
Google Earth icon
  Google Earth Placemark
  • Country
  • Volcanic Region
  • Primary Volcano Type
  • Last Known Eruption
  • 43.1°N
  • 118.75°W

  • 1435 m
    4707 ft

  • 322170
  • Latitude
  • Longitude

  • Summit
    Elevation

  • Volcano
    Number

The Global Volcanism Program has no activity reports for Diamond Craters.

The Global Volcanism Program has no Weekly Reports available for Diamond Craters.

The Global Volcanism Program has no Bulletin Reports available for Diamond Craters.

Basic Data

Volcano Number

Last Known Eruption

Elevation

Latitude
Longitude
322170

5610 BCE

1435 m / 4707 ft

43.1°N
118.75°W

Volcano Types

Volcanic field

Rock Types

Major
Basalt / Picro-Basalt

Tectonic Setting

Rift zone
Continental crust (> 25 km)

Population

Within 5 km
Within 10 km
Within 30 km
Within 100 km
66
66
136
6,969

Geological Summary

Diamond Craters volcanic field consists of a 60 sq km area of basaltic lava flows and numerous cinder cones and maars located between the SE Oregon town of Burns and Steens Mountain. A basaltic pahoehoe lava field is overlain by deposits from phreatomagmatic and strombolian eruptions that formed a late-stage central vent complex of about 20 craters and cones that densely fill a 1.1 x 1.6 km box-shaped caldera. The age of Diamond Craters is constrained to within 7320-7790 calibrated years Before Present by radiocarbon-dated floodplain deposits below the lava flows and paloemagnetic evidence (Sherrod et al., 2012). Structural doming at Diamond Craters has created a series of six overlapping topographic highs. The highest of these is known as Graben Dome; its 1435-m-high summit is cut by a NW-SE-trending graben 0.4 x 2.1 km long and 30 m deep. Lava flows on the eastern side of the volcanic field and scattered cinder cones and maars formed during the last stage of activity.

References

The following references have all been used during the compilation of data for this volcano, it is not a comprehensive bibliography.

Benedict E, 2000. Diamond Craters, Oregon's geologic gem. U S Bur Land Management brochure BLM/OR/WA/GI-00/027-1122.32.

Chitwood L A, 1994. Inflated basaltic lava--examples of processes and landforms from central and southeast Oregon. Oregon Geol, 56: 11-21.

Friedman I, Peterson N, 1971. Obsidian hydration dating applied to dating of basaltic volcanic activity. Science, 172: 1028.

Green J, Short N M, 1971. Volcanic Landforms and Surface Features: a Photographic Atlas and Glossary. New York: Springer-Verlag, 519 p.

Russell J K, Nicholls J, 1987. Early crystallization history of alkali olivine basalts, Diamond Craters, Oregon. Geochim Cosmochim Acta, 51: 143-154.

Sarna-Wojcicki A M, Champion D E, Davis J O, 1983. Holocene volcanism in the conterminous United States and the role of silicic volcanic ash layers in correlation of latest Pleistocene and Holocene deposits. In: Wright H E (ed) {Late-Quaternary Environments of the United States}, Minneapolis: Univ Minnesota Press, 2: 52-77.

Sherrod D R, Champion D E, McGeehin J P, 2012. Age and duration of volcanic activity at Diamond Craters, southeastern Oregon. J Volc Geotherm Res, 247-248: 108-114.

Smith R L, Shaw H R, 1975. Igneous-related geothermal systems. U S Geol Surv Circ, 726: 58-83.

Smith R L, Shaw H R, Luedke R G, Russell S L, 1978. Comprehensive tables giving physical data and thermal energy estimates for young igneous systems of the United States. U S Geol Surv Open-File Rpt, 78-925: 1-25.

Smith W D, 1927. Contribution to the geology of southeastern Oregon (Steens and Pueblo Mountains). J Geol, 35: 421-440.

Wood C A, Kienle J (eds), 1990. Volcanoes of North America. Cambridge, England: Cambridge Univ Press, 354 p.

Eruptive History


Summary of Holocene eruption dates and Volcanic Explosivity Indices (VEI).


Start Date Stop Date Eruption Certainty VEI Evidence Activity Area or Unit
5610 BCE ± 470 years Unknown Confirmed 4 Radiocarbon (corrected)

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.


Cones

Feature Name Feature Type Elevation Latitude Longitude
Big Bomb Crater Pyroclastic cone 1308 m
Lava Pit Crater Shield volcano 1305 m
Red Bomb Crater Pyroclastic cone 1323 m

Craters

Feature Name Feature Type Elevation Latitude Longitude
Central Crater Complex Caldera 1378 m
Diamond Pond (Malheur Maar) Maar 1286 m
Dry Maar Maar 1268 m
East Twin Crater Maar 1326 m
Keyhole Explosion Crater Crater
Malheur Maar Maar 1286 m
Nolf Crater Maar
Oval Crater Crater
West Twin Crater Maar 1326 m

Photo Gallery


Diamond Craters in SE Oregon is a 60 sq km volcanic field consisting of basaltic lava flows and numerous cones and craters. The central vent complex in this photo formed as a result of explosive eruptions from as many as 20 craters and cones. The age of the latest volcanic activity is not known precisely, but could be as young as late Pleistocene or early Holocene.

Oregon Dept. Geology and Mineral Industries photo in Green and Short (1971).
Lava flows of West Dome, one the structural highpoints of Diamond Craters, rise NE of lake-filled Malheur Maar. The shallow 2-m-deep lake occupies one of many maars (the rest of which are dry) of the Diamond Craters volcanic field. Diamond Craters consists of a 60 sq km area of basaltic lava flows, cinder cones, and maars that form a unique geologic environment in the high desert country of SE Oregon. Initial eruptions of pahoehoe lava flows were followed by magma injection that produced six structural highs of up to 120 m.

Photo by Lee Siebert, 2002 (Smithsonian Institution).

Smithsonian Sample Collections Database


A listing of samples from the Smithsonian collections will be available soon.

Affiliated Sites

Large Eruptions of Diamond 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.