Two craters on the SW caldera wall linked to a 1993 eruption
Alcedo . . . had two new craters when visited by Jonathan R. Green during 16-18 February 1994. According to him and Jim Stimac, who saw the craters in February 1995, the craters were located on the S wall of the caldera. At the same two points, Geist and others (1994) had previously mapped sulfur veneer and fumaroles in 1991. The points lie ~1.4 km W of El Geyser, a fumarole that lies within a similar crater and sits farther E along a common fault. . . . Geist confirmed that there were no craters in this vicinity when he made his map, and in addition Green clearly reported that these two craters were new.
Besides the opening of these new craters, Green (1994) described Alcedo activity during November-December 1993, and January 1994. This included local tremor, explosions, noises from one or more subterranean sources, and increased fumarolic activity. The larger crater was associated with adjacent deposits of ash, debris, and mud. The craters were also observed during a July 1994 helicopter flyover. A videotape made during the flyover (archived at Galápagos National Park Headquarters) documented vigorous steam plumes coming from both craters, similar to plumes seen by Green in February 1994. Green, who showed the craters on a sketch in his report, estimated that the larger crater was 75 x 100 m.
Although groups do occasionally visit, Alcedo is uninhabited and no one witnessed the eruption. Green's report stated: "Additional information from other guides places this activity later than mid-November 1993 and prior to the end of December 1993."
Later observations were made when J. Stimac and Fraser Goff sampled fumaroles . . . from 5 to 10 February 1995. At that time the larger new crater issued a vigorous steam plume from a small vent along one side; the smaller crater issued less steam. Stimac estimated that the elliptical larger crater had a diameter of 100-150 m, and a depth of 35-40 m. The smaller crater had a diameter of 10 m and a depth of 3 m.
Layered tephra, up to perhaps 2-m thick, lies at the crater margins and extends for several hundred meters, Stimac reported. Based on the observed deposits, and on crater morphology and location, visiting volcanologists concluded the craters were formed by hydrothermal explosions.
Geist and others (1994) point out that Alcedo is distinct from other Galápagos volcanoes (and many oceanic islands) in that it has erupted rhyolite and not just basalt as seen on all the adjacent islands.
References. Geist, D., Howard, K., Jellinek, A. M., and Rayder, S., 1994, The volcanic history of Volcán Alcedo, Galápagos Archipelago: A case study of rhyolitic oceanic volcanism: Bulletin of Volcanology, v. 56, no. 4, Springer-Verlag, p. 243-260.
Green, J., 1994, Recent activity in Alcedo volcano, Isabela Island: Noticias de Galápagos, no. 54 (H. Snell, editor): The Charles Darwin Foundation for the Galápagos Islands (100 N. Washington St., Suite 311, Falls Church, VA 22046 USA), p. 11-13.
Information Contacts: J. Green, Quito; D. Geist, University of Idaho; J. Stimac and F. Goff, LANL, Los Alamos.
The Global Volcanism Program has no Weekly Reports available for Alcedo.
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.
False activity report caused by a fire
Card 1038 (02 November 1970) Bluish smoke emanating from near the rim seen from research vessel
The following is from Forest Nelson. The research vessel "Alpha Hellix" of Scripps Institution in La Jolla, heading south from James Bay to Santa Cruz, sighted quite a bit of smoke emanating near the rim, either inside or outside the rim, of the south wall of the crater Alcedo which is the third volcano from the north--really the third volcano on Isabella--the one with the geyser inside the crater and lots of tortoises around the rim and also in the interior. This is the first time I have heard of or known of any activity in the Alcedo area. At night they were not able to see if there was any flame or glow because of heavy cloud cover over the area. There was no activity on the siesmograph at the station here.
The following report was radioed to Scripps by Captain Haines of the "Alpha Hellix." "At noon on 26 October several persons aboard "Alpha Hellix" sighted what could have been volcanic activity from a crater at Lat 0° 25.5 south Long. 91° 06.5 west on Isla Isabella. Activity was in the form of conspicuous, but not spectacular, smoke. It had a bluish tint. The phenomenon was visible during the daylight hours on the 26th, but could not be observed on the 27th due to cloud cover. The ship departed the Galapagos on the 28th."
Card 1045 (10 November 1970) No seismic or satellite evidence of activity
"Initial inspections of the National Oceanic and Atmospheric Administration (NOAA) world-wide networks show no evidence of seismicity or infrasonic disturbances in the Galapagos around the time of the reported activity in Alcedo. ITOS satellite photos show no sign of a volcanic cloud despite generally clear conditions during this period.
"Under good conditions, normal vapor emission from the Alcedo geyser area has been seen from 40 km away, but the description given by the "Alpha Hellix" suggests above-normal activity."
Card 1051-1052 (17 November 1970) Fire was the source of smoke, not volcanism
The following report was received by radio from Craig MacFarland on 17 November 1970. "The activity is not a volcanic eruption but a large fire of unknown cause. I checked the area carefully, and the fire is still burning. We couldn't go down into it because it was on the inside wall and was simply too steep to even attempt to go down. The ashes from the fire were very deep and it was just plain dangerous. From surveying the fire from above and from many places on the rim far away, we couldn't see anything that looked like fumarole activity or lava or anything of that sort in that area. The location appears to be on the southeast wall of the caldera. As far as I could tell the wildlife population was not affected.
"The burned area was relatively large but small in relation to the whole rim, and occurred only on the inside wall of the rim to about one-half way to the floor. The longest side of it was actually on the rim and I would estimate that it went for 500-600 m along the rim and from there coming in a triangle from the southern and the northern side going toward the floor. I checked the ash only on the rim and it varied from a few centimeters deep to roughly two feet deep in the deepest place.
"The fire destroyed all the vegetation which consisted mostly of shrubs and herbs. The shrubs were a maximum height of 6-7 feet and there was an occasional taller tree. In some areas within the main body of the fire and on the edges, it actually burned everything including the undergrowth.
"In terms of animals that wouldn't be able to get away from the fire quickly, I immediately thought of the tortoises. Their tracks came right up the side of the wall right through the ash and onto the rim where the burning had stopped. I surveyed the area with field glasses from various places and could see no tortoise carcasses. I couldn't see that any other animals were harmed by the fire. I suspect most birds left the area immediately; also the burros. The whole volcano has the largest population of tortoises on the island (estimated to be 3-6 thousand tortoises). The particular area on the rim where the fire started and including all the burned area, was the area of densest tortoise population. At any given time there might be 50-60 tortoises in the total burned area and apparently they had been able to get away before it burned. Their tracks occurred along the crater rim up to where the fire had occurred and on the fifth night of the fire below the rim on the inner wall we could see animals, so they had clearly gotten away from it.
"We were up in the caldera for 4 days. We went up November 11 and came down November 15th. It was burning during the entire time. Occasionally a little smoke would come up above the rim. The day we came down to the beach we continued to see smoke. I suspect that itis still burning."
Information Contacts:
Card 1038 (02 November 1970) Forest Nelson, Santa Cruz, Galapagos Islands, Ecuador; Carl Hubbs, Scripps Institute of Oceanography, La Jolla, California, USA.
Card 1045 (10 November 1970) NOAA; T. Simkin, SI.
Card 1051-1052 (17 November 1970) Craig MacFarland, Academy Bay, Galapagos Islands, Ecuador; Darwin Biological Research Station, Galapagos Islands, Ecuador.
Loud booming sounds with accompanying felt shocks; changes at fumarolic area
Loud "booms" (sounds like underground detonations, of varying intensities and seemingly different source directions), first reported by scientists in mid-March, were documented during fieldwork 20-27 March. The loudest, at around 1800 on 21 March, was almost immediately followed by a strongly felt shock (estimated to have 2-3 cm of vertical displacement at one location). Less intense "booms," occasionally followed by felt shocks, were heard at a rate of 2-13/day; variations may reflect location and activity of the observers. One notable "boom" and shock was followed by ground shaking that lasted more than a minute. While inside the caldera, observers reported a fairly constant "very low, barely audible, throbbing rumble" which they compared to the engines of a large ship.
No substantial changes were noted at the fumarole area (in the SW portion of the caldera) since the previous visit in 1986. However, vegetation had receded possibly as much as 20 m from around most fumarole areas. Numerous fresh, hairline fissures, two to several dozen meters long, were visible along the lower border of the fumarole field, coinciding with devegetation. Steam emission from a large vent on the SE caldera wall, a geyser until drying up in 1970, was substantially weaker than in 1986 and the sound had changed from a jet roar to "more of an underground rumble".
The first earthquake (mb 4.9) to be located in Galápagos since [5 July 1990] occurred at [0659] on 3 March. Its hypocenter was [25] km [NW] of Alcedo, but accurate locations are difficult in that region and the threshold for locatable earthquakes normally exceeds M 4.
Information Contacts: T. De Roy and M. Jones, Isla Santa Cruz; NEIC.
Sonic activity and felt earthquakes decline; minor changes to hydrothermal system
Late-April fieldwork revealed continued but diminished sonic activity, no evidence of an eruption, and only minor changes to the volcano's hydrothermal system.
Biologist Milton Friere, working on the island since February, reported that he felt a strong shock, apparently on 9 March at about 1900. Hunters on Santiago Island, 35 km NE of Alcedo, also felt a large earthquake around that time but there is uncertainty about the date and the WWSSN recorded only the 3 March event (16:3). Immediately after the felt earthquake, explosion sounds began to be heard daily at Friere's camp on the caldera's N rim. The initial sounds were the most intense and frequent, then they declined gradually, and by late April were heard only once every few days from the N rim camp. Fewer than 5 earthquakes were felt at the camp until 5 April. Others were documented on 5 April at 1740, 7 April at 1700, and 17 April at 1725. Events of similar intensity may have gone unnoticed during active fieldwork.
While camped on the caldera's S rim during a 23-28 April field survey, Dennis Geist heard eight explosion sounds in 3 days, compared to 2-13 heard daily by Tui DeRoy and Mark Jones in late March (16:3). All were heard in camp, with none noticed during fieldwork. The sounds, consisting of deep rumbling lasting about a second, were likened to thunder generated ~ 10 km away. Although the sounds were clearly directional, each seemed to come from a different direction. None were accompanied by discernible changes in fumarole output, but two were followed 10-15 seconds later by a felt earthquake. The stronger earthquake lasted 5-10 seconds, whereas the weaker one continued for more than 30 seconds after a strong initial jolt.
The seismicity and sonic activity were preceded by the first heavy rains in the Galápagos for several years. Between 26 February and 4 March, 5-10 cm of rain fell daily on Alcedo. Heavy rains also fell on 6, 8, 10, 19, and 30 March, and 10 and 15 April.
Geist noted only subtle changes to the hydrothermal system. Before the 1991 activity, hundreds of fumaroles were distributed around both the southern ring faults and a vent that erupted voluminous rhyolitic pumice and obsidian flows about 90,000 years ago. Fewer than 10 small new fumaroles (identified by remains of recently killed plants) were observed, and no significant increase in total gas output was evident. A large fumarole (called "the Geyser" because it formerly ejected water) may have been somewhat more vigorous than during Geist's previous visits in 1989 and 1983. The vapor plume from this fumarole varied dramatically over periods of hours, and at times there was no visible cloud. No recently formed fissures or fault scarps were observed.
Information Contacts: D. Geist, Univ of Idaho.
Two craters on the SW caldera wall linked to a 1993 eruption
Alcedo . . . had two new craters when visited by Jonathan R. Green during 16-18 February 1994. According to him and Jim Stimac, who saw the craters in February 1995, the craters were located on the S wall of the caldera. At the same two points, Geist and others (1994) had previously mapped sulfur veneer and fumaroles in 1991. The points lie ~1.4 km W of El Geyser, a fumarole that lies within a similar crater and sits farther E along a common fault. . . . Geist confirmed that there were no craters in this vicinity when he made his map, and in addition Green clearly reported that these two craters were new.
Besides the opening of these new craters, Green (1994) described Alcedo activity during November-December 1993, and January 1994. This included local tremor, explosions, noises from one or more subterranean sources, and increased fumarolic activity. The larger crater was associated with adjacent deposits of ash, debris, and mud. The craters were also observed during a July 1994 helicopter flyover. A videotape made during the flyover (archived at Galápagos National Park Headquarters) documented vigorous steam plumes coming from both craters, similar to plumes seen by Green in February 1994. Green, who showed the craters on a sketch in his report, estimated that the larger crater was 75 x 100 m.
Although groups do occasionally visit, Alcedo is uninhabited and no one witnessed the eruption. Green's report stated: "Additional information from other guides places this activity later than mid-November 1993 and prior to the end of December 1993."
Later observations were made when J. Stimac and Fraser Goff sampled fumaroles . . . from 5 to 10 February 1995. At that time the larger new crater issued a vigorous steam plume from a small vent along one side; the smaller crater issued less steam. Stimac estimated that the elliptical larger crater had a diameter of 100-150 m, and a depth of 35-40 m. The smaller crater had a diameter of 10 m and a depth of 3 m.
Layered tephra, up to perhaps 2-m thick, lies at the crater margins and extends for several hundred meters, Stimac reported. Based on the observed deposits, and on crater morphology and location, visiting volcanologists concluded the craters were formed by hydrothermal explosions.
Geist and others (1994) point out that Alcedo is distinct from other Galápagos volcanoes (and many oceanic islands) in that it has erupted rhyolite and not just basalt as seen on all the adjacent islands.
References. Geist, D., Howard, K., Jellinek, A. M., and Rayder, S., 1994, The volcanic history of Volcán Alcedo, Galápagos Archipelago: A case study of rhyolitic oceanic volcanism: Bulletin of Volcanology, v. 56, no. 4, Springer-Verlag, p. 243-260.
Green, J., 1994, Recent activity in Alcedo volcano, Isabela Island: Noticias de Galápagos, no. 54 (H. Snell, editor): The Charles Darwin Foundation for the Galápagos Islands (100 N. Washington St., Suite 311, Falls Church, VA 22046 USA), p. 11-13.
Information Contacts: J. Green, Quito; D. Geist, University of Idaho; J. Stimac and F. Goff, LANL, Los Alamos.
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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Calderon, Volcan | ||||
Craters |
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Feature Name | Feature Type | Elevation | Latitude | Longitude |
Cowley Island | Fissure vent | 0° 23' 0" S | 90° 57' 0" W |
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There is data available for 2 confirmed Holocene eruptive periods.
1993 Dec 5 ± 20 days Confirmed Eruption VEI: 1
Episode 1 | Eruption | South caldera wall | |||||||||||||||||||||||||||||||||||||||
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1993 Dec 5 ± 20 days - Unknown | Evidence from Observations: Reported | |||||||||||||||||||||||||||||||||||||||
List of 6 Events for Episode 1 at South caldera wall
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[ 1954 Nov 9 ] Discredited Eruption
1953 Jul 2 ± 7 years ± 182 days Confirmed Eruption VEI: 0
Episode 1 | Eruption | SE flank near Cartago Bay | |||||||||||||||||||
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1953 Jul 2 ± 7 years ± 182 days - Unknown | Evidence from Observations: Reported | |||||||||||||||||||
List of 2 Events for Episode 1 at SE flank near Cartago Bay
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There is data available for 2 deformation periods. Expand each entry for additional details.
Reference List: Hooper et al. 2007.
Full References:
Hooper A, Segall P, Zebker H, 2007. Persistent scatterer InSAR for crustal deformation analysis, with application to Volcán Alcedo, Galápagos. J. Geophys. Res., 112, B07407. https://doi.org/10.1029/2006JB004763
Reference List: Amelung et al. 2000.
Full References:
Amelung F, Jónsson S, Zebker H, Segall P, 2000. Widespread uplift and "trap-door" faulting on Galápagos volcanoes observed with radar interferometry. Nature, 407, 993-996. https://doi.org/10.1038/35039604
There is no Emissions History data available for Alcedo.
The Global Volcanism Program has no maps available for Alcedo.
The following 7 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 |
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NMNH 117455-41 | Obsidian | -- | -- |
NMNH 117455-42 | Obsidian | -- | -- |
NMNH 117455-43 | Obsidian | -- | -- |
NMNH 117455-44 | Obsidian | -- | -- |
NMNH 117455-45 | Obsidian | -- | -- |
NMNH 117455-46 | Obsidian | -- | -- |
NMNH 117455-47 | Pumice | -- | -- |
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 Alcedo. 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 Alcedo. 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. |
Large Eruptions of Alcedo | 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). |