Copyright © 1995, 1996, 1997 by Rosanna L. Hamilton. All rights reserved.
|Introduction to Hawaiian Volcanoes|
The volcanic mountains creating the Hawaiian islands are among the greatest mountain ranges on earth. They rise an average of 4,572 meters (15,000 feet) to reach sea level from their base on the sea floor with the highest (Mauna Loa) climbing an additional 4,170 meters (13,680 feet) above sea level. As shield volcanoes, they are built by thousands of accumulated lava flows growing no more than 3 meters (10 feet) at a time to form a broad, gently sloping, flat domed volcanic cone. The islands progressed from northwest to southeast with the first volcanoes becoming extinct as the activity moved southeast. Some researchers believe the archipelago, or group of islands, originated from the accumulation of basalt piles over a great fissure, with the activity shifting progressively to the south. Another hypothesis suggests the Pacific plate is moving over a fixed "hot spot" in the mantle. Today only two volcanoes are left active, the Mauna Loa and the Kilauea at the southeasternmost end of the chain.
After volcanic mountains reach the surface, they are subject to the effects of erosion; unless lava continues to flow, the whole mass could wear away. In the early stages of erosion, a fringing reef will attach to the shore, such as occurred off Waikiki Beach in Honolulu. A fringing reef will eventually become separated from the shore by a lagoon, forming a barrier reef. Eventually erosion or submergence might completely overcome the island and the barrier reef might form an atoll, which is a ring-shaped coral island forming a lagoon. When the top is completely worn away, it leaves a shoal cutting across the volcanic cone several fathoms below sea level, similar to the French Frigate Shoal.
Eruptions in the Hawaiian volcanoes are usually preceded by a series of earthquakes which open fissures and allow magma to reach the surface. Initially lava fountains, known as "curtains of fire," hurl streams of lava hundreds of feet into the air from many points along the fissure. Hawaiian flows are considered to issue forth relatively quietly since the lava is quite fluid, and the gases escape readily without the disruption of the lava into ash or cinders. Great floods of lava will then flow down the mountainside. Eruptions have lasted from a few days to ten months, frequently followed in two or three years by a flank eruption.
Mauna Loa is considered the "monarch of mountains." It is the largest volcano and the largest single mountain of any kind in the world. It is 97 kilometers (60 miles) long, 48 kilometers (30 miles) wide, and rises about 8,742 meters (28,680 feet) from its base on the sea floor. The slopes of Mauna Loa are no steeper than 12°, with a mere 4° slope near the top. On the summit is an oval shaped caldera called Mokuaweoweo which is 4.8 kilometers (3 miles) long, 2.4 kilometers (1.5 miles) wide, and 183 meters (600 feet) deep. Eruptions usually begin as lava fountains on the floor of Mokuaweoweo and are followed by great volumes of lava, although sometimes eruptions flow without the initial outbreak. Mauna Loa is extremely prolific producing .9 to 4.5 million metric tons (1 to 5 million tons) of lava per hour in the early stages of an eruption. In 1831, three-fifths of a cubic mile was added to its mass. During the period between 1831 to 1950, Mauna Loa averaged an eruption every 3.6 years and was active nearly 6.2% of the time [Press, 1986].
The Kilauea Volcano is located about 3,048 meters (10,000 feet) below the summit of Mauna Loa. It is a shield volcano approximately 80 kilometers (50 miles) long and 22.5 kilometers (14 miles) wide that accumulated along the side of Mauna Loa. The summit of Kilauea is 1,250 meters (4,090 feet) above sea level, 6,096 meters (20,000 feet) above the ocean floor. The summit caldera is 4 kilometers (2.5 miles) long, 3.2 kilometers (2 miles) wide, and about 120 meters (400) feet deep. Near the southwestern edge of the caldera is the "fire pit," known as Halemaumau (House of Everlasting Fire), which has at times contained a lake of boiling lava. The pit is enlarged periodically by steam blasts and collapsing walls. In 1924, it was enlarged from 610 to 1,070 meters (2,000 to 3,500 feet) in diameter and measured 396 meters (1,300 feet) deep. Typical eruptions consist of lava flows forming lava lakes in Halemaumau or elsewhere on the caldera through fissures and rift zones. However, Halemaumau seems to be the principle conduit where lava reaches the surface.
The unifying agent among volcanoes is the active ingredient of gas. The primary gas given off in an eruption is water vapor or steam. When water changes from a liquid state to a solid state, the expansion is about one ninth of its volume. When water changes from a liquid state to a gaseous state its volume increases 1,000 times; thus producing the force necessary for a volcanic eruption. Before eruption, water and dissolved gases are confined by the pressure of the overlying rocks, but as the magma rises to the surface the pressure drops and the gases are released. Gas is necessary to move the magma, and magma is the vehicle carrying the gas.
As magma is released from the vent, lava flows along Earth's surface and eventually takes one of two contrasting but related forms which Hawaiians have named aa and pahoehoe (pronounced ah ah and pahoyhoy). Pahoehoe is formed as a layer of "skin" covers the underlying liquid lava and the movement of the continued lava flow below begins to wrinkle the surface creating a ropy or billowy appearance. Pahoehoe in Hawaiian means "ropy." Aa is what a barefoot Hawaiian would say while walking on it: "ah . . . ah . . . oh . . . ah" [Press, 1986]. Its sharp, angular, jagged blocks have dangerously sharp edges and spiny projections on a noncontinuous surface. Some flows issue from the vent as pahoehoe and change to aa as they are stirred, cooled, lose gas, and increase in crystallization. Lava does not convert from aa to pahoehoe. Once a crust has formed on pahoehoe, lava tubes below continue to move the remaining liquid for long periods of time. The size of the tubes range from only a few inches to many feet in diameter. When the source of lava stops, the liquid continues to drain, leaving lava tubes or caves. Spatter cones are steep sided, conical hills built from the spatter of lava fountains. Underwater flows produce pillow lava which are ellipsoidal, sacklike blocks about a meter in dimension budding off of lava tongues or tubes. Lavas can have many features depending on the rate in which they cool.
|Views of Hawaiian Volcanoes|
A'a Lava Flow, Hawaii
A'a lava flows are typically blocky, usually approximately 3-20 meters (10 to 66 feet) thick, and rolls over itself across the ground like a tank track. The jagged flow front normally creeps forward and steepens until a section becomes unstable and breaks off, revealing the incandescent central core. This flow is about 4 meters (13 feet) thick. (Courtesy of S. Rowland/LPI)
Pahoehoe Lava Flow, Hawaii
As a pahoehoe flow spreads out across the ground, the flow surface cools and the majority of lava transport takes place through a series of tubes. In this view the leading edge of the flow field is advancing via a series of breakouts of lava from such a tube system. As can be seen from the scale bar in the image (which is marked in 5-centimeter increments), pahoehoe flows are much thinner than a'a flows, sometimes being only 30-50 centimeters (12 -20 inches) thick. (Courtesy of P. Mouginis-Mark, LPI)
Pahoehoe Lava Flow, Hawaii
The classic "ropy" texture of a pahoehoe lava flow is shown here. Scale bars is marked in 5-centimeter (2-inch) increments. (Courtesy of P. Mouginis-Mark, LPI)
Pu'u O'o Lava Channel, Hawaii
During many of the eruptions of Pu'u O'o Volcano, Hawaii, pahoehoe lava flows became channelized so that the margins (called "levees") became more solid and the lava was moving most rapidly in a central channel. These central channels can also be found within certain lunar and Martian lava flows; they are thought to be an indicator of high discharge rates (more than 100 million kilograms - 220 million pounds - per second). The central channel shown here is approximately 4 meters (13 feet) wide. (Courtesy of S. Rowland/LPI)
Thurston Lava Tube, Hawaii
In Hawaii, many lava flows form tubes that may extend for several kilometers. This is an efficient way for the lava to travel comparatively large distances without significant cooling. Thurston Lava Tube, located close to the summit of Kilauea Caldera, is a fine example of this type of landform. Here the tube is approximately 3 meters (10 feet) in diameter. Note two lava benches on the wall on the left. (Courtesy of P. Mouginis-Mark, LPI)
Fire Fountain Eruption, Pu'u O'o, Hawaii
Scientists studied fire fountains from the phase 34 eruption (August 1984) of Pu'u O'o in Hawaii to investigate the dispersal and cooling of ejected materials. In this view, the incandescent part of the plume is approximately 200 meters (660 feet) high. Large clasts from this fire fountain retained their heat to such an extent that they coalesced on the ground to form a lava flow that moved away from the vent (at right in this view). Pu'u O'o is located about 15 kilometers (9.3 miles) down rift from the summit of Kilauea Caldera, on the East Rift Zone. (Courtesy of P. Mouginis-Mark, LPI)
Channels on Koko Crater, Oahu, Hawaii
The flanks of Koko Crater on the island of Oahu, Hawaii, show signs of extensive gully erosion. Koko Crater is approximately 400 meters (1,320 feet) high. Here we see valleys 3-5 meters (10-16 feet) deep that have been caused primarily by surface water flow and, close to the summit, by sapping. Although spaced further apart on Martian volcanoes such as Tyrrhena Patera, similar valleys might have formed on the older volcanoes on Mars as water from the original explosive eruptions was released at the surface. Note, however, that the valleys on Tyrrhena Patera might be 3-5 kilometers (1.9-3 miles) wide, which is wider than the entire Koko Crater cone. (Courtesy of P. Mouginis-Mark, LPI)
Kupaianah Lava Lake, Hawaii
Using a spectroradiometer, scientists were able to measure the radiative temperature and thermal output from the Kupaianaha Lava Lake. This instrument collects spectra from 0.4-3.0 micrometers in over 800 channels, thereby permitting an accurate determination of the blackbody temperature of the surface. Such studies are of value because they show that the surface of a lava lake (or a lava flow) is remarkably cool - perhaps only a few hundred degrees centigrade - compared to the eruptive temperature of approximately 1,150°C (2,102°F). Such temperatures are quite similar to those the Voyager 1 spacecraft measured for the volcanic activity on Io, suggesting that silicate lavas, as opposed to molten sulfer, could exist within lava lakes on Io. (Courtesy of P. Mouginis-Mark, LPI)
Kilauea Volcano, Hawaii
This is a color composite radar image of the Kilauea volcano on the Big Island of Hawaii. The city of Hilo can be seen at the top. The image shows the different types of lava flows around the crater Pu'u O'o. Ash deposits which erupted in 1790 from the summit of Kilauea volcano show up as dark in this image, and fine details associated with lava flows which erupted in 1919 and 1974 can be seen to the south of the summit in an area called the Ka'u Desert. In addition, the other historic lava flows created in 1881 and 1984 from Mauna Loa volcano (out of view to the left of this image) can be easily seen despite the fact that the surrounding area is covered by forest. The Kilauea volcano has been almost continuously active for more than the last 11 years. A moving lava flow about 200 meters (660 feet) in length was observed at the time of the shuttle overflight. (Courtesy NASA/JPL)
Mauna Loa Volcano, Hawaii
This image of the Mauna Loa volcano on the Big Island of Hawaii shows the capability of imaging radar to map lava flows and other volcanic structures. Mauna Loa has erupted more than 35 times since the island was first visited by westerners in the early 1800s. The large summit crater, called Mokuaweoweo Caldera, is clearly visible near the center of the image. Leading away from the caldera (towards top right and lower center) are the two main rift zones shown here in orange. Rift zones are areas of weakness within the upper part of the volcano that are often ripped open as new magma (molten rock) approaches the surface at the start of an eruption. The most recent eruption of Mauna Loa was in March and April 1984, when segments of the northeast rift zones were active. If the height of the volcano was measured from its base on the ocean floor instead of from sea level, Mauna Loa would be the tallest mountain on Earth. Its peak (center of the image) rises more than 8 kilometers (5 miles) above the ocean floor. The South Kona District, known for cultivation of macadamia nuts and coffee, can be seen in the lower left as white and blue areas along the coast. North is toward the upper left. The area shown is 41.5 by 75 kilometers (25.7 by 46.5 miles), centered at 19.5 degrees north latitude and 155.6 degrees west longitude. The different color combinations in this radar image are caused by differences in surface roughness of the lava flows. Smoother pahoehoe flows are depicted in red, and rougher a'a flows are shown in yellow and white. (Courtesy NASA/JPL)
Mauna Kea Summit, Hawaii
The Landsat Thematic Mapper (TM) obtains data of volcanoes on Earth in six spectral bands between 0.4 and 2.4 micrometers at 30-meters/pixel resolution, and one band between 8 and 12 meters at 100 meters/pixel. Here, TM data allows iron oxides (shown in red) in the cinder cones of Mauna Kea to be identified. Also visible in blue is the distribution of debris generated during the last ice age, which shows that Mauna Kea has not been active for several thousand years. North is at the top. (Courtesy LPI. Landsat 5 path 63, row 40; image enhanced by H. Garbeil)
Vent Area, Kilauea, Hawaii
The December 1974 lava flow erupted from a series of en echelon fissures close to the summit of Kilauea Caldera. Here is an example of a fissure approximately 2 meters (6.6 feet) wide. Fissures of comparable dimensions may also have been the vents for the flows on the flanks of Sif Mons, Venus. (Courtesy of L. Gaddis and LPI)
Mauna Loa Volcano and Mauna Kea Cinder Cones
The shallow slopes of Mauna Loa are clearly seen in this photograph taken looking south from the southern flank of Mauna Kea. Notice some of the cinder cones of Mauna Kea in the foreground; these cones are up to 400 meters (1,312 feet) high. (Courtesy of P. Mouginis-Mark, LPI)
|References and Credits|
Many of the images and captions were taken from the Mouginis-Mark slide set.
Bullard, Fred M. Volcanoes. University of Texas Press Austin & London, 1976.
Press, Frank and Raymond Siever. Earth. W. H. Freeman and Company, New York, 4th edition, 1986.
Mouginis-Mark, Peter. Volcanic Features of Hawaii and Other Worlds. Lunar and Planetary Institute, slide set.