Ringing rocks

Ringing Rocks are rocks that have the property of resonating like a bell when struck, such as the Musical Stones of Skiddaw in the English Lake District as well as the stones in Ringing Rocks Park, in Upper Black Eddy, Bucks County, Pennsylvania USA and the Bell Rock Range of Western Australia. Ringing rocks are also known as sonorous rocks or lithophonic rocks, as used in idiophonic musical instruments called lithophones.

Contents

Ringing Rocks Park

Ringing Rocks Park is a county park in Upper Black Eddy, Pennsylvania at .[1] The ringing rocks in that area are diabase. In 1965, geologist Richard Faas of Lafayette College took a few of the rocks back to his lab for testing. He found that when the rocks were struck they created a series of tones at frequencies lower than the human ear can hear. An audible sound is only produced because these tones interact with each other. Although Faas's experiments explained the nature of the tones, they did not identify the specific physical mechanism in the rock which made them.[2]

Diabase Ringing Rock Boulder Fields in Pennsylvania and New Jersey

In southeastern Pennsylvania and southern New Jersey there is a series of boulder fields which contain boulders that ring when struck by a hard object. Although various rock types are known to develop the ringing ability, these boulder fields fall into a specific category of being composed of olivine diabase. The boulder fields formed from a group of diabase sills located in the geologic Newark Basin. The sills were formed when mafic magma from the upper mantle injected into the sedimentary basin 200 million years ago (Early Jurassic Period). When the diabase sills were still molten crystals of olivine and pyroxene settled to the bottom of the sill and formed a thin, separate unit. By the Pleistocene Epoch (most recent Ice Age - 2,588,000 to 11,700 years BP) the sills had been exposed to the surface by crustal uplift and erosion. During the Pleistocene outcrops of the olivine diabase were not buried by the glacial sheets, however they were subjected to severe freezing, or periglacial, conditions. The periglacial environment caused the outcrops to be broken into extensive boulder fields.

Location of the Diabase Ringing Rock Boulder Fields

Although there have been over a dozen diabase ringing rock boulder fields identified (see Pontolillo 1993 for an extensive inventory of sites), the majority are either on private property or have been obliterated by urban development. There are three sites north of Philadelphia which are readily accessible to the public: Ringing Rocks County Park in Bridgeton Township near Upper Black Eddy; Stony Garden on the north slope of Haycock Mountain (PA State Game Lands Tract #157); and the Ringing Hill Park in Lower Pottsgrove Township. The Bridgeton site is the one most commonly identified with ringing rocks, and has been the subject of numerous nature and travel articles.

Geology of the Boulder Fields

These particular ringing rock boulder fields formed from a rock type called olivine diabase. Approximately 200 million years ago stretching of the Earth’s crust allowed basaltic magma to travel up from the upper mantle and inject as sills into a series of shale formations of the Newark Basin. Phenocrysts of two minerals that had crystallized in the upper mantle, olivine and pyroxene, quickly settled out of the magma and collected along the base of the sills. When fully solidified this crystal-rich layer formed a separate rock unit 10’-15’ (3-5 m) thick (McCray 1997). The basal olivine unit is similar to the one found in the Palisades Sill in New Jersey and New York. The olivine diabase unit is significantly harder, denser, and more resistant to weathering than the upper portions of the diabase sill.

Most observers did not make the distinction between the upper 'normal' diabase which is found over wide areas, and the thin olivine diabase unit found at the base of the sills which actually produces the ringing rock boulder fields. A main factor in the confusion is the outward appearance of the rocks. Both the normal and olivine diabase rocks are dark grey to black in color. It is difficult to distinguish the two in hand specimens, and often requires microscopic examination to identify the differences.

Although the Newark series diabase sills crop out in a belt throughout the length of the Appalachian Mountains, only a narrow band of outcrops in southeastern Pennsylvania and New Jersey develop ringing rock boulder fields. The probable reason is that these areas were at the southern edge of the Pleistocene glaciers, and would have been subject to extreme periglacial conditions. Periglacial boulder fields are a common feature in Pennsylvania and New Jersey.

All of the observed ringing rock boulder fields in southeastern Pennsylvania and New Jersey are a form of felsenmeer. Felsenmeer is a german term meaning "sea of rock". These barren block fields occur in periglacial environments where outcrops of resistant rock are exposed with a slope of less than 25°. Frost wedging breaks up the upper portion of the rock formation, and the slight dip of the field allows the fine weathering materials to be flushed away before soil can develop. Often the boulders are lifted and rotated by the accumulation of snow and ice, leaving a considerable amount of vacant space between them. The felsenmeer boulder fields form in-situ due to the low slope angles. In situations where the slope angles are steeper than 25°.gravity tends to move the boulders downhill to form scree or talus slopes. In fields where the angle is too flat the spaces between the boulders fills with soil and the boulders break down due to weathering.

Because the olivine diabase unit is relatively thin there was an additional requirement for the formation of the ringing rock boulder fields: the olivine diabase unit had to be dipping in the same direction as the slope of the ground surface. This specific dip-slope situation allowed broad expanses of olivine diabase to be exposed and provided enough material to create the fields. In all of the observed boulder fields the structural dip of the unit was approximately 8-10°, and the ground surface slope was <15° in the same direction. Typically this occurred where the olivine diabase unit dipped at right angles into a shallow drainage. Where the olivine diabase does not dip in the same direction as the ground surface there is generally numerous boulders embedded in the soil (boulder colluvium), but no boulder fields.

Ringing Ability of Individual Boulders

There has been a great deal of controversy concerning the ringing ability of the boulders, conversely there has been an almost complete lack of testing to support the conjectures. Conditions such as size and shape of the boulders, and the way that the boulders are supported or stacked certainly influences the sounds that the boulders make, but do not in themselves impart the ringing ability.

Although the sound is often described as metallic, it is most likely due to a combination of the density of the rock and a high degree of internal stress. The sound can be duplicated on a small scale by tapping the handle of a ceramic coffee cup.

The iron content of the diabase is often identified as the source of the ringing ability. Actual chemical analysis of the Coffman Hill diabase (McCray 1997) shows that iron content (as Fe2O3) ranges between 9-12% of the whole rock for various samples throughout the diabase sill. Although comparatively high for an average igneous rock type (3% is typical for granite), it is within the normal range for a basalt. This point suggests that the iron content is not a primary factor in the ringing ability.

So far there has been only one published scientific experiment on the source of the ringing ability. In the 1960's a Rutgers University professor did an informal experiment where specimens of 'live' and 'dead' ringing rock boulders from the Bucks County park site were sawn into thin slices and then measured for changes in shape (Gibbons 1970). The rock slices were measured with delicate foil strain gauges which could measure minute changes in size. According to the professor, the dead rocks showed no change after the rocks were sawn, however the live rocks showed a distinctive expansion or 'relaxation' within 24 hours after they were cut. This relaxation indicates that the rock was under internal elastic stresses which were released by the mechanical sawing of the rock. The professor went on to make the observation that the live rocks were generally found toward the middle of the boulder fields where they did not come in contact with soil and the shade of the surrounding trees. He then theorized that the slow weathering rate in the dry 'microclimate' of the fields caused the stresses because the outside skin of the boulders would expand due to the conversion of pyroxene to montmorillonite (a clay mineral). Boulders along the periphery of the fields weather too quickly and break apart before the stresses can develop.

Although more rigorous testing needs to be done to verify these results, it does suggest strongly that the ringing ability is a direct result of internal elastic stresses. Less likely is the assertion that outside weathering conditions created the stresses. It is very improbable that the expansion of a thin skin around the outside of a large boulder could set up a balance of forces that would create the severe stresses found in the ringing rock boulders. The result of such a situation would be that the outside skin of the boulders would peel or exfolliate, a condition that is virtually non-existent in any of the ringing rocks sites. In addition, the majority of the weathering in the boulders occurs at the exposed top surfaces, not on the bottoms, thus the stresses would not be balanced. As a reality check, if slow weathering created the stresses then there would be ringing rock boulder fields in deserts throughout the world, a condition which does not occur.

An important point made in the experiment is the observation that the rock slices expanded when the stress was released. This distinction requires that the rock was under extreme compressive stress, not tension as the slow weathering theory implies.

A more plausible theory is that the elastic stresses remained in the rock when the boulder fields formed, and the slow weathering rate keeps the stresses from dissipating. A possible source of the stresses would likely be the loading stresses from the time when the rock crystallized. The diabase sill formed at roughly 2-3 kilometers beneath the surface (Sevon 1999). The overlying column of rock creates severe stresses in rocks. The effects of these stresses can be seen in deep mines (> 1 mile depth), where the sudden decompression creates rock bursts. Residual loading stresses would be evenly distributed throughout the boulders. This theory supports the observation that usually less than a third of the boulders in any given field are 'live'. The stresses are relieved in boulders that have been either mechanically broken or are severely weathered, and therefore no longer ring.

This 'relict stress' theory implies that the ringing rock boulders act much like a guitar string. When a guitar string is limp it does not resonate, but a plucked string will provide a range of sounds depending on the level of applied tension. Likewise, a ringing rock boulder will only emit a dull thud if the boulder is de-stressed, however boulders will resonate at various frequencies depending on the level of residual stress.

The boulders continue to ring when removed from the boulder fields. Myths have been developed by authorities to discourage the theft of boulders from the fields. At the current stage, however, most fields have been picked clean of small portable 'ringers', and breaking of large boulders into smaller pieces releases the internal stresses - thus causing them to stop ringing (ie, breaking a piece off of a large ringing rock will only gain a dead chunk of rock and destroy a natural curiosity forever.) 'Small' ringers found today weigh over a ton, and would have to be dragged out of the boulder fields using large equipment.

Weathering textures

A curious aspect of the ringing rock boulders in all of the boulder fields is the presence of odd weathering textures. Often the weathering textures take on the form of channels, grooves, 'potholes', 'mudcracks', and intense pitting. In some cases the textures are so distinctive that some geologists refer to them in terms of carbonate rock solution features (Sevon 1999). Inspection of the boulders reveals that the weathering patterns are not due to any internal variations in the rock, but have been superimposed onto the surfaces. The probable source of these textures was chemical weathering along joint surfaces at the time that the rock was still in place and before the boulders were broken out by frost heaving (Psilovikos 1982). The soft weathered portion of the outer surfaces flaked off once the boulders were exposed to the air. Small features on the boulder surfaces became exaggerated as the weathered material was removed, so that adjoining fissures became channels, dents became 'potholes', and old surfaces became intensely pitted.

Ringing Rocks Pluton, Jefferson County, Montana

The Ringing Rocks Pluton is located in the mountains of southwest Montana between Butte and Whitehall, and is notable for a large tor of boulders which ring when struck with a hard object. The pluton is the deep-seated vent for a volcano which erupted 76 million years ago. The peculiar aspect of the pluton is that it is an excellent example of magma mixing in a conduit, specifically between olivine basalt and granitic magmas. Mixing of the magmas created a curious hybrid rock type which crystallized against the outer wall of conduit. After millions of years of uplift and erosion the thin walls of hybrid rock were exposed to the surface. During the Pleistocene Epoch periglacial freezing shattered the high standing walls to form a substantial tor.

Location

The Ringing Rocks Pluton is located on the southwestern flank of Dry Mountain in Jefferson County, 15 miles southeast of Butte in T.2 N., R.5 W., sections 4 and 9. Section 4 is included in the Deerlodge National Forest, and section 9 is under the jurisdiction of the U.S. Bureau of Land Management. A distinctive tor is marked on the U.S. Geological Survey Dry Mountain 7½' quadrangle. The NW¼ of Section 9, which includes the tor, was established as the Ringing Rocks Recreation Area by the USBLM in 1964. Access is by a gravel road leading 3 miles north of the Pipestone exit off I-90.

Geology of the Ringing Rocks Pluton

The Ringing Rocks Pluton is a small-scale intrusive ring complex with a high degree of symmetry. The overall geometry is cylindrical, with an average diameter of one kilometer. The pluton consists of two major units: an inner core of quartz-bearing felsic units with a diameter of 600 meters; and an outer mafic unit composed of coaxial concentric layers. In map view the complex has a bulls eye configuration. The outer zone of the pluton consists of two alternating mafic hybrid rock types. In chemical analysis the rocks are nearly identical, however the early stage minerals, olivine and pyroxene, were preserved in one and not the other, giving the rocks sharply different weathering properties. The rock that retained the olivine and pyroxene crystals (OPM) is extremely resistant to weathering and is the material which forms the tors. The altered rock (AM) conversely is very weak and readily breaks down to a coarse soil. The inner felsic core is a medium grained quartz monzonite that gradually grades into granite at the center. The transitional unit between the mafic zone and the felsic core units is completely obscured, and is represented by distinctive low-lying swales. A series of radial dikes punctured the mafic units, beginning in the felsic zone and terminating at the outer border of the intrusion. The dikes are generally 2-4 meters wide where they are in contact with the felsic unit. The composition is highly variable, but for the most part is composed of fine to medium grained leucocratic monzonite. The dikes become narrower as they extend toward the outer border, and generally taper to less than 0.5 m in width.

Microscopic Quench Textures in the Olivine Pyroxene Monzonite

There are numerous textures in the hybrid OPM unit which indicate that the rock was rapidly quenched during crystallization.

Crystals of cryptoperthetic orthoclase up to 1 cm in length can be seen in hand specimens throughout most of the OPM units. The cryptoperthite crystals typically show as deep blue flashes, although white and yellow flashes can be seen in rocks nearer to the contacts. The flashes are due to labradorescent internal reflections, sometimes called a moonstone effect. In early reports (Butler 1983, Johannesmeyer 1999) this mineral was mistakenly identified as labradorite. Cryptoperthite textures form when orthoclase (a feldspar mineral containing both potassium and sodium cations) is quenched very rapidly. Sodium has a much larger ionic radius than potassium does, so during the quench event the sodium ions pop out of the crystal framework. These sodium ions form tiny oriented lenses of albite (sodium silicate feldspar) that are too small to be seen even using a microscope. It is the reflections from these albite laminae that produces the flash.

Apatite occurs as elongated needles . Many of the needles enclose narrow fluid inclusions, giving the crystals the appearance of being ‘hollow’.

Zircon crystals were identified in skeletal frameworks.

Similar Intrusions

The Ringing Rocks Pluton is one of several bimodal vent complexes that are located within a 20 km belt east of the main Butte Pluton. Radiometric dating and cross-cutting relationships place most of these intrusions as post-Elkhorn Mountains Volcanics and pre-Butte Pluton. Similar intrusions can be found in the Rader Creek Pluton.

The Ringing Rocks Tor

The pile of loose boulders at the south end of the pluton which contains the ringing rocks is called a tor. The reason the tor developed is that the OPM units are extremely resistant to weathering, and conversely the adjoining AM and ABM units are very weak. As the Dry Creek drainage began to erode the NW corner of the pluton, the softer AM and ABM units were quickly stripped away, leaving vertical thin walls of OPM units standing high above the surrounding landscape. Intense freezing and thawing during the Pleistocene periglacial period slowly shattered the walls, much like breaking tempered glass. The remnants of the OPM walls is the material which formed the tor. At the north end of the pluton the orientation of the OPM units was at an acute angle to the Dry Creek drainage so that the tor there did not develop very well. On the south end, however, the OPM outcrop was nearly at a right angle to the drainage, producing a prominent tor.

Ringing Properties of the Individual Boulders

Although the rocks are from different geologic settings, the Montana ringing rocks share significant characteristics with the Pennsylvania diabase ringing rocks. These characteristics include being composed of igneous mafic rock types with high percentages of olivine and pyroxene phenocrysts, having the individual boulders isolated from severe weathering by the formation of well-drained boulder fields, and having similar sounds and surface weathering.

The iron content of the olivine pyroxene monzonite (as FeO) is 7% of the whole rock (Butler 1983, Johannesmeyer 1999). As in the Pennsylvania diabase ringing rocks, this point suggests that iron content is not a primary factor in the ringing ability.

Despite the broad public interest in the ringing ability of the ringing rocks there has not been any actual scientific studies to identify the source of the phenomenon.

Weathering Textures in the Olivine Pyroxene Monzonite

Boulders of the olivine pyroxene monzonite develop odd surface weathering patterns, similar to the textures seen in the Pennsylvania diabase ringing rocks. These textures include channels, grooves, and 'potholes'.

REFERENCES

Blake, S., and Campbell, I., 1986, The dynamics of magma-mixing during flow in volcanic conduits: Contributions to Mineralogy and Petrology, v.94, p. 72-81

Butler, B.A., 1983, Petrology and geochemistry of the Ringing Rocks Pluton: unpublished B.A. thesis, University of Montana, Missoula, 70 p.

Carrigan, Charles R., and Eichelberger, J., 1990, Zoning of magmas by viscosity in volcanic conduits: Nature, v. 343, p. 248-251

Daniel, F., and Berg, R., 1981, Radiometric dates of rocks in Montana: Montana Bureau of Mines and Geology Bulletin 114, 136 p.

Haggerty, S.E., and Baker, I., 1967, The alteration of olivine in basaltic and associated lavas -- part I: High temperature alteration: Contributions to Mineralogy and Petrology, v. 16, p. 233- 257

Hibbard, M.J., 1979, Myrmekite as a marker between preaqueous and postaqueous saturation in granitic systems: Geological Society of America Bulletin, v. 90 (part 1), p. 1047-1062

--- 1981, The magma mixing origin of mantled feldspars: Contributions to Mineralogy and Petrology, v. 76, p. 158-170

Huppert, H.E., Sparks, R., and Turner, J., 1982, Effects of volatiles on mixing in calc-alkaline magma systems; Nature, v. 297, pp. 554-557

--- and Sparks, R., 1988, The generation of granitic magmas by intrusion of basalt into continental crust: Journal of Petrology, v. 29, p. 599-624

--- 1989, Chilled margins in igneous rocks: Earth and Planetary Science Letters, v. 92, p. 397-405

Johannesmeyer, Thomas C., 1999, Magma mixing and mingling in the Late Cretaceous Ringing Rocks Pluton, Jefferson County, Montana, and implications for the generation of the Boulder Batholith: unpublished M.S. thesis, University of Montana, Missoula, 208 p.

Koyaguchi, T., 1985, Magma mixing in a conduit: Journal of Volcanology and Geothermal Research, v. 25, p. 365-369

Lambe, R.N., 1981, Crystallization and petrogenesis of the southern portion of the Boulder Batholith, Montana: unpublished PhD thesis, University of California, Berkeley, 202 p.

Lofgren, G.E., and Gooley, R., 1977, Simultaneous crystallization of feldspar intergrowths from the melt: American Mineralogist, v. 62, p. 217-228

Prostka, H.J., 1966, Igneous geology of the Dry Mountain Quadrangle, Jefferson County, Montana: U.S. Geological Survey Bulletin 1221-F, 21 p.

Robinson, G.D., Klepper, M., and Obradovich, J., 1968, Overlapping plutonism, volcanism, and tectonism in the Boulder Batholith Region, Western Montana: in Coats, R.R., Hay, R.L., and Anderson, C.A. (eds), Studies in Volcanology; Geological Society of America Memoir 116, p. 557-576

Rutland, C., 1985, Geochemistry of the Elkhorn Mountains Volcanics, Southwestern Montana: implications for the early evolution of a volcanic-plutonic complex: unpublished MS thesis, Michigan State University, Kalamazoo, 96 p.

Schmidt, C.J., Smedes, H., and O'Neill, J., 1990, Syncompressional emplacement of the Boulder and Tobacco Root batholiths (Montana- USA) by pull-apart along old fault zones: Geological Journal, v. 25, p. 305-318

Smedes, H.W., 1973, Regional setting and general geology of the Boulder Batholith, Montana, in Guidebook for the Butte Field Meeting of the Society of Economic Geologists, R.N. Miller ed., pp. E1-E18

Sparks, R.S.J., and Marshall, L., 1986, Thermal and mechanical constraints on mixing between mafic and silicic magmas: Journal of Volcanology and Geothermal Research, v. 29, p. 99-124

Vejmelek, L., and Smithson, S., 1995, Seismic reflection profiling in the Boulder Batholith, Montana: Geology, vol. 23, pp. 811-814

Watson, E. B., 1979, Zircon saturation in felsic liquids: experimental results and applications to trace element geochemistry: Contributions to Mineralogy and Petrology, v. 70, p. 407-419

Wyllie, P.J., Cox, K., and Bigger, 1962, The habit of apatite in syenite systems and igneous rocks: Journal of Petrology, v. 3, p. 238-243

Bell Rock Range

The Bell Rock Range is a large ultramafic gabbro-peridotite intrusion in the Musgrave Block of Western Australia, near Warburton, 40 kilometres (25 mi) south of the Wingellina community in the Ngaanyatjarra lands.[3] It is composed of massive, heavily indurated intrusive rocks and forms a prominent 15 kilometres (9.3 mi) long range of mountains and hills. The intrusion is called the Bell Rock Range because, when struck, the rocks ring like a bell. It is also the site of an exploratory gold mine.[3]

List of sites

See also

References

Gibbons, J., and Schlossman, S., 1970, Rock Music: Natural History, v. 79, p. 36-41

McCray, S. S., 1997, Petrogenesis of the Coffman Hill diabase sheet, Easton Pennsylvania; unpublished B.S. thesis, Lafayette College, Easton

Pontolillo, J., and Pontolillo, J. 1993, Ringing Rocks Sites in Pennsylvania and New Jersey; INFO Journal #68 [Comprehensive review of all known ringing rock sites in PA and NJ.]

Psilovikos, A., and Van Houten, F., 1982, Ringing Rocks barren block field, East - Central Pennsylvania: Sedimentary Geology, v. 32, p.233-243

Sevon, W. D., and Fleeger, G., 1999, Ringing Rocks Block Field; Guidebook, 64th Annual Field Conference of Pennsylvania Geologists, Allentown, Pennsylvania, pp. 112-121

Further reading

Corliss, W.R., 1989, Anomalies in Geology: Physical, Chemical, Biological: The Sourcebook Project, Glen Arm, MD, p. 218-224

Fackenthal, B.F., Jr., 1932, Ringing Rocks of Bridgeton Township, Bucks County, Pennsylvania, Bucks County Historical Society, Paper 5, pp. 212-221

Faas, R. W., and Flocks, J., 1966, Some acoustic properties of the ringing rocks diabase, Kintersville, Pennsylvania (abs.): Pennsylvania Academy of Science Proceedings, v. 40, no. 1, p. 12

Sanderson, Ivan T., "Things": Pyramid Books, New York, 1967

Stroud, A.E., 2008, Ringing Rock Boulder Fields in SE Pennsylvania; Phactum 10/2008, pp. 10-11

Wherry, E. T., 1912, Apparent Sun-Crack Structures and Ringing-rock Phenomena in the Triassic Diabase of Eastern Pennsylvania; Proceedings of the Academy of Natural Science, Philadelphia, pp. 169-172

There have been numerous non-technical travel articles published on the internet for several of the Pennsylvania ringing rock sites. Many of these articles provide audio and video clips which provide good views of the boulder fields and examples of the sounds that are given off by the individual boulders.

External links