Sailing stones

A sailing stone in Racetrack Playa.

Sailing stones, sliding rocks, and moving rocks all refer to a geological phenomenon where rocks move and inscribe long tracks along a smooth valley floor without human or animal intervention. Tracks from these sliding rocks have been observed and studied in various locations, including Little Bonnie Claire Playa in Nevada, and most notably Racetrack Playa, Death Valley National Park, California where the number and length of tracks are notable. At Racetrack Playa, these tracks have been studied since the early 1900s, yet the origins of stone movement are not confirmed and remain the subject of research for which several hypotheses exist.

The stones move only every two or three years and most tracks develop over three or four years. Stones with rough bottoms leave straight striated tracks while those with smooth bottoms tend to wander. Stones sometimes turn over, exposing another edge to the ground and leaving a different track in the stone's wake.

Trails differ in both direction and length. Rocks that start next to each other may travel parallel for a time, before one abruptly changes direction to the left, right, or even back to the direction from which it came. Trail length also varies – two similarly sized and shaped rocks may travel uniformly, then one could move ahead or stop in its track.

Description

Tracks are sometimes non-linear.

The Racetrack’s stones speckle the playa floor, predominately in the southern portion. Historical accounts identify some stones hundreds of feet from shore, yet most of the stones are found relatively close to their respective originating outcrops. Three lithologic types are identified: (1) syenite, found most abundant on the west side of the playa; (2) dolomite, subrounded blue-gray stones with white bands; and (3) black dolomite, the most common type, found almost always in angular joint blocks or slivers. This dolomite composes nearly all stones found in the southern half of the playa, and originates at a steep promontory, 850 ft-high (260 m), paralleling the east shore at the south end of the playa. Intrusive igneous rock originates from adjacent slopes (most of those being tan-colored feldspar-rich syenite). Tracks are often tens to hundreds of feet long, about 3 to 12 inches (8 to 30 cm) wide, and typically much less than an inch (2.54 cm) deep. Most moving stones range from about six to 18 inches in diameter.

A balance of very specific conditions is thought to be needed for stones to move:

• a saturated yet non-flooded surface
• a thin layer of clay
• very strong gusts as initiating force
• strong sustained wind to keep stones going

And in some hypotheses:

• ice floes

Research history

Two rocks in Racetrack Playa.

Early investigation

The first documented account of the sliding rock phenomenon dates to 1915, when a prospector named Joseph Crook from Fallon, Nevada visited the Racetrack Playa site. In the following years, the Racetrack sparked interest from geologists Jim McAllister and Allen Agnew, who mapped the bedrock of the area in 1948 and published the earliest report about the sliding rocks in a Geologic Society of America Bulletin. Their publication gave a brief description of the playa furrows and scrapers, stating that no exact measurements had been taken and suggesting that furrows were the remnants of scrapers propelled by strong gusts of wind – such as the variable winds that produce dust–devils – over a muddy playa floor. Controversy over the origin of the furrows prompted the search for the occurrence of same phenomenon at other locations. Such a location was found at Little Bonnie Claire Playa in Nye County, Nevada, and the phenomenon was studied there as well.

Naturalists from the National Park Service later wrote more detailed descriptions and Life magazine featured a set of photographs from the Racetrack. In 1952, a National Park Service Ranger named Louis G. Kirk recorded detailed observations of furrow length, width, and general course. He sought simply to investigate and record evidence of the moving rock phenomenon, not to hypothesize or create an extensive scientific report. Speculation about how the stones move started at this time. Various and sometimes idiosyncratic possible explanations have been put forward over the years that have ranged from the supernatural to the very complex. Most hypotheses favored by interested geologists posit that strong winds when the mud is wet are at least in part responsible. Some stones weigh as much as a human, which some researchers, such as geologist George M. Stanley, who published a paper on the topic in 1955, feel is too heavy for the area's wind to move. After extensive track mapping and research on rotation of the tracks in relation to ice floe rotation, Stanley maintained that ice sheets around the stones either help to catch the wind or that ice floes initiate rock movement.

Progress in the 1970s

Bob Sharp and Dwight Carey started a Racetrack stone movement monitoring program in May 1972. Eventually thirty stones with fresh tracks were labeled and stakes were used to mark their locations. Each stone was given a name and changes in the stones' position were recorded over a seven-year period. Sharp and Carey also tested the ice floe hypothesis by corralling selected stones. A corral 5.5 feet (1.7 m) in diameter was made around a 3 inches (7.6 cm) wide, 1 pound (0.45 kg) track-making stone with seven rebar segments placed 25 to 30 inches (64 to 76 cm) apart. If a sheet of ice around the stones either increased wind-catching surface area or helped move the stones by dragging them along in ice floes, then the rebar should at least slow down and deflect the movement. Neither appeared to occur; the stone barely missed a rebar as it moved 28 feet (8.5 m) to the northwest out of the corral in the first winter. Two heavier stones were placed in the corral at the same time; one moved five years later in the same direction as the first but its companion did not move during the study period. This indicated that if ice played a part in stone movement, then ice collars around stones must be small.

A panorama of the Milky Way with the tracks of sailing stones below. Notice the stone on the right side.

Ten of the initial twenty-five stones moved in the first winter with Mary Ann (stone A) covering the longest distance at 212 feet (65 m). Two of the next six monitored winters also saw multiple stones move. No stones were confirmed to have moved in the summer and some winters none or only a few stones moved. In the end all but two of the thirty monitored stones moved during the seven-year study. At 2.5 inches (6.4 cm) in diameter, Nancy (stone H) was the smallest monitored stone. It also moved the longest cumulative distance, 860 feet (260 m), and the greatest single winter movement, 659 feet (201 m). The largest stone to move was 80 pounds (36 kg).

Karen (stone J) is a Template:Convert/3 block of dolomite and weighs an estimated 700 pounds (318 kg). Karen did not move during the monitoring period. The stone may have created its 570 feet (170 m) long straight and old track from momentum gained from its initial fall onto the wet playa. However, Karen disappeared sometime before May 1994, possibly during the unusually wet winter of 1992 to 1993. Removal by artificial means is considered unlikely due to the lack of associated damage to the playa that a truck and winch would have caused. A possible sighting of Karen was made in 1994 a half mile (800 m) from the playa. Karen was rediscovered by San Jose geologist Paula Messina in 1996.

Continued research in the 1990s

Professor John Reid led six research students from Hampshire College and the University of Massachusetts Amherst in a follow-up study in 1995. They found highly congruent trails from stones that moved in the late 1980s and during the winter of 1992-1993. At least some stones were proved beyond a reasonable doubt to have been moved in ice floes that may be up to half a mile (800 m) wide. Physical evidence included swaths of lineated areas that could only have been created by moving thin sheets of ice. Consequently, both wind alone and wind in conjunction with ice floes are thought to be motive forces.

Another sailing stone in Racetrack Playa.

Physicists Bacon et al. studying the phenomenon in 1996, informed by studies in Owens Dry Lake Playa, discovered that winds blowing on playa surfaces can be compressed and intensified because of a playa's smooth, flat surfaces. They also found that boundary layers (the region just above ground where winds are slower due to ground drag) on these surfaces can be as low as 2 inches (5.1 cm). As a result, stones just a few inches high feel the full force of ambient winds and their gusts, which can reach 90 miles per hour (140 km/h) in winter storms. Such gusts are thought to be the initiating force while momentum and sustained winds keep the stones moving, possibly as fast as a moderate run (only half the force required to start a stone sailing is needed to keep it in motion).

Wind and ice both are the favored hypothesis for these sliding rocks. Noted in "Surface Processes and Landforms", Don J. Easterbrook mentions that because of the lack of parallel paths between some rock paths, this could be caused by degenerating ice floes resulting in alternate routes. Even though the ice breaks up into smaller blocks, it is still necessary for the rocks to slide.

Recent developments

Further understanding of the geologic processes at work in Racetrack Playa goes hand in hand with technological development. In 2009, development of inexpensive time-lapse digital cameras allowed the capturing of transient meteorological phenomena including dust devils and playa flooding. These cameras were aimed at capturing various stages of the previously mentioned phenomena, though discussion of the sliding stones ensued. The developers of photographic technology describe the difficulty of capturing the Racetrack’s stealthy rocks, as movements only occur about once every three years and last approximately ten seconds. Their next identified advancement is wind-triggered imagery, vastly reducing the ten million seconds of non-transit time they must sift through.

In a study published in 2011 it is postulated that small rafts of ice form around the rocks and the rocks are buoyantly floated off the soft bed thus reducing the reaction and friction forces at the bed. Since this effect depends on reducing friction, and not on increasing the wind drag, these ice cakes need not have a particularly large surface area if the ice is adequately thick, as the minimal friction allows the rocks to be moved by arbitrarily light winds.

Research development published in 2013 pointed out narrowing trails, occurrence of intermittent spring systems, and absence of rocks at the end of the trails. They identified the Racetrack mountain area that drains water towards the Racetrack playa while ice covered the intermittent lake. They suggest that it is this water that lifts the icebergs with rocks allowing for the caligraphy. Study also provides mapping and analysis of the effect of artificial ditch preventing the visitors from driving on the playa and they claim that it may interfere with the sliding rock phenomenon.

Explanation

Ralph Lorenz, a NASA scientist, investigated the phenomenon in 2006. Lorenz developed an experiment using a kitchen-table model. Using a Tupperware container to show how heavy rocks might glide across the surface of the lake bed. A bed of sand is added to the bottom of the tupperware. A rock is placed on the sand, water was added until there is only a small edge of the rock sticking out. After putting the container in the freezer and letting it melt, Lorenz could end up with a small slab of floating ice with a rock embedded in it. All he had to do was gently blow on the floating ice sheet to get the rock to drag across the sand. Gunther Kletetschka with his NASA's academy students showed the process of lifting small stone in a thin aquarium and captured the lifting process with camera.

• 
  Illustration of the lifting mechanism of the rocks at the Racetracks Playa.

Theft of rocks

On 30 May 2013, the LA Times reported that park officials are looking in to the theft of several of the rocks.

See also

• Rocking stone

References

• Messina, P., 1998, The Sliding Rocks of Racetrack Playa, Death Valley National Park, California: Physical and Spatial Influences on Surface Processes. Published doctoral dissertation, Department of Earth and Environmental Sciences, City University of New York, New York. University Microfilms, Incorporated, 1998.
• Messina, P., Stoffer, P., and Clarke, K. C. Mapping Death Valley's Wandering Rocks. GPS World April, 1997: p. 34-44
• Sharp, R.P., and A.F. Glazier, 1997, Geology Underfoot in Death Valley and Owens Valley. Mountain Press Publishing Company, Missoula. ISBN 0-87842-362-1
• Stanley, G. M., 1955, Origin of playa stone tracks, Racetrack Playa, Inyo County, California. Geological Society of America Bulletin, v. 66, p. 1329-1350.
• Reid, J.B., Jr., Bucklin, E.P., Copenagle, L., Kidder, J., Pack, S. M., Polissar, P.J., and Williams, M. L., 1995, Sliding rocks at the Racetrack, Death Valley: What makes them move?. Geology v. 23, p. 819-822
• Sharp, R.P., Carey, D. L., Reid, J.B., Jr., Polissar, P.J., and Williams, M.L., 1996, Sliding rocks at the Racetrack, Death Valley: What makes them move?; Discussion and Reply. Geology, v. 25, p. 766-767

External links

• The Sliding Rocks of Racetrack Playa by Paula Messina
• The Mystery of the Rocks on the Racetrack at Death Valley by Lena Fletcher and Anne Nester
• http://www.physicsforums.com/showthread.php?p=437132
• Moving Rocks of Death Valley's Racetrack Playa by Brian Dunning
• Why Are Death Valley's Rocks Moving Themselves? by Philip Schewe (FoxNews)
• How Do Death Valley’s “Sailing Stones” Move Themselves Across the Desert? Smithsonian Magazine, June 2013