Racetrack Playa

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Racetrack Playa
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Racetrack Playa
Location Death Valley National Park
Inyo County, California
Coordinates 36°40′53″N117°33′46″W / 36.6813°N 117.5627°W / 36.6813; -117.5627
Lake type Endorheic basin
Primary outflows Terminal (evaporation)
Basin  countries United States
Max. length4.5 km (2.8 mi)
Max. width2 km (1.2 mi)
Surface area 7 km2 (2.7 sq mi)
Shore length112 km (7.5 mi)
Surface elevation1,132 m (3,714 ft)
References U.S. Geological Survey Geographic Names Information System: The Racetrack
1 Shore length is not a well-defined measure.

The Racetrack Playa, or The Racetrack, is a scenic dry lake feature with "sailing stones" that inscribe linear "racetrack" imprints. It is located above the northwestern side of Death Valley, in Death Valley National Park, Inyo County, California, U.S.

Contents

Geography

Racetrack playa is approximately 3 miles long and 1.2 miles wide and is located at a height of 3708 feet in a north-south valley east of the Panamint Range within Death Valley National Park. It receives only 3 inches of annual precipitation and is bounded on all sides by north-south ranges rising 1500 to 2000 feet. The overall drainage area is around 70 square miles, with most of it flowing onto the playa from eastern mountain rivers. [1]

The surface of the playa, which is mainly dried clay, provides a hard, smooth, and level pavement. The distribution of stones varies, with some regions a few hundred feet from the shore having 5-10 tiny stones per square yard. There is evidence of downgrade transit in a few places. [1]

Rocks weighing up to 320 kg travel across Racetrack Playa in northern Death Valley National Park, California, leaving tracks. This phenomenon, which has been documented since 1948, is not unique and has been observed in various playas in southern California, the Tunisian Sahara, and South Africa. [2]

Traditionally, these rocks were considered to be pushed by wind over a wet and slippery playa surface. Recent observations from 2014 called this assumption into question. Norris et al. observed pebbles being transported as thin sheets of ice melted in 4-5 m/s winds. The ice panels moved several rocks at speeds of up to 80 mm/s. [2]

While these discoveries give information on the physics, several aspects of the tracks remain a mystery. Kletetschka et al. proposed that when an ice sheet arises, rocks with better thermal conductivity than water or ice could become frozen to the rock's base. This permits the ice sheet to be moved together with the rock and silt by the wind. [2]

A thorough system was put up for the investigation of Racetrack Playa's rock movement, including a weather station near the playa, time-lapse cameras centered on the southeast corner, and 15 GPS-equipped boulders on the surface. The researchers went to the location for maintenance and data retrieval 5-8 times per year. From November to March each year, the time-lapse camera recorded hourly conditions. [3]

Interwoof GPS loggers were installed in limestone blocks northeast of natural stones and captured GPS and temperature data every 60 minutes. They began recording constantly at one-second intervals after being triggered. [3]

The Racetrack Playa is 3,714 feet (1,132 m) above sea level, and 2.8 mi (4.5 km) long (north-south) by 1.3 mi (2.1 km) wide (east-west). The playa is exceptionally flat and level with the northern end being only 1.5 inches (3.8 cm) higher than the southern. This occurrence is due to major influx of fine-grained sediment that accumulates at the north end. The highest point surrounding the Racetrack is the 5,678-foot (1,731 m) high Ubehebe Peak, rising 1,964 feet (599 m) above the lakebed 0.85 miles (1.37 km) to the west.[ citation needed ]

The playa is in the small Racetrack Valley endorheic basin between the Cottonwood Mountains on the east and Nelson Range to the west. During periods of heavy rain, water washes down from the surrounding mountains [4] draining into the playa, forming a shallow, short-lived endorheic lake. Under the hot desert sun, the thin veneer of water quickly evaporates leaving behind a surface layer of soft slick mud. As the mud dries, it shrinks and cracks into a mosaic pattern of interlocking polygons.[ citation needed ]

The shape of the shallow hydrocarbon lake Ontario Lacus on Saturn's moon Titan has been compared to that of Racetrack Playa. [5]

Deathvalleysky nps big.jpg
360° night-time panorama of the Racetrack Playa. The Milky Way is the visible arc in the center above a sailing stone and tracks from others.

Features

Racetrack is dry for almost the entire year and has no vegetation. When dry, its surface is covered with small but firm hexagonal mud crack polygons that are typically 3 to 4 inches (7.5 to 10 cm) in diameter and about an inch (2.5 cm) thick. The polygons form in sets of three mud cracks at 120° to each other. [6] A few days after a precipitation event, small mud curls, otherwise known as "corn flakes" form on the playa surface. Absence of these indicates that wind or another object has scraped away the tiny mud curls.

Sailing stone in Racetrack Playa Runningrock2.jpg
Sailing stone in Racetrack Playa

During the bimodal rainy season (summer and especially winter) a shallow cover of water deposits a thin layer of fine mud on and between the polygons of Racetrack. Heavier winter precipitation temporarily erases them until spring when the dry conditions cause new mud cracks to form in the place of the old cracks. Sandblasting wind continually helps to round the edges of exposed polygons. Annual precipitation is 3 to 4 inches (75 to 100 mm) and ice cover can be 1 to 2.5 inches (2.5 to 6.5 cm) thick. Typically only part of the playa will flood in any given year.

The Racetrack was vandalised in late 2016. [7]

A portion of the playa's shoreline indicates ice activity, notably on the east side of the southernmost arm. A pavement of angular rock fragments and periodic alignments of bigger stones reveal little ice ramparts. Stone traces and ridges near the shore suggest ice thrusting and shearing. [1]

Despite its thin grain, the pavement has closely matched parts that provide a mosaic-like effect. The pavement is lined with faint stone footprints, mostly to the northeast. Although modest, ice ramparts rise a few inches above the chip pavement. Ice along the beach seemed to be thrusting and shearing, with stones periodically scouring windows in the pavement. [1]

Racetrack Playa's distinctive traits, including its low precipitation, large clay surface, and indications of ice action along the shore, add to its remarkable natural landscape. [1]

Mapping

Detailed plots were made by nailing numbered tabs of tracing fabric to the clay along specific paths. Baselines, aligned by alidade beside paths, marked stations at 25 or 50-foot intervals. Distances were measured to the closest 0.005 feet using a 100-foot tape. Trigonometric computations were used to precisely connect the basis lines. [1]

Rock mobility was associated with clear days following sub-freezing nights, which were caused by light breezes and the morning sun breaking up floating ice. Rocks were moved by ice disintegration, with over 60 moving in a single occurrence. Ice frequently fractured near rocks, causing wakes downstream. Some rocks went ahead of others, covering varied lengths. Ice fractures altered neighboring rocks, even those that were close together. The presence of a playa pool with precise depth parameters was a critical requirement for rock motion. [3]

Other elements included floating ice, appropriate temperatures, sunlight, and mild winds, which were most common around midday when the ice melted. Because of their origin beneath the ice, the formation of rock trails was difficult to detect. The rocks moved slowly, lasting up to 16 minutes at speeds ranging from 2 to 5 meters per minute. During the coldest weeks, weather station data revealed freezing temperatures and winds of up to 3-5 m/s. Episodic rock motion, which can last for years or decades, has been related to occasional rain or snow episodes that build winter ponds. [3]

Sailing stones

The sailing stones are a geological phenomenon found in the Racetrack. Slabs of dolomite and syenite ranging from a few hundred grams (few ounces) to hundreds of kilograms (pounds) inscribe visible tracks as they slide across the playa surface, without human or animal intervention. Instead, rocks move when ice sheets just a few millimeters thick [8] start to melt during periods of light wind. These thin floating ice panels create an ice shove that moves the rocks at up to five meters (16') per minute. [3]

The 2017 documentary Principles of Curiosity explores as its central theme the story of how the sailing stones' movement had been a mystery which came to be solved using the scientific method and critical thinking. [9]

Islands

The Grandstand in the northwest area of the playa Death Valley NP - Racetrack Playa - Grandstand.JPG
The Grandstand in the northwest area of the playa

Two islands of bedrock outcrops rise dramatically above the playa's surface at its northern end. The larger landmark is The Grandstand, a 73-foot (22 m) high dark quartz monzonite outcrop, rising in dramatic contrast from the bright white surface of the Racetrack. The second 'island' feature is a smaller carbonate outcrop.

Springs

Depressions in the Racetrack playa are intermittent springs that are active at time of precipitation. Detailed view illustrate conical holes where the water comes out on the surface when this area receive excess of precipitation. Gindarja Springs.jpg
Depressions in the Racetrack playa are intermittent springs that are active at time of precipitation. Detailed view illustrate conical holes where the water comes out on the surface when this area receive excess of precipitation.

There are three areas of aligned depressions (intermittent springs) in the playa.

Spinal Springs is in the central part of the Racetrack playa. It is 550 metres (600 yards) long and starts, at its northern end, with conical depressions only a few centimeters (inches) deep. Traced southward the depressions increase to ~5 metres (16') in width with scattered creosote shrubs. They then narrow and become shallower again, and finally disappear. Further north and south along this linear formation, there were several other depressions that may be a continuation of the Spinal Springs alignment. [4]

Edge Springs is an alignment of the depressions along the southeastern edge of the Racetrack playa. The alignment parallels the toes of alluvial fans along the base of the steep mountain range. [4]

Gindarja Springs is an alignment of depressions that consists of three large indentations aligned in a northwesterly direction within the Racetrack playa. Two are completely within the playa and the third is on the edge. All three are associated with significant vegetation. [4]

Visiting

Access is via Racetrack Road, reached at the Grapevine Junction near Scotty's Castle. The 28 mile rough gravel road heading south-west from Ubehebe Crater is passable with non-4WD vehicles but requires high ground clearance. It rounds the western side of the playa to a parking area with descriptive signs by the National Park Service. A bench here, placed by the Mano Seca Group, has scenic views of The Racetrack, The Grandstand, and mountain scenery. Another access to Racetrack Playa is Lippincott pass road that enters the Racetrack valley from the south west, climbing up from Saline Valley. Lippincott Pass and the roads in Saline Valley are extremely rough and negotiable for high clearance 4WD vehicles with all-terrain tires only.

Camping, while not allowed on the playa, is available in "primitive campsite" areas to the north and south. Visiting remote areas of Death Valley National Park bears considerable risk. Summer temperatures can surpass 120 °F (49 °C) in certain spots, large areas are without cellphone reception, roads are treacherous and the closest gas station is in Panamint Springs.

An observation from the early 1970s calls the current thinking[ as of? ] into question. During April or May 1972 or 1973, rocks up to 0.25 m in length were spotted moving purely owing to high winds on the wet playa surface. This calls into question the notion that strong winds and a water-slickened playa surface were both required for boulder movement on Racetrack Playa. [10]

While recent observations have indicated movement by wind alone and by wind operating on small sheets of ice, many features of the phenomena, particularly those involving bigger ice sheets, still require additional investigation. [10]

See also

Related Research Articles

<span class="mw-page-title-main">Geomorphology</span> Scientific study of landforms

Geomorphology is the scientific study of the origin and evolution of topographic and bathymetric features generated by physical, chemical or biological processes operating at or near Earth's surface. Geomorphologists seek to understand why landscapes look the way they do, to understand landform and terrain history and dynamics and to predict changes through a combination of field observations, physical experiments and numerical modeling. Geomorphologists work within disciplines such as physical geography, geology, geodesy, engineering geology, archaeology, climatology, and geotechnical engineering. This broad base of interests contributes to many research styles and interests within the field.

<span class="mw-page-title-main">Dry lake</span> Basin or depression that formerly contained a standing surface water body

A dry lake bed, also known as a playa, is a basin or depression that formerly contained a standing surface water body, which disappears when evaporation processes exceed recharge. If the floor of a dry lake is covered by deposits of alkaline compounds, it is known as an alkali flat. If covered with salt, it is known as a salt flat.

<span class="mw-page-title-main">Transverse Ranges</span> Group of mountain ranges of southern California

The Transverse Ranges are a group of mountain ranges of southern California, in the Pacific Coast Ranges physiographic region in North America. The Transverse Ranges begin at the southern end of the California Coast Ranges and lie within Santa Barbara, Ventura, Los Angeles, San Bernardino, Riverside and Kern counties. The Peninsular Ranges lie to the south. The name Transverse Ranges is due to their east–west orientation, making them transverse to the general northwest–southeast orientation of most of California's coastal mountains.

<span class="mw-page-title-main">Aeolian processes</span> Processes due to wind activity

Aeolian processes, also spelled eolian, pertain to wind activity in the study of geology and weather and specifically to the wind's ability to shape the surface of the Earth. Winds may erode, transport, and deposit materials and are effective agents in regions with sparse vegetation, a lack of soil moisture and a large supply of unconsolidated sediments. Although water is a much more powerful eroding force than wind, aeolian processes are important in arid environments such as deserts.

<span class="mw-page-title-main">Glacial erratic</span> Piece of rock that has been moved by a glacier

A glacial erratic is a glacially deposited rock differing from the type of rock native to the area in which it rests. Erratics, which take their name from the Latin word errare, are carried by glacial ice, often over distances of hundreds of kilometres. Erratics can range in size from pebbles to large boulders such as Big Rock in Alberta.

<span class="mw-page-title-main">Geology of the Death Valley area</span> Geology of the area in California and Nevada

The exposed geology of the Death Valley area presents a diverse and complex set of at least 23 formations of sedimentary units, two major gaps in the geologic record called unconformities, and at least one distinct set of related formations geologists call a group. The oldest rocks in the area that now includes Death Valley National Park are extensively metamorphosed by intense heat and pressure and are at least 1700 million years old. These rocks were intruded by a mass of granite 1400 Ma and later uplifted and exposed to nearly 500 million years of erosion.

<span class="mw-page-title-main">Places of interest in the Death Valley area</span>

Places of interest in the Death Valley area are mostly located within Death Valley National Park in eastern California.

<span class="mw-page-title-main">Desert pavement</span> Type of desert earth surface

A desert pavement, also called reg, serir, gibber, or saï is a desert surface covered with closely packed, interlocking angular or rounded rock fragments of pebble and cobble size. They typically top alluvial fans. Desert varnish collects on the exposed surface rocks over time.

<span class="mw-page-title-main">Plucking (glaciation)</span> Glacial erosion of bedrock

Plucking, also referred to as quarrying, is a glacial phenomenon that is responsible for the weathering and erosion of pieces of bedrock, especially large "joint blocks". This occurs in a type of glacier called a "valley glacier". As a glacier moves down a valley, friction causes the basal ice of the glacier to melt and infiltrate joints (cracks) in the bedrock. The freezing and thawing action of the ice enlarges, widens, or causes further cracks in the bedrock as it changes volume across the ice/water phase transition, gradually loosening the rock between the joints. This produces large pieces of rock called joint blocks. Eventually these joint blocks come loose and become trapped in the glacier.

<span class="mw-page-title-main">Exfoliation joint</span> Type of weathering joint

Exfoliation joints or sheet joints are surface-parallel fracture systems in rock, and often leading to erosion of concentric slabs. (See Joint ).

<span class="mw-page-title-main">Outwash fan</span> Type of sediment deposition by a melting glacier

An outwash fan is a fan-shaped body of sediments deposited by braided streams from a melting glacier. Sediment locked within the ice of the glacier gets transported by the streams of meltwater, and deposits on the outwash plain, at the terminus of the glacier. The outwash, the sediment transported and deposited by the meltwater and that makes up the fan, is usually poorly sorted due to the short distance traveled before being deposited.

<span class="mw-page-title-main">Sailing stones</span> Geological phenomenon where rocks move, leaving tracks

Sailing stones are part of the geological phenomenon in which rocks move and inscribe long tracks along a smooth valley floor without animal intervention. The movement of the rocks occurs when large, thin sheets of ice floating on an ephemeral winter pond break up in the sun. Trails of sliding rocks have been observed and studied in various locations, including Little Bonnie Claire Playa, in Nevada, and most famously at Racetrack Playa, Death Valley National Park, California, where the number and length of tracks are notable.

<span class="mw-page-title-main">Abrasion (geology)</span> Process of erosion

Abrasion is a process of erosion which occurs when material being transported wears away at a surface over time. It is the process of friction caused by scuffing, scratching, wearing down, marring, and rubbing away of materials. The intensity of abrasion depends on the hardness, concentration, velocity and mass of the moving particles. Abrasion generally occurs in four ways: glaciation slowly grinds rocks picked up by ice against rock surfaces; solid objects transported in river channels make abrasive surface contact with the bed and walls; objects transported in waves breaking on coastlines; and by wind transporting sand or small stones against surface rocks.

Hydrothermal explosions occur when superheated water trapped below the surface of the Earth rapidly converts from liquid to steam, violently disrupting the confining rock. Boiling water, steam, mud, and rock fragments are ejected over an area of a few meters up to several kilometers in diameter. Although the energy originally comes from a deep igneous source, this energy is transferred to the surface by circulating meteoric water or mixtures of meteoric and magmatic water rather than by magma, as occurs in volcanic eruptions. The energy is stored as heat in hot water and rock within a few hundred feet of the surface.

<span class="mw-page-title-main">Ice lens</span> Ice within soil or rock

Ice lenses are bodies of ice formed when moisture, diffused within soil or rock, accumulates in a localized zone. The ice initially accumulates within small collocated pores or pre-existing crack, and, as long as the conditions remain favorable, continues to collect in the ice layer or ice lens, wedging the soil or rock apart. Ice lenses grow parallel to the surface and several centimeters to several decimeters deep in the soil or rock. Studies from 1990 have demonstrated that rock fracture by ice segregation is a more effective weathering process than the freeze-thaw process which older texts proposed.

The Grandstand is a natural rock monolith located near the northerly end of Racetrack Playa, north of Death Valley in the Cottonwood Mountains of Death Valley National Park, in Inyo County, California.

<span class="mw-page-title-main">Ice segregation</span> Geological phenomenon

Ice segregation is the geological phenomenon produced by the formation of ice lenses, which induce erosion when moisture, diffused within soil or rock, accumulates in a localized zone. The ice initially accumulates within small collocated pores or pre-existing cracks, and, as long as the conditions remain favorable, continues to collect in the ice layer or ice lens, wedging the soil or rock apart. Ice lenses grow parallel to the surface and several centimeters to several decimeters deep in the soil or rock. Studies between 1990 and present have demonstrated that rock fracture by ice segregation is a more effective weathering process than the freeze-thaw process which older texts proposed.

In geology, the term exhumation refers to the process by which a parcel of rock, approaches Earth's surface.

<span class="mw-page-title-main">Lake Manly</span> Lake in Death Valley, California, United States

Lake Manly was a pluvial lake in Death Valley, California, covering much of Death Valley with a surface area of 1,600 square kilometres (620 sq mi) during the so-called "Blackwelder stand". Water levels varied through its history, and the chronology is further complicated by active tectonic processes that have modified the elevations of the various shorelines of Lake Manly; during the Blackwelder stage they reached 47–90 metres (154–295 ft) above sea level. The lake received water mainly from the Amargosa River and at various points from the Mojave River and Owens River. The lake and its substantial catchment favoured the spread of a number of aquatic species, including some lizards, pupfish and springsnails. The lake probably supported a substantial ecosystem, and a number of diatoms developed there.

<span class="mw-page-title-main">Lake Panamint</span>

Lake Panamint is a former lake that occupied Panamint Valley in California during the Pleistocene. It was formed mainly by water overflowing through the Owens River and which passed through Lake Searles into the Panamint Valley. At times, Lake Panamint itself overflowed into Death Valley and Lake Manly.

References

  1. 1 2 3 4 5 6 7 Stanley, George M. (1955). "Origin of Playa Stone Tracks, Racetrack Playa, Inyo County, California". Geological Society of America Bulletin. 66 (11): 1329. Bibcode:1955GSAB...66.1329S. doi:10.1130/0016-7606(1955)66[1329:OOPSTR]2.0.CO;2. ISSN   0016-7606.
  2. 1 2 3 Jones, Ronald; Hooke, Roger LeB. (2015). "Racetrack Playa: Rocks moved by wind alone". Aeolian Research. 19: 1–3. Bibcode:2015AeoRe..19....1J. doi:10.1016/j.aeolia.2015.08.001.
  3. 1 2 3 4 5 6 Norris, Richard D.; Norris, James M.; Lorenz, Ralph D.; Ray, Jib; Jackson, Brian (2014). "Sliding Rocks on Racetrack Playa, Death Valley National Park: First Observation of Rocks in Motion". PLOS ONE. 9 (8): e105948. Bibcode:2014PLoSO...9j5948N. doi: 10.1371/journal.pone.0105948 . PMC   4146553 . PMID   25162535.
  4. 1 2 3 4 Kletetschka, Gunther; Hooke, Roger LeB.; Ryan, Andrew; Fercana, George; McKinney, Emerald; Schwebler, Kristopher P. (2013). "Sliding stones of Racetrack Playa, Death Valley, USA: The roles of rock thermal conductivity and fluctuating water levels". Geomorphology. 195: 110–117. Bibcode:2013Geomo.195..110K. doi:10.1016/j.geomorph.2013.04.032.
  5. Lorenz, R. D., B. Jackson and A. Hayes, "Racetrack and Bonnie Claire : Southwestern US Playa Lakes as Analogs for Ontario Lacus, Titan", Planetary and Space Science, 58, 723–31, 2010
  6. Sharp, Robert P. and Allen F. Glazner, Geology Underfoot In Death Valley and Owens Valley, 161–73, 1997
  7. Sahagun, Louis (27 September 2016). "Investigators think they know who tore up Death Valley's fragile Racetrack Playa in an SUV". Los Angeles Times .
  8. Lorenz, Ralph; Norris, J.; Jackson, B.; Norris, R.; Chadbourne, J.; Ray, J. (June 2014). "Trail formation by ice-shoved "sailing stones" observed at Racetrack Playa, Death Valley National Park" (PDF). Earth Surface Dynamics Discussions. Copernicus. 2 (2): 110–17. Bibcode:2014ESuDD...2.1005L. doi: 10.5194/esurfd-2-1005-2014 .
  9. Gerbic, Susan (2017-07-26). "Principles of Curiosity Review - CSI". www.csicop.org. Archived from the original on 2017-07-26. Retrieved 2017-10-28.
  10. 1 2 3 Jones, Ronald; Hooke, Roger LeB. (2015). "Racetrack Playa: Rocks moved by wind alone". Aeolian Research. 19: 1–3. Bibcode:2015AeoRe..19....1J. doi:10.1016/j.aeolia.2015.08.001.