YARDANGS OF THE LUT DESERT
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| Plate E-19 |
Map |
The Lut Basin in southeastern Iran contains several
ancient interior drainage systems separated by low ridges
and residual mountains. Selivanov (1982) describes the
recent paleoclimatology as alternations of wet and dry
periods. He contends that these alternations, coupled with
tectonic compression of the basin fill sediments into scarcely
perceptible folds, resulted in unusual types of relief being
formed during the second half of the Quaternary.
The yardangs up to 80 m high of the western Lut Desert,
in the center of this Plate, are among the largest yardangs on
Earth. They are carved out of the Lut Formation, a fine-
grained horizontally bedded silty clay and limy gypsiferous
sands with an estimated thickness of 135 to 200 m. Salt,
gypsum, and silty clay encrust the unit (Krinsley, 1970).
These yardangs were described by Gabriel (1938) as
deposits from Lut Lake that resemble desert cities separated
by "boulevards." He notes that no erosion
channels on the ground and no evidence of water erosion are
found and that "the surface of the land had been formed
merely by the wind" (p. 198).
The yardangs trend north-northwest, parallel
to the prevailing winds, and are separated by 100 m or
more of troughs. According to McCauley et al.
(1977), the surfaces of the yardangs are covered by a
layer of gypsiferous clay 10 to 15 cm thick. This clay
layer swells when wet and prevents rainwash from
penetrating the pronounced running-water-
eroded gullies on the flanks of the yardangs.
As shown in
Figure E-19.1 and
Figure E-19.2, oblique aerial photographs, only the broadest
yardangs have flat or rounded summits. In the other yardangs, the
ridges are narrow. Most of the yardangs in the foreground of Figure
E-19.2 have similar widths.
Figure E-19.3, a vertical aerial photograph of 10 km of the Lut
yardangs, shows some of the relief on top of the yardangs. The
spacing between many of the yardangs appears to be regular. On some
of the yardangs, the horizontal bedding of the Lut Formation may be
seen on the gullies.
Note the small, scattered crescentic dunes on the troughs
to the right of and behind the front central yardang in Figure
E-19.2. The orientation of the dunes parallels the orientation
of the yardangs, which suggests that the wind was coming
from the direction of the foreground of this photograph. The
salt stains in the furrows on the front yardang at the far left in
this figure indicate that the floor of the yardang area has been .
This is mentioned by Dresch (1968), who notes that the base
of the convex ridge slope makes a steep angle with the floor due
to erosion from periodic floodwaters. The waters from the north
penetrate the furrows and sap the base of the slopes to a height
of 1 to 2 m.
As noted in the index map, the yardangs are bounded on
the west by alluvium from the Kerman Mountains. Thrust faults
and fractures cut through the Mesozoic sedimentary rocks in
this range. The plateau of the Lut Formation bounds the field
on the north and east. Buttes and small yardangs north of the
field are separated from the Lut Formation by a scarp. Salt playas
locally surround the yardang area. Their boundaries are actually
mobile zones that shift with each flooding (Krinsley, 1970). The
elongated salt-crusted playa southeast of Shahdad, in the
left center of the Plate, is flooded periodically.
A few star dunes are found east of the yardang field. Star
dunes are believed to form in areas where effective winds blow
from several directions. Therefore, evidence exists for two wind
regimes, an early strong NNW-SSE regime that created the
yardangs, followed by a more recent multidirectional wind regime
that created the star dunes. The relief of the yardangs probably
controls the wind regime among the yardangs to create crescentic
dunes, although star dunes exist above the yardang field. Southeast
of the Lut Desert, yardangs are sand ridges that Krinsley (1970)
believes are derived from materials excavated from the furrows
between the yardangs. The sand ridges terminate in a sand sea in
eastern Lut Desert, which can be seen on Plate E-20. Landsat
2592-05510-7, September 5, 1976.
Continue to Plate E-20 |
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