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Tracing the Vedic Saraswati River in the Great Rann of Kachchh

  • Scientific Reports 7, Article number: 5476 (2017)
  • doi:10.1038/s41598-017-05745-8
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The lost Saraswati River mentioned in the ancient Indian tradition is postulated to have flown independently of the Indus River into the Arabian Sea, perhaps along courses of now defunct rivers such as Ghaggar, Hakra and Nara. The persistence of such a river during the Harappan Bronze Age and the Iron Age Vedic period is strongly debated. We drilled in the Great Rann of Kachchh (Kutch), an infilled gulf of the Arabian Sea, which must have received input from the Saraswati, if active. Nd and Sr isotopic measurements suggest that a distinct source may have been present before 10 ka. Later in Holocene, under a drying climate, sediments from the Thar Desert probably choked the signature of an independent Saraswati-like river. Alternatively, without excluding a Saraswati-like secondary source, the Indus and the Thar were the dominant sources throughout the post-glacial history of the GRK. Indus-derived sediment accelerated the infilling of GRK after ~6 ka when the Indus delta started to grow. Until its complete infilling few centuries ago, freshwater input from the Indus, and perhaps from the Ghaggar-Hakra-Nara, probably sustained a productive marine environment as well as navigability toward old coastal Harappan and historic towns in the region.


The Great Rann of Kachchh (GRK) is a landlocked and largely infilled shallow marine basin connected to the Arabian Sea, neighboring the Indus delta to the east. Thar Desert and Aravalli Hills border GRK to the north and northeast respectively (Fig. 1a and b). At present GRK is a monotonous, salt-encrusted, vast mudflat, largely dried up during early summer (i.e., March–July) and inundated during the summer monsoon and winter season (i.e., July to February). Strong summer monsoon winds push seawater from the Arabian Sea into the GRK; usually the water does not evacuate or evaporate until the next summer1, 2. Owing to the harsh conditions, lack of accessibility and limited sediment exposure, only a few geomorphological and geoarchaeological studies are available for the region1,2,3,4,5,6.

Figure 1
Figure 1

(a) Regional drainage pattern for the western continental margin of the Indian plate. Dotted lines are the paleochannels of the Vedic Saraswati River after Ghose et al.11 and Kar and Ghose48. The box represents the area shown in b. Location of the Dhordo core site and river sediment samples analyzed are also shown. (b) Geomorphic setting of the Great Rann of Kachchh (GRK) basin with surrounding hinterland and core locations. NPF- Nagar Parkar Fault, IBF- Island Belt Fault, KMF- Kachchh mainland Fault, KHF- Katrol hill Fault, NKF- North Kathiawar Fault, SWF- South Wagad Fault, P- Pachham Island, K-Khadir Island, B- Bela Island and C- Chorar Island. Core location: DH- Dhordo core raised from central GRK basin. Maps were prepared using a licensed copy of Ocean Data49 View (

Several sites of the Bronze Age Harappan civilization flourished in and around GRK, including the large town of Dholavira on Khadir Island (Fig. 1b). As the Harappan coastal economy was probably dependent on maritime trade, the history of these towns was controlled by access to the Arabian Sea, which in turn was dependent on local sea level and fluvial infilling of the GRK7, 8. Previous studies postulated that a now extinct Vedic Saraswati River sourced in the Himalaya9 or Sub-Himalaya8, 10 reached down into the Arabian Sea as an independent river, parallel to the Indus11, 12. Such a river must have discharged into the paleo-gulf of GRK to reach the Arabian Sea. However, in spite of its geological and archaeological significance, GRK remains one of the least investigated regions of the Harappan domain13.

One of the keys to understand the geological and geomorphological evolution of the GRK is to fingerprint and resolve its potential sediment sources. Such sources may include the Indus River, the postulated Saraswati, the Arabian Sea shelf, the mainland Kachchh, Thar Desert and the Aravalli Ranges. In the present study we reconstruct sediment sources for the past ~17 ka6 using radiogenic tracers (i.e., Nd and Sr isotopes) in sediment core recovered from the GRK. The main goal of our study is to assess whether a Himalayan/Sub-Himalayan river reached the GRK independently of the Indus and for how long such a river was active, if at all.

Neodymium and strontium isotopes are some of the most robust provenance proxies. Nd is undergoing negligible alteration during erosion, sediment transport and deposition14,15,16,17 whereas Sr has been shown to be a good indicator of provenance in our study area18, 19. In our regional context, such studies have proven useful to explore erosion patterns, transport pathways, and provenance shifts for the Ganga–Brahmaputra17, 20, 21 as well as the Indus19, 22 fluvial systems. In addition, terrains neighboring the GRK such as the Thar Desert23,24,25, outcropping volcanics26 and Mesozoic rocks on Kachchh mainland27 have also been investigated for their Nd-Sr isotopic compositions.


The sediment core was recovered from the GRK (Fig. 1) near Dhordo village (23°49′37.9“N; 69°39′09“E) from the central Kachchh basin. Based on our previously published radiocarbon dates28, the Dhordo core recovered sediments as old as 17.7 ka down to ~60 m from the present day Rann surface. The subsurface GRK sediments studied in our core are consistently fine-grained in nature (i.e., silty-clay to clayey silts with negligible sand content; SI Fig. 1). Fine-grained sediments are typical for the GRK mudflats and remarkably consistent spatially and temporally in the entire basin1, 3, 6, 29. Our core at Dhordo is located far off from the elevated regions of mainland Kachchh, outside significant local sediment input, thus representing GRK basin wide changes. We assume that sedimentation is still active or non-erosional at Dhordo as the site is inundated during the summer monsoon.

The Dhordo core shows 87Sr/86Sr ratios range from 0.725 to 0.732 whereas εNd varies from −14.34 to −12.63. (SI Table 1). To characterize potential end members, we also analyzed modern sediments from three local rivers, namely the Luni, Rupen as well as a local stream called Saraswati (no connection with the Vedic counterpart). The sample from the Luni River, which flows through the Thar yields 87Sr/86Sr and εNd values of as 0.73 and −13.97. The local Saraswati stream and the Rupen River draining the Aravalli Hills yielded 87Sr/86Sr and εNd values of 0.735, 0.731 and −15.22, −14.86 respectively (SI Table 1). For other sediment sources such as the fluvial or eolian sediments along the proposed Vedic Saraswati, the Indus courses and shelf as well as the Thar Desert we discuss published data below.


Presence of foraminifera throughout the core section indicates marine sedimentation throughout6, 30. To allow for fine-grained marine sedimentation at ~18 ka30, when the eustatic sea level in the Arabian Sea was below 100 m relative to present level31, 32, the Dhordo site must have been uplifted significantly since then. GRK is largely compressional and uplift of ca. 5 m is recorded for a marine sedimentary sequence on Khadir Island in the last 500 years5, so uplift at Dhordo is not surprising.

Sediment Provenance

Marine sediments accumulating at the core location show a very tight range of variability within the Nd-Sr space (Fig. 2) The Aravalli sedimentary source is similar in isotopic composition to our sediments (present study; Fig. 2) but it cannot account for a significant contribution to the infilling of a large volume GRK basin. The mica-rich mineralogy of sediments (i.e., illite and chlorite) is indicative instead of their Himalayan and/or Karakoram origin18, 28. Similarly the Kachchh mainland hills were probably not a significant source of sediments given their small areal extent and geomorphology (i.e., the hydrographic network of short rivers is preferentially oriented southward). Therefore the remaining potential sediment sources for GRK sediments are Himalayan and/or Sub-Himalayan rivers including the Indus and the postulated Vedic Saraswati. In fact our sediments plot as a mixture of Indus sediments18, 22 with high εNd and low radiogenic Sr typical for the Karakoram and low εNd and high radiogenic Sr in Ghaggar-Hakra sediments18, 22, 23 indicative of High and Lesser Himalayan sources (Figs 2 and 3). Sediments coming from the Thar Desert25, 33 could also account for a significant contribution to GRK (Fig. 2), but this is not surprising as the Thar has been interpreted as a mixture of Himalayan and Sub-Himalayan sediments from the Indus and Ghaggar-Hakra systems23. However, Thar Desert is a vast sediment reservoir that is still poorly characterized geochemically.

Figure 2
Figure 2

Scatter plot of 87Sr/86Sr and εNd isotope compositions of our GRK sediments, Indus delta/floodplain (Clift et al.18, 22), Aravalli rivers (present study), Thar Desert (Tripathi et al.25), Ghaggar-Hakra fluvial system (East et al.23; Singh et al.33; Alizai et al.50 and the Indus shelf northwest of the Indus Canyon (Limmer et al.19) along with various potential end-members such as High Himalayan Crystalline, Lesser Himalaya and Siwaliks (Singh et al.17; Tripathi et al.24, 25 and references therein). Graph was prepared using a licensed copy of Sigma Plot v.10.

Figure 3
Figure 3

Deglacial and Holocene downcore variations in εNd and 87Sr/86Sr ratio values for GRK sediments plotted along with Indus River, Indus Shelf and Ghaggar-Hakra system. Ranges of variability for potential sources are shown at the top of each graph. Graphs were prepared using a licensed copy of Sigma Plot v.10.

Sedimentation History

The temporal variability in Nd and Sr composition for the marine sediments at our GRK site is remarkably subdued (see Fig. 3) when compared to similar compositional histories of potential sources (i.e., Indus, Ghaggar-Hakra and Thar). However it is clear that GRK sediments before 10 ka plot between the two sources of sediments (Fig. 3) possibly indicating input from the Himalayas (Higher and/or Lesser) in addition to Indus sediments that include Karakoram and Tethyan Himalayan signals. A Thar Desert origin for the sediments is also possible but this vast region may exhibit a large variability in Nd and Sr isotopic composition that needs to be better assessed (Fig. 2). After that period the sediments in the GRK are practically indistinguishable from the Indus when using Nd and Sr fingerprinting. In contrast sediments from the Indus continental shelf, at least those located west of the Indus canyon that have been measured so far, appear more radiogenic in Nd and have lower 87Sr/86Sr values due to alongshore contributions from the Bela ophiolite19, 22. Thus another alternative interpretation explaining the divergence between GRK and Indus isotopic signatures before 10 ka could be that the Indus sediments themselves contain a significant contribution from the Bela Ophiolite before 10 ka (Fig. 3). Such an input could have come alongshore from the west into the GRK and Indus paleo-estuary when its delta was only incipiently developing more inland.

The rather invariant history of the GRK sediment composition since deglaciation contrasts with the Indus record (Fig. 3), which shows an increasing Lesser Himalayan input22. On the other hand Ghaggar-Hakra sediments show an increasingly Thar-like signature in the later Holocene (Fig. 3), a trend that cannot be recognized in the GRK sediments. In that case the GRK sediments could have been a mixture of Indus and Ghaggar-Hakra sediments since the beginning of our core records. The GRK record could also be interpreted to be strongly dominated by Thar sediments if we assume that a desert is somewhat homogenous (Fig. 3). As such, the signature for an independent Saraswati extending the course of the Ghaggar-Hakra towards the Arabian Sea cannot be discerned in the GRK using the Nd-Sr isotopic system. The most likely reason for that is not the mixing between Indus and Ghaggar-Hakra sediments per se but the input from the mixed Thar reservoir.

Landscape Dynamics

Many courses for the Vedic Saraswati have been proposed over the years4, 11, 34,35,36 but they generally lack continuity in subsurface data and/or chronological information. Our new isotopic data suggests that a river, flowing parallel to and independent of the Indus, may have existed and reached the GRK before 10 ka (Fig. 3). At the time the Ghaggar-Hakra system may have been a much larger river tapping the Sutlej and/or the Yamuna8, 10, 33, 37, 38. However, this interpretation is dependent on the isotopic homogeneity of the vast sediment reservoir of the Thar Desert, which is still to be assessed. Whether such a river reached the Arabian Sea via the GRK during the Holocene and especially, during Vedic times remains to be demonstrated.

Recent studies of the upper courses of the proposed Saraswati in Haryana and Cholistan suggested that river desiccation started ~6.5 ka B.P.8, 10, 24, 34, 38. However, Giosan et al.8 showed that fluvial sedimentation was still active in the western part of the Thar Desert as late as ~3 ka, with river courses joining the Nara valley. Currently we do not know if the Nara was independent or received input from the Indus near Sukkur or further down after emerging from below the Rohri Hills (Fig. 1). However, the isotopic composition of the GRK sediments are not in contradiction with the idea of a dwindling Ghaggar-Hakra-Nara under the aridification of South Asia as the monsoon declined in the late Holocene39,40,41.

The Holocene sedimentation pattern in the GRK basin shows a regressive pattern with the basin becoming shallower as the sea level rose and rivers provided infill. During the deglaciation when sea level was considerably lower, a Saraswati-like river had a better chance to deliver a pure signal to GRK if it possessed its own Pleistocene incised valley, independent of the Indus incised valley10, 22, 41. However, by ~5 to 6 ka the Indus delta extended into the western GRK and probably provided sediments directly into the GRK41. Historical maps and documents42,43,44,45 suggest that GRK may have still been a gulf ca. 500 years ago5, 46. A deeper GRK with fresh water input from the Indus and potentially Ghaggar-Hakra-Nara would have provided a more productive marine environment and navigable ways for the old coastal Harappan towns in the region (e.g, Dholavira) as well as for later historical settlements.


The Nd and Sr isotopic composition of sediments from our Dhordo core site in the Great Rann of Kachchh suggests that a large Himalayan or Sub-Himalayan Saraswati-like river may have discharged into the Arabian Sea until 10 ka. However, our study also shows that radiogenic isotope fingerprinting of the GRK sediments is unlikely to detect a gradually drying Saraswati-like river after that time, due to contamination with sediments from the Thar Desert and/or the Indus. Alternatively the Thar may have been the dominant sediment source along with the Indus for the entire post-glacial history of the GRK. Future studies should concentrate instead on geophysical imaging, dating and geochemical fingerprinting of subsurface deposits from infilled channels along potential river courses in the Thar Desert. However, the Holocene sedimentary evolution of the Great Rann should be better explored to understand its role in Harappan and historical coastal habitation.

Sampling and methodology

The continuous sediment core was raised from the GRK basin (Fig. 1; SI Fig. 1). A ~60 m long core was drilled from the central part of the basin at Dhordo (23°49′37.9” N and 69°36′09.9” E). The entire core section was then X-radiographed before it was opened. The core pipes were then split longitudinally into two halves: one half of the core was sampled at 2 cm intervals while the other half was preserved as an archive. The GRK sediments are typically fine-grained, dominated by silts and clays with occasional sands6 (SI Fig. 1). The samples obtained from our cores at various depth intervals were analyzed for Nd-Sr radiogenic isotopes (SI Table 1) and radiocarbon chronologies (reported in Khonde et al.28). We also collected samples for Sr-Nd measurements from the Luni and Rupen rivers and the local stream Saraswati that discharge into the Great and Little Rann basins from the east. These rivers come from the Aravalli Hills, which lie further to the east and northeast.

Nd and Sr isotopic systematics

Measurements were carried out on carbonate- and organic matter-free silicate fraction. A known amount (~100 mg) of this fraction taken in Teflon vials (Savillex) was spiked with 84Sr and 150Nd and subjected to acid digestion with concentrated HF-HNO3-HCl at 90 °C to complete dissolution. Pure Nd and Sr fractions were separated from the solution following standard ion exchange procedures17, 47. The fractions were then dried and redissolved in 4 ml of 0.4 N HNO3. Both Nd and Sr measurements were done on MC-ICP-MS in static multi-collection mode at PRL15, 17. The measured 87Sr/86Sr and 143Nd/144Nd ratios were corrected for instrumental mass fractionation by normalizing them with 86Sr/88Sr, 0.1194 and 146Nd/144Nd, 0.7219. The Nd and Sr concentrations for these samples were obtained by isotope dilution method. A standard solution of 200 ppb of SRM 987 Sr-standard was measured several times on MC-ICP-MS that yielded an average value of 0.710307 ± 0.000010 (1σ, n = 10) for 87Sr/86Sr whereas 143Nd/144Nd in 100 ppb solution of JMC standard yielded 0.511732 ± 0.000016 (1σ, n = 10) respectively. Replicate samples were also measured for Nd and Sr concentrations and isotopic compositions on selected samples to check the overall reproducibility of the Nd-Sr measurements (SI Tables 2 and 3). Based on replicate measurements, the average variation was found to be 0.0002 and 0.2 for 87Sr/86Sr and εNd respectively. However the standard errors for 87Sr/86Sr and143Nd/144Nd are 0.0014%, 0.0010% respectively.

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  1. 1.

    Glennie, K. W. & Evans, G. A. Reconnaissance of the recent sediments of the Ranns of Kutch, India. Sedimentology 23, 625–64 (1976).

  2. 2.

    Roy, A. B. & Merh, S. S. The Great Rann of Kachchh: An intriguing Quaternary terrain. Recent Research in Geology 9, 100–108 (1981).

  3. 3.

    Bilham, R. Slip parameters for the Rann of Kachchh, 16 June 1819 earthquake, quantified from historical accounts. Geol. Soc. Lon. Spec. Pub. 146, 295–319 (1998).

  4. 4.

    Burnes, A. Memoir on the eastern branch of the River Indus. Trans. Roy. Asia. Soc. 3, 550–88 (1835).

  5. 5.

    Khonde, N. et al. Environmental significance of raised Rann sediments along the margins of Khadir, Bhanjada and Kuar bet islands in Great Rann of Kachchh, Western India. Curr. Sci. 101(11), 1429–1434 (2011).

  6. 6.

    Maurya, D. M. et al. Subsurface sediment characteristics of the Great Rann of Kachchh, western India based on preliminary evaluation of textural analysis of two continuous sediment cores. Curr. Sci. 104(3), 1071–1077 (2013).

  7. 7.

    Gaur, A. S. et al. Was the Rann of Kachchh navigable during the Harappan times (Mid-Holocene)? An archaeological perspective. Curr. Sci. 105(11), 1485–1491 (2013).

  8. 8.

    Giosan, L. et al. Fluvial Landscapes of Harappan civilization. Proc. Natl. Acad. Sci. 109(26), E1688–94 (2012).

  9. 9.

    Valdiya, K. S. The River Saraswati was a Himalayan-born river. Curr. Sci. 104(1), 42 (2013).

  10. 10.

    Clift, P. D. et al. U-Pb zircon dating evidence for a Pleistocene Sarasvati River and capture of the Yamuna River. Geology 40(3), 211–14 (2012).

  11. 11.

    Ghose, B., Kar, A & Husain, Z. The lost courses of the Saraswati River in the Great Indian Desert: New evidence from landsat imagery. Geogr. Jour. 446–451 (1979).

  12. 12.

    Oldham, C. F. The Saraswati and the Lost River of the Indian Desert.Jour. Roy. Asi. Soc. of Great Britain and Ireland (New Series) 25(01), 49–76 (1893).

  13. 13.

    Merh, S. S. The Great Rann of Kachchh: Perceptions of a field geologist. Jour. Geol. Soc. Ind. 65, 9–25 (2005).

  14. 14.

    Galy, A. & France-Lanord, C. Higher erosion rates in the Himalaya: geochemical constraints on riverine fluxes. Geology 29(1), 23–26 (2001).

  15. 15.

    Goswami, V. et al. Temporal variations in 87Sr/86Sr and ɛNd in sediments of the southeastern Arabian Sea: Impact of monsoon and surface water circulation. Geochem, Geophy. Geosys. 13(1), Q01001 (2012).

  16. 16.

    Grousset, F. E. et al. Neodymium isotopes as tracers in marine sediments and aerosols: North Atlantic. Earth. Planet. Sci. Lett. 87, 367–378 (1988).

  17. 17.

    Singh, S. K., Rai, S. K. & Krishnaswami, S. Sr and Nd isotopes in river sediments from the Ganga Basin: Sediment provenance and hot-spots of physical erosion. Jour. Geophys. Res. 113, F3 (2008).

  18. 18.

    Clift, P. D. et al. Monsoon control over erosion patterns in the western Himalaya: possible feed-back into the tectonic evolution. Geol. Soc. Lond. Spec. Publ. 342(1), 185–218 (2010).

  19. 19.

    Limmer, D. R. et al. Geochemical record of Holocene to Recent sedimentation on the Western Indus continental shelf, Arabian Sea. Geochem. Geophy. Geosys. 13(1), Q01008 (2012).

  20. 20.

    France-Lanord, C., Derry, L. & Michard, A. Evolution of the Himalaya since Miocene time: isotopic and sedimentological evidence from the Bengal Fan. Geol. Soc. Lond. Spec. Publ. 74 (1), 603–621 (1993).

  21. 21.

    Singh, S. K. & France-Lanord, C. Tracing the distribution of erosion in the Brahmaputra watershed from isotopic compositions of stream sediments. Ear. Plant. Sci. Lett. 202(3), 645–662 (2002).

  22. 22.

    Clift, P. D. et al. Holocene erosion of the Lesser Himalaya triggered by intensified summer monsoon. Geology 36, 79–82 (2008).

  23. 23.

    East, A. E. et al. Fluvial–eolian interactions in sediment routing and sedimentary signal buffering: an example from the Indus Basin and Thar Desert. Jour. Sedi. Res. 85(6), 715–728 (2015).

  24. 24.

    Tripathi, J. K. et al. Is River Ghaggar, Saraswati? Geochemical constraints. Curr. Sci. 87(8), 1141–1145 (2004).

  25. 25.

    Tripathi, J. K., Bock, B. & Rajamani, V. Nd and Sr isotope characteristics of Quaternary Indo-Gangetic plain sediments: Source distinctiveness in different geographic regions and its geological significance. Chem. Geol. 344, 12–22 (2013).

  26. 26.

    Sen, G. et al. Deccan plume, lithosphere rifting, and volcanism in Kutch, India. Ear. Plant. Sci. Lett. 277(1), 101–111 (2009).

  27. 27.

    Patil. D. J. et al. C, O, Sr isotope compositions of sediments of sediments of the Mesozoic Kutch basin, NW India. Paper presented at 21st Goldschmidt Conference, 1606 (2011).

  28. 28.

    Khonde, N., Maurya, D. M. & Chamyal, L. S. Late Pleistocene-Holocene clay mineral record from the Great Rann of Kachchh basin, Western India: Implications for palaeoenvironments and sediment sources. Quat. Int., 443, 86–98, doi:10.1016/j.quaint.2016.07.024 (2017).

  29. 29.

    Tyagi, A. K. et al. Mid-Holocene sedimentation and landscape evolution in the western Great Rann of Kachchh, India. Geomorphology 151, 89–98 (2012).

  30. 30.

    Khonde, N. Holocene environments and geomorphic evolution of the Great Rann of Kachchh, Western India. PhD Thesis. (The M. S. University of Baroda, Vadodara, 2014).

  31. 31.

    Camoin, G. F., Montaggioni, L. F. & Braithwaite, C. J. R. Late glacial to post glacial sea levels in the Western Indian Ocean. Mar. Geol 206(1), 119–146 (2004).

  32. 32.

    Kench, P. S. et al. Geological effects of tsunami on mid-ocean atoll islands: the Maldives before and after the Sumatran tsunami. Geology 34(3), 177–180 (2006).

  33. 33.

    Singh, A. et al. Geochemistry of buried river sediments from Ghaggar Plains, NW India: Multi-proxy records of variations in provenance, paleoclimate, and paleovegetation patterns in the Late Quaternary. Palaeogeogr. Palaeoclimat. Palaeoecol. 449, 85–100 (2016).

  34. 34.

    Pal, Y. et al. Remote sensing of the ‘lost’ Saraswati river. Proc. Ind. Nat. Sci. Acad. (Earth and Planetary Sciences) 89(3), 317–331 (1980).

  35. 35.

    Rao, S. M. Use of isotopes in search of Lost River. J. Radioanal.and Nucl. Chem. 257(1), 5–9 (2003).

  36. 36.

    Saini, H. S. et al. Reconstruction of buried channel-floodplain systems of the northwestern Haryana Plains and their relation to the ‘Vedic’ Saraswati. Curr. Sci. 97(11), 1634–43 (2009).

  37. 37.

    Maemoku, H. et al. Geomorphological Constraints on the Ghaggar River Regime During the Mature Harappan Period. Climates, Landscapes, and Civilizations, 97–106pp (2013).

  38. 38.

    Saini, H. S. & Mujtaba, S. A. I. Depositional history and palaeoclimatic variations at the northeastern fringe of Thar Desert, Haryana Plains, India. Quat. Int. 250, 37–48 (2012).

  39. 39.

    Enzel, Y. et al. High-resolution Holocene environmental changes in the Thar Desert, northwestern India. Science 284(5411), 125–128 (1999).

  40. 40.

    Ponton, C. et al. Holocene aridification of India. Geophy. Res. Lett. 39(3) (2012).

  41. 41.

    Giosan L. et al. On the control of climate- and human-modulated fluvial sediment delivery on river delta development: The Indus: Eos (Transactions, American Geophysical Union), 87, 52, OS14A–04 (2006).

  42. 42.

    Rajendran, C. P. & Rajendran, K. Characteristics of deformation and past seismicity associated with the 1819 Kutch earthquake, northwestern India. Bull. Seism. Soc. Amer 91(3), 407–426 (2001).

  43. 43.

    Rao, S. R. Lothal and Indus Civilization (Asian Publishing House, NY, 1973).

  44. 44.

    Sivewright, R. Cutch and the Ran. Geog. Jour. 29(5), 518–535 (1907).

  45. 45.

    Wynne, A. B. & Fedden, F. Memoir on the Geology of Kutch: To Accompany the Map Compiled by AB Wynne and F. Fedden, During the Seasons of 1867–68 and 1868–69. Geol. Sur. Ind. (1872).

  46. 46.

    Frere, H. B. E. Notes on the Runn of Cutch and neighbouring region. Jour. Roy. Geog. Soc. Lond. 181–207 (1870).

  47. 47.

    Rahaman, W. et al. Climate control on erosion distribution over the Himalaya during the past ~100 ka. Geology 37(6), 559–562 (2009).

  48. 48.

    Ghose, B. & Kar, A. The Former Stream courses in the Indian Desert and their Effects on Natural Resources. In Proceedings of the Indo-US Workshop on Arid Zone Research, CAZRI, Jodhpur. pp. 140–149 (1984).

  49. 49.

    Schlitzer, R., Ocean Data View, (2016).

  50. 50.

    Alizai, A. et al. Pb isotopic variability in the modern-Pleistocene Indus River system measured by ion microprobe in detrital K-feldspar grains. Geoch. Cosm. Acta 75(17), 4771–4795 (2011).

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The drilling effort and subsequent study of the cores was funded by Department of Science and Technology (DST), Government of India sponsored research project to DMM (Project No. SR/S4/ES-21/Kachchh Window/P1) under the science of Shallow Subsurface Programme (SSS). N. Khonde gratefully acknowledges Indo-US Post-doctoral Fellowship sponsored by SERB-IUSSTF for research work at Woods Hole Oceanographic Institution, USA during the revision of the paper. We thank Amal Kar and Peter Clift for their valuable suggestions during revision.

Author information

Author notes

    • Nitesh Khonde

    Present address: Birbal Sahni Institute of Palaeosciences, Lucknow, 266007, India


  1. Department of Geology, The M. S. University of Baroda, Vadodara, 390002, India

    • Nitesh Khonde
    • , D. M. Maurya
    •  & L. S. Chamyal
  2. Physical Research Laboratory, Navrangpura, Ahmedabad, 380009, India

    • Sunil Kumar Singh
    •  & Vinai K. Rai
  3. Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, USA

    • Liviu Giosan


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D.M.M., N.K., L.S.C., S.K.S. designed research, N.K., S.K.S. performed research; V.K., S.K.S. analyzed data, N.K., D.M.M., S.K.S. and L.G. interpreted the data and wrote the paper.

Competing Interests

The authors declare that they have no competing interests.

Corresponding author

Correspondence to D. M. Maurya.

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