Tectonic Fabric, Geochemistry, and Zircon-Monazite Geochronology as Proxies to Date an Orogeny: Example of South Delhi Orogeny, NW India, and Implications for East Gondwana Tectonics

We have dated the South Delhi orogeny, Aravalli-Delhi Mobile Belt (ADMB), NW India, using the tectonic fabric, geochemistry, and zircon-monazite geochronology as the proxies. The South Delhi Terrane (SDT), a passive margin domain in the ADMB, consists of multiply deformed (D1–D4) greenschist facies rocks and several granite plutons. The D1 deformation is characterized by pervasive isoclinal recumbent F1 fold and axial planar tectonometamorphic fabric, S1, developed in all rock types. The S1 minerals belong to peak greenschist facies metamorphism, M1, suggesting syntectonic nature of M1 with D1. The age of the D1-M1 is constrained by the syncollisional peralkaline S type Sewariya granite which is characterized by magmatic/submagmatic fabric (Sm) coplanar with the S1. The margin of the pluton is turned into quartzofeldspathic gneiss carrying the evidence of high temperature deformation. The age of Sewariya granite is estimated at ca. 878 Ma by zircon geochronology. The D1-M1 is further constrained by monazite geochronology of the mica schist at ca. 865–846 Ma. The other granite plutons and metarhyolite are pre-D1 and emplaced at ca. 992–946 Ma. The D2 deformation produced NE-SW trending open upright F2 folds coaxial with the F1, and northwesterly vergent F2–axial planar thrusts. Monazite geochronology constrains the D2 at ca. 811–680 Ma. The D3 is characterized by small to large scale NW-SE folds, and the D4 by faults and fractures marking the brittle deformation in the rocks. The D4 is constrained by monazite geochronology at ca. 588–564 Ma. There are upper amphibolitic tectonic slivers along the D2-Phulad thrust, belonging to the pre-Delhi rocks, which show ca. 1,638 Ma metamorphism age. From the above study, it is suggested that the South Delhi orogeny belongs to ca. 878–680 Ma marking the final amalgamation of Marwar Craton with the rest of India. This overlaps the early phase of the Pan-African orogeny (900–630 Ma). The brittle deformation, D4, coincides with Kuunga orogeny (650–500 Ma). Our study implies that India, like other continents in the East Gondwana, underwent amalgamation of internal blocks until the late part of the Neoproterozoic.


INTRODUCTION
Amalgamation of continents took place through accretion and continental collision giving rise to supercontinental assembly. Orogens were created along the zone of amalgamation, which are marked by ductile as well as brittle deformation of rocks, different types of metamorphism, and intrusion of variety of magmatic rocks (Twiss and Moores, 1992;Kearey et al., 2009). A correlative study between tectonometamorphic fabric with geochronology of magmatic rocks and metamorphic mineral could estimate the life span of a supercontinental cycle (Hawkesworth et al., 2017). The earth underwent several orogenic cycles in the past since Neoarchean to Tertiary period. The Nuna orogeny was responsible for the formation of the Columbia Supercontinent (ca. 2.1 to 1.8 Ga, Rogers and Santosh 2002;Zhao et al., 2002), the Grenvillian orogeny was responsible for the Rodinia Supercontinent (ca. 1.3 to 1.0 Ga; Valentine and Moores, 1970;McMenamin and McMenamin, 1990;Meert and Torsvik, 2003;Cawood, 2005;Li et al., 2008), and the Pan-African orogeny created the Gondwana Supercontinent (0.9-0.5 Ga, Stern, 1994;Kroner and Stern, 2005;Fritz et al., 2013;Oriolo et al., 2017). Each orogeny comprises several phases of subduction and arc accretion that vary temporally and spatially at different parts of the Supercontinent. For example the Pan-African orogeny consists of an earlier phase of subduction and arc accretion (0.9-0.63 Ga) as observed in the Arabian-Nubian shield (Kroner and Stern, 2005) and a late phase of collision (Kuunga orogeny, ca. 0.65-0.50 Ga) in Madagascar, Tanzania, and other parts of Africa (Meert and Lieberman, 2008;Lehmann et al., 2016).
In this paper, we studied the South Delhi orogeny of the Archean-Neoproterozoic Aravalli-Delhi Mobile Belt (ADMB) in NW India that consists of several terranes juxtaposed along shear zones ( Figures 1A,B). The terranes are Hindoli-Jahazpur, Mangalwar, Sandmata, Aravalli, North Delhi, South Delhi, and Sirohi terranes. The ADMB bears the imprint of the Nuna, Grenvillian, and Pan-African orogenies. The age of the South Delhi orogeny is still debated, if it is equivalent to Grenvillian or Pan-African, because most of the studies are based on single proxy. For instance, with very little analysis of magmatic vs. solid state fabric of the diorite (1.0 Ga, Volpe and Macdaugall, 1990), the Godhra granite (0.95 Ga, Gopalan et al., 1979), and the Chang granite ( Table 1, 0.97 Ga, Tiwana et al., 2019), a Grenvillian age for the South Delhi orogeny was advocated (Roy, 2001). Similarly, based on monazite ages of Pilwa-Chinwali area without much consideration to deformation fabric Grenvillian age has been considered (Bhowmik et al., 2018). Contrarily, Singh et al. (2010) used zircon geochronology of granite and deformation history of host rocks and deduced ca. 0.87-0.65 Ga age, suggesting Pan-African age. Similar ages (ca. 0.87-078 Ga) were obtained by Tiwari and Biswal (2019a) who applied a combined study of monazite geochronology and deformation fabric to Ambaji granulite. We adopted a new approach wherein multiple proxies have been applied that include deformational structure in the metasediments and granite plutons to know chronological sequence of granite intrusion with deformation. Further, geochemistry of granites was studied to decipher the tectonic setting of their intrusion. Furthermore, zircon and monazite geochronology were conducted to date the granite plutons and tectonometamorphic fabric in the metasediments. Based on these studies, the South Delhi orogeny was found not directly related to Grenvillian or Kuunga orogeny (late part of Pan-African) rather to the early part of Pan-African orogeny. Therefore, we suggest that some of the orogenies observed in different continents may not have direct match with global scale orogenies which was responsible for building supercontinental assembly.

Field Setting
Mapping of litho-units and meso-microfabric study of rocks were carried out and the structural map of the area (Singh et al., 2020) was updated with addition of a greater amount of structural data and stereoplots for areas like large scale fold hinges and shear zones. Large scale structures were interpreted with the help of structural cross sections. Mica schist and calcareous schist are the major metasedimentary units in the area ( Figures 2B,C). The mica schist is marked by close spaced schistosity (S 1 ) ( Figures  3A,B) and calcareous schist contains rib structure produced by differential weathering between carbonate layer and silicate layers ( Figures 3C-H). The calcareous schist grades into impure marble and calcareous quartzite. The impure marble carries bedding parallel epidote-garnet skarnoid bands as at Rupnagar ( Figure 3D). Metaconglomerate formation having width ranging from m to 10 m occurs within mica schist, in the west of Babra ( Figure 2B). The metaconglomerate consists of alternate mica schist and quartzite layers with several ellipsoidal quartzite and granite pebbles ( Figures 3I,J). The Phulad thrust passes along the metaconglomerate formation and converted the rock into a micaceous mylonite. The pebbles and quartzite layers within the thrust are flattened and stretched down-dip, forming boudin, mullion, and rodding structures. Further, meter scale slivers of basement pelitic-gneissic rocks ( Figure 3K) occur within the thrust zone; they carry garnet, tourmaline, quartzofeldspathic pockets, and sillimanite needles visible on the schistosity surface.
Concordant bands of metarhyolite and amphibolite occur within mica schist and calcareous schist (thickness varying from few cm to m) near Rupnagar and Babra (Figures 2B,C,3L,M). These rocks are marked by flow layers (S 0 ) and filled-in vesicles ( Figure 3M).
Several deformed granite plutons occur in the area, namely, Sendra, Chang, Pratapgarh, Sumel, and Sewariya plutons (Figures 2A-C). Heron (1953) included all of them within Erinpura granite while later workers (Bhattacharjee et al., 1993;Gupta et al., 1997;Pandit et al., 2003) classified them into Sendra granite (Sendra, Chang, Pratapgarh, and Sumel pluton) and Erinpura granite (Sewariya pluton). Field relation suggests that the Sewariya granite is the youngest as its apophyses crosscut the metasediments as well as other granite plutons ( Figures 3F,N). The Pratapgarh and Sumel plutons are coarse grained with prominent NE-SW trending S 1 fabric; it carries several metasedimentary and metavolcanic roof pendants and xenoliths which are folded and metamorphosed along with the pluton ( Figure 3N). Sewariya pluton occurs as a linear body in the western part of the area (Figures 2A,b) containing magmatic/ semimagmatic (S m ) and solid state deformation fabric, S 1 ( Figures 3O,Q). Tourmalines are segregated into ellipsoidal to ribbon shape pockets ( Figure 3R-inset 1) and amphibolite-mica schist xenoliths are more common in the central part of the Sewariya granite ( Figure 3R-inset 2). The pluton shows distinct textural variation from core to the margin ( Figure 3R). The core part of the pluton is characterized by magmatic/submagmatic fabric (S m ) due to shape preferred alignment of quartz, plagioclase, and K-feldspar minerals ( Figure 3R). It is coplanar with S 1 fabric albeit the S 1 fabric anastomoses around the coarse grains of feldspar and quartz. The pluton exhibits an increase in intensity of deformation from core to the margin. The granite converts to a quartzofeldspathic gneiss near the host rock contact ( Figure 3R). The pluton and host rock fabric are coupled as the S m parallel S 1 fabric in the granite is coplanar with the S 1 fabric in the host rock and together participated in subsequent folding. This evidences the syntectonic emplacement of granite with D 1 deformation (cf. Vernon et al., 1989;Bouchez et al., 1990;Miller and Paterson, 1994;Paterson et al., 1998;Buttner, 1999;Biswal et al., 2007). Such gneisses occur at several places, e.g., Kalakot, Bar, and Babra, which were earlier identified as pre-Delhi gneiss (Figure 2A, Heron, 1953). At Bar (near Makarwali village, Figure 2A), there is a spectacular gradation of mica schist into granite gneiss. The mica schist contains quartzofeldspathic layers derived from lit-par-lit injection of Sewariya granite pluton; the  quartzofeldspathic layers increase in number and thickness and grade into granite gneiss.

Textural Study
Mica schist contains alternate thin quartzofeldspathic and micaceous bands, and the muscovite and biotite show shape preferred orientation defining the S 1 fabric in the rock ( Figure 4A). The calcareous schist carries layers of tremoliteactinolite with shape preferred orientation parallel to S 1 ( Figure 4B). Occasionally, plagioclase and epidote porphyroblasts with inclusions of tremolite and actinolite occur in the rock. The tectonic slivers within metaconglomerate contain garnet, staurolite, tourmaline, quartz, feldspar, and ± sillimanite assemblage ( Figure 4C). Along the thrusts, micaceous mylonite is developed that contains quartz ribbons which are recrystallized into smaller grains ( Figure 4D). Further, the tectonic slivers show tailed garnet and staurolite grains ( Figures 4E,F) and the rock shows retrogression of sillimanite to muscovite and staurolite to biotite ( Figure 4E). The metarhyolite comprises quartz (40-50%), plagioclase (30-40%), hornblende, and epidote; the grain size varies between 100 and 120 µm ( Figure 4H). Hornblende is euhedral and shows shape preferred orientation parallel to S 1 fabric. Epidote is produced from retrogression of hornblende during shearing ( Figure 4G). Plagioclase retains its euhedral shape characteristic of magmatic origin. Quartz is subrounded and show bulging grain margin indicating low temperature dynamic recrystallization. Amphibolite shows granoblastic to well-foliated character (with S 1 fabric) and contains hornblende-epidote-biotite-quartz-plagioclase minerals ( Figure 4I).
The Pratapgarh pluton is coarse grained containing microcline, quartz, and plagioclase that show an equigranular mosaic (grain size 450-500 µm) ( Figure 4J). Biotite, muscovite, and rare garnet, sillimanite, and tourmaline are present in the rock; garnet and sillimanite represent the undigested phases. Microcline and plagioclase maintain euhedral shape, and the polysynthetic lamella in plagioclase is in random orientation to suggest the absence of any magmatic fabric in the rock. However, the rock shows low temperature deformation fabric indicated by bulging recrystallization of quartz and shape preferred orientation of mica minerals parallel to S 1 fabric. The Sumel pluton is inequigranular, coarse grained, and porphyritic containing plagioclase phenocrysts in the groundmass of K-feldspar, quartz, tourmaline, and biotite. Plagioclase still preserves euhedral shape indicating magmatic origin ( Figure 4K). Biotite shows shape preferred orientation defining deformation fabric (S 1 ) in the rock. The pluton is marked by N-S trending pegmatite veins intruded along fractures and ductile shear zones. Absence of magmatic fabric and development of greenschist facies deformation fabric (S 1 ) similar to the metasediments point toward pre-D 1 intrusion of these plutons.
The Sewariya granite is coarse grained and consists of quartz, K-feldspar, plagioclase, muscovite, biotite, and tourmaline. The magmatic/submagmatic fabric S m is best visible on the polished surface of the sample, having been defined by alignment of longer dimension of the euhedral plagioclase and K-feldspar crystals ( Figure 4L). Some grains are oriented at an angle probably due to lack of space for rotation during flow of magma (cf. Bouchez et al., 1990). Under microscope the twin planes of these minerals are oriented parallel to the S m . The K-feldspar and plagioclase phenocrysts contain mica inclusions in mutually perpendicular orientation, one parallel to cleavage and the other perpendicular to it ( Figure 4M). Surrounding the feldspar phenocrysts, smaller quartz grains are dynamically recrystallized, which are characterized by chess board twinning and grain boundary migration. Plagioclase and K-feldspar occasionally show dynamic recrystallization into smaller grains ( Figure 4N). Toward the margin of the pluton, the rock exhibits increase in degree of dynamic recrystallization and segregation into alternate quartzofeldspathic and mica rich bands ( Figures 4O,P). Smaller grains of plagioclase, K-feldspar, and quartz are developed out of such dynamic recrystallization; quartz shows chess board twinning; all these features indicate higher temperature of deformation at about 650-700°C (cf. Stipp et al., 2002;Passchier and Trouw, 2005).

Structures
Three stages of ductile deformation (D 1-3 ) and one stage of brittle deformation (D 4 ) affected the rocks. The D 1 deformation produced cm to m scale NE-SW axial oriented tight to isoclinal recumbent/reclined to upright F 1 folds ( Figures  3A,C). These are developed not only in the metasediments but in the amphibolite, metarhyolite, and granite also. Due to syn-D 1 greenschist facies metamorphism (M 1 ), pervasive F 1 axial planar schistosity (S 1, Figures 3A,B) and intersection lineation between bedding and S 1 fabric ( Figure 3A) are developed in all the rock types. The D 2 deformation developed cm to 10 m scale NE-SW trending upright F 2 folds (Figures 3B,E) coaxially with the F 1 (type 3 interference pattern, Ramsay, 1967). Crenulation cleavage and pucker axes associate with the F 2 fold ( Figures 3B and 4B) and axial planar thrusts were developed ( Figure 3D). The F 2 fold bears testimony of buckling (parallel folding, disharmonic folding, etc., Figure 3B) and was ascribed to a NW-SE horizontal compression during D 2 . The D 3 developed m to 10 m scale NW-SE to N-S trending F 3 folds, attributed to NE-SW shortening of the orogen ( Figure 3F). Type 1 ( Figure 3G) and type 2 interference patterns ( Figure 3H) were produced due to superposition of F 3 on the F 2 and F 1 folds, respectively. Ductile deformation was followed by brittle deformation (D 4 ) which is represented by N-S and NNE-SSW brittle fractures; late-stage pegmatite veins intrude the fractures at places ( Figure 3P).
Several NE-SW trending F 1 folds are mapped in the metarhyolite-amphibolite-calc schist sequence to the north of Rupnagar ( Figure 2C and profile section Figure 2I); the S 1 fabric crosscut the litho-units at the F 1 hinge zone. The F 1 axial planes are refolded by NW-SE trending F 3 fold to produce type 2 interference pattern in map scale. Further, to the west of Rupnagar, the F 1 folds in marble-metarhyolite-amphibolite sequence are refolded by an F 2 fold producing type 3 interference pattern which is indicated by girdle distribution of S 1 fabric in stereoplot; the β axis lies in ESE direction ( Figure 2G).
Frontiers in Earth Science | www.frontiersin.org February 2021 | Volume 8 | Article 594355 The F 1 -F 2 axes are rotated from NE direction toward ESE direction by the F 3 fold. Further, F 2 folds are present to the NE of Ratariya and Pratapgarh in the calc and mica schist units; the core of the fold is occupied by the Pratapgarh granite pluton (profile section Figure 2I). The F 1 fold and S 1 fabric in metasediments as well as in the granite are refolded around the hinge zone of the F 2 fold. The axis of the fold is oriented toward SSW as indicated by the β axis in stereoplot ( Figures  2E,F). The lineation plots do not coincide with the β axis suggesting that the lineations are rotated to a large extent by the F 3 fold. The entire structure surrounding the Pratapgarh pluton represents dome and basin structure in large scale. In addition, the mica schist amphibolite sequence describes large scale F 2 fold with NNE-SSW trending β axis to the west of Babra ( Figure 2D, structural profile Figure 2H). The stereoplot shows an incomplete girdle suggesting either F 2 hinges are too tight or they are obliterated by thrusting. The lineations in the stereoplot show concentration in NE as well as SW quadrant indicating plunge reversal due to the F 3 folding. In this domain, the Sewariya pluton is marked by F 1 fold and S 1 fabric. The S 1 fabric remains parallel with the litho-contact between the pluton and mica schist as well as the S 1 within mica schist. In both the mapped areas, west of Babra as well as around Rupnagar ( Figures Naylor and Sinclair, 2008). The most prominent amongst them is Phulad thrust passing along the metaconglomerate-mica schist formations west of Babra ( Figure 2A). The thrust is marked by quartz-biotite mylonite with crudely defined S-C fabric ( Figure 3I). The mylonitic foliation dips to SE and the stretching lineation is nearly down-dip ( Figure 2D, 3J). The stretching lineation is defined by muscovite and biotite minerals. The conglomerate pebbles are stretched parallel to stretching lineation. Apart from that, large number of boudins ( Figure 3I), mullions, and rodding of quartzite, granite, and gneisses associate with stretched pebbles. These boudins are long drawn out on both vertical and horizontal section; vertical stretched axis is 5-10 times longer than the horizontal stretched axis. Though the boudin long axes are parallel with the mylonitic foliation, these are tilted with a smaller angle with mylonitic foliation (∼15°) nearly in more than 50% of cases ( Figure 3I). The boudins can be classified as symmetrical-drawn boudins to asymmetrical-shear boudins (cf. Goscombe et al., 2004) suggesting effect of vertical shearing in the formation of boudin structures. As the boudins are detached both horizontally and vertically, they can be termed as chocolate boudins (Ghosh, 1988). Vertical shearing with large component of pure shear component during D 2 -thrusting has flattened the boudins and pebbles and made them near parallel to the mylonitic foliation ( Figure 3I, Dasgupta et al., 2012). A low plunging intersection lineation between S and C fabric is developed on C-surface in a few instances ( Figure 3J). The lensoidal quartz aggregates show dynamic recrystallization of quartz grains by subgrain rotation; the quartz grains are oriented at an angle to the mylonitic foliation (C). Temperature of deformation is around 450°C (e.g., Stipp et al., 2002). Lensoidal quartz aggregates, mica fishes, and S-C fabric on the XZ section of the mylonites indicate top-to-NW sense of thrust-slip kinematics ( Figure 3I). The upper amphibolite grade tectonic slivers contain several rounded garnet and tourmaline grains. Garnet contains quartz-biotite inclusion trails ( Figure 4C). The orientation of such inclusion trails varies from grain to grain suggesting variable amount of rotation of host garnet grains during D 2 shearing. Sillimanite and staurolite grains are retrogressed during shearing to muscovite and biotite to form porphyroclastic tail in the strain shadow zone of the garnet (Figures 4C,E,F). The sigma type garnet porphyroclasts indicate top-to-NW vergence thrusting (Figures 4C,E-G). In addition, a pair of thrusts occurs on western and eastern edge of the Pratapgarh granite pluton, both jointly named as Pratapgarh thrust. The western thrust passes through the mica schist. The lensoidal aggregate contains dynamically recrystallized quartz grains ( Figure 4D). These grains show top-to-NW thrust sense of shear. The S fabric is at high angle (60°) to C fabric, which suggests there is volume gain during thrusting due to fluid injection (e.g., Ramsay and Huber, 1987). Rupnagar thrust occurs on the eastern edge of the metarhyolite formation ( Figure 2A). The metarhyolite is sheared and produced muscovite-biotitequartz-epidote assemblage. The mylonite contains SE plunging stretching lineations, and the S-C fabric indicates top-to-NW thrusting ( Figure 4G). In addition to these ductile shear zone, brittle fault, namely, Chang fault, occurs at the contact between the pre-Delhi granite gneiss and metasedimentary sequence east of Rupnagar and Babra fault, west of Babra. The fault zone is marked by crushed rock of the amphibolite and marble ( Figure 3P).

Metamorphism
The rock types show greenschist facies metamorphism. Mica schist and calcareous schist contain muscovite, biotite, tremolite-actinolite, and epidote minerals characteristic of greenschist facies assemblage ( Figures 4A,B). Interbedded metarhyolite contains quartz grains which show bulging; plagioclase and K-feldspar still preserve magmatic habit ( Figure 4H); the amphibolite band consists of hornblende, albite, and epidote ( Figure 4I). Pratapgarh-Sumel granite shows growth of mica and grain boundary migration in quartz; feldspar retains magmatic habit ( Figure 4J). All these corroborate to greenschist facies of metamorphism that represents the peak metamorphism in the area (M 1 ) syntectonic with the D 1 deformation. The Sewariya granite shows dynamic recrystallization of plagioclase and K-feldspar (Figures 4M,N,P) indicating higher temperature of metamorphism (M 1 ), nearly 700°C (Pryer, 1993;Kruhl, 1996;Rosenberg and Stuniz, 2003), but under similar pressure condition as greenschist facies. The D 2 -D 3 indicates greenschist facies metamorphic condition. This is indicated by the crystallization of mica along the axial plane of the folds. The pelitic gneiss slivers within metaconglomerate show upper amphibolite facies metamorphism as they contain garnet-staurolite-tourmaline-quartz-feldspar-sillimanite assemblage (Figures 4C,E,F). During D 2 shearing, fluid activity along the thrust retrograded sillimanite to muscovite, staurolite to biotite, and hornblende to epidote (Figures 4E-G).

MATERIALS AND METHOD FOR GEOCHEMISTRY AND GEOCHRONOLOGY
Principle Geochronology, geochemistry, and tectonic fabric of a granite serve as important proxies for dating an orogeny. For example, rifting of continent creates synsedimentary bimodal volcanism and granite intrusion in the basin (e.g., New England Orogen, Allen et al., 1998;Liu and Han, 2019). Further, when the basin closes through subduction/collision the rocks undergo high grade metamorphism and melting at depth producing synorogenic granites (Finnacca et al., 2019). Postorogeny granite is emplaced in extensional setting (Pearce, 1996;Zhang et al., 2018). Granites intruding at different period of orogenesis are distinguished by their geochemical signature and tectonic fabric. For instance, the preorogenic granite reflects extensional or rift setting geochemistry and it undergoes ductile deformation recording multiple solid state deformation fabric during orogenesis. Synorogenic granite shows S type geochemistry and contains magmatic/semimagmatic fabric coupled with solid state deformation fabric (Bouchez et al., 1990;Chappell and White, 1992;Paterson et al., 1998). Postorogenic granite lacks solid state deformation fabric. The granites are dated by zircon geochronology because zircon has the higher closure temperature to U-Th -Pb system (>900°C.; Dahl, 1997;Cherniak and Watson, 2001). However, zircon cannot reset the age in response to low temperature shearing. For dating fluid induced low temperature deformation, monazite geochronology is most suitable. Monazite crystallizes in response to fluid activity (alkali rich) at different period of deformation and develops compositional domains corresponding to each phase of growth (Williams and Jercinovic, 2002;Pyle et al., 2003;Foster et al., 2004;Mahan et al., 2006). As the closure temperature of monazite for Th-Utotal Pb is ca. 800°C, each domain retains its age of formation and can be used as geochronometer (Cherniak et al., 2004;Cherniak and Pyle, 2008).

Geochemistry
Geochemistry of granite and metarhyolite was carried out with 15 samples collected at 100 m interval across the strike of the pluton ( Figures 2B,C). Major elements were analyzed for all samples; however, trace element for seven samples was carried out in an ICP-AES (ARCOS, Simultaneous ICP Spectrometer) at the Sophisticated Analytical Instrument Facility, Indian Institute of Technology, Bombay, adopting the following procedure, and discriminatory diagrams were plotted (Table 2, Figure 5). A 0.25 g of powdered sample was fused with 0.75 g lithium metaborate and 0.50 g lithium tetraborate in platinum crucibles at a temperature of 1,050°C in a muffle furnace. After cooling, the crucible was immersed in 80 ml of 1 M HCl contained in a 150 ml glass beaker and then magnetically stirred until the fusion bead dissolved completely. Then the sample volume was made up to 100 ml in a standard volumetric flask. The same procedure was adopted to make standard solutions and blank sample. The standards used for the analyses include BIR-1 (Basalt), BHVO-2 (Basalt), BCR-2 (Basalt), AGV-2 (Andesite), and GSP-2 (Granodiorite) (USGS Reference standards, 2005). Major and trace elements and LOI were estimated from the above solution by ICP-emission spectrometry.

Zircon U-Pb Geochronology
Zircon geochronology is performed on four granite and metarhyolite samples, collected one from each pluton (Sewariya pluton, near Bar, Figure 2A, Sample No TKB-1; Rupnagar metarhyolite, Sample No TKB-2; Pratapgarh pluton, Sample No TKB-3; Sumel pluton, Sample No TKB-4, Figures  2B,C). Textural study of zircon was carried out on CL images ( Figure 6). Magmatic zircon was distinguished by its euhedral shape with rings, from xenocrystic zircon that has irregular geometry (Biswal et al., 2007). A U-Pb isotope of the zircon was estimated on the SHRIMP ion microprobe at the John de Laeter Center for Mass Spectrometry at Curtin University in Perth, Australia. Zircon of all shapes and sizes was handpicked and mounted in epoxy resin together with natural zircon standard BR266 (Stern, 2001), TEMORA-2 (Black et al., 2003(Black et al., , 2004, and CZ3 (Pidgeon et al., 1994). The samples were loaded in the SHRIMP sample lock 24 h prior to analysis and pumped to ∼5 × 10-7 Torr to allow degassing. Analytical procedure of the SHRIMP follows methods as described in detail by Claoue-Long (1994). Working conditions for both sessions included a primary beam current of 2-3 nA, slightly elliptical spot size of ∼25-30 μm, the sensitivity of >20 counts per ppm Pb and per nA primary beam current, and a mass resolution of >4,500. Measurements were conducted on Zr2O+, 204Pb+, background, 206Pb+, 207Pb+, 208Pb+, 238U+, 232ThO+, and 238UO2 + in sets of six scans, with a total analysis time of about 15 min per sample spot. Analyses of unknown and BR266 standard zircon were interspersed at a ratio 3:1, allowing calibration of 238U/206Pb  ratios and U content using an age of 559 Ma and U content of 909 ppm (Stern, 2001). TEMORA-2 and CZ3 were used as control standards and yielded 206Pb/238U ages within the error of those reported for them (Pidgeon et al., 1994;Black et al., 2003Black et al., , 2004. Common Pb correction is based on measure nonradiogenic 204Pb isotope, and a common Pb composition applied following the Pb-evolution model of Stacey and Kramers (1975). Because analyses that recorded high counts on 204Pb during the first scan were aborted, corrections are small and insensitive to the choice of common Pb composition. Nevertheless, some analyses were characterized by very low contents of U, which, combined with the relatively young age, lead to low amounts of radiogenic Pb. In these cases, proportions of common Pb can become relatively high, even though counts on 204Pb were barely above background. Because of the low signalto-noise ratio of the 204Pb signal, 204-correction suffers from imprecision particularly in these cases, and we, therefore, report uncorrected ratios in the table (Table 3) and in some cases used these uncorrected values to regress the data to common Pb and constrain an intercept age. Standard calibration errors are reported in Table 3 but were not included in single spot ages and pooled age calculations. Single spot ages are reported at the 1σ confidence level, while pooled ages are reported at 95% confidence ( Figure 7).

Th-U-Total Pb Monazite Geochronology
Monazite geochronology was carried out on monazite grains in the mica schist samples (sample location in Figures 2B,C; BSE and X-ray images in Figures 8, 9, analytical data in Table 4). Monazite developed during metamorphism of the mica schist. Either a detrital monazite was recrystallized or elements like REE, Th, U, and P present in different minerals reacted in Ca poor condition producing monazite grains (Wawrzenitz et al., 2012). Crystallization of monazite occurred along with other minerals like quartz, feldspar, and biotite. The monazite grains have equant shape and are aligned parallel to S 1 fabric that results from dislocation creep, Sample No. B5 and R4 (cf. Passchier and Trouw, 2005). Subsequently, fluid action along the shear zone reprecipitates the monazite by dissolution precipitation creep (e.g., Wawrzenitz et al., 2012). Those monazites are elliptical in shape and aligned parallel to the mylonitic fabric, Sample No. CG1 and B4. Further, monazites undergo reprecipitation during brittle deformation due to fluid action and those monazites contain fractures. All these microfabrics of monazite in relation to host rock fabric were studied under BSE images and the events of crystallization/precipitation of monazite were identified.
Nine samples were analyzed, and 194 spot analyses were performed. Finally, we presented four representative samples (CG1, B4, B5, and R4) where the monazite shape could be unequivocally correlated with a particular deformation event. We used the Cameca SX-FIVE Electron Probe Micro-Analyzer (with five WDS spectrometers including LLIF and LPET crystals) for monazite geochronology, in the Department of Earth Sciences, IIT, Bombay. The single point/average method was used for finding the dates of the monazite grains (Montel et al., 1996). The age analyses were conducted at an   standards were used in calibrating major and trace elements in monazite. PbMa, ThMa, and UMb spectral lines were calibrated with crocoite (PbCrO4), Th glass (ThO2-5 wt.%), and U glass (UO2-5 wt.%) standards and simultaneously analyzed in two spectrometers for 240, 160, and 160 s, respectively, using subcounting methodology (cf. Spear and Wark, 2009;Prabhakar, 2013). The total counts of PbMa were acquired in the exponential mode to better define the distantly located background positions (Jercinovic and Williams, 2005;Jercinovic et al., 2008;Spear and Wark, 2009;Gonçalves et al., 2016). Background values for Th, U, Pb, and K are calculated from a nonlinear regression of high-precision wavelength dispersive scans (Jercinovic et al., 2008;Williams et al., 2006). Background values for the rest of the elements are based on linear interpolation of intensities between paired off-peak wavelength positions. The matrix effects (ZAF) were reduced with X-PHI method (Merlet, 1992 Pandey et al. (2013), and Tiwari and Biswal, (2019a). By applying these conditions, detection limit was achieved as 100 ppm for Th, 110 ppm for U, and 80 ppm for Pb. BSE images and X-ray mapping of all monazite grains in individual samples were documented. Individual domains were identified from such images, and two to three points in each domain were chemically analyzed ( Table 4). PbO vs. ThO 2 * diagram plotted (ThO 2 * measured ThO 2 plus ThO 2 equivalent   3 | (Continued) Zircon U-Pb SHRIMP data (2σ error of the mean of 0.94%) samples TKB-1 (26,015′50''/74,013′06″), TKB-2 (26,010′36''/74,017′30″), TKB-3 (26,012′24''/74,018′15″), and TKB-4 (26,013′36''/ 74,019′48″). of measured UO 2 ). Data points are arrayed linearly to provide an isochron; the slope of the line (m) is used to calculate the age of the event (Suzuki and Dunkley, 2014).

CG1
Geochemistry of the granites and metarhyolite can be summarized as the Pratapgarh pluton is meta-aluminous, I type, and emplaced in intraplate rift setting; metarhyolite is peralkaline, I type, and emplaced in intracontinental rift setting; these intruded during pre-D 1 stage. The Sewariya granite is peraluminous, S type, and emplaced in syncollisional setting, syn-D 1 .

Sample No. TKB-1
The sample is collected from the gneissic part of the Sewariya pluton near Bar, where high temperature solid state fabric is prominently developed (Figure 2A). The zircon crystals are subangular in shape. The CL image reveals oscillatory zoning patterns, consistent with magmatic zircon (Figure 6, textural details in Appendix). The isotopic data plot in a well-defined cluster on Concordia, with two analyses within that population plotting with larger errors and off Concordia, corresponding to the two analyses with the highest f 206 (Figure 7, TKB1-25, TKB1-26, TKB-1). The concordant points correspond to a Concordia age of 878 ± 9 Ma, which we take to be the best estimate for the emplacement age of the granitoid. One analysis, TKB1-14, plots well away from the Concordia age and corresponds to a darker CL zircon (Figure 6), with a 207 Pb/ 206 Pb age of 1,634 ± 22 Ma (2σ confidence, 101% concordant, Figure 7 TKB-1). This represents the xenocrystic component age.

Sample No. TKB-2
The sample is collected from Rupnagar metarhyolite ( Figure 2C). The rock is foliated with close spaced S 1 fabric. The zircon grains are dominantly subangular to subrounded. The CL image reveals oscillatory zoning patterns, consistent with magmatic zircon (Figure 6, textural details in Appendix). The data plot in a welldefined cluster on Concordia (Figure 7), with the exception of TKB-2-15 and TKB-2-17, which record the highest f 206 values and plot off Concordia. The concordant population of 27 zircons defines a Concordia age of 982 ± 3 Ma, which is the best approximation of the emplacement age of the granite protolith. The sample belongs to the Pratapgarh granite pluton ( Figure 2B). The zircon grains are subangular in shape, with some subrounded zircon. The CL image reveals relatively low response, with dark oscillatory zoning patterns, consistent with magmatic zircon (Figure 6, textural details in Appendix). Twenty-one analyses were conducted on twenty-one zircons and resulted in variable f 206 values between 0 and 21.7%. One zircon (TKB-3-16) recorded very high U and Th values, but the Uranium and Thorium content for all other zircons range between 100 and 1802 and 29 and 1,071 ppm, respectively (Table 3), resulting in Th/U ratios between 0.02 and 1.96. The lowest Th/U values were recorded on angular euhedral zircon with clear oscillatory patterns, and the overall range of Th/U values and CL patterns suggest the zircon to be magmatic in character. Two zircon grains record older 207 Pb/ 206 Pb ages, with the one near-concordant point (TKB-3-7) giving an age of 2,765 ± 18 Ma. These are considered to record some xenocrystic components in the granite protolith ( Figure 7). The remaining points plot along a Pb-loss trend anchored at an upper concordant cluster with a Concordia age of 992 ± 12 Ma (Figure 7). The Pb-loss pattern is consistent with present-day loss.

Sample No. TKB-4
The sample is collected from Sumel granite ( Figure 2C). The zircons range from euhedral crystals to irregular shape indicating the presence of various xenocrystic components. Faintly observable oscillatory zoning suggests magmatic growth ( Figure 6, textural details in Appendix). One analysis yielded an older age of ca 2,890 ±87 Ga, but plots slightly under Concordia (TKB-4-3, Figure 7). This grain is interpreted to reflect a xenocrystic component in the granite dyke. The remaining analyses mainly plot along a broad Pb-loss trend, with the highest U grains plotting inversely discordant ( Figure 7). The trend appears to be subparallel to Concordia and most likely related to ancient Pb-loss, possibly during intrusion of the regional granite suites or during subsequent metamorphism. The oldest cluster of concordant grains in the population and also the zircon with the lowest f 206 provide a Concordia age of 946 ± 18 Ma, which could reflect the emplacement age of the granite dyke. One zircon (TKB-4-7), analyzed twice during the session, provides a concordant data point at 270 ± 12 Ma and corresponds to a subangular zircon grain with faint sector zoning. This young grain would put the age of emplacement of the granite dykes at 270 Ma, with the older populations reflecting inheritance of ca. 950 Ma aged zircon, recording Pb-loss due to a metamorphic event either at or before 270 Ma. Zircon geochronology suggests that the granites of the study area were emplaced during two distinct periods, one at 992-946 Ma and the other at ca. 878 Ma ( Table 1). The former is pre-D 1 while the latter is syn -D 1 .

Sample No. CG1
The sample belongs to mica schist mylonite of the Phulad thrust. The mylonite is foliated containing dynamically recrystallized elliptical quartz grains arranged oblique to the mylonitic foliation; these oblique grains define mylonitic S foliation. The monazites are elliptical in shape and occur oblique to the C fabric indicating its synshearing recrystallization ( Figure 8A). The monazite grains contain domains; the lighter domain shows low Y and high Th values and produces an age of 813 Ma to 716 Ma ( Figures 8B-D). This age corresponds to D 2 events. The darker domain contains fractures and produces an age of ca. 590 Ma suggesting the age of brittle deformation event. Isochron plot and probability curve indicate three events 819-680-588 Ma and 811-700-569 Ma, respectively ( Figures 8E,F). The D 2 deformation and thrusting belong to ca 811-680 Ma and the brittle deformation is at ca. 588-569 Ma.

Sample No. B4
The sample is collected from pre-Delhi upper amphibolite facies slivers emplaced within Phulad thrust; there are several elliptical monazite grains aligned parallel to the mylonitic foliation ( Figures 8G,I). Grains are fractured along the edge and yield ages as ca. 706 Ma and 550 Ma ( Figure 8H), indicating age of the D 2 and D 4 brittle deformation events, respectively. In addition, several rounded grains ( Figure 8J) resembling the rounded garnet grains ( Figure 4C) occur in the rock. These monazite grains crystallized during pre-Delhi metamorphism and yield higher ages as 1,595 to 1,638 Ma. Isochron and probability curve indicate two age clusters ( Figures 8K,L). The pre-Delhi metamorphism is at ca. 1,611-1,609 Ma and the D 2 is at ca. 704-686 Ma.

Sample No. B-5
The sample is collected from the mica schist, west of Babra. The monazite grains are equant in shape with moderate to low ellipticity ( Figures 9A-D). They occur parallel to S 1 fabric in the rock and developed during D 1 -M 1 . It contains domains; the lighter domains, lying at the outer edge of the grain, are Y poor and Th rich and yield higher age as ca. 886 Ma while the darker domains, present in the center of the grain, show ages as ca. 783-597 Ma ( Figure 9B). Fracture along the grain margin channelized the fluid into the core of the grain resulting in rejuvenation of the age. There are three isochrons indicating as many events as 864 Ma for D 1 , 718 Ma for D 2 , and 588 Ma for brittle deformation ( Figure 9E). Probability graph indicates three peaks at ca. 846, 697, and 564 Ma ( Figure 9F), for D 1 , M 1 , and D 2 and brittle deformation events, respectively.

Sample No. R4
The sample is collected from the mica schist ( Figure 9G) close to the Pratapgarh. The monazite grains occur within biotite and are rounded to ellipsoidal with compositional domains ( Figures  9H-J). The Y low/high Th domains yield higher ages as ca. 863 Ma corresponding to D 1 -M 1 , and Y poor domains yield ca. 792 Ma corresponding to D 2 ( Figure 9H). The isochrons indicate two ages ca. 865 and 720 Ma ( Figure 9K) and probability curve contains peaks at ca. 852 and 743 Ma ( Figure 9L) corresponding to D 1 and D 2 , respectively. The result of the monazite geochronology can be summarized that the D 1 -M 1 is ca. 865 Ma; it continued up to 846 Ma. The D 2 is ca. 811-680 Ma and D 4 brittle deformation is ca. 588 to 564 Ma. The pre-Delhi deformation and metamorphism were at 1,638 Ma ( Table 1). The D 1 deformation age nearly coincides with D 1 age derived from zircon age of Sewariya granite (878 Ma). Combining these ages, we define the D 1 -M 1 age as 878-846 Ma. The D 2 event included both folding and thrusting. Therefor a spread in ages is indicated (811-680 Ma). Thrusting is marked by fluid flow and therefore resets the ages to ca. 680 Ma, in most cases. Therefore, we are taking ca. 680 Ma as the lower age limit for thrusting. The roll of D 3 deformation cannot be ruled out for such wide spread of ages. The age of D 4 deformation is at ca 588-564 Ma.

Tectonic Setting of Metarhyolite and Granite
The Chang, Sendra, and Pratapgarh plutons ( Figure 2C) intruded the calcareous schist and folded the surrounding rocks in the core of the SDT, showing similar geochemical character and isotopic age (Tobisch et al., 1994;Pandit et al., 2003, Tiwana et al., 2019present study). Previous studies by Pandit et al. (2003) and Tiwana et al. (2019) suggest that these are A2-subtype granites (cf. Eby, 1992) and are generated from subcontinental lithosphere or lower continental crust in postcollisional or postorogenic settings, perhaps during late-stage extensional collapse. Based on initial Sr isotope composition (0.710), the Chang pluton was suggested to be derived from basic magmatic source, produced from remelting of Archaean Banded Gneissic Complex in an Andean type magmatic setting (Pandit et al., 2003). The plutons were metamorphosed during South Delhi orogeny. Our study suggests that the Pratapgath granite is meta-aluminous, I type, and calc-alkaline ( Figure 5) and was produced from the remelting of basic igneous rocks at 750-800°C (zircon saturation temperature). Further, Rb, NB, and Y values indicate the granite to represent within plate magma intruded in intracontinental rift setting. These led to implication that the post-Aravalli (globally post-Columbia and Grenvillian) rifting of the Marwar Craton formed the South Delhi basin and granite was intruded in the basin in an extensional setting. Rupnagar metarhyolite was studied for the first time by us. It occurs as synsedimentary lava flows. Geochemical data indicates it is peralkaline, I type, and alkalic to alkali-calcic composition ( Figure 5). The Rb-Nb-Y and Na 2 O + K 2 O-(CaO + MgO) *5 Fe 2 O 3 (t) * 5 plot shows within plate magma intruded in a continental rift setting. This implies that the rifting of the Marwar Craton led to alkali volcanism in the South Delhi basin. The Sewariya pluton exhibits a different tectonic setting altogether. Previous study (Bhattacharjee et al., 1993;Ray et al., 2015;Sivasubramaniam et al., 2019) shows that the granite is peraluminous being produced from melting of Delhi metasediments at higher water pressure (3 kb) at 750°C by muscovite breakdown reaction in a subduction zone setting.
More peraluminous nature implies there is little contribution from mantle (Ray et al., 2015). Our study finds similar result as the granite is peraluminous, S type, more calcic, and syncollisional in nature ( Figure 5). However, some of the analysis lies in rift setting ( Figure 5F). Collision/subduction of the South Delhi Terrane resulted in the melting of the Delhi metasediments and produced such granite.

Life Span of South Delhi Orogeny
The South Delhi orogeny is constrained by multiple proxies as deformation, metamorphism, geochemistry, and geochronology of pre-and synorogenic granites and tectonometamorphic fabric. The study area is represented by greenschist facies rocks which are intruded by two phases of granites; the Sewariya granite is the youngest. All the plutons carry the imprint of D 1 deformation; hence the D 1 deformation cannot be older than Sewariya pluton. Geochemically it is S type and produced in a syncollisional setting. In addition, we have illustrated that the Sewariya pluton shows a transition from magmatic/submagmatic to solid state deformation fabric S 1 , from core to the margin. At the margin it shows perfect coupling with S 1 fabric in the host mica schist. This is an evidence of syntectonic (syn-D 1 -M 1 ) nature of granite intrusion. The granite yields a zircon age of ca. 0.87 Ga that marks the initiation of the South Delhi orogeny. We did the monazite dating of tectonometamorphic fabric which further constrains the D 1 -M 1 age at ca. 0.86-0.84 Ga. The D 2 event is constrained at ca. 0.81 to 0.68 Ga. Though D 3 event could not be dated, the spread in D 2 ages (nearly hundred years) may be partly due to the D 3 event. Considering all these ages, it is suggested that the South Delhi orogeny is ca. 0.87-0.68 Ga old and much younger than the Grenvillian orogeny (1.3 Ga to 1.0 Ga/ Li et al., 2008) and may be synchronous with early phase of Pan-African orogeny (ca. 0.9-0.7 Ga, Rogers and Santosh, 2002;Kroner and Stern, 2005;Rino et al., 2008;, Singh et al., 2010;Tiwari and Biswal, 2019a). The postorogenic brittle deformation in the SDT belongs to ca. 0.58-0.56 Ga that coincides with the period of Kuunga orogeny (0.65-0.5 Ga, Meert, 2003;Pradhan et al., 2009) representing the later part of Pan-African orogeny (Ambaji area, 0.76-0.65 Ga, Tiwari and Biswal, 2019b; Pali area, ca. 0.6 Ga, Bhardwaj and Biswal, 2019).
Our study shows a similarity with other parts of the SDT. The D 1 event was dated at ca. 0.87-0.86 Ga and thrusting at ca. 0.81-0.78 Ga from Ambaji area (Tiwari and Biswal, 2019a) and thrusting at ca. 0.81 Ga from Phulad area (Chatterjee et al., 2017). Further, on the eastern flank of the SDT near Srinagar, the granite bears post-0.98 Ga deformation imprint (Ruj and Dasgupta, 2014;Bose et al., 2017). The Sirohi Terrane in the west of SDT shows a deformation age between 0.89 and 0.8 Ga (Arora et al., 2017).
Earlier view that the South Delhi orogeny is Grenvillian comes from 1.0 Ga age of Pratapgarh, Sumel, Chang, and Sendra plutons (0.98 Ga, Tobisch et al., 1994;0.96 Ga/Pandit et al., 2003;0.97 Ga/ Tiwana et al., 2019), but geochemistry of these granites suggests that these are I type, produced from remelting of basic rocks, and intruded in postorogenic intracontinental extensional setting. The granites lack magmatic fabric, deformed by all phases of deformation as the metasediments and metamorphosed in greenschist facies. The plagioclase and K-feldspar retained their magmatic habit. Based on these we interpret that these plutons are preorogenic to SDT and intruded at the time of rifting of South Delhi basin. As far as age of rifting and sedimentation are concerned, previous study on SDT constrained it at ca. 1.7-1.0 Ga (Wang et al., 2014) and ca. 1.2-0.86 Ga (Singh et al., 2010). Our study on the Rupnagar metarhyolite that stands as an unequivocal evidence of synsedimentary bimodal volcanism like many in the SDT (Bhattacharjee et al., 1988) provides an age of 0.98 Ga that lies within the above age range. Thus, the rifting and formation of South Delhi basin overlap with Rodinia amalgamation event (ca. 1.3-0.9 Ga). Hence, while many continents were experiencing orogenic event, the SDT was undergoing rifting.
Another viewpoint that advocates the South Delhi orogeny to be Grenvillian is the 1.0 Ga metamorphic imprint on 1.7-1.5 Ga old granulite of the Pilwa-Chinwali area. As these outcrops occur in the north of the study area Bhowmik et al. (2018) considered the granulite to be part of SDT. However, Fareeduddin et al. (1994) suggested the granulite to be pre-Delhi and belongs to Sandmata Terrane. Our finding suggests that the upper amphibolite grade slivers of ca. 1.6 Ga (equivalent to Pilwa-Chinwali granulite) occur within SDT as tectonic inclusions along the Phulad thrust. The mineral assemblage is in sharp contrast with the surrounding mica schist. We suggest that the Pilwa-Chinwali granulite represents basement for the SDT and it has been exhumed by thrusting and normal faulting along Govindgarh-Jethana fault. Further, the xenocrysts in the Pratapgarh and Sewariya granites yield similar ages (ca. 1.6 Ga, 2.7 Ga, and 2.8 Ga). Furthermore, the Beawar gneiss occurs as exhumed basement block to the east of the study area and shows the age as ca. 0.8 Ga, 1.0 Ga, 1.6 Ga, and 2.8 Ga old (Kaur et al., 2020). Hence 1.0 Ga metamorphic event is an event in the basement not in the SDT.

South Delhi Orogeny in Relation to East Gondwana Tectonics
The East Gondwana includes much of the continents of Australia, India, and Antarctica, which underwent several phases of amalgamation and separation in the Proterozoic period (Fitzsimons, 2000;Collins and Pisarevsky, 2005;Pradhan et al., 2009). It was not a coherent mass during much of Rodinia and Gondwana amalgamation; they finally joined together in Neoproterozoic-Cambrian period in bits and pieces. Thus, individual continents in the assembly were not even completely amalgamated; this is proven from India (Collins and Pisarevsky, 2005). For example the Eastern Ghats Mobile Belt provides evidence for final suturing between India and Antarctica during Cambrian (ca. 0.51 Ga/ Biswal et al., 2007). The present study on SDT points to amalgamation of Marwar Craton with Bundelkhanda Craton during Neoproterozoic (ca.0.87 Ga). Based on our finding we are proposing a model for the SDT in reference to amalgamation of Rodinia and Gondwana, using the reconstruction of Supercontinents proposed by several researchers (Figure 10, cf. Powell and Pisarevsky, 2002;Li et al., 2008;Meert et al., 2013;Johansson, 2014;Pisarevsky et al., 2014;Oriolo et al., 2017).
i. Before 1.0 Ga ( Figure 10A): At 1.2 Ga India was in the polar latitude (Pradhan et al., 2009) as a separate landmass, away from Rodinia Supercontinent. By then, the Dharwar Craton of India was separated from Sarmatia at 1.3 Ga, the eastern margin of India was not connected to Antarctica and Australia, and the Marwar Craton, Madagascar, and Syechelles were bordering the western margin of India (Pisarevsky et al., 2013). The Arabian-Nubian shield was located to the south ( Figure 10). ii. Ca. 1.0-0.9 Ga ( Figure 10B): Grenvillian orogeny took place, consequently India amalgamated with Antarctica, the Eastern Ghats Mobile Belt and Rayner Complex formed through subduction and collision (Dasgupta et al., 2013), and in turn Antarctica and Australia amalgamated with the Laurentia completing the assembly of the Rodinia. Thus Eastern Ghats Mobile Belt is considered to be a Grenvillian Mobile Belt. Further, the NW India witnessed discrete metamorphic events, e.g., Sandmata Terrane (Bhowmik and Dasgupta, 2012) and North Delhi Terrane (Pant et al., 2008) of the ADMB. Following this, the NW India underwent extension and rifting reflecting a top-down process (e.g., Cawood et al., 2016). iii. After Rodinia ( Figure 10B inset-1): Extension led to rifting in the Marwar-Aravalli-Bhilwara-Bundelkhanda Craton in NW India forming South Delhi basin. A simple shear extension model (cf. Wernicke, 1985) with westward inclined detachment probably created the South Delhi basin (Biswal et al., 1998a, b). In the simple shear model, the rotation of the faulted blocks is easier due to listric nature of the detachment fault which is steeper at the surface and gradually becomes gentler and horizontal at brittle-ductile boundary. This type of model has been applied to Basin and Range province, Bay of Biscay, and northwestern European continental shelf (Montadert et al., 1979;Kusznir et al., 1987;Lister et al., 1991). However, a pure shear model as proposed by McKenzie (1978) cannot be ruled out. In the pure shear model, lithospheric stretching takes place through conjugate planar faults. The slips along conjugate faults oppose each other (Ramsay and Huber, 1987) which is not there in a listric detachment fault postulated in the simple shear model. However, mechanism of basin formation is beyond the scope of the paper. The sediments were deposited in fault-bounded basin. Thick erosional unconformity with conglomerate formed at several parts of the SDT. Biomodal volcanism produced rhyolite and basalt flows (Rupnagar metarhyolite) which are dated at ca. 0.98 Ga in the study area. Granites emplaced in extension setting, namely, Bilara granite and Sendra-Chang-Pratapgarh-Sumel plutons at ca. 1.0-0.9 Ga. With progressive lithospheric stretching, the MOR developed on the east ( Figure 10C inset −1); the Phulad ophiolites, Ranakpur diorite, and Sirohi plagiogranite (ca. 1.0 Ga, Volpe and Macdougall, 1990;Dharma Rao et al., 2013) were part of the oceanic crust. This represents the introversion tectonics as the juvenile crust formed out of such rifting is younger than the age of the breakup (cf. Murphy and Nance, 2013). iv. Rodinia breakup and South Delhi orogeny (0.88-0.65 Ga, Figure 10C). Rodinia broke up and India was detached from Antarctica and Australia along Eastern Ghats and was placed near the north pole by 0.82 Ga (Powell and Pisarevsky, 2002). Breakup of Rodinia gave rise to the opening of major oceans, namely, Mozambique Ocean ( Figure 10C) and Iapetus Ocean ( Figure 10D) (e.g., Cawood et al., 2001;Meert and Torsvik, 2003;Li et al., 2008). However, the SDT witnessed subduction/collision between Bundelkhanda + Aravalli Craton and Marwar Craton. The oceanic crust was subducted westward forming continental arc with granite magmatism ranging in ca 0.87-0.76 Ga ( Figure 10C, inset 1,2) (Erinpura granite, Ambaji granite, and Sewariya granite, Malani Igneous Suite; Sinha Roy, 1988;Sugden et al., 1990;Synchanthavong and Desai, 1977;Biswal et al., 1998b;Singh et al., 2010). Possibly, the detachment zone in the basin converted to a northwesterly dipping subduction zone/collision zone. Seismic reflection data support a NW dipping thrust plane at the contact between SDT and Sandmata Terrane (Satyavani et al., 2004). The magmatic arc was extending upto Madagascar in the south (Singh et al., 2010) and South China in the north (Zhao et al., 2018) as indicated by the presence of similar age granite (ca. 0.7 Ga, Singh et al., 2010) in those far-off continents ( Figure 10C). The Marwar Craton, which was forming the overriding plate, was completely metacratonized by intrusion of these granitic rocks. The metacratonization was so extensive that Archean outcrops are hardly survived in Marwar Cratonic domain; the Azania block in Madagascar may be the survived part of extensive Marwar Craton (Singh et al., 2010). Along the magmatic arc, several low grade metasedimentary outcrops (roof pendants) occur within expansive granite outcrops, which constitute the Sirohi Terrane ( Figure 1B). With progressive subduction/collision, compression led to exhumation of rocks at 0.81-0.68 Ga by thrusting (cf. Tiwari and Biswal, 2019a). The SDT is marked by pro-as well as retro-wedge thrust belts (cf. Naylor and Sinclair, 2008). The study area Beawar-Babra sector belongs to retrowedge thrust belts while the eastern part around Shyamgarh ( Figure 2A) belongs to pro-wedge thrust belt, together forming a doubly-vergent orogen (Hahn et al., 2020) v. The SDT type Tonian-Cryogenian (1.0-0.72 Ga) rifting occurred between landmasses in the West Gondwana (Oriolo et al., 2017). The Arabian-Nubian shield shows signature of ca. 0.88-0.7 Ga accretion of island arcs and juvenile crust (Kroner and Stern, 2005); the Dahomey Belt has subduction with associated back-arc extension and development of island arc (Ganade et al., 2016); Borborema Province has ca. 0.85-0.75 Ga juvenile material (Ganade de Araujo et al., 2014) and the São Gabriel Block has ca. 0.9-0.7 Ga old intraoceanic subduction (Fortes de Lena et al., 2014). vi. Ca.0.6-0.53 Ga (Amalgamation of Gondwana Supercontinent): Collision and strike-slip shearing led to amalgamation of different Gondawana blocks along Pan-African orogens ( Figure 10D). The Mozambique ocean closed through Kuunga orogeny (0.65-0.5 Ga), bringing together the West and East Gondwana continents along East African Orogen ( Figure 10D, Collins and Windley, 2002;Meert, 2003). India initially joined with Australia at ca. 0.6 Ga through strike-slip shearing (Powell and Pisarevsky, 2002) and later at 0.53 with Antarctica through collision. The Eastern Ghats Mobile Belt thrusts over Bastar Craton along the terrane boundary shear zone at 0.51 Ga (TBSZ, Biswal et al., 2007). During this period, the SDT experienced extensional tectonics ( Figure 10D inset-1) that produced several prominent faults, namely, Kui-Chitraseni fault, Surpagla-Kengora fault, and Govindgarh-Jethana fault. Extensional basins like Sindreth and Punagarh developed in the intra-arch region ( Figure 10C, inset-3, cf. Schobel et al., 2017). The brittle tectonics in the ADMB continued till the breakup of Gondwana. The N-S fractures that host 0.27 Ga pegmatite veins in the study area probably belong to Gondwana breakup period.

CONCLUSION
(1) We applied the tectonic fabric and geochemistry of the granite and metarhyolite in combination with zircon and monazite geochronology to date the South Delhi orogeny. The Pratapgarh-Sumel granite plutons intruded in extensional setting during rifting, Rupnagar metarhyolite extruded during sedimentation, and all these yielded an age of ca. 992-946 Ma. The Sewariya granite is syncollisional and produced an age of ca. 878 Ma. It is syntectonic with D 1 as indicated by coplanar attitude of magmatic Sm and S 1 fabrics. The monazite geochronology estimated the age of D 1 -M 1 metamorphism at 865-846 Ma, the D 2 at 810-680 Ma, and brittle deformation D 4 at 588-564 Ma. We suggest that the South Delhi orogeny is ca. 878 to 680 Ma old and coeval with early part of the Pan-African orogeny.
(2) The South Delhi orogeny brought amalgamation of the Marwar Craton with Aravalli-Bhilwara-Bundelkhanda Craton that led in process to forming a united Indian FIGURE 10 | Synchronously, the South Delhi basin closed by subduction/collision, to form SDT, pro-and retro-wedge thrust belts formed. The study area belongs to retro-wedge part (C, insets 1, 2, 3, model of subduction, collision, and extension, cf. Allen and Allen, 2013) subcontinent, in the East Gondwana assembly. This strengthens the view that the East Gondwana blocks were sutured in bits and pieces till Neoproterozoic-Cambrian period. (3) The Marwar Craton was extensively metacratonized by ≤878 Ma granites during South Delhi orogeny so that the Archaean rocks are totally lost from the cratonic domain. Similar metacratonization is also observed in Mangalwar and Sandmata terranes during Aravalli orogeny. Migmatization of Archean rocks and intrusion of charnockitic magma completely reset the age of the rocks in those terranes to Mesoproterozoic.

DATA AVAILABILITY STATEMENT
The original contributions presented in the study are included in the article/Supplementary Material, further inquiries can be directed to the corresponding authors.