Abstract:Geomorphological study of some of the just more than 200 known terrestrial impact structures has demonstrated that despite extensive degradation, important geomorphological keys, such as drainage pattern, topographic signatures, erosional landforms, and depositional features, can still be assessed. They can provide possible indicators to assist in the recognition of further impact structures, especially on Precambrian shields and cratonic landmasses. This study documents the surface features and landforms of t… Show more
“…The impact melt rocks of the Dhala impact structure show minor postimpact alteration (Pati et al., 2010; Singh et al., 2021a). However, these postimpact hydrothermal events do not significantly affect the magnetic fabrics of the impact melt rock (Singh et al., 2021b).…”
Section: Discussionmentioning
confidence: 99%
“…These fractured basement granitoids possess a ∼12 m thick suevite horizon in between (Pati et al., 2019). The fractured target basement of the Dhala impact structure contains about 201 large to small outcrops of the monomict lithic breccia (Singh et al., 2021b), which spread over an area of about 45 km 2 in the outermost annular zone of the Dhala impact structure. The fractured target basement is overlain by the impact melt rock.…”
We investigate the magnetic fabrics and magnetic mineralogy of the impact melt rock at the Dhala impact structure to understand its emplacement mechanism. Pseudo‐single domains of Ti‐poor magnetite and Ti‐hematite are the prime magnetic carriers in the impact melt rock. The magnetic foliations show a range of dip amounts. The overall trend of the magnetic foliation of the impact melt rock draws a resemblance with the flood basalts or lava flows. A well‐developed magnetic lineation (K1) indicates the strong alignment of Ti‐poor magnetite grains. Therefore, the magnetic carriers may have crystallized and aligned themselves along the flow direction before the emplacement. It may be possible that after the crystallization of the magnetic carriers, the impact melt moved in a semi‐molten state similar to lava flows with temperatures below c. 1,500°C, which is the melting point of Ti‐magnetite and was emplaced as crater‐fill deposits. Among the three principal magnetic susceptibility axes, K1 aligns best with the mesoscopic flow indicators. K1 of individual specimens' trends between NW and SW, while the mean K1 at all the sites trends westward. Thus, at the studied sites, the impact melt flow was dominantly eastward. In the sites located to the NW and W, the eastward flow could be due to gravity‐driven crater inward flow toward the center. At site IM2, which is located to E, the eastward flow of the impact melt is possibly due to crater outward excavation flow.
“…The impact melt rocks of the Dhala impact structure show minor postimpact alteration (Pati et al., 2010; Singh et al., 2021a). However, these postimpact hydrothermal events do not significantly affect the magnetic fabrics of the impact melt rock (Singh et al., 2021b).…”
Section: Discussionmentioning
confidence: 99%
“…These fractured basement granitoids possess a ∼12 m thick suevite horizon in between (Pati et al., 2019). The fractured target basement of the Dhala impact structure contains about 201 large to small outcrops of the monomict lithic breccia (Singh et al., 2021b), which spread over an area of about 45 km 2 in the outermost annular zone of the Dhala impact structure. The fractured target basement is overlain by the impact melt rock.…”
We investigate the magnetic fabrics and magnetic mineralogy of the impact melt rock at the Dhala impact structure to understand its emplacement mechanism. Pseudo‐single domains of Ti‐poor magnetite and Ti‐hematite are the prime magnetic carriers in the impact melt rock. The magnetic foliations show a range of dip amounts. The overall trend of the magnetic foliation of the impact melt rock draws a resemblance with the flood basalts or lava flows. A well‐developed magnetic lineation (K1) indicates the strong alignment of Ti‐poor magnetite grains. Therefore, the magnetic carriers may have crystallized and aligned themselves along the flow direction before the emplacement. It may be possible that after the crystallization of the magnetic carriers, the impact melt moved in a semi‐molten state similar to lava flows with temperatures below c. 1,500°C, which is the melting point of Ti‐magnetite and was emplaced as crater‐fill deposits. Among the three principal magnetic susceptibility axes, K1 aligns best with the mesoscopic flow indicators. K1 of individual specimens' trends between NW and SW, while the mean K1 at all the sites trends westward. Thus, at the studied sites, the impact melt flow was dominantly eastward. In the sites located to the NW and W, the eastward flow could be due to gravity‐driven crater inward flow toward the center. At site IM2, which is located to E, the eastward flow of the impact melt is possibly due to crater outward excavation flow.
“…The annular region between the CEA and the monomict breccia ring is mainly occupied by sub‐horizontal intercalated purplish‐brown siltstone and greenish‐white sandy siltstone, together with pockets of conglomerate lenses within a clastic matrix (Pati, Reimold, et al., 2008). Despite the prolonged erosion and multiple post‐impact tectono‐thermal activities in the region, the impactites of the Dhala structure are relatively well preserved as revealed by the field observations (Pati et al., 2010; Singh et al., 2021). The presence of shatter cones, impact‐diagnostic microscopic shock metamorphic features, and the chemical signature of extraterrestrial components within impact melt breccia also confirmed the well‐shielded nature of the Dhala structure (Pati et al., 2019 and references therein).…”
Section: Geological Setting Of the Dhala Impact Structurementioning
confidence: 98%
“…Nevertheless, the precise age of the Dhala impact event is not determined so far and is stratigraphically constrained between 2.5 and 1.7 Ga corresponding to the ages of the target granitoids and the post‐impact sediments of the Vindhyan Supergroup, respectively (Pati et al., 2010). In the Dhala area, the CEA is surrounded by a ring of >200 monomict breccia outcrops occurring in the outermost annular region of the structure (Singh et al., 2021). These breccia bodies mostly comprise sheared, fractured, and extensively brecciated fragments of the target rocks.…”
Section: Geological Setting Of the Dhala Impact Structurementioning
The Dhala structure in north-central India is a confirmed complex impact structure of Paleoproterozoic age. The presence of an extraterrestrial component in impactites from the Dhala structure was recognized by geochemical analyses of highly siderophile elements and Os isotopic compositions; however, the impactor type has remained unidentified. This study uses Cr isotope systematics to identify the type of projectile involved in the formation of the Dhala structure. Unlike the composition of siderophile elements (e.g., Ni, Cr, Co, and platinum group elements) and their inter-element ratios that may get compromised due to the extreme energy generated during an impact, Cr isotopes retain the distinct composition of the impactor. The distinct e 54 Cr value of À0.31 AE 0.09 for a Dhala impact melt breccia sample (D6-57) indicates inheritance from an impactor originating within the non-carbonaceous reservoir, that is, the inner Solar System. Based on the Ni/Cr ratio, Os abundance, and Cr isotopic composition of the samples, the impactor is constrained to be of ureilite type. Binary mixing calculations also indicate contamination of the target rock by 0.1-0.3 wt% of material from a ureilite-like impactor. Together with the previously identified impactors that formed El'gygytgyn, Zhamanshin, and Lonar impact structures, the Cr isotopic compositions of the Dhala impactites argue for a much more diverse source of the objects that collided with the Earth over its geological history than has been supposed previously.
“…One of the most interesting landforms in the Bundelkhand craton in peninsular India is the Dhala impact crator, which has attracted the attention of geologists for several decades (Pati et al, 2008(Pati et al, , 2015(Pati et al, , 2017Sinha et al, 2011). In the most recent paper, Singh et al (2021) have documented the surface features and landforms of the Dhala crator. With an age bracketed between 1.7 and 2.5 Ga, the Dhala is The use of fractals should add a new dimension to understand the complex interaction of various geologic and geomorphic processes in topographic evolution.…”
This commentary is designed to highlight the recent contributions on Indian geomorphology that have been published in Earth Surface Processes and Landforms (ESPL). A large number of papers included in this commentary have been published as part of the special issue on Indian geomorphology. However, I have taken the liberty of including a few others that appeared in ESPL in the last couple of years. These papers have covered a variety of topics ranging from erosion rates in Himalayan basins, miliolites in peninsular India, flood risk, connectivity concept, socio‐hydrology, and paleoclimatic reconstruction from lake sediments. They have also utilized a wide range of methodologies and tools including fractals, remote sensing, cosmogenic nuclides, and modelling. It is hoped that this commentary will put the diversity of Indian geomorphology in the correct perspective and will encourage geomorphologists across the world to continue their excellent research.
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