Proc Indian Natn Sci Acad 86 No. 1 March 2020 pp. 245-261
Printed in India.
DOI: 10.16943/ptinsa/2020/49791
Status Report 2016-2019
Contemporary Researches and Issues Related to the Deccan Volcanism
AMIT KUMAR, SUCHARITA PAL and J P SHRIVASTAVA*
Department of Geology, University of Delhi, Delhi 110 007, India
(Received on 31 August 2019; Accepted on 30 September 2019)
In the past few decades, late Cretaceous Deccan volcanism witnessed extensive researches, focused on nature, variety and
genesis of magma, emplacement span [entail Cretaceous /Palaeogene (K/Pg) transition] and attendant faunal crisis; however
several issues remain to be addressed. In this gamut, researches in the past five years have been reviewed, encompassing
petrochemical, Nd-Sr-Pb isotopic, and geochronology studies to comprehend origin, age and duration of volcanism and
attendant K/Pg transition events. Low/high TiO2 tholeiites of Deccan Traps and associated rocks from a rifted basin
revealed existence of varied mantle sources for synchronously formed tholeiitic and alkaline magma involved sub-continental
lithospheric mantle. Moreover, later magma type ascended with faster rate through the lithosphere and subsequently led to
rapid gaseous release, accounted for the Cretaceous/Palaeogene boundary (KPB) mass extinction. Flow-by-flow
palaeomagnetic measurements for the Mandla basalt revealed multiple magnetic polarity events: implying for C29n-C28rC28n magnetostratigraphy.
40Ar/39Ar
ages for Mundwara and Sarnu-Dandali complexes assign polychronous emplacement, concomitant with the
post-breakup of Indo-Madagascar. Both complexes show comparable evolution from early to late Cretaceous Period. U-Pb
zircon age data based Deccan eruption rates when combined with the Chicxulub impact triggered seismicity, inferred four
major eruptive phases, each lasted for ≤100 ka. In the second eruptive phase, Poladpur Formation eruption began tens of
thousands of years before, but peaked out at K/Pg mass extinction event. Consequently, carbonate dissolution, climatic
cooling and late Maastrichtian global warming attendant to Deccan volcanism, induced ocean acidification which led to high
environmental stress worldwide. Present review also covers applied aspects, including CO2 sequestration in Deccan basalt
and suitability of silicic phase for nuclear waste disposal. Additionally, it ends-up with a note on future direction of
researches in Deccan basalt.
Keywords: Deccan Volcanism; Cretaceous/Palaeogene Boundary; Palaeoenvironment;
Inter-Trappeans
Introduction
The Deccan Volcanic Province (DVP) represents one
of the largest Continental Flood Basalt (CFB)
provinces in the world (cf. 1.6, Ernst, 2014), covering
an area of 0.51 × 106 km2 (Fig. 1), which records
vast accumulation of basalt in a relatively short time
span entailing the Cretaceous/Paleogene boundary
(KPB). The Deccan volcanic activity initiated prior
to the KPB, however, main episode occurred at ~300
ka prior to or at the KPB itself (Schoene et al., 2015).
Lithospheric versus asthenospheric contributions to
Deccan Traps when compared to the Ethiopia-Yemen
and Karoo continental flood basalt revealed similar
parental magmas and fractionation trends (Natali et
*Author for Correspondence: E-mail:
[email protected]
40Ar/39Ar
Ages; Infra-
al., 2016). Such continental flood basalt represents
similar zonal arrangement for the hottest and deepest
picrite-basalt magmas in the central area and cooler
and shallower basalts at the peripheral areas. Further,
superheated picrite-basalt supposedly coeval with the
alkaline-carbonatite complexes and rhyolitic
differentiates often lie at the intersection of extensional
lineaments and at the top of picrite-basalt lavas,
respectively. Additionally, more or less unaffected
mantle Sr-Nd isotopic values of picrate-basalt together
with the lithospheric values of the peripheral basalt
marked common geodynamic setting (Natali et al.,
2016).
One of the thickest (~ 1.5 km) Deccan Traps
246
Amit Kumar et al.
Fig. 1: Studies on Deccan volcanic province (green shaded area) carried out in the past five years shown with bold numbers
enclosed within the parentheses. Work responsibility: (1) Shrivastava et al. (2015), (2) Parisio et al. (2016), (3) Font et al.
(2016), (4) Pande et al. (2017), (5) Sheth et al. (2017), (6) Schoene et al. (2017), (7) Shrivastava et al. (2017), (8) Sheth et al.
(2018), (9) Cucciniello et al. (2018), (10) Schoene et al. (2019), (11) Chatterjee and Sheth (2015), (12) Petersen (2015), (13)
Rani et al. (2015), (14) Richards et al. (2015), (15) Widdowson et al. (2015), (16) Ray et al. (2016), (17) Rani et al. (2016), (18)
Natali et al. (2016), (19) Pathak et al. (2016), (20) Sheth (2016), (21) Shrivastava et al. (2016), (22) Alexander and Purohit
(2019), (23) Mishra et al. (2017), (24) Sinha et al. (2017), (25) Kumar et al. (2017), (26) Vedanti et al. (2018), (27) Kumar and
Shrivastava (2019), (28) Prasanth et al. (2019), (29) Pal et al. (2015a), (30) Pal et al. (2015b), (31) Punekar et al. (2015), (32)
Keller et al. (2017), (33) Chenming and Demin (2018), (34) Sprain et al. (2019) and (35) Renne et al. (2019). Note: references
in italics refer to studies carried out on Deccan volcanism
Contemporary Researches and Issues Related to the Deccan Volcanism
accumulation occurs in the Mahabaleshwer area of
Western Deccan Volcanic Province (WDVP). In
Koyna-Warna-Panchgani area, Sinha et al. (2017)
and Mishra et al. (2017) reported 932 and 1251 m
thick sub-surface lava packages, comprised of 30 and
46 lava flows, respectively. Although, stratigraphy of
the lava flows, age and duration of volcanism in the
Koyna-Warna-Panchgani area needs to be correlated
with special reference to the main WDVP.
Petrophysical and elastic studies of Vedanti et al.
(2018) on 338 m thick sub-surface basalt package
from Killari (KLR-1) borehole revealed presence of
FeO (~13.4 wt%) rich and SiO2 (47.8 wt%) poor
Ambenali and Poladpur-like lava flows, characterized
by a mean density of 2.91 g/cm3 and P, S wave
velocities of 5.89 and 3.43 km/s, respectively. Overall,
low velocity of P, S waves observed in this sequence
is ascribed to energy loss and intrinsic attenuation due
to the prolific glass and high Fe contents and their
intensely altered nature. Although, high order of
attenuation is also noticed in few massive basalt types,
either glassy or contain high proportion of chlorophaeite
and other secondary silicates. Activities were mainly
focused on Deccan volcanism and related fields (Fig.
1) and produced vast information (Table 1), however,
to identify forthcoming research problems, an attempt
has been made to review significant research
contributions published in the journals of national and
international repute in last five years. Outcome of the
work is summarized and discussed under subsequent
sections:
247
central part, whereas, later occurs in the form of subhorizontal flows in the southern part of the Kutch
basin. Alkaline and tholeiitic magma types require
varied degree of partial melting and mantle sources,
however in a mantle plume scenario; alkaline
magmatism precedes and possibly follows the main
phase of tholeiitic magmatism. Parisio et al. (2016)
established existence of varied mantle sources for
the synchronously formed alkaline and tholeiitic
magmas and require sub-continental lithospheric
mantle involvement at the time of Deccan magmatism.
Both alkaline and tholeiitic magmatism occurred during
early and late phases, therefore, their derivation from
same mantle source is highly unlikely. Ray et al. (2016)
reported disc-shaped spinel peridotite mantle xenolithxenocrysts (of spinel lherzolite and spinel wehrlite
compositions) bearing monogenetic alkali basaltic plugs
(few connected to feeder dykes) and tholeiitic basalt
lava flows from the fault controlled uplifted block of
the Kutch basin. These observations were supported
by prolifically present feeder dykes (with greater
width) which contain large xenocrysts and xenoliths
with thick alteration aureole around olivine xenocrysts.
Commonality in the chemico-mineralogical attributes
of these isolated alkali basalt is suggestive of cogenetic nature, implying for a common source, age
and eruption mechanism. Alkali basalt contains,
fractured olivine (Fo>90) fragments (Figs. 2 and 3)
with embayed margins as xenocryst and less forsteritic
(~Fo80) olivine grains as phenocrysts (compared to
groundmass grains). Alkali magma ascended through
Tholeiitic and Alkali Basalt-Carbonatite
Associations
The DVP dominantly composed of tholeiitic basalts
(with a minor amount of alkaline, carbonatite, and silicic
rocks) and is sub-divided into low (TiO2 < 2.5; Ti/Y <
500) and high (TiO2> 2.5; Ti/Y > 500) Ti basalt types
and inferred involvement of multiple mantle
components assigning derivation from the depleted
mantle sources (Prasanth et al., 2019). Alkaline rocks
are commonly associated with the rift zones. Most of
the researches carried out in the past five years were
focused on the pericratonic rift basin in the Kutch
area of northwestern India (Ray et al., 2016;
Cucciniello et al., 2018). Both alkali and tholeiitic
basalt types occur together in this area. Former is
cropping out as an isolated, relatively small, eroded,
cinder cone-like volcanic plugs within a linear belt in
Fig. 2: Photomicrograph of olivine (Ol) with alteration veins
and melt inclusions (MI). Source: Chatterjee and
Sheth (2015)
248
Amit Kumar et al.
Table 1: Location-wise summarized published work on Deccan volcanism and related fields
Locations
Summary of the work done
References
Dating
1.
Post-K/PB younger 40Ar-39Ar ages of the Mandla lavas: Implications for the duration of Shrivastava et al. (2015)
the Deccan volcanism,
2.
40Ar/39Ar ages of alkaline and tholeiitic rocks from the northern Deccan Traps:
implications for magmatic processes and the K-Pg boundary
Parisio et al. (2016)
3.
Mercury anomaly, Deccan volcanism, and the end-Cretaceous mass extinction
Font et al. (2016)
4.
40Ar/39Ar
dating of the Mumbai tholeiites and Panvel flexure: intense 62.5Ma onshoreoffshore Deccan magmatism during India-Laxmi Ridge-Seychelles breakup
Pande et al. (2017)
5.
Recurrent Early Cretaceous, Indo-Madagascar (89-86 Ma) and Deccan (66 Ma) alkaline
magmatism in the Sarnu-Dandali complex, Rajasthan: 40Ar/39Ar age evidence and
geodynamic significance
Sheth et al. (2017)
6.
U-Pb geochronology of the Deccan Traps and relation to the end-Cretaceous mass
extinction
Schoene et al. (2015)
7.
Feeder and post Deccan Trap dyke activities in the northern slope of the Satpura
Mountain: Evidence from new 40Ar-39Ar ages
Shrivastava et al. (2017)
8.
Geochemistry and 40Ar/39Ar geochronology of the Nandurbar Dhule mafic dyke swarm: Sheth et al. (2018)
Dyke sill flow correlations and stratigraphic development across the Deccan flood
basalt province
9.
Mineralogy, geochemistry and 40Ar-39Ar geochronology of the Barda and Alech
complexes, Saurashtra , northwestern Deccan Traps: early silicic magmas derived by
flood basalt fractionation
Cucciniello et al. (2018)
10.
U-Pb constraints on pulsed eruption of the Deccan Traps across the end-Cretaceous
mass extinction
Schoene et al. (2019)
Petrology and Geochemistry
11.
Origin of the Powai ankaramite, and the composition, P-T conditions of equilibration
and evolution of the primary magmas of the Deccan tholeiites
Chatterjee and Sheth (2015)
12.
End-Cretaceous extinction in Antarctica linked to both Deccan volcanism and meteorite
impact via climate change
Petersen (2015)
13.
Natural glass from Deccan volcanic province: an analogue for radioactive waste form.
Rani et al. (2015)
14.
Triggering of the largest Deccan eruptions by the Chicxulub impact
Richards et al. (2015)
15.
The geochemistry of Indian bole horizons: palaeoenvironmental implications of
Deccan intravolcanicpalaeosurfaces
Widdowson et al. (2015)
16.
Mantle xenolith-xenocryst-bearing monogenetic alkali basaltic lava field from
Kutch Basin, Gujarat, Western India: Estimation of magma ascent rate
Ray et al. (2016)
17.
Long-term performance assessment of nuclear waste and natural glasses in the
geological repository: A geochemical modelling
Rani et al. (2016)
18.
Comparison among Ethiopia-Yemen, Deccan, and Karoo continental flood basalts
of central Gondwana: Insights on lithosphere versus asthenosphere contributions
in compositionally zoned magmatic provinces
Natali et al. (2016)
19.
Tectonomagmatic setting of lava packages in the Mandla lobe of the eastern Deccan
volcanic province, India: palaeomagnetism and magnetostratigraphic evidence
Pathak et al. (2016)
20.
Giant plagioclase basalts: Continental flood basalt-induced remobilization of
anorthositic mushes in a deep crustal sill complex
Sheth (2016)
21.
Geochemical Modeling and Experimental Studies on Mineral Carbonation of Primary
Silicates for Long-term Immobilization of CO2 in Basalt from the Eastern Deccan
Volcanic Province
Shrivastava et al. (2016)
22.
At last! Giant plagioclase basalt from Sagar district
Alexander and Purohit (2019)
Contemporary Researches and Issues Related to the Deccan Volcanism
249
23.
A 1251m-thick Deccan Flood Basalt Pile Recovered by Scientific Drilling in the
Koyna Region, Western India
Mishra et al. (2017)
24.
The Subsurface Megascopic Characteristics of Basalt and Basement Rocks from
Koyna-Warna Area of Maharashtra, India
Sinha et al. (2017)
25.
Mineral carbonation reactions under water-saturated, hydrothermal-like conditions
and numerical simulations of CO2 sequestration in tholeiitic basalt of the Eastern
Deccan Volcanic Province, India
Kumar et al. (2017)
26.
Ultrasonic P- and S-Wave Attenuation and Petrophysical Properties of Deccan
Flood Basalts, India, as Revealed by Borehole Studies
Vedanti et al. (2018)
27.
Thermodynamic Modelling and Experimental Validation of CO2 Mineral Sequestration
in Mandla Basalt of the Eastern Deccan Volcanic Province, India
Kumar and Shrivastava (2019)
28.
Tholeiitic basalts of Deccan large igneous province, India: An overview
Prasanth et al. (2019)
Lava-flow stratigraphy
29.
Polycyclic aromatic hydrocarbon compound excursions and K/Pg transition in the
late Cretaceous–early Palaeogene succession of the Um Sohryngkew river section,
Meghalaya
Pal et al. (2015a)
30.
Physils and organic matter-basepalaeoenvironmental records of the K/Pg boundary
transition from the late Cretaceous-early Palaeogene succession of the Um-Sohryngkew
River section of Meghalaya, India
Pal et al. (2015b)
31.
A multi-proxy approach to decode the end-Cretaceousmass extinction
Punekar et al. (2015)
32.
Environmental changes during the Cretaceous-Paleogene mass extinction and
Paleocene-Eocene Thermal Maximum: Implications for the Anthropocene
Keller et al. (2017)
33.
Study on the Relationship Between Deccan LIPs and Chicxulub Crater Based on
“Collisions Aggregation Effect”
Chenming and Demin (2018)
34.
The eruptive tempo of Deccan volcanism in relation to theCretaceous-Paleogene
boundary
Sprain et al. (2019)
35.
State shift in Deccan volcanism at the Cretaceous-Paleogene boundary, possibly
induced by impact
Renne et al. (2019)
Fig. 4: Giant plagioclase basalt from BijasanGhat showing
well-developed, lath-shaped plagioclase megacrysts
(5 cm in length). Source: Sheth et al. (2016)
Fig. 3: Photomicrograph of alkali basalt type from the Kutch
area showing olivine xenocryst with fractures filled
up with glassy groundmass. Microphenocrysts and
groundmass olivine grains are also present along
with the olivine xenocryst. Abbreviations: Ol(x)olivine xenocryst; Ol(mp)-microphenocryst of olivine.
Source: Ray et al. (2016)
the lithosphere with faster rate, where mantle xenoliths
were broken-up into smaller fragments. These
processes were considered as major causative factors
for the K/Pg mass extinction. Chatterjee and Sheth
(2015) studied ankaramite from Powai in the Bombay
area which contains zoned olivine crystals. Primary
magmas for this area as well as voluminous Ambenali
and Mahabaleshwar Formation tholeiites in the
250
Western Ghats representing primitive tholeiites (MgO
8.74-11.77 wt%, Mg# 70-74). Such magma types last
equilibrated with the mantle peridotite at a temperature
and pressure ranging between 1268-1332°C (±12°C)
and 8.0-13.0 kb (±0.8 kb) corresponding to the depth
between 30-49 km (±3 km), respectively. Moreover,
primary magmas originated by ≤15 % batch melting
of the mantle and these magma types underwent
olivine gabbro fractionation. As a result, mafic
cumulate piles (Ol+Cpx+Opx) produced at the bottom
of magma chambers. Later tholeiitic magma batches
penetrated cumulate piles which led to the formation
of cumulate rich ankaramite and underwent dissolution
of the orthopyroxene and subsequent crystallization
of augite, olivine, and plagioclase. The voluminous
Ambenali and Mahabaleshwar tholeiites of the
Western Ghats last equilibrated with the spinel
lherzolite mantle which was neither Fe rich nor
anomalously hot.
Amit Kumar et al.
Dhule tholeiitic dyke swarms (Sheth, 2018). These
dykes served as feeders to few Western Ghats and
Saurashtra lavas, located ~200 km away from the
dyke swarms. Moreover, compositionally distinct (high
TiO2), but, majority of them are isotopically akin to
Mahabaleshwar and Panhala Formations of the upper
Western Ghats that lie within a narrow isotopic array
and represent distinctive chemical signatures
somewhat comparable to distant (~600 km) dykes,
sills, and lavas of the Pachmarhi, Shahdol, and Mandla
areas in the Satpura and Narmada regions in the
eastern Deccan Traps. Distinctive isotopic signatures
of Nandurbar-Dhule tholeiitic dyke swarms were
somewhat similar to the dykes, sills, and lavas of the
Pachmarhi (Shrivastava et al., 2008; Kumar and
Shrivastava, 2009) and Mandla (Shrivastava, 2014)
areas, located ~ 900 km to the east, thus, justify a
separate entity of eastern Deccan lava stratigraphy.
Age and Duration of Deccan Volcanism
Giant Plagioclase Basalt
The Giant Plagioclase Basalt (GPB) containing long
(~ 5 cm) plagioclase megacrysts (Fig. 4) attending as
a marker horizon for the upper of the Deccan
stratigraphic formational boundaries. These
megacrysts form anorthositic mushes embedded
within the ferrodioritic interstitial glassy groundmass.
On the basis of unusual occurrence of such type of
basalt, Sheth (2016) proposed a model, where
residency period of ~ 15 ka in a deep crustal sill
complex was postulated for the magma to grow
plagioclase megacrysts before being erupted. Of late
Alexander and Purohit (2019) reported GPB from
lava flows in the northeastern basalt in the Sagar area
of Madhya Pradesh. However, stratigraphic
correlation between these two GPB horizons and
details pertaining to lava flows (which lie immediately
below as well as above) is lacking in the literature.
DVP Associated Anorogenic, Intra-plate Silicic
Magmatism
Cucciniello et al. (2018) recognized advanced
fractional crystallization of basaltic magmas, crustal
assimilation coupled with fractional crystallization,
partial melting of basalt and anatexis of old basement
crust as important processes responsible for their
formation. Sr-Nd-Pb isotopic data in conjunction with
the geochemical data, assigned process of multiple
magma injections to the ENE-WS trending Nandurbar-
Earlier reported Deccan basalt ages recognized that
bulk of magma was emplaced within a period of 67 65 Ma, however, with the exception of some early
alkaline activity in the Cambay graben at 69 Ma. But,
Shrivastava et al. (2015) assigned significantly
younger ages of 63-65 Ma (weighted mean age of
64.21 ± 0.33 Ma) to the stratigraphically controlled ~
900 m thick Mandla lobe succession (which contains
37 lava flows) on the eastern margin of Deccan
volcanic province. New ages are consistent, however,
with the geochemical correlation of the Mandla lobe
lavas with the uppermost succession (PoladpurAmbenali-Mahabaleshwar Formations) of
southwestern Deccan Traps, indicated that this post
KPB youngest phase of flood basalt activity erupted
over much of the province. The Deccan volcanic
activity occurred in several phases - an earlier phase
was accountable for the formation of great western
succession of lava flows, whereas, later phase resulted
in the formation of terminal lava flows of the southwest
region and entire succession of the Mandla lobe in
the east (Shrivastava et al., 2015). The post-KPB
younger 40Ar-39Ar ages of the Mandla lavas have
serious implications on the duration of Deccan
volcanism (Shrivastava et al., 2015). A large number
of Deccan basalt dykes associated with the east-west
trending Narmada-Tapti-Son lineaments are
supposedly synchronous with Deccan volcanic
eruptions. But, in the northern slope of Satpura
Contemporary Researches and Issues Related to the Deccan Volcanism
Mountain range (~800 km NE of the Western Ghats
escarpment), Shrivastava et al. (2017) recognized
feeder and post-Deccan Traps dyke activities solely
on the basis of new 40Ar-39Ar ages of 66.56 ± 0.42
and 56.95 ± 1.08 Ma from two distinct dykes (Fig. 5)
which cut across the lava flows near Mohpani and
Olini villages, respectively. The new age data on the
Mohpani dyke yielded an age of 66.56 ± 0.42 Ma,
which is earlier to or contemporaneous with the nearby
Mandla lavas. It is evident that the lava flowed through
major fractures/faults and emplaced as dykes and
served as conduits for the lava flows. Thus, dykes
possibly served as feeders. The new ages are also
consistent with geochemical correlation of the Mandla
lavas and with uppermost Poladpur, Ambenali and
Mahabaleshwar Formation lavas of the southwestern
Deccan (Shrivastava et al., 2014). The dyke near
Fig. 5: Field photographs showing dykes located (a) near
Olini (sample P7) and (b) Mohpani villages (sample
P18) in Betul area. Chilled contact zones vary in
thickness from 3 to 8 cm, lying between the dyke and
lava flows marked in the photograph. Source:
Shrivastava et al. (2017)
251
Olini village represents an age of 56.95 ± 1.08 Ma
which is much younger and represents the terminal
stage of dyke activity.
Recent 40 Ar- 39 Ar ages from the northern
portion of the DVP provided new constraints on the
relationship between two magma series and on the
evolution of Deccan magmatism (Parisio et al., 2016)
and further assigned an age of 65.86 ± 1.68 Ma for
the first stage of magmatism in the Rajpipla area.
Besides this, the Rajpipla basalt and Pavagadh rhyolite
(64.9 ± 0.8 Ma) represent a maximum and minimum
duration of the tholeiitic Deccan magmatism of 3 Ma
and <1 Ma, respectively. Conversely, alkaline
magmatism lasted within 4 Ma, starting from 69.62 ±
0.08 Ma to 65.25 ± 0.29 Ma. Significantly, recalculated
40Ar-39Ar ages suggested that the magmatic activity
started at the boundary between magnetic chrons
C31r and C31n with the emplacement of the Sarnu
Dandali and Mundwara complexes, and Deccan
magmatism lasted at least 4 Ma. Moreover, 40Ar-39Ar
ages of Parisio et al. (2016) for the Pavagadh
complex and Phenai Mata alkaline rocks indicated
incidence of late-phase of magmatism in the northern
Deccan volcanic province. 40Ar/39Ar ages of Pande
et al. (2017) for the Mumbai tholeiitic and Panvel
flexure flows, and post-flexure dykes yielded similar
ages of 62.5 Ma and suggested rapid formation of
Panvel flexure at 62.5 Ma. These observations are
congruent with the Dongri rhyolite flow ages of 62.5
Ma from the uppermost part of Mumbai volcanic
sequence. Post-rift magmatism ages of 60.8-60.9 and
60-61 Ma assigned to the Manori trachyte and Gilbert
Hill basalt in the Mumbai area, respectively. Thus,
these units were coeval with the rift-to-drift transition
of breakup between the Seychelles and the Laxmi
Ridge-India, thus clearly recognize pre-, syn- and postrift Deccan magmatism associated with the breakup
of Seychelles from the Laxmi Ridge and India. The
longest (~79 km), Nandurbar-Dhule tholeiitic dyke
swarms in the Deccan Traps represent 40Ar/39Ar ages
of 67.06-63.43 ± 0.48 Ma, suggestive of ≥2.5
emplacement span under regional crustal extension
(Sheth et al., 2018).
Sheth et al. (2017) reported new 40Ar/39Ar ages
of 88.9-86.8 Ma from the Sarnu-Dandali alkaline
complex, Rajasthan and suggested that the syenite,
nephelinite, phonolite and rhyolite rocks were much
older than Deccan basalt (66 Ma) rock types present
252
within the complex, thus, assigned two diverse
emplacement episodes entailing a time lag of ~ 20
Ma in the late Cretaceous Period (for these two
distinctive rock groups). Pande et al. (2017) on the
basis of 40 Ar/39Ar ages suggested polychronous
emplacement for the Mundwara alkaline complex,
located ~ 120 km southeast of Sarnu-Dandali in
Rajasthan. Moreover, 84-80 Ma ages obtained from
the Mundwara alkaline complex represents postbreakup stages of the Indo-Madagascar. Thus, akin
to the Mundwara complex, Sarnu-Dandali complex
is also polychromous in nature and characterized by
Amit Kumar et al.
periodically replenished alkaline magma. Temporally,
both the complexes show comparable evolution from
early to late Cretaceous period and spatially record
Indo-Madagascar flood basalt volcanism to
northwestern India. Of late, Schoene et al. (2019)
estimated Deccan eruption rates using U-Pb zircon
as chronometer. They recognized four major eruptive
phases (Fig. 6); each lasted for ≤100 ka and separated
by periods of relative volcanic quiescence. Moreover,
one of the phases initiated tens of thousands of years
prior to both the bolide impact and the K/Pg extinction.
Coincidental with the second major eruptive phase,
Fig. 6: Major eruptive phases, timing of the K/Pg transition events and organo-molecular compounds (associated with the
marine Um-Sohryngkew river section) calibrated with respect to biozonation and GSSP El kef (Tunisia) sections (as a
reference) further correlated with the Jhilmili and Anjarintertrappeans and EDVP bole beds successions. Data Source:
Bhandari et al. (1987); Mukhopadhyay (2008, 2009, 2010, 2012a,b, 2013); Shrivastava et al. (2013); Pal et al. (2015a-c),
where, * = Parvularugoglobigerinaeugubina, ** = Guembelitriacretacea, *** = Plummeritahantkeninoides, **** =
Pseudoguembelinahariaensis, 1 = Schoene et al. (2019); 2 = Shrivastava et al. (2015), 3 = Punekar et al. (2016), 4, 5 = Pal et
al. (2015 a,b), 6 = Shrivastava et al. (2013), 7 = Keller et al. (2009), 8 = Pal et al. (2013), 9 = Pal et al. (In press a), 10 =
Bhandari et al. (1987), 11 = Shrivastava and Ahmad (2005); 12 = Pal et al. (In press b), 13 = Keller and Lindinger (1989),
14 = Gross (2017). Abbreviations: Geol. Periods = Geological Periods, Mag. Chrons= Magnetic chrons, Erupt. = eruption, Bus. =
Bushe, Ocean acid. = Oceanic acidification, Carb. crisis= carbonate crisis, LMW PAH= low molecular weight polycyclic aromatic
hydrocarbon compounds, SA= short chain n-alkanes, HMW PAH = high molecular weight polycyclic aromatic hydrocarbon
compounds, Ce anom.= Ce anomaly, Dec.= Deccan, Vol.= Volcanism, GH effects= Greenhouse effects, P. elegans =
Pseudotextulariaelegans, Brack.-Marine = Brackish-Marine, Intert. = Intertrappean, Ostro. = Ostrocod, Plank. Foram. = Planktonic
foraminifera, incurs. = incursion, Mont. = montmorillonite, Lacust. = Lacustrine, Ir. anom. = Iridium anomaly, Aliph. = aliphatic,
NAP= napthalene, A= anthracene, Pyr = pyrene, +ve = positive. Symbols: and denotes transgression and regression, respectively
Contemporary Researches and Issues Related to the Deccan Volcanism
Poladpur Formation eruption began tens of thousands
of years before, but, peaked out at the K/Pg mass
extinction event which continued after it, but in a
subdued manner. Finding out Chicxulub impact
signature (if any) may provide a precise stratigraphic
reference point within Deccan stratigraphy.
Palaeomagnetism and Magnetostratigraphy
In the Mandla area of Eastern Deccan Volcanic
Province (EDVP), flow-by-flow palaeomagnetic
measurements (Pathak et al., 2016) for the 37 lava
flows (from the ~ 900 m-thick, isolated lava pile)
revealed multiple magnetic polarity events: implying
for the C29n-C28r-C28n magnetostratigraphy.
However, based on recent palaeomagnetic data from
Deccan dyke swarms of the Mumbai area, Basavaiah
et al. (2018) suspected more reversals than three
Chrons (n-r-n) flow magnetostratigraphy. These
results when traced out from section to section,
maintaining the order of superposition, resolved that
the lava packages of contrasting characters are
juxtaposed near Deori area. In Dindori and also
towards south, the distinct lava packages are
juxtaposed and explained by the presence of four
normal post-Deccan faults in the Nagapahar, KundamDeori, Dindori and Badargarh-Amarkantak sectors,
thus, justify structural complexity with the vertical shifts
of 150-300 m. To some extent, observed magnetic
polarity bias (transitional direction) might be the result
of combined effects of tectonic disturbance in the
area, lesser availability of the unaltered lava flows
and their altitude based correlation. Considering the
highly wavy palaeo-surfaces and faulting due to postDeccan isostatic adjustments over a distance of ~
800 km along the strike length, there is a possibility of
disorder in the stratigraphic heights of lava packages,
which, therefore, constrains the altitude-based
correlation of lava packages over such a vast area.
Magnetostratigraphic correlation of the Mandla
lavas with that of the main DVP is mainly based either
on: (a) magnetic polarity correlation as a function of
altitude or (b) available 40Ar/39Ar ages of the Mandla
lava flows. Later correlation is solely based on new
40Ar/39Ar ages (Shrivastava et al., 2015) which are
consistent with the GPTS (Cande and Kent, 1995;
Gradstein et al., 2012), thus, pointing to the idea that
the entire Mandla lava package were laid down in
the chrons C29n-C28r-C28n. The later correlation
253
seems to be more reliable as it lies well within the
GPTS of Gradstein et al. (2012). As compared to the
southwestern lavas, Mandla lavas erupted at different
times. In view of the palaeomagnetic results, it is
suggested that the Mandla lavas erupted from different
feeder system(s). Proposed C29n-C28r-C28n
magnetostratigraphy of the Mandla lavas revealed that
they are significantly younger than the majority of
main DVP lava sequences documented from the
Western Ghats.
Magnetic chron reversals in conjunction with
field and chemical data supported these findings
(Pathak et al., 2016). Further, compositionally these
lavas are akin to Bushe, Poladpur, Ambenali and
Mahableshwar Formational lavas, and follow the
same stratigraphic order as in the Western Ghats.
Alternating field (AFD) and thermal demagnetizations
(THD) isolate the normal mean direction of the
Mandla lobe. The Virtual Geomagnetic Pole (VGP)
position determined for these lavas, when compared
to the Deccan Super Pole, indicates concordance with
the main DVP, thus, assigning eruption ages close to
the KPB for the eastern and western Deccan Traps.
Deccan Volcanism and K/Pg Transition Events
Punekar et al. (2016) discussed excessive amount of
CO2 and SO2 release during the most violent phase
of Deccan volcanism introduced into the atmosphere
which was the causative factor for carbonate crisis
in the oceans and severe stress to the marine calcifiers,
ultimately led to the mass extinction (Fig. 6). Highly
stressed environment initiated for planktic foraminifera
is evidenced by ~50 cm below the KPB layer at
Bidart (France) and Gamsbach in Austria and ~ 4.5
m below the KPB at Elles in Tunisia. Moreover,
corresponding interval in India documented stronger
carbonate dissolution effects in the intertrappean
sedimentary units which lie between the longest lava
flows and culminated with the mass extinction. Based
on these observations, Punekar et al. (2016) inferred
that the widespread dissolution event stratigraphically
matches with the climatic cooling and followed by
the late Maatrichtian global warming. These major
events perhaps were attendant to Deccan volcanism
induced ocean acidification (Fig. 6). Further, late
Maastrichtian CF1 zone in the former two areas
revealed events within the latest ~160 ka of late
Maastrichtian and considered as critical as far as role
254
of the Deccan volcanism in global high stress
environments is concerned. Sudden rise in
temperature (>140ºC) during the formation of illite in
the upper part of biozone CF3 is comparable to the
KPB layer of Caravaca section of Spain (Pal et al.,
2015a). Moreover, humid tropical to arid-semiarid
climatic and thermal variation across the succession
were linked to the contemporaneous Deccan volcanic
activities. Total organic carbon together with the short
chain n-alkane and fatty acid spikes (Fig. 6) are
concomitant with the sudden rise in the palaeotemperature (>140oC) of the yellowish brown organic
rich clay layer in biozone CF3 (Pal et al., 2015b;
2019a). These organic macro-molecules reflected
global fire, induced by the heat supplied by late
Cretaceous Deccan extrusions initiated prior to the
KPB, however, the main episode of Deccan volcanic
activity occurred ≥300 ka earlier or after the KPB
itself. Punekar et al. (2016) provided evidence of
Deccan-related environmental changes at the onset
of K/Pg mass extinction from Bidart section (France).
In this area, the sedimentary layer which lie
immediately ~80 cm below and ~50 cm above the
KPB layer contains anomalously high Hg
concentrations (>2 orders of magnitude) coincidental
with the low magnetic susceptibility interval (Font et
al., 2016). The K/Pg mass extinction is universally
attributed to the Chicxulub impact; however Deccan
volcanism contributed to as a major factor (Keller et
al., 2017). Although, the Hg anomalies pointed out
that the major Deccan eruptions accelerated during
last 10 ka and reached to its maxima which led to
mass extinction. Thus, Chicxulub asteroid impact
(Mexico) and gigantic Deccan volcanic eruptions
were proposed as the major causes for the endCretaceous mass extinction, including sudden demise
of nonavian dinosaurs. But, high resolution U-Pb
zircon ages determined by Schoene et al. (2015)
provided an idea that the main phase of eruptions
initiated ~250 ka prior to the KPB, where >1.1 million
km2 of basalt erupted in ~750 ka. These results are
consistent with the idea that the Deccan volcanism
contributed to the latest Cretaceous environmental
change and the biologic turnover that culminated in
the marine and terrestrial mass extinctions. However,
the main phase of Deccan volcanism occurred at 66
Ma, but, its activity started ~ 0.5 Ma prior to and
terminated after the KPB and the Chicxulub impact
dated at 66.04 ± 0.09 Ma and 66.04 ± 0.05 Ma,
Amit Kumar et al.
respectively (Sprain et al. 2019). A noticeable 7.8 ±
3.3 °C warming which was synchronous with the onset
of Deccan volcanism, however, a second, smaller
warming was at the time of meteorite impact (Petersen
et al., 2016). Although, eruption pattern, as well as
rate of Deccan volcanism at the KPB was primarily
affected by the Chicxulub impact (Renne et al., 2015;
Richards et al., 2015). To understand relationship of
the Deccan volcanism across the KPB at Um
Sohrynkew and Jhilmili sections in India, Sial et al.
(2017) employed Hg, Hg/TOC and Al2O3 as proxies
for volcanism and recorded true Hg anomalies and
three prominent Hg/TOC spikes: (1) within the CF2
planktic foraminiferal biozone, (2) at the KPB, and
(3) within the P1a planktic foraminiferal sub-zone of
the former as well as in the Jhilmili sections. They
further concluded that Hg anomalies possibly
attributed to strong volcanic incidences of the Deccan
phase-2 (started 250 ka before the KPB and lasted
for 750 ka). These incidences were accountable for
prolific sulfuric aerosols and carbon dioxide emissions.
Moreover, Hg isotopic spike 2 in Meghalaya KPB
layer, spike 1 in CF2 biozone and spike 3 in Jhilmili
are consistent with the peak volcanic Hg emissions,
thus Hg enriched in paleoenvironment at three distinct
stages during the Deccan phase-2. However,
Mukhopadhyay et al. (2017) pointed out that the KPB
reported by Sial et al. (2016) is not compatible with
the existing planktonic foraminiferal succession across
K/Pg boundary in the Um Sohryngkew River section,
Meghalaya India. Owing to the meteorite impact and
the Deccan Traps formed by the collisions, aggregation
effect of the Chicxulub crater impact triggered
massive mass extinctions (at 65 Ma of the K/Pg
boundary) and accelerated the Indian Plate drift
(Chenming et al., 2018). The eruptive pulse of Deccan
volcanism studied with reference to the KPB
concluded that the late Cretaceous records of climate
change coincided temporally not with the major and
most violent phase, but, with the eruption of smallest
Deccan Trap phases (Sprain et al., 2019). They
opined that either the release of climate-modifying
gases was not directly related to eruptive volume or
Deccan Traps volcanism, therefore, Deccan
volcanism was not the source of late Cretaceous
climate change. However, diverse ideas emerged out
of the studies (Sprain et al. 2019; Schoene et al.,
2019) on relative timing of Deccan Traps
emplacement and mass extinction. On the basis of
Contemporary Researches and Issues Related to the Deccan Volcanism
age data-sets, the stratigraphic position of KPB was
assigned within Deccan Traps stratigraphy. But the
subtle difference in placement significantly alters the
balance of accountability between the bolide impact
and the Deccan volcanic events (Burgess, 2019).
Thus, finding out Chicxulub impact signature (if any)
may provide a precise stratigraphic reference point
within Deccan stratigraphy.
Infra/-interflow Volcanic Bole Beds
Widdowson et al. (2015) discussed Deccan intravolcanic bole horizons, representing weathered
products formed at the time of major hiatuses between
two successive major volcanic episodes. Both bole
beds and altered lavas represent a comparatively early
stage of weathering because residual elements, such
as Al and Fe are closer to the fresh basalt than the
laterite. Nevertheless, there is clear evidence in
support of significant chemical alteration as the more
mobile elements such as Ca and Na have been
substantially removed. Several Deccan Traps
associated bole beds are in fact weathered pyroclastic
material, where pyroclastic content of the basaltic
succession is very large. A significant pyroclastic input
during Deccan eruptions has important
palaeoenvironmental implications for the fate of late
Cretaceous fauna and flora that existed in the
Peninsular India.
Red bole horizons formed by pervasive subaerial weathering of the previously exposed igneous
materials together with the locally associated lacustrine
and fluvial sediments. Yet, unlike the lava sequences,
intertrappean bole horizons have received little
geological attention, although, it is accepted that the
formation of these weathering horizons temporally
represents greater part of the history of CFB
provinces. Geochemical study of the weathered bole
horizons established the role of elemental mobilization
during chemical weathering, but indicated that the
geochemical data cannot always be reconciled with
the established patterns of elemental depletion (typical
of alteration of a basaltic precursor). In addition, thin
sections indicate that the fine-grained portions of some
boles contain glass shards and fresh phenocrysts of a
pyroclastic origin. Though, the Deccan intertrappean
surfaces, all that resulted from the same endogenetic
process (namely the development of lava fields during
flood basalt volcanism), the saprolitic and pyroclastic
255
boles recorded two different types of
palaeoenvironmental conditions. The former group
formed by protracted, in-situ alteration of the lava
surfaces during the periods of volcanic quiescence.
By contrast, the cherty boles resulted from a
‘blanketing’ of the lava landscape by extensive ash
fall-out which possibly led to the widespread
destruction of established fauna and flora. Weathering
studies of Shrivastava et al. (2017) on interflow
volcanic boles from Mandla lobe, EDVP were
primarily focused to trace out paleoenvironment and
degree of pedogenic/non-pedogenic conditions that
existed during the Deccan volcanism. Owing to limited
time intervals during successive eruptions, majority
of the bole beds represent incipient to moderate
weathering. However, few red and brown bole beds
show baking effects rather than pedogenesis.
Moreover, comparison of magnetic properties of bole
from EDVP and WDVP shows significant differences
in the weathering intensity, duration and heating
related alterations from the upper flows. But, both
EDVP and WDVP bole beds indicate similar first order
paleoenvironmental conditions without any major
pedogenesis. Crystallographic defects in the smectites
of the Jhilmili intertrappean provided evidence of KPB
transition induced environmental changes which
include global warming, acid rains and pCO2 rise in
the atmosphere (Pal et al., 2019b).
Applied Aspects
CO2 Sequestration in Deccan Basalt
Shrivastava et al. (2016) reported CO2 sequestration
under natural conditions as evidenced by abundant
thick limestone and inter-calcarious lithofacies that
occur as infra (visibly below lava flows)/inter (between
two lava flows) - trappean beds. On the basis of field
observations, Shrivastava et al. (2016) considered
tholettic basalt lava flows of the Mandla area as a
suitable matrix for mineral carbonation reactions and
for long-term storage of CO2 as they contain high
amount of reactant minerals such as Ca, Mg and Fe
rich silicates. Computer based basalt-water-CO2
interaction modeling and laboratory induced reactions
under hydrothermal-like conditions form the basis of
study. A series of experiments performed at
accelerated conditions and post-experimental residues
indicate formation of calcite, aragonite, siderite and
magnesite. They observed that the basalt dissolution
256
rate was faster and reaction is primarily driven by the
secondary mineral replacement and growth of
minerals. Formation of carbonates is largely due to
the breakdown of pyroxene, feldspar and glass.
Kumar et al. (2017) performed Deccan basaltwater-CO2 saturated interaction experiments and
numerical simulations under hydrothermal-like
conditions. Data revealed appearance of calcite,
aragonite, ankerite, huntite and siderite along with the
secondary silicates. Moreover, tiny calcite crystals
were developed over larger calcite crystals (Fig. 7A),
incipient-disordered calcite formed with imperfections
on its crystal faces (Fig. 7B) and cubic chabazite
crystals surrounded by chlorite grains (Fig. 7C).
Formation of disordered rhombic calcite in these
experiments is ascribed to a partial carbonation
reaction, whereas well-defined rhombic calcite crystal
faces (Fig. 7A) formed over basalt is suggestive of a
complete carbonation reaction. Experiments run for
shorter time periods show formation of secondary
carbonates which predominated over the silicates;
however, with increased reaction times, carbonates
no longer persisted in the system as they were
Amit Kumar et al.
dissolved and replaced by silicates. As a result, thin
layer of neo-formed SS form adjacent to the basalt
grains. Thus, basalt grains restricted to form
carbonates. In this manner, neo-formed SS act as
barrier. As a result, basalt-water-CO2 interaction rate
is also reduced considerably and limiting availability
of Ca, Mg and Fe cation to form carbonates (Kumar
and Shrivastava, 2019a). Mixing trends (Kumar et
al., 2017) between basalt and Ca-Mg-Fe carbonates
and chlorite/smectite were observed in case of
phyllosilicates. However, ankerite, calcite and siderite
recorded enrichment of (i) Ca, (ii) Fe-Mg and (iii) Fe.
Secondary silicates formed adjacent to the basalt
grains clog basalt-water-CO2 interaction pathways,
thus, reduced the amount of CO2 mineralization.
Formation of carbonates and secondary silicates is
mainly influenced by time; however, pressure, pH and
temperature play subordinate roles. Kumar and
Shrivastava (2019b) further validated modeling results
by the experiments run in laboratory time framework
and resolved that the negative entropy (∆S) and
enthalpy (∆fH) suggested feasibility of plagioclase,
pyroxene and magnetite dissolution. The negative
Fig. 7: SEM images of secondary minerals showing (a)
stepped growth of calcite and chlorite coatings on
basalt, (b) siderite and incipient-disordered rhombic
calcite grain with imperfections on crystal faces and
(c) chlorite coatings over chabazite grain.
Abbreviations: Cal = Calcite, Ch = Chlorite, Chb =
Chabazite, DB = Deccan Basalt and Sm = Smectite.
Source: Kumar et al. (2017)
Contemporary Researches and Issues Related to the Deccan Volcanism
Gibb’s free energy (∆fG), ∆fH and ∆S values for
calcite, dolomite and magnesite indicated spontaneous
reaction, whereas, positive ∆fG and negative ∆fH and
∆S values of the siderite suggested non-spontaneous
and opposing reactions. Calcite was the first carbonate
mineral to form, but, at a faster rate. Magnetite
dissolution begins after a time lag (not initiated along
with the plagioclase and pyroxene). Kumar and
Shrivastava (2019a) concluded that largely,
thermodynamic models do not agree well with the
experimental results as numerical models indicate
larger carbonate growth. Additionally, transition state
theory based models worked well to predict dissolution
rates for most of the minerals, but, they over-predict
growth of the secondary minerals. Rietveld refinement
(RR) results indicate that, weakened Ca-O and C-O
bond length led to calcite degeneration after 80 hours
of experiments; therefore, no calcite persisted in the
system. Further, the crystal structure of experimentally
and naturally formed calcite and chabazite was alike
to each other (Kumar and Shrivastava, 2019c). The
mass balance estimates after each experiment run
revealed that the maximum 30.75 mol % of ions from
parent basalt reacted during carbonation reaction. As
a result, 22.88 mol % of CO2 mineralized in the form
of carbonates (such as calcite and dolomite) at 100oC
under 5 bar CO2 for 70 h of experiment (Kumar and
Shrivastava, 2019d).
257
elements into the solution. By evolution of secondary
layer and retention of less soluble ions, the obstructive
effect of secondary layer increases and constant
release rate initiated slowly to diminish with time.
Process of devitrification along the cracks and
formation of spherulite-like structures, yellowish
brown palagonite, chlorite, calcite, zeolite and finally
white coloured clay minerals largely correspond to
altered obsidian that existed in the natural environment
since inception (~ 66 Ma ago). Moreover, low
elemental release rate from the glass matrix is
suggestive of high order of chemical durability of glass.
Obsidian, a natural analogue for the nuclear waste
glass is durable enough to withstand natural
environmental conditions for a period of ~300 years
till the radioactivity of Ce isotopes is ceased. The
chemico-mineralogical attributes of the obsidian are
analogous to radioactive waste form; therefore,
obsidian is suitable for safe disposal of high-level
nuclear waste in the geological repository. Process
and extent of palagonitization and the formation of
smectite are comparable to the experimentally altered
as well as naturally weathered glass. The
microtextures and microchemistry of altered glass
revealed evolutionary changes partly to complete
alteration and growth of palagonite, smectite, illite,
montmorillonite, calcite and zeolite.
Future Directions
Impact glass and Obsidian: A Natural Analogue
of Nuclear Waste Glass
Rani et al. (2015) and Kumar et al. (2019) discussed
Deccan basaltic glass (associated with the
differentiation centers of vast basaltic magmas) for
its suitability as a standad reference for radioactive
waste containment. The suitability primarily depends
upon alteration behavior under hydrothermal-like
conditions. Alteration results when compared to the
naturally altered glass show partial to complete release
of all the ions; however, abundant release of Si and
Na ions is noticed. Altered residue shows
morphologies of smectite, montmorillonite and illite
inside as well as outside of the secondary layers.
Octahedral cation occupancies of smectite were
found consistent with the dioctahedr alsmectite. The
secondary layer composition indicates retention for
Si, Al, and Mg cations, indicating their fixation, but
remarkably high retention of Ti, Mn and Fe cation
suggested release of very small amount of these
Present review discusses several important findings
covering almost all the aspects related to Deccan
volcanism, however, a few important issues that
remain to be addressed include:
1.
Most of the new bulk, mineral chemistry, NdSr-Pb isotopic and 40Ar- 39Ar age data-sets
restricted to differentiation centers, located in
the western part of Deccan volcanic province;
however, such data is rare for the peripheral
areas.
2.
Comprehensive flow by flow stratigraphic
framework, age and duration of volcanism for
the peripheral areas and sub-surface KoynaWarna-Panchgani sections are required with
special reference to their stratigraphic
correlations with the main DVP to understand
source, eruption mechanism, and rate of host
magma ascended, age and duration of Deccan
volcanism.
258
Amit Kumar et al.
3.
To find out possible link (if any) between the
Sagar GPB and the type GPB section of the
western DVP.
4.
Parental magmas and the fractionation trends
for various basalt suites required to be assessed
particularly for the central and peripheral areas.
5.
Mechanism to understand derivation of alkaline
and tholeiitic magma from the mantle sources
6.
To understand geodynamic setting of the magma
suites with contrasting characters.
7.
Lherzolite mantle equilibration trends need
thorough investigations.
8.
Timing of the dykes such as pre, syn or post to
the lava flows is required to be resolved.
9.
Inconsistency in the ages with southward
migration of volcanism due to northward journey
of the Indian plate above the Reunion hotspot
need to be re-visited.
1.
Petrography, mineral chemistry, whole-rock
major, trace elemental and Nd-Sr-Pb isotopic
data in conjunction with the 40Ar-39Ar ages,
revealed that the Deccan Traps associated silicic
magmatism post-dates flood basalt eruptions.
The Barda granophyre intrusions pre-dated
intense and most prolific 66-65 Ma Deccan flood
basalt phase by 3 to 4 Ma, thus, entailed a total
duration of ~ 8 Ma. These observations are in
conformity with the finding of Salil et al. (1997)
and supportive of prolong duration of the Deccan
volcanism (Shrivastava et al., 2012).
2.
Moreover, the 69-68 Ma Barda granophyre
plutonism took place within-plate tectonic setting
(Bhattacharya and Yatheesh, 2015). The
voluminous basalt fractionation-derived silicic
magmatism in Barda and Alech complexes
suggested temporal evolution of the Deccan
flood basalt volcanism. Further, magma evolution
represents a pulsating mantle melting regime,
where such activity continued for > 1 Ma. The
Deccan volcanism is constrained by these ages
and belongs to the magnetic chrons C31-C29.
But, recalculated ages pointing towards initiation
of the first phase of alkaline Deccan magmatism
in Sarnu and Mundwara complexes in northern
Deccan (Basu et al., 1993) was coincidental
with the boundary between the magnetic chrons
C31r and C31n.
3.
New U-Pb zircon age data (Schoene et al.,
2019) recognizes four major eruptive phases
(Fig. 6); each lasted for ≤100 ka and separated
by periods of relative volcanic quiescence.
Moreover, one of the phases initiated tens of
thousands of years prior to both bolide impact
and the K/Pg extinction. Coincidental with the
second major eruptive phase, Poladpur
Formation eruption began tens of thousands of
years before, but peaked out at K/Pg mass
extinction event which continued after it, but in
a subdued manner. Finding out Chicxulub impact
signature (if any) may provide a precise
stratigraphic reference point within the Deccan
stratigraphy.
4.
Stratigraphically, widespread dissolution event,
climatic cooling, followed by the late Maatrichtian
global warming (Punekar et al., 2016) attendant
10. More age data is required to ascertain accurate
timing of the periodically replenished alkaline
magma with respect to Mundwara and SarnuDandali complexes.
11.
Flow-by-flow palaeomagnetic measurements
and magnetostratigraphic correlation are
required to understand structural complexities
with special reference to palaeo-surfaces and
faulting due to post-Deccan isostatic
adjustments.
12. To find out possible link between the main
phases of Deccan volcanic eruptions and the
timing of the K/Pg transition events.
13. To understand late Cretaceous palaeoenvironmental implications (for the fauna and flora),
pyroclastic input needs to be accessed
thoroughly.
14. To establish Chicxulub impact signature as a
precise stratigraphic reference point within the
Deccan stratigraphy.
Conclusions
Present review on late Cretaceous Deccan volcanism
and related issues concluded with the following
remarks:
Contemporary Researches and Issues Related to the Deccan Volcanism
to Deccan volcanism induced ocean acidification
and high stress environments.
5.
Both modeling and experimental results revealed
that maximum amount of carbonation of Deccan
basalt is possible under short-term hydrothermallike conditions. Suitability of silicic phase for
nuclear waste disposal is also discussed.
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