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Extensive 200-Million-Year-Old Continental Flood Basalts of the Central Atlantic Magmatic Province

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The Central Atlantic Magmatic Province (CAMP) is defined by tholeiitic basalts that crop out in once-contiguous parts of North America, Europe, Africa, and South America and is associated with the breakup of Pangea. 40Ar/39Ar and paleomagnetic data indicate that CAMP magmatism extended over an area of 2.5 million square kilometers in north and central Brazil, and the total aerial extent of the magmatism exceeded 7 million square kilometers in a few million years, with peak activity at 200 million years ago. The magmatism coincided closely in time with a major mass extinction at the Triassic-Jurassic boundary.
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Extensive 200-Million-Year-Old
Continental Flood Basalts
of the Central Atlantic
Magmatic Province
Andrea Marzoli,
1,2
* Paul R. Renne,
1,3
Enzo M. Piccirillo,
2
Marcia Ernesto,
4
Giuliano Bellieni,
5
Angelo De Min
2
The Central Atlantic Magmatic Province (CAMP) is defined by tholeiitic basalts
that crop out in once-contiguous parts of North America, Europe, Africa, and
South America and is associated with the breakup of Pangea.
40
Ar/
39
Ar and
paleomagnetic data indicate that CAMP magmatism extended over an area of
2.5 million square kilometers in north and central Brazil, and the total aerial
extent of the magmatism exceeded 7 million square kilometers in a few million
years, with peak activity at 200 million years ago. The magmatism coincided
closely in time with a major mass extinction at the Triassic-Jurassic boundary.
Many aspects of the genesis and consequenc-
es of continental flood basalt provinces
(CFBPs) remain poorly known and contro-
versial. The definition of a CFBP, as well as
their genetic relations with other phenomena
such as rifting of continents, hot spot tracks,
and mass extinctions, commonly hinges on
geochronology. Such is the case for the Cen-
tral Atlantic Magmatic Province (CAMP),
which is associated with the disruption of
Pangea and the opening of the central Atlan-
tic Ocean (1–3). The CAMP (Fig. 1) is rep-
resented by tholeiitic dikes, sills, and lava
flows in North and South America, Africa,
and Europe. Components of the CAMP have
been studied for decades, but only through
recent high-precision geochronologic analy-
sis can magmatism represented by this prov-
ince now be related to a single brief magmat-
ic episode.
40
Ar/
39
Ar (4) and U/Pb (5) data
permit recognition of extensive basaltic mag-
matism in West Africa, eastern North Amer-
ica, and northernmost South America at
200 64 million years ago (Ma), with an
estimated original extent of the volcanism
over an area of at least 4.5 310
6
km
2
(4–7).
Here we present
40
Ar/
39
Ar data that indicate
that CAMP basalts are widespread also in
northern and central Brazil, over a previously
unrecognized area of about 2.5 310
6
km
2
.
Most of the South American CAMP mag-
matism occurred far inland, up to 2000 km
from the Atlantic margin, in northern and
central Brazil. These tholeiitic flows, sills,
and dikes occur in Archean–Early Proterozo-
ic cratonic areas and Late Proterozoic to Pa-
leozoic basins. Lava flows (for example, in
the Maranha˜o, Anari, and Tapirapua˜ subprov-
inces) are mostly preserved in the Paleozoic
sedimentary basins and presently cover a rel-
atively restricted area of 3 310
5
km
2
, reach-
ing a maximum thickness of 300 m and a
total estimated volume of 6 310
4
km
3
(8,9).
The sills of the Amazonian basin cover an
area of ;1310
6
km
2
and have an average
thickness of ;500 m and an estimated vol-
ume of ;4310
5
km
3
(10). The only known
extrusive remnant of the Amazonian magma-
tism is in the Maranha˜o basin, where the
so-called Mosquito basalts are geochemically
similar to the Amazonian sills (9,10). About
0.4 310
6
km
2
of strongly weathered and
deeply eroded areas in the Guyana and Am-
azonian cratons are intruded by dominantly
north-south–striking dike swarms. Some of
these swarms (for example, in the Roraima
and Cassipore´ subprovinces) are character-
ized by a high density of dikes 200 to 300 m
thick and up to 300 km long and therefore are
comparable to feeder dike swarms of other
CFBPs (11–13).
The basalts in Brazil have compositions
similar to those of CAMP magmatic rocks
from North America and West Africa. They
range in composition from tholeiitic basalts
to andesitic basalts, and alkaline and silicic
rocks are scarce. CAMP tholeiites are char-
acterized by low TiO
2
concentrations (typi-
cally ,2 weight %), negative mantle-normal-
ized Nb anomalies (relative to K and La), and
moderately to strongly enriched rare Earth
element patterns (6,8,9, our data). No sys-
tematic compositional differences are noted
between the different regions of CAMP. De-
spite this common signature, relatively few
evolved tholeiites from single localities in
Brazil as well as West Africa and eastern
North America have relatively variable trace
element and isotopic compositions (Fig. 2).
Such compositional variations cannot be at-
tributed uniquely to low-pressure differentia-
tion processes and suggest [as inferred for
other Gondwana CFBPs (12,13)] important
contributions of heterogeneous, possibly
lithospheric mantle in the petrogenesis of
these rocks.
We dated fresh tholeiitic dikes from Ro-
raima and Amapa´ (Cassipore´ dikes), tholei-
itic lava flows from the Maranha˜o basin and
the Anari-Tapirapua˜ region, and one alkaline
lava flow from Lavras da Mangabeira basin
(Ceara´) of northern and central Brazil by
40
Ar/
39
Ar incremental heating (11). Ages
were calculated relative to an age of 28.02
Ma for the Fish Canyon sanidine (FCs) neu-
tron fluence monitor (14 ).
Plateau ages, defined by 10 to 45 contig-
uous steps and by 50 to 84% of total
39
Ar
released, were obtained for 10 samples (Fig.
3). Apparent age spectra for lava flows are
little affected by argon loss or excess argon
1
Berkeley Geochronology Center, 2455 Ridge Road,
Berkeley, CA 94709, USA.
2
Dipartimento di Scienze
della Terra, Universita´ di Trieste, via Weiss 8, 34127
Trieste, Italy.
3
Department of Geology and Geophys-
ics, University of California, Berkeley, CA 94720, USA.
4
Instituto Astrono´mico e Geofı´sico, Universidade de
Sa˜o Paulo, R. do Mata˜o 1226, 015508-900 Sa˜o Paulo,
Brazil.
5
Dipartimento di Mineralogia e Petrologia, Uni-
versita´ di Padova, Corso Garibaldi 37, 35100 Padova,
Italy.
*Present address: Department de Mine´ralogie, Univer-
site´ de Gene`ve, 13 rue des Maraichers, 1211 Geneva
4, Switzerland.
To whom correspondence should be addresssed. E-
mail: prenne@bgc.org
Fig. 1. Location map of the CAMP (4–7, present
data) in a Pangea reconstruction at 200 Ma,
also showing the Siberian and Karoo-Ferrar
CFBPs in the inset. The area presently recog-
nized as being part of CAMP is shown by a
dashed contour, with sample sites indicated: R,
Roraima; M, Maranha˜o; C, Cassipore´; Ce, Ceara´;
A, Anari; and T, Tapirapua˜.
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and yield plateau ages ranging from 190.5 6
1.6 to 198.5 60.8 Ma (Maranha˜o, Mosquito
basalts) and from 196.6 61.8 to 198.0 60.8
(Tapirapua˜ and Anari samples, respectively).
The alkaline basalt lava flow from Ceara´
yields a plateau age of 198.4 61.4 Ma. Dikes
from Roraima and Cassipore´, which intrude
Proterozoic basement, yield saddle-shaped
age spectra typical of excess argon contami-
nation, as is common for plagioclases of
dikes intruding wall rocks of much greater
age. Nonetheless, detailed step heating (32 to
84 steps for each sample) allowed definition
of plateaus on two Roraima (8818 and 8820)
and three Cassipore´ (8026, 8034, and 8041)
dike samples. Moreover, one dike from Ro-
raima (8804) yields a near plateau, defined by
43% of total
39
Ar released and 16 contiguous
steps. In some of the dikes,
39
Ar/
40
Ar versus
36
Ar/
40
Ar isotope correlation plots confirm
the presence of substantial excess
40
Ar and
permit determination of isochron ages, which
tend to be slightly younger than plateau ages
(Fig. 3). In these cases, to minimize the pos-
sible effect of excess argon, we adopted iso-
chron ages for the dikes (samples 8026, 8804,
8818, and 8820). In summary, ages for Ro-
raima and Cassipore´ dikes range from
197.4 61.9 to 201.1 60.7 and from 191.5 6
0.9 to 202.0 62.0 Ma, respectively.
All available radioisotopic dates for the
CAMP (4,5, present data) are between 191
and 205 Ma, with a mean age of 199.0 62.4
Ma and the peak at 200 Ma (Fig. 4). Our data
show that tholeiites from Brazil are similar in
age to those of the CAMP in Africa and
North America. The two distinguishably
younger samples (5013 and 8034, from the
Maranha˜o and Cassipore´, respectively) are
from the northernmost portion of the Brazil-
ian CAMP. A similar relation is shown on the
African continental margin in Guinea (4).
Thus, after the main pulse, magmatism may
have continued further toward the future rift-
ed margin of each continent [for example,
(15)].
Paleomagnetic data from widely distribut-
ed sites in the South American CAMP occur-
rences provide further evidence of a brief
coeval magmatic event in the circum-Atlantic
region (Fig. 5). Paleomagnetic poles for
South America are available from the Mar-
anha˜o, Guacamaya, Anari, and Tapirapua˜
volcanic rocks and the Guyana, Bolivar, Pe-
natecaua, and Cassipore´ dikes (9,16,17 ).
Data from seven independent sites in low-Ti
tholeiitic dikes and flows from Roraima yield
a paleomagnetic pole located at 235.0°E,
80.1°S (N57; 95% confidence angle a
95
5
6.6; concentration parameter k584). Con-
sidering uncertainties in the Euler poles used
to enact the continental reconstructions, the
average of these poles is in good agreement
with contemporaneous poles from western
Fig. 2. Initial (200 Ma) «Sr-«Nd isotopic com-
positions of CAMP basalts (6,8, and 32 data
samples from the present study). Compositions
of low-TiO
2
(LTi) and high-TiO
2
(HTi) basalts
from the Parana`(12) and the Karoo (13) Me-
sozoic Gondwana CFBPs, as well as mantle
components [EM, enriched mantle; HIMU,
high-m(
238
U/
204
Pb normalized for radioactive
decay to the present) mantle] and normal mid-
ocean ridge basalt (N-MORB) fields (29), are
shown for comparison. HTiP, Parana` high-TiO
2
basalts.
Fig. 3. Apparent age spectra of plagioclase
separated from dikes (8804, 8818, and
8820: Roraima; 8026, 8034, and 8041: Cas-
sipore´) and lava flows (5013 and 5042:
Maranha˜o; 8232: Ceara´; ANG-7: Anari; TRG-
10: Tapirapua˜) from north and central Bra-
zil. Isochron ages are reported in cases with
the statistic mean square of weighted de-
viates ,1.0. Plateau and isochron ages are
given in million years ago (Ma) with 2serrors, which include analytical uncertainty in neutron
fluence parameter Jvalue.
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Africa, southern Europe, and eastern North
America (18 –20). Magnetizations of most
CAMP tholeiites from South America (9,16 ,
17, present data), eastern North America (20),
southern Europe (18), and West Africa (19)
are of normal polarity. A ;4- to 5-million-
year normal polarity interval characterizes
the latest Triassic [uppermost Rhaetian (20)]
and earliest Jurassic [lower Hettangian (21)]
and is preceded and followed by long inter-
vals of reversed polarity or very frequent
polarity reversals (20,21). Thus, the CAMP
paleomagnetic data provide independent sup-
port for brevity of peak magmatism.
The CAMP thus includes the ;2.5 310
6
km
2
widespread magmatism in central and
northern Brazil and had a total extent of at
least 7 310
6
km
2
. Assuming conservatively
that preserved volcanic sections averaging
200 to 300 m thick in distal portions of the
CAMP are representative (6,8 –10), an orig-
inal volume of 2 310
6
km
3
is implied. The
geochronological and paleomagnetic data
suggest that most of this widespread magma-
tism occurred in a few million years, with a
peak at ;200 Ma. Similarly widespread and
short-lived tholeiitic magmatism characteriz-
es other well-studied CFBPs, for example,
the Siberian Traps (22) or the Karoo-Ferrar
(23,24 ) (Fig. 4).
Such brief and extremely widespread tho-
leiitic magmatism, occurring up to 2000 km
from the continental margin, implies that
anomalously hot mantle extended over a very
wide area and melted extensively. Consider-
ing the geochemical and isotopic composi-
tions of CAMP basalts, an important contri-
bution of lithospheric mantle is suggested.
The debate concerning the origin of CAMP is
open, and various models have been pro-
posed invoking the presence of either a man-
tle plume (1,2,25) or a shallow thermal
anomaly (7). In general, our data and previ-
ous (4–6,8 –10) geochemical and geochro-
nological data on CAMP are consistent with
models that suggest that an upwelling plume
head was trapped beneath the lithosphere and
separated from the plume tail (25), with
plume material spread over a very large area
by ambient mantle flux (2). However, these
models require modification to account for
CAMP magmatism not only in North Amer-
ica and Africa but also in South America.
The Triassic-Jurassic (T-J) boundary is
one of the five major Phanerozoic mass ex-
tinction events and involved marine and ter-
restrial genera and families (26 ). The timing
of the huge CAMP magmatic event overlaps
within errors with modern estimates for the
age of the T-J boundary. CAMP basaltic
dikes and flows (for example, the 201 Ma
Palisades and Gettysburg sills and the Orange
Mountain flow) of eastern North America
essentially define this boundary in the
Culpeper, Fundy, and Newark basins (5,20,
27 ) of North America. Documentation of the
enormous spatial extent of the CAMP, and its
temporal brevity, support the possibility of a
genetic relation with the T-J extinctions (28).
References and Notes
1. P. R. May, Geol. Soc. Am. Bull.82, 1285 (1971).
2. M. Wilson, J. Geol. Soc. London 154, 491 (1997).
3. M. P. Withjack, R. W. Schlische, P. E. Olsen, AAPG Bull.
82, 817 (1998).
4. J. F. Sutter, U.S. Geol. Surv. Bull. 1776, 194 (1988); A.
Sebai, G. Fe`raud, H. Bertrand, Earth Planet. Sci. Lett.
104, 455 (1991); L. Fiechtner, H. Friedrichsen, K.
Hammerschmidt, Geol. Rundsch. 81, 45 (1992); K.
Deckart, G. Fe`raud, H. Bertrand, Earth Planet. Sci.
Lett. 150, 205 (1997); A. K. Baksi and D. A. Archibald,
ibid. 151, 139 (1997).
5. G. R. Dunning and J. P. Hodych, Geology 18, 795
(1990); J. P. Hodych and G. R. Dunning, ibid. 20,51
(1992).
6. C. Alibert, Earth Planet Sci. Lett. 73, 81 (1985); C.
Dupuy et al.,ibid. 87, 100 (1988); W. J. Pegram, ibid.
97, 316 (1990); J. G. McHone, Geology 24, 319
(1996).
7. W. S. Holbrook and P. B. Kelemen, Nature 364, 433
(1993).
8. G. Bellieni et al.,Neues Jahrb. Mineral. Abh. 162,1
(1990).
9. C. R. Montes-Lauar et al.,Earth Planet. Sci. Lett. 128,
357 (1995).
10. F. M. F. De Almeida, Rev. Bras. Geociencias 16, 325
(1986).
11. P. R. Renne et al.,Earth Planet. Sci. Lett. 144, 199
(1996).
12. E. M. Piccirillo and A. J. Melfi, Eds., The Mesozoic Flood
Volcanism of the Parana` Basin: Petrogenetic and Geo-
physical Aspects (University of Sa˜o Paulo, Sa˜o Paulo,
Brazil, 1988).
13. K. G. Cox, in Continental Flood Basalts, J. D. Macdou-
gall, Ed. (Kluwer Academic, Dordrecht, Netherlands,
1988), pp. 239–272.
14. P. R. Renne et al.,Chem. Geol. (Isot. Geosci. Sect.)
145, 117 (1998).
15. M. A. Richards, R. A. Duncan, V. E. Courtillot, Science
246, 103 (1989); I. H. Campbell and R. W. Griffiths,
Earth Planet. Sci. Lett. 99, 79 (1990).
16. S. D. C. Guerreiro and A. Schult, Mu¨nchner Geophys.
Mitt. 1, 37 (1986).
17. M. Ernesto, I. G. Pacca, R. Siqueira, paper presented at
the International Union of Geodesy and Geophysics
Meeting, Boulder, CO, 1995.
18. J. J. Schott, R. Montigny, R. Thuizat, Earth Planet. Sci.
Lett. 53, 457 (1981).
19. A. E. Rapalini, A. L. Abdeldayen, D. H. Tarling, Tec-
tonophysics 220, 127 (1993).
20. W. K. Witte, D. V. Kent, P. E. Olsen, Geol. Soc. Am.
Bull. 103, 1648 (1991); D. V. Kent, P. E. Olsen, W. K.
Witte, J. Geophys. Res. 100, 14965 (1995).
21. Z. Yang et al.,J. Geophys. Res. 101, 8025 (1996).
22. P. R. Renne and A. R. Basu, Science 253, 176 (1991).
23. R. A. Duncan et al.,J. Geophys. Res. 102, 18127
(1997).
24. A. Heimann et al.,Earth Planet. Sci. Lett. 121,19
(1994).
25. A. M. Leitch, G. F. Davies, M. Wells, ibid. 161, 161
(1998).
26. D. M. Raup and J. J. Sepkoski, Science 231, 833
(1986); P. E. Olsen, N. H. Schubin, M. H. Anders, ibid.
237, 1025 (1987).
27. S. Fowell and A. Traverse, Rev. Palaeobot. Palynol. 86,
211 (1995).
28. V. E. Courtillot et al.,Geol. Soc. Am. Spec. Pap. 307,
513 (1996).
29. S. Hart and A. Zindler, in Mantle Convection. Plate
Tectonics and Global Dynamics, W. R. Peltier, Ed.
(Gordon and Breach Science, New York, 1989), pp.
261–388.
30. E. Irving and G. A. Irving, Geophys. Surv. 5, 141
(1982); J. Besse and V. E. Courtillot, J. Geophys. Res.
96, 4029 (1991).
31. P. D. Rabinowitz and J. LaBrecque, J. Geophys. Res.
84, 5973 (1979).
32. This research was funded by Italian (Ministero
dell’Universita` e della Ricerca Scientifica e Tecno-
logica and Consiglio Nazionale delle Ricerche), Bra-
zilian (Programa da Apoio ao Desenvolvimento Cien-
´fico e Tecno´logico/Financiadora de Estudos e Pro-
jectos and Conselho Nacional de Desenvolvimento
Cientı´fico e Tecnolo´gico), and U.S. (NSF grant EAR-
9496326) agencies and the Ann and Gordon Getty
Foundation. We thank M. Iacumin, P. Antonini, M.
Hirschmann, and W. Sharp for discussions; Compan-
hia de Pesquisa de Recursos Minerais for logistical
support in sampling the Roraima dikes; C. Montes-
Lauar (Anari and Tapirapua˜) and A. Novello (Ceara´)
for providing samples; and T. Becker for argon labo-
ratory assistance. Special thanks are due to geologist
Sandoval Pinheiro for his help during fieldwork.
14 December 1998; accepted 10 March 1999
Fig. 4. Age probability spectra for CAMP (4,5,
present study) from North America (five data
samples), West Africa (20 data samples), and
South America (16 data samples). The curve
labeled “CAMP All” (41 data samples) allows
comparison of the
40
Ar/
39
Ar with the U/Pb data
by including uncertainties in decay constants,
errors in K-Ar data for
40
Ar/
39
Ar standards, and
2sanalytical errors (14). The curve labeled
“CAMP Ar/Ar” (36
40
Ar/
39
Ar data samples) in-
cludes only 1sanalytical errors and provides
the best estimate of duration of a brief mag-
matism, similar to those of the Karoo (23) and
Siberian Traps (22) CFBPs. All
40
Ar/
39
Ar data
are normalized to the same standard basis
[FCs 528.02 Ma (14)].
Fig. 5. Circles show the mean paleomagnetic
poles (95% confidence) of CAMP tholeiites of
South America (SA) (9,16,17, present data),
southern Europe (SE) (18), western Africa
( WA) [compiled by (19)], and North America
(NA) (20). The Apparent Polar Wander Path
from 300 to 125 Ma (open diamonds) for
North America is shown for comparison (30).
Rotation poles of South America to Africa
and North America to Africa are after (17)
and (31), respectively.
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Province
Extensive 200-Million-Year-Old Continental Flood Basalts of the Central Atlantic Magmatic
Andrea Marzoli, Paul R. Renne, Enzo M. Piccirillo, Marcia Ernesto, Giuliano Bellieni and Angelo De Min
DOI: 10.1126/science.284.5414.616
(5414), 616-618.284Science
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... Several second-order gravity and magnetic anomalies are noted onshore, while their origins are enigmatic (Figures 1b and 1c). In the coastal plain, abundant basaltic dikes and sills are distributed approximately in the N-S and NE-SW direction, which was caused by the syn-rifting emplacement of the Central Atlantic Magmatic Province (CAMP), the Earth's largest igneous province (e.g., Marzoli et al., 1999Marzoli et al., , 2018McHone et al., 2005). Additionally, two ancient volcanoes are found near the southern Appalachians, whose formation is thought to be associated with post-rift magmatism (Figure 1a; Mazza et al., 2014Mazza et al., , 2017. ...
... Extensive continental rifting initiated at ∼230 Ma, accompanied by the formation of multiple normal faults and rift basins (Leleu & Hartley, 2010;Withjack et al., 2013). During rifting, the CAMP was emplaced along the margin over a short period of less than 1 million years at ∼201 Ma (Marzoli et al., 1999(Marzoli et al., , 2018. The western limit of the CAMP in the SENAM runs roughly along the southern Appalachian Front interpreted as the boundary between the Laurentia craton and the passive margin, and its eastern limit could extend as far as the continental shelf ( Figure 1a; Marzoli et al., 2018). ...
... The SENAM has experienced multiple magmatic events that can lead to the emplacement of plutons within the crust (Withjack et al., 2013). Among these events, the magmatism associated with the CAMP has been interpreted to have the largest intensity and form abundant basaltic dikes along the coastal plain (Marzoli et al., 1999(Marzoli et al., , 2018. Furthermore, the horizontal distribution of high-velocity anomalies in our model roughly correlates with the CAMPrelated basaltic dikes in Virginia, northeastern and central North Carolina, and northern South Carolina (Figure 9a). ...
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The southern portion of the eastern North American margin (SENAM) is an archetypical volcanic passive margin formed during Mesozoic rifting. How past magmatic events affect the evolution of the SENAM remains an open question of fundamental importance. To better understand this question, here we construct a high‐resolution 3‐D crustal velocity model from the oceanic side to the continental interior with a combination of multimodal dispersion inversion and full‐waveform ambient noise tomography. Our new model reveals an oceanic‐continental transitional crust over a short horizonal distance of 100–150 km across the SENAM, with a local‐scale lower‐than‐surrounding velocity anomaly directly beneath the transitional crust. Furthermore, the new model shows three intra‐crustal higher‐than‐average velocity anomalies beneath the SENAM continent. We suggest that the magmatism assisted the Mesozoic rifting process to form the narrow ocean‐continent transitional crust along the coastline. The underplating of magma beneath the transitional crust led to a reduction of seismic velocity of the uppermost mantle. In addition, it is probable that the emplacement of the Central Atlantic Magmatic Province caused widespread magmatic intrusions within the continental crust of the SENAM, which were later solidified into intra‐crustal high‐velocity plutons. Our findings provide new insights into crustal modification history at the passive margin.
... During the youngest extrusive sequence, the Hampden basalt, the first flow is a sheet lobe deposited onto the soft sediments of East Berlin formation, indicating that the basin mainly was under subaerial conditions at that location. Based on different geochemistry, the three principal basaltic formations Talcott, Holyoke, and Hampden basalts correspond to 3 lava flow fields (Figure 8) [17,18,[100][101][102][103][104][105]. According to [57], the chemistry and mineralogy of the three northeasterly trending diabase dykes that cross Southern New England correlate with the three basaltic episodes of the Hartford basin. ...
Preprint
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The morphology, internal architecture, and emplacement mechanisms of the Central Atlantic Magmatic Province (CAMP) lava flows of the Hartford and Deerfield basins (USA) are presented. The Talcott, Holyoke, and Hampden formations within the Hartford basin constitute distinct basaltic units, each exhibiting chemical, mineralogical, and structural differences corresponding to flow fields. Each flow field was the result of several sustained eruptions that produced both inflated pahoehoe flows and subaquatic extrusions: 1–5 eruptions in the Talcott formation and 1-2 in Holyoke and Hampden basalts, where simple flows are dominant. The Deerfield basin displays the Deerfield basalt unit, characterized by pillow lavas and sheet lobes, aligning chemically and mineralogically with the Holyoke basalt unit. Overall, the studied flow fields are composed of thick, simple pahoehoe flows that display the entire range of pahoehoe morphology, including inflated lobes. The three-partite structure of sheet lobes, vertical distribution of vesicles, and segregation structures are typical. The characteristics of the volcanic pile suggest slow emplacement during sustained eruptive episodes and are compatible with a continental basaltic succession facies model. The studied CAMP basalts of the eastern United States are correlated with the well-exposed examples on both sides of the Atlantic Ocean (Canada, Portugal, and Morocco).
... The distension within Pangea started in the Trias with the separation between the Gondwana and the Laurentia at Late Sinemurian (Sahabi et al., 2004) and a rifting marked by the Central Atlantic Magmatic Province (CAMP), a major igneous eruptions dated about 200 Ma (May 1971;Marzoli et al., 1999;Berrocal et al., 2004). Within the Gondwana, the disruption occurred during the early Jurassic (Norton and Sclater, 1979;Paton et al., 2017;Eagles and König, 2008;Thompson et al., 2019) coinciding with the Karoo volcanism. ...
... During the Mesozoic-Cenozoic, the evolution of the Anti-Atlas is ill-established due to the lack of relevant deposits on the Anti-Atlas chain. Multiple NE-SW Lower Liassic mafic dikes bellowing to the CAMP magmatic event crosscut the Anti-Atlas, indicating the Pangea disintegration at the Triassic-Jurassic boundary (Marzoli et al., 1999). The most important is the Foum Zguid dyke through the Bou Azzer inlier. ...
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