223
Tectonophysics, 116 (1985) 223-253 Elsevier Science Publishers B.V., Amsterdam - Printed in The Netherlands
ASSOCIATED MIDDLE TO L,ATEJURASSIC VOLCANISM AND EXTElNSION IN SOUTHERN SOUTH AMERICA
D.A. GUST I*, K.T, BIDDLE *, D.W. PHELPS * and M.A. ULIANA ‘** ‘. SN4
NASA,
Johnson Space Center, Houston, TX 77058 (U.S.A.)
’ Exxon Production Research Company, Box 2189, Houston, TX 77252.2189 J Esso SAPA,
(U.S.A.)
Deiia Polera 297, 1001 Buenos Aires (Argentina)
(Received July 8, 1984; revised version accepted January 24, 1985)
ABSTRACT Gust, D.A., Biddle, K.T., Phelps, D.W. and Uliana, M.A., 1985. Associated Middle to Late Jurassic volcanism and extension in southern South America. Tectonophysics, 116: 223-253. The extrusive products of a Middle to Late Jurassic volcanic event occur throughout a wide area of southern South America. These volcanic rocks are associated in time and space with a series of NNW-trending grabens. The extension that produced the grabens began perhaps in the latest Triassic and continued throughout most of the Jurassic. The Middle to Late Jurassic volcanic rocks represent the culminating event of this period of extension. The Jurassic volcanic rocks described here are dominantly rhyolites and basal&, but flows of intermediate composition are also present. Major element gmhemistry on a suite of samples taken from a west-east transect near 44*S latitude shows that these rocks are not related directly to convergent arc volcanism along Ihe margin of South America, but are the products of a separate tectonic/magmaric event that involved significant crustal anatexis. The extension and related vokanism directly preceded the opening of the Rotas Verdes marginal basin along the western margin of Chile and may have led to the initial separation of South America and South Africa. As such, the Middle-to-Late Jurassic extension and volcanism heralded the breakup of part of Gondwanaland. INTRODUCTION
During the Middle and Late Jurassic, a major igneous event affected most of southern South America. The extrusive products of this event occur throughout an area of over l,OOO,OOOkm2 (Fig. l), and range in composition from basalt to rhyolite. Although these rocks form a major volcanic province, comparable in size to major ignimbrite provinces, little is known of their field reIations or geochemistry outside of Argentina.
* Currentaddress: Lunar and Planetary Institute, 3303 NASA Road 1, Houston, TX 77058 {U.S.A.). ** Currentaddress:ExxonProduction Research Company, Box 2189, Houston, TX 77252.2189 (U.S.A.).
OO4O-1951/85/$03.3O
0 1985 Elsevier Science Publishers B.V.
224
70”
‘40
1
66” /
I
', ,_i i
62”
:OMPLEJO
1”
NERERO’B’.#&CHON
AIKE
CHON
’
;A
AIKE
MATILDE
OUTCROP LATE JUR P VOLCANI’ C LOCATION OF WELL THATENCOUNTERED MID TO LATE VOLCANIC ROCKS IN THE SUBSURFACE
r
GROUPS FORMATIONS
SERIE TOBIFERA .
KILOMETERS
Fig. 1. Map of southern of Middle-to-Late related provides
South America
Jurassic
volcanic
to Late Triassic-Jurassic an indication
Oi;250
I 70”
1 740
showing outcrop
distribution
and selected subsurface
rocks. Also shown are zones of numerous
extension.
The distribution
of the total area affected
of the Middle-to-Late
by the extensional
I 58”
62”
66”
event.
grabens
occurrences
and half grabens
Jurassic
volcanic
rocks
225
This
volcanic
extensional
event
represents
deformation
of a number
the volcanism
were soon followed
the western
margin
of a widespread
that began in the Late Triassic
the formation
oceanic
the culmination
of basins
in southern
of Gondwanaland
crust in the South Atlantic
or Early Jurassic
South America.
by the formation (Dalziel,
(Rabinowitz
episode
and led to
The extension
of a small oceanic 1981)
and
of
basin
and along
by the formation
and La Brecque,
of
1979).
An understanding of the Middle to Late Jurassic extension and volcanism is critical for several reasons. First, these events heralded the breakup of Gondwanaland. Second, they initiated the formation of basins such as the Magallanes and Malvinas of Argentina and Chile, and, third, the associated thermal event set the stage for hydrocarbon maturation in those basins. In this paper, the Middle and present
we will summarize the complicated stratigraphic nomenclature Upper Jurassic volcanic rocks of southern South America,
new petrographic
traverse
near
44”s
and geochemical
latitude.
Using
analyses
of samples
this information,
from a west-east
in concert
interpretations based on previous work and subsurface data, tectonic significance of this period of extension and volcanism.
of and
with
structural
we will discuss
the
STFUTIGRAPHY
Pre-Lower
Triassic stratigraphy
The volcanic rocks discussed here overlie a heterogeneous assemblage of sedimentary, metamorphic and igneous rocks which range from possibly Precambrian to Early Jurassic. Basement rocks include Precambrian(?) to Permian gneisses and amphibolites; pre-Silurian phyllites, slates, and metamorphosed volcanic rocks; and Silurian-Devonian to Lower Carboniferous schists (Gonzalez Bororino and Aguirre, 1970; Halpern, Riccardi represent
and
1973; Natland Rolleri,
1980;
the products
margin (present-day Permian. In limited
areas
et al., 1974; Miller, Herve
of episodic
coordinates)
subduction
and
of Gondwanaland
west of 69”W
1976; de Guisto
et al., 1981). The
longitude
basement
accretion
et al., 1980;
rocks along
probably
the western
from the latest Precambrian
the crystalline
to
basement rocks are elastics, tillites and Rio Genoa
overlain by a series of Upper Carboniferous and Permian continental and rhythmically bedded marine sedimentary rocks (e.g., the Tepuel
Groups in Argentina and the Panguipulli Formation in Chile). The erosional remnants of these rocks define a narrow basin that trends obliquely across Patagonia (Suero, 1961; Lesta and Ferello, 1972). This basin has been recently interpreted as a forearc basin by Herve et al. (1981) and Forsythe (1982). Permian to Lower Triassic plutonic and volcaniclastic rocks east of 70°W longitude document the southern extension of the well-known late Paleozoic magmatic arc of western Argentina and Chile (Polanski, 1970; Herve et al., 1981;
LATE PALEOZOIC FORE-ARC BASIN OF
-
Ml”
TO
LATt J”HA>blL VOLCANIC ROCKS
G&p?~
-PALEOZOIC TRENDS
STRUCTURAL WHEMATICI
KILOMETERS I 74
Fig. 2. Distribution Jurassic
volcanic
of Late Paleozoic-Early rocks.
o-
/ 70”
66”
Mesozoic
tectonic
250 62”
belts and superimposed
I 580
Middle
to Late
221
Forsythe,
1982). The locations
belt of igneous
activity
in the central
at least 500 km wide (Nunez and Methol,
1980; Cortes,
The distribution superimposed
1981; Forsythe,
of Paleozoic
Patagonia,
regional
cini, 1968; Stipanicic, occurrences
and eastern
and
rocks define
parts of northern
Upper
Patagonia
that is
1975; Lesta et al., 1980; Stipanicic
trends
and
the known
extent
rocks are illustrated
Triassic
and
Lower
Jurassic
of the
in Fig. 2.
rocks
that cuts into the rocks described
1969), and are mostly confined
in fault-bounded
trending
stratigraphy
unconformity
or half grabens.
a northwest
1982).
older
Middle and Upper Jurassic volcanic
In northern
grabens
granitic
et al., 1975; Ramos,
Upper Triassic- Lower Jurassic
pronounced
of dated
depressions.
rest
on a
above (Bracac-
to thick, but areally restricted
Seismic data show these depressions
They are filled with continental
sedimentary
to be
rocks, local
marine Liassic rocks and volcanic rocks of various types. The Upper Triassic and Lower Jurassic stratigraphy of Patagonia has been summarized by Stipanicic (1969), Stipanicic and Bonetti (1969, 1970a, b), Stipanicic and Rodrigo (1970a, b), Lesta et al. (1980), de Giusto et al. (1980), and Cortes (1981). Upper Triassic and Lower to Middle Jurassic
volcanic
rocks
are
common
throughout much of southern South America, and are related to the slightly younger volcanic rocks discussed here. In northern Patagonia the Upper Triassic Los Menucos and Garamilla Formations include rhyolitic, rhyodacitic, and dacitic ignimbrites, tuffs and lapillites (Stipanicic and Methol, 1980; Pesce, 1976; Nullo et al., 1978; Coira, 1979). To the south units of the same general stratigraphic position yield Late Triassic floras and locally include basaltic flows and sills (de Giusto et al., 1980). In the eastern Formation
part of northern
is composed
Patagonia,
of tuffs, volcanic
the Lower Jurassic
agglomerates
and
rhyolitic
Puesto
Piris
ignimbrites
(Nunez et al., 1975), which have been dated by the K-Ar method as 189 + 5 Ma (Cortes, 1981). Other Lower Jurassic, volcanic-rich units include the El Cordoba Formation (Panza and Zaccomani, 1981), the Puntudo Alto Formation 1981) and the Sanico Formation (Gulisano and Pando, 1981). Pliensbachian to Bajocian (Lower to Middle Jurassic) tuffs,
(Musacchio, volcanic
ag-
glomerates, and rhyolitic ignimbrites of the eastern Somoncura massif have been described as the La Porfia Formation (Cortes, 1981). The equivalent Los Martires Formation to the south has yielded radiometric dates (K-Ar) of 176 it 10 Ma and 172 f 10 Ma from andesites and rhyolites (Pesce, 1978). To the west, close to the Andes, lower Middle Jurassic rocks of the Carnerero Formation are dominantly andesitic (Musacchio, 1981). Unfortunately, the paucity of diagnostic fossils and marker beds makes correlation of the older Mesozoic units between isolated outcrops difficult. As a result, in poorly exposed areas where massive volcanic rocks are dominant, these units and the younger Jurassic volcanics cannot be easily distinguished.
228
Middle and Upper Jurassic volcanic rocks The stratigraphic terminology South America is complicated. between
the volcanic
la Patagonia, named
designation, describe
Cuarciferos
and ignimbritic
which he called the Complejo volcanic
Tobifera
volcanic
An informal rocks,
broadly
rocks of Middle
used
by many
to Late Jurassic
de
which he
stratigraphic
has been used to
of these rocks in the Magallanes
has been
Porfirico
rocks of the Andes
de la Cordillera.
or simply
occurrence term
to the Jurassic volcanic rocks of southern (1949, 1950) initially drew a distinction
time-equivalent y Porfiritas
Serie Tobifera
the subsurface
1949). The informal rhyolitic
rocks of Patagonia,
and the roughly
Porfiros
applied Feruglio
Basin (Thomas,
workers
to describe
age throughout
southern
South America. In the recent literature, Middle and Upper Jurassic volcanic rocks are commonly referred to as lithostratigraphic units of group rank (Bahia Laura Group, Marifil
Lonco Trapial Group, Lago la Plata Group, El Quemado Complex). Numerous formational names have been proposed
Complex, and to account for
area1 changes in the dominant composition of the volcanic pile. The current stratigraphic nomenclature is summarized in Fig. 3. We will use the term mid-Jurassic volcanic rocks when referring to these rocks in a general sense. However, when referring to a specific locality, we will use the appropriate group name. The relationships between the various units shown on Fig. 3 are poorly understood primarily because of complexities caused by rapid lateral changes in thickness and facies (Bruhn et al., 1978; de Giusto et al., 1980). In some areas the combinations of eruptive and sedimentary processes produced unconformable relationships with only limited chronologic
significance
(Lesta and Ferello,
1972). These peculiari-
ties and the general lack of detailed studies limit many of the stratigraphic subdivisions to only local importance (Riccardi and Rolleri, 1980). As a consequence, ideas on regional
trends
of lithologic
and petrographic
composition
obtained
ture surveys are necessarily a crude first approximation. Radiometric ages obtained by K-Ar dating of the mid-Jurassic cluster at 160 Ma and outline
an episode of dominant
activity
between
from literavolcanic 155-165
suite Ma
(Stipanicic and Bonetti, 1970a; Creer et al., 1972; Codignotto et al., 1978; Pesce, 1978; Lesta et al., 1980; Cortes, 1981). Along the North Patagonian-Andean belt the complex is thought to include some younger, Late Jurassic rocks (Haller et al., 1981; Haller and Lapido, 1982) although Late Cretaceous granitic intrusives preclude reliable K-Ar dating of the volcanic rocks in this area. The available stratigraphic and radiometric ages indicate a pronounced increase in eruptive activity in Patagonia both in volume and in area1 extent in the late Bajocian (Lesta and Ferello, 1972). This phase lasted about lo-15 Ma with volcanism persisting until early Callovian-Oxfordian times (Tithonian?) to the west in Leanza, 1968; Ramos et al., During the accumulation
in eastern Patagonia and into the latest Jurassic some segments of the Andean belt (Feruglio, 1936; 1982). of the mid-Jurassic volcanic rocks, depositional sites
229
r
40’
PI N
44
,,ZOl+ODORO
_
RIVADAVIA
PUERTO
DESEADO
AND JURRASSIC 4f
5:
KILOMETERS I
Fig. 3. Stratigraphic
nomenclature
I
for Middle to Late Jurassic
01
y-250 _~
volcanic
rocks of southern
I
South America.
230
covered,
without
accumulation mid-Jurassic Paleozoic
major
discontinuities,
occurs within volcanic
basement.
Within
the troughs,
Jurassic
volcanic
volcanic-rich
between
the Triassic
and
volcanic
rocks is disputed
Lower
however,
the boundary
early
(Lesta and Ferello,
chio, 1981; Franchi and Page, 1980). Prevailing ideas on the composition
graben
location fill and
1972; de Giusto
of the mid-Jurassic
Thickest
the grabens,
the
discontinuity
on
is not always clear
conformable
In some instances, Jurassic
Outside
and structural
rocks are nearly
units.
South America.
grabens.
rocks rest with sharp lithologic
cut since the mid-Jurassic Lower
most of southern
Late Triassic-Jurassic
on Triassic
and
of the boundary the mid-Jurassic
et al., 1980; Musac-
volcanic
rocks in northern
Patagonia indicate a dominance of silicic (rhyolitic) extrusives in the eastern outcrops of the Somoncura area (upper part of the Marifil Complex, Cortes, 1981) with a gradual change to andesites, basaltic andesites and basalts to the west (Lesta et al., 1980). In most areas, the mid-Jurassic suite is composed of a complex mixture of flows, pyroclastics. ash-flow tuffs and reworked volcanic and non-volcanic detritus (e.g., Mazzoni et al.. 1981). Close to the Atlantic Coast
ignimbrites
massive
and Llambias,
units (Fig. 4) (Malvicini
form
a broad
plateau
consisting
1974). This suite includes
of
rocks of
trachytic, rhyodacitic and rhyolitic composition and is known to occur in the eastern Rio Negro area (Malvicini and Llambias, 1974; Cortes, 1981) eastern Chubut (Lesta
Fig. 4. Massive ignimbrite flows of the Lonco Trapial Group exposed in the valley of the Chubut River.
231
et al., 1980; Creer et al., 1972), eastern et al., 1981) and the southernmost Sparse subsurface
control
1973), Magallanes
(Natland
support In
the regional
in the eastern
Chubut,
south
complex
is referred
Canadon
Puelman
Formations,
(Lesta rhyolitic
San Jorge (Lesta,
of the
to as Lonco
Lesta and Ferello,
by olivine
ignimbrites
the Chubut
andesite (Panza
Massif,
the
(Cajon
with cogenetic
the mid-Jurassic
1981)
tends to
mid-Jurassic
de Ginebra
1972) and is reported
flows and andesitic-dacitic
and Zaccomani,
basins
trend.
Group
and basalts River,
et al., 1978).
1970; Lesta and Bianchi,
Somoncura Trapial
to basic suite of andesites
et al., 1980). Near
represented
et al., 1980; Mazzoni
et al., 1974; Bruhn
of this eastern compositional
volcanic
an intermediate
(Dalziel
et al., 1974; Riggi, 1969) and Malvinas
continuity
north-central
Santa Cruz (de Giusto
Andes
and
to consist of volcaniclastics
volcanic
ignimbrites,
suite
overlain
and locally covered
is by
by a group
of olivine basalts (Null0 and Proserpio, 1975; Pesce, 1978). The compositional change from the silicic ignimbrites in the east to the intermediate and basic members of the Lonco Trapial occurs gradually around 67”3O’W (Lesta et al., 1980). Farther west, the central Chubut suite can be followed to 70”3O’W into the andesites and basaltic-andesites of Sierra de Tepuel (Haller et al., 1981). In outcrops along the Andean belt located north of 44’S, the Middle to Late Jurassic event is represented by andesites overlain by dacites and rhyodacites (Lago la Plata Formation, Haller and Lapido, 1982). At about 46”S, the volcanic complex is described (Ibanez
as a bimodal
Formation-Baker
suite of basaltic-andesite
lavas and rhyolitic
et al., 1981). South of 46”s
ash-flow
the proportion
tuffs
of andesite
decreases (Ramos et al., 1982). In the Andean outcrops from 47”s to Tierra de1 Fuego, the volcanic package is a series of rhyolitic to rhyodacitic rocks (Lemaire Formation,
Tobifera
flows and volcanic complex
volcanics-Bruhn agglomerates
et al., 1978; Ramos
have been described
north of Lago San Martin
at 48”3O’S (El Quemado
1978); the upper part of the complex Plutonic mid-Jurassic 41’S
(granitoid) bodies volcanic complex
and usually
is a mixture
et al., 1982). Andesitic
only in the lower part of the
of dacitic
Complex-Nullo and rhyolitic
with radiometric ages roughly are reported along the Andean
lie west of the line of volcanic
outcrops
et al., tuffs.
equivalent to the belt from 52”s to
(Nelson
et al., 1980).
However, away from the Andes, most of the studied and dated plutonic rocks of Patagonia seem to be either older or younger than the mid-Jurassic volcanic episode (Lesta et al., 1980). PETROLOGY
A suite of 35 samples of the mid-Jurassic volcanic suite was acquired during this study. Twenty-eight of the samples come from a west-east traverse that runs from the crest of the Andes across the Somoncura Massif to the Atlantic coast of Argentina (Fig. 5). Seven samples come from the Deseado Massif near the town of Puerto Deseado (Fig. 5).
this study.
Fig. 5. Location
map showing
740 w
outcrop
distribution
of Middle
to Late Jurassic
70” w
volcanic
rock> in north-central
Patagonia
660 w
of samples
analyzed
KILOMETERS
DESEADO
and location
PUERTO
MID JURASSIC VOLCANIC ROCKS
in
233
Petrography The basalts and morphosed
andesites
to lower greenschist
character.
of the sampled
facies but preserve
The effects of this metamorphism
ment of olivine mineral
basaltic
and
phenocrysts
by chlorite,
of the mafic
phenocrysts
are occasionally
saussuritized
groundmass
of some samples. Alteration
phases
rocks
are meta-
much of their original
are generally
serpentine
chloritization
volcanic restricted
pseudomorphing
of the original
in the groundmass.
and small patches
igneous
to the replacePlagioclase
of zoisite occur in the
of these rocks in near-surface
environments
is recorded by the presence of calcite and zeolites. The samples retain igneous textures that range from aphyric and intersertal (glass replaced by chlorite) to porphyritic and intergranular to sub-ophitic (Fig. 6). Olivine, clinopyroxene and plagioclase typify the phenocryst assemblages. Olivine phenotrysts, when not replaced by metamorphic minerals, are euhedral to subhedral with thick iddingsite rims. Clinopyroxene phenocrysts are complexly zoned and twinned. Basaltic Plagioclase phenocrysts have sieve textures, and are usually corroded. andesites
have more plagioclase
than the basalts
and contain
olivine
quartz xenocrysts with clinopyroxene reaction rims (Fig. 6). The few andesites that were sampled possess similar metamorphic
and embayed characteristics
as observed in the mafic rocks. Original igneous textures are somewhat obscured by metamorphism (probably due to the high glass content of the original andesite) and are restricted primarily to phenocryst mineralogy and morphology. Plagioclase, clinopyroxene and amphibole are common phenocryst phases in the mafic andesites and are joined by quartz and alkali feldspar in high-silica andesites. High-silica andesites also contain lithic fragments of volcanic origin, suggesting a pyroclastic origin. Rhyolites and dacites are petrographically similar and include all varieties of crystal and lithic tuffs (Fig. 6). Original igneous textures are preserved in all samples to some degree-if banding,
flattened
only by pseudomorphs glass shards
(Fig. 6). In many samples
and welded
of phenocrysts. textures
Trachytic
are observed
these textures have been obscured
textures,
flow
in some samples
by devitrification
of the
groundmass glass to a dense, cryptocrystalline assemblage of quartz and alkali feldspar. Most samples exhibit a pervasive iron stain due to alteration of iron oxides and some also contain veins of quartz and patches of calcite. Broken,
euhedral
to subhedral
phenocrysts
of alkali feldspar,
plagioclase
feldspar
and quartz are present in varying proportions in the rhyolites and dacites. Quartz phenocrysts are often embayed and feldspars are sericitized or saussuritized but preserve optical evidence of oscillatory zoning, complex twinning and perthitic textures. Biotite and amphibole occur in only minor amounts and are rimmed to variable extents by fine-grained aggregates of opaque oxides and silicate minerals. Muscovite, apatite and zircon are rare phenocryst phases. Lithic fragments which are included in some rhyolites generally possess volcanic textures and are probably rhyolitic, although some fragments are pieces of coarse-grained granitoids.
234
235
Geochemistry Major elements, Assay Laboratory
Rb, Sr, and Zr were analyzed by X-ray fluorescence by X-ray of Canada. In addition, loss on ignition (LOI) was also de-
termined.
Selected analyses
calculated
on a volatile-free
contain
less than
are presented
in Tables
1 and 2 along with CIPW norms
basis with Fe0 adjusted
2.0% LO1 and
appear
to 0.85 total Fe. Most samples
to be relatively
fresh;
however,
several
samples, mostly basalts, contain up to 10.0% LOI. Samples with LO1 greater than 7.0% have not been included in Tables 1 and 2. Several rhyolites were significantly altered by silicification resulting in greater than 80 wt.% SiO,. The samples are classified on a chemical basis (volatile-free) Peccerillo basaltic
and Taylor andesites,
(1976) (Fig. 7). The rocks comprise
potassic
rhyolites,
and high-Si
abundant, are high-K varieties. The analyzed basalts are hypersthene
a bimodal
dacites.
normative
using the scheme of suite of basalts,
Andesites,
tholeiites.
which are not
One basalt
is slightly
quartz normative (possibly an artifact of the Fe0 recalculation procedureSchwarzer and Rogers, 1974) (Table 1). Examination of the normative An (100 An/An + Ab) of the basalts with respect to their normative hypersthene contents suggests that sodium has been enriched through low-grade greenschist metamorphism (Lipman and Mehnert, 1975). Similar sodium enrichment has been reported from altered basalts and spilites (Smith, 1968; Valiance, 1969). Thus, the alkali contents
of these rocks probably
do not reflect the original
chemistry
of the magma.
In a similar sense, burial metamorphism has altered CaO and MgO contents, so that they exhibit an inverse relationship (Smith, 1968). TiO, contents are relatively low and exceed
1.2 wt.% only in rocks with low Mg numbers,
indicating the evolved character than 16.0 wt.%) in all basalts. The basaltic tions varying
andesites between
of those magmas.
(52-55
wt.% SiO,)
Al,O,
(Mg/Mg
contents
are fairly mafic with MgO concentra-
3.5 and 6.5 wt.% and Mg numbers
of 50-63.
are highly variable suggesting that these rocks, like the basalts, metasomatism accompanying burial. Abundances
of Rb, Sr and Zr in the basalts and basaltic
Fig. 6. Photomicrographs photographs A. Basaltic trysts
of selected samples
illustrating
well-preserved
Alkali contents were affected
andesites
volcanic
by
are comparable
textures.
Scale bar in all
is equal to 5 mm. andesite
with fine-grained
of sieve-textured
plagioclase,
B. Crystal-rich
welded rhyolitic
alkali-feldspar.
Small lithic fragments
talline mixture
of quartz
C. Crystal-rich
rhyolitic
embayed
+ Fe x loo),
are high (greater
groundmass
and embayed
of plagioclase, xenocrysts
tuff with phenocrysts
clinopyroxene,
of quartz
of biotite,
quartz,
are also visible. Groundmass
and opaques,
with pyroxene
reaction
zoned plagioclase
glass has been altered
and embayed to a cryptocrys-
and feldspar. tuff with
large
altered
glass
shards
and
phenocrysts
of alkali
feldspar
quartz.
D. Dense rhyolite,
pheno-
rims,
possibly
obsidian
with large euhedral
phenocrysts
of alkali feldspar
and biotite.
and
CIP w “Otm (
4.12 31.70 33.12 7.60 15.99 _ 2.17 0.55 _
2.25 0.56 3.16
12.18 33.43 15.44 11.19 18.17 _
10.53 2.24 0.48
0.99 6.09 19.86 33.22 23.43 _
_ 2.47 49.67 22.73 18.43 1.55 0.26 0.74
_ 13.32 28.69 27.26 11.88 1.88 8.75 3.72 1.50 _
_
59 31 20 1600 70 40
99.95
49.5 0.76 18.4 8.35 0.14 5.57 4.41 5.78 0.39 0.11 6.54
14
11.08 26.67 27.17 17.01 3.17 7.23 3.30 1.33
45 49 60 700 180 80
99.04
49.0 1.86 17.1 9.40 0.09 3.49 8.01 3.22 2.14 0.65 4.08
23
2.81 12.52 28.11 28.97 13.07 8.37 2.48 1.27
14.58 1.36 0.25
50 51 50 840 200 90
99.55
52.1 1.26 17.7 7.62 0.06 3.52 8.26 3.20 2.04 0.56 3.23
21
6.18 6.88 15.21 31.70 20.88 _
0.85XFe.
6.64 34.93 30.01 6.05 6.30 11.61 1.88 0.49
_
60 67 50 310 130 150
100.19
99.86 63 46 40 370 120 40
52.6 0.70 15.5 9.59 0.15 6.43 9.90 1.76 1.14 0.11 2.31
13
52.0 0.97 18.6 6.72 0.09 5.12 9.00 4.04 1.10 0.22 2.00
33
a Mg number = 100 Mg/Mg + 0.85 Fe b An = 100 An/An + Ab ’ Norms are calculated using analyses summed to 100%. volatile free. with Fe’+=
AP C
HYP 01 Di 11
Ab An
Qtz Qr
_
59 63 20 360 110 120
69 32 50 520 60 140
56 50 50 670 160 140
98.89
99.66
98.81
99.83
Mg number ’ Anb Bb (ppm) Sr Zr Cr
Sum
LO1
p205
K2O
MS0 CaO Na,O
MnO
Fe203
57 51 10 290 60 130
1.66 16.4 9.61 0.12 5.61 7.62 3.01 1.79 0.58 3.39
1.12 16.3 9.93 0.16 6.42 9.08 2.23 0.98 0.21 4.62
1.11 17.0 9.35 0.14 9.48 3.20 3.70 1.93 0.24 5.16
1.05 17.5 10.3 0.21 6.35 6.71 3.44 0.64 0.23 8.00
-’
A1203
49.1
25
TiO;
4
48.6
1
41.5
(wt.%\ 45.4
SiO,
Sampie number: 16
7.94 2.69 0.86 _
3.15 0.81 36.69 26.88 18.49 _
60 42 20 730 180 110
99.94
51.8 1.34 16.2 7.79 0.13 5.27 7.42 4.10 0.13 0.37 5.39
2
11.21 1.89 1.06 _
5.44 14.08 22.79 23.27 17.50 _
55 50 80 600 120 190
99.15
53.6 0.96 15.0 8.81 0.12 4.93 7.74 2.60 2.30 0.47 2.62
22
Major and trace element analyses and CIPW norms of basal& and andesites from the Lonco Trapial and Bahia Laura groups
TABLE 1
6.93 2.53 1.Ol
8.16 12.80 29.32 23.92 12.98 _
49 45 70 730 170 90
99.72
55.7 1.29 16.3 7.49 0.09 3.32 6.85 3.36 2.10 0.45 2.17
20
1.90 0.52 3.24
10.03 19.81 31.82 10.56 19.84 _
57 25 170 230 210 30
99.12
57.4 0.96 16.2 7.21 0.24 4.37 2.31 3.60 3.21 0.23 3.39
3 18
14.91 23.98 29.44 14.09 8.67 _ _ 2.84 1 .Oh
25 32 170 410 330 20
98.86
60.5 1.45 14.8 7.21 0.09 1.10 3.94 3.37 3.93 0.47 2.00
237 TABLE 2 Major and trace element analyses and CIPW norms of rhyolites from the Lonco Trapial and Bahia Laura groups Sample Number: SiO, (wt .%I TiO, A’ ~0s Pa@, MnO
19
27 78.8 0.12 10.9
28
35
77.5 0.16 10.2
75.9
15.7 0.23
0.15 12.4
11
9
11.4
75.9
74.3 0.30
0.29 11.2
29
12.5
6
15
75.1 0.19 13.3
74.5 0.35 13.0
74.0 0.25 11.8
0.46
0.31
0.66
0.80
1.43
1.23
0.42
1.30
2.25
0.01
0.01
0.01
0.01
0.01
0.01
0.01
0.02
0.01
MSG CaO
0.08
0.03
0.17
0.07
0.34
0.23
0.01
0.26
0.23
0.14
0.82
0.21
0.25
0.39
0.36
0.09
1.50
0.36
Na,O
1.79
1.57
0.33
0.23
0.48
3.10
3.76
3.93
2.07
K,G
5.80
6.59
7.45
8.67
7.56
5.57
5.81
3.80
6.98
PsG, LO1
0.02
0.34
0.04
0.02
0.07
0.08
0.02
0.16
0.04
1.23
1.00
1.31
1.39
1.39
1.23
0.62
1.16
1.39
Sum
99.35
98.53
98.63
98.77
99.06
98.91
99.33
99.98
99.38
250
230
340
310
380
220
290
140
Sr
20
50
120
60
10
90
30
290
20
Zr
90
130
90
230
130
160
240
260
410
Bb (ppm)
210
UP w nOrm* Qz
46.50
43.36
45.80
41.36
43.38
34.32
31.12
33.70
33.77
Or
34.93
39.93
45.24
52.61
45.74
33.70
34.78
22.71
42.09 17.87
Ab
15.44
13.62
2.87
2.00
4.16
26.85
32.23
33.71
An
0.59
1.36
0.83
1.15
1.56
1.35
0.33
6.59
1.58
HYP
0.63
0.48
1.08
0.87
2.28
1.73
0.29
2.13
3.14 0.48
I1
0.23
0.08
0.29
0.45
0.56
0.58
0.37
0.31
AP
0.04
0.31
0.09
0.04
0.16
0.18
0.04
0.35
0.09
C
1.49
0.76
3.59
1.26
1.71
0.91
0.71
0.04
0.38
Sample Number: SiO, (wt .%I TiO, A’@,
30
32
73.4 0.12 14.8
73.2 0.15 14.8
26
7
72.5 0.23 13.8
34
71.4 0.40 14.0
5
70.7 0.28 14.6
66.7 0.42 15.7
AGV-1
AGV-lb
58.9
59.0
1.03 16.9
1.04 17.25
Pesos MnO
0.95
0.52
1.65
2.08
2.75
3.26
6.76
6.76
0.02
0.01
0.04
0.02
0.07
0.02
0.09
0.09
MS0 CaO
0.33
0.33
0.18
0.36
1.25
0.79
1.49
1.53
1.20
1.29
0.30
1.31
1.91
2.67
4.93
4.90
Na,O
4.31
4.89
3.36
4.24
4.32
3.77
4.28
4.26
K,G
3.34
3.54
5.98
4.46
2.17
3.65
2.84
2.89
p20,
0.06
0.09
0.03
0.12
0.18
0.30
0.47
0.49
LOI
1.08
0.93
1.16
1.54
1.77
2.85
1.85
1.27
Sum
99.61
99.75
99.23
99.93
100.00
100.13
99.54
99.48
238 TABLE
2 (continued) ._
_.__._____
Sample Number:
30
32
26
7
34
Bb (ppm)
120
100
220
120
130
5 70
AGV-I 70
AGV-1 h 61
Sr
660
570
110
230
550
560
750
657
Zr
70
110
300
260
90
250
240
225
(‘IP w nor* d
Qt7
32.62
28.30
28.96
26.11
30.85
Or
20.03
21.17
36.03
26.79
13.05
22.17
Ab
37.01
41.87
28.99
36.46
37.21
32.79
An
5.68
5.94
1.34
5.89
x.57
11.80
HYP
1.92
1.29
2.31
3.00
6.43
5.65
II
0.23
0.29
0.45
0.77
0.54
0.82
AP
0.13
0.20
0.07
0.27
0.40
0.67
C
2.07
0.78
1.35
0.08
2.10
1.38
a Norms
are calculated
using analyses
h Values from Flanagan
summed
23.70
to 100%. volatile free with Fe2 ’ = O.RSXFe
(1973).
to some island arc basalts (Perfit et al., 1980) and tholeiites from flood provinces, such as the Karoo and Parana (Basaltic Volcanism Study Project, Characterization of the tectonic setting of the Lonco Trapial and Bahia basalts using the available immobile trace elements data (Ti and Zr-Pearce
basalt 1981). Laura and
Cann, 1973) is ambiguous because continental and oceanic within plate basalts exhibit a broad range of Ti and Zr contents that encompass and extend beyond the ocean floor and talc-alkalic basalt discriminant fields. The andesites are high-K varieties but do not compare kalic high-K (Bailey,
andesites
1981). TiO,,
from erogenic
regions
well with typical
(Gill, 1981) or Andean-type
Pz05, Rb, and Zr contents
are higher
calc-alandesites
and CaO contents
are
much lower in the andesites of the mid-Jurassic suite versus erogenic, talc-alkalic andesites. The high Rb may be an artifact of metamorphism; however the high Zr, TiO,
and P20, are probably
primary
magmatic
characteristics.
The mid-Jurassic silicic suite consists of talc-alkalic and high-potassium rhyolites (Fig. 7). The talc-alkalic rhyolites are restricted to the Deseado Massif, and the high potassium rhyolites were sampled in the Somoncura region. Both are peraluminous, suggesting that both types are equivalent to S-type granites (Chappell and White, 1974). However, the relatively low Zr contents (approximately 100 ppm) and high Sr contents (500 ppm) of the talc-alkalic rhyolites are more similar to I-type granites. The geochemistry of the talc-alkalic rhyolites compares favorably with erogenic talc-alkalic rhyolites (Ewart, 1979). The high-potassium rhyolites are most like rhyolites from extensional environments involving anatexis of continental crust (Hildreth, 1981). Two types of low-temperature burial metamorphism occur in the rhyolites. The
1.0 -
2.0 -
3.0 -
4.0 -
5.0 -
andesites
samples
.
SAMPLES
SAMPLES
TRAPIAL
SHOSHINITE
LAURA
GROUP GROUP
rocks by K,O
AND
Deseado
possess
a talc-alkahc
DACITE
119761
,
,
DACITE
character.
Deseado
, 70 0
proposed
*
.
LOW-K
-
by Peccerillo
+
region. The suite is essentially
using divisions
WT%
65.0
I
LOW-K
(CALC-ALKALICI
DACITE
HIGH-K
& TAYLOR
SO2
contents
from the Puerto
and SO,
.
PECCERILL~
ANOESITE
EANAKITE
HIGH-K
and crosses are samples
volcanic
I-K EAS.
from Puerto
traverse
Samples
from our west-east
and rhyohtes.
LONCO
BAHIA
_+.s
FROM
FROM
of mid Jurassic
ABSAROKITE
+
Fig. 7. Classification
:
f
6.0 -
7.0 -
6.0 -
g’oc
l-
75 0
I
,
bimodal,
I
60 0
I
.
2
I
into basalts
Filled circles
I
being divisible
(1976).
.
RHYOLITE
ICALC-ALKALICI
LOW-K
l+
RHYOLITE
RHYOLlTE
HIGH-K
. .
and Taylor
.
.
to
are
6.00
-
5.00
-
4.00
-
3.00
-
0
LONCO
TRAPIAL
+
BAHIA
LAURA
!
WITH
Si02
> 65 WEIGHT
?+
GROUP
+
+ ae
SAMPLES
GROUP
+ 0
N
s
l
2 .oo
1 .oo
I 0.00
I
I
I
0 00
1 .oo
I
2 .oo
3 .oo
I
I 4.00
5.00
K20
Fig. 8. Plot of Na,O
versus
these alkali abundances
K,O
suggests
for samples potassium
I
I
I
6 .oo
7.00
8 .oo
0 9.00
WT%
with
> 65 wt.% SO,.
metasomatism.
Symbols
The negative
correlation
between
as in Fig. 7.
most prevalent type is not petrographically apparent and involves the replacement of sodic plagioclase by potassic feldspar, resulting in an increase in K ,O and a decrease in Na,O contents (Fig. 8) (Izett, 1981). Similar alteration has been noted in Tertiary rhyolites from the Mogollon-Datil volcanic province in New Mexico where K,O may be as high as 13.5 wt.% (Chapin et al., 1978; Chapin and Glazner, 1983). Chapin
and Glazner
(1983) have shown that unaltered
rhyolites
from the Mogollon-
Datil field rarely have K,O contents greater than 6.0 wt.% and K,O/Na,O values greater than 3.0. Bahia Laura and Lonco Trapial rhyolites, on the other hand, have K,O/Na,O
values which range from 0.5 to 27, indicating
potassium
metasomatism
in the rhyolites with K,O/Na,O greater than about 13. The positive correlation of Rb and K,O indicates that Rb has also been affected by this metasomatic event. The second type of alteration involves leaching of K,O from the rock. Thus, rhyolites that have high LOI totals (greater than 7.0 wt.‘%) also have low K,O contents. CaO and Sr contents are enriched in these samples which also contain significant modal calcite. Petrogenesis It is difficult to propose a detailed petrogenetic scenario for the mid-Jurassic suite of basalts and basaltic andesites on the basis of the data we have collected.
241
Alteration of the basalts has been shown to modify the original magmatic character of the rocks. It is also likely that these basalts experienced fractional crystallization prior to eruption, further obscuring information about their source. Geochemical similarities between the suite of mid-Jurassic basalts and basalts from flood basalt provinces suggest that their petrogeneses may also be similar. We cannot however evaluate whether these basalts are derived from tholeiitic or picritic primary magmas (Cox, 1980) or to what extent their chemistry has been influenced by crustal contamination. We believe that the geochemistry of the Lonco Trapial and Bahia Laura basalts is consistent with that expected within extensional environments. The whole-rock chemical analyses of the mid-Jurassic rhyolites suggests anatexis of crustal material. The least altered of the mid-Jurassic rhyolites are plotted in Fig.
WT.
PERCENT
ALBITE
ORTHOCLASE
Fig. 9. Experimentally-determined
phase relations in the quartz-albite-orthoclase
water pressure (from Tuttle and Bowen, 1958) with normative compositions rhyolites points.
superimposed.
Calc-alkalic
rhyolites
from the Puerto Deseado
ternary at 1 kb and 5 kb
of least-altered
mid-Jurassic
region are the three leftmost
242
9 on the normative Qz-Ab-Or ternary (weight percent). The talc-alkalic rhyolites from the Deseado Massif and some of the potassic rhyolites lie near the minimum melt composition
expected
for pressures
19.58). A number
of high potassium
may reflect a shift in the minimum Ah/An
ratio
Jurassic
rhyolites
of the parent
in this diagram
anatexis
of crustal
materials
between
rhyolites
1 kb and 5 kb (Tuttle
also fall along the Qz-Or
melt composition
decreases
(Winkler,
is consistent
and Bowen, cotectic
and
from the left to the right as the 1979). The behavior
with a petrogenesis
whose major components
are quartz
of the midinvolving
the
and feldspar.
The
S-type characteristics of these rhyolites suggests anatexis of sedimentary source material (Chappell and White, 1974) and is consistent with our structural interpretations (see following section). This inference is also supported by the field observation of a lack of any parental material from which the rhyolites may have been derived by fractional crystallization. The differences observed between the calc-alkalic rhyolites of the Deseado Massif and the high-K rhyolites of the Somoncura region may reflect differences in their crustal sources. A possible scenario of the petrogenesis of the mid-Jurassic volcanics rocks (i.e., large volumes of silicic pyroclastics associated with small volumes of basalt and intermediate rock types) is one of an extremely energetic magma system under stress conditions favoring marked crustal extension (Hildreth, 1981). In this model, basalts generated by partial melting of the mantle are ponded at the base of the crust erupting only infrequently. This input of hot material into the crust causes melting, which in an extensional
regime, develops
large silicic magma
chambers.
Eventually,
these chambers rupture and large volumes of pyroclastic material are ejected. chemical or petrologic relationship exists between the silicic and basaltic rocks. EXTENSIONAL
DEFORMATION
Both stratigraphic preceded
No
and
and accompanied
structural
evidence
the volcanism
show that
described
above.
extensional
deformation
This extensional
event
produced numerous north-northwest-trending fault-bounded troughs in Patagonia and Tikrra de1 Fuego (Fig. 1). Most of these are half grabens with the faults on the eastern sides generally showing the largest displacements. The half grabens are best seen on seismic data from the Magallanes, Malvinas and San Jorge basins, but also have surface expression on the Deseado Massif. Here, a northwest-trending narrow depression is filled with Lower Jurassic and uppermost Triassic sedimentary and volcanic rocks (Bracaccini, 1968; de Giusto et al., 1980). In the Magallanes, western San Jorge and Malvinas basins, thick, areally restricted graben fill underlies well dated Upper Jurassic marine sedimentary rocks. The faults that form the grabens are steeply dipping normal faults, some of which have listric profiles at depth. These faults display several different relationships with the mid-Jurassic volcanic rocks that, together with the stratigraphic data, provide information on the timing of extension.
243
Most of the normal thinner
high-side
volcanic-rich
faults separate
accumulations.
section has been sampled
little as 20 m of equivalent few show limited
displacement
rocks are confined
horst block is devoid mid-Jurassic volcanic
low-side
by drilling
section is present
Most of these faults die out upward volcanic
thicker
volcanic-rich
As much as 2000 m of Middle
sections
to Upper
on the low side of a fault, while as
on the high side (Natland
in the mid-Jurassic
higher in the section. to the downthrown
from
Jurassic
volcanic
et al., 1974).
rocks, although
a
In some cases, the mid-Jurassic
side of the fault, and the adjacent
of deposits (Natland et al., 1974). Finally, in some areas, the rocks cover faults with no significant thickness variation on
either the high or low side of the fault. These relationships,show that extension, accommodated by normal faulting at high crustal levels and some volcanism, began considerably before the major mid-Jurassic volcanic event discussed here, but extension continued during mid-Jurassic volcanism and finally died out with the cessation of mid-Jurassic volcanism, or shortly thereafter. We have no direct
evidence
of the amount
of extension
that took place across
southern South America during the Jurassic, but because the extension was associated with significant crustal anatexis, as expressed by the volume of ignimbrites, we feel that it must have been considerable. DKXUSSION
The distribution of the mid-Jurassic volcanic rocks shown on Figs. 1 and 2 provides an indication of the area affected by the extension and volcanism that we have described. This is a minimum estimate, however. Similar volcanic rocks have been described from the Antarctic Peninsula (Saunders and Tarney, 1982), and although siliceous volcanic rocks of the appropriate age are not present on the Falkland
Islands
(Islas Malvinas),
bimodal,
mid-Jurassic
volcanic
rocks have been
reported from the Algoa Basin in South Africa (Marsh et al.,. 1979), and abundant devitrified glass shards and volcanic fragments occur in the Jurassic sedimentary rocks of the Karroo Basin (Elliot and Watts, 1974; Bristow and Saggerson, 1983). This suggests that the area affected present Pacific margin of South crust boundary along Argentina’s north to at least the reconstructed
by the volcanic
event extended
from nearly
the
America east to at least the oceanic-continental eastern edge, and from the Neuquen Basin in the position of the Antarctic Peninsula in the south.
Extensional deformation also began in the Cape Fold Belt of southern about the same time that grabens were forming in southern South America
Africa at (Table 3)
(Lock et al., 1975; Lock, 1978). Although the culminating volcanic episode that produced the Tobifera volcanics, the Bahia Laura and Lonco Trapial Groups, and related volcanic rocks was of limited duration, the associated extension and preceding volcanism occurred (perhaps sporadically) throughout most of the Late Triassic and Jurassic. There is good evidence that the western edge of southern South America was a
paleo-pole
Carboniferous
3
Mid-Jurassic
Late Triassic
to
Permian
mid-Triassic
Early
to Early Permian
Late
Time
Magnetic
TABLE
to
1976; Vilas, 1981)
and Vilas, Bahia
Laura,
Lonco
Trapial
Groups).
event
culminates volcanic
volcanism, mid-Jurassic
silicic to bimodal
widespread
(Tobifera,
in
localized
basalts
Hoachanas
by
Suurberg basalts (Bristow
Basm
1982) and the extensive m the Karroo
and Smith.
Basin indicated
Drakenberg
1983). favas in AC wells (Gerrard
and rhyolites. and Saggerson.
basahs
uolcanrsm
Bank, and Orange $yntectonic
Agulhas
(Valencio
Newark-type
gether
formation,
Extensronai deformatton --produces graben
basins (Lock et al., 1975) in the Cape Fold Belt,
America,
southwestern
S.
Back -arc extension and crustal anatexis to-
America,
Africa
(Beaufort
accommo-
K/Ar
Semr -Stable
Cr.)
Basin up megasequence
deposition - Karroo a shallowing
Foreiand dates
resets
orogeny) S. Africa
(Gondwanide offshore et al., 1978)
event ages (Gentle
Thermal
(?) in S. America
South
Chile.
but and
Argentina
narrower
north of 36’N in central
matic arc was 500 km wide in N. Patagonia,
Eq.) (Forsythe,
arc
basin Mag-
Fm. and
Fm.) and magmatic 1982).
(Choiyoi
(Rio Genoa-Panguipulli
de Dios Fm. ) forearc
accretion-
(Madre
and Vilas,
included:
ary prism
1976; Vilas, 1981)
complex
(Vaiencio
time
onset of Ecca
gether
deformation
or
suggests
Cape Fold Belt (Lock. 1978) and Sierras Auscrales
1978)
polarity in Dwyka
Back -arc compressional
(Lock,
regime
margin
et al..
contractional
Subduction, accretion and arc magmatism
Herve
Carbonifer-
convergent
to-
1976:
to Lower
America,
1981)
(Miller,
Silurian
South
Africa
deformed
ous accumulations
cludes
Semt -stable
1976; Vilas, 1981)
and Vilas.
IOforeland deposition
in depositional
(Valencio
in-
gether
substratum
reversal
edge of Gondwanaland,
Epicratonic
Africa
Subductson, accretion and arc mugmatism
Africa
western
to-
Africa
Southern
and southern
America,
South America
events
South America
South
Africa
Major tectonic-magmatic
events in southern
Rapid shqt
S. America/S.
pole positions
Paleo
and major tectonic/magmatic
Magnetic
positions
Late Early ceous
Greta-
Late Jurassic to Early Cretaceous
South America Rapid Shift Africa (Vale&o and Vilas, 1976; Vitas, 1981)
Semi-stable
-western margin of South America (Hailer and Lapido, 1982; Ramos et al., 1982) Thermally induced subsidence in Magaltanes, and San Jorge basins. Continental to marine sedimentation in broad depressions (Inoceramus shale-Upper Las Heras Group) Subduction and arc magmatism
Unknown Late Jurassic Back-arc extension -mostly confined to opening Rapid Shift (Early Creta- of Rotas Verdes marginal basin by 140 Ma ceous) South America (Daiziel, 1981) Africa together (Valencio Wuning of volcanism and normal faulting in and Was, 1976; ViIas, 1Y81) central eastern Patagonia Onset of thermally driven subsidence in the Magallanes and Malvinas basins
sedimentation -in the Agulhas and Orange basins (early drift sequence-Upper Sundays River, Gerrard and Smith, 1982; Du Toit, X979)--waning of magmatic activity.
Subsidence and pass&e-margin
Extensional deformation -Agulhas Bank (Du Toit, 1979) and Orange basin (Gerrard and Smith, 1982). Onshore faulting associated with silicic and basaltic volcanics (Bristow and Saggerson, 1983). Central Karroo volcanism dies out after 160 Ma. Sedimentary accumulation mostly confined to fault bounded depressions (rift valley sequence = Pre-Sundays River). Opening of the south Atlantic around 130 m.y.
246
subducting
margin
with an associated
(Nelson
et al., 1980). The widespread
indicate
that they represent
activity
associated
margin Jurassic
arc during extension
a tectonic/magmatic
with the marginal
event
The
cause
of the extension
separate
arc. The geochemical
volcanic rocks presented here support this contention silicic volcanic rocks had a crustal magma source. and
volcanism
much
of the Mesozoic
and mid-Jurassic
data on the mid-Jurassic
and indicate
remains
volcanism
from the igneous that most of the
speculative.
Any
model
proposed to explain these two phenomena must also explain several other aspects of the history of southern South America and southern Africa. We believe that the major
events
that affected
ceous are related. We postulate
both areas from the Late Paleozoic
Table 3 summarizes that a series of events
and Range extension
and bimodal
to the Early Creta-
these events. similar
volcanism
to those proposed
in the western
United
to explain
Basin
States (Lipman,
1980) provides the best model for the current data from southern South America. Bruhn et al. (1978) have also compared the mid-Jurassic volcanism of southern South America with the Tertiary volcanism of the Basin and Range province. Following Lock (1980) we propose that the dip of the lithospheric slab being subducted beneath southern South America changed from a steeply dipping configuration in the Late Paleozoic to a more shallowly dipping slab in the latest Paleozoic and Early Mesozoic. This caused the magmatic arc in southern South America to expand in width to perhaps 500 km in Patagonia by Middle Triassic time. To the north, in Chile, the Early Mesozoic magmatic arc retained a more conventional width indicating segmentation of the subducted slab. The shallowly dipping slab also allowed back-arc
compressive
range
America
of South
and
deformation the Cape
to take place in the Sierra de la Ventana Fold
Belt of southern
removed from the subducting margin (Lock, 1980). By the Late Jurassic, the subducted slab appears to have returned and the associated southern
arc magmatism
South America.
was limited
As arc magmatism
to a narrow migrated
Africa,
both
far
to a steep dip,
belt along the margin
of
back to the South American
margin, Patagonia, Tierra de1 Fuego, and the Cape Fold Belt area of southern Africa began to extend as the subducted slab returned to a steeply dipping state. The extension resulted in the intrusion of basaltic magma into the lower crust, triggering significant crustal melting and the tremendous outpouring of mid-Jurassic volcanic rocks in southern South America. This is envisioned as the beginning of fragmentation of western Gondwanaland. The extension that preceded and accompanied the mid-Jurassic volcanism culminated in the formation of a back-arc basin, the Rotas Verdes Basin, along the western edge of southern South America (Bruhn et al., 1978; Saunders et al.. 1979; Nelson et al., 1980; Dalziel, 1981). have formed in this basin by 140 event we have discussed here. Once Basin, normal faulting essentially
Dalziel (1981) has shown that oceanic crust must Ma, or near the end of the extensional/volcanic oceanic crust began forming in the Rotas Verdes stopped to the east in Patagonia and Tierra de1
247
2
-
t
CONDOR-l
0
ELFONDO-1
0
EVANS-
ff
MANZANO
z fki 0
-3
1 -1 -4
&I
11
fl
11
11
150
11
TIME. IN MILLIONS
Fig. 10. Subsidence Jurassic during
I
*
I 50
100
curves
and their shapes
8
I
5
OF YEARS
for four wells in the Magallanes
and Early Cretaceous,
I(
suggest
Basin. The curves are similar
that subsidence
was driven
for the Late
by thermal
decay
that time.
Fuego, and the extended areas began to subside, giving rise to the post-rifting phase of subsidence of the Magallanes and Malvinas basins. Results of standard backst~pping procedures on data from wells from the Magallanes Basin (Natland et al., 1974) support the supposition that the early history of these basins is related to a rifting event that ended in Late Jurassic time. Using backstripping techniques similar to those of Steckler and Watts (1978), we constructed total subsidence curves and thermo-Teutonic subsidence curves (subsidence that would have occurred if there was no loading due to sediments) assuming Airy isostasy for four wells from the Magallanes Basin (Fig. 10). Corrections were made for sediment decompaction, water depth changes, and long term eustatic sea level changes. All four curves start with deposition of the Sp~n~ll Sandstone immediately following the Tobifera volcanic episode (151 Ma). The shape of the thermo-tectonic subsidence curves for the Late Jurassic and Early Cretaceous for the Evans-l, Manzano-7, and El Fondo-1 wells all approach the shape expected from thermal decay following a rifting event (McKenzie, 1978; Steckler and Watts, 1978) that ended in the Late Jurassic. Similar styles of subsidence are seen in the San Jorge basin and on the Malvinas Plateau at about the same time. The magnitude of the subsidence reflects position in the basin. For example, the Condor-l well, which is located on a structurally high block, shows little tectonically controlled subsidence (Fig. 10). Finally, the abrupt increase in the rate of subsidence in the Late Cretaceous and Early Tertiary reflects flexural loading in response to contractional
248
deformation in the Andes the mid-Jurassic event. The separation Rotas
Verde basin.
South Atlantic
to the west (Winslow,
of Africa and South America The oldest
known
oceanic
followed
the South African,
anomaly
identified
area of Patagonia
is M4 (Rabinowitz
related
soon after opening
crust on the Argentine
occurs to the east of the Somoncura
the oldest magnetic
to
of the
side of the
(Fig. 1). Here,
and LaBrecque,
1979). On
side, Larsen and Ladd (1973) picked Ml1 as the oldest identified
magnetic anomaly, although recently released multichannel (Jaunich,
1981) and is not directly
1983). The magnetic
this has been called into question by a number of seismic lines from the western margin of South Africa anomalies
show that the creation
of oceanic
crust
began in the southern South Atlantic Ocean certainly before 122 Ma and perhaps as early as about 130 Ma (using the time scale of Van Hinte, 1976). This is about 25-30 Ma after the peak of the ignimbritic America
eruptions
and only 10 Ma after formation
the extension
and volcanism
in the mid-Jurassic
of the Rotas
in southern
South
Verdes basin. Thus, we view
that began in the Late Triassic
and culminated
in the
mid-Jurassic ignimbritic eruption and the opening of the Rotas Verdes basin as the initial stages of crustal extension that led directly to the opening of the south Atlantic. These events also have direct economic importance. Decay of the thermal signature associated with mid-Jurassic extension initiated subsidence in the commercially-producing petroliferous basins of southern Chile and Argentina. In the Magallanes, Malvinas and Neuquen basins, and to some degree the San Jorge Basin, the thermally driven subsidence controlled facies distributions and depositional thicknesses after the initial phase of fault-related sedimentation and volcanism. The heat released into the upper crust by extension and volcanism presumably important role in the maturation of hydrocarbons in these basins.
played
an
CONCLUSIONS
(1) Timing relationships show that extension, accompanied by limited volcanism, began in the Late Triassic-Early Jurassic in southern South America and continued into Late Jurassic time. The mid-Jurassic volcanic rocks described here represent the culmination of that event. (2) The geochemical data on the mid-Jurassic rhyolitic volcanic rocks indicate that they were produced by melting of a crustal source. Differences in geochemical signatures of rhyolites from the Somoncura and Deseado massifs may reflect differences in source areas. (3) Although there was an active margin arc along the South American edge of Gondwanaland during most of the Jurassic, the geochemistry and distribution of the mid-Jurassic volcanic rocks show that they are not directly related to igneous processes associated with that arc, but instead represent a separate tectonic/magmatic event. We propose that these rocks are related to events associated with the
249
transition from a shallowly dipping subducted slab to a steeply dipping configuration. (4) The extension and volcanism were precursors to the opening of the Rotas Verdes marginal basin to the west (present day coordinates) and to the initial separation of South America and Africa. As such, they heralded the breakup of western Gondw~aIand. (5) Decay of the thermal event associated with the extension and volcanism began the post-rifting subsidence of the Magallanes, Malvinas, San Jorge, and Neuquen basins, and presumably set the stage for later maturation of hydrocarbons in these basins. ACKNOWLEDGMENT
We wish to thank G. Chebli of Yacimientos Petroliferos Fiscales, Argentina and R.F.N. Page of Servicio Geologic0 National, Argentina, for assistance in assembling the suite of samples analyzed during this study, and Dr. M.G. Fitzgerald for assistance in preparing the subsidence curves. We thank anonymous reviewers for their efforts and useful comments. Exxon Production Research Company, Esso Exploration Inc., and Esso SAPA approved this work for publication. A portion of this research was done while D.A. Gust was a visiting scientist at the Lunar and Planetary Institute. This paper is Lunar and Planetary Institute Contribution No. 546. REFERENCES
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