cenozoic magmatism in kalimatan and its related geodynamic evolution
TRANSCRIPT
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PERGAMON Journal of Asian Earth Sciences 17 (1999) 2545
Ceno zoic magmatism in Kalimantan and
its related geodynamic evolution
R. Soeria-Atmadja *, D.Noeradi, B. Priadi
Teknik Geologi, Institut Teknologi Bandung, Jalan Ganesa 10, Bandung, 40132, Indonesia
Received 27 November 1997;accepted 29 April 1998
Abstract
The NESW Tertiary magmatic belt of central Kalimantan is related to two
separate periods of subduction; during the Eocen eOligocene and Late
Oligocen eMiocene. The younger magmatic belt is superimposed upon the
earlier belt. This magmatic belt is characterized chie y by Late
Oligocen eMiocene volcanic products, among which limited exposures of the
Eocene volcanics have also been mapped by previous investigators. This calc-
alkaline magmatic belt has become known as the
gold belt' of Central West Kalimantan on account of a number of discoveries of
Neogene epithermal gold mineralization. This mineralization is found in central to
proximal volcanic settings and occurred at relatively shallow depths. The earliest
known subduction-related magmatism took place in the Eocen eEarly
Oligocene with the emplacement of calc-alkaline silicic pyroclastics, followed
by a period of continental collision. Subsequent subduction-related
magmatism continued from Late Oligocen ePleistocene, during which time the
magma evolved from calc-alkaline to potassic calc-alkaline. Plio-Pleistocene
magmatism resulted in the formation of basalt ows. The present available KAr
ages of the Cenozoic volcanics range from 51
to 1 Ma. # 1999 Elsevier Science Ltd.All rights reserved.
1. Introduc tion
The search for gold in central
Kaliman tan during the early
eigh ties has produced valuab le
info rmation concerning the
tecto nic setting and the geological
en- viron ments of format ion of
the mine ral deposits. A num ber
of epithermal gold occurrences in
the region are dis tributed along a
SWNE trend ing belt within the
Terti ary mag matic arc (van
Leeuwen et al., 1990). This gold
belt repre sents an epithermal
environ ment, whe re mine ralizat ion
occurred most commo nly in cen-
tral to proxi mal volcanic settingsat shal low depth. The host rocks
are typi cally eusives or
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pyrocl astics of inte rmediate to
acidic calc-alka line rock series,
and show feat ures suggesting
derivation from near-n eutral pH
geothe rmal uids. The character
of the ore ui ds and the types of
mine ralizat ion, as well as assoc iated
alt eration indicate thatmineral ization occ urred in a
* Correspon ding author. Tel.: +62-22-250-0970; fax: +62-22-250-
2201; e-mail: rubini@ gc.itb.ac.id.
low sulp hide environ ment. Most
commo nly mine raliz- ation in the
region occ urs in hydrothe rmal
brecc ias, vein stru ctures and quartz
stock works. These volcan ic- hosted
gold deposits are, acc ording to
White and Hede nquist (1990 ),
typical ly epitherma l.
Rock chemistry as well as KAr
ages of the volcan ic host rocks
indic ate that the calc-alka line
mag matism was related to late
Oligoce neEa rly Mioce ne SSE -dip-
ping subduction from the osh ore
region to the north of Kaliman tan
(Ha milton, 1979; Ca rlile and
Mitc hell,1994). Carlile and Mitchell
(1994) identi ed the Te rtiary
mag matic arc by remnan ts of
Ea rly Tert iary andesitic volcanic
centr es with wh ich the
epithermal gold mineral izati on is
assoc iated. Accor ding to their
observations epith ermal gold
mine ralizat ion in
Indonesia is best developed above
contin ental crus t, such as in the
we stern Sunda-Ba nda and the
central Kal imantan arcs,
whe reas porphyry-t ype
mine ral deposits are
for med in island arc as well as in
conti- nental setting s; e.g. the
coppe rgold por phyry of Ba tu
Hi jau, Sumba wa (Me ldrum etal., 1994) and the
1367-9120 /99 - see front matter # 1999 ElsevierScience Ltd. All rights reserved. PII: S 0 7 4 3 - 9 5 4 7( 9 8 ) 0 0 0 6 2 -2
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2 R. Soeria-Atmadja et al. / Journal of Asian Earth Sciences 17 (1999) 2545
molybde num por phyry of the
Mala la dis trict, northe rn arm of
Sula wesi (van Leeuwen, 1994). Th is
pap er is an att empt to summarize
the avai lable geological data,
contributed by sever al work ers as
the result of the inten sive search
for gold in Cen tral Kaliman tan,
high- lighting some of the feat ures
of the related mag matism and its
tecto nic set ting.
2. Geology of the Tertiary magmatic belt
2.1. Regional geologic setting
Van Be mmelen (1949) noted
the charac teristic fra mework of
arcua te structures of Kaliman tan
island with their convex sides
towards the south and south-
west. These stru ctures are mos tly
EW trend ing in cen- tral
Kaliman tan and are bound ed in
the south by the Schwaner
Mountain magmat ic arc, wh ich
is paired with a Cretaceous
mel ange comple x. The region al
geo- logic set ting of the northe rn
part of Kalima ntan, es- pecia lly
Borneo (Ma laysi an and Bru nei
ter ritories) has been described by
Hutch ison (1996 a) based on pre-
vious work s. He distingui shed
three major tecto nic zones fromthe northwest to southea st, the
Miri, Sib u- Ra jang and Kuc hing
zones (Fig. 1).
Acco rding to Hutch ison (1996 a)
the Miri Zone rep- resen ts part of
the Lucon ia continental block
wh ich is limi ted to the northwest
by the Pala wan Trench, the trace
of a Miocene sub duction zone
(Ha milton, 1979), whe reas thesouthea stern limit has been
referred to as the Mersing Line.
The oldest rock expos ures in this
zone include roc ks of the Long
Bawan and Kal alan for mations
which consi st of stron gly folded
uvio-d el- taic sedi ments of Late
Cretaceou sEocene age. The
overl ying Eo-O ligocene
sedime nts of the
Mulu Fo rmation consi st of
limes tones which, accord ing to
Hutch ison (1996 a), we re
deposited on a relativ ely stab le
contin ental shelf. You nger
Miocen ePliocene sedi ments were
deposited in a delt aic to braided
str eam environ ment in syncl inal
basins formed during a pre- vious
period of fold ing.
The Sibu-Rajang Zone consi sts
of inten sely folded, weak ly
metamorp hosed ysch sedi ments of
the Rajang Group. The Rajang
Group is composed of the Late
Cretaceou sOlig ocene Balaga,
Lurah and Crocker for- mati ons. The stron gly deformed Upper
Cr etaceou s Eoc ene ysch
seq uence of the Embaluh Group
for ms the south wards exten sion of
the Ra jang Group into
Kaliman tan. These ysch
sedi ments have been inte r- preted
by Hutchis on (1996 a) as
turbi dites wh ich were scraped
into an accre tionary prismduring Late Oligoce ne time, as
the result of convergence of the
Lucon ia continental block with the
northe rn margin of Sund aland.
Neoge ne v olcanics, of basaltic to
daci tic comp osition, overlie the
Pale ogene sedime nts unco n-
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R. Soeria-Atmadja et al. / Journal of Asian Earth Sciences 17 (1999) 2545 2
for mably. The Lupar Sut ure
Line, along wh ich Cretaceous
ophiol ites are exp osed, marks the
bound- ary bet ween the Sib u-
Rajang and the Kuching zones.
Ophio lite mel anges also occur along
the Bukit Mersi ng Li ne and in the
Semitau Ridge. The oph iolites
rep- resent the basem ent of the
Rajang Gro up and indic ate the
trace of a Late
Cretaceou sOligocene subduction
zone. The eastwa rd continuation
of this suture line is not clea r,
possibly it may be con nected
with the no rth south trend ing
Long Ara nWititi thrust fault or
the Adio sutur e.
Acco rding to Hutch ison (1996a)
the Kuching Zone marks the
northe rn margin of Sund aland.
Along this zone Pale ozoic
crystal line schi sts are overl ain by
car- bon ates and siliciclas tic
sedi ments of Pale ogene to
Mesozoic age. The PaleogenePiyab ung Vo lcanics and Neog ene
Sintang Intru sives (Her yanto et al.,
199 3) are the mag matic rocks in
this zone. The southern limit of the
Kuching Zone is marked by an
EW trend ing faul t, which
acc ording to Tanean et al.
(1996) con- tinues as far as the
Ada ng Fault separa ting the Kutai
Ba sin in the north from the Bari to
Ba sin to the south. Th is zone can
possib ly be fol lowed fur ther
eastwa rds into the Up per Kutai
Basin, whe re Neogene and
Pale ogene volcan ics have also
been document ed (Ke lian, Muara
Wahau) and then swings
north wards into the Upper
Tar akan Basin.
2.2. Tertiary volcanic rock association
Carlile and Mitc hell (1994)
tent atively projec ted the Te rtiary
mag matic arc from northea st
Kal imantan southwards through
central and west Kal imant an to
Sarawak, followi ng the southern
bound ary of the Kuc hing High.
Va luable geological informa tion on
the volcanic rock-associa tion,
geolog ic setting and rela ted
mine ralizat ion have been
document ed from sever al dis- tricts
along the magm atic arc (among
others Busang, Kel ian, Muyup, Mt.
Muro, Mas uparia, Muara Wa hau
and Sintan g; Fig. 2). The volcan ic
rock series are pro- ducts of
Early Tertiary calc-alka line
mag matism. Th ree mag matic
episodes have been ide ntied by
pre- vious workers, Eoc ene acid ic
volcan ism was fol lowed by Late
Oligocen eMiocene
andesiti c rhyolit ic volcan- ism
(prec eding epithermal
mine ralizat ion) and then by Plio -Plei stocene basalt volcan ism; the
latter gave rise to basal tic lava
ows and dykes of region al exten t.
Felderh of et al. (1996) ident ieda maar diatrem e
do me complex and assoc iated
epith ermal gold mineral- iza tion in
the Busa ng area northea st of
Keli an. They described the local
geolog ic setting as a NWSE trend-
ing semi-circ ular gra ben stru cture
of Early Tert iary age, intru ded by
a Mid-Te rtiary maar diat reme
and dacitic do me comple x; the
dome hosts gold mine raliz- ation
along northwest trendi ng frac ture
zones in whi ch the mine ralizat ion
style is due to hydrofr acturing.
The
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Fig.1.Tectonicframework
ofKalimantanandsurroundingislands
(modiedfrom
Taneanet
al.,1996
).
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Fig. 2. Distribution of volcanic outcrops and KAr dated volcanic rocks in Kalimantan.
Data from Kirk, 1968; van de Weerd et al., 1987; Pieters et al., 1987; Tate, 1991; Bellon
and Rangin, 1991; Harahap, 1993; Heryanto et al., 1993; Thomps on et al., 1994; van
Leeuwen, 1994; Carlile and Mitchell, 1994; Tanean et al., 1996. 1, Non-del ineated outcrops;
2, delineated outcro ps; 3, Miocene and Plio-Pleisto cene; 4, Miocene;
5, Oligo- Miocene; 6, Eo-Oligo cene and Miocene; 7, Eocene; 8,KAr ages in Ma; 9, folded belt.
volcan ic membe rs of the maar
deposi ts are acid ic tus, wh ich
include rhyolit ic crystal tu,
andesitic lapilli ash tu and
rhyolit icdacitic pyrocl astic roc ks;
the assoc i- ated sedi ments of
ysch facies consist of met amor-
pho sed muds tones and
clay stones. Acco rding to
Felderh of et al. (1996) the dome
com plex is ma de up larg ely of early
phase volcan ics showing a
grada tional cha nge towards the
periphe ry from mediu m- to coarse-
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grain ed quartz- hornblende dacite
to porphyritic rhyo- daci te, and
are charac terized by a very ne-
grained grou ndmass; the late
phase volcan ics are represented
by ne-gr ained aphyric
andesi tedacite plugs, as well as
subparallel sheet ed dykes of
porphyritic andesi te and dacite.
The se v olcanic rocks are the
products of a phase ofMid-Te rtiary calc-
alkaline mag matism. Fel derhof et
al. (1996) also document post -
mine raliz- ation mag mati sm,
represented by basalt and quart z
rhy olite plugs and dy kes.
In the Kel ian mini ng distric t,
southwest of the Busang area, the
oldest exposed volcanic rocks
occur as a Late Eoce ne silic icpyr oclastic unit, 300 m thick,
includ ing pyrocl astic, as well as
epiclast ic-rocks of
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rhyol itic c omposition (epi clastic,
air-fall as we ll as wel ded
pyrocl astic ow deposits)
contai ning pumice, crys tal and
lithic fragment s.
Acco rding to van Leeuwen et
al. (1990) this unit is overl ain by a
thick pile of Eoce neOlig ocene
sedi ments with local tu ac- eous
intercala tions, cut by rhyol itic
dy kes and sma ll andesitic stocks
and dykes. These int rusions were
empl aced in the Early Mioce ne
alo ng NS and NE SW trendi ng
fractures and faul ted zones andwe re fol- lowed by four -stage
sequence of hydrothe rmal activi ty
and mineral izatio n. Intru sions of
inte rmedi ate po r- ph yry cutting
andesitic volcan ic cou ntry rock
at Muyup, close top Kel ian, have
also been report ed by van Leeuwen
et al. (1990).
In the Gu nung Mas area,
south west of Mt. Muro, goldmine ralizati on occurs as gold-
bearing ssure veins and
stockw orks in the contact
zone between a Cr etaceous
granit oid and a djacent
sedimentary roc ks (van Lee uwen,
1994). Gold mine ralizat ion at
Mirah, south west of Gunu ng
Mas, occurs along zones of
quartz stock works, hydrothe rmal
bre ccias and veins foll owing NNW
trend ing frac tures. The host
roc ks consist of stron gly altered
(argil lic) pyrocl astics, bound ed to
the west by an andesi te plug
(van Leeuwen, 1994), possibly of
Eoc ene age.
Van de Weerd et al. (1987)
obtain ed a KAr age range of
24.0 Ma14.4 Ma from nine
samples of ande- site and basalt
coll ected from an area between
Kelian and Mt. Muro, whe reas
van Leeuwen et al. (1990) record
an age of 22.9 2 0.5 Ma from a
rela tively fresh
andesite. These volcan ic roc ksreprese nt a phase of lateOligoce neEarly Miocene calc -
alka line mag matism. Post-
mine ralizati on mag matism
resu lted in the extru- sion of
widespread plateau basalts.
Volca nic rock outcrops forming
the remna nts of a volcan ic crat er
at Masuparia, south west of
Kel ian, consist of calc-alka line
intrusive bodies (Diorite, mon-
zonite, gra nodiorite) and many
dior ite plugs, lava
ows, proxi mal pyr oclastic ow
breccias and tus of
andesiti cdacitic composition
(Thom pson et al., 1994). Most of
these volcan ic ows and tus are
plag ioclas e- phyric, with minor
pyr oxene and hornblende.Towards the periphe ry of this
volcanic cente r, the volcanic sedi-
ments are inte rbedded with
sedi ments of the Barito Basin.
Accor ding to Thom pson et al.
(1994) this area repre sents a
stratovo lcan o. Tho mpson et al.
(1994) postu late a three-s tage
magmat ichydrothe rmal sys- tem,
in which the second- stage ui ds
we re resp onsible for the
mine ralizat ion. Miner alization is
assoc iated with either NW
trend ing stru ctural zones or a
N9 08100 E8 trend ing line ament. A 24.620.4 Ma KAr agewas obtain ed from these volcan ics.
The wholeasse m- blage is overl ain
by oliv inebasalt ows representing
a Plio -Pleistocene magmat ic event.
A simil ar volcanic rock
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assoc iation is exposed in the
Mt. Muro area, direc tly east ofMasupar ia, where
there is an interbe dded sequence of
subaerial calc-alka- line andesi te
and basal tic andesite ows,
breccias and tu s (Si mmons and
Browne, 1990). These rocks are
porphyritic, consisting
pre dominan tly of plag ioclasephenocrys ts with minor pyroxene
and amphibo le. Sim mons and
Br owne (1990) noted that
conjuga te pairs of NW- and NE-
tre nding shears and faults gen-
eral ly lack mine ralizat ion; ins tead
mine ralizat ion took place along
NNW -trend ing tens ional fracture s.
In co nnection with a region al
study project of the Kutai Ba sin
und ertaken by VICO (Virginia
Indonesia Company), Tan ean et al.
(1996) samp led Tertiary vol-
canics of the Muara Wahau area.
The roc ks of the Muara Wahau
Forma tion are ma de up chie y of
clay with inter calations of
sands tone and volcan ic ma-
ter ials. The lat ter include
hornblend eandesite ows and
dacitic pyrocl astic tus with
andesite dykes. The ir stron gly
por phyritic text ures and rock
chemistry suggest an island-a rc
calc-alka line rock seri es. Tanean et
al. (1996) obtain ed a KAr age
range of 21.2 20.39Ma 16.9 2 0.3 Ma from veanaly sed samp les. Resu lt
of stud ies on the volcan icfrag ments c ontained in the Ea rly
Miocene (N4N7) and Mid dle
Mioce ne (N8 A N10) sandst ones
sugges ts two di erent
source sthe Sintang and Muara
Wa hau volcan ics.
The earliest Tertiary mag mati sm,
represe nted by the Piya bung
volcan ics, is recorded from the
Sintang area (Sem itau Rid ge),for ming the westward
prolonga tion of the mag matic
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arc. Acco rding to Hery anto et
al. (1993) these volcan ics are the
products of subaer ial air -fall and
ash- ow volcanism, composed
chie y of crys tal-lithic tus,
pumice-bearing crystal -lithic tus
and agglo merates, partly welded.These tus have been dated at
49.9 2 1.0 Ma, and are perhaps
correlatab le
with the silicic pyr oclastic unitof Kel ian dis trictrep orted by van Leeuwen (1994).
The distribu tion of Late Eoce ne
volcan ics is sporad ic. Besides
Kel ian, Mirah and the Semitau
Rid ge (Sin tang), Late Eoc ene
volcanics (ac id to inte rmediatetu , agglomerate, igni mbrite and
dacite) are also known from
Ma hakam area of the West Kutai
Basin (Ny aan Volca nics) which
have given K/Ar ages of 48.6 Ma
(Tate, 1991) and
50 22.5 Ma (Pie ters et al., 1987).Eoc ene volcan ics
near Singka wang (dacites of the
Serant ak Volcanic s) gave a K/Arage of 51.3 Ma (Hutchison,
1996b) and those of the Mandai
Ba sin from the Muller Mountains
were dated at 40.9 Ma (Pieters et
al., 1987).
Pro ducts of subseque nt
mag matism in central west
Kal imantan occur as iso lated
outcrops of hig h-level stock s, sills,
dykes and pl ugs, referred to as
the Sintang Intru sives of the
Ketun ggau Basin and the east ern
part of the Mela wi Basin
(Wi lliams and Harah ap, 1987;
Harah ap, 1993; Hery anto et al.,
1993). Petro graphic types vary
from granitoid rocks, dacite,
dacite porphyry, andesite, with
minor rhyol ite, rhy oda- cite,
dolerite, basalt and gabbro. Based
on their geo-
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logi cal setting and the relative
abundances of volcanic rock types,
Harah ap (1993) dis tinguis hed
three dier- ent province s. From
the chem ical analy ses (Hara hap,
1993), the southe rn p rovince
(Ear ly Cretaceous base- ment)
shows pred ominantly basalt and
rhyol ite, the centr al province
(Me lawi Basin) is charac terized
mos tly by andesi tes and daci tes
(without basalts ), whe reas the
northe rn province (Ke tunggau
Basin) has abund ant basal tic
andesites but no rhyolites. Twe lveK/Ar dates on separated mine rals
gave an age range of 30.4 Ma
16.4 Ma, corre spondi ng toOligoce neMiddle Miocenemag matism (Wi lliams and
Harah ap, 1987); the age range
ass igned to the Muara Wahau
volcan ics of Upper Kutai district
also fal ls within the same age
range (Tanean et al., 1996). Eight
rock samples were coll ected from
the Tertiary Sintang Intru sives and
ana- lysed by Pro uteau et al.
(1996). They include six grano-
dior ites of adakitic type, yiel ding
two K/ Ar ages 18.3
Ma and 19.2 Ma, and t wo calc-
alka line dacites of younger age
(16.5 Ma and 16.7 Ma).
Accor ding to Prouteau et al.
(1996) the adakites are related to
the incip ient subduction of the
Proto-Sou th Ch ina Sea,
whe reas the lat er calc-alka line
dacit es represe nt a more advanced
stage of the subduct ion proces s.
The inte rior of Bor neo, along the
border of Sara wak andKal imanta n, is occu pied by
platea ux of Cenozo ic lavas and
pyrocl astic cones. Acco rding to
Hutch ison (1996 a), this volcan ic
arc should be paired with the
Nor thwe st Borneo trench,
repre senting a NW- facing
subduction system. The bulk of
this volcan ic ser ies appears to be
of Miocene age. These platea ux
rise to altitu des of up to 2600 m
and consi st main ly of calc-al-
kaline to potassic calc-alka line
volcani cs, includi ng rhy odacites,
andesi tes and basal ts. Dac itic,
igni mbrite- tu s, glassy lavas and
brecc ias are impo rtant products of
this phase of volcan ism. Ki rk
(1968) reports K/Ar ages vary ing
from 25 Ma to 4 Ma. This
volcan ic arc can be trac ed furth er
NE to the Dent Peninsula of
Sabah, where the volcan ics
occur within Late
Miocene-E arly Plioce nerocks
of the Tungku
Fo rmation (Ha ile et al., 1965).
A sum mary of Tertiarymagm atism in Kal imant an is given
in Table 1.
Table 1
Summary of Cenozoic magmatism in Kalimantan
Period Magmatism
and related
tectonic
environm ent
Distribu tion of volcanic products
Plio-Pleis tocene Within-pla temagmatism
(tholeiitic)
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Late Miocen ePleistoc ene Subduction-r elated
(calc-alkali ne somehigh Mg)
Middle Miocen ePliocene Subduction-r elated
(high Kcalc-alkali ne)
Late Oligocen eMiddle MioceneSubduction-r elated
magmatism
(calc-alkali ne)
Eocen eEarly Oligocene Subduction-r elatedmagmatism
(calc-alkali ne)
Busang: basalt plugs and dykes;
Kelian and Mt. Muro:
plateau basalts;
Masup aria: olivine-b asalt
ows; Sintang: basalts;
Usun Apau:
basalt ows;
Linau-B alui:
basalts.
Dent and Semporna
Peninsula s: ows, tus
and basalts;
Upper Tarakan
basin: andesites,
basalts and tus;
Sulu Ridge: a sequence of
andesites, basaltic ows
and pyroclastic rocks.
Usun Apau: dacite andignimbrite tus;
Nieuwe nhuis Mt:
andesites and basalts;
Kinabal u: granito ids
intrusions;
Hose Mt.: dacite
tus and lavas;
Linau-B alui Plateau;
dacites, andesites and basalts;
Cagayan ridge: basalts and
porphyri tic andesites. Busang:
acidic tus (andesites, dacite s,rhyolites ); Masup aria: granitoid
intrusions,
andesite- dacitic pyroclastic and ows;
Mt. Muro: andesite and basaltic andesite
ows breccia and tus; Kelian and
Muyu p: andesite stocks, dykes;
Muara Wahau: andesi te ows and
pyroclastic tus (dacite), dacitic
dykes;
Sintang: basalts, andesites,
dacites, rhyolites.
Singkawa ng: dacites;
Manda i: dacites;
Piyabung: pyroclastic
tus and breccia; Kelian:
silicic pyroclastic
(rhyolit e);
Nyaan: agglomera tes, ignimbrites anddacites.
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Fig. 3. Diagram showing major elements versus SiO 2 from the volcanic rocks
of Kalim antan.
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Fig. 4. Rock anity after Peccerillo and
Taylor (1976). Symbols asin Fig. 3.
3. Chemical characteristics of the volcanic rock
For the purpose of this paper
availa ble analytical data on the
rock chemistry of the Tert iary
volcan ics (Table 2 (a)(d)) from
various districts in Kaliman tan has
been used, among other s, the
Oli go-Mio cene vol- canics of
Masupar ia (Thompson et al.,1994); Mou nt Muro (Simmo ns and
Browne, 1990); the Sintang area,
Cen tral Kal imant an (He ryanto et
al., 1993) and the Miocene to Plio -
Pleistoce ne v olcanics of Sabah
(Bellon and Rang in, 1991). Major,
trace a nd rare earth el- ement
data are available on ly for the
Oligoce ne Miocene volcan ics,
whe reas for the Miocene toPliocene -Plei stocene volcan ics only
major eleme nt ana- lyses are
avai lable. Eoc eneEarly Oligoce ne
and Plio- Plei stocene mag matism
are not supp orted by rock
chem istry (Ta ble 1). Analysis with
LOI values (loss on ignition) higher
than 4 have been excluded, to
av oid the eects of secondary
alterat ion. In general, chem ical
patt erns disp lay posi tive
corre lations bet ween Al 2O3, K2O,
Na2O, MnO and P2O5 with
incre asing silica con- tent, wh ile
TiO 2, Fe2O3, MgO and CaO
conten ts decrea se (Fig. 3). In the
K2OSi O2 diagr am (Peccer illo andTaylor, 1976) rock anities range
from tholeii tic and calc -alkaline to
high- K. Tho leiites are poorly rep-
resen ted; calc-alka line roc ks
being most common (Fig. 4).
Gener ally the chem ical patterns
of the Tert iary vol- canics in the
region are characteriz ed by high
alumina contents, varyi ng between
12. 619.4 %, low conten ts of
MgO, alka lies (Na2O + K2O less
than 8%) and Ti O2
(0. 05 1.28 %), enriched patt erns
of Chrond rite-norm al- ized spider
diagr ams, with negat ive
anomalies in HF SE, some times
acc ompani ed by enrich ment of
Th and U. The above chemical
feat ures are charac teristic ofsub duction-re lated mag matism on
an act ive conti- nental margin,
except that variations in the Zr
and Y
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contents are more charac teristic ofwithin -plate basalts
(Pearce and Norr y, 1979) (Tables2a1, 2a2, 2b, 2c1
2c3,2d).
3.1. OligoceneMiocene
Rel atively fresh volcanics fromMount Muro (50 .0
62.5% Si O2) and Masuparia
(55 .361.3% Si O2) h ave high
pot assium conten ts, a nd have
potas sic calc-alka- line to
shosho nitic a ni ties, wh ich may
indic ate vary- ing degrees ofcrus tal conta mination. The se
potas sic roc ks show enriched
spider diagr ams, 815 times
MORB and 10 times MO RB, in
wh ich compa tible el- ement
patt erns are rather steep. Tho se
from Mount Muro are
charac terized by negative
anomalies in Sr, Nb, Ti, and V,
while those from Masupar ia
show negative anoma lies in Nb,
with relativ ely enriched Sr, Pb,
and U conten ts.
The cogenetic nature of the
volcan ic roc ks in the region is
evident from overla pping patterns
in the spi- der diagr am, as
illustrated by basal ts, basaltic -
ande- sites, andesi tes and dacites
(Fig. 5) from the Sintang area.
They show similar patt erns in their
extended spi- der diagr ams. The ir
modera tely steep patt erns show
di erent (La/Yb)N ratios of
618, 720 and 922, in roc ks
from the centr al, northe rn and
southe rn parts of Sintan g,
respec tively. They sh ow enriched
patterns, with negat ive anoma lies
in Ti, rela ted to FeTi oxide
frac tionatio n, and Nb rela ted to
sub duction proces ses (Wi lson,
1989). High conten ts of Th and U
may indi- cate a contribution from
contin ental mat erials.
Ho wever, sever al basaltic roc kscollected from the
Sintang area have higher MgO(higher than 6%) and Ti O2
(1.5 62.26 %) contents. A high
MgO content nor- mal ly corre lates
with a pri mary mag ma
comp osition, wh ile a high TiO 2
indic ates possible crustal co ntami-
nation; both charac teristi cs are
compar able with those of
continental basalts (Wi lson, 1989).
These basalts have not been dated;
perhaps they repre sent products of
a younger mag mati sm episode,
compared to the ma- jor ity of the
volcanic rocks in the region.
Fig. 5 demons trates that the
rhyolite data from the Sintang
area show a distinct pattern in
that the (La/ Yb)N rati os range
between 150 600, to give steep
pat- terns cutti ng across the
curves for other rock types types.
Gener ally, they show low
contents of HREE with
fractiona tion eects on the Ti
content. This volca- nic suite
shows the c haracteri stics of
subd uction-re- lat ed mag mati sm.
Several rock sampl es show ada kitic
characters (Defant andDru mmond, 1996) with Y < 10
pp m, norma lized Yb < 5 and
Sr>500 pp m. Their low HREE
contents show the eects of
met asomatism on the adakitic
mag ma prior to melting, as
sugges ted by Prouteau et al.
(1996 ). Adak itic mag matism took
place at 19.2 818.31 Ma,
fol lowed by subd uction-re latedmag matism between 16.7 216.49
Ma (K/Ar age).
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Table 2a1
Chemical analyses of Tertiary volcanics from Kalim antan(a) Masuparia (Thompson et al.,1994), Oligo-Mi ocene
924-25A 924-22A 924-23A 924-26A 924-27A 924-27BOND 1.142 OND1.141 OND1.165 OND1.264
Si O2 55.53 57.97 61.26 53.37 52.50 52.82 53.96 52.29 54.02 50.59TiO 2 0.99 0.55 0.57 0.92 0.93 0.93 0.75 0.83 0.7 0.89Al 2O3 17.58 16.98 16.61 18.57 18.41 18.61 14.70 15.86 15.54 16.27Fe 2O3 9.03 7.00 5.53 10.16 10.40 10.37 6.46 4.88 7.6 8.96
MnO 0.18 0.18 0.13 0.02 0.02 0.02 0.33 0.26 0.2 0.23MgO 4.05 3.92 2.39 3.98 4.02 4.07 4.46 3.04 3.8 5.06CaO 8.24 7.42 5.44 8.85 8.86 9.05 4.62 4.77 3.2 2.72Na 2O 2.60 3.06 3.62 3.13 3.11 3.07 2.00 0.10 2.9 0.70K2O 0.69 1.71 2.39 0.60 0.59 0.57 3.34 5.43 3.1 5.82P2O5 0.13 0.14 0.14 0.14 0.13 0.13 0.13 0.15 0.1 0.13SO 3 0.02 nd 0.01 0.01 0.01 0.01 0.25 2.95 2.4 0.47LOI 1.57 1.20 1.43 0.49 0.48 0.43 8.93 8.35 5.8 7.73
Total 100.61
100.13
99.52 100.24
99.46 100.08
99.93 98.91 99.82 99.57
Rb 12 5 7 9 1 9 108 17 106 183Ba 281 442 477 147 142 146 501 1023 405 623Sr 361 643 479 489 488 484 173 8 238 8La 12 2 2 9 6 7 1 1 1 1Ce 23 3 4 2 1 1 2 4 1 2
PrNd 14 1 2 8 1 1 1 2 1 1Sm
EuGd
DyEr
YbY 31 1 2 2 2 2 3 3 2 2Zr 108 8 156 6 6 6 122 12 128 9Nb 2.4 3.5 5.7 1.8 2.5 1.6 2. 3.1 2. 2Sc 28 1 1 2 2 2 2 2 2 2V 263 175 125 250 246 249 179 22 374 283Cr 128 2 1 7 7 5 1 1 2 2Ni 48 1 6 9 1 9 4 4 8 1
Th 4 8.1 2.4 2.8 0.6 4. 2 4. 2.Pb 6 1 9 5 7 5 1 1 1 4Zn 89 6 4 6 6 6 9 5 8 8Cu 36 7 3 4 4 4 146 3 4 7U 1.4 1 2.9 1.5 1. 2.Ga 17 1
614
20
19
20
15
16
15
15
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Table 2a2
924-25A 924-22A 924-23A 924-26A 924-27A 924-27BOND 1.142 OND1.141 OND1.165 OND1.264
Si O2 55.53 57.97 61.26 53.37 52.50 52.82 53.96 52.29 54.02 50.59TiO 2 0.99 0.55 0.57 0.92 0.93 0.93 0.75 0.83 0.7 0.89Al 2O3 17.58 16.98 16.61 18.57 18.41 18.61 14.70 15.86 15.54 16.27Fe 2O3 9.03 7.00 5.53 10.16 10.40 10.37 6.46 4.88 7.6 8.96MnO 0.18 0.18 0.13 0.02 0.02 0.02 0.33 0.26 0.2 0.23MgO 4.05 3.92 2.39 3.98 4.02 4.07 4.46 3.04 3.8 5.06CaO 8.24 7.42 5.44 8.85 8.86 9.05 4.62 4.77 3.2 2.72Na 2O 2.60 3.06 3.62 3.13 3.11 3.07 2.00 0.10 2.9 0.70K2O 0.69 1.71 2.39 0.60 0.59 0.57 3.34 5.43 3.1 5.82P2O5 0.13 0.14 0.14 0.14 0.13 0.13 0.13 0.15 0.1 0.13SO 3 0.02 nd 0.01 0.01 0.01 0.01 0.25 2.95 2.4 0.47LOI 1.57 1.20 1.43 0.49 0.48 0.43 8.93 8.35 5.8 7.73
Total 100.61
100.13
99.52 100.24
99.46 100.08
99.93 98.91 99.82 99.57
Rb 12 5 7 9 1 9 108 17 106 183Ba 281 442 477 147 142 146 501 1023 405 623Sr 361 643 479 489 488 484 173 8 238 8La 12 2 2 9 6 7 1 1 1 1Ce 23 3 4 2 1 1 2 4 1 2PrNd 14 1 2 8 1 1 1 2 1 1Sm
EuGd
DyEr
YbY 31 1 2 2 2 2 3 3 2 2Zr 108 8 156 6 6 6 122 12 128 9Nb 2.4 3.5 5.7 1.8 2.5 1.6 2. 3.1 2. 2Sc 28 1 1 2 2 2 2 2 2 2V 263 175 125 250 246 249 179 22 374 283Cr 128 2 1 7 7 5 1 1 2 2Ni 48 1 6 9 1 9 4 4 8 1Th 4 8.1 2.4 2.8 0.6 4. 2 4. 2.Pb 6 1 9 5 7 5 1 1 1 4Zn 89 6 4 6 6 6 9 5 8 8Cu 36 7 3 4 4 4 146 3 4 7
U 1.4 1 2.9 1.5 1. 2.Ga 17 16
14
20
19
20
15
16
15
15
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Table 2b
Mount Muro (Simmons and Browne, 1990), Oligo-Mioc ene
45- 64-114 71- 80- 74-168 17- 17-107 74145 47-
Si O2 50.54 55.86 56.45 55.84 56.96 54.21 57.66 61.56 65.0TiO 2 0.93 0.90 0.87 0.84 0.72 1.03 0.95 0.67 0.6Al 2O3 18.62 17.08 17.16 16.57 16.48 16.43 17.73 17.04 16.9Fe 2O3 8.99 7.95 7.49 7.12 8.70 8.55 8.74 3.94 3.7MnO 0.98 0.47 0.28 0.30 0.22 0.51 0.05 0.19 0.1MgO 4.91 3.37 3.12 2.93 2.72 5.24 1.39 3.30 1.0CaO 8.11 5.66 5.96 4.09 3.05 0.53 0.32 0.26 0.0Na 2O 2.94 3.73 3.39 2.84 3.64 2.63 0.47 1.66 0.0K2O 1.29 2.05 2.57 3.73 2.76 3.81 4.46 6.52 5.1
P2O5 0.22 0.22 0.23 0.30 0.18 0.29 0.20 0.18 0.0LOI 2.17 1.75 1.83 3.65 2.78 5.28 7.72 3.61 5.9H2O 0.19 0.19 0.16 0.41 0.16 0.09 0.24 0.27 0.6
Total 99.89 99.23 99.51 98.62 98.37 98.60 99.93 99.20 99.4Rb 3 4 5 8 7 106 136 154 13Ba 336 277 381 966 502 415 236 870 59Sr 671 525 518 761 392 113 5 177 6La 2 1 1 2 1 1 1 1 2CePrNd
Sm
EuGd
Dy
ErYbY 2 2 2 2 2 2 2 2 1Zr 131 156 162 174 174 138 147 168 12Nb
ScV 270 189 198 126 158 208 170 139 17Cr 2 6 9 7 0 6 7 1 1Ni 1 7 8 9 8 0 0 2 1Th 9 0 1 1 6 0 0 0 6Pb 1 1 2 1 2 2 3 2 2Zn 9 102 9 124 162 115 3 168 6Cu 612 3 4 4 239 5 1 6 3UGa
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Table 2c1
Sintang, Central West Kalimantan (Harahap, 1993; Heryanto et al., 1993), Oligo-Mioc ene
69292 69293 69295 69294 69299 69303 69301 69355 69350 69375 69372 6936869365 69366 69379 69307 69343 69341 69347
Southern area Central area
Si O2 46. 48. 48. 49. 51. 51. 55. 61. 63. 69. 71. 72. 75. 75. 75. 60. 60. 61. 62.
TiO 2 2. 0. 0.9 1. 1. 1. 1. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.3Al 2O3 15. 16. 17. 19. 18. 17. 17. 16. 15. 16. 15. 16. 12. 13. 12. 17. 16. 17. 16.Fe 2O3 15. 9. 9.7 10. 9. 7. 7. 5. 3. 2. 1. 1. 1. 0. 1. 5. 4. 7. 3.9MnO 0. 0. 0.1 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.8MgO 5. 8. 7.5 4. 4. 3. 2. 0. 1. 0. 0. 0. 0. 0. 0. 3. 2. 1. 2.8CaO 8. 9. 9.7 10. 7. 6. 6. 4. 4. 3. 0. 1. 0. 0. 0. 6. 3. 1. 5.2Na 2O 3. 2. 2.3 3. 3. 4. 4. 3. 3. 3. 4. 4. 3. 3. 3. 3. 4. 5. 4.1K2O 0. 0. 0.5 0. 1. 1. 1. 2. 1. 1. 2. 2. 4. 4. 3. 0. 1. 0. 0.8P2O5 0. 0. 0.2 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0. 0.1LOI 2. 0. 0. 1. 2. 1. 1. 4. 5. 1. 2. 2. 1. 1. 1. 2. 4. 2. 3.2
Total 100. 97. 96.96 99. 95. 99. 99. 99. 99. 99.67 99. 99. 99.83 99.89 100.61Rb 13 8 12 24 58 20 12 40 39 41 82 60 137 120 112 27 59 20 42
Ba 473 95 220 366 467 360 155 430 453 574 758 674 60 766 801 247 460 423 294Sr 508 329 603 818 798 1172 343 624 694 639 413 416 45 72 113 492 768 260 536La 28 9 10 9 21 29 15 25 28 16 22 18 117 43 28 10 30 27 11
Ce 69 23 22 22 53 67 33 53 61 30 46 41 140 78 49 22 68 66 18Pr 8. 3. 7. 4. 2. 2.1Nd 40 14 15 16 28 32 18 23 25 13 16 19 99 29 14 11 28 33 9Sm 9. 3. 5. 3. 2. 1.7Eu 3. 1. 1. 1. 0. 0.6Gd 9. 3. 4. 4. 2. 1.7Dy 8. 4. 3. 4. 2. 1.5Er 5. 2. 1. 2. 1. 0.9
Yb 4. 2. 1. 2. 1 0.7Y 46 25 19 20 21 21 27 18 17 9 13 6 89 28 16 13 15 38 10Zr 269 88 78 78 208 199 100 145 167 93 143 48 549 81 77 89 167 187 0Nb 8 2 3 3 12 12 6 13 10 4 6 8 34 12 11 3 16 8 3Sc 29 36 33 25 18 12 25 10 11 9 2 2 6 1 5 18 13V 316 187 272 243 174 147 186 84 71 49 10 3 3 8 15 119 99 64 80Cr 33 281 26 9 36 3 151 2 22 10 2 2 2 2 2 71 41 13 92
Ni 58 194 35 23 20 7 133 4 15 6 1 1 2 1 1 24 20 9 35
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Y 1 11 19 6 9 6 8 1 7 2 4 19 42 18 4Zr 16 87 223 10 114 82 114 28 51 1 28 12 235 17 265Nb 1 3 9 3 4 2 5 4 6 1 1 5 9 14 1Sc 1 9 7 6 9 9 10 3 2 3 3 21 21 15 1V 9 66 21 50 57 52 62 3 4 327 23 15 185 98 5Cr 6 22 2 29 50 44 35 3 2 258 8 15 40 57 5Ni 4
319 1 28 31 29 26 1 1 177 6 8 34 33 3
Table 2c2
69345 69344 69481 69340 69342 69338 69325 69336 69327 69337 69363 6936169362 69297 69308 69306 69310 69334 69328
Central area Northern area
Si O2 62. 62. 64. 64. 64. 64. 65. 65. 65. 65. 72. 72. 73. 49. 54. 56. 56. 63. 63.TiO 2 0.4 0. 0.3 0. 0. 0.4 0. 0. 0. 0. 0.0 0.0 0. 1.9 1.5 0.8 1. 0. 0.8Al 2O3 17. 15. 16. 16. 17. 16. 16. 15. 15. 16. 15. 15. 15. 15. 15. 18. 16. 15. 15.Fe 2O3 4.0 4. 3.4 3. 4. 2.5 2. 3. 2. 3. 0.9 0.9 0. 10. 10. 6.8 7. 4. 5.6MnO 0.1 0. 0.0 0. 0. 0.0 0. 0. 0. 0. 0.0 0.0 0. 0.1 0.2 0.1 0. 0. 0.1MgO 1.7 2. 2.9 2. 0. 1.9 1. 2. 1. 1. 0.3 0.2 0. 7.6 4.1 4.1 3. 2. 1.1CaO 6.2 5. 4.5 4. 3. 4.1 4. 4. 4. 4. 2.5 2.7 1. 9.7 6.6 7.2 6. 4. 3.4
Na 2O 3.6 3. 4.4 5. 4. 4.6 4. 3. 3. 5. 4.2 4.2 4. 2.7 3.2 3.8 3. 3. 4.9K2O 1.3 3. 1.0 1. 1. 1.7 1. 1. 0. 1. 2.3 2.2 0. 0.1 1.3 1.1 1. 2. 1.8P2O5 0.1 0. 0.1 0. 0. 0.1 0. 0. 0. 0. 0.0 0.0 0. 0.4 0.4 0.2 0. 0. 0.2LOI 1.5 1. 2.0 1. 1. 1.5 2. 2. 4. 0. 0.8 1.0 1. 0.0 2.5 0.2 1. 0. 2.1
Total 99.42 100.76 99.60 99.91 99.96 98.60 99.88
Rb 63 2 29 3 55 28 48 90 32 1 4 39 41 108 73Ba 518 274 344 309 399 358 21 589 520 117 332 293 257 1078 387Sr 706 1060 714 1099 526 838 992 504 538 503 323 556 333 475 298La 28 1 28 1 5 12 18 2 15 8 26 16 19 22 25Ce 59 2 58 2 27 24 36 4 34 21 65 34 43 46 58Pr 6. 3 6. 0.3 3.0 4.1Nd 24 1 25 9. 11. 9 15 1.8 14 16 33 17 25 19 31Sm 4. 2 4. 0.4 3.7 3.Eu 1. 1 1. 0.2 1.5 1.Gd 3. 2 3. 0.4 4.1 3.
Dy 2. 2 2. 0.1 3.8 3.Er 1. 1 1. 0.1 2.0 1.Yb 1. 1 1. 0.1 1.3 1.
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Table 2c3
PR068B BH200A AM076A PR077B DT053B PW108A DS071B PP001A
SS108A DS079A CP206B PW110A CP274A Northern area
Si O2 (%) 64.27 61.91 65.68 65.69 65.75 63.53 65.87 72.80 73.87 54.00 56.4656.76 63.47
TiO 2 0.41 0.75 0.35 0.38 0.32 0.88 0.34 0.03 0.07 1.56 0.85 1.28
0.66
Al 2O3 16.88 17.70 16.47 15.75 15.48 15.80 16.68 15.77 15.52 15.32 18.78 16.75
15.93Fe 2O3 3.77 7.48 2.74 3.45 2.67 5.62 3.13 0.93 0.93 10.84 6.86 7.95
4.96
MnO 0.05 0.16 0.04 0.07 0.05 0.13 0.05 0.04 0.05 0.28 0.11 0.120.09
MgO 2.01 1.13 1.71 2.21 1.57 1.18 1.73 0.25 0.35 4.13 4.13 3.322.57
CaO 4.31 1.65 4.30 4.33 4.47 3.44 4.50 2.72 1.98 6.69 7.27 6.894.68
Na 2O 5.26 5.53 4.47 3.90 3.77 4.97 5.18 4.22 4.86 3.23 3.83 3.36
3.78
K2O 1.08 0.86 1.47 1.40 0.99 1.85 1.61 2.21 0.59 1.31 1.19 1.39
2.48
P2O5 0.19 0.50 0.15 0.13 0.11 0.26 0.19 0.04 0.10 0.47 0.21 0.29
0.29LOI 1.68 2.94 2.50 2.58 4.65 2.16 0.49 1.07 1.49 2.51 0.27 1.30
0.98
Total 99.91 100.61 99.88 99.89 99.83 99.82 99.77 100.08 99.81 100.3499.96 99.41 99.89
Rb (ppm) 22 20 38 55 28 73 48 90 32 4 39 41108
Ba 274 423 309 399 358 387 21 589 520 332 293 2571078
Sr 1060 260 1099 526 838 298 992 540 538 323 556 333475
La 12 27 13 5 12 25 18 2 15 26 16 1922
Ce 26 66 29 27 24 58 36 4 34 65 34 43
46Pr 2.89 0.38 4.19
Nd 12 33 9.4 11.3 9 31 15 1.88 14 33 17 2519
Sm 2.06 0.46 3.7
Eu 0.73 0.22
1.19 Gd 1.89 0.48
3.48 Dy 1.61
0.19 3.36 Er 0.94
0.17 1.81 Yb 0.73
0.17 1.52
Y 11 38 6 9 6 46 8 1 7 47 19 42
18Zr 87 187 107 114 82 265 114 28 51 285 120 235
170
Nb 3 8 3 4 2 11 5 4 6 10 5 9
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14
Sc 9 2 6 9 9 18 10 3 2 30 21 2115
V 66 64 50 57 52 53 62 3 4 235 152 18598
Cr 22 13 29 50 44 5 35 3 2 88 15 4057
Ni 19 9 28 31 29 3 26 1 1 6 8 34
33
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Table 2d
Sabah, Dent and Semporna (Bellon and Rangin, 1991), Miocen ePleistocene
13 S.8792 12 S.129 11 S.8411 10S8734 9S264.1 5 S 266 6 S 266 4S87.91 3S87.901S138.1
Sabah/Kinabalu Dent Semporna
Si O2 (%) 58.40 52.00 60.20 48.50 53.10 62.20 62.20 62.35 64.30 59.5TiO 2 1.06 2.27 0.64 0.69 0.98 0.57 0.64 0.50 0.54 0.7Al 2O3 16.19 14.12 16.65 18.92 17.58 15.85 16.69 15.98 15.53 16.0Fe 2O3 7.56 13.10 5.92 8.06 8.26 5.31 5.44 5.88 5.26 6.6MnO 0.15 0.15 0.14 0.17 0.14 0.10 0.08 0.11 0.10 0.1MgO 3.39 6.07 2.39 5.32 3.75 2.64 1.92 2.46 2.23 2.9CaO 4.47 6.60 5.51 10.03 8.92 5.13 6.51 6.00 4.84 6.0Na 2O 3.48 3.06 2.98 2.92 2.54 3.21 3.01 2.73 3.06 2.8K2O 1.58 0.25 2.85 0.48 1.52 2.30 2.11 2.31 2.53 1.6P2O5 0.25 0.15 0.20 0.05 0.30 0.20 0.25 0.12 0.10 0.1LOI 0.69 0.80 1.69 4.91 2.11 2.44 0.47 1.72 1.74 1.9
Total 97.22 98.57 99.17 100.0 99.20 99.95 99.32 100.1 100.2 98.6Rb 55 9 1 6 6 100 8 8 9 5
Ba 371 7 409 7 335 439 365 312 349 430Sr 350 162 466 326 457 482 423 270 245 210LaCePrNd
Sm
EuGd
DyEr
YbY
Zr
Nb
ScV 80 167 153 280 271 121 167 140 120 182Cr 68 232 1 3 1 3 2 1 1 3Ni 40 150 8 1
619
19
17
8 8 9
3.2. Middle to Late Miocene
Middle to Late Miocene rocks
are known from the Dent and
Samp orna peninsulas. They are
mostly inte r- medi ate in
compos ition (dacites to
andesi tes) with minor basaltic
rocks. The low Ti O2 and MgO and
the high alka li content are
indic ative of potassic calc -alka-
line anity and suggest a generic
rela tionship to sub- duction.
3.3. Late MiocenePliocene
Late Mioce nePlioce ne mag matic
act ivity gave rise to the for mation
of the mag matic rocks of Sabah
and Kinab alu. The dior ites of
Mount Kinab alu exhibit a normal
to potas sic calc-alka line ani ty,
with the charac teristi cs of
subd uction-re lated mag matism.The Pliocene volcanics consist of
thole iitic basal ts, some of wh ich
disp lay relativ ely high MgO
(high er than 6%) and TiO 2
(high er than 2.0% ); these
major eleme nt
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characteri stics point to
mag matism related to within-
plate geody namics.
Table 1 gives a sum mary ofCenozo ic mag matism
and possib le cha nges in the
respec tive tect onic environ- ment,
as inte rpreted from the main
chem ical signa tures revea led by
geochemistry and rock suite
ani ties.
4. Geodynamic interpretat ion
Based on the present data
concerning Te rtiary mag- mat ism
and the region al geology of
Kal imantan (inc luding Borne o)
four major periods of geodynam ic
evolution have been disting uished as
fol lows:
Acco rding to Dain es (1985)
rifting of the marg in of As ia to
pr oduce the South Chi na Sea
took place during
Eoc eneOligoce ne time, resu lting in
southeast- wa rd mo vement of the
Lucon ia continental block and
lead ing to the sub duction of part
of the South Chi na Sea Plate
beneath the northe rn marg in of
Sund aland.
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Fig. 5. Chondrite normalized extended spider-di agram of volcanic rocks (normaliza tionvalues after Sun and McDonou gh, 1989).
The Eoc eneEarly Oligoce ne
mag matic belt along this
continental margin can be follow ed
from Sintang (cen- tral West
Kaliman tan), through Kel ian to
the Up per Tara kan Basin. This
mag mati sm is conside red to be re-
lat ed to southea sterly
subduct ion in the Rajang
Tre nch. The proposed subduct ion
mo del is comparable to an active
contin ental margin of Chili an type
(Fig. 6).
Collision and doc king of the
Luconia contin ental block with
the northe rn margin of
Sund aland must have taken place
during the Middle Olig ocene, as
the youngest sedi ments involved in
the inten se foldi ng ofthe Rajang
Trench are of Early Oligoce ne
age (Hu tchison, 1996a).Defo rmation at this time is also
recorded by the Early Olig ocene
unco nformity in the Mela wi Basin
(Pieters et al., 1987). The suture
related to this collision, the Lupar
Line, is marked by imb ri- cated
ophi olites (Fig. 7).
Late Oligocen eMiddle Miocene
subduct ion-re lated mag matism is
superimposed on the Eoc ene
mag matic belt, and may be trac ed
from Sintang (the western most
part of the mag matic belt)
eastwa rds through
Masu paria and further
north wards to Mou nt Muro,
Kelia n, Muyup, Busang, Muara
Wahau and along the northe rn
ank of Mangkali hat and
Sesayap, Middle Miocen ePlioce ne
volcan ics are doc umented from
the region of the fossil Ra jang
Tre nch (Mo unt Hose,UsunApau and Niewenhu is), to
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Kinab alu and the Cag ayan Ridge,
while Late Miocene to Pleistocene
mag matism extends from the
Upper Tar akan Basin,
into the peninsulas of Dent
and Samporna and throu gh the
Sulu Arc to Mindanao.
The Late Oligoce neMiddle
Miocene mag matic ac- tivity is
perhaps related to remna nts ofthe Eoce ne subducted slab,
whe reas the Middle
Miocen ePlioce ne mag matic
activi ty along the Sibu-Rajang Zone
and Cag ayan Ridge is rela ted to
subduct ion in the Palaw an Trench
(Fig. 8). Th is Mioce ne subduction
could be the resu lt of
countercl ockwise rotation of
Bo rneo, as pro- posed by Hall(1996 ). Miocene subd uction-re lated
mag matism is also recorded from
Mo unt Kinab alu, the subma rine
oceanic ridge of Cag ayan and
Pan ay Isl and in the Phil ippines
(Bellon and Rang in, 1991).
In Cen tral Kalima ntan Miocene
volcan ic rocks are repre sented by
the Sintang Intrusives of potas sic
calc- alka line ani ty (He ryanto et
al., 1993) which are prob- ably
related to crustal thicke ning as
the resu lt of the collision with
the Lucon ia Bloc k. Hutchis on
(1996 a) sugges ts that Miocene
mag matism along the Cagay an
Rid ge does not continue into
Saba h. Ho wever, Bellon and
Rang in (1991) point out that theintrusive rocks of Mo unt Kinab alu
are also of calc-alka line anity,
wh ich may indicate that the
mag matism of the Cag ayan belt
does not extend west wards into
Sabah. The Late
Miocen ePlei stocene mag matic
arc of the Sulu Sea continues into
the Dent and Sampor na penin-
sula s. This mag matism is regard ed
as rela ted to sub- duction in the
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Sulu Tre nch (Hutchison, 1996a;
Be llon and Rangi n, 1991; Rang in
and Silv er, 1991). The wes- tern
part of this sub duction sys tem is
bound ed by a
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Fig. 6. A, The magmatic belt of Central Kalimantan during Eo-Oligo cene time. B, Schematicregional cross-secti on (modied from James, 1984).
1, Magmatic belt; 2, accretionary prism belt. Numb ers are K/Ar dates from volcanic rocks.
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Fig. 7. A, Collision belt of North Kalimantan during Middle Oligocene time. B, Schema tic
cross-secti on. 1, Folded belt/collisi on zone; 2, mag- matic belt. Numbers are Ka/Ar ages from
volcanic rocks.
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Fig. 8. A, Magmatic belt of Kalimantan during Late Oligoce neMiddle Miocene and Late
Miocen ePleistocene times. 1, Late Oligoce neMiddle Miocene magmatic belt related to the
Eocene subducted slab; 2, Middle Miocen ePliocene magmatic belt related to subduction inthe Palawan Trench; 3, Late Miocen ePleistocene magma tic belt related to subduction in
the Sulu Trench. B, Schematic cross-secti on. Numbers are K/Ar ages from volcanic rocks.
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NN W SSE sinist ral strike- slip fault
wh ich may be a north ward
extension of the Palu Koro Fault
(Fig. 8). Nor thward mov ement of
Celebes Sea Plate, as a conse-
quence of the collision of
Ban ggai-Sula with eastern
Sula wesi, may have ini tiated the
subd uction which for med the Sulu
Arc.
Relat ively large outcrops of
Plio -Pleistoce ne vol- canics have
been mapped by Pieters et al.
(1987) in the Niewen huis
Mo untains and Maha kam region,howev er none of them have been
described. Gener ally they are
basal tic in composition and their
rock chem istry shows continental
basalt anity. Basaltic roc ks from
Sintang and Sabah display
relativ ely high magne sia conten ts,
indic ating a more pri mitive
compos ition, sugges ting the
invol vement of oceanic basem entin their for- mati on.
The val idity of the inte rpretation
of the geo dynamic his tory of
Kaliman tan and Bo rneo as
presented above may be subject to
revision when recent work by
Fuller et al. (1999) is taken into
account. Fuller et al. (1999) report
two signi cant co untercloc kwise
rotations of Borneo which are not
incorpor ated in current synth- eses.
A better und erstan ding of the
geodynam ic hist ory of Kalima ntan
and Bo rneo will resu lt from
furth er geo physical work,
espec ially in those
areas of Kaliman tan whe re
eld data is scarce or unavaila ble.
Acknowledgements
The present authors are grat eful
to R.C. Maury and H. Bello n,
Univ ersite de Bretagne
Occide ntale, Brest (France ), for
their commen ts on the
geochem istry. We also thank J.P.
Rampnou x, Univ ersite de Savoie,
Le Bou rget du lac (France ), for his
sugges tions concerning the
geody namic inte rpretation.
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