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, OCTOBER 2015, 66, 5, 409—426 doi: 10.1515/geoca-2015-0034
Depositional environment, organic matter characterization
and hydrocarbon potential of Middle Miocene sediments
from northeastern Bulgaria (Varna-Balchik Depression)
ALEXANDER ZDRAVKOV
1
, ACHIM BECHTEL
2
, STJEPAN ĆORIĆ
3
and
REINHARD F. SACHSENHOFER
2
1
Department of Economic Geology, University of Mining and Geology “St. Ivan Rilski”, 1700 Sofia, Bulgaria; alex_zdravkov@mgu.bg
2
Department Angewandte Geowissenschaften und Geophysik, Montanuniversität Leoben, Peter-Tunner-Str. 5, A-8700 Leoben, Austria;
achim.bechtel@unileoben.ac.at; reinhard.sachsenhofer@unileoben.ac.at
3
Geological Survey of Austria, Neulinggasse 38, A-1030 Vienna, Austria;
stjepan.coric@geologie.ac.at
(Manuscript received January 9, 2015; accepted in revised form June 23, 2015)
Abstract: The depositional environments and hydrocarbon potential of the siliciclastic, clayey and carbonate sedi-
ments from the Middle Miocene succession in the Varna-Balchik Depression, located in the south-eastern parts of
the Moesian Platform, were studied using core and outcrop samples. Based on the lithology and resistivity log the
succession is subdivided from base to top into five units. Siliciclastic sedimentation prevailed in the lower parts of
units I and II, whereas their upper parts are dominated by carbonate rocks. Unit III is represented by laminated clays
and biodetritic limestone. Units IV and V are represented by aragonitic sediments and biomicritic limestones, corre-
lated with the Upper Miocene Topola and Karvuna Formations, respectively. Biogenic silica in the form of diatom
frustules and sponge spicules correlates subunit IIa and unit III to the lower and upper parts of the Middle Miocene
Euxinograd Formation. Both (sub)units contain organic carbon contents in the order of 1 to 2 wt. % (median: 0.8 for
subunit IIa; 1.3 for unit III), locally up to 4 wt. %. Based on Hydrogen Index values (HI) and alkane distribution
pattern, the kerogen is mainly type II in subunit IIa (average HI = 324 mg HC/g TOC) and type III in unit III (average
HI ~ 200 mg HC/g TOC). TOC and Rock Eval data show that subunit IIa holds a fair (to good) hydrocarbon genera-
tive potential for oil, whereas the upper 5 m of unit III holds a good (to fair) potential with the possibility to generate
gas and minor oil. The rocks of both units are immature in the study area. Generally low sulphur contents are prob-
ably due to deposition in environments with reduced salinity. Normal marine conditions are suggested for unit III.
Biomarker composition is typical for mixed marine and terrestrial organic matter and suggests deposition in dysoxic
to anoxic environments.
Key words: organic geochemistry, hydrocarbon potential, Euxinograd Formation, NE Bulgaria, Eastern Paratethys.
Introduction
The western Black Sea has long been recognized as a region
with high petroleum potential. The Tyulenovo Field (Fig. 1b)
was detected in the Bulgarian sector of the Black Sea in the
1950s. It contains significant oil ( ~ 30 Mbs) and gas reserves
( ~ 30 Bcf; Georgiev 2012). Additional potentially oil- and
gas-bearing structures have been identified on and offshore
Bulgaria in the 1990s. One of them, the Galata deposit, off-
shore cape Galata near Varna, already produced dry gas of
about 55 Bcf (Georgiev 2012).
The question of active source rocks is an important issue
for understanding petroleum systems. Georgiev (2012) con-
sidered the Middle to Late Jurassic shales from the Etropole
and Provadia Formations, drilled in the Galata area, as the
most likely source rocks for the formation of Tyulenovo oil.
The same author, however, reports the presence of oleanane,
which is an indicator for post-Jurassic source rocks, within
this oil. Sachsenhofer et al. (2009) studied Oligocene clays
of the Ruslar Formation and determined a good potential for
hydrocarbon generation. Apart from Oligocene rocks,
Eocene successions, which are of considerable thickness in
the deeper parts of the western Black Sea may hold a source
potential (Georgiev 2012).
No studies have been conducted so far on the Miocene
succession, although there are some notes on the presence
of organic matter-rich lenses within the diatomaceous clays
of the Middle Miocene Euxinograd Formation (Koleva-
Rekalova 1997). Thus, the limited knowledge on the amount
and origin of the organic matter within the Miocene rocks
leaves a gap in our understanding of the petroleum system in
NE Bulgaria and its off-shore part.
Therefore, the main aim of the present paper is to study li-
thology, depositional environment, and hydrocarbon potential
of the Miocene Euxinograd Formation and to explore vertical
and partly lateral facies variations. To reach this goal, core
material from Miocene rocks from borehole C-180a (Fig. 1b)
was studied. Additional samples from the upper part of the
Euxinograd Formation were taken from an outcrop near
Albena resort. The present investigation is based on bulk
geochemical parameters (inorganic and organic carbon, sul-
phur, hydrogen index), biomarker, and stable carbon isotope
composition of the organic matter. Since the lower part of the
Miocene succession, especially in the Balchik area, is not well
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studied due to limited core material, we also investigate rocks
underlying the Euxinograd Formation.
Geological setting
Miocene rocks are present in the southeastern part of the
Moesian Platform in Bulgaria and Romania (Popov et al.
1986; Popov & Kojumdgieva 1987; Fig. 1) and have been
studied intensively, because of their rich macro- and micro-
fauna, as well as diatom flora (Kojumdgieva 1965;
Kojumdgieva & Dikova 1978; Kojumdgieva & Popov 1987;
Darakchieva 1989; Temniskova-Topalova 1990).
The Miocene succession, about 300 m thick, has been depos-
ited in the relatively small, south-east widening Varna-Balchik
Depression (Fig. 1c) of the Eastern Paratethys (Kojumdgieva
& Popov 1981). The sediments overlie denudated Late Oli-
gocene clays (Ruslar Fm) and represent the time span from
the early Middle Miocene (Tarkhanian) to the middle Late
Miocene (Khersonian) (Popov & Kojumdgieva 1987). Based
on differences in sedimentary facies, Kojumdgieva & Popov
(1981), Popov et al. (1986) and Popov & Kojumdgieva (1987)
subdivided the Varna-Balchik Depression into the Varna
part, dominated by shallow marine siliciclastic deposits, and
the Balchik part, in which (sub-)littoral sandy to clayey sedi-
mentation prevailed (Figs. 1c, 2).
The following summary of basin evolution is based
mainly on Popov et al. (1986) and Popov & Kojumdgieva
(1987), who subdivided the Miocene succession into seven
formal and two informal lithostratigraphic units (Fig. 2).
The oldest Miocene rocks are biogenic limestones, 2 to
3 m thick, of Middle to Late Tarkhanian age (Karapelit Fm;
not shown in Fig. 2). They were formed in a relatively nar-
row strait along the South Dobrudzha lowlands (Fig. 1c),
which at that time connected the Eastern Paratethys with the
Fore Carpathian Basin. Within the Varna part of the depres-
sion, Tarkhanian sediments are represented by a few meters
of laminated clays near the base of Galata Formation. A ma-
Fig. 1. a – Tectonic map of Bulgaria, showing the position of the study area within the south-eastern part of the Moesian Platform (simplified
after Dabovski et al. 2002); b – Simplified geological map of the studied area (modified after Cheshitev et al. 1994a,b, 1995); c – Schematic
scheme of the paleogeography of the studied area during the Miocene (modified after Popov & Kojumdgieva 1987).
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rine regression triggered by enhanced tectonic activity inter-
rupted the connection with the Fore Carpathian Basin at the
end of the Tarkhanian.
The overlying Galata Formation is limited to the Varna part
of the depression (Fig. 2). It is composed predominantly of
mid- to coarse-grained sands, intercalated by frequent clay
and rare limestone and clayey sandstone beds. Ori (2004)
investigated outcrops south of Varna and established a shal-
low marine environment with predominant beach sands,
tidal deposits and deltaic channels. According to Popov &
Kojumdgieva (1987), the southern part of the depression be-
came dry land at the end of the Chokrakian shifting the area of
maximum sedimentation northwards. North of Varna, deposi-
tion of the sediments of the Galata Formation continued until
Early Volhynian time (Fig. 2), but the quantity of siliciclastic
material was significantly reduced (Popov & Kojumdgieva
1987). At the same time up to 85 m of white-greenish calcare-
ous clays, irregularly alternating with marls, and oolitic, bio-
genic, or bioclastic limestones were deposited in the Balchik
part of the depression (Clay-limestone formation; Fig. 2). The
rocks are known from few wells and poorly studied.
The overlying Euxinograd Formation (Fig. 2) is made up
of finely laminated, diatomaceous pelites with frequent thin
(2—20 mm) coquina intercalations composed of well-stratified
shell fragments. Koleva-Rekalova (1997) also reported the
presence of lenses, rich in plant remains. Thin interlayers of
sandstone or limestone are very rare. Some rocks were de-
scribed as diatomite (Popov & Kojumdgieva 1987). However,
Koleva-Rekalova (1997) showed that opal sponge spicules
prevail over diatom frustules. Studies performed by Koleva-
Rekalova (1997, 1998), indicate deposition in a sublittoral low
energy environment, influenced by surface water currents, in-
troducing significant amounts of bioclastic material to the
deeper zones of the depression. Based on the abundant fauna
Kojumdgieva & Dikova (1978), estimate a water depth of less
than 100 m, which is consistent with the predominance of
Fig. 2. Lithological columns of the Miocene suc-
cession in the Varna-Balchik Depression (modified
after Popov & Kojumdgieva 1987). Correlation of
regional stages after Steininger & Wessely (2000).
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benthic foraminifera (Darakchieva 1989) and with high
amounts of sponge spicules (Koleva-Rekalova 1998). The
thickness of the Euxinograd Formation varies considerably
and exceeds 100 m in the central part of the depression north
of Varna (Popov & Kojumdgieva 1987). North and west of
Balchik, the sand-limestone formation splits the Euxinograd
Formation into a lower and an upper unit (Fig. 2 – Popov &
Kojumdgieva 1987) and reduces its thickness significantly.
Increased terrigenous input from the north (sand-limestone
fm) and south (Franga Fm), was probably a result of late
Volhynian uplift of surrounding areas (Fig. 2 – Popov &
Kojumdgieva 1987), limited the area of deposition of the
Euxinograd Formation to the central basin between Balchik
and Albena resort. This situation lasted until the Early
Bessarabian, when decreased terrigenous input allowed ex-
pansion of the area of clay deposition to the northern part of
the depression.
After the Middle Bessarabian water salinity increased rap-
idly resulting in carbonate sedimentation. The area of the ba-
sin gradually diminished and was generally restricted to the
Balchik part of the depression. Koleva-Rekalova (1994,
1997, 1998); Koleva-Rekalova & Darakchieva (2002) pro-
vide a comprehensive overview of the Sarmatian rocks. Po-
rous bioclastic to oolitic limestones with micritic cement
(Odarci Fm; Fig. 2) were deposited in shallow environments,
followed by massive aragonitic sediments that in upper part
show seasonal lamination (Topola Fm; Fig. 2). According to
Koleva-Rekalova (1998) these rock formed due to chemical
precipitation of needle-like aragonite crystals in shallow wa-
ter under specific conditions. The youngest Miocene rocks
are micritic limestones with varying abundance of bivalve
shells (Karvuna Fm; Fig. 2).
Methods
The present study is based on 47 core samples from well
C-180a drilled during the 1980s. The aim of the well was to
study the Lower Cretaceous (Valanginian) carbonate succes-
sion, the main aquifer in north-eastern Bulgaria. Unfortunately
there is no information on Miocene rocks. Therefore, we use
geophysical data from well C-180, located about 20 m north
of C-180a, to reconstruct the lithology of the missing parts of
the studied core. Twelve additional samples were taken from
an outcrop near Albena resort (Fig. 1b), representing about
5 m from the upper part of the Euxinograd Formation.
For microscopic investigations thin slides were prepared
and studied under transmitted light using polarized micro-
scope Leica DM 2500P.
Total carbon (TC) and sulphur (S) contents were deter-
mined with an Eltra Helios C/S analyser. Total organic car-
bon (TOC) content was determined on samples pretreated
with phosphoric acid. Total inorganic carbon (TIC =TC—TOC)
contents were used to calculate calcite equivalent percentages
(calcite
eq
= TIC
×8.34). Rock-Eval pyrolysis was performed
using a Rock-Eval 6 instrument. S
1
and S
2
(mg HC/g rock)
values were used to calculate Hydrogen index (HI = 100
×S
2
/
TOC[mg HC/g TOC]) and Production index (PI = S
1
/(S
1
+ S
2
);
Espitalié et al. 1977). The temperature of maximum hydro-
carbon generation (T
max
) was recorded as a maturity para-
meter.
Biogenic silica contents were measured using the method
proposed by Zolitschka (1998) and a Perkin-Elmer 3000
AAS spectrometer. The silica contents were used to calculate
the opal percentages ( = biogenic silica
×2.4).
21 samples, mostly containing TOC greater than 1 wt. %,
were chosen for biomarker analysis. Approximately 10 g of
each sample were extracted for approximately 1 h using
dichloromethane (DCM) in a Dionex ASE 200 accelerated
solvent extractor. Asphaltenes were precipitated from a hex-
ane-DCM solution (80 : 1) and separated by centrifugation.
The hexane-soluble fractions were subdivided into saturated
and aromatic hydrocarbons and NSO components using a
Köhnen-Willsch MPLC instrument (Radke et al. 1980). No
separation of the aliphatic and aromatic fractions was conducted
only in the case of sample C-20, due to the low amount of ex-
tract. This sample was analysed by GC-MS as total fraction.
The saturated and aromatic hydrocarbons fractions were
analysed by a gas chromatograph-mass spectrometer (GC-MS)
Thermo Fisher Trace Ultra, equipped with a silica capillary
column. Oven temperature was programmed from 70-300 °C
with steps of 4 °C/min, followed by an isothermal period of
15 min. Helium was used as the carrier gas. The device was
set in electron impact mode with a scan rate of 50—650 Daltons
(0.7 sec/scan). Data were processed with Thermo-Fisher
Xcalibur ® v. 2.0. Identification of biomarkers is based on
retention time and comparison of mass spectra with pub-
lished data. The determination of absolute concentrations of
biomarkers was done using internal standards (deuterated
n-tetracosane for the aliphatic fraction and 1,1’-binaphthyl
for the aromatic fraction). The concentrations were normal-
ized against the total organic carbon contents.
Carbon isotope determination of n-alkanes and isoprenoid
hydrocarbons was performed on 11 samples using a Trace GC
ultra attached to a ThermoFisher DELTA-V ir-MS via a com-
bustion interface (GC Isolink, ThermoFisher). For calibration,
a CO
2
standard was injected at the beginning and end of each
analysis. The GC coupled to the ir-MS was equipped with the
column described above and the temperature program was the
same as for GC-MS analysis. Isotopic composition is reported
in the
δ notation relative to the PDB standard.
Results and discussion
The lithological profile of well C-180a is plotted together
with the resistivity log in Fig. 3. Based on lithology, the Mio-
cene succession can be divided into five units, which in gen-
eral correspond to the lithostratigraphic units introduced by
Popov & Kojumdgieva (1987).
Lithology
Unit I
Unit I discordantly overlies finely laminated Oligocene
brownish clays and correlates with the Clay-limestone for-
mation from the northern part of the Varna-Balchik Depres-
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sion and with the Galata Formation from its southern part
(Popov & Kojumdgieva 1987). The unit is 87 m thick (Fig. 3)
and can be subdivided into two subunits.
Subunit Ia – is about 35 m thick and is represented by
white-greenish, very soft fine-grained glauconitic sands. The
rocks appear homogenous, but sedimentary structures within
the non-lithified sands may have been obliterated during
coring. Carbonate contents are typically low (<3 wt. %;
Table 1), but reach up to 25 wt. % in the upper part of the
section. Carbonate is exclusively represented by micrite crys-
tals. No biogenic carbonate remains were detected. Micro-
scopic investigations showed that the detrital material is
predominantly of fine- and very fine sand-size fractions. The
mineral composition is relative uniform and is dominated by
quartz and glauconite. Rare feldspar (mostly orthoclase; rare
microcline), as well as mica flakes, can also be found. Some
samples contain lithic fragments, composed of polycrystal-
line quartz, and fine charcoal fragments. Irregular-shaped,
subangular to subrounded quartz grains are the predominant
detrital component. Significant amounts (15—30 wt. %) of
light green glauconitic pellets with very fine sand sizes give
the rocks a pale greenish colour. Under the microscope, most
glauconite grains show red-brownish colours, indicating
initial oxidation. Although an authigenic origin of glau-
conite is possible, we assume a detrital origin, because glau-
conite-bearing Cretaceous and Paleogene rocks exist in the
hinterland.
Subunit Ib – about 52 m thick (Fig. 3), is composed of
hard, but highly porous biomicritic limestone layers with
randomly orientated intact and fragmented bivalve shells.
These rocks alternate irregularly with marlstones, up to 1 m
thick. A thin layer of oolitic limestone was observed in the
upper part of the subunit. Although the core representing the
lower part of subunit Ib is missing, a gradual upward in-
crease in resistivity suggests a continuous transition from
subunits Ia to Ib.
Popov et al. (1986) give a similar description for the rocks
from the Clay-limestone formation in two other drill holes
from the Balchik area. Considering the above data, we as-
sume that deposition of subunit Ia commenced in a sand and
mud dominated shallow marine environment, characterized
by high terrigenous input. The small grain size indicates for-
mation in a relatively low energy environment, probably
within the inner shelf below the wave-dominated zone. Ac-
cording to Kojumdgieva (1965), the Chokrakian was a time
of reduced salinity. Very low sulphur contents in sediments
of unit Ia may support this interpretation.
During the later stages of subunit Ia sediment deposition, a
gradual decrease of the terrigenous input enabled increased
carbonate deposition. Apart from this, the sedimentary envi-
ronment most probably did not change significantly. The
dominance of biomicritic limestone with random orientation
of the fossils in subunit Ib argues for deposition in shallow
marine environments with bottom currents and/or waves.
Oolitic limestone interbeds in the upper part of the subunit
indicate a change to a very shallow, high energy environ-
ment (Tucker & Wright 1990).
Unit II
Unit II, about 47 m thick, follows above unit I with a sharp
boundary. Similar to unit I, two subunits can be distinguished
(Fig. 3).
Subunit IIa – is composed of 13-m-thick sandy limestone
in transition to fine sand with micrite matrix. The rocks are
white to white-grey, very soft and friable. The carbonate con-
tent varies significantly between 21 and 80 wt. % and is rela-
tive low in the middle part of the subunit (Table 1, Fig. 4).
Carbonates are almost exclusively represented by micrite
crystals. With the exception of few foraminifera, detected by
light microscopy, no other organic remains were detected.
The siliciclastic component is composed of fine and very
fine sand-sized quartz grains and rare feldspar and glauco-
nite grains. The clastic fraction is further characterized by
the presence of detrital mudstone fragments, often including
small charcoal fragments. This shows that at least part of the
organic matter is redeposited.
Fig. 3. Lithologi-
cal profile of well
C-180a, together
with geophysical
resistivity log.
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Table 1: Depth from surface, sulphur (S), total organic carbon (TOC), total inorganic carbon (TIC), calcite equivalent (eq.) percentages, biogenic
silica (BSi), TOC/S ratio, Rock Eval parameters (S
1
, S
2
, T
max
), hydrogen index (HI), production index (PI), soluble organic matter yield (SOM),
and relative proportion of saturated (Sat. HC) and aromatic (Aro. HC) hydrocarbons, polar compounds (NSO) and asphaltenes (Asph.).
Sample Depth Unit
S TOC TIC Calcite eq. BSi
TOC/S
S
1
S
2
Tmax
HI PI
SOM
(mg/g TOC)
Sat. HC Aro. HC NSO Asph.
(wt. %)
mg HC/g
rock
(°C)
(wt. %, SOM)
Drillhole C-180a
C-1
107.0
U
n
it
II
I
0.2 1.6 6.6
54.9 2.4
6.7 0.2 4.2 423 254 0.04
19 16
2
67
14
C-2
107.4 0.7
1.6
6.4
53.0 2.6
2.4 0.2 3.7 424 229 0.04
C-3
107.9 0.0
0.7
9.9
82.3 1.2
93.6 0.1 1.6 429 210 0.05
29 18
0
71
10
C-4
108.2 1.0
2.6
4.2
35.3 6.5
2.6 0.4 7.9 422 301 0.05
C-5
108.5 1.4
4.3
4.0
33.1 1.9
3.0 0.5 8.6 423 201 0.05
25 22
2
65
12
C-6
108.8 1.5
3.7
3.4
28.1 3.9
2.5 0.4 7.5 422 205 0.05
C-7
109.0 1.0
3.2
5.2
43.4 2.4
3.1 0.3 6.5 422 203 0.04
21 12
0
72
15
C-8
109.3 1.2
2.9
4.7
39.4 1.7
2.4 0.3 5.2 424 176 0.05
C-9
109.5 0.4
1.8
7.2
60.0 0.9
4.8 0.1 3.2 423 179 0.04
18 16
2
71
11
C-10
109.8 0.4
1.2
7.3
60.6 1.0
3.4 0.1 2.8 425 227 0.04
C-11
110.2 0.5
1.3
6.6
55.2 2.4
2.8 0.1 2.2 425 174 0.04
35 34
1
58
7
C-12
110.6 0.3
1.2
6.2
51.6 2.4
4.8 0.1 3.3 422 272 0.03
26 18
0
67
14
C-13
110.7 0.2
0.6
8.0
66.8 1.0
3.3 0.1 1.0 428 172 0.06
C-14
111.5 0.7
1.1
6.0
49.7 1.9
1.7 0.2 3.8 425 333 0.04
35 14
0
74
12
C-15
112.0 0.5
1.3
5.1
42.5 1.9
2.5 0.1 1.7 426 129 0.05
30 16
1
74
9
C-16
113.0 0.0
0.6
8.6
71.6 1.0
49.8 0.1 1.3 429 213 0.05
51 42
0
55
2
C-17
113.7 0.0
0.6
8.8
73.4 2.0
80.9 0.1 1.2 429 194 0.05
37 12
0
84
3
C-18
114.0 0.0
0.6
8.3
69.0 1.7
94.6 0.1 0.9 428 136 0.06
C-19
114.2 0.0
0.6
7.6
63.1 1.9 184.7 0.0 0.6 433 96
0.06
C-20
114.5 0.0
0.2
10.4
86.4 0.9 146.7 –
–
–
–
–
41 –
–
–
–
C-21
148.7
Uni
t IIa
0.0 1.7 8.1
67.7 0.5
63.1 0.2 3.8 420 223 0.06
16 31
18
37
14
C-23
149.4 0.0
0.7
5.6
47.0 9.0
37.3 0.2 2.2 419 318 0.06
C-24
149.8 0.0
0.3
7.7
63.8 5.1
45.9 0.1 1.0 419 309 0.07
C-25
150.3 0.0
0.8
8.0
66.3 2.1
48.4 0.2 2.5 419 318 0.07
C-26
152.0 0.5
1.1
4.5
37.8 3.3
2.2 0.3 4.3 416 397 0.07
21 9
5
83
3
C-27
153.0 0.0
0.9
4.6
38.3 11.8
38.0 0.3 3.4 415 359 0.08
C-28
153.9 0.0
1.0
7.8
64.9 14.3
47.2 0.3 3.8 421 360 0.07
20 24
10
59
7
C-29
154.7 0.1
0.8
2.9
24.4 4.5
6.2 0.2 3.4 418 427 0.06
C-30
155.2 0.0
0.5
6.6
55.0 8.7
27.3 0.1 1.4 418 287 0.07
C-22
155.7 0.9
2.8
2.5
20.9 2.4
3.1 0.5 7.3 419 257 0.06
14 31
13
41
15
C-31
157.9 0.0
1.0
3.7
31.0 22.1
40.4 0.4 4.8 419 464 0.08
40 18
9
62
11
C-32
158.6 0.0
0.9
4.2
35.1 11.1
46.3 0.3 4.4 422 501 0.06
C-34
159.7 0.0
0.2
6.7
55.5 1.5 260.2 0.0 0.3 423 186 0.08
C-35
160.5 0.0
0.7
8.4
69.7 1.5
42.9 0.1 1.4 420 209 0.06
18 22
13
55
9
C-36
161.5 0.0
0.6
9.6
80.2 1.3
43.2 0.1 1.6 423 248 0.07
C-37
214.3
Uni
t Ia
0.3 0.1 0.3
2.3 –
0.2 –
–
–
–
–
C-38
215.3 0.1
0.1
2.3
19.5 –
0.6 –
–
–
–
–
C-39
216.4 0.2
0.1
2.4
19.6 –
0.4 –
–
–
–
–
C-40
219.2 0.0
0.2
3.1
25.5 –
33.9 –
–
–
–
–
C-41
221.0 0.0
0.0
0.9
7.1 –
11.0 –
–
–
–
–
C-42
230.0 0.0
0.1
0.1
0.5 –
18.7 –
–
–
–
–
C-43
231.0 0.0
0.0
0.0
0.2 –
17.7 –
–
–
–
–
C-44
232.0 0.0
0.0
0.0
0.4 –
11.2 –
–
–
–
–
C-45
236.0 0.1
0.1
0.1
0.8 –
0.5 –
–
–
–
–
C-46
238.0 0.0
0.0
0.2
1.5 –
13.4 –
–
–
–
–
C-47
240.0 0.0
0.1
0.1
0.9 –
16.4 –
–
–
–
–
C-48
241.0 0.0
0.1
0.3
2.6 –
44.2 –
–
–
–
–
Outcrop near Albena resort*
A-1
3.7
Uni
t III
0.0 0.1 0.2
1.4 8.2
1.9 – –
–
–
–
A-2
4.1 1.1
0.9
1.5
12.2 8.5
0.8 0.1 1.5 411 166 0.06
A-3
4.4 0.8
1.1
1.8
14.7 12.8
1.4 0.2 2.4 414 216 0.06
21 11
5
53
31
A-4
4.8 1.0
1.2
1.9
16.2 1.4
1.2 0.2 2.5 417 213 0.06
A-5
5.2 0.4
1.0
2.2
18.4 11.6
2.7 0.1 2.0 417 200 0.05
A-6
5.6 0.3
0.7
3.0
25.0 7.3
2.2 0.1 1.3 413 171 0.06
A-7
6.0 0.6
1.1
2.5
21.1 10.6
1.8 0.1 2.4 412 207 0.02
15 12
6
51
31
A-8
6.4 0.4
0.7
3.4
28.2 3.7
1.7 0.2 0.6 419 77
0.22
A-9
6.7 0.6
1.1
2.8
23.3 8.6
1.8 0.1 2.4 419 213 0.04
A-10
7.1 0.5
1.0
3.5
29.1 9.9
2.0 0.1 2.5 415 256 0.05
A-11
7.6 0.5
1.3
4.1
33.8 5.5
2.5 0.1 2.2 415 175 0.05
19 12
7
42
39
A-12
8.1 0.5
1.1
2.7
22.3 1.6
2.1 0.1 2.4 423 220 0.04
* — Sampling position in meters above sea level.
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Fig. 4. Vertical distribution of total organic carbon (TOC), sulphur, calcite equivalent percentages, biogenic silica (BSi), hydrogen index (HI),
relative proportions of n-alkanes, CPI, pristane/phytane ratio, sterane and hopane concentrations in core samples from subunit IIa and
unit III, and outcrop samples.
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Rocks from subunit IIa contain varying amounts of bio-
genic silica derived from diatom frustules (Table 1). Diatom
remains were previously detected mostly within clays of
the Euxinograd Formation (Popov & Kojumdgieva 1987;
Temniskova-Topalova 1990). This suggests that subunit IIa
is coeval with the lower part of this formation. Biogenic
silica contents reach a maximum of 22 wt. % about 4 m
above the base of the subunit (C-31) and decrease upwards
(Fig. 4, Table 1). However, the biogenic silica content may
significantly under estimated diatom contents. For example,
microscopic inspection revealed that sample C-23 (9 wt. %
silica) contains significantly more than 50 % of diatoms. The
abundance of diatoms reflects a high nutrient supply and dis-
solved silica (DeMaster 2003). High nutrient supply is also
supported by the frequent occurrence of calcareous nanno-
plankton assemblage rich in Braarudosphaera bigelowii
(Gran & Braarud 1935) Deflandre, 1947 in sample C-31,
which also argues for reduced salinity and cold water envi-
ronment. High nutrient and silica supply may be related to
rhyolitic volcanic activity, indicated by tephra layers within
the Euxinograd Formation (Milakovska et al. 2001). The oc-
currence of Cyclicargolithus floridanus (Roth & Hay in Hay
et al. 1967) Bukry, 1971 shows that sample C-23 is not
younger than 13.33 Ma (Lourens et al. 2004).
Subunit IIb – is represented by white to grey-white
biomicritic limestone, similar to that in subunit Ib. Although
significant parts of the core are missing, the resistivity log
suggests the presence of limestone within the missing inter-
vals. The similarity of the lithologies of units I and II suggest
that the rocks formed in similar sedimentary environments.
Unit III
Unit III in well C-180a is about 14 m thick and represents
the upper part of the Euxinograd Formation (Figs. 2, 3). Its
characteristics are similar to the 5-m-interval studied in the
outcrop section. At both sites unit III is composed of a mo-
notonous succession of fine-laminated clays and detritus of
bivalve shells. With the exception of a few samples, the
Fig. 5. Graphs of TOC versus calcite equivalent percentages.
rocks contain no detrital sand-sized grains. Needle-shaped
siliceous sponge spicules are extremely abundant in the up-
per part of the unit (samples C-10 to C-1) where biogenic
silica contents reach up to 6.5 wt. % (Table 1).
The presence of sponge spicules proves deposition in a low
energy sedimentary environment (Krautter 1998). A low en-
ergy environment and oxygen-depleted conditions are also
supported by the lamination of the rocks (see also
Kojumdgieva & Dikova 1978; Koleva-Rekalova 1998). The
presence of ascidian spicules indicates shallow water condi-
tions and enrichment in the nutrient supply (Toledo et al.
2007). Whereas sponge spicules are abundant in well C-180a,
diatoms are more frequent in the outcrop samples, maybe
due to different distance from the shoreline.
Redeposited coaly organic material is present, as in sub-
unit IIa.
Units IV and V
Units IV and V correlate with the Upper Miocene Topola
and Karvuna Formations (Popov & Kojumdgieva 1987),
respectively. They are represented mainly by white mas-
sive and fine laminated aragonitic sediments (Topola Fm;
Fig. 2 – Koleva-Rekalova 1994) and biomicritic limestones
(Karvuna Fm; Fig. 2). Since the rocks do not contain organic
matter, they are not considered in this study.
TOC and Rock-Eval parameters
Total organic carbon (TOC) contents are listed in Table 1
and are plotted versus depth in Fig. 4. TOC contents in
subunit Ia are very low ( < 0.2 wt. %; Table 1) and vary be-
tween 0.2 and 4.3 wt. % in the rest of the samples. The high-
est TOC contents (1.8—4.3 wt. %) were detected in the upper
part of unit III from well C-180a (Table 1, Fig. 4). Single
samples with TOC contents up to 2.8 wt. % also exist in the
middle and upper part of subunit IIa (Table 1, Fig. 4).
Fig. 5 shows the relationship between TOC and calcite eq.
percentages. Whereas there is no linear relation for units Ia
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and IIa, and the studied outcrop (unit III), a strong negative
relation (correlation coefficient: —0.86) exists for samples
from unit III from well C-180a. Ricken (1991) points out
that a negative correlation is indicative for roughly constant
organic matter production and dilution by varying amounts
of calcite. Calcite in this unit is mostly derived from calcare-
ous bivalve shell fragments.
Because of very low TOC contents, TOC/S ratios have not
been calculated for samples from subunit Ia. For samples
from units IIa and III TOC/S ratios range between 1.7 and
260.2. In general, the ratios are higher in subunit IIa (me-
dian: 42.9) than in unit III (3.4). High values in subunit IIa
are consistent with a salinity-reduced environment. The
TOC/S trend in unit III suggests an upward increase of salin-
ity to normal marine conditions during deposition of the up-
permost part of the Euxinograd Formation. Anoxic conditions
indicated by TOC/S ratios below 2.8 (Berner 1984; Raiswell
& Berner 1986) are not reflected by the data.
Hydrogen index (HI) values are summarized in Table 1.
Their vertical distribution is shown in Fig. 4. Peters (1986)
points out that pyrolysis experiments usually give erroneous
results in samples with low TOC contents. For that reason HI
was not calculated for samples, containing less than 0.2 wt. %
TOC. These are mostly from subunit Ia, but also samples
C-20 and A-1 from unit III. HI values vary significantly be-
tween 77 and 501 mg HC/g TOC.
Surprisingly, the sandy subunit IIa exhibits higher HI val-
ues (Fig. 6a; average: 324 mg HC/g TOC), than the clayey
unit III (205 and 192 for core and outcrop samples, respec-
tively). This is also reflected in plots of S
2
versus TOC
(Langford & Blanc-Valleron 1990) and HI versus T
max
(Fig. 6b – Espitalié et al. 1984). Whereas kerogen types II-III
prevails in unit III, kerogen type II predominates in sub-
unit IIa. Because biomarker data (see below) argue against a
higher contribution of landplants to the organic matter in
unit III, the difference might reflect enhanced microbial al-
teration of the organic matter in unit III.
Hydrocarbon potential
Peters (1986) proposed a classification scheme for source
rocks based on TOC, S
2
and HI values. The respective average
values for subunit IIa (TOC : 0.9 wt. %; S
2
: 3.0 mg HC/g rock;
HI : 324 mg HC/g TOC) show that it holds a fair to good hy-
drocarbon generative potential for oil. The upper 5 m of unit III
(TOC:1.7 wt. %; S
2
:3.5 mg HC/g rock; HI:205 mg HC/g TOC)
show that this thin interval holds a good to fair potential with
the possibility to generate gas and minor oil.
The low maturity and the relatively low thickness of both
diatom-bearing intervals, which are considered equivalents
of the Euxinograd Formation, prevent significant hydrocar-
bon generation in onshore areas. However, both, thickness
and maturity may increase towards the east in offshore areas.
Molecular composition of the hydrocarbons
The normalized yields of the soluble organic matter (SOM)
are presented in Table 1 together with the contents of satur-
ated and aromatic hydrocarbons, hetero-compounds (NSO)
and asphaltenes. The contents of SOM are generally low
(14—51 mg/g TOC), which is in accordance with a low matu-
rity of the organic matter. In all samples, the SOM is mainly
represented by polar compounds (37—84 wt. %; Table 1). It is
noticeable, that most borehole samples show increased con-
tents of saturated hydrocarbons and are depleted in aromatics
and asphaltenes, in relation to outcrop samples. This finding
might be an indication of the presence of free hydrocarbons in
these samples. However, very low PI values (Table 1) are not
consistent with the presence of mobile products.
n-Alkanes
The total ion current (TIC) chromatograms of the saturated
hydrocarbon fractions of eight samples are shown in Fig. 7.
The vertical trends of the n-alkanes and CPI (Carbon Prefer-
ence Index after Bray & Evans 1961) in units IIa and III in
well C-180a, are presented in Fig. 4.
Fig. 6. Plots of S2 versus TOC (a) and HI versus T
max
(b). Dashed
lines in Fig. 6a represent HI values of 200 mgHC/gTOC (kerogen
type III) and 700 mgHC/gTOC (kerogen type I).
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ZDRAVKOV, BECHTEL, ĆORIĆ and SACHSENHOFER
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All samples are characterized by the presence of n-alkanes
in the range of n-C
15
to n-C
33
(Fig. 7). However, their distri-
butions vary justifying the definition of three groups.
(i) Most samples from subunit IIa and six samples from
unit III are characterized by a predominance of short-chain
n-alkanes (n-C
15—20
; Table 2, Fig. 7) and contain minor amounts
of mid- and long-chain hydrocarbons. Typically, the domi-
nant n-alkane is n-C
17
, accompanied by appreciable amounts
of n-C
16
and n-C
18
, with no odd-over-even predominance.
(ii) Outcrop samples from unit III show distributions domi-
nated by mid- (n-C
21—25
) and long-chain n-alkanes (n-C
27—33
;
e.g. sample A-7 in Fig. 7), with maximum concentrations of
n-C
29
or n-C
31
. The CPI is moderately high (1.7—2.2; Table 2),
and short-chain hydrocarbons are usually absent.
(iii) Another six borehole samples from unit III are domi-
nated either by n-C
20—22
, with a maximum at n-C
21
(e.g. C-5,
C-9) and a CPI of 1.2 to 1.7, or by n-alkanes in the range of
n-C
23—33
with a low CPI (1.1—1.3; e.g. C-11; Fig. 7).
Short-chain n-alkanes originate mostly from algae and mi-
croorganisms (Blumer et al. 1971; Cranwell 1977). Han et al.
(1968) and Han & Calvin (1969) established a marked pre-
dominance of n-C
17
in blue-green algae, and appreciable
amounts of n-C
16
and n-C
18
in photosynthetic and non-photo-
synthetic bacteria. Considering the predominance of n-C
17
, a
significant contribution from phytoplankton and microorgan-
isms can be suggested for samples with a type (i) distribution.
Mid-chain n-alkanes (n-C
21—25
) are typical mostly for sub-
merged aquatic plants and some moss species (Cranwell
Fig. 7. Gas chromatograms of the saturated hydrocarbon fraction (Std. = standard). The numbers correspond to n-alkanes with the respective
carbon atoms. Asterisk numbers correspond to iso-alkanes with the respective carbon atoms.
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Table 2: Molecular composition of the organic matter.
n
-C
15—20
/n-C
15—33
= ; n-C
21—25
/n-C
15—33
= ; n-C
27—31
/n-C
15—33
= .
CPI — Carbon Preference Index (according to Bray & Evans 1961),
CPI = 0.5*( + ).
Pri – Pristane, Phy – Phytane;
C-27/steranes = ; C-28/steranes = ; C-29/steranes = .
Ts – 18
α-22,29,30-trisnorneohopane, Tm – 17α-22,29,30-trisnorhopane, MN – methyl naphtalenes, DMN – dimethyl naphtalenes,
TMN – trimethyl naphtalenes, P – phenanthrene, MPh – methyl phenanthrenes, PAH – polyaromatic hydrocarbons (fluoranthrene
+ pyrene + benzo[a]pyrene + chrysene).
Aryl Isoprenoids =
di-MTTC/tri-MTTC = .
Σ
20
i=15
(n-Ci)
Σ
33
i=15
(n-Ci)
Σ
25
i=21
(n-Ci)
Σ
33
i=15
(n-Ci)
Σ
33
i=27
(n-Ci)
Σ
33
i=15
(n-Ci)
(n-C
25
+n-C
27
+n-C
29
+n-C
31
+n-C
33
)
(n-C
24
+n-C
26
+n-C
28
+n-C
30
+n-C
32
)
(n-C
25
+n-C
27
+n-C
29
+n-C
31
+n-C
33
)
(n-C
26
+n-C
28
+n-C
30
+n-C
32
+n-C
34
)
1977; Ficken 2000). However, Han & Calvin (1969) estab-
lished that mid-chain n-alkanes are typical components of
bacterial lipids, especially in sulphate-reducing bacteria, thus
indicating that microorganisms could also be a source of
these hydrocarbons.
Long-chain n-alkanes with a high CPI are characteristic of
waxes from vascular plants (Eglinton & Hamilton 1967).
This suggests a major contribution of land plants for outcrop
samples with a type (ii) distribution and a minor contribution
for type (i) samples. However, other possible sources for
long-chain n-alkanes have also been recognized. These in-
clude different bacterial communities, which produce mostly
hydrocarbons with lower odd-over-even predominance (Albro
& Dittmer 1967; Han & Calvin 1969; Johnson & Calder
1973; Volkman et al. 1980, 1983; Lichtfouse et al. 1994).
Furthermore bacterial degradation of organic matter is known
to reduce the CPI (Allen et al. 1971; Johnson & Calder 1973;
Gagosian et al. 1983; Meyers 1994; Volkman & Tanoue
2002). Considering the partly high amount of long-chain
n-alkanes with a low CPI in samples with a type (iii) distri-
bution, a significant contribution of bacterial sources to the
long-chain n-alkanes can be assumed. As seen in Table 3,
the isotopic fractionation of the long- and short-chain n-al-
kanes do not differ significantly, which might be due to their
similar origin. Nevertheless, the higher plant contribution to
the long-chain alkanes is also noticeable by the slight deple-
tion in
13
C ( ~ 0.5 ‰) of these compounds. On the other
hand, redeposition of terrestrial organic matter might also
Σ αααC
27
(20S+20R)
Σ
29
i=27
αααC
i
(20S+20R)
ΣαααC
28
(20S+20R)
Σ
29
i=27
αααC
i
(20S+20R)
ΣαααC
29
(20S+20R)
Σ
29
i=27
αααC
i
(20S+20R)
Σ
21
i=13
C
i
trimetyl (2,3,6)-alkylbenzol.
dimethylated 2-methyl-2-(4´,8´,12´-trimethyltridecyl)chroman
trimethylated 2-methyl-2-(4´,8´,12´-trimethyltridecyl)chroman
Sa
m
p
le
n-Alkanes
CP
I
Isoprenoids
Steranes Hopanespanes
Naphthalenes
S
u
m
(
µ
g/
g
TO
C
)
n
-C
15–20
/n
-C
15–33
n
-C
21–25
/n
-C
15–33
n
-C
26–31
/n
-C
15–33
S
u
m
(
µ
g/
g
TO
C
)
Pr/Ph
S
u
m
(
µ
g/
g
TO
C
)
C
27
/Σ
st
era
n
es
C
28
/Σ
st
era
n
es
C
29
/Σ
st
era
n
es
S
u
m
(
µ
g/
g
TO
C
)
Ts
/(
Ts
+
T
m)
2
2
S
/(
22
S+22
R)
C
-31-
H
o
p
a
n
es
Ho
p-1
7
(2
1
)-e
n
(µ
g/
g T
O
C)
S
a
t.
D
it
erp
en
oid
s
(µ
g/
g T
O
C)
MN (µ
g/
g T
O
C)
DMN (µ
g/
g T
O
C)
TM
N
(
µ
g/
g
TO
C
)
M
P
(
µ
g/
g
TO
C
)
P
A
H
(
µ
g/
g
TO
C
)
A
ryl
I
sop
ren
oid
s
(µ
g/
g T
O
C)
Chr
o
m
a
ns
(µ
g/
g T
O
C)
d
i-
M
TTC
/t
ri-
M
TTC
C-1
102.8 0.5 0.2 0.2 2.4 23.8 1.3 0.6 0.4 0.1 0.5
7.0 0.23 0.43 0.5 0.0 0.1 1.5 1.1 0.6 0.6 0.8 0.07 0.3
C-3
208.3 0.6 0.2 0.1 2.5 54.1 1.0 0.1 0.3 0.2 0.5
3.0 0.36
– 0.0 0.0
0.0 0.7 1.3 1.6 0.6 1.5 0.02 0.3
C-5
747.5 0.1 0.7 0.1 1.2 33.6 0.9 1.0 0.5 0.2 0.4
2.9
–
0.63 0.6 0.0 0.1 5.2 4.2 1.3 1.9 3.1 0.26 0.6
C-7
226.9 0.2 0.4 0.2 1.3 21.5 0.9 0.4 0.4 0.3 0.3
1.5
–
0.38 0.6 0.3 0.1 0.8 0.8 1.0 0.5 1.5 0.19 0.7
C-9
188.8 0.4 0.4 0.1 1.7 36.0 1.0 1.3 0.5 0.3 0.3
3.8 0.23 0.54 0.2 0.0 0.2 1.6 2.0 2.8 1.4 1.7 0.24 0.2
C-11
795.5 0.2 0.4 0.2 1.2 79.8 0.8 1.3 0.4 0.4 0.3
5.2
–
–
1.9 0.9 0.4 4.1 4.5 2.2 1.1 5.3 0.01 0.7
C-12
460.8 0.2 0.6 0.1 1.3 50.6 1.3 1.3 0.5 0.2 0.3
2.9 0.25
–
0.0 0.0 0.1 0.7 0.8 0.6 0.4 1.9 0.04 0.4
C-14
314.5 0.5 0.3 0.2 1.8 60.1 0.9 5.6 0.4 0.1 0.5 11.8 0.36 0.47 0.4 0.8 0.0 0.7 1.2 0.6 0.4 1.2 0.08 0.3
C-15
205.2 0.6 0.2 0.1 1.9 41.1 0.7 0.3 0.7 0.2 0.2
6.6 0.15 0.51 0.2 1.2 0.2 1.2 0.9 0.5 0.4 0.9 0.02 0.1
C-16 3132.8 0.1 0.5 0.3 1.1 70.1 0.8 0.3 0.4 0.1 0.5
–
–
–
–
0.0 0.0 0.7 1.2 1.0 0.7 1.5 0.09 0.1
C-17
253.2 0.6 0.2 0.1 1.8 68.9 0.9 0.8 0.5 0.3 0.2
2.3 0.25 0.59 0.2 1.3 0.5 4.4 3.2 1.3 1.3 1.9 0.03 0.1
C-20
469.8 0.3 0.3 0.3 1.4 84.3 1.0
–
–
–
–
–
–
–
–
–
–
–
–
8.7
–
–
–
–
C-21
71.5 0.3 0.4 0.2 1.2 12.2 0.9 0.4 0.4 0.2 0.4
7.4 0.80 0.65 0.8 0.8 0.0 0.0 0.0 0.6 0.4 0.0 0.00
–
C-26
368.2 0.5 0.3 0.1 1.4 40.2 0.6 0.4 0.4 0.2 0.4
3.8 0.50 0.57 1.2 1.2 0.0 0.3 0.5 0.5 1.0 0.0 0.00
–
C-28
42.2 0.5 0.2 0.1 2.1 13.2 0.7 0.0 0.4 0.2 0.4
2.4 0.50 0.63 0.2 0.2 0.0 0.1 0.1 0.2 0.2 0.0 0.00
–
C-22
27.5 0.6 0.2 0.1 2.2
8.0 0.8 0.4 0.5 0.2 0.4
0.8 0.34 0.66 0.2 0.2 0.0 0.1 0.1 0.1 0.4 0.0 0.00
–
C-31
155.2 0.4 0.2 0.2 2.0 36.1 0.7 0.3 0.2 0.2 0.6
2.4 0.54 0.65 0.2 0.2 0.1 0.7 0.8 0.6 1.7 0.0 0.00
–
C-35
86.3 0.4 0.3 0.2 1.7 11.9 0.5 0.6 0.4 0.2 0.4
1.8 0.66 0.66 0.0 0.0 0.0 0.2 0.6 0.1 4.0 0.0 0.00
–
A-3
164.1 0.1 0.4 0.4 2.0
2.8 0.6 0.4 0.4 0.2 0.4
1.5 0.57 0.57 0.2 0.2 0.2 0.0 0.0 0.1 0.1 0.0 0.01 0.2
A-7
163.8 0.0 0.4 0.4 2.2 1.3 0.6 0.1 0.4 0.2 0.4
2.0 0.36 0.41 0.1 0.1 0.2 0.0 0.0 0.1 0.2 0.0 0.01 0.2
A-11
154.5 0.0 0.4 0.4 1.7 0.9 0.7 0.2 0.4 0.2 0.4
2.7 0.54 0.51 1.3 1.3 0.2 0.0 0.6 1.0 4.7 0.0 0.07 0.1
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represent a substantial factor for the low CPI values, ob-
served in the studied samples.
Isoprenoids
In the studied samples, the isoprenoids are represented by
a series of compounds in the C
14—20
range (Table 2). Among
them, pristane and phytane are the most important, because
of their ubiquity in sediments and oils of different maturity
(Brooks et al. 1969). The relative proportions of isoprenoids
depend on the Eh setting of the environment, since anoxic
conditions favour the formation of phytane and more oxic
conditions favour the formation of pristane (e.g. Volkman &
Maxwell 1986). Hence, the pristane/phytane (Pr/Ph) ratio
can be used to evaluate the Eh potential of the depositional
environment (Didyk et al. 1978).
However, because pristane is formed during maturation of
the organic matter, the Pr/Ph ratio is also influenced by ther-
mal maturity (Goossens et al. 1984; Volkman & Maxwell
1986; Hughes et al. 1995; Koopmans et al. 1999). Moreover,
pristane may be formed from the isoprenoidal side-chain of to-
copherols (Goossens et al. 1984; ten Haven et al. 1987), phy-
toplankton and bacteria (Han et al. 1968; Han & Calvin 1969;
Volkman 1988), and phytane may be formed from bacterial
lipids (e.g. Volkman & Maxwell 1986; Volkman 1988).
Minor contributions from additional sources to both pris-
tane and phytane cannot be completely discarded. However,
since the low maturity of the rocks suppresses a significant
contribution to pristane concentrations due to thermal matu-
rity, the Pr/Ph ratio is considered an indicator of the oxic/
dysoxic depositional conditions. Furthermore, the isotopic
ratios of both pristane and phytane do not differ significantly
(Table 3), which might be an indication for their common
origin from chlorophyll-a. The Pr/Ph ratio is 1.3 for samples
C-12 and C-1 from the middle and upper parts of unit III
(Table 2, Fig. 4) indicating dysoxic conditions. The Pr/Ph of
all remaining samples ranges between 0.5 and 1.0 (Table 2),
Sample
A-7 C-1 C-5 C-7 C-11 C-14 C-16 C-21 C-22 C-26 C-35
n-C
15
–28.3 –28.2 –28.7 –29.1 –29.3
n-C
16
–28.6
–28.3
–28.8
–29.4
–29.1
–29.5
–29.0
–29.5
–28.6
n-C
17
–28.5 –28.7 –28.7 –29.5 –29.4 –29.9 –29.6 –29.4 –29.1 –29.1
Pristane
–30.1 –29.8 –29.8 –30.2 –30.1 –30.4 –29.9 –30.2 –30.4 –29.9
n-C
18
–29.0 –28.7 –28.7 –29.5 –29.3 –29.4 –29.1 –29.3 –28.5 –29.4
Phytane
–29.9 –29.8 –30.1 –30.7 –30.5 –30.2 –30.1 –30.2 –30.1 –30.2
n-C
19
–28.5
–28.6
–28.5
–28.4
–29.0
–28.7
–28.8
–28.8
–28.7
–29.2
n-C
20
–28.1 –28.3 –28.7 –28.5 –28.0 –28.3
–29.2 –27.9 –29.0
n-C
21
–27.9 –28.2 –28.1 –28.8 –27.7
–28.6 –28.5
n-C
22
–28.3
–28.1 –27.7 –27.2 –28.1 –27.4
–27.6 –28.0
n-C
23
–27.5
–28.3 –28.1 –27.0 –28.3 –27.6
–28.5 –27.9
n-C
24
–28.0
–27.5
–26.9
–26.8
–27.8
–26.9
–27.8
–28.1
–27.7
n-C
25
–27.7 –28.6 –28.0 –27.2 –26.6 –28.1 –27.0 –28.6 –28.8 –28.7 –28.1
n-C
26
–27.7 –28.7 –27.8 –27.4 –26.5 –28.4 –26.9 –28.2 –27.9 –28.0 –27.8
n-C
27
–28.1 –28.1 –28.6 –27.6 –27.0 –29.2 –27.1 –28.8 –29.2 –28.8 –28.8
n-C
28
–28.3 –27.6 –29.1 –28.2 –26.7 –28.7 –27.0 –28.6 –28.0 –28.4 –27.9
n-C
29
–28.8
–28.9
–28.6
–28.1
–27.5
–29.1
–27.1
–28.9
–28.9
–29.3
–28.9
n-C
30
–29.5 –28.4 –28.5 –27.8 –27.7 –29.1 –26.9 –28.7 –28.5 –28.3 –28.1
n-C
31
–29.7 –28.7 –28.5 –28.4 –28.2 –29.3 –26.9 –29.1 –29.4 –29.2 –28.9
n-C
32
–29.1
–26.4 –28.5 –27.8 –28.2 –28.5
n-C
33
–29.2 –27.2
–27.6
–27.6 –27.8
Table 3: Compound-specific carbon isotopic composition of selected samples (
δ
13
C, ‰; PDB).
which argues for deposition of organic matter in a strongly
oxygen depleted environment.
Steroids and hopanoids
All the studied sediments are characterized by the occur-
rence of C
27
—C
29
regular steranes in very low concentrations.
For the most samples, the steroid contents vary between 0.1
and 0.6 µg/g TOC (Table 2), although higher concentrations
(0.8—1.3 µg/g TOC) were also found, mostly in the middle
and upper parts of the core samples from unit III. Only sample
C-14 is characterized by raised steroid contents (up to 5.6 µg/g
TOC; Table 2). Interestingly, diasteranes or diasterenes were
not detected, despite the high amounts of clay in the samples.
Furthermore, the aromatic fraction is characterized by com-
plete absence of aromatic steroids indicating the low maturity
of the organic matter (Mackenzie et al. 1981).
In all samples, comparable steroid distribution patterns,
composed of either nearly equal amounts of C
27
and C
29
steranes, or a slightly predominating C
27
compounds, were de-
tected (Table 2, Fig. 8). For most samples, the C
28
steranes
are present in very low amounts (10—20 %; Table 2). Slightly
increased C
28
concentrations (up to 40 %) exist only within
the core samples from unit III. The steranes show very low
20S/(20S + 20R) ratios of the
ααα isomers (Fig. 8). In addi-
tion to the regular steranes, a series of C
28
—C
30
4-methylster-
anes in almost equal amounts were detected in sample C-14.
Steranes originate from sterols present in living organisms
(Mackenzie et al. 1982; Waples & Machihara 1991; Meyers
1997; Volkman 2003, 2005). The main sources of C
29
sterols
are photosynthesizing organisms, including terrestrial plants,
while C
27
sterols are more characteristic for marine phy-
toplankton (Brassell & Eglinton 1981; Volkman 1986;
Barrett et al. 1995; Volkman et al. 1998). However, numer-
ous results from biomarker studies indicate that phytoplank-
ton and microalgae also produce high proportions of C
29
sterols (Volkman et al. 1998; Volkman 1999, 2003). The
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Fig. 8. Typical mass chromatogram (m/z 217 + 231) of the steroids and their methyl substituted derivatives.
most probable source of C
28
steranes are marine microalgae,
as suggested by the presence of significant amounts of C
28
sterols in marine diatoms (Kates et al. 1977; Barrett et al.
1995; Volkman et al. 1998; Volkman 2003). Methyl steroids
are also related to marine and lacustrine microalgal precursors
(Volkman et al. 1990, 1998). A specific class of C
30
4-me-
thyl steranes with dinosterol structure is a biomarker for dino-
flagellates (Robinson et al. 1984; Mansour et al. 1999).
Considering these facts, the steranes distribution patterns ar-
gue for mixed organic matter, composed predominantly of
marine phytoplankton, but with significant contributions from
terrestrial plants. Enhanced contributions of C
29
steranes are
observed in few core samples from unit III (e.g. C-1, C-3,
C-14; Table 2), as well as in sample C-31 from unit IIa,
(Table 2). None of these samples shows increased concentra-
tion of long-chain n-alkanes. Therefore, the slight predomi-
nance of C
29
steranes in these samples might reflect a change
in the phytoplankton communities. It is noticeable that in con-
trast to n-alkanes distribution, the steranes distributions are
similar in outcrop and core samples from unit III. Therefore,
significant compositional changes in the short-chain hydrocar-
bons, possibly due to weathering, can be assumed.
Hopane concentrations range from 1.5 to 11.8 µg/g TOC
(Table 2, Fig. 4). Two set of samples can be separated based
on the hopane composition. The first set comprises the core
samples from unit III, in which hopanes are represented by
17
α,21β(H)-, 17β,21α(H), and 17β,21β(H) compounds with
27—32 carbon atoms (Fig. 9a). C
28
hopanes are missing. An
overall positive correlation in these samples exists between
the hopane and sterane concentrations (r = 0.76), suggesting a
proportional increase of bacterial activity together with the
increase of organic matter input (see also Fig. 4). The second
set comprises samples from subunit IIa and the outcrop
samples, in which hopanes are represented by 17
α,21β(H)-,
17
β,21α(H) and 17β,21β(H) compounds with 27—35 carbon
atoms, with the C
28
hopane absent (Fig. 9b). For subunit IIa
the vertical distribution of the hopanoids shows a marked
upward increase (Fig. 4). However, no correlation exists be-
tween the hopane and sterane concentrations, suggesting that
the increase of bacterial activity is probably related to a shift
to a more oxygen-rich environment, as recent studies indi-
cated aerobic bacteria as the main source of hopanes (Talbot
et al. 2008; Rezanka et al. 2010).
For both sets the hopane distribution is characterized by a
marked predominance of hopanoids in the 17
α(H),21β(H)
configuration (Fig. 9 – Ourisson et al. 1979). Dominant in all
samples are 17
α(H)-C
29
and 17
α(H)-C
30
hopanes (Fig. 9), ac-
companied by 17
β,21α(H)—C
30
moretane and C
27
hopanes.
The core samples from unit III are characterized by low
Ts/(Ts+Tm) ratios (0.2—0.4; Table 2). This ratio and appreci-
able amounts of hopanes with 17
β,21β(H) configuration
(Fig. 9a) argue for a low maturity of the organic matter. In con-
trast, Ts/(Ts + Tm) ratio is significantly higher (0.4—0.8;
Table 2) for subunit IIa samples and the outcrop samples, in-
dicating enhanced diagenetic changes. Furthermore, the ratio
of 22S/(22S + 22R) C
31
-hopanes shows generally very high
values (0.38—0.66), which are typical for marginal mature
organic matter. However, both ratios are known to be influ-
enced by facies variations (Waples & Machihara 1991; Peters
et al. 2005).
The most probable biological precursors of hopanoid
biomarkers are bacteriohopanepolyol derivatives, and to a
lesser extent 3-desoxyhopanes (Ourisson et al. 1979; Rohmer
et al. 1992), identified in the membrane of aerobic bacteria
such as cyanobacteria, and heterotrophic and methano-
trophic bacteria (e.g. Gibson et al. 2008; Talbot et al. 2008;
Rezanka et al. 2010).
The extended hopanes with 31 to 35 carbon atoms are rep-
resented in relatively low amounts (data not shown) (Fig. 9).
According to Van Dorselaer et al. (1975), the formation of
17
α,21β(H)-homohopane (22R) implies complex reactions
in acidic environments under oxic conditions. However, a
direct bacterial input to the organic matter should also be
considered, as Thiel et al. (2003) has proved the presence of
homohopanoic acids with
αβ configuration in living micro-
bial mats.
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Hop-17(21)-ene was detected in small amounts ( < 1.9 µg/g
TOC; Table 2) in almost all samples. Its biological precursor
has not yet been established (Bottari et al. 1972; Ourisson et
al. 1979; Brassell et al. 1980; Volkman et al. 1986; Wakeham
et al. 1980b; Wolff et al. 1992; Sabel et al. 2005).
Other terpenoids with non-hopanoid skeleton
Terpenoids are widespread in the geosphere (Thomas
1969) as part of the tissues of higher plants. Among them,
Fig. 9. Typical mass chromatograms (m/z 191) of the hopanoid hydrocarbons.
di-and tri-terpenoids are valuable biomarkers for determin-
ing the type of precursor vegetation (Simoneit 1977, 1986,
1999). In most of the studied samples very low amounts
(<1.3 µg/g TOC; Table 2) of diterpenoids were detected.
They are represented by hydrocarbons with phyllocladane
and pimarane type structure. The individual compounds
identified are
α-phyllocladane, occurring as a major compo-
nent, whereas the samples from subunit IIa and the outcrop
samples also contain trace amounts of
β-phyllocladane and
pimarane. Phyllocladanes are biomarkers for gymnosperms
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Fig. 10. a – Typical gas chromatogram of the aromatic fraction: MN – methyl naphthalenes, DMN – dimethyl naphthalenes, TMN – tri-
methyl naphthalenes, Ph – phenanthrene, MPh – methyl phenanthrenes; b – Gas chromatogram of the aryl isoprenoids (m/z 133) and chro-
mans (m/z 400 + 414): ar-i-C
14 ÷ 19
trimethyl (2,3,6)-alkylbenzol, Di-MTTC – dimethylated 2-methyl-2-(4’,8’,12’-trimethyltridecyl)chroman;
Tri—MTTC – trimethylated 2-methyl-2-(4’,8’,12’-trimethyltridecyl)chroman.
(e.g. Podocarpaceae, Taxodiaceae, Araucariaceae and
Cupressaceae – Noble et al. 1985; Sukh Dev 1989; ten Haven
et al. 1992; Otto & Wilde 2001). Triterpenoids with oleanane,
lupane and ursane type skeleton structure and their aromatic
derivatives, derived from angiosperm plants (Philp 1985;
Simoneit 1986), were not detected in the studied samples.
Aromatic hydrocarbons
The composition of the aromatic fraction in all the studied
samples is relative uniform and comprises methyl-, dim-
ethyl- and trimethyl-naphthalenes, phenanthrene and its me-
thyl derivatives, as well as low amounts of polyaromatic
hydrocarbons (PAHs), represented by fluoranthrene, pyrene,
benzo[a]pyrene and chrysene (Table 2, Fig. 10a). PAHs may
form due to diagenetic alteration of natural biolipids, but
most authors accept an origin by wildfires (e.g. LaFlamme &
Hites 1979; Wakeham et al. 1980a,b; Venkatesan & Dahl
1989; Killops & Massoud 1992; Yunker 2002, 2003). Con-
sidering this, we speculate that the detected PAHs are of ter-
restrial origin and were transported into the basin together
with charcoal particles.
The aromatic hydrocarbon composition is further charac-
terized by the occurrence of aryl isoprenoids in the range
C
13
—C
21
with a 2,3,6-trimethyl substitution pattern for the
aromatic ring and a tail-to-tail isoprenoid chain (Fig. 10b).
They are present in low amounts in the core samples from
unit III (Table 2). The aryl isoprenoids are derived from
isorenieratene, which is known to be synthesized by photo-
synthetic green sulphur bacteria. These organisms are pho-
totrophic anaerobes and require both light and H
2
S for growth
(Summons 1993; Pfennig 1997). Therefore, aryl isoprenoids
are widely used as a biomarker for green sulphur bacteria
and photic zone anoxia (e.g. Summons & Powell 1987;
Sinninghe Damsté et al. 2001). However, Koopmans et al.
(1996) found out that aryl isoprenoids with a 2,3,6-trimethyl
substitution pattern can also form due to diagenetic transfor-
mation of the more ubiquitous carotenoid
β-carotene, and,
therefore, have only limited applicability as a biomarker. In
the present case, isorenieratene itself has not been identified
in the samples.
The aromatic fraction of the samples from unit III is fur-
ther characterized by very low amounts of di- and trimethyl-
ated 2-methyl-2-trimethyltridecylchromans (MTTC; Table 2,
Fig. 10b). Among them, tri-MTTCs predominate (di-/tri-
MTTCs ratios: 0.1—0.4; Table 2). There are, however, samples
(e.g. C-5, C-7, C-11), which also contain appreciable amounts
of di-MTTCs (di-/tri-MTTCs ratios: 0.6—0.7).
The origin of the methyl substituted MTTCs is still un-
known (e.g. Li et al. 1995). Sinninghe Damsté et al. (1987,
1993) suggest that MTTCs form in the upper parts of the water
column, either from photosynthetic or non-photosynthetic or-
ganisms. On the contrary, Barakat & Rullkötter (1997) sug-
gested that chromans are a result of cyclization of alkylated
phenols. Despite this limitation, methyl-substituted chromans
are widely used as a paleosalinity indicators (e.g. Schwark &
Püttmann 1990; Sachsenhofer et al. 2009). Sinninghe Damsté
et al. (1987, 1993) indicate that formation and preservation of
mono-, di- and trimethyl substituted chromans require marine
environments with normal to enhanced salinity and stratifica-
tion of the water column. Furthermore, the authors observed
increasing di-/tri-MTTC ratios with increasing salinity. Con-
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sidering this, fully marine conditions are suggested during the
deposition of unit III, perhaps with a salinity stratified water
column. This suggestion is supported by the lamination of the
clays, as well as by the overall positive correlation between
the concentrations of MTTC and sulphur (r = 0.51) as well as
MTTC and aryl isoprenoids (r = 0.68).
Conclusions
The Middle to Upper Miocene succession in the Varna-
Balchik Depression, located in the south-eastern part of the
Moesian Platform, is up to 300 m thick and is represented by
sandy, clayey and carbonate rocks. Based on lithology and
resistivity log response, the succession is subdivided from
base to top into five units.
Sedimentation of fine-grained siliciclastic material pre-
vailed during deposition of the lower parts of units I and II
(subunits Ia and IIa, respectively), whereas their upper parts
(subunits Ib, IIb) are composed of biomicritic limestone.
Based on high diatom contents, subunit IIa is considered co-
eval with the lower part of the Euxinograd Formation.
Unit III represents the upper part of the Euxinograd Forma-
tion. It is composed of laminated clays with bioclastic layers
and significant amounts of biogenic silica, which are mainly
derived from sponge spicules in core samples and from dia-
tom frustules in outcrop samples. Units IV and V are repre-
sented predominantly by carbonate rocks and are correlated
with the Upper Miocene Topola and Karvuna Formations.
Whereas TOC contents in subunit Ia are negligible
(<0.2 wt. %), TOC contents in subunit IIa and unit III
(Euxinograd Fm) are generally between 1 and 2 wt. %, but
can reach 4 wt. % in unit III. Sulphur contents are typically
low ( < 0.5 %) and exceed 1.0 % only in samples from
unit III. Low sulphur contents may be due to deposition in
environments with reduced salinity. Normal marine condi-
tions are suggested for unit III.
The biomarker composition is typical for mixed marine and
terrestrial organic matter, and shows no significant changes
in subunit IIa and unit III. The molecular composition and
biomarker ratios support the presence of immature organic mat-
ter, deposited in dysoxic to anoxic environments. Kerogen is
mainly type II in subunit IIa (average HI = 324 mg HC/g TOC)
and type III for unit III (average HI ~ 200 mg HC/g TOC).
Considering the classification scheme of Peters (1986),
TOC and Rock Eval data show that subunit IIa holds a fair to
good hydrocarbon potential for oil, whereas the upper 5 m of
unit III holds a good to fair potential with the possibility to
generate gas and minor oil. Both units are immature in on-
shore areas, but thickness and maturity may increase towards
the east in offshore areas.
Acknowledgments: Financial support from OMV, awarded
to AZ, is greatly appreciated. In addition, the authors would
like to express their gratitude to E. Kozhukharov, OMV
Bulgaria, for his technical assistance. The manuscript also
benefited from the valuable suggestions made by Dr. P.
Kosakowski, Dr. M. Stefanova, Dr. E. Koleva-Rekalova and
an anonymous reviewer.
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