Research paper
Characterization of the source rocks of a paleo-petroleum system
(Cameros Basin) based on organic matter petrology and geochemical
analyses
Silvia Omodeo-Sal
e
a, *
, Isabel Su
arez-Ruiz
b
, Jos
e Arribas
a
, Ram
on Mas
c
, Luis Martínez
d
,
Maria Josefa Herrero
a
a
Departamento de Petrología y Geoquímica, UCM, IGEO (UCM-CSIC), Madrid, Spain
b
Instituto Nacional del Carb on, INCAR-CSIC, Oviedo, Spain
c
Departamento de Estratigrafía, UCM, IGEO (UCM-CSIC), Madrid, Spain
d
EOST, Universit e de Strasbourg, Strasbourg, France
article info
Article history:
Received 29 January 2015
Received in revised form
4 January 2016
Accepted 4 January 2016
Available online 5 January 2016
Keywords:
Source rocks
Cameros Basin
Hydrothermalism
Paleo-petroleum system
Organic petrography
abstract
The Cameros Basin is a paleo-petroleum system formed in the north-eastern Iberian Peninsula. The basin
formed during the Mesozoic Iberian Rift and was later inverted during the Alpine orogeny. Hydrothermal
events took place during the post-extensional and inversion stages, producing an important impact on
the thermal history of the basin. In order to determine the source rock of the petroleum system of the
basin, organic matter characteristics, the petroleum generation potential and the maturity of the basin
infill are determined by means of petrology and geochemical analyses.
Several organic rich units of the stratigraphic record of the basin are potential source rocks for hy-
drocarbons generation, although their characteristics differ depending on their location. Organic matter
content in the northern sector is scarce and limited to vitrinite, inertinite and solid bitumen particles. The
residual total organic carbon (TOC < 1%), the low hydrocarbon potential (S2 < 0.3 mg HC/g rock,
HI < 50 mg HC/g TOC), the mature to overmature thermal stages (%Ro from 1.7 to 4.6) and the presence of
solid bitumen particles indicate that hydrocarbons have been already generated by these rocks. In
contrast, the southern sector of the basin is characterized by abundant organic matter remnants (TOC
from 2 to 17%) and immature to early oil-window thermal conditions (0.38e0.75%Ro), indicating a high
hydrocarbonpotential for these rocks (S2 from 11 to 123 mg HC/g and HI values from 23 to 715 mg HC/g
TOC).
The different evolution of the source rocks in the basin is the result of the combination of differential
subsidence rates, which determine different thermal histories and of the circulation of hydrothermal
fluids in the northern-central sector during the evolution of the basin.
© 2016 Elsevier Ltd. All rights reserved.
1. Introduction
Source-rock characterization is an important risk-reduction tool
that is essential to ensure an effective search in oil and gas pro-
specting, especially in the case of basins with complex thermal
evolutions and those affected by hydrothermalism (Tissot and
Welte, 1984; Magoon and Dow, 1994). Source rock characteriza-
tion includes the type and amount of organic matter contained in
the rocks and their hydrocarbon generation potential. In the case of
mature-to-overmature deposits, these data can be difficult to
obtain.
This paper presents an interesting case-study that is not
commonly reported in the literature: a paleo-petroleum system
(the Cameros Basin petroleum system) where the original source
rocks are currently in an overmature thermal stage. For this pur-
pose, the petrographic and geochemical “signature” of a source
rock that has already completely generated and expelled hydro-
carbons is reconstructed. The knowledge obtained could provide
the key to determining whether the exploitation of a petroleum
system is feasible.
* Corresponding author. Current address: Direction G eosciences, IFPEN, Rueil
Malmaison, France.
E-mail address: silvia.omodeo@geo.ucm.es (S. Omodeo-Sal e).
Contents lists available at ScienceDirect
Marine and Petroleum Geology
journal homepage: www.elsevier.com/locate/marpetgeo
http://dx.doi.org/10.1016/j.marpetgeo.2016.01.002
0264-8172/© 2016 Elsevier Ltd. All rights reserved.
Marine and Petroleum Geology 71 (2016) 271e287