Elsevier

Earth-Science Reviews

Volume 135, August 2014, Pages 122-140
Earth-Science Reviews

Remote sensing based approach for mapping of CO2 sequestered regions in Samail ophiolite massifs of the Sultanate of Oman

https://doi.org/10.1016/j.earscirev.2014.04.004Get rights and content

Abstract

Documentation of chemical weathering and CO2 sequestration in the Samail ophiolite massifs of the Sultanate of Oman represents an important case study for Geological Carbon Capture and Storage System (GCCSS). The present research study demonstrates the capability of remote sensing technique for mapping of weathered zones and potential CO2 sequestration area abundances at different scales within peridotites in the northern mountain region of the Samail ophiolite massifs. The carbonate mineral index (CI) applied with other mineral indices to the TIR wavelength region of Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) TIR spectral bands 13 and 14 mapped CO2 sequestered minerals along the structural- and wadi-controlled CO2 flowing regions. Peridotites, the source rocks of CO2 sequestration in the study area, were mapped using an ASTER 8, 3 and 1 band combinations. The decorrelated Landsat TM image discriminated the rock types associated with peridotites of ophiolite sequences and delineated the region of weathered and altered serpentinized peridotites in the zone of CO2 sequestration. CO2 sequestration mapping was carried out using Landsat TM satellite data that span 20 years (1986, 1998, 2000, 2003 and 2006) to assess the present status of CO2 sequestration in this region. The image interpretations are verified with existing geological maps and through field and laboratory studies.

The spectral measurements of carbonate minerals at 1300 to 2500 nm with the spectral resolution of ~ 7 nm using a PIMA SP infrared spectrometer in the field and laboratory show the presence of hydroxyl-bearing minerals and carbonates that have spectral absorption features around 1.4 μm, 1.9 μm and 2.35 μm. The strong absorptions around 2.35 μm are mainly due to Csingle bondO bonds in carbonate minerals such as calcite (CaCO3), dolomite (CaMg(CO3)2), magnesite (MgCO3), aragonite (CaCO3) and siderite (FeCO3), which form 15 to 57%, 12 to 53%, 9 to 38%, 11 to 21% and 3 to 8% respectively in the samples. The absorptions around 1.4 μm and 1.9 μm are caused by hydration effects of hydroxyl minerals including antigorite and montmorillonite present at 10 to 21% and 37 to 81% respectively in the samples. The alterations of serpentinite are evidenced by the presence of antigorite and lizardite minerals. X-ray powder diffraction analyses further confirms the occurrence of CO2 sequestered major carbonate minerals such as aragonite, calcite and dolomite in the samples. The study demonstrates that the ASTER and Landsat TM satellite multispectral sensors are useful to detect the carbonate minerals, to delineate the peridotites and to discriminate the areal abundance of potential CO2 sequestration. This technique is a useful tool to map and monitor the region of CO2 sequestration in well exposed arid and semi-arid regions and to analyze and understand this aspect of the world geological carbon capture and storage system.

Introduction

The continued increase in CO2 emissions and the related changes in the concentration of the greenhouse gas in the atmosphere and ocean is a global issue, and much consideration is being given to how CO2 can be removed from the atmosphere. Rutt Bridges (2011) stated that the Carbon Capture and Storage (CCS) system faces storage challenges in site selection, CO2 transportation costs, pipeline and site permits, and uncertainties in monitoring CO2 sequestration. But, in Earth history, nature is performing silicate weathering at the earth's surface which is estimated to remove CO2 from the atmosphere equivalent to approximately 150 Mt C per year (Gaillardet et al., 1999), over an order of magnitude smaller than the 5.5 Gt C emitted by fossil fuel combustion (IPCC, 2007). If weathering rates can be increased over large areas even within the range observed today, the acceleration of weathering processes could play a meaningful role in an integrated strategy for atmospheric removal of CO2.

CO2 is a major weathering agent in silicate rocks such as peridotites by the conversion of nearly all of the CaO and part of the MgO to carbonate minerals. Over the past several years many papers have been published that discuss the advantages of CO2 injection into mafic and ultramafic rock formations, including deep-sea basalts (Goldberg et al., 2008, Oelkers et al., 2008) and peridotites (Kelemen and Matter, 2008, Andreani et al., 2009, Matter and Kelemen, 2009, Kelemen et al., 2011). The two recent workshops report on geological carbon capture and storage in mafic and ultramafic rocks (Godard et al., 2011), and the scientific drilling in the Samail ophiolite of Oman (Kelemen et al., 2013) emphasizes the importance of research studies on the geological carbon capture and storage system and the need of scientific drilling in the Samail ophiolite of Oman. Thus, the study of CO2 sequestration in ultramafic peridotites of ophiolite regions is of great worldwide importance. CO2 sequestration due to weathering in peridotites in ophiolite sequences of the Samail massifs of the Sultanate of Oman is a major and typical example and needs to be studied in more detail. Due to the 1169 km2 extent of the Samail ophiolite massifs and extremely rugged topography with elevations between 0 and 2500 m, exhaustive sampling and detailed mapping are impossible to assess the potential of CO2 sequestration in this region. Remote sensing is able to provide more continuous mineralogical and lithological mapping in the almost continuous barren rock exposures in an arid climate like the region of the Samail massifs. The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) and Landsat sensors cover the wavelengths of absorption regions of peridotites and CO2 bearing minerals. Several works on mapping of ophiolite sequences using remote sensing have been carried out (Abrams et al., 1983, Abrams and Hook, 1995, Sabins, 1997, Abdeen et al., 2001, Kusky and Ramadan, 2002, Rowan and Mars, 2003, Rowan et al., 2003, Combe et al., 2006, Mars and Rowan, 2006, Gad and Kusky, 2007, Rajendran et al., 2012, Rajendran et al., 2013, Rajendran and Nasir, 2013, Rajendran and Nasir, 2014), but few studies have focused on the application of remote sensing to mapping of CO2 sequestration worldwide. This study suggests that the detection of CO2 sequestered carbonate minerals and mapping of peridotite (the source rock) occurrences are of great importance in the GCCSS and global monitoring of CO2 which will increase the knowledge among scientists to improve and create a sustainable GCCSS in the future. Thus, the present study is undertaken to demonstrate the capability of remote sensing techniques to detect the occurrences of CO2 sequestered carbonate minerals, to discriminate the peridotites (the source rock of CO2 sequestration) and to map the region of CO2 sequestration ongoing in the ophiolite sequences of northern Samail massifs of the Sultanate of Oman (Fig. 1) as a part of research work on the GCCSS.

Section snippets

CO2 sequestration rationale

In brief, the removal of carbon dioxide from the atmosphere and ocean by the natural weathering processes of silicate rocks like peridotites is one of the long-term mechanisms of balancing the CO2 concentration in the atmosphere. Peridotite is composed of > 40% of the mineral olivine (Le Maitre, 1989). The typical residual mantle peridotite exposed on the seafloor and in ophiolites is composed of 70–85% of olivine, together with dunite composed of more than 90% olivine. During the weathering

Peridotites and associated geology of the Samail ophiolite massifs

The study region, part of the northern mountain region of the Samail ophiolite massifs (Fig. 1B) is located parallel to the east coast of the Gulf of Oman on the Arabian plate, and includes rocks formed during the Late Cretaceous (Glennie et al., 1973, Glennie et al., 1974, Searle and Malpas, 1980, Coleman, 1981, Boudier et al., 1985, Lippard et al., 1986). The Samail massifs represent a 600 km long by up to 150 km wide slab of oceanic crust and mantle emplaced due to the closure of the Tethyan

Spectral characteristics of peridotite minerals

The reflectance spectrum of a rock depends on the mineralogical composition of its surface, which is usually a mixture of the whole rock mineralogy and weathering minerals. The absorption bands in the visible and short wavelength infrared are from either electronic or vibrational processes in these minerals (Hunt and Salisbury, 1970). Comprehensive spectral absorption–compositional studies can provide important insights into the causes of spectral variations and quantitative data for use in the

Satellite data

The ASTER sensor onboard the Earth Observing System (EOS) TERRA platform is a multispectral imaging system, launched in December 1999, which travels in a near circular, sun-synchronous orbit with an inclination of approximately 98.2°, an altitude of 705 km and a repeat cycle of 16 days. It measures visible reflected radiation in three spectral bands (VNIR between 0.52 and 0.86 μm, with 15-m spatial resolution) and infrared reflected radiation in six spectral bands (SWIR between 1.6 and 2.43 μm,

Mapping of CO2 sequestered minerals

As described above, the five TIR spectral bands of the ASTER satellite data were processed using the mineral indices for mapping of CO2 sequestered minerals to the selected area in a large scale and the result in RGB color composite image (R: CI; G: QI; B: MI) is given in Fig. 3. The occurrences of CO2 sequestered minerals are well detected on the image due to a unique absorption of Csingle bondO bonding (near 11.4 μm for calcite and 11.2 μm for dolomite) in cyan color along the Wadis (drainages) and

Conclusions

The present study is carried out to map the areal abundance of CO2 sequestration in peridotite rocks in the northern mountain region of the Samail ophiolite massifs of the Sultanate of Oman using the capability of multi-spectral remote sensing data. The improved spatial and spectral resolutions in VNIR, SWIR and TIR bands of ASTER spectral regions detected the areal abundance of CO2 sequestered minerals in the study area. The developed ASTER 8, 3 and 1 visible and near infra-red spectral band

Acknowledgments

The authors are thankful to NASA Land Processes Distributed Active Archive Center User Services, USGS Earth Resources Observation and Science (EROS) Center (https://LPDAAC.usgs.gov) for providing the ASTER and Landsat data. The PIMA SP infrared spectrometer used in this study is supported by Sultan Qaboos University. The study is partially supported by the National Natural Science Foundation of China (Grants 91014002, and 40821061) and the Ministry of Education of China (B07039) to Prof.

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