Handbook on Sediment Quality
A Special Publication
Prepared by A Treatise on Sediment Quality Task Force of the Water Environment Federation
Raymond C. Whittemore, Chair
Alok Bhandari Edward R. Long Washington Braida G. Fred Lee Jennifer Byrnes Brower Drew McAvoy Jerome M. Diamond Allen J. Medine Robert M. Engler Robin Landeck Miller Mark W. Fitch George D. Nichol Upal Ghosh Tina Reese Cesar Gomez Joseph E. Rathbun Ferdinand Hellweger Tamara L. Sorell James E. Kilduff Paul Kevin Sibley Peter F. Landrum John R. Wolfe Eugene Joseph LeBoeuf
Under the Direction of the Water Quality and Ecology Subcommittee of the Technical Practice Committee
2002 Water Environment Federation 601 Wythe Street Alexandria, VA 22314-1994 USA http://www.wef.org IMPORTANT NOTICE The contents of this publication are not intended to be a standard of the Water Environment Federation (WEF) and are not intended for use as a reference in purchase specifications, contracts, regulations, statutes, or any other legal document. No reference made in this publication to any specific method, product, process, or service constitutes or implies an endorsement, recommendation, or warranty thereof by WEF. WEF makes no representation or warranty of any kind, whether expressed or implied, concerning the accuracy, product, or process discussed in this publication and assumes no liability. Anyone using this information assumes all liability arising from such use, including but not limited to infringement of any patent or patents.
Library of Congress Cataloging-in-Publication Data
Handbook on sediment quality / prepared by a Treatise on Sediment Quality Task Force of the Water Environment Federation under the direction of the Water Quality and Ecology Subcommittee of the Technical Practice Committee. p. cm.—(A special publication) Includes bibliographical references and index. ISBN 1-57278-201-3 (pbk.) 1. Sediments (Geology)—Analysis I. Water Environment Federation. Treatise on Sediment Quality Task Force. II. Water Environment Federation. Water Quality and Ecology Subcommittee. III. Special publication (Water Environment Federation) QE471.2 .H33 2002 628.1'61—dc21 2002011318
Copyright © 2002 by the Water Environment Federation All Rights Reserved.
Printed in the USA 2002 Water Environment Federation
Founded in 1928, the Water Environment Federation (WEF) is a not-for-profit technical and educational organization with members from varied disciplines who work toward the WEF vision of preservation and enhancement of the global water environment. The WEF network includes more than 100,000 water quality professionals from 77 Member Associations in 31 countries.
For information on membership, publications, and conferences, contact
Water Environment Federation 601 Wythe Street Alexandria, VA 22314-1994 USA 703-684-2400 http://www.wef.org
iii Special Publications of the Water Environment Federation
The WEF Technical Practice Committee (formerly the Committee on Sewage and Industrial Wastes Practice of the Federation of Sewage and Industrial Wastes Associations) was created by the Federation Board of Control on October 11, 1941. The primary function of the Committee is to originate and produce, through appropriate subcommittees, special publications dealing with technical aspects of the broad interests of the Federation. These publica- tions are intended to provide background information through a review of technical practices and detailed procedures that research and experience have shown to be functional and practical.
Water Environment Federation Technical Practice Committee Control Group
T. L. Krause, Chair G. T. Daigger, Vice-Chair G. Abbott B. G. Jones M. D. Nelson A. B. Pincince T. E. Sadick
iv Contents
Chapter Page 1. An Introduction to Sediments 1
2. Sorption of Organic Compounds by Soils and Sediments: Equilibrium and Rate Processes 7 Introduction 8 Sorption Mechanisms 10 Intermolecular Forces 12 Partitioning 12 Ion Exchange 12 Covalent Bonding 13 Modeling Contaminant-Phase Distribution Equilibria 14 Partitioning Theory 15 Estimation of Activity Coefficients 17 Flory–Huggins Theory 19
Correlations of Kd to Molecular Properties 21 Correlations with the Octanol–Water Partition Coefficient 22 Isotherm Models 24 The Generalized Langmuir Isotherm and Its Simplifications 26 Potential Theory 30 Combined Models 31 Materials and Methodologies for Collecting Sorption Data 34 Batch and Column Equilibration Techniques 34 Batch Equilibration Techniques 34 Fixed-Bed (Column) Reactor Techniques 37 Obtaining Representative Samples 38 Composition of the Solution Phase 39 Criteria for Achieving Equilibrium 40 Loss Mechanisms and Controls 41 Reactors and Reactor Components 43 Phase Separation 43 Desorption 44 Sorption Phenomena 45 Isotherm Linearity 45 Linear Partitioning to Isolated Mineral Surfaces 45 Linear Partitioning to Soils and Sediments 46 Nonlinear Sorption of Neutral Hydrophobic Organics 49 Nonlinear Sorption of Ionizable Organics 59 Competitive Effects 61 Competitive Adsorption Models 61 Ideal Adsorbed Solution Theory 62 Polanyi-Based Models 63
v Chapter Page Evidence for Sorbate Competition 64 Desorption Hysteresis and Reversibility 65 Effects of Particle Size 68 Effects of Organic Matter Composition and Structure 68 Chemical Characterization: Polarity and Aromaticity 68 Rubbery/Glassy Models 69 Microporosity 69 Crystallinity 70 Solids-Concentration Effect 72 Sorption Rate Processes 75 Local Equilibrium 76 Langmuir Kinetics 77 Empirical Rate Models 77 Mass-Transfer Controlled Kinetics 79 External Mass Transfer 79 Homogenous Solid-Phase (Surface) Diffusion 81 Pore and Combined Pore-Surface Diffusion 82 Diffusion in Macromolecules 83 Case I Transport 84 Case II Transport 84 Anomalous or Non-Fickian Transport 85 Macromolecular Diffusion Behavior in Natural Systems 86 Summary and Conclusions 86 References 87
3. Bioavailability in Sediments 99 Introduction 100 Current Research on Bioavailability in Sediments 102 Measuring Bioavailability 102 Alternative Extraction Methods 102 Membrane Analogs 103 Importance of Sediment Characteristics in Determining Bioavailability 104 Pore Water Concentrations Determine Bioavailability 104 Bioavailability of Sediment-Associated Contaminants 105 Remediation Using Bioavailability Reduction 106 Modeling 106 Field Studies 108 Bays 108 Lakes 109 Wetlands 109 Factors-Controlling Bioavailability 109 Acid-Volatile Sulfide 109 Organic Carbon 111
vi Chapter Page Processes Affecting Bioavailability in Sediments 112 Aging 112 Sorption 112 Seasonality 114 Bioturbation 114 Measuring Bioavailability 115 Acid-Volatile Sulfides 116 Equilibrium Partitioning 118 Toxicity Tests With Algae, Bacteria, or Representative Species 120 Current Regulatory Directions 121 Toxicity Calculations 122 References 123
4. Methods for Collecting, Storing, and Manipulating Sediments and Interstitial Water Samples for Chemical and Toxicological Analyses 139 Introduction 140 Potential Interferences and Artifacts in Sediment and Interstitial Water Collection, Handling, and Manipulation 141 Noncontaminant Factors 141 Changes in Bioavailability 142 Presence of Indigenous Organisms 143 Safety Concerns 143 Field Operation 144 Laboratory Operations 144 Special Considerations for Explosive Contaminated Sediments 144 Disposal of Sediments and Pore-Water Samples 144 Facilities, Equipment, and Supplies 144 Field Facilities 144 Laboratory Facilities 145 Equipment and Supplies 146 Equipment Cleaning and Decontamination 147 Procedures for Sediment and Interstitial Water Collection 148 Sediment Collection 148 Grab Samplers 150 Core Samplers 153 In Situ Interstitial Water Collection 158 Peeper Methods 160 Suction Methods 161 Retrieval of Interstitial Water Samples 161 Sample Transport and Storage 162 Sample Holding Times 163 Subsampling, Homogenizing, and Compositing Samples 164 General Information 164 Subsampling 165 Homogenization 168
vii Chapter Page Compositing 169 Sediment Sample Manipulations 170 Sieving 170 Recommended Sieves 171 Press Sieving 171 Wet Sieving 172 Alternatives to Sieving 172 Spiking Sediments 172 Preparation for Spiking 172 Spiking Methods 173 Verifying Homogeneity 173 Equilibration Times 174 Formulated Sediments and Organic Carbon Modification 175 Sediment Dilutions 176 Sediment Elutriates 176 Isolation of Interstitial Water 177 Centrifugation 178 Sediment Squeezing 179 Pressurized Devices 180 Quality Assurance and Quality Control 180 General Considerations 180 Quality Assurance and Quality Control Procedures for Sediment Collection and Manipulation 181 The Quality Assurance Project Plan 182 Data Quality Objectives 182 Project Organization 183 Standard Operating Procedures 183 Sediment Sample Documentation 183 Sample-Tracking Documentation 184 Recordkeeping 185 Quality Assurance Audits 185 Corrective Action (Management of Nonconformance Events) 185 Data Reporting 186 References 186
5. Testing for Toxicity and Bioaccumulation in Freshwater Sediments 199 Introduction 200 Selection of Test Protocols 201 Selection of Test Species 203 Assessing Species Sensitivity 205 Selecting Measurement Endpoints 208 Selection of Control Sediments 211 Selection of Sediment Phases for Use in Toxicity Testing 212 Introduction 212 Whole Sediments 212 Pore-Water Phase 215 viii Chapter Page Elutriate Phase 216 Suspended Phase 216 Comparative Toxicity of Whole Sediments, Elutriates, and Pore Water 218 Overview of Freshwater Species Used in Sediment-Toxicity Testing 219 Vascular Plants 219 Oligochaetes and Worms 221 Amphipods 221 Mayflies 222 Midges 222 Cladocerans 223 Fish 224 Amphibians 224 Miscellaneous Species 225 Methods to Assess Bioaccumulation in Freshwater Sediments 226 Invertebrate Bioaccumulation Tests 227 Fish Bioaccumulation Tests 232 Field Methods for Assessing Sediment Bioaccumulation 232 Field-Collected Samples 233 Transplantation and In Situ Exposures 234 Future Research Directions 235 Development of Bioassays and Endpoints 236 Issues Related to Exposure 237 In Situ Studies 237 Development of Sediment Quality Criteria and Bioassessment Approaches 238 Bioaccumulation and Risk Assessment 238 Concluding Remarks 239 References 239
6. Toxicity Tests of Marine and Estuarine Sediment Quality: Applications in Regional Assessments and Uses of the Data 259 Introduction and Background 260 Results from Surveys Performed Throughout North America 262 The Types of Toxicity Tests Commonly Used in Regional Monitoring 262 Spatial Gradients (or Patterns) in Toxicity 266 Incidence of Toxicity 279 Spatial (or Surficial) Extent of Toxicity 282 Predicting Toxicity with Numerical Sediment-Quality Guidelines 285 Ecological Relevance of Toxicity Tests 299 Conclusions and Outlook 303 References 307
ix Chapter Page 7. Empirical and Theoretical Shortcomings of Sediment- Quality Guidelines 317 Introduction 318 Co-occurrence Sediment-Quality Guidelines 318 Equilibrium Partitioning Sediment-Quality Guidelines 320 Empirical Test of Sediment-Quality Guidelines 320 Theoretical Limitations to Chemical Predictors 323 Conclusions 324 References 324
8. Sediment-Quality Modeling 327 Introduction 328 Model Framework 329 Basic Processes Affecting Sediment-Quality 329 Transport Processes 330 Water Column Transport 330 Settling 331 Resuspension 331 Sedimentation 331 Sediment–Water Diffusion 332 Mixing Within Bed Sediments 332 Reaction Processes 332 Sorption 332 Volatilization 333 Degradation–Decay 334 Advanced Model Features 334 Multiple Sorbent Classes 334 Water Column Solids 335 Non-Equilibrium Partitioning 336 Sediment Resuspension 336 Cohesive Sediments 337 Noncohesive Sediments 338 Behavior of Metals 338 Spatial Resolution 339 Commonly Used Model Frameworks 340 Hydrodynamic Models 341 UNET 342 DYNHYD5 342 RMA-2V 342 Princeton Ocean Model 343 Sediment-Transport Models 343 HEC-6 343 SED2D 344 SEDZL 344
x Chapter Page Chemical Fate and Transport Models 344 SMPTOX 344 HSCTM-2D 344 WASP5/IPX 344 EFDC 345 Model Calibration 345 Calibration Sequence 346 Short-Term Versus Long-Term Calibration 347 Alternate Observations 347 Calibration Sufficiency 348 Model Application 348 Remediation 348 Future Enviornmental Conditions 349 Natural Attenuation 350 Dredging 350 Capping 351 Case Study 351 Prevention of Sediment Contamination 353 Limitation and Proper Use 354 Bayou D’Inde Case Study 354 Outstanding Issues 357 Artifical Bed Mixing 357 Data Sufficiency to Validate Resuspension Rates 359 Bioturbation and Enhanced Sediment Diffusion 360 Model Representation of Active Management Scenarios 360 References 360
Index 367
xi
List of Tables
Table Page 2.1 The GL isotherm and its simplifications. 27 2.2 Studies finding linear partitioning to sediments and other sorbents. 47 2.3 Studies finding nonlinear partitioning to sediments and other sorbents. 52 2.4 Ideal adsorbed solution theory model formulation. 63 4.1 Recommended sampling containers, holding times, and storage conditions for common types of sediment analyses. 147 4.2 Typical sediment volume requirements for various analyses. 149 4.3 Advantages and limitations of commonly used grab samplers. 151 4.4 Advantages and limitations of commonly used core samplers. 154 4.5 Optimal interstitial water collection methods. 159 5.1 Common organisms used in toxicity testing. 202 5.2 Comparison of the relative sensitivities of several freshwater species used in bulk sediment toxicity testing. 207 5.3 Some advantages and limitations of using different sediment phases in toxicity testing. 213 5.4 Compilation of laboratory tests incorporating standard test invertebrates in assessments of bioaccumulation of organic and metal contaminants from freshwater sediments. 229 6.1 Sediment toxicity tests and other analyses selected for use in 35 large-scale environmental assessments. 263 6.2 Incidence of toxicity in amphipod survival tests performed in studies conducted by NOAA and EMAP in U.S. estuaries. Tests were performed with A. abdita. 280 6.3 Frequency distribution of results of six toxicity tests performed on marine sediments. 281 6.4 Percent incidence of sediment samples classified as toxic or highly toxic in six toxicity tests. 282 6.5 Spatial extent of toxicity in amphipod survival tests performed with solid-phase sediments from 27 U.S. bays and estuaries. 283 6.6 Spatial extent of toxicity in sea urchin fertilization tests performed with 100% sediment pore waters from 22 U.S. bays and estuaries. 285 6.7 Incidence of toxicity in either amphipod tests alone or any of the two to four tests performed among samples in which individual ERMs were exceeded. 288 6.8 Incidence of toxicity in either amphipod tests alone or any of the two to four tests performed among samples in which individual PELs were exceeded. 289
xiii Table Page 6.9 Percent incidence of highly toxic samples and average percent amphipod survival in marine sediment samples classified according to numerical sediment quality guidelines. 290 6.10 Relationships between incidence of degraded benthic populations and mean SQG quotients with data summarized for Carolinian, Virginian, and Louisianian provinces. 292 6.11 Macrobenthic trophic structure in estuarine sediments of the northern Gulf of Mexico in randomly selected samples versus those in which chemical concentrations were nearly equal to or greater than the ERL values. 293 6.12 Relationships between total numbers of macrobenthic species and mean SQG quotients in northern Puget Sound. 294 6.13 Percentages of field-collected samples that were correctly predicted to be toxic in amphipod tests in relation to predicted sum of PAH toxic units in samples in which PAHs were principal contaminants of concern and samples in which other chemicals were present. 294 6.14 Incidence of toxicity in amphipod survival tests in samples within four ranges in total PAH concentrations defined by consensus-based, sediment-effect concentrations. 295 6.15 Incidence of toxicity in amphipod tests in samples in which ERM or PEL values were exceeded for sums of low- molecular-weight (LMW) PAHs, high-molecular-weight (HMW) PAHs, or 13 PAHs. 296 6.16 Incidence of toxicity and average percent survival in amphipod tests within five ranges in total PCB concentrations defined by consensus SECs. 297 6.17 Percentages of samples that were toxic in amphipod survival tests when predicted to be either toxic or nontoxic with different sets of sediment quality guidelines for trace metals. 298 6.18 Toxicity thresholds for total DDT in sediments derived from field-collected samples. 299 6.19 Incidence of toxicity in amphipod tests and average percent survival within 10 ranges in mean SQG quotients. 300 6.20 Percentages of samples estimated with logistic regression models to be toxic in amphipod survival tests with chemical concentrations equivalent to several SQG concentrations. 300 7.1 The ERLs and ERMs from Long et al. 319 7.2 Sediment quality guidelines based on equilibrium partitioning of neutral organic compounds or acid-volatile sulfide. 321 7.3 Frequencies of 10-day amphipod toxicity in samples with chemical concentrations in excess of a SQG. 322
xiv List of Figures
Figure Page 2.1 Schematic depiction of sediment heterogeneity (containing mineral and organic surfaces) and sorption mechanisms (partitioning, electrostatic bonding, ion-exchange, and covalent bonding). 11 2.2 A comparison of several different isotherm models over a wide range of concentrations. 29 2.3 An example of a distributed reactivity isotherm. 32 2.4 An example of a dual-mode isotherm. 33 2.5 A comparison of predictions made using the dual-mode (or dual-reactive domain) model. 35 2.6 An example of how sorbent heterogeneity, as exemplified by several distinct Langmuir sites, can result in nonlinear, Freundlich-type sorption behavior. 51 2.7 Hypothesized sequence of sorption by exposed mineral surfaces (domain I), amorphous organic matter (domain II) and condensed organic matter (domain III). 54 2.8 The effect of co-solute sorption observed by Chiou and Kile. 66 2.9 Folded-chain model for crystallinity (after Rosen, 1993). 71 2.10 Hopfenberg–Frisch chart of anomalous transport phenomena (after Vieth, 1991, from Hopfenberg and Frisch, 1969). 84 3.1 The effect of fractional approach to equilibrium, f, on the relationship between the apparent partition coefficient (Kd) and the sorbent concentration (s). 107 2– 3.2 Typical profiles of sulfate (SO4 ), total sulfide [S(II)], and oxygen (O2) in the overlying water and pore water of aquatic sediments. 110 4.1 Alternatives for subsampling and compositing sediment grab samples. 166 4.2 Alternatives for sampling and compositing sediment core samples. 167 6.1 Distribution of toxicity in Charleston Harbor as determined with Microtox tests. 268 6.2 Distribution of toxicity in Charleston Harbor as determined with urchin fertilization tests. 269 6.3 Distribution of toxicity in Sabine Lake as determined with urchin fertilization tests. 270 6.4 Distribution of toxicity in Boston Harbor as determined with amphipod survival tests. 271 6.5 Distribution of toxicity in Pensacola Bay as determined with urchin fertilization tests. 272 6.6 Distribution of toxicity in central Biscayne Bay as determined with amphipod survival tests. 273
xv Figure Page 6.7 Distribution of toxicity in southern Biscayne Bay as determined with urchin fertilization tests and amphipod survival tests. 274 6.8 Distribution of toxicity in Port Gardner Bay of northern Puget Sound as determined with urchin fertilization tests. 275 6.9 Distribution of toxicity in central Puget Sound as determined in cytochrome P-450 RGS assays. 276 6.10 Distribution of toxicity in Newark Bay as determined with amphipod survival tests. 277 6.11 Distribution of toxicity in San Diego Bay as determined with amphipod survival tests. 278 6.12 Average abundance of benthic amphipods in sediment samples within eleven ranges in percent amphipod survival. 302 6.13 Generalized relationship between increasing chemical contamination of sediments and measures of adverse biological effects. 305 8.1 Schematic of major contaminated sediment model properties. 330 8.2 Model framework considering sulfide precipitation of metals. 340 8.3 Example of two dimensionality of predicted velocity for Hudson River. 341 8.4 Demonstration of types of model output generated for remediation assessment. 349 8.5 Hudson River site map. 352 8.6 Example of calibration plot for the Hudson River. 353 8.7 Typical model-predicted sediment concentration comparison for prevention analysis showing long-term insensitivity to time. 354 8.8 Bayou d’Inde site map. 355 8.9 Example of Bayou d’Inde model results of HCB in the water column and sediments (1 mile × 1.609 = km). 356 8.10 Model abstraction of actual vertical sediment concentration distribution into a series of idealized layers. 357 8.11 Model abstraction of sediment bed immediately after a resuspension event. 358 8.12 Predicted efficiency of dredging with different modeling assumptions. 361
xvi Preface
Dr. Ray C. Whittemore, NCASI
HISTORY. Sediments, or the sand, dirt, and land runoff litter that lie on the bottom of every waterbody, are part of the aquatic system’s ecology because of the habitat they provide for plants and animals and their role in bearing the legacy of historical effluent treatment management practices. Most impor- tantly, sediments provide shelter, food, and rearing grounds for bottom- dwelling organisms that are eaten by fish and larger animals in the traditional aquatic food web. Some fish species such as salmon, in fact, use gravel bottom substrates as a hatching medium. In recent years, attention to fish and shellfish consumption by humans and wildlife has been increasingly of public concern and gives rise to issues relating to bioaccumulation and biomagnifica- tions. Toxic compounds can bind to the organic carbon in fine sediment particles and gradually become integrated to the biomass of the sediment itself. The importance of sediments in the United States was first noted in the late 19th Century following public health concerns in cities along the Mississippi River. Although these early concerns were ultimately linked to bacterial contamination in raw untreated wastewater, they heightened scientific attention to this medium. Over the past few decades it has become widely understood that many different organic and inorganic chemicals have signifi- cantly contaminated the sediments of rivers, lakes, and estuaries in some locations. When these compounds are persistent, sediments contain a long- term record of past inputs to the aquatic system from atmospheric deposition to nonpoint and point sources. A number of processes, such as sorption and complexation, tend to immobilize this record and their aquatic effects, whereas others, such as bioturbation and other forms of sediment, scour, disturb, and disperse the record of inputs. Under certain conditions, contaminants can be released to overlying waters, either slowly by diffusion or current processes or in bulk during storm-induced wave actions. Thus, the sediments may become an important source of chemicals to surface water in which direct point source input, littoral, and atmospheric sources have been reduced or eliminated.
REGULATORY EVOLUTION. The study of the role of sediments in the fate and transport of contaminants is a relatively new phenomenon, although many would argue that the role of sediments as an ultimate sink of chemicals has long been known or, at a minimum, predicted. The regulation of sediment contamination is also an emerging process in the United States with the evolution of new regulatory policies and programs that began in the 1980s. Research and development of sediment-quality criteria (SQC) and sediment- quality guidelines methodologies and supporting toxicity test developments began in the late 1980s and results began to appear in the early 1990s. Widespread acceptance of any regulatory approach has not occurred and is
xvii hotly debated in some circles. Most significant of these is the apparent rift between the U.S. Army Corps of Engineers and the U.S. Environmental Protection Agency (U.S. EPA) over the significance of the terminology that includes “criteria”, which has legal connotations that would undermine historical U.S. Army Corps of Engineers mandates. Another relates to controversy surrounding the use of empirically derived sediment-quality measures (co-occurrence). Several significant technical and policy pieces, however, are still evolving within the U.S. EPA and serve as the regulatory justification of this book. States are being forced now to deal with contami- nated sediment issues through total maximum daily load (TMDL) and other initiatives.
CONTAMINATED SEDIMENT MANAGEMENT STRATEGY. While independent academic research into issues related to sediment contamination has been ongoing for some time (Baker, 1980), more formal U.S. EPA attention emerged in the mid-1980s with the formation of an internal agency- wide steering committee to examine programmatic issues related to sediment contamination. This Technical Advisory Committee, formed in 1986 by then Administrator Reilly, reinforced the need for a more consistent U.S. EPA plan and started to examine possible approaches for deriving SQC. In 1988, the U.S. EPA formed two oversight committees to take a comprehensive look at the whole range of contaminated sediment issues—the Sediment Oversight Committee and the Sediment Oversight Technical Committee. While both have responsibilities in forming a cohesive contaminated sediment manage- ment strategy, the latter committee is dedicated to scientific and implementa- tion issues. Representation includes U.S. EPA Headquarters, Office of Research and Development (ORD), and regional staff, with significant reliance on input from numerous public and academic consultants. The coordination of sediment management issues is necessary because the U.S. EPA has the authority under numerous statutes to address contaminated sediments as further described in Contaminated Sediments—Relevant Statutes and EPA Program Programs (U.S. EPA, 1990).
STRATEGY PROVISIONS. The U.S. EPA’s contaminated sediment management strategy describes actions that the agency will take to accom- plish four strategic goals: (1) prevention of further sediment contamination that may cause unacceptable ecological or human health risks; (2) establish when practical, clean-up of existing sediment contamination that adversely affects the nation’s waterbodies or their uses, or that cause other significant effects on human health or the environment is warranted; (3) ensure that sediment dredging and dredged material disposal continue to be managed in an environmentally sound manner; and (4) ensure development and applica- tion of consistent methodologies for analyzing contaminated sediments. The strategy is composed of six component sections: assessment, prevention, remediation, dredged material management, research, and public outreach. In each section, the agency describes actions it may take to accomplish the four broad goals. Each will be separately discussed in the following paragraphs.
xviii Assessment. In the assessment section, the U.S. EPA proposes that many agency program offices use standard toxicity test methodologies and chemi- cal-specific sediment-quality criteria to determine when sediments are contaminated. These same program offices will use sediment-quality criteria, when they are promulgated, to assess contaminated sediment sites in combi- nation with toxicity testing and use these criteria to interpret sediment chemistry data. Upon promulgation, states may adopt and use these as water quality standards in their application to establish National Pollutant Discharge Elimination System (NPDES) permit limits. These criteria could also be used with other appropriate information to make site-specific decisions concerning corrective action at hazardous waste facilities and to assess Superfund sites. The agency has not yet determined how sediment-quality criteria will be used in dredged material testing. An additional element of the assessment section is the National Sediment Inventory (NSI) that will be used by U.S. EPA program offices as an assess- ment tool (U.S. EPA, 1994a). It will be used to identify contaminated sedi- ment sites for consideration for remedial action; target facilities for possible injunctive relief or supplemental enforcement projects; identify problem pesticides and toxic substances that may require further regulation or be targeted for enforcement action; identify impaired waters for National Water Quality Inventory reports or development of TMDLs; target watersheds for nonpoint source management practices; and help select industries for further effluent guidelines development.
Prevention. To regulate the use of pesticides that may accumulate to toxic levels in sediments, the U.S. EPA intends to propose that acute sediment- toxicity tests be included in procedures required in support registration, deregistration, and special review of pesticides likely to sorb to sediments. To prevent other toxic substances from accumulating in sediments, the U.S. EPA will also propose incorporating acute sediment-toxicity tests and sediment- bioaccumulation tests to routine chemical review processes required under the Toxic Substances Control Act. In addition, the U.S. EPA intends to call for the development of guidelines for design of new chemicals to reduce bioavail- ability and partitioning of toxic chemicals to sediments. The agency’s Office of Enforcement and Compliance Assurance will take action to prevent sediment contamination by negotiating, in cases of noncom- pliance with permits, enforceable settlement agreements to require recycling and source reduction activities. The Office of Enforcement will also monitor the progress of federal facilities toxic emissions in reducing and will monitor the reporting of toxic releases to the public. The agency’s Office of Water and other program offices will work with nongovernmental organizations and the states to prevent point and nonpoint source contaminants from accumulating in sediments. The agency will (1) promulgate new and revised best-available treatment effluent guidelines for industries that discharge sediment contaminants; (2) encourage states to use biological sediment test methods to interpret water quality standards and adopt SQC as water quality standards; (3) encourage states to develop
xix TMDLs for impaired watersheds specifying point and nonpoint source load reductions necessary to protect sediment quality; (4) use the NSI to target active point sources of sediment contaminants for permit-compliance track- ing; (5) ensure that discharges from Comprehensive Environmental Response, Compensation, and Liability Act sites and Resource Conservation and Recovery Act facilities subject to NPDES permits comply with permit requirements that protect sediment quality; and (6) use the NSI to target watersheds where technical assistance and grants would effectively be used to reduce nonpoint source loads of sediment contaminants.
Remediation. Several U.S. EPA program offices, including the Office of Water, Office of Emergency and Remedial Response, Office of Solid Waste, and Office of Enforcement will use the NSI to help target sites for enforce- ment action requiring contaminated sediment remediation. The Agency’s standard sediment toxicity and bioaccumulation tests (U.S. EPA, 1989 and 1994b) will be used to identify sites for remediation, assist in determining clean-up goals for contaminated sites, and monitor the effectiveness of remedial actions.
Dredged Material Management. The U.S. Army Corps of Engineers estimates that a small percentage of the total volume of sediment dredged for navigational channel maintenance requires handling due to the presence of toxics. The NSI inventory will be used to identify sites where dredged materials are contaminated. The agency’s standard sediment toxicity and bioaccumulation tests are now used in dredged material testing (U.S. EPA, 1994a).
Research. The agency’s ORD, through its Environmental Monitoring and Assessment Program, will continue to collect new chemical and biological data on sediment quality. These data will be included in the Agency’s NSI. The ORD will also develop new biological methods to assess ecological and human health effects of sediment contaminants, chemical-specific sediment- quality criteria, methods to conduct sediment toxicity evaluations, dredged material disposal fate and transport models, sediment wasteload allocation models, and technologies for remediation of contaminated sediment.
Outreach. The Agency will undertake a program of outreach and technology transfer to educate target audiences about contaminated sediment risk management. These target audiences include other federal agencies, state and local agencies, the regulated community, the scientific community, environ- mental advocacy groups, the news media, and the general public. Technical and nontechnical information will be provided to these audiences by develop- ing a range of outreach products. The National Contaminated Sediment Task Force will monitor implementation of the U.S. EPA’s contaminated manage- ment strategy and subsequent development of a federal strategy.
BOOK ORGANIZATION. This book organizes material from respected academic researchers and consultants with interrelated experiences and xx viewpoints. In addition, significant viewpoints from federal agency personnel are included that are not intended to be the viewpoints of the U.S. EPA. We collectively acknowledge that sediment science remains an evolving area and that much more needs to be known before the management of contaminated sediments becomes routine and universally accepted. This book begins to address this need. The book is not without controversy, however, as Chapters 6 and 7 seemingly clash with respect to the interpretation of the validity of empirical sediment-effects data and what constitutes cause and effects proof. We decided that juxtaposition of these two viewpoints was proper because many who must use sediment-effects data in regulatory decision-making do not have expertise in weight-of-evidence determinations and might benefit from both viewpoints. I deeply thank this group for their dedication, hard work, and patience during the writing, review, and publication process. This effort was conceived and supported by the Water Environment Federation’s Toxic Substances Committee.
REFERENCES Baker, R. A. (Ed.) (1980) Contaminants and Sediments: Fate and Transport, Case Studies, Modeling, Toxicity. Vol. 1, Butterworth-Heinemann. U.S. Environmental Protection Agency (1989) Short-Term Methods for Estimating the Chronic Toxicity of Effluents and Receiving Waters to Freshwater Organisms. 2nd ed., EPA-600/4-89-001. U.S. Environmental Protection Agency (1990) Contaminated Sediments— Relevant Statutes and EPA Program Programs. U.S. Environmental Protection Agency (1994a) Framework for Development of the National Sediment Inventory. EPA-823/R0003, Washington, D.C. U.S. Environmental Protection Agency (1994b) Methods for Measuring the Toxicity and Bioaccumulation of Sediment-Associated Contaminants with Freshwater Invertebrates. EPA-600/R-94-024, Office of Research and Development, Duluth, Minnesota.
ACKNOWLEDGMENTS. This publication was produced under the direc- tion of Raymond C. Whittemore, Chair. Principal authors and chapters for which they were responsible are
Jennifer Byrnes Brower (3) Jerome M. Diamond (4) David Dilks (8) Dr. Robert M. Engler (1) James E. Kilduff (2) Edward R. Long (6)
xxi Thomas P. O’Connor (7) Stan J. Pauwels (5)
Additional content and review was provided by
Allen Burton (4) Gary Cecchine (3) Rick Haley Kay T. Ho Eugene Joseph LeBoeuf (2) Marianne Nyman (2) Jerry Schnoor John Scott (4) Paul Sibley (5)
Authors’ and reviewers’ efforts were supported by the following organizations:
Abt Associates, Inc., Cambridge, Massachusetts Camp, Dresser & McKee, Detroit, Michigan Connecticut Agricultural Experiment Station, New Haven, Connecticut G. Fred Lee & Associates, El Macero, California Great Lakes Environmental Research, Ann Arbor, Michigan HydroQual, Inc., Mahwah, New Jersey IT Corporation, Mahwah, New Jersey Kansas State University, Manhattan, Kansas Limno Tech, Inc., Ann Arbor, Michigan Medine Environmental Engineering, Boulder, Colorado National Council for Air and Stream Improvement, Lowell, Massachusetts National Oceanic and Atmospheric Administration, Seattle, Washington, and Silver Spring, Maryland Proctor & Gamble, Cincinnati, Ohio RAND, Arlington, Virginia Rensselaer Polytechnic Institute, Troy, New York SAIC, Narragansett, Rhode Island Stanford University, Stanford, California Tetra Tech, Inc., Owings Mills, Maryland Triad Engineering, Inc., Milwaukee, Wisconsin U.S. Army Engineer Waterways Experiment Station, Vicksburg, Mississippi U.S. Environmental Protection Agency, Narragansett, Rhode Island University of Guelph, Ontario University of Iowa, Iowa City, Iowa University of Missouri, Rolla, Missouri Vanderbilt University, Nashville, Tennessee Wright State University, Dayton, Ohio
xxii Chapter 1 An Introduction to Sediments
Robert M. Engler, U.S. Army Engineer Waterways Experiment Station, Vicksburg, MS
Sediments in the aquatic ecosystem are the analogue to soil in the terrestrial ecosystem, as they are the source of substrate nutrients and micro- and macroflora and fauna that are the basis of support to living aquatic resources. Sediments are the key drivers of environmental food cycles and the dynamics of water quality. Aquatic sediments are derived and composed of natural physical, chemical, and biological components as generally related to their watersheds. Sediments range in particle distribution from micron-sized clay particles through silt, sand, gravel, rock, and boulders. Sediments originate from bed-load transport, beach and bank erosion, and land runoff, and are naturally sorted by size through prevalent hydrodynamic conditions. In general, fast-moving water will host coarse-grained sediments and quiescent water will host fine-grained sediments. Mineralogical characteristics of sediments vary widely and reflect watershed characteristics. Organic material in sediments is derived from tissues of plants, animals, aquatic and terrestrial sources, and various point and nonpoint wastewater discharges, and increase in concentration proportional to decreasing sediment particle size. Dissolved chemicals in the overlying and interstitial waters are a product of the inor- ganic and organic sedimentary materials as well as from runoff and ground- water and range from fresh to marine in salinity. This sediment/water mileau varies significantly over space and time, and its characteristics are driven by complex biogeochemical interactions among the inorganic and living and nonliving organic components. The sediment biotic community includes micro-, meso-, and macrofauna and flora that are interdependent among each other and their host sediment’s biogeochemical characteristics.
1 To appreciate the effect that sediments have on water quality and aquatic organisms, one must understand how chemical constituents, which may have various effects on aquatic organisms, are associated with aquatic sediments. Sediments may be separated into several components or phases that are classified by their composition and mode of transport to their aquatic location. Among them are detrital and authigenic phases. Detrital components are those that have been transported to a particular area, typically by water. Detrital materials are derived from soils of the surrounding watershed and from within the aquatic system, and can include (1) mineral grains and rock fragments (soil particles) as well as stable aggregates, (2) associated organic material, and (3) culturally contributed components derived from agricultural runoff and industrial and municipal waste discharges. Authigenic components are those that are formed in place or have not undergone appreciable transport. These materials are typically the result of aquatic organisms and, as an example, may include shell material (calcium chloride, CaCO3), diatom frustules (silicon dioxide), some organic com- pounds, and products of anaerobic or aerobic transformations. Human (anthropogenic) physical and chemical activities have drastically, if not radically, modified natural sediment systems. Physical modifications range from enhanced sedimentation caused by various land-use practices to sediment deprivation caused by stream alteration (e.g., dams, levees, and channelization). These modifications range from positive to negative influ- ences on the overall sedimentary system. The most serious anthropogenic activities, however, are the introduction of synthetic chemicals to waterways by point and nonpoint sources as a result of agricultural, urban, and industrial activities; “natural” chemicals through mining, agricultural, and urban land practices; and pathogenic microbes from human and animal waste. Radiological contamination in sediments is another, but somewhat limited, concern from atmospheric nuclear testing, nuclear power and processing plants, and waste streams from hospitals and other sources. Contamination of the water invariably results in contamination of their underlying sediments. Significant sediment contamination is most often associated with the high surface area of inorganic and organic small silt- and clay-sized particles and organic coatings on silt and clay particles. For the better part of the industrial and agricultural revolution, there were few if any controls on point or nonpoint sources of contaminants. The growth of large urban areas did not necessarily include the treatment of domestic waste other than aquatic discharge. It was generally thought that sediments, especially fine-grained sediments, were efficient sinks for contaminants entering the system. This belief also applied to previously contaminated soil particulates entering the system. In general, contaminated sediments under appropriate geochemical conditions and with moderate organic matter content and a stable hydrodynamic environment can be an effective sink for metals and nonpolar organic contaminants. However, a better understanding of the short- and long-term toxicological effects of contaminated sediment has shown that some contaminated sediments can be a significant and long-term source of contaminants, and represent an unacceptable ecological and human
2 Handbook on Sediment Quality health risk. Sediment contamination ranges in severity from Superfund sites to insignificant contamination in nonindustrial locations. With regard to the ecological effect of sediments to water quality and aquatic organisms, one must understand how chemical constituents, which may have various toxicological effects on aquatic organisms, are associated with sediments. The following discussion is simply a broad overview of the complexity of chemical constituent distribution and interaction within and among sediments. Detailed discussions of sediment geochemistry, toxicology, and water quality interrelations are presented in the following chapters. A general examination of the in situ association of trace elements and compounds in sediments with various sediment phases requires that the water contained in interparticle voids or interstices be considered. This is termed interstitial water (IW), which is also called pore water. In relation to the overlying water, chemical constituents frequently may be enriched in the IW by several exchange mechanisms/locations, including exchange site of the silicate phase, and those that are associated with organic matter or trace elements complexed with the organic phase. Synthetic nonpolar organics such as polychlorinated biphenyls may be associated with active silicate as well as with the natural organic fraction or other organic fractions such as oil. Consequently, only a small amount of these low-solubility or slightly soluble constituents is found dissolved in the IW and, in fact, may be strongly resistant to desorption from the particulate fraction. An element or molecule can be present (partitioned) in a sediment in one or more sediment fractions (locations) with varying degrees of resistance to desorption. Possible locations include the lattice of crystalline minerals, the interlayer positions of polysilicate (clay) minerals, adsorption on mineral surfaces, association with hydrous iron and manganese oxides that exist as surface coatings on discrete particles, absorption or adsorption to sediment organic matter, and partitioned within the organic matrix. These locations represent a wide range of potential mobility and bioavailability. They range from stable components in the mineral lattices, which are essentially insolu- ble, to soluble components in the IW, which are readily mobile. Elements or molecules are also incorporated to living terrestrial and aquatic organisms and are relatively stable; however, they may be released during decomposition or defecation at the sediment water interface or within the sediment. Numerous sediment characterization procedures to elucidate the phase distribution of contaminants in dredged material have been applied to many types of marine and freshwater sediments, both aerobic and anaerobic. Physicochemical (Eh, pH) changes that occur after anaerobic bottom sediment is disturbed and resuspended may result in either solution or precipitation of many elemental species. Furthermore, disturbance of samples to be used for sediment characterization must be minimal because drying, grinding, and contact with atmospheric oxygen are undesirable. The general sediment phases are presented in a simplified fashion in the following list in their relative order of mobility and bioavailability. Interstitial water is the most mobile and, consequently, the most available. When contaminants enter a body of water and subsequently enter sediment particu- late matter, they typically enter two or three phases in various concentrations
An Introduction to Sediments 3 that cannot be readily distinguished from levels of concern or bioavailability by bulk or total analysis.
• Interstitial water—an integral part of sediment, is in dynamic equilibrium with the silicate and organic-exchange phases of the sediment as well as with the easily decomposable organic phase. • Mineral-exchange phase—the portion of the chemical constituent (ion) that can be removed from cation-exchange sites of the sediment. In addition to cation exchange, ions can become associated with the surfaces of mineral sediments such as clays at nonexchange sites. Ionic organic contaminants may sorb to this phase in a manner that may be highly resistant to desorption. • Reducible phase—this phase is composed of hydrous oxides of iron and manganese as well as hydroxides of iron and manganese, which are relatively stable under reducing (anaerobic) conditions. Of particular importance are the toxic metals (arsenic, copper, cadmium, nickel, cobalt, and mercury) that may be associated with these discrete phases. • Organic phase—this phase or partition of the chemical constituents is considered to be solubilized after destruction of the organic matter or through harsh solvent extraction and contains very tightly bound con- stituents as well as those loosely complexed by organic molecules. • Residual phase—the residual phase contains primary minerals and particles as well as secondary weathered minerals and recalcitrant organics that are, for the most part, a stable portion of the sediments.
The toxicology and biogeochemical characteristics of sediments are much too site specific to review on a national or even regional basis. Effects are dominated by local pollution control measures, or the lack thereof, local watershed characteristics, geomorphology, physicochemistry, geochemistry, and more. Although a total chemical characterization may be useful in deter- mining which contaminants are present, it rarely can be used to estimate or predict potential biological effects. A preferred approach would be based on a weight of evidence developed from various physical, chemical, and ecotoxico- logical measures. These are discussed generally below and in detail throughout the remainder of this report. Biological effects are a dose response, which is contingent on bioavailability of the contaminants, duration of exposure, life history of the organism, and a multitude of other environmental variables. For example, the bioavailability of nonpolar organics may be a function of the total organic carbon and even the forms of organic carbon in the sediment or of sulfides that may control the bioavailability of heavy metals. Because of the biogeochemical complexity of sediments, it is unlikely that a clear relationship between sediment chemistry and subsequent environmen- tal effects such as biological availability will be developed in the foreseeable future. Slight changes in pH can significantly alter biological availability and mobility of metals. A change in the composition of organic carbon (plant- derived organic carbon versus soot) can significantly alter the sorption/desorp- tion kinetics and subsequent biological availability of toxic organic chemicals.
4 Handbook on Sediment Quality Various toxicological assessment techniques have been developed to estimate the risks associated with contaminated sediments and are presented in detail in the following chapters. These evaluations range from simple water extracts to biologically derived water quality criteria or multiorganism chronic and acute benthic bioassays. These effects-based approaches recognize that aquatic sediments, in contrast to most industrial and domestic waste, are a complex mixture of natural and anthropogenic components whose potential environmental risks must be evaluated on a case-by-case basis using a weight of evidence approach. This introductory chapter has presented a rather simplistic overview of aquatic sediments. The following chapters of this book will thoroughly address these complex interactions and propose solutions to this complexity. The reader will find an examination and discussion of sorption processes, bioavailability, sediment collection and assessment techniques, toxicity testing, advantages and disadvantages of chemical sediment-quality guide- lines, and sediment-quality modeling. These timely discussions will help the reader better comprehend the dilemma facing those who have to identify, assess, and manage contaminated sediments.
An Introduction to Sediments 5
Chapter 2 Sorption of Organic Compounds by Soils and Sediments: Equilibrium and Rate Processes
James Kilduff, Rensselaer Polytechnic Institute, Troy, NY Eugene LeBoeuf, Vanderbilt University, Nashville, TN Marianne Nyman, Rensselaer Polytechnic Institute, Troy, NY
8 Introduction 22 Correlations with the 10 Sorption Mechanisms Octanol–Water Partition 12 Intermolecular Forces Coefficient 12 Partitioning 24 Isotherm Models 12 Ion Exchange 26 The Generalized Langmuir 13 Covalent Bonding Isotherm and Its 14 Modeling Contaminant-Phase Simplifications Distribution Equilibria 30 Potential Theory 15 Partitioning Theory 31 Combined Models 17 Estimation of Activity 34 Materials and Methodologies for Coefficients Collecting Sorption Data 19 Flory–Huggins Theory 34 Batch and Column
21 Correlations of Kd to Molecular Equilibration Techniques Properties
7 34 Batch Equilibration 65 Desorption Hysteresis and Techniques Reversibility 37 Fixed-Bed (Column) Reactor 68 Effects of Particle Size Techniques 68 Effects of Organic Matter 38 Obtaining Representative Composition and Structure Samples 68 Chemical Characterization: 39 Composition of the Solution Polarity and Aromaticity Phase 69 Rubbery/Glassy Models 40 Criteria for Achieving 69 Microporosity Equilibrium 70 Crystallinity 41 Loss Mechanisms and Controls 72 Solids-Concentration Effect 43 Reactors and Reactor 75 Sorption Rate Processes Components 76 Local Equilibrium 43 Phase Separation 77 Langmuir Kinetics 44 Desorption 77 Empirical Rate Models 45 Sorption Phenomena 79 Mass-Transfer Controlled 45 Isotherm Linearity Kinetics 45 Linear Partitioning to 79 External Mass Transfer Isolated Mineral Surfaces 81 Homogenous Solid-Phase 46 Linear Partitioning to Soils (Surface) Diffusion and Sediments 82 Pore and Combined Pore- 49 Nonlinear Sorption of Surface Diffusion Neutral Hydrophobic 83 Diffusion in Macromolecules Organics 84 Case I Transport 59 Nonlinear Sorption of 84 Case II Transport Ionizable Organics 85 Anomalous or Non-Fickian 61 Competitive Effects Transport 61 Competitive Adsorption 86 Macromolecular Diffusion Models Behavior in Natural 62 Ideal Adsorbed Solution Systems Theory 86 Summary and Conclusions 63 Polanyi-Based Models 87 References 64 Evidence for Sorbate Competition
INTRODUCTION The fate of contaminants in sediment–water systems is, in large part, gov- erned by sorptive interactions with sediment solids, including both mineral and organic constituents, and with dissolved and colloidal natural organic matter present in the solution phase. Contaminant sequestration by sediments may include such mechanisms as adsorption, ion exchange, partitioning, chemical bond formation, and diffusion-limited mass transport (Luthy et al., 1997, and Ononye and Graveel, 1994). Sorption processes may include adsorption, or accumulation on a two-dimensional surface, and absorption, or accumulation in a three-dimensional phase. These processes profoundly influence the behavior of chemicals in the environment. Sorption influences contaminant availability to the aqueous phase and, therefore, its mobility,
8 Handbook on Sediment Quality toxicity, and potential for phase transfer across the air–water interface. Sorbed species may exhibit different reactivity from those in free solution. For example, they may be less available to microorganisms and shielded from radiation and thus participate to a lesser extent in photochemical reactions. An understanding of contaminant sequestration is necessary to improve the prediction of organic compound fate, availability, and sediment toxicity. This, in turn, provides a basis for assessing exposure, evaluating risk, and defining remediation endpoints. We have restricted our focus to hydrophobic organic contaminants, an important class of pollutants including petroleum-derived aromatics, chlorinated solvents, pesticides, and such compounds as polychlo- rinated biphenyls (PCBs) that are no longer manufactured but exhibit long- term persistence in the environment. In this chapter, the underlying chemical and physical phenomena that contribute to organic contaminant sequestration by sediments are reviewed. In addition, we consider the many models available for describing sorption equilibria and kinetics and methodologies for collecting sorption data. Our primary concern is understanding sorption processes in sediments. However, many of the factors affecting sorption processes in sediments are analogous to those affecting uptake by soils and other “geosorbents.” In fact, most researchers do not restrict their research exclusively to either soils or sedi- ments. A review of the literature will reveal many papers containing data for both soil and sediment; in part, this is because sorption mechanisms are similar for the two geosorbents. In addition, it is often necessary (or desir- able) to study a wide range of sorbents, even including synthetic polymers, to fully understand sorption mechanisms. Therefore, we do not attempt to restrict our scope to sediments exclusively. In the Sorption Mechanisms section, fundamental intermolecular forces and mostly descriptive discussions of partitioning, ion exchange, and covalent bonding are reviewed. In the Modeling Contaminant-Phase Distribution Equilibria section, quantitative approaches to modeling sorption equilibria in natural systems are explored. This section begins with a detailed treatment of partitioning theory, based on the idea that sediment organic matter provides a phase into which organic chemicals can absorb or partition in a manner analogous to octanol–water partitioning. This analogy is pursued further in the section where correlations between partition coefficients and such chemical properties as solubility and octanol–water partition coefficient are developed. Models to describe adsorption equilibrium are discussed still later in the section using the Langmuir model as a starting point for more complex models such as the generalized Langmuir (GL) mode and its simplifications, Polanyi potential theory, and composite models that combine different isotherm models to represent physically realistic mechanisms. The next section discusses methodologies for collecting sorption data. Whereas such experiments are conceptually straightforward, there are many potential pitfalls, and we attempt to point out the significant ones. The next section reviews sorption phenomena and current theories in the context of current literature. The material presented in this section builds on all previous sections. The issue of isotherm linearity is investigated in detail, because isotherm shape can have a significant effect on pollutant transport. In addi-
Sorption of Organic Compounds 9 tion, the mathematics of pollutant transport becomes more complex when the sorption isotherm is nonlinear. Competitive effects are also treated in detail because they too can be important in assessing organic compound fate and such effects provide valuable insight to sorption mechanisms. Desorption hysteresis and reversibility are discussed later in the section as these phenom- ena may govern contaminant availability and sediment toxicity. The effects of particle size are reviewed, as is the influence of organic matter composition and structure, including effects of aromaticity, crystallinity, and microporosity. These concepts are used to help interpret sorption mechanisms. Finally, the last section addresses sorption rate processes. These mathematical relation- ships are important elements of the pollutant material balance, which form the basis for simulation of contaminant fate and transport. The section begins with the assumption of local equilibrium and its implications. This assump- tion can dramatically simplify the solution to material balance equations. In later sections, rate expressions based on the Langmuir model as well as other models that are often empirically based are considered. The influence of mass transfer on sorption kinetics and the models used to incorporate such effects are also discussed. Finally, the special features of diffusion in macromolecules are presented. There is mounting evidence that sorption by natural organic matter displays some characteristics of sorption by polymers, including diffusion-controlled sorption rates.
SORPTION MECHANISMS Sorption mechanisms governing equilibrium partitioning of organic com- pounds depend on the physical and chemical properties of both the organic compound and the sorbent phase (e.g., Hassett et al., 1980; Karickhoff, 1981; and Zierath et al., 1980). Organic pollutants of interest include hydrophobic organic compounds (HOCs) such as PCBs, polyaromatic hydrocarbons, dioxins and furans, substituted aromatics, chlorinated benzenes, chlorinated phenols, triazine herbicides, carbamate pesticides, and organophosphate pesticides, among others. The polarity of such compounds depends on halogen-substitution patterns, the presence of oxygen- and nitrogen-contain- ing moieties, and the presence of ionizable functional groups. Many such compounds do not contain ionizable functional groups, but others do, and such moieties can significantly influence chemical properties and sorption behavior. Natural sediments are heterogeneous, and this heterogeneity is likely to occur on multiple scales. This is depicted schematically in Figure 2.1. Individual particles may have different origins and composition (e.g., shale and quartz), and each particle may be composed of different materials (e.g., mineral surfaces coated with organic matter). Mineral surfaces contain oxide functional groups that give the surface a pH-dependent charge and that can be involved in electrostatic and ligand-exchange reactions. The mineral surfaces may contain pores, both mesoporous (having widths between 2 and 50 nm)
10 Handbook on Sediment Quality Figure 2.1 Schematic depiction of sediment heterogeneity (containing mineral and organic surfaces) and sorption mechanisms (partitioning, electrostatic bonding, ion-exchange, and covalent bonding).
and micropores (having widths smaller than 2 nm). In many cases, the organic constituents of the sediment phase dominate sorption behavior, which can include both partitioning (absorption) and adsorption mechanisms. The dominant mechanism appears to depend on the source, composition, and age of the organic matter (e.g., Binkley, 1993; Hassett et al., 1980; Karickhoff, 1981; McGinley and Weber, 1993; Sikka et al., 1978; Wu and Gschwend, 1986; Zachara et al., 1984; Zachara et al., 1986; and Zhang et al., 1993). Soil and sediment organic matter is a heterogeneous mixture of partially or completely degraded molecules of plant and animal origin. The organic constituents may exist as fulvic and humic acids, humin, kerogen, or some combination. These classes of organic compounds, generally defined operationally, can be viewed as lying on a spectrum of diagenetic alteration. Some investigators have made a distinction between younger, amorphous organic matter, and older, denser, more crystalline forms. The latter may include shales and combustion residues such as soot, which can exhibit high sorption capacities. Ion exchange and adsorption to mineral surfaces may contribute signifi- cantly to the sorption of compounds having ionizable functional groups; in such cases, geosorbent cation-exchange capacity and solute speciation as a function of pH are important (Ainsworth et al., 1987). Some hydrophobic organic compounds have been shown to form covalent bonds with sediment humic substances, mineral surfaces, or both. All sorption processes are driven, in part, by some combination of intermolecular forces.
Sorption of Organic Compounds 11 INTERMOLECULAR FORCES. Sorption mechanisms include specific interactions between dissolved solutes and solid surfaces (or surface coatings) and thermodynamic gradients (solution entropy), important for solvophobic compounds. Specific interactions are generally categorized as chemical, electrostatic, and physical. Each classification has a characteristic energy of interaction and interaction range (Atkins, 1994). Short-range chemical forces leading to hydrogen bonding or covalent bonding (chemisorption) are characterized by large heats of adsorption, on the order of 20 kJ/mol for hydrogen bonds and higher for covalent bonds. Electrostatic ion–ion interac- tions can arise between ionizable solutes and surface moieties and are characterized by large interaction energies on the order of 250 kJ/mol and vary inversely to their separation distance, or as 1/r. Ion–dipole interactions exhibit much lower interaction energies, on the order of 15 kJ/mol, and vary as 1/r 2. Physical sorption is caused by net attractive interactions between partial charges of molecules (van der Waals forces). These include dipole–dipole interactions between polar molecules, dipole-induced dipole interactions between polar and ionizable molecules, and induced-dipole− induced-dipole interactions (London dispersion forces) between nonpolar molecules. Dipole–dipole interactions vary as 1/r 3 for fixed orientations and 1/r 6 for freely rotating orientations; other van der Waals interactions also vary as 1/r 6. Physical adsorption bonding forces are relatively weak, on the order of only a few kJ/mol. However, these may be amplified by a favorable thermodynamic gradient in solution entropy, effectively driving hydrophobic molecules out of solution (Voice and Weber, 1983).
PARTITIONING. An important mechanism of organic compound uptake by soils and sediments is partitioning into one or more organic phases associated with the mineral fraction. This process is conceptualized as contaminant distribution between two immiscible (Schwarzenbach et al., 1993) or partially miscible (Chiou et al., 1983) solutions. The contaminant is essentially considered dissolved or absorbed into a three-dimensional organic matrix consisting of a porous structure of macromolecule chains. Xing and Pignatello (1997) point out that this dissolution domain is composed of thermodynamically dynamic sites, whose energies average out as in a liquid. Thus, this process is analogous to the partitioning of a solute between water and an organic solvent phase (Chiou et al., 1983). In general, the extent of partitioning is governed by the difference between the partial molar excess free energy of the solute in the aqueous (w) and the sediment organic matter (om) phases.
ION EXCHANGE. Ion exchange is defined as the replacement of one adsorbed ion with another (Sposito, 1989). We restrict this to the sorption of fully solvated ionic species and exclude specific adsorption processes that involve the formation of an inner-sphere surface complex. Ion-exchange sites may exist on mineral surfaces and as part of the sediment-dissolved organic matter structure. Ion-exchange reactions are driven primarily (but not exclu- sively) by electrostatic (coulombic) interactions between exchange sites and dissolved ions in solution. In addition, van der Waals forces between
12 Handbook on Sediment Quality hydrophobic moieties on an organic ion and nonpolar regions of the solid phase can enhance sorption. The ion-exchange reaction is expressed generi- cally by the following reactions (Sposito, 1994):
b+ a+ bAXa(s) + aB (aq) ⇔ aBXb(s) + bA (aq) (2.1)
d– c– dCYc(s) + cD (aq) ⇔ cDYd(s) + dC (aq) (2.2)
Where a, b, c, and d = stoichiometric coefficients, A, B, C, and D = ions, X = 1 mol negative charge, and Y = 1 mol positive charge carried by the solid surface.
Cation exchange has been shown to be the predominant mechanism for sorption of organic bases (Karickhoff and Brown, 1979; Lee et al., 1997; and Nicholls and Evans, 1991), even at pH values 2 to 3 log units greater than the
solute pKa (Ainsworth et al., 1987; Bellin, 1993; and Zachara et al., 1986). The cation-exchange capacity (CEC) is used as a measure of a soil’s capacity to sorb cations; it is defined as the total number of exchangeable cations associated with negatively charge sites. For example, the following reaction represents the exchange of an inorganic cation (e.g., K+), initially present on the solid-phase surface, for a monovalent organic cation (BH+):
+ + KX(s) + BH (aq) ⇔ BXb(s) + K (aq) (2.3)
The preference for certain ions is related first to ionic charge and second to solvation energy, as manifested in the hydrated radius. The method for analyzing CEC assumes that exchange sites are primarily occupied by exchangeable cations (e.g., Na+,K+,Ca2+, and Mg2+) and that cation displace- ment is entirely attributable to the ammonium ion (Thomas, 1982). Sorption of aromatic bases is often positively correlated with both the CEC and the organic carbon content of the solid phase, and is influenced by solution phase
speciation (i.e., solution pH and solute pKa).
COVALENT BONDING. Some hydrophobic organic compounds (e.g., aromatic amines, phenolic compounds, and 2,4,6-trinitrotoluene) have been shown to undergo covalent bonding with natural organic matter (e.g., humic substances) from sediments, soils, and natural water. Such reactions lead to slow disappearance from the solution phase and possible immobilization (Achtnich et al., 1999; Burgos et al., 1996; and Ononye et al., 1989). The composition of natural organic matter as well as functional groups on syn- thetic organic sorbates have been recently studied to understand both reversible and irreversible covalent bonding of such compounds to soil or sediment organic matter (Achtnich et al., 1999, and Dec and Bollag, 1997). Organic bases, such as aromatic amines, are capable of forming covalent bonds with soil and sediment particles. Zachara et al. (1984) observed that
Sorption of Organic Compounds 13 sorption of aniline was partially irreversible for a relatively high carbon content soil, whereas sorption appeared to be reversible upon removal of the organic matter from the soil. Graveel et al. (1985) concluded that sorption of benzidine, α-naphthylamine, and p-toluidine involved a reaction with the phenolic components of humus-type material. Later, Ononye and Graveel (1994) studied reactions between α-naphthylamine and 4-methylaniline (as model solutes) and quinones (as representative of humic acid moieties). They found that imine formation was fast and reversible, whereas 1,4-nucleophilic addition of the amino group to the quinone ring was slower and irreversible. Parris (1980) showed that imine formation for aniline is also reversible. In contrast, both the imine and 1,4-nucleophilic additions were irreversible for benzidine (1,1'-biphenyl-4,4'-diamine) (Ononye et al., 1989). Weber et al. (1996) investigated the covalent bonding pathway for reactions of aromatic amines with dissolved organic matter. Like Ononye et al. (1989), they observed biphasic kinetics, which they attributed to rapid and slow sorption steps. These researchers concluded that dissolved organic matter was not a significant sink for aromatic amines in most aquatic environments. Instead, they suspected that the aromatic amines are more likely to be removed by covalent bonding to natural organic matter associated with bottom sediments. In a subsequent paper, Thorn et al. (1996) studied the nucleophilic addition reactions of aniline to humic substances. The study suggested that the formation of anilinohydroquinone nitrogen is a reversible step and that the anilinohydroquinone nitrogen represents a fraction of the covalently bound aniline. Additionally, their study suggested that the anilide nitrogens are also subject to exchange by other amines. Natural soils and sediments have also been shown to be oxidation catalysts (Bollag, 1992; Burgos et al., 1996; and Park et al., 1999). Phenolic com- pounds can undergo oxidative coupling reactions catalyzed by carbon surfaces, enzymes, and metal oxides (Bollag, 1992; Grant and King, 1990; and Park et al., 1999). Oxidative coupling is a surface reaction in which phenol multimers are formed through ether linkages, which are promoted by high pH, temperature, and the presence of dissolved oxygen. The lack of reversibility of phenol sorption by natural geosorbents (Bhandari et al., 1996, and Burgos et al., 1996) and model adsorbents (Grant and King, 1990, and Kilduff and King, 1997) has been shown to decrease as a result of oxidative coupling. It is possible that this reaction results in chemisorption or the formation of strongly physisorbed reaction products.
MODELING CONTAMINANT - PHASE DISTRIBUTION EQUILIBRIA
Of fundamental importance to both fate and transport predictions and risk assessment is the equilibrium distribution of a contaminant species (sorbate) between the aqueous and sediment phases (sorbent). The distribution coeffi-
14 Handbook on Sediment Quality cient is defined as the ratio of the solute concentration in the sorbed phase, qe, to the concentration in the solution phase, Ce (mol/L), at equilibrium
qe Kd = – (2.4) Ce
Typically, sorbed-phase concentrations have units of moles (or mass) per unit mass (or surface area) of sorbent. In general, the distribution coefficient is a function of temperature and aqueous-phase concentration of the sorbate of interest as well as the aqueous-phase concentrations of all solutes that may compete for sorption sites or change sorbate activity (in solution or in the sorbed phase)
N
Kd,i = Kd,i [T, xi, Σ xj] (2.5) j=1 Where
xi = the mole fraction of the contaminant of interest, xj = the mole fraction of species that may compete for sorption sites or otherwise affect sorption uptake, and T = temperature.
The relationship between qe and Ce at constant temperature is the sorption isotherm. The simplest possible isotherm is the linear isotherm, which results
when Kd is constant. This is rigorously true for adsorption only when surface coverage is low and the surface is energetically uniform. A constant Kd is typical of partitioning processes for compounds of environmental interest over
concentration ranges of practical importance. Often, a constant Kd is taken as evidence of a linear partitioning process. When a partitioning mechanism is either demonstrated or assumed, the constant distribution coefficient is often
referred to as Kd. From a practical perspective, Kd is approximately constant when the concentration range of interest is sufficiently small to guarantee that
the change in Kd is negligible or within limits of experimental error.
PARTITIONING THEORY. At least to some extent, nearly all soil and sediment organic matter provides an environment composed of a porous, three-dimensional organic matrix of macromolecule chains into which organic compounds can partition. The tendency of an organic compound to move from the aqueous phase to the sediment organic-matter phase and the result- ing equilibrium distribution is governed by the difference between the partial molar excess free energy of the solute in each phase. Therefore, at least in part, uptake or organic compounds by soils and sediments is due to partition- ing into one or more organic phases associated with the mineral fraction. This process is analogous to the partitioning of a (hydrophobic organic) solute between water and an organic solvent phase (Chiou et al., 1983). Note that from a mechanistic point of view partitioning occurs into organic matter; however, sediment organic matter is generally measured in terms of organic carbon (oc). Most natural organic matter has a carbon content of approxi-
Sorption of Organic Compounds 15 mately 50%; therefore, the mass fraction of organic matter, fom, is approxi- mately twice the mass fraction of organic carbon, foc. At equilibrium, chemical potentials in the organic-matter-saturated aqueous and water-saturated organic-matter phases must be equal. Using subscripts to designate components, superscripts to designate phases, and designating the organic solute as component 1, chemical potentials are written
µµwo=+ γ womwom,, 11RTln 11 x (2.6)
µµom=+ o γ om,, w om w 11RTln 11 x (2.7)
Where µ = the chemical potential (kJ/mol); µo = the standard chemical potential (kJ/mol); R = gas constant; T = temperature;
γ1 = the organic solute activity coefficient; x1 = solute mole fraction; om,w = the water-saturated organic-matter phase; and w,om = the organic-matter-saturated aqueous phase (Chiou et al., 1983).
An equivalent criterion for equilibrium is that fugacities (i.e., ideal pressures that characterize the escaping tendency from a phase) in each phase are equal
ˆˆwom,,,,,,=== womγγ wom omw omw omw fx11111111 ffx f (2.8)
Where ˆ w,om ˆ om,w f 1 and f 1 = the fugacities of the organic solute in aqueous solution and water-saturated organic matter, respectively, and
f1 = a reference-state fugacity, typically taken as the pure component (or subcooled liquid) fugacity.
Using the same standard state for both phases
γ wom, x om, w ln1 = ln 1 γ om, w wom, (2.9) 1 x1
In the nomenclature of eq 2.4, we convert mole fraction units into concentra- tion units more typically used for Ce (mol/L) and qe (mol/kg sediment)
x wom, fxom, w C ==1 and q om 1 (2.10) e V wom, e V om,, wρ om w
Where V w,om and V om,w = the molar volumes of the aqueous-solution phase and the water-saturated sediment organic phase, respectively (L/mol);
16 Handbook on Sediment Quality ρom,w = the sediment organic matter density (kg/L); and
fom = the mass fraction of organic matter in the sediment.
Chiou et al. (1983) used a value of 1.2 for the organic matter specific gravity based on a comparison of similar polymeric materials. It is generally valid to assume that pure water and water in equilibrium with organic matter have the same molar volume (V w,om = V w). Combining eq 2.9 and 2.10 yields the following relationship for the distribution coefficient
om,, wρ om w =−−γγwom,, omw V lnKd ln11 ln ln w (2.11) Vfom
The distribution coefficient is often normalized to the mass fraction of total
organic carbon, foc, which is typically measured by oxidation (combustion) and detection of evolved carbon dioxide. The organic carbon–normalized distribution coefficient is
om,, wρ om w =−−γγwom,, omw V − lnKoc ln11 ln lnw ln foc (2.12) Vfom
Equations 2.11 and 2.12 contain several parameters that may be expected to remain constant with organic contaminant concentration over the range expected for hydrophobic organic solutes. These include properties of the organic mater (molar volume, density, and mass fraction of the solid sorbent) and properties of the solution phase (molar volume). Therefore, it is clear
from these relationships (eqs 2.11 and 2.12) that Kd and Koc will remain constant as long as the activity coefficients in the aqueous and organic phases are constant. The following analysis will show that this is likely to be the case for sparingly soluble hydrophobic organic contaminants.
Estimation of Activity Coefficients. The aqueous-phase activity coefficient, w γ 1, is rigorously a function of mixture composition. It can be correlated using a model of excess Gibbs free energy. One such model is the van Laar equa- tion (Smith et al., 1996, and Tsonopoulos and Prausnitz, 1971)
∞ −2 ∞ ⎡ x ln γ ⎤ lnγγw =+ ln ⎢1 11⎥ (2.13) 11 − γ ∞ ⎣ ()ln1 x12⎦
Where 1 = the infinite dilution activity coefficient of organic solute in water, and 2 = the infinite dilution activity coefficient of water in organic solute.
These can be estimated from correlations (Lyman et al., 1990, and Tsonopoulos and Prausnitz, 1971) or from mutual solubility data (Carlson and Colburn, 1942). Equation 2.13 can be used to demonstrate that the expected range of aqueous activity coefficients for most hydrophobic organic solutes is small.
Sorption of Organic Compounds 17 Values for all necessary parameters are available for benzene, which is relatively soluble in comparison to many contaminant classes of interest, including hydrocarbons, substituted benzenes, polycylic aromatic hydrocar- bons (PAHs), phthalates, PCBs, and pesticides (Schwarzenbach et al., 1993). w,sat !4 For the benzene/water system, 1 = 2400, 2 = 430, and x1 = 4.2 × 10 . w,sat Using these values in eq 2.13 yields a value of 2378 for 1 , the activity coefficient in water saturated with organic solute, differing from 1 by less than 1%. For less soluble contaminants, the difference will be even smaller. For contaminants that are solids at environmental temperatures and pressures, an expression for the solution-phase activity coefficient at satura- tion can be developed by considering equilibrium between the aqueous phase (w) and the pure-solid phase (s), as described by
ˆˆw=== w,, satγγ w sat l s s s s fx11111111 ffxf (2.14)
Where w,sat x1 = the mole fraction solubility, w,sat 1 = the activity coefficient in water saturated with solid organic solute, ˆs f 1 = the fugacity of the pure solid, and l f1 = the fugacity of the pure subcooled liquid (found by extrapolating the vapor pressure curve from the triple point to the temperature of the solution).
Other terms have been defined previously. Assuming negligible solubility of water in the solid-organic phase, it is valid to assume that the mole fraction and activity coefficient of the organic species in the solid phase is unity: s s x1 1 =1; therefore ⎛ f s ⎞ x w,, satγ w sat = ⎜ 1 ⎟ (2.15) 11 ⎝ f l ⎠ 1 pure organic
The fugacity ratio was shown by Prausnitz (1969) to be
⎛ f s ⎞ ∆H f ⎛ T ⎞ ∆∆c ⎛ T ⎞ c T ln⎜ 1 ⎟ =−t −11+−p t − p ln t (2.16) ⎝ l ⎠ ⎝ ⎠ ⎝ ⎠ f1 RTt T R T R T Where H f = the enthalpy of fusion,
Tt = the triple point temperature, and cp = equal to the difference between the liquid- and solid-phase heat
capacities, (cp,liquid – cp,solid).
This expression essentially accounts for the energy required to overcome intermolecular forces in the crystalline organic solid. Application of this equation to phenanthrene was demonstrated by Huang and Weber (1997) and Tsonopoulos and Prausnitz (1971). The activity coefficient at saturation was
18 Handbook on Sediment Quality extrapolated to infinite dilution by Tsonopoulos and Prausnitz (1971) using a simplified two-suffix Margules equation
w, sat ∞ ln γ ln γ = 1 1 − 2 (2.17) ()1 x1
–7 For phenanthrene, having a mole fraction solubility of x1 = 1.31 × 10 , it is clear that there is negligible difference between infinite dilution activity coefficients and those at saturation.
FLORY–HUGGINS THEORY. The Flory–Huggins theory has been used to quantify the activity coefficient of the organic contaminant in the sediment om,w organic matter phase, 1 . The sediment organic matter phase is treated as an amorphous polymer, which is thought to be a reasonable representation. Chin and Weber (1989), Chiou et al. (1983), LeBoeuf and Weber (1999), Spurlock and Biggar (1994a, 1994b, 1994c) and have invoked this theory, which relates solute activity to a solute–organic matter interaction parameter
V1 ln(aom,w) = ln(xom,w γ om,w) = ln φ + φ 1 – –– + χφ 2 (2.18) 1 1 1 1 om Vom,w om Where