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Fugitive Mercury Emissions from Two Gold Mines in Nevada


On November 20, 2009, Dr. Chris Eckley, a post doctoral researcher working with
Dr. Mae Gustin presented a preview of his work and that by a graduate student,
Matthieu Miller, on fugitive mercury emissions from two gold mines in Nevada
(see the attached slides). The research focused on measuring mercury emissions
from a variety of surfaces disturbed by mining activities at Newmont’s Twin Creeks
Mine northeast of Winnemucca, Nev., and Cortez Pipeline, a Barrick property
located south of Battle Mountain, Nev, and used this information to develop an
estimate of emissions for the mine surface area. Fugitive emissions from waste
rock, heap leaches, tailings impoundments, active pit surfaces, stockpiles and
reclaimed sites were estimated and compared to mercury releases from sites
undisturbed by mining.


The results showed that mercury emissions from mining disturbances are
approximately 20 percent of the total mercury emitted at these two gold mines. The
study showed heap leaching and tailings impoundments produced the greatest
emissions and that current reclamation practices can reduce the current emissions to
near natural levels.


Importantly, the work showed that the amount of mercury emitted from these types
of disturbances can vary significantly among mines, depending primarily on the
mercury concentration at the disturbed site, the moisture content of the tailings and
whether or not the heaps are actively being leached with cyanide. Because there are
a variety of factors (such as mercury concentration, age of the materials, climatic
conditions, weather, ore type, ore processing techniques, etc.) that can affect the
emission of fugitive mercury from different mining surfaces and the uncertainty
associated with each of those factors, this data, developed for these two mines,
cannot be extrapolated to come up with emissions estimates for other mines.
Additionally since a mine is a dynamic entity with surfaces changing over time, and
the emission estimates developed in the UNR study represent the surfaces present at
the two mines s in 2008, the amount of Hg released in future years may differ
depending on the types and extent of mining related surfaces at each facility.


The data contained in the attached power point presentation have not been peer reviewed.
Fugitive Mercury Emissions From
         Nevada, USA Gold Mines
           Eckley, CSa, Gustin, Ma, Miller, MBa, Marsik, Fb




a   University of Nevada Reno, Department of Natural Resources and Environmental Science
b   University of Michigan, Department of Atmospheric, Oceanic and Space Sciences
Acknowledgements
                                   Nevada’s mining companies

                      Fugitive Mercury Emissions Project Oversight committee


    Project Participation




Note: Information presented has not be subjected to final scientific
peer review
Mercury (Hg) is a pollutant of global concern
  Hg emissions to air
                        Transport and Transformation


                                            Mercury exposure through fish



                           Methyl-Hg




      Numerous studies have identified Hg enriched
            soils are a source Hg to the air
Project Context
                              Mineral trends with high gold content
 The modern gold rush         are often enriched in Mercury (Hg)




                                    NV Cinnabar (HgS)




                 ~$1,000 oz




                                Graphs from Nevada Bureau of Mines
                                and Geology
Nevada Gold mines contain point sources of Hg
 emissions:
           2,000 kg/yr(NDEP 2006/2007)




                                 Point Source Emissions
                                         Hg




Nonpoint source Hg emissions from Nevada Gold
mines: ???? kg/yr
Project Objectives:
 1) Quantify nonpoint source Hg emissions from active
    gold mines




 2) Quantify natural nonpoint source Hg emissions from
    adjacent undisturbed areas
Introduction to Mine Processes

                       Holes drilled and ore examined for grade and
                       metallurgical properties




                                             Blast rock


                                                  Based on gold content trucks deliver the
                                                  ore to different processing locations




Schematic pictures
from Nevada Mining
Association Brochure
Schematic pictures
                                                          from Nevada Mining
                                                          Association Brochure
                                Waste Rock/Overburden

                      High grade ore

                                              Grinding Mill


Low grade ore                                  Sulfide
                 Carbonaceous
                                   Oxide



                                                                 Tailings pond
Heap Leach Pad




         Gold Collected on Activated Carbon
Two mines chosen for study




                   ¸



 0   1,500 m                             0      1,000 m

Twin Creeks Gold Mine        Cortez Gold Mine
Two mines chosen for study
Different materials have         Waste rock
different surface areas that
change over the life of a mine



                            ¸
                                 Heap Leach




                                 Tailings




                                 Old/Reclaimed


 0    1,500 m                                                0      1,000 m

Twin Creeks Gold Mine                            Cortez Gold Mine
Undisturbed Areas: Similar rock types excavated at mines



Twin Creeks Area        Outcrops              Cortez Area




                        Hills Alluvium




                        Valley Alluvium




                                          0      3,000 m
Method to measure emission:

Outside air                        Inside chamber
sample line                        sample line

                                                    Tekran Total Gaseous
                                                    Mercury Analyzer

                                                    ng per m3 of air

Dynamic Flux Chamber
 Flux = (Cinside-Coutside *(Q/A)

 Flux is emission or deposition per unit area
 per time

 Units
 ng (10-9g) per m2 per hour or
 ng per m2 per day
Methods: General Research Approach
1) Identify important factors controlling flux using laboratory
   experiments




                                                 • 48 tubs—3 from each
                                                   surface type

                                                 • Each tub: 24 hr fluxes
                                                   twice per season

                                                 • >400 diel flux
                                                   measurements

                                                 • Meteorological data
                                                   collected on site
Active Gold Mine          UNR Greenhouse
                                                 • Develop algorithms
Methods: General Research Approach
1) Identify important factors controlling flux using laboratory
    experiments
2) Measure fluxes at the mines
       compare with laboratory derived data
       develop data for surfaces not represented in lab study


Winter           Spring
                                    ~ 1 week at each mine each season

                                    24 hours sampled from each surface
                                    Day               Night

Summer           Fall
Methods: General Research Approach
1) Identify important factors controlling flux using laboratory
    experiments
2) Measure fluxes at the mines
       compare with laboratory derived data
       develop data for surfaces not represented in lab study


2 flux
Winter   chambers   Spring         2 Tekrans
                                    ~ 1 week at each mine each season

                                    24 hours sampled from each surface
                                    Day               Night

Summer              Fall
Methods: General Research Approach
1) Identify important factors controlling flux using laboratory
    experiments
2) Measure fluxes at the mines

3) Estimate emissions for each mine based on current surface
areas and environmental conditions over the year of study

Twin Creeks           Cortez Pipeline
                                            Geographic Information System
                                            (GIS)
Results: Laboratory

    Fluxes vary:
                   Daily
Results: Laboratory

    Fluxes vary:
                     Daily

               Seasonally


                   Leach (pre-cyanide)Twin Creeks mine (2.7 µg g-1)
Results: Laboratory


Fluxes influenced by:
      surface type, material Hg content




                                       Dry            Wet
                           29000       Winter
                                       Spring
    Hg Flux (ng m-2 d-1)




                                       Summer
                                       Fall
                           19000




                           9000




                           -1000
                                   0   3      6   9    12   15   18   21   24      27   30   33   36   39   42   45   48
                                                                           Tub #
Results: Laboratory


Fluxes influenced by:
      surface type, material Hg content

precipitation events—4-fold emission increase

                                                                                600                                                     Dry –November
                                       Dry            Wet                                                                              November, 10 2008
                                                                                                                                        Wet—December
                           29000       Winter                                   500                                                    December, 26 2008
                                                                                                                                        Dry –January
                                       Spring                                                                                          January, 1 2009
                                                                                400
    Hg Flux (ng m-2 d-1)




                                       Summer
                                                            Hg Flux (ng/m2/h)




                                       Fall
                           19000                                                300

                                                                                200

                           9000                                                 100

                                                                                  0
                                                                              00:00:00       06:00:00          12:00:00          18:00:00              00:00:00
                           -1000
                                   0   3      6   9    12                   -100 18
                                                                            15         21   24      27   30   Time of 36
                                                                                                                33    Day   39    42     45     48
                                                                                            Tub #
Results: Laboratory

Use statistical analyses to determine most
important variables and develop model
equations


                                            Daily Hg Flux                                        Hourly Hg Flux
                                         (between materials)                                  (individual materials)
                                         Winter
                                         Spring
                         29000                                                               Median             Median
                                         Summer
     Parameter                           Fall
                                                      T-statistic          p-value           T-statistic        p-value
  Hg Flux (ng m-2 d-1)




     Substrate Hg
      19000                                           15.2                 <0.001            -----              -----
     Substrate moisture                               3.4                  0.001             -----              -----
     Solar radiation
       9000                                           2.2                  0.023             8.3                <0.001
     Air temperature                                  3.3                  0.001             2.8                <0.001
     Relative Humidity                                2.5                  0.014             -0.3               <0.001
                         -1000
                                 0   3      6     9   12    15   18   21    24     27   30      33   36    39   42      45   48
     Wind speed                                       3.3                  0.001             -0.2               <0.001
                                                                           Tub #
Results: Laboratory


      Develop equations that allows us to predict flux
      as a function of material Hg concentration and
      solar radiation



      Twin Creeks dry tub data                                                                               Cortez-Pipeline dry tub data
                                                                                                             10000
                       50000                                                                                             low solar        y = 110x + 373 r² = 0.25
                                                                                                              9000
                       45000       low solar        y = 71x + 568 r² = 0.71
                                                                                                              8000       middle solar y = 338x - 132 r² = 0.66
                       40000


                                                                                      Hg Flux (ng m-2 d-1)
                                   middle solar       y = 99x + 1335 r² = 0.50
Hg Flux (ng m-2 d-1)




                                                                                                              7000       high solar       y = 419x + 143 r² = 0.60
                       35000       high solar       y = 507x + 985 r² = 0.77                                  6000
                       30000
                                                                                                              5000
                       25000
                       20000                                                                                  4000
                       15000                                                                                  3000
                       10000                                                                                  2000
                        5000                                                                                  1000
                           0                                                                                     0
                               0               20            40           60     80                                  0                 5               10            15
                                                    Substrate Hg (µg g-1)                                                             Substrate Hg (µg g-1)
Results: Laboratory simulation of surface disturbance




                                                                                                                             Surface disturbance

                                                                                                                             Increases flux 7-fold

                                                                                                                             Effect of disturbance
                                                                                                                             decreases over time
                        300
                                                                       Hg Flux
                                                                       DFC Temp              100
                                                                                                                             (~ 7 days)
                                                                       Solar Radiation
                        250

                                                                                             80




                                                                                                   Solar radiation (W m-2)
                        200
Hg Flux (ng m-2 h -1)




                                                                                                      Temperature (C)
                                                                                             60
                        150

                                                                                             40
                        100


                        50                                                                   20


                         0                                                                   0
                              0   1   2      3          4         5    6           7     8
                                          Days following disturbance
Field Measurements:
     -Characterize Hg concentrations in substrate
     -Collect data from field for comparison with laboratory data
     -Measure flux from surfaces not represented in laboratory study
      Active leach                Reclaimed tailings




                                 Old leach pad
      Tailings material
Results: Field data

     Characterization of Hg concentrations in substrate


Twin Creeks Gold Mine        Cortez-Pipeline Gold Mine
Results: Surface area/concentration

      Characterization of Hg concentrations in substrate
  Twin Creeks Gold Mine             Cortez-Pipeline Gold Mine
Spatial Ave Substrate Hg: 5.9 µg/g                     Spatial Ave Substrate Hg: 1.3 µg/g




                                     Solid Hg (µg/g)
                                         0 -12
                                         12 - 24
                                         24 - 36
                                         36 - 48
                                         48 - 60
                                         60 - 72
                                         72 - 84
                                         84 - 96
                                         96 - 108
                                         108 - 120
Results: Surface area/flux
Spatial Variability of Hg fluxes

Lowest Emissions:
• Waste rock materials                 Surface Area
  (~10’s to 100’s ng m-2 d-1)
                                             Cortez   Twin Cks
Highest Emissions:
• Active leach pads & tailings
  (~1,000’s to 100,000’s ng m-2 d-1)
Comparison of field data with laboratory derived model


>80% of field measurements were within the 95% prediction intervals of the laboratory
data




                           Twin Creeks Gold Mine                                                         Cortez-Pipeline Gold Mine
                       50000
                                                                                                     10000
                       45000       high solar--lab y = 507x + 985 r² = 0.77
                                                                                                     9000        high solar--lab
                       40000                                                                                                       y = 419x + 143 r² = 0.60
                                   high solar--field
                                                                                                     8000
Hg Flux (ng m-2 d-1)




                       35000                                                                                     high solar--field


                                                                              Hg Flux (ng m-2 d-1)
                                                                                                     7000
                       30000
                                                                                                     6000
                                                                                                                  Tailings
                       25000
                                                                                                     5000
                       20000                                                                         4000
                       15000                                                                         3000
                       10000                                                                         2000
                        5000                                                                         1000
                                                                                                                                       Old leach
                           0                                                                             0
                               0             20            40            60                                  0              5             10                  15
                                               Substrate Hg (µg g-1)                                                      Substrate Hg (µg g-1)
Comparison of field data with laboratory derived model




                           Twin Creeks Gold Mine                                                         Cortez-Pipeline Gold Mine
                       50000
                                                                                                     10000
                       45000       high solar--lab y = 507x + 985 r² = 0.77
                                                                                                     9000        high solar--lab
                       40000                                                                                                       y = 419x + 143 r² = 0.60
                                   high solar--field
                                                                                                     8000
Hg Flux (ng m-2 d-1)




                       35000                                                                                     high solar--field


                                                                              Hg Flux (ng m-2 d-1)
                                                                                                     7000
                       30000
                                                                                                     6000
                                                                                                                  Tailings
                       25000
                                                                                                     5000
                       20000                                                                         4000
                       15000                                                                         3000
                       10000                                                                         2000
                        5000                                                                         1000
                                                                                                                                       Old leach
                           0                                                                             0
                               0             20            40            60                                  0              5             10                  15
                                               Substrate Hg (µg g-1)                                                      Substrate Hg (µg g-1)
Hg fluxes from tailings
 Heterogeneous
 Hg content (19 to 177 µg g-1),
 Moisture (0.1% to liquid solution)
 Flux (889 to 684,000 ng m-2 d-1).

 Magnitude of emissions best correlated with % moisture r 2 = 0.55 p=0.001


  Twin Creeks
Results: Cyanide Heap Leaching


Hg fluxes from substrate actively under leach only obtained at Twin Creeks
     Typical Cortez leach




      Twin Creeks Leach
Results: Cyanide Heap Leaching
                                                                                        Twin Creeks Spring Data
                    12000                                                           Pre leach: 2,280 ± 1,470 ng/m2/d
                                 Active CN
                                 Pre CN
                    10000
                                 Post CN                                            Active leach: 101,300 ± 53,400
                    8000                                                                                      ng/m2/d
Hg Flux (ng/m2/h)




                    6000
                                                                                    Post leach: 1,750 ± 572 ng/m2/d
                    4000


                    2000


                        0
                       0:00:00      6:00:00     12:00:00       18:00:00   0:00:00

                    -2000
                                              Tim e of Day


                    Pre CN         3 µg/g                  CN Addition 4 µg/g               Post CN    5 µg/g
Results: Cyanide Heap Leaching
Daily Emissions increase ~4-fold from the effect of wetting alone

Daily Emissions ~35-fold higher during leaching than from pre and post
leaching

Mean Hg Content of leach solution:
17 µg/L (Cortez)                              Nevada rainwater:0.002-0.4 µg/ L
                                              (Mercury Deposition Network Data Station: NV02, 2007 data)
470 µg/L (Twin Creeks)

A component of Hg emitted during active leaching is from the cyanide solution
Results: Material age/reclamation

Emissions from capped tailings Twin Creeks (spring, 2008 data)


            Ave flux from tailings: 27,600 ng/m2/d

            Ave flux from capped tailings: 1,160 ng/m2/d

            Fluxes may be greatly reduced post-reclamation



Data from 5 year old/inactive leach suggest fluxes decline as
materials age
Annual Emission Estimates

•   1) Calculate fluxes
    – Use substrate Hg concentrations versus solar radiation relationship for dry and wet
      surfaces


        Make adjustments based on field data
       Tailings
    –   Leach pads during cyanide addition
    –   Account for surface disturbance
    –   Account for surface age


•   3) Scale emissions: Flux (ng/m2/d) X surface area (m2) X days

•   4) Sum fluxes from each surface for all days of the year = total
    emissions

•   5) Sensitivity and Uncertainty analysis performed on the models
Annual Emission Estimates

Total nonpoint source (NPS) emissions kg/yr:
        Twin Creeks:    105 (range 60 to 121)
        Cortez-Pipeline: 19 (range 16 to 43)
tailings and active heap leach < 15% area at both mines released >75% of Hg

waste rock/reclaimed/inactive leach >85% area at both mines released <25% Hg

Total point source emissions kg/yr :
        Twin Creeks:      449
        Cortez-Pipeline: 94
         (Nevada Division of Environmental Protection data)




Total emissions point and NPS kg/yr:
    Twin Creeks: 554 (509 to 570); Cortez-Pipeline: 113 (110-137)
% of total mine emissions that are NPS:
        Twin Creeks: 19% (12 to 21%); Cortez-Pipeline: 17% (15 to 31%)

% increase in total mine emissions from NPS: Twin Creeks: 23% (13 to 27%)
Cortez-Pipeline: 20% (17 to 46%)
Annual Emission Estimates

  Total nonpoint source emissions kg/yr:
          Twin Creeks:     105
          Cortez-Pipeline: 19


 Emissions prior to mining kg/yr:
        Twin Creeks: 1.5
        Cortez:      0.25




 Projected emissions post mine reclamation

 Twin Creeks:       <8 kg/yr
 Cortez-Pipeline:   <3 kg/yr
Concluding remarks:
• Large differences in emissions between mines

• Emission estimate reflects one stage in the life of a mine
   – Emissions will vary depending on activity, age, and reclamation

• Factors important to consider:
      mercury concentration/host rock characteristics
      surface area of mining disturbed materials
      characteristics of tailings impoundments
      climatic conditions
      ore-processing techniques (i.e heap leaching)
      age of materials and reclamation
Questions?

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Fugitive Mercury Emissions from Nevada, USA Gold Mines

  • 1. Fugitive Mercury Emissions from Two Gold Mines in Nevada On November 20, 2009, Dr. Chris Eckley, a post doctoral researcher working with Dr. Mae Gustin presented a preview of his work and that by a graduate student, Matthieu Miller, on fugitive mercury emissions from two gold mines in Nevada (see the attached slides). The research focused on measuring mercury emissions from a variety of surfaces disturbed by mining activities at Newmont’s Twin Creeks Mine northeast of Winnemucca, Nev., and Cortez Pipeline, a Barrick property located south of Battle Mountain, Nev, and used this information to develop an estimate of emissions for the mine surface area. Fugitive emissions from waste rock, heap leaches, tailings impoundments, active pit surfaces, stockpiles and reclaimed sites were estimated and compared to mercury releases from sites undisturbed by mining. The results showed that mercury emissions from mining disturbances are approximately 20 percent of the total mercury emitted at these two gold mines. The study showed heap leaching and tailings impoundments produced the greatest emissions and that current reclamation practices can reduce the current emissions to near natural levels. Importantly, the work showed that the amount of mercury emitted from these types of disturbances can vary significantly among mines, depending primarily on the mercury concentration at the disturbed site, the moisture content of the tailings and whether or not the heaps are actively being leached with cyanide. Because there are a variety of factors (such as mercury concentration, age of the materials, climatic conditions, weather, ore type, ore processing techniques, etc.) that can affect the emission of fugitive mercury from different mining surfaces and the uncertainty associated with each of those factors, this data, developed for these two mines, cannot be extrapolated to come up with emissions estimates for other mines. Additionally since a mine is a dynamic entity with surfaces changing over time, and the emission estimates developed in the UNR study represent the surfaces present at
  • 2. the two mines s in 2008, the amount of Hg released in future years may differ depending on the types and extent of mining related surfaces at each facility. The data contained in the attached power point presentation have not been peer reviewed.
  • 3. Fugitive Mercury Emissions From Nevada, USA Gold Mines Eckley, CSa, Gustin, Ma, Miller, MBa, Marsik, Fb a University of Nevada Reno, Department of Natural Resources and Environmental Science b University of Michigan, Department of Atmospheric, Oceanic and Space Sciences
  • 4. Acknowledgements Nevada’s mining companies Fugitive Mercury Emissions Project Oversight committee Project Participation Note: Information presented has not be subjected to final scientific peer review
  • 5. Mercury (Hg) is a pollutant of global concern Hg emissions to air Transport and Transformation Mercury exposure through fish Methyl-Hg Numerous studies have identified Hg enriched soils are a source Hg to the air
  • 6. Project Context Mineral trends with high gold content The modern gold rush are often enriched in Mercury (Hg) NV Cinnabar (HgS) ~$1,000 oz Graphs from Nevada Bureau of Mines and Geology
  • 7. Nevada Gold mines contain point sources of Hg emissions: 2,000 kg/yr(NDEP 2006/2007) Point Source Emissions Hg Nonpoint source Hg emissions from Nevada Gold mines: ???? kg/yr
  • 8. Project Objectives: 1) Quantify nonpoint source Hg emissions from active gold mines 2) Quantify natural nonpoint source Hg emissions from adjacent undisturbed areas
  • 9. Introduction to Mine Processes Holes drilled and ore examined for grade and metallurgical properties Blast rock Based on gold content trucks deliver the ore to different processing locations Schematic pictures from Nevada Mining Association Brochure
  • 10. Schematic pictures from Nevada Mining Association Brochure Waste Rock/Overburden High grade ore Grinding Mill Low grade ore Sulfide Carbonaceous Oxide Tailings pond Heap Leach Pad Gold Collected on Activated Carbon
  • 11. Two mines chosen for study ¸ 0 1,500 m 0 1,000 m Twin Creeks Gold Mine Cortez Gold Mine
  • 12. Two mines chosen for study Different materials have Waste rock different surface areas that change over the life of a mine ¸ Heap Leach Tailings Old/Reclaimed 0 1,500 m 0 1,000 m Twin Creeks Gold Mine Cortez Gold Mine
  • 13. Undisturbed Areas: Similar rock types excavated at mines Twin Creeks Area Outcrops Cortez Area Hills Alluvium Valley Alluvium 0 3,000 m
  • 14. Method to measure emission: Outside air Inside chamber sample line sample line Tekran Total Gaseous Mercury Analyzer ng per m3 of air Dynamic Flux Chamber Flux = (Cinside-Coutside *(Q/A) Flux is emission or deposition per unit area per time Units ng (10-9g) per m2 per hour or ng per m2 per day
  • 15. Methods: General Research Approach 1) Identify important factors controlling flux using laboratory experiments • 48 tubs—3 from each surface type • Each tub: 24 hr fluxes twice per season • >400 diel flux measurements • Meteorological data collected on site Active Gold Mine UNR Greenhouse • Develop algorithms
  • 16. Methods: General Research Approach 1) Identify important factors controlling flux using laboratory experiments 2) Measure fluxes at the mines compare with laboratory derived data develop data for surfaces not represented in lab study Winter Spring ~ 1 week at each mine each season 24 hours sampled from each surface Day Night Summer Fall
  • 17. Methods: General Research Approach 1) Identify important factors controlling flux using laboratory experiments 2) Measure fluxes at the mines compare with laboratory derived data develop data for surfaces not represented in lab study 2 flux Winter chambers Spring 2 Tekrans ~ 1 week at each mine each season 24 hours sampled from each surface Day Night Summer Fall
  • 18. Methods: General Research Approach 1) Identify important factors controlling flux using laboratory experiments 2) Measure fluxes at the mines 3) Estimate emissions for each mine based on current surface areas and environmental conditions over the year of study Twin Creeks Cortez Pipeline Geographic Information System (GIS)
  • 19. Results: Laboratory Fluxes vary: Daily
  • 20. Results: Laboratory Fluxes vary: Daily Seasonally Leach (pre-cyanide)Twin Creeks mine (2.7 µg g-1)
  • 21. Results: Laboratory Fluxes influenced by: surface type, material Hg content Dry Wet 29000 Winter Spring Hg Flux (ng m-2 d-1) Summer Fall 19000 9000 -1000 0 3 6 9 12 15 18 21 24 27 30 33 36 39 42 45 48 Tub #
  • 22. Results: Laboratory Fluxes influenced by: surface type, material Hg content precipitation events—4-fold emission increase 600 Dry –November Dry Wet November, 10 2008 Wet—December 29000 Winter 500 December, 26 2008 Dry –January Spring January, 1 2009 400 Hg Flux (ng m-2 d-1) Summer Hg Flux (ng/m2/h) Fall 19000 300 200 9000 100 0 00:00:00 06:00:00 12:00:00 18:00:00 00:00:00 -1000 0 3 6 9 12 -100 18 15 21 24 27 30 Time of 36 33 Day 39 42 45 48 Tub #
  • 23. Results: Laboratory Use statistical analyses to determine most important variables and develop model equations Daily Hg Flux Hourly Hg Flux (between materials) (individual materials) Winter Spring 29000 Median Median Summer Parameter Fall T-statistic p-value T-statistic p-value Hg Flux (ng m-2 d-1) Substrate Hg 19000 15.2 <0.001 ----- ----- Substrate moisture 3.4 0.001 ----- ----- Solar radiation 9000 2.2 0.023 8.3 <0.001 Air temperature 3.3 0.001 2.8 <0.001 Relative Humidity 2.5 0.014 -0.3 <0.001 -1000 0 3 6 9 12 15 18 21 24 27 30 33 36 39 42 45 48 Wind speed 3.3 0.001 -0.2 <0.001 Tub #
  • 24. Results: Laboratory Develop equations that allows us to predict flux as a function of material Hg concentration and solar radiation Twin Creeks dry tub data Cortez-Pipeline dry tub data 10000 50000 low solar y = 110x + 373 r² = 0.25 9000 45000 low solar y = 71x + 568 r² = 0.71 8000 middle solar y = 338x - 132 r² = 0.66 40000 Hg Flux (ng m-2 d-1) middle solar y = 99x + 1335 r² = 0.50 Hg Flux (ng m-2 d-1) 7000 high solar y = 419x + 143 r² = 0.60 35000 high solar y = 507x + 985 r² = 0.77 6000 30000 5000 25000 20000 4000 15000 3000 10000 2000 5000 1000 0 0 0 20 40 60 80 0 5 10 15 Substrate Hg (µg g-1) Substrate Hg (µg g-1)
  • 25. Results: Laboratory simulation of surface disturbance Surface disturbance Increases flux 7-fold Effect of disturbance decreases over time 300 Hg Flux DFC Temp 100 (~ 7 days) Solar Radiation 250 80 Solar radiation (W m-2) 200 Hg Flux (ng m-2 h -1) Temperature (C) 60 150 40 100 50 20 0 0 0 1 2 3 4 5 6 7 8 Days following disturbance
  • 26. Field Measurements: -Characterize Hg concentrations in substrate -Collect data from field for comparison with laboratory data -Measure flux from surfaces not represented in laboratory study Active leach Reclaimed tailings Old leach pad Tailings material
  • 27. Results: Field data Characterization of Hg concentrations in substrate Twin Creeks Gold Mine Cortez-Pipeline Gold Mine
  • 28. Results: Surface area/concentration Characterization of Hg concentrations in substrate Twin Creeks Gold Mine Cortez-Pipeline Gold Mine Spatial Ave Substrate Hg: 5.9 µg/g Spatial Ave Substrate Hg: 1.3 µg/g Solid Hg (µg/g) 0 -12 12 - 24 24 - 36 36 - 48 48 - 60 60 - 72 72 - 84 84 - 96 96 - 108 108 - 120
  • 29. Results: Surface area/flux Spatial Variability of Hg fluxes Lowest Emissions: • Waste rock materials Surface Area (~10’s to 100’s ng m-2 d-1) Cortez Twin Cks Highest Emissions: • Active leach pads & tailings (~1,000’s to 100,000’s ng m-2 d-1)
  • 30. Comparison of field data with laboratory derived model >80% of field measurements were within the 95% prediction intervals of the laboratory data Twin Creeks Gold Mine Cortez-Pipeline Gold Mine 50000 10000 45000 high solar--lab y = 507x + 985 r² = 0.77 9000 high solar--lab 40000 y = 419x + 143 r² = 0.60 high solar--field 8000 Hg Flux (ng m-2 d-1) 35000 high solar--field Hg Flux (ng m-2 d-1) 7000 30000 6000 Tailings 25000 5000 20000 4000 15000 3000 10000 2000 5000 1000 Old leach 0 0 0 20 40 60 0 5 10 15 Substrate Hg (µg g-1) Substrate Hg (µg g-1)
  • 31. Comparison of field data with laboratory derived model Twin Creeks Gold Mine Cortez-Pipeline Gold Mine 50000 10000 45000 high solar--lab y = 507x + 985 r² = 0.77 9000 high solar--lab 40000 y = 419x + 143 r² = 0.60 high solar--field 8000 Hg Flux (ng m-2 d-1) 35000 high solar--field Hg Flux (ng m-2 d-1) 7000 30000 6000 Tailings 25000 5000 20000 4000 15000 3000 10000 2000 5000 1000 Old leach 0 0 0 20 40 60 0 5 10 15 Substrate Hg (µg g-1) Substrate Hg (µg g-1)
  • 32. Hg fluxes from tailings Heterogeneous Hg content (19 to 177 µg g-1), Moisture (0.1% to liquid solution) Flux (889 to 684,000 ng m-2 d-1). Magnitude of emissions best correlated with % moisture r 2 = 0.55 p=0.001 Twin Creeks
  • 33. Results: Cyanide Heap Leaching Hg fluxes from substrate actively under leach only obtained at Twin Creeks Typical Cortez leach Twin Creeks Leach
  • 34. Results: Cyanide Heap Leaching Twin Creeks Spring Data 12000 Pre leach: 2,280 ± 1,470 ng/m2/d Active CN Pre CN 10000 Post CN Active leach: 101,300 ± 53,400 8000 ng/m2/d Hg Flux (ng/m2/h) 6000 Post leach: 1,750 ± 572 ng/m2/d 4000 2000 0 0:00:00 6:00:00 12:00:00 18:00:00 0:00:00 -2000 Tim e of Day Pre CN 3 µg/g CN Addition 4 µg/g Post CN 5 µg/g
  • 35. Results: Cyanide Heap Leaching Daily Emissions increase ~4-fold from the effect of wetting alone Daily Emissions ~35-fold higher during leaching than from pre and post leaching Mean Hg Content of leach solution: 17 µg/L (Cortez) Nevada rainwater:0.002-0.4 µg/ L (Mercury Deposition Network Data Station: NV02, 2007 data) 470 µg/L (Twin Creeks) A component of Hg emitted during active leaching is from the cyanide solution
  • 36. Results: Material age/reclamation Emissions from capped tailings Twin Creeks (spring, 2008 data) Ave flux from tailings: 27,600 ng/m2/d Ave flux from capped tailings: 1,160 ng/m2/d Fluxes may be greatly reduced post-reclamation Data from 5 year old/inactive leach suggest fluxes decline as materials age
  • 37. Annual Emission Estimates • 1) Calculate fluxes – Use substrate Hg concentrations versus solar radiation relationship for dry and wet surfaces Make adjustments based on field data  Tailings – Leach pads during cyanide addition – Account for surface disturbance – Account for surface age • 3) Scale emissions: Flux (ng/m2/d) X surface area (m2) X days • 4) Sum fluxes from each surface for all days of the year = total emissions • 5) Sensitivity and Uncertainty analysis performed on the models
  • 38. Annual Emission Estimates Total nonpoint source (NPS) emissions kg/yr: Twin Creeks: 105 (range 60 to 121) Cortez-Pipeline: 19 (range 16 to 43) tailings and active heap leach < 15% area at both mines released >75% of Hg waste rock/reclaimed/inactive leach >85% area at both mines released <25% Hg Total point source emissions kg/yr : Twin Creeks: 449 Cortez-Pipeline: 94 (Nevada Division of Environmental Protection data) Total emissions point and NPS kg/yr: Twin Creeks: 554 (509 to 570); Cortez-Pipeline: 113 (110-137) % of total mine emissions that are NPS: Twin Creeks: 19% (12 to 21%); Cortez-Pipeline: 17% (15 to 31%) % increase in total mine emissions from NPS: Twin Creeks: 23% (13 to 27%) Cortez-Pipeline: 20% (17 to 46%)
  • 39. Annual Emission Estimates Total nonpoint source emissions kg/yr: Twin Creeks: 105 Cortez-Pipeline: 19 Emissions prior to mining kg/yr: Twin Creeks: 1.5 Cortez: 0.25 Projected emissions post mine reclamation Twin Creeks: <8 kg/yr Cortez-Pipeline: <3 kg/yr
  • 40. Concluding remarks: • Large differences in emissions between mines • Emission estimate reflects one stage in the life of a mine – Emissions will vary depending on activity, age, and reclamation • Factors important to consider: mercury concentration/host rock characteristics surface area of mining disturbed materials characteristics of tailings impoundments climatic conditions ore-processing techniques (i.e heap leaching) age of materials and reclamation