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reserves (lower bound), for the following mineral commodities: mercury (1960), ar-
senic (1971), tin (1979), lead (1989), gold (1994), silver (1995), cadmium (1996),
antimony (1998), zinc (1999), zirconium (2003), manganese (2007), wolfram (2007)
and copper (2012). Considering world resources (upper bound), the peak might
have been reached for mercury (1965), tin (1986), silver (1999), gold (2001), anti-
mony (2006) and zirconium (2006). From the latter minerals, silver, antimony and
zirconium haven't really reached a real production peak. Indeed, it should be stated
that for silver and antimony, no world resources data are currently available and
that their theoretical peaks have been obtained through reserve base data (of 2006).
Furthermore, silver and zirconium are extracted as byproducts from other major
ones and antimony has associated with it environmental and supply concentration
problems, hence why Hubbert theory may not apply. Figs. 13.36 through 13.45
show a selection of the curves studied.
x 10 4
4
8000
3.5
7000
3
2001
6000
2.5
5000
1960
2
4000
1.5
3000
2000
1
1000
0.5
0
0
1900
1950
2000
2050
1900 1920 1940 1960 1980 2000 2020 2040 2060 2080 2100
(a) Gold
(b) Mercury
Fig. 13.36 The Hubbert Peak applied to the gold reserve base (a) and mercury reserves (b). Data
obtained from USGS (2010)
2500
4000
3500
2000
3000
1999
2500
1500
2006
2000
1000
1500
1000
500
500
0
0
1900 1920 1940 1960 1980 2000 2020 2040 2060 2080 2100
1900 1920 1940 1960 1980 2000 2020 2040 2060 2080 2100
(a) Silver
(b) Antimony
Fig. 13.37 The Hubbert Peak applied to silver (a) and antimony (b) reserve base. Data obtained
from USGS (2010)
 
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