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Stable Isotope Basics |

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Introduction
All matter is composed of atoms. Atoms occur as
various nuclides depending on their nuclear structure. Nuclides are
composed of protons (+ charge) and neutrons (no
charge) in the nucleus, and electrons (- charge) in outer
“shells” surrounding the nucleus. For a given nuclide, the number of
protons (Z) defines element, and the number of neutrons (N)
determines which isotope is present (the word isotope is derived
from the Greek words, isos meaning equal, and topos
meaning place). For a given nuclide, the sum of its protons and
neutrons gives the atomic weight (A), expressed using the notation
AZNuN. For example, the most common
isotope of the element oxygen (O) contains 8 protons and 8 neutrons,
and has an atomic weight of 16. Thus, it is expressed as 168O8.
A less common oxygen isotope, containing 8 protons and 10 neutrons,
and having an atomic weight of 18, is expressed as 188O10.
To simplify the expressions, conventional notation uses only the
elemental symbol and atomic weight (e.g 16O or 18O).
The number of neutrons can vary, and the number in the nuclide
determines which isotope of the nuclide is present, but the range of
that variance is limited by the degree of instability resulting from
having too few, or too many neutrons present in the nucleus.
Isotopes can thus be unstable (radioactive) or stable in nature.
Radioactive isotopes will disintegrate spontaneously by some mode of
decay to become stable. Stable isotopes do not undergo decay. The
decay rate of a given radioactive isotope is expressed in terms of a
half-life, which represents the amount of time necessary for ½ the
amount of the isotope to decay.
Stable Isotopes in Hydrologic
Studies
A number of stable isotopes are used in hydrologic studies, and have
been termed “environmental isotopes”. These include oxygen-18 (18O),
deuterium (2H), carbon-13 (13C), chlorine-37 (37Cl),
sulfur-34 (34S), and nitrogen-15 (15N), for
example. Stable isotopes are typically used to identify the source
(origin) of the waters, or their dissolved constituents and any
physical, chemical and biological processes which may have impacted
the waters since their origin. Stable oxygen and deuterium
isotopes are typically used to trace water movement within the
hydrologic cycle. Thus, know in the isotope composition of
precipitation is important and is often viewed as the "starting
point" on a parcel of waters journey throughout the water cycle.
Oxygen-18 and Deuterium
Stable isotopes are measured as the ratio of the two most abundant
isotopic forms of the element. For oxygen, it is the ratio of
18O, with an abundance of 0.204%, to 16O (the more
common form), with an abundance of 99.796%. Thus, the 18O/16O
ratio is about 0.00204. For hydrogen, it is the ratio of 2H
(also written as “D”- deuterium), with an abundance of 0.015%, to
the more common form, 1H (protium), with an abundance of
99.985%, giving a 2H/1H ratio of about
0.000150.
Stable Isotope Notation
Stable isotope concentrations are expressed as the difference
between the measured ratio of the sample and the measured ratio of a
reference standard. Isotope results are reported as parts per
thousand (‰) with respect to the standard using the (d)
notation expressed as,
dsample
= { (Rsample - Rstandard) / (Rstandard)
} X 1000
where, Rsample is the ratio of 18O/16O
or 2H/1H, for example in the sample and
Rstandard is the ratio of the international standard for oxygen and
hydrogen, VSMOW (Vienna Standard Mean Ocean Water). The analytical
precision for d18O
and d2H
are 0.2 and 2.0 ‰, respectively. Other stable isotopes will have a
different reference standard and different analytical precision, but
their ratios can be expressed in the same manner.
When using the delta notation, seawater will have a
d18O value
of 0‰. Thus, waters which have negative d18O
(and d2H
as well) values (such as is typical with precipitation, or
groundwater samples) are said to be depleted relative to
seawater, and those with positive d
values are said to be enriched. These terms can also be used
to describe two isotope compositions relative to each other. For
example, a precipitation sample which has a
d18O of
-25‰ is said to be depleted relative to a precipitation sample with
a d18O
of -11‰. Likewise, a groundwater with a d18O
of -5‰ is said to be enriched relative to a groundwater that has a
d18O
of -12‰. Within the literature, the terms heavy and light
may also be used interchangeably with enriched and depleted when
referring stable isotope d18O
and d2H
values. For example, a precipitation sample with a
d18O value
of -25‰ is said to be isotopically lighter (or simply light)
when compared to a precipitation sample having a
d18O of
-8‰. A surface water sample with a d18O
value of -5‰ is considered isotopically heavier (or simply
heavy) when compared to a groundwater sample with a
d18O value
of -10‰. A simple rule to follow with regard to the terminology is -
“the more negative the value...the lighter or more depleted it is,
the more positive the value...the heavier or more enriched the
sample is said to be."
Oxygen/Hydrogen Isotope Relationships
A plot of d18O
vs d2H
can be used to determine examine the seasonal variations in the
composition of precipitation (as a function of temperature) and to
identify subsequent modification of the waters composition by
various processes. The d18O
and d2H
values of global precipitation generally plot close to a straight
line, called the global meteoric water line, GMWL (Craig, 1961). The
equation of this line is d2H
= 8 X d18O
+ 10. Local meteoric water lines also exist, having slightly
different slopes and intercepts than the GMWL, as a result of
differences in altitude, local climate and distance from the
moisture source. The location of the long-term stable isotope
precipitation record is Chicago, Illinois (IAEA, 1992). Recently,
local meteoric water lines were determined for Mead (Harvey, 2001)
and North Platte (Harvey and Welker, 2000), Nebraska and the Pawnee
National Grasslands, Colorado (Harvey, 2005) using archived
precipitation data made available by the National Atmospheric
Deposition Project (NADP). If groundwater
d18O and
d2H
values plot near the present precipitation water line for the
sampling area, the waters are likely meteoric in origin, that is to
say, derived from precipitation without subsequent modification. If
they do not plot along this line, they have been impacted by some
physical or chemical process prior to recharge, or during the
groundwater's journey through the aquifer.
Once a water is “formed” as meteoric, a number of processes
may alter the water’s signature (the combined
d18O
and d2H
values) as a result of differences in the degree to which the
various isotope participate in physical and chemical processes, or
due to the different rates of interaction of each isotope, which
result from differences in mass and/or molecular size (referred to
as isotopic fractionation). The figure at the right illustrates the
effect of such processes on a meteoric water. The process most
relevant to hydrological studies is evaporation. As a water
evaporates from an open surface (river, lake or irrigated field) its
signature moves away from the meteoric water line along a line
having a slope of between two and about five (depending on the
effect of humidity). This shift off the line occurs due to the
difference in the vapor pressures of H218O and
2HHO, which imparts disproportional enrichments in the
water phase during evaporation (Clark and Fritz, 1997). For a given
water, the greater the degree of evaporation, the farther from the
water line the resulting signature will be. Rivers and lakes
typically undergo greater evaporation than groundwaters and thus,
generally plot off the water line along an evaporation line.
However, if a groundwater plots off the line, along an evaporation
line, one of two possibilities can be concluded: (a) the
groundwaters have been impacted by evaporation prior to recharge
(water reaching the saturated zone), or (b) the groundwater
represents a mixture of two “end member” waters; one of meteoric
origin (plotting on the water line), and one having undergone
evaporation (a river, lake or wetland for example, plotting off the
line).
References:
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Clark, I. & P.
Fritz, 1997, Environmental Isotopes in Hydrogeology, Lewis
Publishers, CRC Press, 328 p.
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Craig, H, 1961,
Isotopic variations in meteoric waters, Science 133, pg 1702.
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Harvey, F.E., 2005, Stable Hydrogen and Oxygen Isotope
Composition of Precipitation in Northeastern Colorado, Journal of
the American Water Resources Association, 41(2), p. 447-459.
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Harvey, F.E., 2001, Use of NADP Archive Samples to Determine the
Isotope Composition of Precipitation: Characterizing the Meteoric
Input Function for Use in Ground Water Studies,
Ground Water, 39(3),
p. 380-390.
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Harvey, F.E. and J. M. Welker, 2000, Stable Isotopic Composition of
Precipitation in the Semi-Arid North-Central Portion of the U.S.
Great Plains, Journal of Hydrology, 238(1-2), p. 90-109.
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Copyright 2009 - F. Edwin Harvey, University of Nebraska - All Rights
Reserved
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