The Samarium-Neodymium (Sm-Nd) system is a powerful tool in isotope geochemistry for dating rocks and understanding Earth's evolution. It uses the radioactive decay of 147Sm to 143Nd to determine ages and trace geological processes over billions of years.
This system provides crucial insights into crustal formation, mantle differentiation , and planetary evolution. The long half-life of 147Sm makes it ideal for dating ancient rocks, while its resistance to disturbance during geological processes ensures reliable results.
Sm-Nd system overview
Samarium-Neodymium (Sm-Nd) system serves as a powerful tool in isotope geochemistry for dating rocks and understanding Earth's evolution
Utilizes the radioactive decay of 147Sm to 143Nd to determine ages and trace geological processes
Provides insights into crustal formation, mantle differentiation, and planetary evolution over billions of years
Isotopes of Sm and Nd
Naturally occurring isotopes
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Samarium consists of seven naturally occurring isotopes (144Sm, 147Sm, 148Sm, 149Sm, 150Sm, 152Sm, 154Sm)
Neodymium comprises seven stable isotopes (142Nd, 143Nd, 144Nd, 145Nd, 146Nd, 148Nd, 150Nd)
147Sm decays to 143Nd through alpha decay, forming the basis of the Sm-Nd dating system
Relative abundances of these isotopes vary slightly due to radioactive decay and fractionation processes
Radioactive decay process
147Sm undergoes alpha decay to produce 143Nd
Decay equation 143 N d = 143 N d 0 + 147 S m ( e λ t − 1 ) ^{143}Nd = ^{143}Nd_0 + ^{147}Sm(e^{\lambda t} - 1) 143 N d = 143 N d 0 + 147 S m ( e λ t − 1 )
Decay constant (λ) of 147Sm equals 6.54 × 10^-12 yr^-1
Alpha particle emission changes the atomic number from 62 (Sm) to 60 (Nd)
Process occurs over billions of years due to the long half-life of 147Sm
Sm-Nd dating principles
Half-life of 147Sm
147Sm has a half-life of approximately 106 billion years
Long half-life makes the Sm-Nd system suitable for dating very old rocks and minerals
Allows for accurate age determinations of early Earth and planetary materials
Decay rate remains constant regardless of temperature, pressure, or chemical environment
Isochron method
Plots 143Nd/144Nd ratio against 147Sm/144Nd ratio for multiple cogenetic samples
Slope of the isochron line determines the age of the rock or mineral suite
Y-intercept provides the initial 143Nd/144Nd ratio at the time of formation
Requires samples with varying Sm/Nd ratios but identical initial Nd isotopic compositions
Equation for the isochron ( 143 N d 144 N d ) m = ( 143 N d 144 N d ) i + ( 147 S m 144 N d ) m ( e λ t − 1 ) (\frac{^{143}Nd}{^{144}Nd})_m = (\frac{^{143}Nd}{^{144}Nd})_i + (\frac{^{147}Sm}{^{144}Nd})_m(e^{\lambda t} - 1) ( 144 N d 143 N d ) m = ( 144 N d 143 N d ) i + ( 144 N d 147 S m ) m ( e λ t − 1 )
Geochemical behavior of Sm-Nd
Fractionation during melting
Sm and Nd behave similarly during most geological processes due to their similar ionic radii and charge
Slight fractionation occurs during partial melting of the mantle
Nd preferentially enters the melt phase compared to Sm
Results in lower Sm/Nd ratios in crustal rocks compared to the mantle
Fractionation factor between Sm and Nd typically ranges from 1.1 to 1.3
Compatibility in minerals
Both Sm and Nd are incompatible elements in most rock-forming minerals
Preferentially concentrate in the liquid phase during magmatic processes
Garnet strongly partitions Sm relative to Nd, leading to higher Sm/Nd ratios
Plagioclase slightly favors Nd over Sm, resulting in lower Sm/Nd ratios
Clinopyroxene and amphibole show minimal fractionation between Sm and Nd
Sm-Nd in crustal evolution
CHUR model
CHUR stands for Chondritic Uniform Reservoir
Represents the bulk Earth composition based on chondritic meteorites
Serves as a reference for comparing Nd isotopic compositions of rocks
CHUR evolution line describes the change in 143Nd/144Nd ratio over time for bulk Earth
Equation for CHUR ( 143 N d 144 N d ) C H U R = 0.512638 − 0.1967 × ( 147 S m 144 N d ) C H U R × ( e λ t − 1 ) (\frac{^{143}Nd}{^{144}Nd})_{CHUR} = 0.512638 - 0.1967 \times (\frac{^{147}Sm}{^{144}Nd})_{CHUR} \times (e^{\lambda t} - 1) ( 144 N d 143 N d ) C H U R = 0.512638 − 0.1967 × ( 144 N d 147 S m ) C H U R × ( e λ t − 1 )
Depleted mantle model
Represents the evolution of the upper mantle after extraction of continental crust
Characterized by higher Sm/Nd ratios compared to CHUR
Results in more radiogenic Nd isotopic compositions over time
Used to calculate model ages for crustal rocks
Depleted mantle evolution line lies above the CHUR line on Nd isotope diagrams
Epsilon Nd notation
Calculation and interpretation
Expresses the deviation of a sample's 143Nd/144Nd ratio from CHUR
Calculated using the formula ϵ N d = [ ( 143 N d 144 N d ) s a m p l e / ( 143 N d 144 N d ) C H U R − 1 ] × 1 0 4 \epsilon Nd = [(\frac{^{143}Nd}{^{144}Nd})_{sample} / (\frac{^{143}Nd}{^{144}Nd})_{CHUR} - 1] \times 10^4 ϵ N d = [( 144 N d 143 N d ) s am pl e / ( 144 N d 143 N d ) C H U R − 1 ] × 1 0 4
Positive εNd values indicate derivation from a depleted mantle source
Negative εNd values suggest incorporation of older crustal material
εNd = 0 represents a composition identical to CHUR
Temporal variations
εNd values change over time due to radioactive decay and crustal evolution
Present-day εNd values differ from initial εNd values at the time of rock formation
Crustal rocks generally evolve towards more negative εNd values over time
Mantle-derived rocks tend to develop more positive εNd values with age
Plotting εNd vs. time reveals trends in crustal growth and recycling
Applications in geochronology
Igneous rock dating
Determines crystallization ages of igneous rocks and minerals
Particularly useful for dating mafic and ultramafic rocks poor in other datable minerals
Applies to a wide range of igneous rock types (basalts, granites, pegmatites)
Provides insights into magma source characteristics and crustal contamination
Often combined with other isotope systems for cross-validation (U-Pb, Rb-Sr)
Dates metamorphic events by analyzing newly formed or recrystallized minerals
Garnet commonly used due to its high closure temperature for the Sm-Nd system
Helps constrain timing of high-grade metamorphism and crustal evolution
Can reveal multiple metamorphic events in polymetamorphic terranes
Useful for dating eclogites and other high-pressure metamorphic rocks
Sm-Nd in provenance studies
Sedimentary rock analysis
Determines the source areas of sedimentary rocks and sediments
Utilizes the fact that Sm-Nd ratios remain relatively unchanged during weathering and transport
Compares Nd isotopic compositions of sediments to potential source rocks
Helps reconstruct paleogeography and sediment transport pathways
Useful in petroleum geology for understanding basin evolution and sediment routing
Crustal residence time
Calculates the time since extraction of crustal material from the mantle
Uses the depleted mantle model to estimate Nd model ages
Provides insights into the age and evolution of continental crust
Helps distinguish between juvenile and recycled crustal components
Equation for Nd model age T D M = 1 λ ln [ 1 + ( 143 N d 144 N d ) s a m p l e − ( 143 N d 144 N d ) D M ( 147 S m 144 N d ) s a m p l e − ( 147 S m 144 N d ) D M ] T_{DM} = \frac{1}{\lambda} \ln[1 + \frac{(\frac{^{143}Nd}{^{144}Nd})_{sample} - (\frac{^{143}Nd}{^{144}Nd})_{DM}}{(\frac{^{147}Sm}{^{144}Nd})_{sample} - (\frac{^{147}Sm}{^{144}Nd})_{DM}}] T D M = λ 1 ln [ 1 + ( 144 N d 147 S m ) s am pl e − ( 144 N d 147 S m ) D M ( 144 N d 143 N d ) s am pl e − ( 144 N d 143 N d ) D M ]
Analytical techniques
Mass spectrometry methods
Thermal Ionization Mass Spectrometry (TIMS) provides high-precision Nd isotope measurements
Multicollector Inductively Coupled Plasma Mass Spectrometry (MC-ICP-MS) offers rapid analysis with good precision
Laser Ablation ICP-MS allows for in-situ analysis of minerals with spatial resolution
Secondary Ion Mass Spectrometry (SIMS) enables microanalysis of Sm and Nd isotopes in small sample volumes
Isotope dilution techniques used to accurately determine Sm and Nd concentrations
Sample preparation
Involves careful mineral separation and purification to avoid contamination
Acid digestion of rock samples using HF, HNO3, and HCl
Ion exchange chromatography to separate Sm and Nd from other elements
Ultra-clean laboratory conditions required to minimize blank contributions
Spike addition for isotope dilution analysis to determine elemental concentrations
Limitations and challenges
Analytical precision
Precision limited by low abundance of 147Sm and slow decay rate
Requires large sample sizes for high-precision measurements using TIMS
Interferences from isobaric nuclides (142Ce, 144Sm) must be carefully corrected
Matrix effects in ICP-MS can affect accuracy and precision of measurements
Long counting times often necessary to achieve desired precision levels
Geological complexities
Open-system behavior can disturb the Sm-Nd system, leading to inaccurate ages
Metamorphism may cause partial resetting of the isotope system
Mixing of different source components can complicate interpretation of Nd isotope data
Inherited components in igneous rocks can affect the accuracy of crystallization ages
Crustal contamination of mantle-derived magmas can obscure primary isotopic signatures
Sm-Nd vs other isotope systems
Rb-Sr system comparison
Rb-Sr system has a shorter half-life (48.8 billion years) compared to Sm-Nd
Rb and Sr more susceptible to disturbance during metamorphism and alteration
Sm-Nd system generally more robust for dating older rocks and high-grade metamorphic events
Rb-Sr better suited for dating low-temperature processes and some sedimentary rocks
Combined use of Sm-Nd and Rb-Sr can provide complementary information on petrogenesis
Lu-Hf system comparison
Lu-Hf system has a similar half-life (37.1 billion years) to Sm-Nd
Both systems behave similarly during mantle melting and crustal processes
Lu-Hf system more sensitive to garnet fractionation in the source region
Hf isotopes can be measured in-situ on zircons, providing additional geochronological information
Combining Sm-Nd and Lu-Hf data enhances understanding of mantle evolution and crustal growth
Case studies in Sm-Nd dating
Planetary materials
Sm-Nd dating of lunar rocks constrains the age of the Moon and its magmatic history
Analysis of Martian meteorites provides insights into the geological evolution of Mars
Dating of chondritic meteorites helps determine the age of the solar system
Sm-Nd systematics in differentiated meteorites reveal early planetary differentiation processes
Studies of calcium-aluminum-rich inclusions (CAIs) constrain the earliest stages of solar system formation
Ancient crustal fragments
Sm-Nd dating of Acasta Gneiss Complex in Canada confirms its age as one of the oldest known crustal rocks (>4.0 Ga)
Analysis of Jack Hills zircons from Australia provides evidence for early crustal formation on Earth
Sm-Nd studies of Archean greenstone belts reveal the nature of early crustal growth and mantle evolution
Dating of ancient metamorphic terranes helps reconstruct the assembly and evolution of early continents
Sm-Nd isotope mapping of cratons provides insights into the architecture and growth of continental nuclei