SHRIMP/SIMS
High-Resolution Geochronology with SHRIMP & SIMS
What are SHRIMP & SIMS?
The Sensitive High-Resolution Ion Microprobe (SHRIMP) and Secondary Ion Mass Spectrometry (SIMS) are powerful techniques used for in situ isotopic and elemental analysis, particularly in U-Pb geochronology, light isotopes and trace element studies. These methods allow researchers to analyse mineral domains at a micrometer-scale resolution, providing precise age determinations and geochemical insights into Earth’s history.
Secondary Ion Mass Spectrometry, or SIMS, is a powerful technique for analyzing the composition of solid surfaces at high spatial resolution.

It operates by sputtering a sample with a focused primary ion beam, causing the release of secondary ions that are then analyzed to determine elemental and isotopic compositions.
The concept of ion sputtering dates back to the 1940s–1950s, laying the foundation for modern SIMS applications in geochemistry, materials science, and microanalysis.
This is fundamentally different from laser ablation ICP-MS, which does not ionise the particle during lasing; the particles get ionized inside the spectrometer, within the plasma torch…
Let’s take a closer look at how this process works and its significance in geochronology.”
History

The development of SIMS as a high-resolution analytical tool can be traced back to the pioneering work of Castaing and Slodzian in 1962. They introduced the concept of an ion microprobe for localized micro-scale analysis.
Their seminal work, published in French, initially limited its accessibility to the broader scientific community. It wasn’t until 1967 that the first commercial SIMS instrument was built by Cameca, revolutionizing surface chemistry analysis with high spatial resolution.
Interestingly, while SIMS quickly gained traction in materials science, its application in geology took longer to develop. Let’s explore how this breakthrough paved the way for modern geochemical studies.

The next major leap in SIMS technology was in situ geochronology, which came with the development of SHRIMP. While early SIMS instruments were primarily used in materials science, their potential for U-Pb zircon dating was recognized in the 1970s by Bill Compton and colleagues.
This led to the creation of the first SHRIMP instrument in 1978 by William Compston and the ANU group.
SHRIMP introduced a large-radius electrostatic-magnetic sector and a high-intensity oxygen ion beam, enabling precise U-Pb dating of single zircon domains without extensive chemical digestion.
This innovation made SHRIMP a cornerstone of modern geochronology, allowing researchers to directly date minerals with high spatial resolution and improved accuracy.

Before we start – we just need to make clear that both SHRIMP and SIMS operate under the same principles and produce nearly identical datasets.
How Does SIMS Work?
Secondary Ion Mass Spectrometry (SIMS) operates by bombarding a sample with a focused primary ion beam (e.g., O²⁻ or Cs⁺), which causes the ejection of secondary ions from the sample surface. These ejected ions are then analyzed in a mass spectrometer, allowing the measurement of isotopic ratios and elemental compositions with high sensitivity.
Key Steps in SIMS Analysis
- Primary Ion Beam Generation – A finely focused ion beam (e.g., oxygen or cesium) is directed onto the sample.
- Sputtering Process – The interaction between the ion beam and the sample surface releases secondary ions.
- Mass Spectrometry – The secondary ions are separated and analyzed based on their mass-to-charge ratio (m/z).
- Data Interpretation – Isotopic compositions and elemental abundances are quantified for geological dating and geochemical fingerprinting.
SIMS is particularly useful for studying small-scale variations in minerals, making it ideal for zoned crystals, REE-rich minerals, and low-concentration isotopic studies.

The image illustrates the internal structure and ion optics of the Sensitive High-Resolution Ion Microprobe (SHRIMP), a specialized SIMS instrument designed for precise U-Pb geochronology and isotopic analysis.
- Primary Ion Column: A focused primary ion beam (e.g., O₂⁻ or Cs⁺) bombards the sample, sputtering secondary ions.
- Source Chamber: The sputtered secondary ions are extracted and accelerated into the mass spectrometer.
- Magnetic Sector Analyzer: The ion beam is separated based on mass-to-charge ratio (m/z) using a high-resolution magnet.
- Electrostatic Analyzer (ESA): Further refines the mass separation by filtering ions based on their energy, improving precision.
- Collector System: The selected isotopes are measured in the detector array, providing high-accuracy age determinations.
The SHRIMP system enables in situ isotopic analysis of individual zircon, monazite, and other U-bearing minerals, allowing for high-resolution dating of geological materials while preserving spatial context.
The SHRIMP Advantage
The Sensitive High-Resolution Ion Microprobe (SHRIMP) is a specialized SIMS instrument designed specifically for U-Pb geochronology. It uses a large-radius electrostatic-magnetic sector analyzer, allowing for precise age determination of accessory minerals like zircon, monazite, titanite, and baddeleyite.
Why Use SHRIMP?
- High spatial resolution – Enables in situ analysis of mineral domains as small as 10–30 µm.
- Minimal sample destruction – No need for bulk chemical dissolution, preserving the sample structure.
- High mass resolution – Effectively separates Pb isotopes from molecular interferences.
- Fast U-Pb dating – Provides direct zircon age determinations without extensive chemical processing.
Applications of SHRIMP Geochronology
- Dating igneous and metamorphic rocks to reconstruct geological histories.
- Analyzing detrital zircons for provenance studies in sedimentary geology.
- Understanding planetary processes through isotope studies of meteorites and lunar samples.
- Tracking crustal evolution by studying isotopic inheritance and overgrowths in minerals.
Data Reduction & Interpretation
The data obtained from SIMS and SHRIMP require careful corrections and calibrations to ensure accuracy:
- Background subtraction – Corrects for detector noise and instrumental signals.
- Interference corrections – Adjusts for molecular interferences affecting Pb isotopes.
- Fractionation correction – Accounts for instrumental biases in U/Pb ratios.
- Normalization – Uses reference materials (e.g., zircon standards) to calibrate age determinations.
- Error propagation analysis – Evaluate analytical uncertainties to enhance precision.
These steps ensure high-accuracy age models, typically visualized using Concordia diagrams and probability density plots.