A clock is only as accurate as its reference frequency—and as the experimenters’ accounting for everything that can shift it. At Singapore’s Centre for Quantum Technologies, Murray Barrett’s team developed a lutetium-ion optical clock whose reported fractional frequency uncertainty is near 1 × 10⁻¹⁹. Published in Nature on 23 September 2026, the result is described by the team as the most accurate yet reported for an optical atomic clock.
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How the team built the reference
The clock uses a single charged lutetium-176 ion. A laser probes an optical transition at 848 nanometres, providing the frequency reference for the clock. That fast optical oscillation offers a finely divided measure of time, but it does not guarantee accuracy: electromagnetic fields and thermal radiation can still change the frequency the experiment is trying to measure.
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Barrett’s group had been working toward this result for years. Its 2015 research plan identified hyperfine averaging as a way to make lutetium’s transition suitable for a clock. Rather than relying on one internal atomic state, the method combines measurements across related states so that some state-dependent shifts cancel. The group subsequently demonstrated hyperfine averaging using dynamic decoupling in a multi-ion lutetium clock.
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Other disturbances required separate attention. In 2019, the researchers measured and suppressed frequency differences among ions in a three-ion clock, including effects associated with electric quadrupole moments. Research on lutetium also examines shifts caused by thermal radiation and electric-field gradients. Those results help explain the development path; they should not be mistaken for a claim that lutetium is insensitive to every environmental change.
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What the two record figures measure
The approximately 1 × 10⁻¹⁹ figure describes reported fractional frequency uncertainty for the clock reference. The team also compared two independently built single-ion clocks, reporting a comparison uncertainty of 5.7 × 10⁻¹⁹. The comparison checks whether the references agree; its larger uncertainty is not a second way of stating the individual clock’s accuracy.
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The group has used correlation spectroscopy to compare lutetium frequency references. By reducing the effect of interrogation-laser noise on a comparison, the technique makes a small difference between clocks easier to resolve. It does not, on its own, rule out a systematic shift shared by both clocks. A 200-hour comparison is described in the question’s account of the result, but the supplied source excerpts do not independently establish that duration or its full uncertainty budget.
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The familiar claim that the clock would gain or lose less than a second over 260 billion years is an illustration, not an observation made over that span. At a constant fractional error of 1 × 10⁻¹⁹, the arithmetic gives roughly one second in 317 billion years; at 1.2 × 10⁻¹⁹, it gives roughly 264 billion years. Reports use both uncertainty figures, so the analogy depends on which is meant.
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Why the result matters—and what remains
A more accurate optical reference could contribute to a future redefinition of the second, but a result from one laboratory cannot alone establish reproducibility across laboratories or determine which atomic transition should become the standard. The supplied evidence does not confirm a formal timetable for such a change.
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Accuracy at this scale also makes location part of the measurement. Near Earth’s surface, the gravitational frequency shift across a one-millimetre height difference is roughly 1.1 × 10⁻¹⁹. Comparing clocks at different sites therefore requires knowledge of their gravitational-potential difference, not just confidence in the clocks themselves. Making a transportable version poses another test: it would have to retain control of the ion, laser and environmental shifts—and demonstrate its uncertainty again after moving.
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