From Early Pendulum Experiments to Cutting-Edge Vibration Technology
The gravitational constant G is among the core pillars of physics. While the speed of light and the elementary charge are known with extraordinary precision, the exact value of G remains surprisingly uncertain even today—almost 350 years after Newton. Not surprisingly: Gravity is orders of magnitude weaker than any other fundamental force. Anyone wanting to measure G needs an experimental setup capable of the seemingly impossible—detecting movements smaller than the diameter of an atom, triggered by pure “action at a distance.”
The team around Jürg Dual at ETH Zurich has been taking on this challenge for years, using state-of-the-art laser measurement technology and ingenious experimental designs to set international benchmarks.
The First Step: Vibrating Beams as "Gravity Transmitters"
In a 2022 experiment, the team drew on a classic trick from vibration physics: resonance makes even very weak excitations measurable. In a spectacularly well-isolated laboratory deep in a Swiss mountain fortress, two metal beams about 1 meter long were mounted each within a vacuum chamber. One beam is set into precise vibration, “broadcasting” gravitational signals that act on the other, resonance-tuned beam in the adjacent chamber. The forces transmitted are minuscule—in the picometer range (a billionth of a millimeter)!
This is where laser interferometry comes in: Four highly precise laser vibrometers together with lock-in-amplifiers measured the tiniest trembling of the detector beam, filtering out noise and isolating true signals. The result: a value for G that is only slightly above the international reference—acquired with cutting-edge error analysis and clear potential for further refinement.
Strikingly, this dynamic method minimizes classical pitfalls, such as the influence of surrounding masses. For the first time, gravity’s effect can be directly examined not just “at rest” but in motion.
The Update: Rotating Bars as a Source of Oscillation (2023)
ETH Zurich did not stop there. In their most recent, 2023 study, the group took things a step further: Instead of linearly vibrating beams, the researchers used two slim, 0.5 m long, rotating tungsten rods arranged symmetrically opposite a bending beam resonance detector.
Through synchronized rotation, they generated a dynamic gravitational field that acted on the mechanically decoupled resonance detector beam. Once again: vacuum, meticulous isolation, and the utmost suppression of non-gravitational influences.
Again, state-of-the-art laser interferometry was used to measure the slight displacements of the resonator. The key: For maximum excitation of the detector bar, the rotation frequency of the excitation bars is precisely tuned to half or a quarter of the natural resonance frequency of the detector. If all parameters—rotational speed, alignment, temperature—fit perfectly, so does the measurement: The detector vibrates in remarkable agreement with predictions from classical gravity. The team systematically verified that no other interference could explain the effect—proving the genuinely gravitational origin of the observed signal.
Result: G = 6.6816 × 10−11m3kg−1s−2, with a combined standard uncertainty of about 1.46%. The estimation is about 0.1% higher than the CODATA 2018 value
This new method demonstrates: Even in a laboratory with macroscopic test bodies and at experimentally accessible frequencies (several hertz), it is possible to dynamically and interferometrically measure gravity and use it for resonance experiments—a true first in fundamental physics.
The Role of Laser Measurement Technology
None of these pioneering measurements would be possible without optical interferometry—in particular, the use of laser vibrometers. The sensitivity they offer reaches deep into the sub-nanometer range, enabling real-time detection of the tiniest amplitudes. Interferometry also allows for pinpoint rejection of unwanted signals, compensation for environmental effects, and automated data preparation.
The remaining technical challenges involve integrating additional environmental parameters and further minimizing residual noise. The ETH experiments impressively demonstrate that, for today’s precision and difference measurements, laser-based methods far outperform classical sensors.
Consequences and Outlook
Both experimental approaches push the boundaries of what is possible for direct laboratory measurement of the gravitational constant. They deliver robust data on the force that shapes stars, planets, and galaxies—and pave the way for even more precise gravitational sensors, geophysical applications, or even indirect gravitational wave detection.
For fundamental research, it is exciting to see what progress may come from even more advanced laser technology and data analysis methods. Soon, researchers may be able to significantly reduce the current uncertainties of G, or even find hints of new physics beyond the classical Newtonian model.
One thing is certain: Thanks to a blend of clever experimentation and laser measurement precision, we can now observe what was once considered unmeasurable. The quiet trembling of gravity becomes a loud message to the scientific community.
