Gravity's strength measured more reliably than ever before
Scientists have achieved the most precise measurement yet of the gravitational constant, known as "big G," a fundamental value that quantifies the strength of gravity. The experiment, led by Stephan Schlamminger and his team at the US National Institute of Standards and Technology, involved a highly refined torsion balance apparatus with eight carefully calibrated weights suspended by a human hair. This setup allowed researchers to isolate and measure the minute gravitational attraction between masses with unprecedented accuracy, overcoming challenges that have plagued previous attempts for centuries. Gravity is notoriously difficult to measure because it is far weaker than other fundamental forces and cannot be shielded in experiments. The torsion balance method, first used by Henry Cavendish in 1798, remains the most effective approach to isolating gravitational effects from Earth's dominant pull. Schlamminger’s team spent over a decade meticulously identifying and minimizing sources of error, producing a value for big G of 6.67387×10⁻¹¹ m³/kg/s². This result is slightly lower than the value obtained in a similar 2007 French experiment but is considered the most reliable to date due to the extraordinary precision and comprehensive error analysis. The significance of this measurement lies in its potential to resolve longstanding discrepancies among previous experiments, which have yielded inconsistent values for big G. Such inconsistencies have raised questions about whether unknown physics or experimental flaws were at play. While the new result does not fundamentally alter our understanding of gravity, it represents a major step toward consensus and improved accuracy in fundamental physics. Experts not involved in the study have praised the work as a "game-changer," highlighting the level of care and innovation that went into the experiment. Accurate knowledge of the gravitational constant is crucial for a wide range of scientific fields, from cosmology to geophysics, as it underpins calculations involving planetary motion, black holes, and the structure of the universe. This breakthrough measurement may enable more precise tests of gravitational theories and help refine models that describe the fundamental forces shaping our cosmos.
Original story by New Scientist • View original source
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