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Understanding Ultra-Low Frequency Oscillations

The picohertz (pHz) is a unit of frequency equal to 10⁻¹² hertz, which means one cycle occurs every trillion seconds, or roughly 31,700 years. Picohertz frequencies are incredibly low and are mainly relevant in fields like astrophysics, geophysics, and cosmology, where processes unfold over extremely long timescales.

At picohertz frequencies, waves have extraordinarily long wavelengths, spanning millions to billions of kilometres. Such ultra-low frequencies are associated with phenomena like gravitational waves from massive cosmic events, large-scale oscillations of the Earth’s magnetic field, and long-term climate or geological cycles. Understanding picohertz frequencies allows scientists to study the slowest and largest-scale dynamics of our universe and planet.

Although picohertz frequencies are far beyond human perception and everyday technology, they provide valuable insight into the underlying processes shaping galaxies, solar systems, and Earth’s internal behavior over millennia. Research in this frequency range deepens our knowledge of cosmic evolution, gravitational physics, and Earth sciences.

Using picohertz as a measurement unit helps bridge the gap between familiar time scales and the vast expanses of time and space that govern the natural world at its grandest scale.

The Scale of Interstellar and Cosmological Waves

A petametre (Pm) equals 1,000 terametres (10¹⁵ metres), representing unimaginably vast distances that describe the longest electromagnetic wavelengths in the universe. These wavelengths correspond to frequencies in the attohertz (10⁻¹⁸ Hz) and lower ranges, which are mostly relevant in cosmology, astrophysics, and the study of gravitational waves and large-scale cosmic phenomena.

For context, a frequency of 1 attohertz (10⁻¹⁸ Hz) corresponds to a wavelength of approximately 300 petametres. This scale is far beyond any human-made signals and reflects waves that stretch across entire galaxies or even clusters of galaxies. Such waves help scientists study the cosmic microwave background (CMB) fluctuations, the large-scale structure of the universe, and primordial gravitational waves created shortly after the Big Bang.

Using petametres to measure wavelength allows researchers to grasp the vastness of these cosmic oscillations and the slowest processes influencing the universe’s evolution. These extreme wavelengths provide crucial insight into the origins, expansion, and ultimate fate of the cosmos.