Convert exahertz [EHz] to wavelength in petametres Online | Free frequency-wavelength Converter

The Realm of Ultra-High Frequency Electromagnetic Waves

The exahertz (EHz) is a unit of frequency equal to 1 quintillion hertz (10¹⁸ Hz), representing one quintillion cycles per second. This extremely high frequency lies deep within the gamma-ray region of the electromagnetic spectrum, associated with some of the most energetic processes in the universe.

Exahertz frequencies correspond to electromagnetic waves with extremely short wavelengths—on the order of picometers or smaller—which are produced by nuclear reactions, cosmic rays, and other high-energy astrophysical phenomena. Gamma rays at these frequencies are emitted by events like supernovae, neutron star collisions, and active galactic nuclei.

Due to their immense energy, exahertz waves can penetrate matter deeply and are used in applications such as cancer radiation therapy and high-energy physics experiments. However, generating and detecting such frequencies on Earth remains highly challenging, requiring advanced particle accelerators and specialized detectors.

Studying exahertz frequencies helps scientists explore fundamental physics, including particle interactions, quantum mechanics, and the conditions of the early universe. These investigations provide insights into the nature of matter, energy, and the forces governing the cosmos.

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.