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The Unit of Frequency


The term cycle per second, commonly known as the hertz (Hz), is the standard unit of frequency in the International System of Units (SI). It measures how many complete cycles or oscillations of a periodic event occur in one second. For example, if a wave oscillates 60 times in one second, it has a frequency of 60 Hz. The concept of cycle per second applies to many fields including sound waves, electromagnetic waves, mechanical vibrations, and alternating current electricity.


Frequency determines many important characteristics of waves, such as pitch in sound or color in light. In electrical engineering, frequency dictates the behavior of AC power systems, with the standard mains electricity frequency being 50 or 60 Hz depending on the country. Radio and television broadcasts also rely on specific frequencies to transmit signals.


Using cycle per second as a unit helps scientists and engineers understand and quantify periodic phenomena. The hertz is essential for designing electronic devices, communication systems, and studying natural oscillations. It provides a universal language to describe the repetitive nature of waves and signals, enabling consistent measurement and comparison across different scientific disciplines.


Cosmic Scales of Electromagnetic Waves


A terametre (Tm) is equal to 1 trillion metres (10¹² m), an enormous unit used to describe wavelengths on an interplanetary or even interstellar scale. Such colossal wavelengths correspond to extremely low frequencies in the picohertz to femtohertz range and are primarily relevant in astrophysics, cosmology, and gravitational wave studies. At this scale, electromagnetic or gravitational waves can span distances comparable to the size of the solar system or beyond.


For example, a frequency of 1 femtohertz (10⁻¹⁵ Hz) corresponds to a wavelength of approximately 300 terametres, or 300 billion kilometres — about twice the distance from the Sun to Pluto. These wavelengths are far beyond practical terrestrial communication but are important for understanding phenomena like primordial gravitational waves, cosmic microwave background fluctuations, and large-scale cosmic structures.


Using terametres to express wavelength helps scientists conceptualize and study the vast, slow oscillations that shape the universe over billions of years. These extreme wavelengths offer insight into the very fabric of space-time, the origins of the universe, and processes occurring on the grandest cosmic scales.





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