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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.

Measuring Light and Electromagnetic Waves

A nanometre (nm) is a unit of length equal to one billionth of a metre (1 nm = 10⁻⁹ m) and is commonly used to express wavelengths of light and other electromagnetic waves. In this context, nanometres provide a convenient scale for describing phenomena that occur at the atomic and molecular level. Visible light, for example, spans wavelengths from about 380 nm (violet) to 750 nm (red). Ultraviolet (UV) light has shorter wavelengths, typically between 10 nm and 400 nm, while infrared (IR) light has longer wavelengths, from about 750 nm to 1,000,000 nm.

Wavelengths in nanometres are critical in fields like optics, photonics, spectroscopy, and nanotechnology. They determine the energy and color of light, how it interacts with matter, and how it can be manipulated in devices like lasers, fiber optics, and solar cells. Shorter wavelengths (in the UV or X-ray range) carry more energy and are used in applications such as medical imaging and semiconductor fabrication. Understanding and working with wavelengths in nanometres allows scientists and engineers to explore and control the behavior of light at extremely small scales—down to the size of atoms and molecules.