
"Measurement standards are needed for knowing "how much" exists. Early distance standards, like "cubits" or "feet," were based on body parts. A single "pace" was often used: around one yard/meter. The idea of a "standard meter" came from pendulum observations. A swinging pendulum's period is determined by two factors: length and gravity. A seconds pendulum, where each half-swing lasts one second, requires a pendulum one meter long. Because gravity varies by ~0.2% across Earth, any pendulum-based "length" isn't universal."
"In 1790, the meter was defined as 1/10,000,000th the distance from the North Pole to the equator. That distance was then cast into a platinum bar. After correcting an early error of 0.2 millimeters, these bars became distance standards for decades. Platinum-iridium alloys, with X-shapes to better resist distortions, replaced those originals. In the 1920s, atomic interferometry - based on light's wavelength - superseded the "bar" standard. The right number of wavelengths of light defined the 20th century's meter."
"Platinum-iridium alloys, with X-shapes to better resist distortions, replaced those originals. In the 1920s, atomic interferometry - based on light's wavelength - superseded the "bar" standard. The right number of wavelengths of light defined the 20th century's meter. First cadmium, then mercury, and next krypton atoms defined the meter. Finally, in 1983, a new standard was adopted: the distance light travels in 1/299,792,458th of a second. Because the speed of light in a vacuum is always constant, this definition is universal."
Early length measures used body parts such as cubits and feet, and a common pace approximated one yard or meter. Pendulum observations suggested a seconds pendulum of one meter, but gravity's ~0.2% variation across Earth made pendulum length non-universal. In 1790 the meter was defined as 1/10,000,000th the meridian distance from the North Pole to the equator and embodied in a platinum bar, later corrected by 0.2 mm and replaced by platinum‑iridium X‑shaped bars. Atomic interferometry using light wavelengths in the 1920s replaced bars; later the meter was defined by light travel in 1/299,792,458th of a second.
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