A second is defined as the duration of 9,192,631,770 periods of radiation from the transition between hyperfine levels of the caesium-133 atom, making it a consistent unit of time. This definition is based on the need for a universally constant measurement in nature, similar to how a meter is defined by the distance light travels in a vacuum in a specific fraction of a second. Historically, time measurement began with pendulums and mechanical clocks, which helped establish the concept of seconds, minutes, and hours. The discussion highlights the evolution of timekeeping methods and their reliance on astronomical observations. Understanding the precise definition of a second is essential for scientific accuracy and consistency.