Year: Day to Day Men: February 5
Hidden Face
The fifth day of February in 1924 marks the Royal Greenwich Observatory’s first broadcast of the hourly time signal known as the Greenwich Time Signal. Originally the idea of the Astronomer Royal Sir Frank Watson Dyson and the head of the BBC John Reith, the signal was originally controlled by two mechanical clocks with electrical contacts attached to their swinging pendulums. These sent a signal to the BBC which converted them to the oscillatory tone broadcast.
Situated on a hill in southeast London, the Royal Observatory, Greenwich, played a major role in the history of navigation and astronomy.The site of the observatory was established in 1851 by Sir George Airy as the Prime Meridian, the historic geographical reference line. By 1884, over two-thirds of all ships and tonnage were using it as the reference meridian on their charts and maps. Long symbolized by a brass strip in the observatory’s courtyard and later one of stainless steel, the Prime Meridian is now marked by a powerful green laser. As the Prime Meridian passes through its site, the Royal Observatory gave its name to what became Greenwich Mean Time, today known as Coordinated Universal Time (UTC).
The Greenwich Time Signal (GTS) is a series os six short tones, or beeps, broadcast at one-second intervals by many BBC radio stations. Introduced in 1924, these tones have been generated by the BBC since 1990 to mark the precise start of each hour. The six short beeps occur on each of the five seconds leading to the hour and on the hour itself. Each beep is a one kilohertz tone, approximately a fifth of a semitone above musical B5. The first five beeps last a tenth of a second each; the final beep last half a second. The change of hour occurs at the beginning of the last beep.
The beeps for national radio stations are timed relative to the UTC, the primary time standard by which the world regulates its time. The UTC is based on International Atomic Time (TAI) which is maintained by an ensemble of atomic clocks around the world that measure time by monitoring the resonant frequency of atoms. Electron states in an atom are associated with different energy levels; in transitions between these states, they interact with a specific frequency of electromagnetic radiation. This phenomenon serves as the basis for the International System of Unit’s definition of a second, the basis for International Atomic Time.
Note: The Royal Observatory, Greenwich, has the International Astronomical Union’s code number ooo, the first on the list.


















