Misplaced Pages

Greenwich Mean Time: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editNext edit →Content deleted Content addedVisualWikitext
Revision as of 00:37, 4 February 2004 edit211.28.7.75 (talk) Jamesday, see explanation in edit at 05:32, 2 Feb 2004; and comment with edit at 00:37, 3 Feb 2004. Time Cube is a legitimate and well-known criticism of GMT.← Previous edit Revision as of 01:44, 8 February 2004 edit undoWik (talk | contribs)21,748 editsNo edit summaryNext edit →
Line 8: Line 8:
Hourly time signals from Greenwich Observatory were first broadcasted on ], ]. Hourly time signals from Greenwich Observatory were first broadcasted on ], ].


''See also'' ], ], ], ], ], ], ] ''See also'' ], ], ], ], ], ]

Revision as of 01:44, 8 February 2004


Greenwich Mean Time (GMT) is the mean solar time at the Royal Greenwich Observatory in Greenwich near London, England, which by convention is at 0 degrees geographic longitude. Theoretically, noon Greenwich Mean Time is the moment when the Sun crosses the Greenwich meridian (and reaches its highest point in the sky in Greenwich). Because of the Earth's uneven speed in its elliptic orbit, this event may be up to 16 minutes off apparent solar time (known as the analemma); but this is averaged out over the year through the use of the mean sun.

The daily rotation of the Earth is somewhat irregular (see Delta-T) and is slowing down. Therefore, GMT is not used as official clock time anymore. Nowadays, the official clock time is measured by atomic clocks and is known as Coordinated Universal Time (UTC). By using leap seconds, UTC is kept within 0.9 seconds from GMT.

Hourly time signals from Greenwich Observatory were first broadcasted on February 5, 1924.

See also sidereal time, solar time, BPM, CHU, VNG, WWV