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Farewell Greenwich Mean Time (see you in October) | Farewell Greenwich Mean Time (see you in October) |
(about 14 hours later) | |
It has become something | It has become something |
of a tradition | of a tradition |
on this blog to mark the biannual change of the clocks and, although I no | on this blog to mark the biannual change of the clocks and, although I no |
longer work at the Royal | longer work at the Royal |
Observatory Greenwich, it’s a habit that sticks. This time, as we say | Observatory Greenwich, it’s a habit that sticks. This time, as we say |
farewell to it until the autumn, it seems a good opportunity to reminisce about | farewell to it until the autumn, it seems a good opportunity to reminisce about |
Greenwich Mean Time.* | Greenwich Mean Time.* |
Why Greenwich time? And what’s mean about it? | Why Greenwich time? And what’s mean about it? |
Mean time is clock time. It is a | Mean time is clock time. It is a |
regularised, idealised version of solar time that is tracked not by the | regularised, idealised version of solar time that is tracked not by the |
apparent motions of the Sun, observed by shadows on sundials, but by a | apparent motions of the Sun, observed by shadows on sundials, but by a |
mechanical device that splits the solar day into equal parts. Mean time ticks | mechanical device that splits the solar day into equal parts. Mean time ticks |
away at the same pace no matter the season. The difference between the two is | away at the same pace no matter the season. The difference between the two is |
described by the equation | described by the equation |
of time. | of time. |
Establishing the relationship between mean | Establishing the relationship between mean |
solar time and apparent solar time only really became possible, or useful, with | solar time and apparent solar time only really became possible, or useful, with |
the arrival of the pendulum clock in the 1650s. This made the mechanical clock, | the arrival of the pendulum clock in the 1650s. This made the mechanical clock, |
for the first time, a scientific instrument. Christiaan Huygens, who developed | for the first time, a scientific instrument. Christiaan Huygens, who developed |
the first prototype | the first prototype |
pendulum clock in 1656, was able to produce reasonably accurate tables of | pendulum clock in 1656, was able to produce reasonably accurate tables of |
the equation of time in 1665. | the equation of time in 1665. |
However, it fell to John Flamsteed to publish | However, it fell to John Flamsteed to publish |
tables in 1672-3 that tackled the problem in what became the standard way. He | tables in 1672-3 that tackled the problem in what became the standard way. He |
provided the formula by which apparent solar time could be converted into Mean | provided the formula by which apparent solar time could be converted into Mean |
Time. | Time. |
Just a couple of years later, Flamsteed was | Just a couple of years later, Flamsteed was |
appointed the first Astronomer Royal and moved into the newly built observatory | appointed the first Astronomer Royal and moved into the newly built observatory |
in Greenwich. There, he and his patrons had installed state-of-the-art pendulum | in Greenwich. There, he and his patrons had installed state-of-the-art pendulum |
clocks by the best clockmaker available, Thomas Tompion. With | clocks by the best clockmaker available, Thomas Tompion. With |
observations of the Sun and the help of his tables, Flamsteed set these clocks | observations of the Sun and the help of his tables, Flamsteed set these clocks |
to the local time: Greenwich Mean Time. | to the local time: Greenwich Mean Time. |
Greenwich time became important because | Greenwich time became important because |
there were people measuring it and because other people made use of | there were people measuring it and because other people made use of |
astronomical observations based on it. Flamsteed’s catalogue of stars, which | astronomical observations based on it. Flamsteed’s catalogue of stars, which |
was to become a standard reference work for the following decades, listed their | was to become a standard reference work for the following decades, listed their |
positions based on Greenwich time. | positions based on Greenwich time. |
It was one of Flamsteed’s successors, Nevil Maskelyne, | It was one of Flamsteed’s successors, Nevil Maskelyne, |
Astronomer Royal from 1765 to 1811, who did most to ensure that GMT mattered to | Astronomer Royal from 1765 to 1811, who did most to ensure that GMT mattered to |
more than just astronomers. Under his initiative, observations made at | more than just astronomers. Under his initiative, observations made at |
Greenwich were processed into tables that could be used by navigators and | Greenwich were processed into tables that could be used by navigators and |
cartographers to establish positions at sea or on land. This was the Nautical Almanac, | cartographers to establish positions at sea or on land. This was the Nautical Almanac, |
first published for the year 1767. | first published for the year 1767. |
Surveyors of the Royal Navy and the | Surveyors of the Royal Navy and the |
Ordnance Survey relied on data that was based on observations made at Greenwich, | Ordnance Survey relied on data that was based on observations made at Greenwich, |
meaning that their charts and maps used Greenwich as a reference point. More | meaning that their charts and maps used Greenwich as a reference point. More |
precisely, this was the meridian (north-south line) on which the chief | precisely, this was the meridian (north-south line) on which the chief |
telescope at Greenwich was mounted. The Greenwich meridian thus became a | telescope at Greenwich was mounted. The Greenwich meridian thus became a |
prime meridian for British mapping, and east-west position was measured from | prime meridian for British mapping, and east-west position was measured from |
there. To establish longitudes it was necessary to know the difference between | there. To establish longitudes it was necessary to know the difference between |
local time and GMT. This could be worked out with astronomical observations and | local time and GMT. This could be worked out with astronomical observations and |
the tables of the Nautical Almanac and, increasingly, with chronometers set to | the tables of the Nautical Almanac and, increasingly, with chronometers set to |
GMT. | GMT. |
The move of GMT from the specialist worlds | The move of GMT from the specialist worlds |
of astronomy, navigation and surveying into civilian life was down to the | of astronomy, navigation and surveying into civilian life was down to the |
increasing role of technologies and cultures that demanded standardization. The | increasing role of technologies and cultures that demanded standardization. The |
arrival of railways made timetabling a necessity. Telegraph systems made it | arrival of railways made timetabling a necessity. Telegraph systems made it |
both desirable and possible to know what time it was elsewhere. Factory work | both desirable and possible to know what time it was elsewhere. Factory work |
made production and payment dependent on timekeeping. | made production and payment dependent on timekeeping. |
GMT became “Railway Time” in the 1840s, | GMT became “Railway Time” in the 1840s, |
and Britain’s legal standard time in 1880. Despite what you’ll often read, it | and Britain’s legal standard time in 1880. Despite what you’ll often read, it |
did not become an international standard in 1884. In that year an | did not become an international standard in 1884. In that year an |
international conference did recommend the adoption of the Greenwich meridian | international conference did recommend the adoption of the Greenwich meridian |
as the world’s reference point for time and longitude, but it was just a | as the world’s reference point for time and longitude, but it was just a |
recommendation. | recommendation. |
What actually happened as a result of the | What actually happened as a result of the |
International Meridian Conference, and what did not, is a story for another | International Meridian Conference, and what did not, is a story for another |
post. See you back here on 26 October. | post. See you back here on 26 October. |
* Our standard time is now in fact Coordinated Universal Time (UTC), derived from International Atomic Time but as close as darn it to GMT. | * Our standard time is now in fact Coordinated Universal Time (UTC), derived from International Atomic Time but as close as darn it to GMT. |
Rebekah | Rebekah |
Higgitt is one of the curators of Ships, | Higgitt is one of the curators of Ships, |
Clocks and Stars: the Quest for Longitude (11 July 2014-4 January 2015), a | |
forthcoming exhibition at the National Maritime Museum marking the tercentenary | forthcoming exhibition at the National Maritime Museum marking the tercentenary |
of the first Longitude Act, and which includes the story of the Nautical | of the first Longitude Act, and which includes the story of the Nautical |
Almanac and the development of marine timekeepers. | Almanac and the development of marine timekeepers. |