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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 somethingIt has become something
of a traditionof a tradition
on this blog to mark the biannual change of the clocks and, although I noon this blog to mark the biannual change of the clocks and, although I no
longer work at the Royallonger work at the Royal
Observatory Greenwich, it’s a habit that sticks. This time, as we sayObservatory 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 aboutfarewell 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 aMean time is clock time. It is a
regularised, idealised version of solar time that is tracked not by theregularised, idealised version of solar time that is tracked not by the
apparent motions of the Sun, observed by shadows on sundials, but by aapparent motions of the Sun, observed by shadows on sundials, but by a
mechanical device that splits the solar day into equal parts. Mean time ticksmechanical 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 isaway at the same pace no matter the season. The difference between the two is
described by the equationdescribed by the equation
of time.of time.
Establishing the relationship between meanEstablishing the relationship between mean
solar time and apparent solar time only really became possible, or useful, withsolar 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 developedfor the first time, a scientific instrument. Christiaan Huygens, who developed
the first prototypethe first prototype
pendulum clock in 1656, was able to produce reasonably accurate tables ofpendulum 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 publishHowever, it fell to John Flamsteed to publish
tables in 1672-3 that tackled the problem in what became the standard way. Hetables 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 Meanprovided the formula by which apparent solar time could be converted into Mean
Time.Time.
Just a couple of years later, Flamsteed wasJust a couple of years later, Flamsteed was
appointed the first Astronomer Royal and moved into the newly built observatoryappointed the first Astronomer Royal and moved into the newly built observatory
in Greenwich. There, he and his patrons had installed state-of-the-art pendulumin Greenwich. There, he and his patrons had installed state-of-the-art pendulum
clocks by the best clockmaker available, Thomas Tompion. Withclocks by the best clockmaker available, Thomas Tompion. With
observations of the Sun and the help of his tables, Flamsteed set these clocksobservations 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 becauseGreenwich time became important because
there were people measuring it and because other people made use ofthere were people measuring it and because other people made use of
astronomical observations based on it. Flamsteed’s catalogue of stars, whichastronomical observations based on it. Flamsteed’s catalogue of stars, which
was to become a standard reference work for the following decades, listed theirwas 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 toAstronomer Royal from 1765 to 1811, who did most to ensure that GMT mattered to
more than just astronomers. Under his initiative, observations made atmore than just astronomers. Under his initiative, observations made at
Greenwich were processed into tables that could be used by navigators andGreenwich 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 theSurveyors 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. Moremeaning that their charts and maps used Greenwich as a reference point. More
precisely, this was the meridian (north-south line) on which the chiefprecisely, this was the meridian (north-south line) on which the chief
telescope at Greenwich was mounted. The Greenwich meridian thus became atelescope at Greenwich was mounted. The Greenwich meridian thus became a
prime meridian for British mapping, and east-west position was measured fromprime meridian for British mapping, and east-west position was measured from
there. To establish longitudes it was necessary to know the difference betweenthere. To establish longitudes it was necessary to know the difference between
local time and GMT. This could be worked out with astronomical observations andlocal time and GMT. This could be worked out with astronomical observations and
the tables of the Nautical Almanac and, increasingly, with chronometers set tothe tables of the Nautical Almanac and, increasingly, with chronometers set to
GMT.GMT.
The move of GMT from the specialist worldsThe move of GMT from the specialist worlds
of astronomy, navigation and surveying into civilian life was down to theof astronomy, navigation and surveying into civilian life was down to the
increasing role of technologies and cultures that demanded standardization. Theincreasing role of technologies and cultures that demanded standardization. The
arrival of railways made timetabling a necessity. Telegraph systems made itarrival of railways made timetabling a necessity. Telegraph systems made it
both desirable and possible to know what time it was elsewhere. Factory workboth 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, itand 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 andid not become an international standard in 1884. In that year an
international conference did recommend the adoption of the Greenwich meridianinternational conference did recommend the adoption of the Greenwich meridian
as the world’s reference point for time and longitude, but it was just aas the world’s reference point for time and longitude, but it was just a
recommendation.recommendation.
What actually happened as a result of theWhat actually happened as a result of the
International Meridian Conference, and what did not, is a story for anotherInternational 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.
RebekahRebekah
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 2014), a Clocks and Stars: the Quest for Longitude (11 July 2014-4 January 2015), a
forthcoming exhibition at the National Maritime Museum marking the tercentenaryforthcoming exhibition at the National Maritime Museum marking the tercentenary
of the first Longitude Act, and which includes the story of the Nauticalof 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.