There are two important concepts, related
to latitude and longitude (especially) are local time (LT) and universal time
(UT).
Longitudes are measured from zero to 180
degree east and 180 degree west (or -180), and both 180 degree longitudes share
the same line, in the middle of the pacific ocean.
As the earth rotates around its axis, at
any moment one line of the longitude ‘the noon meridian’ faces the sun, and at
that moment, it will be noon everywhere on it. After 24 hours the earth has
undergone a full rotation with respect to the sun, and the same meridian again
faces noon. Thus each hour the earth rotates by 360/24 = 15 degree.
- The date line and universal time (UT).
Longitude determines only the hour of the
day, i.e. not the date, which is determined separately. The international date
line has been established most of it following the 180th meridian where
by common agreement, whenever we cross it the date advances one day (going
west) or goes back one day (going east).
That line passes the bering strait
between Alaska and Siberia, which thus have different dates, but for most of
its course it runs in mid ocean and does not inconvenience any local time
keeping.
Astronomers, astronauts and people
dealing with satellite data may need a time schedule which is the same
everywhere, not tied to a locality or time zone. The Greenwich mean time, the
astronomical time at Greenwich (average over the year) is generally used here.
It is sometimes called universal time (UT).
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