Summer Time Start and End
Dates.
In the UK, as with all the other countries
that are part of the European Union, we now always change
the clocks at 01:00 UTC on the last Sundays in March
and October. Summer Time starts, and the clocks
will therefore be going forward an hour (you lose an
hour's sleep!), on the night of Saturday 26th and Sunday
27th March 2005. Summer Time will end on the night
of Saturday 29th and Sunday 30th October 2005.
In February 2001, the European Union agreed
to stay with this last Sunday in March and October timing
for the next five years from 2002 to 2006, and requires
all member states to abide by this decision. The
British Parliament formerly adopted this in late May
2001 - see the Greenwich
Mean Time Web Site. The following table shows
the start and end dates for the current decade.
The European Union Parliament has stated that it wants
to specify these dates sufficiently far ahead to allow
everyone to be able to plan ahead, but doesn't intend
to specify the change dates for 2007 onwards until early
in 2006. The final years of the decade in the
table below are therefore speculative, and this page
will be updated as soon as Europe makes up it's mind!
|
British
Summer Time |
|
Starts: |
Ends: |
|
| 2000 |
Sunday, 26th March |
Sunday, 29th October |
| 2001 |
Sunday, 25th March |
Sunday, 28th October |
| 2002 |
Sunday, 31st March |
Sunday, 27th October |
| 2003 |
Sunday, 30th March |
Sunday, 26th October |
| 2004 |
Sunday, 28th March |
Sunday, 31st October |
|
| 2005 |
Sunday, 27th March |
Sunday, 30th October |
| 2006 |
Sunday, 26th March |
Sunday, 29th October |
|
| 2007 |
Sunday, 25th March |
Sunday, 28th October |
| 2008 |
Sunday, 30th March |
Sunday, 26th October |
| 2009 |
Sunday, 29th March |
Sunday, 25th October |
| 2010 |
Sunday, 28th March |
Sunday, 31st October |
Leap Seconds.
Many factors affect the rotational speed
of the Earth, including tides, and the gravitational
pull of the Sun and Moon, etc. Since the creation
of the Caesium atomic clock in the 1950's, it has
been appreciated how relatively irregular the Earth's
rotation actually is. Atomic clocks are now used
throughout the World, but they need correcting at irregular
periods in order that they match the Earth's rotation.
In 1967 the second was defined as the
duration of 9,192,631,770 periods of the radiation corresponding
to the transition between the two hyperfine levels of
the ground state of the caesium 133 atom. However,
since then the Earth has been turning, on average, a
little slower. Extra seconds - "leap-seconds"
- are inserted into our time when it becomes too far
ahead of the Earth. This timescale is called UTC
- "Co-ordinated Universal Time", and is kept
within 0.9 of a second of the Earth's actual rotational
time by the International
Earth Rotation Service. Leap-seconds are usually
only added after the last second of the last day of
June or December, but in exceptional circumstances could
also be added in March or September.
The IERS have recently
announced their predictions
& they currently show that there will be no need
for a leap second at the end of December 2005.
(The last leap-second was on December
31st 1998.)
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