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The
King's Observatory at Kew & The Transit of Venus 1769
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If you walk along the
Thames towpath between Richmond and Kew you will come across a line
of meridian.Glancing through the trees you will see an obelisk and
the King's Observatory Kew, completed in 1769 ostensibly for the
observation of the transit of Venus that occurred on June 3rd 1769.
" His Majesty the King who made his observation with a shorter
reflecting telescope, magnifying Diameter 170 Times was the first
to view the Penumbra of Venus touching the Edge of the Sun's Disk.
The exact mean time (according to civil Reckoning) was attended
to by Stephen Demainbray, appointed to take exact time by Shelton's
Regulator, previously regulated by several astronomical observations."1
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| Transits
of Venus
Transits of Venus across the disk of the Sun are among the rarest
of planetary alignments. They come in pairs, 8 years apart, separated
by approximately 120 years. Prior to the 18th Century and since
the invention of the telescope they had occurred in 1631 and 1639.
The first recorded transit of Venus in this country had been in
1639 and no measurements had been taken.
One of the major questions of 18th century science was the size
of the solar system. Six planets were known that orbited the Sun;
Mercury, Venus, Earth, Mars, Saturn and Jupiter, but the size of
the solar system in a quantifiable measurement was unknown. Astronomers
knew the relative spacing of the known planets but not the absolute
distances.
Edmund Halley (1656-1742) calculated in 1716 that during a transit
of Venus, astronomers could calculate the distance to Venus using
the principles of parallax. If measurements of the start and stop
times of the transit of Venus were taken from other parts of the
world they could determine the distance of the earth from the Sun.
This would determine the measurement of the astronomical unit and
from this then deduct the dimensions of the solar system. |
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Present on that day included
George III, Queen Charlotte, Doctor Stephen C.T. Demainbray, Stephen
Rigaud, Justin Vulliamy, Ben Vulliamy. On the day of the transit
the weather had been rainy and overcast probably due to the prevailing
westerly wind. It cleared at about 4.00pm and the transit began
just after 7.00pm. |
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Above: Manuscript
of Dr. Demainbray's notebook of the Transit of Venus 1769 |
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| The next
Transits of Venus were due in 1761 and 1769. Halley himself never
witnessed a Transit of Venus, but for the 1761 transit the scientific
world was prepared with expeditions to various corners of the world.
The results in 1761 were disappointing as a phenomenon known as 'black
drop' probably caused by the atmosphere of Venus, created a protrusion
in the shape of Venus as it crossed the Sun and thus compromised the
timing of the transit. This disappointment in the international effort
meant that the 1769 Transit became more important as the next transit
was not until 1874 and the scientists would not be able to witness
it. |
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The Path of a Transit of Venus
across the Sun |
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Right - Painting of the Observatory
by unknown artist |
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| The
Observatory
Augusta Princess of Wales, the mother of George III lived at
Kew Palace. There was an observatory attached to it but it had greatly
deteriorated and did not have the facilities to view the transit
of Venus. George III therefore ordered the building of a new observatory
most likely advised by Dr. Stephen C.T. Demainbray.
The Kew Observatory stands on the borders between Richmond and
Kew in the Old Deer Park, built of Portland stone it has seven acres
of grounds. It was originally called the "King's Observatory at
Richmond". Sometime in the early nineteenth century it became known
as Kew Observatory. The Observatory belonged to the Kew Estate and
probably this was the reason why it became known as Kew Observatory,
though it was in the Parish of Richmond. |
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| Sir William Chambers (1726
- 1796) was the architect, he also designed the Pagoda in Kew Gardens
and Somerset House in London. It was built where a Carthusian Priory
"The House of Jesus of Bethlehem at Shene " had formally stood. King
Henry V had founded the priory in 1414, it declined during the Reformation
and was eventually demolished when the building of the observatory
began. It is designed as a villa with a moveable dome observatory
mounted on the top. The building is in its original design state apart
from some raising of side roofs to the level of the observing dome
that happened in the 1880's. |
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| The main
telescopes were in the movable dome that had an opening roof. The
west of the observatory was used for the day to day transit observations.
The room on the east side was used for quadrant observations. There
are three obelisks built in 1769 of Portland stone to aid the alignment
of the instruments. One is positioned to the North of the centre of
the observatory. The two others mark south from the transit and quadrant
rooms. All three obelisks can be seen walking along the towpath due
to the meander of the Thames. When the building of the Observatory
had been completed in 1769, Dr. Demainbray adjusted the instruments
there ready for the transit of Venus. |
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Above: The Obelisks marking South
and Magnetic South from the Observatory |
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The 1769 Transit
of Venus
In 1769 enthusiasm was high, as advances had been made in telescopes
and observation methods. As well as Kew, observations were made
at Greenwich where Nevil Maskelyne (1732-1811) the Astronomer
Royal for England for most of the second half of the 18th century
observed and wrote his account of the transit.
In the South Seas Captain James Cook in His Majesty's Bark
Endeavour had set sail on August 12, 1768, from Plymouth bound for
Tahiti specifically for the purpose of observing this transit. The
worldwide results of the 1769 transit were on the whole disappointing.
The results from the 76 points around the globe were not precise
enough to set the scale of the solar system. |
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Above: Shelton's Regulator used
for the timings of the 1769 Transit at Kew |
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Dr. Demainbray noted
that the observers at Kew were in agreement of their timings within
one second however they were 60 1/2 seconds out with the timings
at Greenwich. This would be reflected in other observations around
the world. The Greenwich observations were recorded and used in
the scientific calculations that were made after the transit, as
were the timings of Captain James Cook.
The Kew observation timings were not published nor used in the
worldwide calculations. The observations of the 1769 transit were
again compromised by the 'black drop' phenomenon and Dr. Demainbray
briefly mentioned this in his notes. Maskelyne at Greenwich however
was far more concerned with the 'black drop' phenomenon as his notes
emphasised this fact more so than Dr. Demainbray's.
Incidentally astronomers didn't manage an accurate calculation
of The Transit of Venus until the 19th century when they used photography
to record the next pair of transits. It was not until the 20th Century
with the advent of radio astronomy that the astronomical unit was
accurately measured and refined to the consistent value it is today.
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The
Transits of Venus 2004 & 2012
The last Transit of Venus took place on June 8th 2004. It was
the most widely photographed and observed transit there has ever
been. The entire transit was visible from Europe, Africa (except
western parts), Middle East, and most of Asia (except eastern parts).
The Sun set during the transit in Australia, Indonesia, Japan, Philippines,
Korea, easternmost China and Southeast Asia. The Sun rose with the
transit already in progress for observers in western Africa, eastern
North America, the Caribbean and most of South America. The transit
was not visible from southern Chile or Argentina, western North
America, Hawaii or New Zealand. |
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Above: Drawing by Captain
Cook of the Transit of Venus, showing the stages of the Transit. |
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| The next transit of Venus
will be on June 6th 2012. The entire transit will be visible from
north western North America, Hawaii, the western Pacific, northern
Asia, Japan, Korea, eastern China, Philippines, eastern Australia,
and New Zealand. The Sun will set during the transit in most of North
America, the Caribbean, and north west South America. The Sun will
rise during the transit for observers in central Asia, the Middle
East, Europe, and eastern Africa. The transit will not be visible
from Portugal or southern Spain, western Africa, and most of the south
eastern area of South America. The next pairs of transits will not
occur until December 2117, December 2125, June 2247, June 2255, December
2360 and December 2368. |
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| Wherever you are for the
next transit in 2012, remember it will be your last opportunity to
witness this most rare of planetary alignments. Perhaps also spare
a thought for George III, Stephen Demainbray, Stephen Rigaud, Justin
Vulliamy, Benjamin Vulliamy and Queen Charlotte who witnessed the
1769 transit and their attempts to contribute to our further understanding
of our solar system. The Kew observatory stands today as a monument
to man's never-ending fascination with the movement of the planets
and our efforts to find our place in the cosmos. |
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Map
showing the path of the 2012 transit |
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Article: Arcadian Times |
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References 1 - Taken
from the manuscript of Dr. Demainbray. This is in the Library of
King's College London.
John Harris in his biography of Sir William Chambers Other references
used: The Meteorological Magazine 98 1969 , Articles by L. Jacobs
" The 200 Years story of Kew Observatory" History of the Kew Observatory
- Robert H. Scott Websites: National Maritime Museum Greenwich,
NASA, The Armagh Observatory, The Science Museum, European Southern
Observatory. Local Studies Unit, Richmond Library. Manuscript of
Dr. Demainbray's notebook of the Transit of Venus 1769, From King's
College London. |
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