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William Herschel and the Bath Museum of Astronomy

William and Caroline Herschel polishing a telescope lens, 1896 Lithograph.

Sir Frederick William Herschel, KH, FRS  (15 November 1738 – 25 August 1822) was a German-born British astronomer, composer, and brother of Caroline Herschel. Born in the Electorate of Hanover, Herschel followed his father into the Military Band of Hanover, before migrating to Great Britain at the age of nineteen.

Replica in the William Herschel Museum, Bath, of a telescope similar to that with which Herschel discovered Uranus
Replica in the William Herschel Museum, Bath, of a telescope similar to that with which Herschel discovered Uranus

Herschel became interested in astronomy in 1773, and after constructing his first large telescope in Bath, in 1774, he spent nine years carrying out thorough sky surveys, where his purpose was the investigation of double stars. The resolving power of the Herschel telescopes revealed that the nebulae in the Messier catalogue were clusters of stars: catalogues of nebulae were published in 1802 (2,500 objects) and 1820 (5,000 objects). In the course of an observation on 13 March 1781 he realized that one celestial body he had observed was not a star, but a planet, Uranus. This was the first planet to be discovered since antiquity and Herschel became famous overnight. As a result of this discovery George III appointed him ‘Court Astronomer’. He was elected as a Fellow of the Royal Society and grants were provided for the construction of new telescopes.

Uranusandrings
A 1998 false-colour near-infrared image of Uranus showing cloud bands, rings, and moons obtained by the Hubble Space Telescope’s NICMOS camera.

Herschel pioneered the use of astronomical spectrophotometry as a diagnostic tool, using prisms and temperature measuring equipment to measure the wavelength distribution of stellar spectra. Other work included an improved determination of the rotation period of Mars, the discovery that the Martian polar caps vary seasonally, the discovery of Titania and Oberon (moons of Uranus) and Enceladus and Mimas (moons of Saturn). In addition, he was the first person to discover the existence of infrared radiation. Herschel was knighted in 1816. He died in August 1822, and his work was continued by his only son, John Herschel.

William Herschel, 1785 by Lemuel Francis Abbot.
William Herschel, 1785 by Lemuel Francis Abbot.

Herschel was born in the Electorate of Hanover in Germany , part of the Holy Roman Empire, one of ten children of Isaac Herschel by his marriage to Anna Ilse Moritzen. His family were Lutheran Christians. The surname, identifying his Jewish origin, is descended–according to Herhsel’s biographer Holden–from Jewish Moravians who converted to Protestantism in the 17th century. His father was an oboist in the Hanover Military Band. In 1755 the Hanoverian Guards regiment, in whose band Wilhelm and his brother Jakob were engaged as oboists, was ordered to England. At the time the crowns of Great Britain and Hanover were united under King George II. As the threat of war with France loomed, the Hanoverian Guards were recalled from England to defend Hanover. After they were defeated at the Battle of Hastenbeck, Herschel’s father Isaak sent his two sons to seek refuge in England in late 1757. Although his older brother Jakob had received his dismissal from the Hanoverian Guards, Wilhelm was accused of desertion (for which he was pardoned by George III in 1782). Wilhelm, nineteen years old at this time, was a quick student of the English language. In England he went by the English rendition of his name, Frederick William Herschel.

In addition to the oboe, he played the violin and harpsichord and later the organ. He composed numerous musical works, including 24 symphonies and many concertos, as well as some church music. Six of his symphonies were recorded in April 2002 by the London Mozart Players, conducted by Matthias Bamert (Chandos 10048).

Original manuscript of Symphony No. 15 in E flat major (1762).
Original manuscript of Symphony No. 15 in E flat major (1762).

Herschel moved to Sunderland in 1761 when Charles Avison immediately engaged him as first violin and soloist for his Newcastle orchestra, where he played for one season. In ‘Sunderland in the County of Durh: apprill [sic] 20th 1761’ he wrote his symphony No. 8 in c minor. He was head of the Durham Militia band 1760–61 and visited the home of Sir Ralph Milbanke at Halnaby Hall in 1760, where he wrote two symphonies, as well as giving performances himself.

"The Octagon Bath" by Ngw2009 - Own work. Licensed under CC BY-SA 3.0 via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:The_Octagon_Bath.jpg#mediaviewer/File:The_Octagon_Bath.jpg
“The Octagon Bath” by Ngw2009 – Own work. Licensed under CC BY-SA 3.0 via Wikimedia Commons – http://commons.wikimedia.org/wiki/File:The_Octagon_Bath.jpg#mediaviewer/File:The_Octagon_Bath.jpg

After Newcastle he moved to Leeds and Halifax where he was the first organist at St John the Baptist church (now Halifax Minster). He became organist of the Octagon Chapel, Bath, a fashionable chapel in a well-known spa, in which city he was also Director of Public Concerts. He was appointed as the organist in 1766 and gave his introductory concert on 1 January 1767. As the organ was still incomplete he showed off his versatility by performing his own compositions including a violin concerto, an oboe concerto and a harpsichord sonata. The organ was completed in October 1767. His sister Caroline came to England in 1772 and lived with him there in New King Street, Bath. The house they shared is now the location of the Herschel Museum of Astronomy. His brothers Dietrich, Alexander and Jakob (1734–1792) also appeared as musicians of Bath. In 1780, Herschel was appointed director of the Bath orchestra, with his sister often appearing as soprano soloist.

The front of the Herschel Museum.
The front of the Herschel Museum of Astronomy in Bath where the Herschels discovered many astronomical wonders, including the planet, Uranus.

Herschel’s music led him to an interest in mathematics and lenses. His interest in astronomy grew stronger after he made the acquaintance of the English Astronomer Royal Nevil Maskelyne. He started building his own reflecting telescopes and would spend up to 16 hours a day grinding and polishing the speculum metal primary mirrors. He “began to look at the planets and the stars” in May 1773 and on 1 March 1774 began an astronomical journal by noting his observations of Saturn’s rings and the Great Orion Nebula (M 42).

Herschel's mirror polisher, on display in the Science Museum, London.
Herschel’s mirror polisher, on display in the Science Museum, London.

Herschel’s early observational work soon focused on the search for pairs of stars that were very close together visually. Astronomers of the era expected that changes over time in the apparent separation and relative location of these stars would provide evidence for both the proper motion of stars and, by means of parallax shifts in their separation, for the distance of stars from the Earth (a method first suggested by Galileo Galilei). From the back garden of his house in New King Street, Bath, and using a 6.2-inch aperture (160 mm), 7-foot focal length (2.1 m) (f/13) Newtonian telescope “with a most capital speculum” of his own manufacture, in October 1779, Herschel began a systematic search for such stars among “every star in the Heavens”, with new discoveries listed through 1792. He soon discovered many more binary and multiple stars than expected, and compiled them with careful measurements of their relative positions in two catalogues presented to the Royal Society in London in 1782 (269 double or multiple systems) and 1784 (434 systems). A third catalogue of discoveries made after 1783 was published in 1821 (145 systems).

An interior of the home at 19 New King Street, Bath, which is now the Herschel Museum of Astronomy.
An interior of the home at 19 New King Street, Bath, which is now the Herschel Museum of Astronomy.

In 1797 Herschel measured many of the systems again, and discovered changes in their relative positions that could not be attributed to the parallax caused by the Earth’s orbit. He waited until 1802 (in Catalogue of 500 new Nebulae, nebulous Stars, planetary Nebulae, and Clusters of Stars; with Remarks on the Construction of the Heavens) to announce the hypothesis that the two stars might be “binary sidereal systems” orbiting under mutual gravitational attraction, a hypothesis he confirmed in 1803 in his Account of the Changes that have happened, during the last Twenty-five Years, in the relative Situation of Double-stars; with an Investigation of the Cause to which they are owing. In all, Herschel discovered over 800 confirmed double or multiple star systems, almost all of them physical rather than virtual pairs. His theoretical and observational work provided the foundation for modern binary star astronomy; new catalogues adding to his work were not published until after 1820 by Friedrich Wilhelm Struve, James South and John Herschel.

In March 1781, during his search for double stars, Herschel noticed an object appearing as a nonstellar disk. Herschel originally thought it was a comet or a star. He made many more observations of it, and afterwards Russian Academician Anders Lexell computed the orbit and found it to be probably planetary. Herschel determined in agreement that it must be a planet beyond the orbit of Saturn. He called the new planet the ‘Georgian star’ (Georgium sidus) after King George III, which also brought him favour; the name did not stick. In France, where reference to the British king was to be avoided if possible, the planet was known as ‘Herschel’ until the name ‘Uranus’ was universally adopted. The same year, Herschel was awarded the Copley Medal and elected a Fellow of the Royal Society. In 1782, he was appointed “The King’s Astronomer” (not to be confused with the Astronomer Royal). He and his sister subsequently moved to Datchet (then in Buckinghamshire but now in Berkshire) on 1 August 1782. He continued his work as a telescope maker and achieved an international reputation for their manufacture, profitably selling over 60 completed reflectors to British and Continental astronomers.

NGC 2683 is an unbarred spiral galaxy discovered by William Herschel on 5 February 1788.
NGC 2683 is an unbarred spiral galaxy discovered by William Herschel on 5 February 1788.

From 1782 to 1802, and most intensively from 1783 to 1790, Herschel conducted systematic surveys in search of “deep sky” or nonstellar objects with two 20-foot focal length (610 cm), 12-inch aperture (30 cm) and 18.7-inch aperture (47 cm) telescopes (in combination with his favoured 6-inch aperture instrument). Excluding duplicated and “lost” entries, Herschel ultimately discovered over 2400 objects defined by him as nebulae. (At that time, nebula was the generic term for any visually extended or diffuse astronomical object, including galaxies beyond the Milky Way, until galaxies were confirmed as extragalactic systems by Edwin Hubble in 1924.)

Herschel published his discoveries as three catalogues: Catalogue of One Thousand New Nebulae and Clusters of Stars (1786), Catalogue of a Second Thousand New Nebulae and Clusters of Stars (1789) and the previously cited Catalogue of 500 New Nebulae … (1802). He arranged his discoveries under eight “classes”: (I) bright nebulae, (II) faint nebulae, (III) very faint nebulae, (IV) planetary nebulae, (V) very large nebulae, (VI) very compressed and rich clusters of stars, (VII) compressed clusters of small and large [faint and bright] stars, and (VIII) coarsely scattered clusters of stars. Herschel’s discoveries were supplemented by those of Caroline Herschel (11 objects) and his son John Herschel (1754 objects) and published by him as General Catalogue of Nebulae and Clusters in 1864. This catalogue was later edited by John Dreyer, supplemented with discoveries by many other 19th century astronomers, and published in 1888 as the New General Catalogue (abbreviated NGC) of 7840 deep sky objects. The NGC numbering is still the most commonly used identifying label for these celestial landmarks.

William and Caroline Herschel polishing a telescope lens, 1896 Lithograph.
William and Caroline Herschel polishing a telescope lens, 1896 Lithograph.

In 1783 he gave Caroline a telescope, and she began to make astronomical discoveries in her own right, particularly comets. She discovered or observed eight comets, eleven nebulae and, at her brother’s suggestion, updated and corrected Flamsteed’s work detailing the position of stars. This was published as the British Catalogue of Stars. She was honoured by the Royal Astronomical Society for this work. Caroline also continued to serve as his assistant, often taking notes while he observed at the telescope.

In June 1785, owing to damp conditions, he and Caroline moved to Clay Hall in Old Windsor. In 1786, the Herschels moved to a new residence on Windsor Road in Slough. He lived the rest of his life in this residence, which came to be known as Observatory House. It is no longer standing.

On 7 May 1788, he married the widow Mary Pitt (née Baldwin) at St Laurence’s Church, Upton in Slough. His sister Caroline then moved to separate lodgings, but continued to work as his assistant.

Herschel's 40-foot telescope.
Herschel’s 40-foot telescope.

During his career, he constructed more than four hundred telescopes. The largest and most famous of these was a reflecting telescope with a 49 12-inch-diameter (1.26 m) primary mirror and a 40-foot (12 m) focal length. Because of the poor reflectivity of the speculum mirrors of that day, Herschel eliminated the small diagonal mirror of a standard newtonian reflector from his design and tilted his primary mirror so he could view the formed image directly. This design has come to be called the Herschelian telescope. On 28 August 1789, his first night of observation using this instrument, he discovered a new moon of Saturn. A second moon followed within the first month of observation. The “40-foot telescope” proved very cumbersome, and most of his observations were done with a smaller 18.5-inch (47 cm) 20-foot-focal-length (6.1 m) reflector. Herschel discovered that unfilled telescope apertures can be used to obtain high angular resolution, something which became the essential basis for interferometric imaging in astronomy (in particular Aperture Masking Interferometry and hypertelescopes).

Herschel was sure that he had found ample evidence of life on the Moon and compared it to the English countryside. He did not refrain himself from theorizing that the other planets were populated, with an special interest in Mars, which was competely in line with most of his contemporary scientists.  At Herschel’s time, scientists tended to believe in a plurality of civilized worlds, while most religious thinkers referred to unique properties of the earth. Herschel went so far to speculate that the interior of the sun was populated.

"Sun in Samuel Dunn Wall Map of the World" by Samuel Dunn and Thomas Kitchin - cropped from (1794 Samuel Dunn Map of the World in Hemispheres). Licensed under CC BY-SA 3.0 via Wikimedia Commons - http://commons.wikimedia.org/wiki/File:Sun_in_Samuel_Dunn_Wall_Map_of_the_World.jpg#mediaviewer/File:Sun_in_Samuel_Dunn_Wall_Map_of_the_World.jpg
Sunspots, 1794 Samuel Dunn Map of the World in Hemispheres. Licensed under CC BY-SA 3.0 via Wikimedia Commons – http://commons.wikimedia.org

Herschel started to examine the correlation of solar variation and solar cycle and climate. Over a period of 40 years (1779–1818), Herschel had regularly observed sunspots and their variations in number, form and size. Most of his observations took place in a period of low solar activity, the Dalton minimum. Therefore solar activity behaved very unusually. This was one of the reasons why Herschel was not able to identify the standard 11-year period in solar activity.  Herschel compared his observations with the series of wheat prices published by Adam Smith in The Wealth of Nations.

1801 Herschel reported his findings to the Royal Society and indicated five prolonged periods of few sunspots correlated with costly wheat.

The result of this review of the foregoing five periods is, that, from the price of wheat, it seems probable that some temporary scarcity or defect of vegetation has generally taken place, when the sun has been without those appearances which we surmise to be symptoms of a copious emission of light and heat.

Herschel’s study was ridiculed by some of his contemporaries but did initiate further attempts to find a correlation. Later in the 19th century, William Stanley Jevons proposed the 11-year- cycle and Herschels basic idea of a correlation between low amount of sunspots and lower yields to explain for recurring booms and slumps in the economy. Herschels speculation on a connection between sunspots and regional climate, using the market price of wheat as a proxy continues to be cited regularly till today.

According a study of the Israel Cosmic Ray Center about the influence of solar activity on the historical wheat market in England, all ten solar cycles between 1600 and 1700 show high wheat prices coinciding with low activity, and vice versa. The topic is still subject of controversies and the significance of the correlation is being doubted by some scientists.

Herschel was a man of science and has several notable discoveries to his credit:

  • In his later career, Herschel discovered two moons of Saturn, Mimas and Enceladus; as well as two moons of Uranus, Titania and Oberon. He did not give these moons their names; they were named by his son John in 1847 and 1852, respectively, after his death.
  • In 2007 evidence was cited by Dr. Stuart Eves that Herschel might have discovered rings around Uranus.
  • Herschel measured the axial tilt of Mars and discovered that the martian ice caps, first observed by Giovanni Domenico Cassini (1666) and Christiaan Huygens (1672), changed size with the planet’s seasons.
  • From studying the proper motion of stars, he was the first to realise that the solar system is moving through space, and he determined the approximate direction of that movement.
  • He also studied the structure of the Milky Way and concluded that it was in the shape of a disk. He incorrectly assumed the sun was in the centre of the disc, a theory known as Galactocentrism, which was eventually corrected by the findings of Harlow Shapley in 1918.
  • He also coined the word “asteroid”, meaning star-like (from the Greek asteroeides, aster “star” + -eidos “form, shape”), in 1802 (shortly after Olbers discovered the second minor planet, 2 Pallas, in late March), to describe the star-like appearance of the small moons of the giant planets and of the minor planets; the planets all show discs, by comparison. By the 1850s ‘asteroid’ became a standard term for describing certain minor planets.
  • On 11 February 1800, Herschel was testing filters for the sun so he could observe sun spots. When using a red filter he found there was a lot of heat produced. Herschel discovered infrared radiation in sunlight by passing it through a prism and holding a thermometer just beyond the red end of the visible spectrum. This thermometer was meant to be a control to measure the ambient air temperature in the room. He was shocked when it showed a higher temperature than the visible spectrum. Further experimentation led to Herschel’s conclusion that there must be an invisible form of light beyond the visible spectrum.
  • Herschel used a microscope to establish that coral was not a plant, as many believed at the time, since it lacked the cell walls characteristic of plants.

William Herschel and Mary had one child, John, born at Observatory House on 7 March 1792. William’s personal background and rise as man of science had a profound impact on the upbringing of his son and grandchildren. He was elected a Foreign Honorary Member of the American Academy of Arts and Sciences in 1788. In 1816, William was made a Knight of the Royal Guelphic Order by the Prince Regent and was accorded the honorary title ‘Sir’ although this was not the equivalent of an official British knighthood. He helped to found the Astronomical Society of London in 1820, which in 1831 received a royal charter and became the Royal Astronomical Society. In 1813, he was elected a foreign member of the Royal Swedish Academy of Sciences.

On 25 August 1822, Herschel died at Observatory House, Windsor Road, Slough, and is buried at nearby St Laurence’s Church, Upton, Slough. Herschel’s epitaph is

Coelorum perrupit claustra.
(He broke through the barriers of the heavens.)

Herschel’s son John Herschel also became a famous astronomer. One of William’s brothers, Alexander Herschel, moved permanently to England, near his sister Caroline and nephew John. Caroline returned to Hanover after the death of her brother. She died on 9 January 1848.

 

From Wikipedia.com

 

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Giovanni Battista Belzoni

Giovanni Balzoni
Giovanni Balzoni
Giovanni Battista Belzoni

November 1778 – 3 December 1823), sometimes known as The Great Belzoni, was a prolific Italian explorer and pioneer archaeologist of Egyptian antiquities.

Belzoni was born in Padua. His father was a barber who sired fourteen children. His family was from Rome and when Belzoni was 16 he went to work there, claiming that he “studied hydraulics.” He intended taking monastic vows, but in 1798 the occupation of the city by French troops drove him from Rome and changed his proposed career. In 1800 he moved to the Netherlands where he earned a living as a barber.

In 1803 he fled to England to avoid being sent to jail. There he married an Englishwoman, Sarah Bane (1783–1860). Belzoni was a tall man at 6 feet 7 inches (2.01 m) tall (one source says that his wife was of equally generous build, but all other accounts of her describe her as being of normal build) and they both joined a travelling circus.They were for some time compelled to find subsistence by performing exhibitions of feats of strength and agility as a strongman at fairs and on the streets of London. One trick he was famous for, was to lift a platform holding twelve people and carry it across the stage. In 1804 he appears engaged at the circus at Astley’s amphitheatre at a variety of performances. Belzoni also had an interest in phantasmagoria and experimented with the use of magic lanterns in his shows.

In 1812 he left England and after a tour of performances in Spain, Portugal and Sicily, he went to Malta in 1815 where he met Ismael Gibraltar, an emissary of Muhammad Ali, who at the time was undertaking a programme of agrarian land reclamation and important irrigation works. Belzoni wanted to show Muhammad Ali a hydraulic machine of his own invention for raising the waters of the Nile. Though the experiment with this engine was successful, the project was not approved by the pasha. Belzoni, now without a job, was resolved to continue his travels. On the recommendation of the orientalist, J. L. Burckhardt, he was sent by Henry Salt, the British consul to Egypt, to the Ramesseum at Thebes, from where he removed with great skill the colossal bust of Ramesses II, commonly called “the Young Memnon”.
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Jonas Hanway: A Man with a Plan

Portrait of Jonas Hanway by James Northcote, circa 1785.
Portrait of Jonas Hanway by James Northcote, circa 1785.
Portrait of Jonas Hanway by James Northcote, circa 1785.

Jonas Hanway (August 12, 1712 – September 5, 1786), English traveller and philanthropist, was born at Portsmouth, on the south coast of England.

While he was still a child his father, a victualler, died, and the family moved to London. In 1729 Jonas was apprenticed to a merchant in Lisbon. In 1743, after he had been some time in business for himself in London, he became a partner with Mr Dingley, a merchant in St Petersburg, and in this way was led to travel in Russia and Persia. Leaving St Petersburg on 10 September 1743, and passing south by Moscow, Tsaritsyn and Astrakhan, he embarked on the Caspian Sea on 22 November and arrived at Astrabad on 18 December. Here his goods were seized by Mohammed Hassan Beg, and it was only after great privations that he reached the camp of Nadir Shah, under whose protection he recovered most (85%) of his property.

His return journey was embarrassed by sickness (at Resht), by attacks from pirates, and by six weeks’ quarantine; and he only reappeared at St Petersburg on 1 January 1745. He again left the Russian capital on 9 July 1750 and travelled through Germany and the Netherlands to England (28 October). The rest of his life was mostly spent in London, where the narrative of his travels (published in 1753) soon made him a man of note, and where he devoted himself to philanthropy and good citizenship.

11-35_2

In 1756, Hanway founded The Marine Society, to keep up the supply of British seamen; in 1758, he became a governor of the Foundling Hospital, a position which was upgraded to vice president in 1772; he was instrumental in establishing the Magdalen Hospital; in 1761 he procured a better system of parochial birth registration in London; and in 1762 he was appointed a commissioner for victualling the navy (10 July); this office he held till October 1783. He died, unmarried, on 5 September 1786 and is now buried in the crypt at St. Mary’s Church, Hanwell.
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Sir Thomas Stamford Raffles: Founder of the City of Singapore, Father of the London Zoo

thomas

thomasSir Thomas Stamford Raffles, FRS (6 July 1781 – 5 July 1826) was a British statesman, best known for his founding of the city of Singapore (now the city-state of the Republic of Singapore) and the London Zoo. He is often described as the “Father of Singapore” and the “Father of the London Zoo”. He was also heavily involved in the conquest of the Indonesian island of Java from Dutch and French military forces during the Napoleonic Wars and contributed to the expansion of the British Empire. He was also an amateur writer and wrote a book titled History of Java (1817).

Raffles was born on the ship Ann off the coast of Port Morant, Jamaica, to Captain Benjamin Raffles (d. June 1797) and Anne Raffles (née Lyde). His father was a Yorkshireman who had a burgeoning family and little luck in the West Indies trade during the American Revolution, sending the family into debt. The little money the family had went into schooling Raffles. He attended a boarding school. In 1795, at the age of 14, Raffles started working as a clerk in London for the British East India Company, the trading company that shaped many of Britain’s overseas conquests. In 1805 he was sent to what is now Penang in the country of Malaysia, then called the Prince of Wales Island, starting his long association with Southeast Asia. He started with a post under the Honourable Philip Dundas, the Governor of Penang. He was appointed assistant secretary to the new Governor of Penang in 1805 and married Olivia Mariamne Fancourt, a widow who was formerly married to Jacob Cassivelaun Fancourt, an assistant surgeon in Madras who had died in 1800. At this time he also made the acquaintance of Thomas Otho Travers, who would accompany him for the next twenty years.

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Jane Austen Waxwork

Jane Austen Waxwork

We had a great time unveiling our new Jane Austen waxwork to the assembled media folk on Wednesday 9th of July.

L to R. Andrea Galer, Mark Richards, David Baldock, Jane Austen and Melissa Dring
L to R. Andrea Galer, Mark Richards, David Baldock, Jane Austen and Melissa Dring

Reaction was overwhelmingly positive when the curtains were parted. The waxwork is now on public display. Developed from a forensic portrait of the author by Melissa Dring, the waxwork has been over 2 years in the making. Members of the team behind her creation, especially brought together for the project, were in attendance at the event, – the internationally-renowned sculptor, an FBI-trained forensic artist and a Bafta and Emmy award-winning costume designer. (See their biographies below) The novels of Jane Austen are known throughout the world, her heroes and heroines have been brought to life in many adaptations, and the industry which has built up around her name is significant. So whilst people happily associate Jane Austen’s characters with the actors who portray them, perhaps most famously Colin Firth as Mr Darcy, there remains a real desire to possess a likeness of the writer herself.

Uncovering the Real Jane Austen (taster) from Grace Productions on Vimeo.

The only verifiable image of Jane Austen is a small watercolour painted by her sister Cassandra but it has been acknowledged by experts as a poor attempt and was described by her niece as ‘hideously unlike’ her aunt Jane. However, there are many contemporary descriptions of her by friends and this is where the Jane Austen Centre enters the picture. The chance reading in 2002 of an article about forensic artist Melissa Dring’s work in creating a likeness of the composer Vivaldi from eye-witness accounts spurred David Baldock, Director of The Jane Austen Centre, into action. David contacted and commissioned Melissa to create a new portrait of Jane. And then a year later, David engaged handwriting expert Patricia Field to reveal further aspects of Jane’s character through a ‘blind’ study of handwriting samples.
waxwork head and shoulders (low res)
Inspired by the overwhelming positive response to these additional pieces of the jigsaw that is Austen’s life and to address the continuing, near insatiable demand for further revelations, David has now taken this process one step further and commissioned a three-dimensional, life-size wax figure. waxwork with real person (low res)The Jane Austen Waxwork is based on the 2002 portrait and its creation has been undertaken by internationally-renowned portrait sculptor Mark Richards. The figure has been dressed in authentic-period costume by Bafta & Emmy award-winning designer Andrea Galer, while the finishing touches have been completed by ex-Madame Tussaud’s hair and colour artist Nell Clarke. The figure is to be displayed at a specially created space within the Jane Austen Centre, in Bath. As the popularity of her work and interest in her life has never been greater, and the modern-day Jane Austen fan (or Janeite) can be very opinionated to the point of over-protectiveness, with some going so far as to see themselves as the self-appointed guardians of her image, this figure is almost certain to provoke controversy. Ultimately though, the Jane Austen Waxwork will hopefully take admirers of her work that one step closer to finally revealing exactly what Jane Austen looked liked.

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Dido Elizabeth Belle

MM03264

MM03264Dido Elizabeth Belle (1761–1804), was an illegitimate daughter of Admiral Sir John Lindsay and an enslaved African woman known as Maria Belle. Dido was sent to live in the household of William Murray, 1st Earl of Mansfield, who was Lindsay’s uncle and thus Dido’s great-uncle. Remarkably, she was brought up as a free young gentlewoman at Kenwood House at the same time as her great-uncle, in his capacity as Lord Chief Justice, was called on to rule on cases affecting the legitimacy of the slave trade.

Born around 1761, she was baptised in 1766 at St. George’s Church, Bloomsbury. Her baptism record shows that she was born while her father, John Lindsay, was in the West Indies and that her mother’s name was Maria Belle. It has been suggested that her mother was an African slave captured from a Spanish ship during the capture of Havana from the Spanish in 1762.Lindsay was at the time a Royal Navy captain on HMS Trent, a warship based in the West Indies that took part in the battle. This is uncertain, however, as there is no reason why any of the Spanish ships (which were immobilised in the inner harbour) would have had women on board when they were delivered up on the formal surrender of the fortress.

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Horace Walpole: Regency Author, Historian, Antiquarian and Politician

Horace Walpole by Joshua Reynolds, 1756
Horace Walpole by Joshua Reynolds, 1756
Horace Walpole by Joshua Reynolds, 1756

Horatio Walpole, 4th Earl of Orford (24 September 1717 – 2 March 1797) was an English art historian, man of letters, antiquarian and Whig politician.

He is now largely remembered for Strawberry Hill, the home he built in Twickenham, south-west London where he revived the Gothic style some decades before his Victorian successors, and for his Gothic novel, The Castle of Otranto. Along with this book, his literary reputation rests on his Letters, which are of significant social and political interest.

Walpole was born in London, the youngest son of British Prime Minister Sir Robert Walpole and his wife Catherine. Like his father, he received early education in Bexley he was also educated at Eton College and King’s College, Cambridge.

Walpole’s first friends were probably his cousins Francis and Henry Conway, to whom Walpole became strongly attached, especially Henry. At Eton he formed with Charles Lyttelton and George Montagu the “Triumvirate”, a schoolboy confederacy. More important were another group of friends dubbed the “Quadruple Alliance”: Walpole, Thomas Gray, Richard West and Thomas Ashton.

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Parson Woodforde: Country Diarist

James Woodforde by his nephew Samuel Woodforde.
James Woodforde by his nephew Samuel Woodforde.
James Woodforde by his nephew Samuel Woodforde.

James Woodforde (1740–1803) was an English clergyman who was nearly an exact contemporary of Jane Austen’s father, George Austen (1731–1805). Best known as the author of The Diary of a Country Parson, his personal recollections of life as clergyman in the Georgian countryside give a valuable glimpse into what the Austen household might have been like.

James Woodforde was born at the Parsonage, Ansford, Somerset, England on 27 June 1740. In adulthood he led an uneventful, unambitious life as a clergyman of the Church of England: a life unremarkable but for one thing — for nearly 45 years he kept a diary recording an existence the very ordinariness of which provides a unique insight into the everyday routines and concerns of 18th century rural England.

The sixth child of the Reverend Samuel Woodforde, rector of Ansford and vicar of Castle Cary, and his wife Jane Collins, James was one of four brothers (one of whom died in infancy) and the only one to attend public school — Winchester College, and university — Oxford. He was admitted to Winchester as a scholar in 1752 and enrolled at Oriel College, Oxford in 1758, migrating to New College in the following year. His diary begins with the entry for 21 May 1759: “Made a Scholar of New College”.

Woodforde was ordained and graduated BA in 1763, became MA in 1767 and BD in 1775. He appears to have been a competent but uninspired student and the portrait he provides of Oxford during his two periods of residence as scholar and fellow (from 1758–1763 and from 1773–1776) only confirm Edward Gibbon’s famously damning opinion that it was a place where the dons’ “dull and deep potations excuse the brisk intemperance of youth”. The diary is a rich source of information on university life in eighteenth-century Oxford.

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