British Astronomical Association


The British Astronomical Association was formed in 1890 as a national body to support the UK's amateur astronomers.
Throughout its history, the BAA has encouraged observers to make scientifically valuable observations, often in collaboration with professional colleagues. Among the BAA's first presidents was Walter Maunder, discoverer of the seventeenth century dearth in sunspots now known as the Maunder Minimum which he achieved by analysing historical observations. Later, this spirit of observing the night sky scientifically was championed by George Alcock, who discovered five comets and five novae using nothing more than a pair of binoculars.
The BAA continues to contribute to the science of astronomy, even despite modern competition from space-based telescopes and highly automated professional observatories. Modern digital sensors, coupled with techniques such as lucky imaging, mean that even modest amateur equipment can rival what professional observatories could have achieved a few decades ago. The vastness of the night sky, together with the sheer number of amateur observatories, mean that BAA members are often the first to pick up new phenomena. In recent years, the Association's leading supernova hunter, Tom Boles, has discovered over 150 supernovae. He now holds the world record for the greatest number of such events discovered by any individual in history.
More recently the BAA has worked increasingly with international partners. Modern communications allow astronomers in different time zones around the world to hand over the monitoring of variable stars and planetary weather systems to colleagues on other continents as the Sun comes up, resulting in a 24-hour watch on the sky. For example, the Association's works closely with the American Association of Variable Star Observers, meanwhile its works with a global network of planetary observers through the .

Publications

The Association's longest standing publication is its , published six times a year and sent to all members. Once a year, the Association also publishes a which comprises an almanac for the following year. Electronic bulletins are issued to give more immediate notice by email of discoveries, astronomical news and BAA meetings.

Structure

The Association operates a wide range of which specialise in particular branches of astronomy, welcoming observers and astronomy enthusiasts of all abilities in a spirit of collaboration and mutual help.
It also founded and supports the Campaign for Dark Skies, a UK-wide campaign against excessive light pollution.
The BAA leases office space from the Royal Astronomical Society, in Burlington House, Piccadilly, London. Many of its meetings are also held there.

History

In October 1890, the BAA was formed to support amateur astronomers in the UK. In many ways it is a counterpart to the Royal Astronomical Society - which primarily supports professional observers - and the two organisations have long shared the same premises. The idea for this organisation was first publicly proposed by Irish astronomer William H. S. Monck in a letter published in The English Mechanic on July 12.
Playing a significant role in the founding of the Association was English astronomer E. Walter Maunder, with the help of his brother Frid Maunder and William H. Maw. The first meeting of the Association was held on 1890 October 24, with 60 of the initial 283 members in attendance. Initially it was decided to run the association with a provisional 48-member Council that included four women: Margaret Huggins, Elizabeth Brown, Agnes Clerke and Agnes Giberne.
The society formed several observing Sections for specialised topics in astronomy. Elizabeth Brown, possibly the only woman in England at the time to own her own observatory, became head of the Solar Section. The Association was presented with or bequeathed various astronomical instruments, but lacked the funds to build their own observatory. A total of 477 instruments were acquired during the first 117 years since the Association was founded.

Branches

The Association held monthly meetings in London, but also established branches to cater for members who could not attend London activities and desired to meet in their own areas.
The first of these was the Northwestern Branch which served members in the Northwest of England, centred on Manchester. The Branch was formed in 1892, in 1903 it seceded from the BAA to form the Manchester Astronomical Society.
In 1891, a group of amateurs in Australia began discussing the idea of setting up branches of the BAA in their own country. What would become the New South Wales Branch was established in 1895 and would be the only one to survive for more than a brief period. This branch became the second oldest astronomy organisation in Australia and is still in existence.
A West of Scotland Branch was established by an inaugural meeting held on 23 November 1894, to be based in Glasgow. In 1905 authority was granted to enrol members from the whole of Scotland, but it was not until 1937 that the name was changed to "Scottish Branch". In 1954 the Branch seceded from the BAA to form the Astronomical Society of Glasgow.
In 1896 an East of Scotland Branch was formed. This Branch was dissolved due to lack of support on 3 October 1902.
In 1897 a second Australian Branch was formed by 13 members living in Victoria. At the London AGM of 1907 the President noted that "the Victoria Branch appears to be in a moribund condition".
The Victoria Branch was re-established in 1951, but only lasted until 1963.
In 1901 at a meeting of the Birmingham Natural History and Philosophical Society it was proposed to form a Midland Branch of the BAA. Support proved to be less than had been envisioned and there are no reports of any activity after 1903.
What would become the BAA Western Australia Branch started as the Western Australian Astronomical Society in 1912. When difficulties were encountered in the mid nineteen-twenties Prof. Ross highlighted the advantages of restarting within the BAA. The inaugural meeting was held on 29 March 1927. However support was still lacking and there is no recorded activity after September 1929.

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