Abstract
‘Modern astronomy’ was introduced to Siam (present-day Thailand) (Siam officially changed its name to Thailand in 1939) when the Belgian Jesuit missionary-astronomer Father Antoine Thomas carried out stellar and lunar eclipse observations during 1681 and 1682 in order to determine the latitude and longitude of Ayutthaya. Three years later a contingent of French Jesuit missionary astronomers observed a total lunar eclipse from Lop Buri, which marked the start of an intensive two-and-a-half year period of observational activity at Lop Buri under the sponsorship of King Narai. During this interval, a partial solar eclipse and two further lunar eclipses were observed from a number of different observing sites. Although a substantial astronomical observatory was constructed in Lop Buri and this was used by French Jesuit missionary-astronomers, ‘modern astronomy’ ended suddenly in 1688 when King Narai died and most Western missionary-astronomers were expelled from Siam.
‘Modern astronomy’ only re-emerged in Siam after a hiatus of almost 200 years when another royal supporter of astronomy, King Rama IV, invited French astronomers to observe the total solar eclipse of 18 August 1868 from Siam, and his son, King Rama V, hosted British astronomers during the 6 April 1875 total solar eclipse. Thailand’s romance with total solar eclipses continued during the 9 May 1929 solar eclipse when King Rama VII visited British and German astronomers based near Siam’s southern border, and this was the catalyst required for the birth of home-grown ‘modern astronomy’. Soon after, Siam’s first astronomy classes began at Chulalongkorn University, and in 1944 this university hosted Siam’s first professional astronomer when Rawee Bhavilai, a solar specialist, joined the Physics Department. The latest phase in the professionalisation of astronomy occurred in 2009 when the Government approval the formation of the National Astronomical Research Institute of Thailand (NARIT).
In this paper we trace the critical roles that solar and lunar eclipses played in the emergence and final adoption of ‘modern astronomy’ in Thailand from 1682 through to the present day.
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Notes
- 1.
All of the times listed in Tables 2, 3, 5, 7 and 9 were calculated using Herald’s OCCULT v3.6 and the NASA Catalog, which agreed to within 1 min in all instances. ‘Local Time’ was defined as UT + 7 h. The Jesuits in Siam in the seventeenth century used local apparent solar time for their eclipse timings. This means that for instance the times given in the table for the 1685 lunar eclipse, for comparison with the timings of the Jesuits should be corrected by −18 min to account for the time difference between the 7 h meridian (105° E) and the meridian of Lop Buri (100.65° E). Additionally, they should be corrected by +6 min by the equation of time to get apparent solar time. The start of the totality, 4:37, will then be corrected to 4:25 local apparent solar time and the time of the end of the totality, 6:21, will be corrected to 6:09, both of which are very close to the times actually reported by the Jesuits.
- 2.
- 3.
- 4.
Note that Fig. 4 is an updated version of Fig. 14 that was published in Orchiston et al. 2016: 39. In Fig. 4 the revised boundary of the water reservoir is now based on the cadastral map that was prepared by A.J. Irwin in the 1890s, but was unavailable when the 2016 paper was researched and written.
- 5.
- 6.
The prostrated individuals in this drawing are King Narai’s court astrologers.
- 7.
- 8.
There is confusion over the correct spelling of Wat San Paulo, with both this (correct) version and ‘Wat San Paolo’ featuring at different times on different interpretive panels at the site itself! Even Soonthornthum (2011: 181) mistakenly uses Wat San Paolo.
- 9.
In fact, by this time only one observatory had been built (cf. Hodges, 1999). Moreover, part of the massive building shown in Fig. 6 was still under construction when Constantine Phaulkon and King Narai died in June and July 1688 respectively (Smithies 2003). Because of their passing, the planned Ayutthaya observatory was never built.
- 10.
This was only 35 s shorter than the longest possible duration of totality of a total solar eclipse, which is 7 min 32 s.
- 11.
Other spellings of his name are Rawee Bhavilai and Rawī Phāwilai.
- 12.
For details of NARIT’s education and outreach accomplishments see Soonthornthum (2017).
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Acknowledgements
We wish to thank Visanu Euarchukiati (Bangkok, Thailand) for locating a copy of A.J. Irwin’s cadastral map of Lop Buri and making this available to us (so that we could prepare Fig. 4). Apart from the calculations for Tables 2, 3, 5, 7 and 9, which were performed by the third author of this paper, research on the seventeenth century eclipses was largely based on data gathered by the first two authors during a detailed literature survey and on three visits to Lop Buri and Ayutthaya in 2014 and 2015. We are grateful to staff from the Lop Buri City Hall, and the Department of Fine Arts at Kraisorm Siharat Pavilion (the ‘Water Reservoir Palace’ in Lop Buri) for their assistance. Finally, we wish to thank the King Prajadhipok Museum, Office of the National Research Council of Thailand, Observatoire de Marseille and the Royal Astronomical Society for kindly supplying Figs. 12, 17, 18, 22, 23 and 24.
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Orchiston, W. et al. (2019). The Role of Eclipses and European Observers in the Development of ‘Modern Astronomy’ in Thailand. In: Orchiston, W., Sule, A., Vahia, M. (eds) The Growth and Development of Astronomy and Astrophysics in India and the Asia-Pacific Region. Astrophysics and Space Science Proceedings, vol 54. Springer, Singapore. https://doi.org/10.1007/978-981-13-3645-4_14
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