Solar eclipse of August 18, 1868

Solar eclipse of August 18, 1868
Map
Type of eclipse
Nature Total
Gamma -0.0443
Magnitude 1.0756
Maximum eclipse
Duration 407 sec (6 m 47 s)
Coordinates 10°36′N 102°12′E / 10.6°N 102.2°E / 10.6; 102.2
Max. width of band 245 km (152 mi)
Times (UTC)
Greatest eclipse 5:12:10
References
Saros 133 (37 of 72)
Catalog # (SE5000) 9207

A total solar eclipse occurred on August 18, 1868. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

Observations

Captain Bullock observed from the Celebes sea, sketching the appearance of the corona,[1] while Gustav Fritsch accompanied an expedition to Aden.[2]

Discovery of helium

French astronomer Pierre Janssen observed the eclipse from Guntur in Madras State, British India. It was the first total eclipse since Gustav Kirchhoff's 1859 theory that the Fraunhofer lines in the solar spectrum correspond to the emission line of the different chemical elements present in the Sun. Correspondingly, Janssen observed the eclipse with the aid of a spectroscope. He noticed a bright yellow line (λ = 587.49 nm) in the spectra of the solar prominences that could not be due to sodium as had previously been assumed, and was subsequently able to observe the same line even without the need for an eclipse. The same result was found independently by British astronomer Norman Lockyer, and both Janssen's and Lockyer's communications were presented to the French Academy of Sciences on October 26, 1868.[3][4]

King Mongkut's calculation

King Mongkut, King of Siam, was able to calculate and predict the solar eclipse two years earlier.[5] The calculations were correct as to the place, the time and the type of the solar eclipse that would happen. The eclipse took place precisely as the King had predicted, the total phase lasting six minutes and 46 seconds. In fact, his calculations were better — by about two seconds — than those of the French astronomers, who acknowledged his accuracy. Court astrologers, however, were also correct that the event portended disaster. To get as close as possible to the centre of the shadow cone, the pavilion for his expedition to observe the event was put on low ground in a mosquito-infested spot: Malaria struck widely among those who had attended. Shortly after he reached Bangkok, Mongkut developed chills and fever. He died on October 18, 1868.[6] According to the Thai Astronomical Society, the international astronomical community calls the eclipse "King of Siam's eclipse".[5]

Related eclipses

It is a part of solar Saros 133.

Notes

  1. ↑ The Indian eclipse, 1898 Report of the expeditions organized by the British ... By Edward Walter Maunder, British Astronomical Association
  2. ↑ Standard Encyclopaedia of Southern Africa
  3. ↑ Leggett, Hadley (August 18, 2009), Aug. 18, 1868: Helium Discovered During Total Solar Eclipse, wired.com, retrieved 2010-03-18.
  4. ↑ "Comptes rendus hebdomadaires des séances de l'Académie des sciences", C. R. Hebd. Acad. Sci. Paris 67, 1868: 836–41.
  5. 1 2 ๒๐๐ ปี พระบาทสมเด็จพระจอมเกล้าเจ้าอยู่หัว พระบิดาแห่งวิทยาศาสตร์ไทย. (Thai)
  6. ↑ Montes-Bradley, Saul M.; Bradley, W.L. (10 January 2006). "Descendants of Danyell Broadley de West Morton". Eighth Generation. Thomas Osgood Bradley Foundation. Archived from the original (964-word excerpt from Siam then, the foreign colony in Bangkok before and after Anna, Pasadena, California, 1981.) on 2013-08-09. Retrieved 9 August 2013. King Mongkut's prediction surpassed those of European scientists. "In the 19th century, King Mongkut of Siam (now Thailand), an amateur astronomer, paid the ultimate price for eclipse-chasing: his life. line feed character in |quote= at position 66 (help)

References

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