Solar eclipse of July 28, 1851

Solar eclipse of July 28, 1851
Solar eclipse of July 28, 1851
	Berkowski made this first solar eclipse photograph at the Royal Observatory in Königsberg, Prussia (now Kaliningrad, Russia)
	Map
Type of eclipse
Nature	Total
Gamma	0.7644
Magnitude	1.0577
Maximum eclipse
Duration	221 s (3 min 41 s)
Coordinates	68°00′N 19°36′W / 68°N 19.6°W
Max. width of band	296 km (184 mi)
Times (UTC)
Greatest eclipse	14:33:42
References
Saros	143 (14 of 72)
Catalog # (SE5000)	9167

The earliest scientifically useful photograph of a total solar eclipse was made by Julius Berkowski at the Royal Observatory in Königsberg, Prussia, on July 28, 1851. This was the first occasion that an accurate photographic image of a solar eclipse was recorded.

Background

A solar eclipse occurs when the Moon passes between the Earth and the Sun, casting a shadow on Earth that temporarily obscures part or all of the Sun's disc. Eclipses can occur only when all three bodies are properly aligned. Partial eclipses, in which only a portion of the Sun's surface is obscured, are relatively common due to the width of the Moon's outer shadow, or penumbra, which may be several hundred miles wide. Total eclipses occur when the Moon's inner shadow, or umbra, reaches the surface of the Earth, completely obscuring the Sun over a much narrower portion of the ground. If the Moon is too far away at the time of an eclipse, its umbra may not reach the Earth's surface, and only a partial eclipse will be visible.

Before the advent of modern science, solar eclipses were often viewed with superstitious dread. However, eclipses are also of interest to science due to the various phenomena that can be observed when they occur. The Sun's outer atmosphere, or corona, is normally invisible due to the brightness of the solar disc, but becomes visible from Earth during a total eclipse. Until the twentieth century, solar eclipses provided the only opportunity for scientists to observe and study the Sun's corona. With the development of photography during the first half of the nineteenth century, it became theoretically possible to record a still image of the Sun during a total eclipse. A variety of processes were used for early photographs, of which the most successful was the Daguerreotype.

Monday, July 28, 1851

Photographing a rare event such as a total eclipse posed unique challenges for early photography, including the extreme contrast between the corona and the dark shadow of the Moon, as well as the unusual angle to which photographic equipment had to be oriented. Prior to the eclipse of July 28, 1851, no properly exposed photograph of the solar corona had yet been produced. For this occasion, the Royal Prussian Observatory at Königsberg (now Kaliningrad, Russia) commissioned one of the city's most skilled daguerreotypists, Johann Julius Friedrich Berkowski, to record a still image of the event.^[1] The observers attached a small six-centimeter refracting telescope to a 15.8 centimeter Fraunhofer heliometer, and Berkowski made an eighty-four second exposure shortly after the beginning of totality.^[2]

Among the other observers were British astronomers Robert Grant and William Swan, and Austrian astronomer Karl Ludwig von Littrow. They deduced that prominences were part of the Sun, because the Moon was seen to cover and uncover them as it moved in front of the Sun.^[3]^{[better source needed]}

Related eclipses

The eclipse of July 28, 1851 was part of Saros Series 143, a sequence of seventy-two partial and total solar eclipses occurring between 1617 and 2897. The only total eclipses in this cycle occurred between 1797 and 1995.^[4]

References

^ Axel D. Wittmann and Reinhard E. Schielicke (2013). "Richard und John Parish, Förderer der Astronomie zur Zeit von Gauß, und die Sonnenfinsternis–Daguerreotypie von Julius Berkowski (1851)" (PDF). University of Jena, Astrophysical Institute and University Observatory. Archived from the original (PDF) on 2015-04-02. Retrieved 2015-03-22.
^ Schielicke, Reinhard; Wittmann, Axel D. (2005). "On the Berkowski daguerreotype (Königsberg, 1851 July 28): the first correctly-exposed photograph of the solar corona". Acta Historica Astronomiae. 25: 128. Bibcode:2005AcHA...25..128S.
^ "Chronology of Discoveries about the Sun". www.mreclipse.com.
^ National Aeronautics and Space Administration, "Saros Series 143", in Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site, retrieved 10 November 2016.

External links

[1] Axel D. Wittmann and Reinhard E. Schielicke (2013). "Richard und John Parish, Förderer der Astronomie zur Zeit von Gauß, und die Sonnenfinsternis–Daguerreotypie von Julius Berkowski (1851)" (PDF). University of Jena, Astrophysical Institute and University Observatory. Archived from the original (PDF) on 2015-04-02. Retrieved 2015-03-22.

[2] Schielicke, Reinhard; Wittmann, Axel D. (2005). "On the Berkowski daguerreotype (Königsberg, 1851 July 28): the first correctly-exposed photograph of the solar corona". Acta Historica Astronomiae. 25: 128. Bibcode:2005AcHA...25..128S.

[3] "Chronology of Discoveries about the Sun". www.mreclipse.com.

[4] National Aeronautics and Space Administration, "Saros Series 143", in Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site, retrieved 10 November 2016.

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