Solar eclipse of June 8, 1918

Source: Wikipedia, the free encyclopedia.
Solar eclipse of June 8, 1918
UTC)
Greatest eclipse22:07:43
References
Saros126 (42 of 72)
Catalog # (SE5000)9324

A total solar eclipse occurred on Saturday, June 8, 1918. The eclipse was viewable across the entire contiguous United States, an event which would not occur again until the solar eclipse of August 21, 2017.

The path

Animated path

The path of totality started south of

Bahamas) on June 8 (Saturday). The largest city to see totality was Denver, although many could theoretically see it as the size of the shadow was between 70 and 44 miles (113 and 71 km) across as it traveled across America. The longest duration of totality was in the Pacific at a point south of Alaska. The path of the eclipse finished near Bermuda.[1]

Besides the path where a total solar eclipse was visible, a partial solar eclipse was visible in the eastern part of

Hawaii Islands, northeastern Russian Empire, the entire North America except the Lesser Antilles, and the northwestern tip of South America
.

1918 Solar eclipse painting by Howard Russell Butler

U.S. Observation team

Baker City, Oregon
, in 1918.

The path of the eclipse clipped

U.S. Naval Observatory (USNO) obtained a special grant of $3,500 from Congress for a team to observe the eclipse in Baker City, Oregon. The team had been making preparations since the year before, and John C. Hammond led the first members to Baker City on April 11.[2] The location was important, as it influenced the probability of cloud cover and the duration and angle of the sun during the eclipse. The team included Samuel Alfred Mitchell as its expert on eclipses, and Howard Russell Butler, an artist and physicist. In a time before reliable colour photography, Butler's role was to paint the eclipse at totality after observing it for 112.1 seconds.[3] He noted later that he used a system of taking notes of the colours using skills he had learned for transient effects.[3]

University of Illinois Observatory made the first photoelectric photometric observations of the solar corona from their observing site near Rock Springs, Wyoming [4]

Observation

As the total eclipse approached, the team watched as clouds obscured the Sun. The clouds did clear, but during their most important observations the Sun was covered by a thin cloud; the Sun was completely visible five minutes later.[2] This was not unusual, as cloudy conditions were reported across the country, where the eclipse was also observed from the Yerkes Observatory, Lick Observatory, and Mount Wilson Observatory.[5]

Following the 1915 prediction of Albert Einstein's General theory of relativity that light would be deflected when passing near a massive object such as the Sun, the USNO expedition attempted to validate Einstein's prediction by measuring the position of stars near the Sun. The cloud cover during totality obscured observations of stars,[6] though, preventing this test of the validity of general relativity from being completed until the solar eclipse of May 29, 1919.

Related eclipses

There were two other eclipses that year. The first was a partial lunar eclipse, during which the shadow of the Earth can be seen on the Moon, and another solar eclipse that took place on December 3 over South America.[1] The other solar eclipse, however, was an annular eclipse, which occurs when the Moon has a smaller apparent diameter and therefore never fully obscures the Sun.

Solar eclipses of 1916–1920

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[7]

Solar eclipse series sets from 1916 to 1920
Ascending node   Descending node
111
December 24, 1916

Partial 		116 June 19, 1917

Partial
121 December 14, 1917

Annular 		126 June 8, 1918

Total
131 December 3, 1918

Annular 		136 May 29, 1919

Total
141 November 22, 1919

Annular 		146 May 18, 1920

Partial
151 November 10, 1920

Partial

Saros 126

It is a part of Saros cycle 126, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810, hybrid eclipses from April 14, 1828 through May 6, 1864 and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. The longest duration of central eclipse (annular or total) was 6 minutes, 30 seconds of annularity on June 26, 1359. The longest duration of totality was 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occurs at the Moon’s descending node.

Series members 42–52 occur between 1901 and 2100
42 43 44

June 8, 1918
June 19, 1936
June 30, 1954
45 46 47

July 10, 1972
July 22, 1990
August 1, 2008
48 49 50

August 12, 2026
August 23, 2044
September 3, 2062
51 52

September 13, 2080
September 25, 2098

Notes

  1. ^
    Bibcode:1918JRASC..12..160M
    .
  2. ^ a b Lawrence, Jenny; Richard Milner (February 2000). "A Forgotten Cosmic Designer". Natural History. Retrieved 19 October 2010.
  3. Bibcode:1918PA.....26..665S
    .
  4. doi:10.1038/102089a0
    .
  5. ^ Siegel, Ethan (2007). "America's Previous Coast-To-Coast Eclipse Almost Proved Einstein Right", Forbes, August 4, 2017, retrieved 24 April 2022.
  6. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

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