Solar eclipse of February 3, 1916

Last updated
Solar eclipse of February 3, 1916
Solar eclipse of February 3, 1916 (cropped).png
SE1916Feb03T.png
Map
Type of eclipse
NatureTotal
Gamma 0.4987
Magnitude 1.028
Maximum eclipse
Duration156 sec (2 m 36 s)
Coordinates 11°06′N67°42′W / 11.1°N 67.7°W / 11.1; -67.7
Max. width of band108 km (67 mi)
Times (UTC)
Greatest eclipse16:00:21
References
Saros 139 (24 of 71)
Catalog # (SE5000) 9317

A total solar eclipse occurred on February 3, 1916. [1] [2] [3] [4] [5] [6] [7] 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. Totality was visible in Colombia, Venezuela, and the whole Guadeloupe except Marie-Galante, Saint Martin and Saint Barthélemy.

Contents

Solar eclipse 1913–1917

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. [8]

Solar eclipse series sets from 1913–1917
Descending node Ascending node
114 August 31, 1913
SE1913Aug31P.png
Partial
119 February 25, 1914
SE1914Feb25A.png
Annular
124 August 21, 1914
SE1914Aug21T.png
Total
129 February 14, 1915
SE1915Feb14A.png
Annular
134 August 10, 1915
SE1915Aug10A.png
Annular
139 February 3, 1916
SE1916Feb03T.png
Total
144 July 30, 1916
SE1916Jul30A.png
Annular
149 January 23, 1917
SE1917Jan23P.png
Partial
154 July 19, 1917
SE1917Jul19P.png
Partial

Saros 139

It is a part of saros series 139, repeating every 18 years, 11 days, 8 hours, containing 71 events. The series started with partial solar eclipse on May 17, 1501. It contains hybrid eclipses on August 11, 1627 through to December 9, 1825 and total eclipses from December 21, 1843 through to March 26, 2601. The series ends at member 71 as a partial eclipse on July 3, 2763. Its eclipses are entabulated in three columns; each one in the same column, every third eclipse, is one exeligmos apart so cast shadows over approximately the same parts of the Earth.

The solar eclipse of June 13, 2132 will be the longest total solar eclipse since July 11, 1991 at 6 minutes, 55.02 seconds.

The longest duration of totality will be produced by member 39 at 7 minutes, 29.22 seconds on July 16, 2186. [9] After that date each duration will decrease, until the series end. This date is the longest solar eclipse computed between 4000 BC and 6000 AD. [10] Saros series eclipses are during the Moon’s ascending node (a term related to our equator and polar-naming conventions).

Series members 24–45 occur between 1901 and 2300
242526
SE1916Feb03T.png
February 3, 1916
SE1934Feb14T.png
February 14, 1934
SE1952Feb25T.png
February 25, 1952
272829
SE1970Mar07T.png
March 7, 1970
SE1988Mar18T.png
March 18, 1988
SE2006Mar29T.png
March 29, 2006
303132
SE2024Apr08T.png
April 8, 2024
SE2042Apr20T.png
April 20, 2042
SE2060Apr30T.png
April 30, 2060
333435
SE2078May11T.png
May 11, 2078
SE2096May22T.png
May 22, 2096
SE2114Jun03T.png
June 3, 2114
363738
SE2132Jun13T.png
June 13, 2132
SE2150Jun25T.png
June 25, 2150
SE2168Jul05T.png
July 5, 2168
394041
SE2186Jul16T.png
July 16, 2186
SE2204Jul27T.png
July 27, 2204
SE2222Aug08T.png
August 8, 2222
424344
SE2240Aug18T.png
August 18, 2240
SE2258Aug29T.png
August 29, 2258
SE2276Sep09T.png
September 9, 2276
45
SE2294Sep20T.png
September 20, 2294

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Notes

  1. "The Total Solar Eclipse of Feb. 3". Janesville Daily Gazette. Janesville, Wisconsin. 1916-02-03. p. 3. Retrieved 2023-12-02 via Newspapers.com.
  2. "To-day's sunset eclipse. The position of Cornwall; longest view in England". The West Briton. Truro, Cornwall, England. 1916-02-03. p. 7. Retrieved 2023-12-02 via Newspapers.com.
  3. "DOES PATH OF SUN'S ECLIPSE PORTEND EARLY END OF WAR? SOME FOLKS THINK SO". Nashville Banner. Nashville, Tennessee. 1916-02-03. p. 13. Retrieved 2023-12-02 via Newspapers.com.
  4. "Don't Worry If You Didn't See Sun's Eclipse For There Are To Be Others". The Cincinnati Post. Cincinnati, Ohio. 1916-02-03. p. 1. Retrieved 2023-12-02 via Newspapers.com.
  5. "PHENOMENON IN SKY ON HEELS OF STORM". The York Dispatch. York, Pennsylvania. 1916-02-03. p. 2. Retrieved 2023-12-02 via Newspapers.com.
  6. "Many See Partial Eclipse". The Washington Herald. Washington, District of Columbia. 1916-02-04. p. 12. Retrieved 2023-12-02 via Newspapers.com.
  7. "Eclipse of Sun Photographed Through 6-Inch Telescope". St. Louis Post-Dispatch. St. Louis, Missouri. 1916-02-04. p. 2. Retrieved 2023-12-02 via Newspapers.com.
  8. 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.
  9. Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.
  10. Ten Millennium Catalog of Long Solar Eclipses, −3999 to +6000 (4000 BCE to 6000 CE) Fred Espenak.

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of June 21, 2001</span> 21st-century total solar eclipse

A total solar eclipse took place on June 21, 2001, with a magnitude of 1.0495. It was the first solar eclipse of the 21st century. 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. Occurring 2.2 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of May 10, 2013</span> 21st-century annular solar eclipse

An annular solar eclipse took place at the Moon's descending node of the orbit on May 9–10 (UTC), 2013, with a magnitude of 0.9544. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of November 3, 2013</span> 21st-century total solar eclipse

A total solar eclipse occurred at the Moon's ascending node on 3 November 2013. It was a hybrid eclipse of the Sun with a magnitude of 1.0159, with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse, and the rest of the path as a narrow total solar eclipse. 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 hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.

<span class="mw-page-title-main">Solar eclipse of March 20, 2034</span> Future total solar eclipse

A total solar eclipse will occur on Monday, March 20, 2034. 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.

<span class="mw-page-title-main">Solar eclipse of July 22, 1990</span> 20th-century total solar eclipse

A total solar eclipse occurred on July 22, 1990. 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. Totality was visible in southern Finland, the Soviet Union, and eastern Andreanof Islands and Amukta of Alaska.

<span class="mw-page-title-main">Solar eclipse of September 14, 2099</span> Future total solar eclipse

A total solar eclipse will occur on September 14, 2099. 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.

<span class="mw-page-title-main">Solar eclipse of May 11, 2078</span> Future total solar eclipse

A total solar eclipse will occur on Wednesday, May 11, 2078. 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.

<span class="mw-page-title-main">Solar eclipse of March 7, 1970</span> 20th-century total solar eclipse

A total solar eclipse occurred on March 7, 1970, visible across most of North America and Central America.

<span class="mw-page-title-main">Solar eclipse of September 9, 1904</span> 20th-century total solar eclipse

A total solar eclipse occurred on September 9, 1904. 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. Totality was visible from German New Guinea on September 10 and Chile on September 9.

<span class="mw-page-title-main">Solar eclipse of June 30, 1992</span> 20th-century total solar eclipse

A total solar eclipse occurred on June 30, 1992. 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. Totality was visible in southeastern Uruguay and southern tip of Rio Grande do Sul, Brazil.

<span class="mw-page-title-main">Solar eclipse of September 2, 2035</span> Solar eclipse

A total solar eclipse will occur on Sunday, September 2, 2035. 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.

<span class="mw-page-title-main">Solar eclipse of February 5, 2046</span> Future annular solar eclipse

An annular solar eclipse will occur on Monday, February 5, 2046. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of June 8, 1937</span> 20th-century total solar eclipse

A total solar eclipse occurred on June 8, 1937. 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. The path of totality crossed the Pacific Ocean starting in Gilbert and Ellice Islands on June 9, and ending at sunset in Peru on June 8 (Tuesday). At sunrise totality lasted 3 minutes, 6.8 seconds and at sunset totality lasted 3 minutes, 5.1 seconds. American astronomy professor Ethelwynn Rice Beckwith traveled to Peru to see this eclipse, and described the event in detail for the Oberlin Alumnae Magazine in 1937, in an article titled "Three Minutes in Peru."

<span class="mw-page-title-main">Solar eclipse of August 10, 1915</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on August 10, 1915. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from the Pacific Ocean, with the only land being Haha-jima Group in Japan, where the eclipse occurred on August 11 because it is west of International Date Line.

<span class="mw-page-title-main">Solar eclipse of September 4, 2100</span> Future total solar eclipse

A total solar eclipse is forecast to occur on September 4, 2100. It will be the last solar eclipse of the 21st century. 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.

<span class="mw-page-title-main">Solar eclipse of May 1, 2079</span> Future total solar eclipse

A total solar eclipse will occur on Monday, May 1, 2079, with a maximum eclipse at 10:48:25.6 UTC. 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. The eclipse will be visible in Greenland, parts of eastern Canada and parts of the northeastern United States.

<span class="mw-page-title-main">Solar eclipse of September 21, 1903</span> 20th-century total solar eclipse

A total solar eclipse occurred on September 21, 1903. 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.

<span class="mw-page-title-main">Solar eclipse of March 6, 1905</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on March 6, 1905. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from Heard Island and McDonald Islands, Australia, New Caledonia, and New Hebrides.

<span class="mw-page-title-main">Solar eclipse of February 14, 1915</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on February 14, 1915. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from Australia, Papua in Dutch East Indies, German New Guinea, and the South Seas Mandate of Japan.

<span class="mw-page-title-main">Solar eclipse of February 25, 1914</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on February 25, 1914.

References