List of solar eclipses visible from the British Isles

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A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially obscuring Earth's view of the Sun. Below is a complete list of total and annular eclipses visible anywhere within the modern extent of the United Kingdom between AD 1 and AD 2090 [1] and a description of forthcoming partial solar eclipses visible in Britain in the next fifteen years or so. [2] For a complete list of solar eclipses visible from the United Kingdom between AD 1501 and AD 2500, see the Journal of the British Astronomical Association, February 2001. [3]

Contents

1st-4th century (1-400)

5th century (401-500)

EclipseOf458-05-28.gif

6th century (AD 501-600)

7th century (601-700)

8th-11th centuries (701-1100)


12th century (AD 1101 – 1200)

13th to 14th centuries (AD 1201 - 1400)

15th to 16th centuries (AD 1401 – 1600)

17th to 19th centuries (AD 1601–1900)

Solar eclipse 1715May03-Cambridge England.png Solar eclipse 1715May03 Halley map.png
3 May 1715 Cambridge, England

20th century (AD 1901 – 2000)

Partial solar eclipses also occurred on 20 May 1966, 22 September 1968, 25 February 1971, 10 July 1972, 30 June 1973, 11 May 1975, 29 April 1976, 20 July 1982, 15 December 1982, 4 December 1984, 21 May 1993 and 10 May 1994. (Source: HMNAO Eclipses On-line Portal.)

21st century (AD 2001 – 2100)

22nd century (AD 2101 – 2200)

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<span class="mw-page-title-main">Solar eclipse of July 22, 2009</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, July 22, 2009, with a magnitude of 1.07991. 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 about 5.5 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 11, 1999</span> Total eclipse

A total solar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, August 11, 1999, with a magnitude of 1.0286. A solar eclipse occurs when the Moon passes between the Earth and the Sun, thereby totally or partly obscuring the light 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 night. 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 about 3.5 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 1, 2008</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Friday, August 1, 2008, with a magnitude of 1.0394. 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 about 2.4 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of November 13, 2012</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, November 13 and Wednesday, November 14, 2012, with a magnitude of 1.05. 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 about 12 hours before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of November 3, 2013</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Sunday, November 3, 2013, with a magnitude of 1.0159. It was a hybrid event, a narrow total eclipse, and beginning as an annular eclipse and concluding as a total eclipse, in this particular case. 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 about 2.9 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 30, 1954</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, June 30, 1954, with a magnitude of 1.0357. 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 about 3.1 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 12, 2026</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, August 12, 2026, with a magnitude of 1.0386. 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 about 2.2 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of August 23, 2044</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit between Monday, August 22 and Tuesday, August 23, 2044, with a magnitude of 1.0364. 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 about 2.1 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of August 2, 2027</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Monday, August 2, 2027, with a magnitude of 1.079. 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 about 2.5 hours before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of August 12, 2045</span> Total eclipse over North America

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, August 12, 2045, with a magnitude of 1.0774. 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 about 7 minutes after perigee, the Moon's apparent diameter will be near its maximum.

<span class="mw-page-title-main">Solar eclipse of June 30, 1973</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Saturday, June 30, 1973, with a magnitude of 1.0792. 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 about 11 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 30, 1992</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Tuesday, June 30, 1992, with a magnitude of 1.0592. 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 about 1.5 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of July 22, 2028</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Saturday, 22 July 2028, with a magnitude of 1.056. 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 about 1.8 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of June 29, 1927</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, June 28 and Wednesday, June 29, 1927, with a magnitude of 1.0128. 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 about 20 hours after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 8, 1918</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit between Saturday, June 8 and Sunday, June 9, 1918, with a magnitude of 1.0292. 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 3.7 days after perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of December 14, 1955</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, December 14, 1955, with a magnitude of 0.9176. 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. Occurring about 1 day before apogee, the Moon's apparent diameter was smaller.

<span class="mw-page-title-main">Solar eclipse of April 30, 1957</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 30, 1997, with a magnitude of 9.9799. 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. Occurring about 6.1 days after apogee, the Moon's apparent diameter was smaller.

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

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, May 1, 2079, with a magnitude of 1.0512. 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 about 1.2 days before perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of April 17, 1912</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, April 17, 1912, with a magnitude of 1.0003. It was a hybrid event, starting and ending as an annular eclipse, with only a small portion of totality. 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 7.4 days after apogee and 5.5 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of June 24, 1778</span> Total eclipse

A total solar eclipse occurred on June 24, 1778. 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.

References

  1. UK Solar Eclipses from Year 1 by Sheridan Williams, Clock Tower Press, ISBN   1-85142-093-2, Published 1996
  2. Fifty Year Canon of Solar Eclipses 1986 – 2035 by Fred Espenak, NASA ISBN   0-933346-45-X, Published 1987
  3. A Millennium of British solar eclipses (1501–2500) AD, Journal of the British Astronomical Association, Vol 111, pp 88–98
  4. Solar eclipse of 2 August 1133
  5. "Chronology and dating". Medievalgenealogy.org.uk. 2009-07-19. Retrieved 2013-10-01.
  6. Archived July 25, 2012, at the Wayback Machine
  7. NASA Technical Publication TP-2006-214141 – http://eclipse.gsfc.nasa.gov/5MCSE/5MCSE-Maps-08.pdf
  8. Solar eclipse of June 24, 1424
  9. Solar eclipse of June 17, 1433
  10. Solar eclipse of March 16, 1485