List of solar eclipses visible from Turkey

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This list of solar eclipses visible from Turkey enumerates the solar eclipses that have been and will be seen over Turkey. [1]

Contents

Eighteenth century and earlier

Total solar eclipses

January 8, 1339 BC June 24, 1311 BC June 15, 762 BC May 28, 584 BC
SolarEclipse BC 1340-01-08.gif SolarEclipse BC 1312-06-24.gif BurSagaleBC762-06-15.gif SoFi-584-05-28.gif
August 2, 1133 August 12, 1654 June 13, 1760
SolarEclipse 1133-08-02.gif Solar eclipse from 1654-08-12.gif SE1760Jun13T.png

Annular solar eclipses

March 13, 1334 BC
SolarEclipse BC 1335-03-13.gif

Partial solar eclipses

January 4, 1639
SE1639Jan04P.png

Nineteenth century

Total solar eclipses

November 19, 1816 July 28, 1851 December 22, 1870
SE1816Nov19T.png SE1851Jul28T.png SE1870Dec22T.png

Annular solar eclipses

September 7, 1820
SE1820Sep07A.png

Twentieth century

Total solar eclipses

August 21, 1914 June 19, 1936 August 11, 1999
SE1914Aug21T.png SE1936Jun19T.png SE1999Aug11T.png

Annular solar eclipses

May 20, 1966 April 29, 1976
SE1966May20A.png SE1976Apr29A.png

Partial solar eclipses

October 31, 1902 January 23, 1917 November 12, 1928 September 10, 1942
SE1902Oct31P.png SE1917Jan23P.png SE1928Nov12P.png SE1942Sep10P.png
April 28, 1949 December 2, 1956 February 25, 1971 May 11, 1975
SE1949Apr28P.png SE1956Dec02P.png SE1971Feb25P.png SE1975May11P.png
December 15, 1982 May 21, 1993 October 12, 1996
SE1982Dec15P.png SE1993May21P.png SE1996Oct12P.png

Twenty-first century

Total solar eclipses

March 29, 2006 April 30, 2060 September 3, 2081 April 21, 2088
SE2006Mar29T.png SE2060Apr30T.png SE2081Sep03T.png SE2088Apr21T.png

Annular solar eclipses

June 1, 2030 July 23, 2093
SE2030Jun01A.png SE2093Jul23A.png

Partial solar eclipses

January 4, 2011 October 25, 2022 November 3, 2032 January 16, 2037
SE2011Jan04P.png SE2022Oct25P.png SE2032Nov03P.png SE2037Jan16P.png
November 14, 2050 February 5, 2065 November 26, 2076 December 6, 2086
SE2050Nov14P.png SE2065Feb05P.png SE2076Nov26P.png SE2086Dec06P.png
February 18, 2091
SE2091Feb18P.png

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of March 29, 2006</span> 21st-century total solar eclipse

A total solar eclipse occurred on March 29, 2006. 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. It was visible from a narrow corridor which traversed half the Earth. The magnitude, that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.

<span class="mw-page-title-main">Solar eclipse of July 22, 2009</span> 21st-century total solar eclipse

A total solar eclipse occurred at the Moon's descending node of the orbit on July 22, 2009, with a magnitude of 1.07991. It was the longest total solar eclipse during the 21st century; the longest total solar eclipse during the 3rd millennium will be on 16 July 2186. It lasted a maximum of 6 minutes and 38.86 seconds off the coast of Southeast Asia, causing tourist interest in eastern China, Pakistan, Japan, India, Nepal and Bangladesh. Its greatest magnitude was 1.07991, occurring only 6 hours, 18 minutes after perigee, with greatest eclipse totality lasting 6 minutes, 38.86 seconds during the Total Solar Eclipse of July 22, 2009.

<span class="mw-page-title-main">Solar eclipse of August 11, 1999</span> 20th-century total solar eclipse

A total solar eclipse occurred on 11 August 1999 with an eclipse magnitude of 1.0286. 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 the moon's shadow began in the Atlantic Ocean and, before noon, was traversing the southern United Kingdom, northern France, Belgium, Luxembourg, southern Germany, Austria, Slovenia, Croatia, Hungary, and northern FR Yugoslavia (Vojvodina). The eclipse's maximum was at 11:03 UTC at 45.1°N 24.3°E in Romania ; and it continued across Bulgaria, the Black Sea, Turkey, northeastern tip of Syria, northern Iraq, Iran, southern Pakistan and Srikakulam in India and ended in the Bay of Bengal.

<span class="mw-page-title-main">June 2011 lunar eclipse</span> Central lunar eclipse

A total lunar eclipse took place on 15 June 2011. It was the first of two such eclipses in 2011. The second occurred on 10 December 2011. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse.

<span class="mw-page-title-main">March 2024 lunar eclipse</span> Penumbral lunar eclipse of 25 March 2024

A penumbral lunar eclipse took place on Monday, March 25, 2024. It was visible to the naked eye as 95.57% of the Moon was immersed in Earth's penumbral shadow, making it the deepest penumbral eclipse overall since May 5, 2023, and the deepest for North and South America since February 11, 2017.

A penumbral lunar eclipse took place on Tuesday, September 27, 1977, the second of two lunar eclipses in 1977. At maximum eclipse, 90.076% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours, 17 minutes and 35.5 seconds overall. Occurring 6.2 days before apogee, the Moon's apparent diameter was 2.2% smaller than average.

A partial lunar eclipse took place on Tuesday, March 13, 1979, the first of two lunar eclipses in 1979. The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours, 17 minutes and 40.6 seconds, with 85.377% of the Moon in darkness at maximum.

<span class="mw-page-title-main">Solar eclipse of March 9, 2016</span> 21st-century total solar eclipse

A total solar eclipse took place at the Moon's descending node of the orbit on March 8–9, 2016. If viewed from east of the International Date Line, the eclipse took place on March 8 (Tuesday) and elsewhere on March 9 (Wednesday). A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. 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 of March 8–9, 2016 had a magnitude of 1.0450 visible across an area of Pacific Ocean, which started in the Indian Ocean, and ended in the northern Pacific Ocean.

<span class="mw-page-title-main">Solar eclipse of January 15, 2010</span> 21st-century annular solar eclipse

An annular solar eclipse occurred at the Moon's ascending node of the orbit on January 15, 2010, with a magnitude of 0.91903. 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. It was the longest annular solar eclipse of the millennium, and the longest until December 23, 3043, with the length of maximum eclipse of 11 minutes, 7.8 seconds, and the longest duration of 11 minutes, 10.7 seconds. This is about 4 minutes longer than total solar eclipses could ever get.

<span class="mw-page-title-main">Solar eclipse of January 4, 2011</span> 21st-century partial solar eclipse

The solar eclipse of January 4, 2011 was a partial eclipse of the Sun that was visible after sunrise over most of Europe, northwestern and South Asia. It ended at sunset over eastern Asia. It was visible as a minor partial eclipse over northern Africa and the Arabian peninsula. The eclipse belonged to Saros 151 and was number 14 of 72 eclipses in the series.

<span class="mw-page-title-main">Solar eclipse of May 20, 2012</span> 21st-century annular solar eclipse

The solar eclipse of May 20, 2012 was an annular solar eclipse that was visible in a band spanning through Eastern Asia, the Pacific Ocean, and North America. As a partial solar eclipse, it was visible from northern Greenland to Hawaii, and from eastern Indonesia at sunrise to northwestern Mexico at sunset. The moon's apparent diameter was smaller because the eclipse was occurring only 32 1/2 hours after apogee.

<span class="mw-page-title-main">Solar eclipse of December 26, 2019</span> 21st-century annular solar eclipse

An annular solar eclipse occurred at the Moon’s descending node of the orbit on Thursday, December 26, 2019. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring 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 August 2, 2027</span> Future total solar eclipse

A total solar eclipse will occur over much of the central Eastern Hemisphere on Monday, August 2, 2027. 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 September 3, 2081</span> Solar eclipse

A total solar eclipse will occur on Wednesday, September 3, 2081. 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 will begin at the Atlantic Ocean, off European mainland at 07:26:49 UTC and will end at Indonesian island of Java at 10:43:03 UTC.

<span class="mw-page-title-main">Solar eclipse of April 29, 1976</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of the orbit on Thursday, April 29, 1976. 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 North Africa, Greece, Turkey, Middle East, central Asia, India, China. 5 of the 14 eight-thousanders in Pakistan and China—Nanga Parbat, K2, Broad Peak, Gasherbrum II and Gasherbrum I, lie in the path of annularity.

<span class="mw-page-title-main">Solar eclipse of June 1, 2030</span> Future annular solar eclipse

An annular solar eclipse will occur on Saturday, June 1, 2030. 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 21, 2020</span> 21st-century annular solar eclipse

An annular solar eclipse occurred on Sunday, June 21, 2020. An annular solar eclipse is a solar eclipse whose presentation looks like a ring, or annulus; it occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most, but not all, of the Sun's light. In this instance, the Moon's apparent diameter was 0.6% smaller than the Sun's.

<span class="mw-page-title-main">Solar eclipse of October 25, 2022</span> Partial solar eclipse

The solar eclipse of October 25, 2022 was a partial solar eclipse visible from Europe, the Urals and Western Siberia, Central Asia, Western Asia, South Asia and from the north-east of Africa. The maximal phase of the partial eclipse occurred on the West Siberian Plain in Russia near Nizhnevartovsk, where more than 82% of the Sun was eclipsed by the Moon. In India, the Sun was eclipsed during sunset ranging from 58% in the north and around 2% in the south. From Western Europe it appeared to be around 15-30% eclipsed. It was visible between 08:58 UTC, the greatest point of eclipse occurred at 11:00 UTC and it ended at 13:02 UTC.

<span class="mw-page-title-main">Solar eclipse of October 2, 1978</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of the orbit on Monday, October 2, 1978. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. The eclipse is a part of the 153 saros cycle. Its the 7th eclipse of the saros cycle. The solar eclipse was visible in most of Asia Except northern Asia, Northeastern Europe, tiny northern part of Oceania, and tiny parts of Guam and other American islands

References

  1. "JavaScript Solar Eclipse Explorer (Asia & Asia Minor)". eclipse.gsfc.nasa.gov. Retrieved April 9, 2024.