Lists of solar eclipses |
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Solar eclipses in antiquity |
Solar eclipses in the Middle Ages |
Modern history |
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See also Lists of lunar eclipses |
This article contains information and statistics about solar eclipses occurring after the modern era, from the 22nd century to the 30th century.
Century | No. | Eclipse type | Longest eclipse [lower-alpha 1] | Two-eclipse months [lower-alpha 2] | Ref. | ||||
---|---|---|---|---|---|---|---|---|---|
Partial (P) | Annular (A) | Total (T) | Hybrid (H) | Length | Date | ||||
22nd | 235 | 79 | 87 | 65 | 4 | 10m55s | 10 January 2168 | [1] | |
23rd | 248 | 92 | 86 | 67 | 3 | 10m38s | 2 February 2204 | December 2206, January 2261, November 2282 | [2] |
24th | 248 | 88 | 86 | 66 | 8 | 09m40s | 3 December 2309 | September 2304, August 2380 | [3] |
25th | 237 | 81 | 89 | 66 | 1 | 10m22s | 28 December 2494 | [4] | |
26th | 225 | 83 | 72 | 64 | 6 | 10m25s | 8 January 2513 | [5] | |
27th | 227 | 77 | 81 | 64 | 5 | 09m17s | 2 January 2690 | [6] | |
28th | 242 | 84 | 92 | 63 | 3 | 10m04s | 16 February 2762 | May 2785 | [7] |
29th | 254 | 95 | 87 | 63 | 9 | 10m20s | 7 January 2885 | [8] | |
30th | 248 | 91 | 82 | 64 | 11 | 10m12s | 19 January 2903 | [9] |
Below is a list of all total eclipses at least 7 minutes long that will occur between the 22nd and 30th centuries. Of the listed eclipses, the first five are in Solar Saros 139, the next three are in Solar Saros 145, and the final four are in Solar Saros 170.
Date of eclipse | Central Duration | Reference | Saros |
---|---|---|---|
25 June 2150 | 07m14s | [1] | 139 |
5 July 2168 | 07m26s | [1] | 139 |
16 July 2186 | 07m29s [lower-alpha 3] | [1] | 139 |
27 July 2204 | 07m22s | [2] | 139 |
8 August 2222 | 07m06s | [2] | 139 |
14 June 2504 | 07m10s | [5] | 145 |
25 June 2522 | 07m12s | [5] | 145 |
5 July 2540 | 07m04s | [5] | 145 |
12 June 2849 | 07m00s | [8] | 170 |
23 June 2867 | 07m10s | [8] | 170 |
3 July 2885 | 07m11s | [8] | 170 |
16 July 2903 | 07m04s | [9] | 170 |
A total solar eclipse will take place at the Moon's ascending node on Monday, April 8, 2024, visible across North America and dubbed the Great North American Eclipse by some of the media. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby 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 only in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
A total lunar eclipse took place on Sunday 16 July 2000, the second of two total lunar eclipses in 2000.
A total lunar eclipse took place on Tuesday, July 6, 1982, the second of three total lunar eclipses in 1982, and the only one that was in the descending node. A dramatic total eclipse lasting 1 hour and 46 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. 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. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 56 minutes in total.
A total lunar eclipse took place on Sunday, July 26, 1953.
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.
A total solar eclipse will occur on Tuesday, May 22, 2096. 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. This will be the first eclipse of saros series 139 to exceed series 136 in length of totality. The length of totality for saros 139 is increasing, while that of Saros 136 is decreasing.
A total solar eclipse occurred on March 18, 1988. 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 Indonesia and southern Philippines.
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.
An annular solar eclipse occurred on September 11, 1969. 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, Peru, Bolivia and the southwestern tip of Brazilian state Mato Grosso. Places west of the International Date Line witnessed the eclipse on Friday, September 12, 1969.
An annular solar eclipse occurred on August 11, 1961. 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. A small annular eclipse covered only 94% of the Sun in a very broad path, 499 km wide at maximum, and lasted 6 minutes and 35 seconds.
A total solar eclipse will occur on May 20, 2050. 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. This eclipse is a hybrid eclipse, starting and ending as an annular solar eclipse.
A total solar eclipse will occur on Saturday, May 22, 2077. 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.
A total solar eclipse occurred on April 16, 1893. 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.
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.
A total solar eclipse occurred on August 31, 1932. 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 Northwest Territories and Quebec in Canada, and northeastern Vermont, New Hampshire, southwestern Maine, northeastern tip of Massachusetts and northeastern Cape Cod in the United States.
A total lunar eclipse will occur on Wednesday, June 9, 2123, with maximum eclipse at 05:06 UTC. A dramatic total eclipse lasting 106 minutes and 6 seconds will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 56 minutes in total. The penumbral eclipse lasts for 6 hours and 14 minutes. Maximum eclipse is at 05:06:28 UT. This will be the longest Total Lunar Eclipse since 16 July 2000, and the longest one until 12 May 2264 and 27 July 3107, though the eclipse on June 19, 2141 will be nearly identical in all aspects. This will also be the longest of the 22nd century and the second longest of the 3rd millennium. The eclipse on June 19, 2141 will be the second longest of the 22nd century and the third longest of the third millennium.