Lists of solar eclipses |
---|
Solar eclipses in antiquity |
Solar eclipses in the Middle Ages |
Modern history |
The future |
Eclipses seen from |
See also Lists of lunar eclipses |
This is a list of selected solar eclipses from antiquity, in particular those with historical significance. Eclipses on this list were not only recorded, but sometimes would have large effects such as ending a war.
Date of eclipse | Type | Saros | Magnitude | Gamma | Time (UTC) | Central Duration | Eclipse Path | Notes | ||
---|---|---|---|---|---|---|---|---|---|---|
Start | Mid | End | ||||||||
22 Oct 2137 BC | Annular | 9 | 0.9736 | 0.3842 | – | 03:25:29 | 02m52s | It is said that Ho and Hi, the Drunk Astronomers failed to predict this eclipse. (story may be fictitious or misinterpreted) | ||
3 May 1375 BC | Total | 16 | 1.0295 | 0.7755 | – | 04:51:04 | 02m07s | Ugarit eclipse. | ||
June 24, 1312 BC | Total | 35 | – | 10:44 | – | 04m33s | Anatolia | Known as Mursili's eclipse, could provide an absolute chronology of the ancient Near East. [1] [2] [3] | ||
5 June 1302 BC | Total | 26 | 1.0805 | 0.2982 | 02:10:48 | 00:06:25 | Early Chinese eclipse. | |||
16 Apr 1178 BC | Total | 39 | 1.0599 | 0.5187 | 10:00:58 | 00:04:33 | Odyssey Eclipse. | |||
21 Apr 899 BC | Annular | 53 | 0.9591 | 0.8964 | 22:21:56 | 00:03:04 | China's 'Double-Dawn' Eclipse. | |||
June 15, 763 BC | Total | 44 | – | 08:23 | – | 04m59s | Attested in Assyrian sources and providing an absolute chronology of the ancient Near East. [4] | |||
6 Apr 648 BC | Total | 38 | 1.0689 | 0.6898 | 08:31:03 | 00:05:02 | Archilochus' Eclipse. | |||
May 28, 585 BC | Total | 57 | – | 14:28 | – | 06m05s | Allegedly predicted by Thales; occurred during the Battle of the Eclipse. [5] [6] | |||
19 May 557 BC | Total | 48 | 1.0258 | 0.3145 | 12:52:26 | 00:02:22 | The Siege of Larisa, firstly recorded by Xenophon. | |||
February 17, 478 BC or October 2, 480 BC | Annular | 42/65 | – | 9:58:51/11:51:0 | – | 06m00s/07m57s | Greece | Eclipse occurring prior to Xerxes' first march against Greece. The exact dating has been debated, as the writings of Herodotus (who chronicled the eclipse) give a date for which there was no eclipse visible in that area of the world. [7] | ||
August 3, 431 BC | Annular | 48 | – | 14:54:51:8 | – | 01m04.5s | Greece, Mediterranean Sea | Recorded by Thucydides; [8] Pericles shows his Greek Army that the eclipse was not much more than a covering of the sun by something bigger than his cloak. [9] | ||
21 Mar 424 BC | Annular | 42 | 0.9430 | 0.9433 | 07:54:29 | 00:04:39 | 8th year of the Peloponnesian War. | |||
May 6, 319 | Total | 72 | – | 14:24:49 | – | 03m56s | Georgia, Europe, Mexico, United States | Thought by astronomers to be the eclipse preceding the Christianization of Iberia by Mirian III of Iberia. [10] | ||
July 17, 334 | Annular | 80 | 0.9759 | 0.3268 | – | 11:21:41 | – | 02m23s | Rome, Mediterranean Sea | Recorded by Firmicus Maternus in his Mathesos. [11] |
Below is a list of the 10 longest total eclipses between the 30th century BC and the 4th century.
Date of eclipse | Central Duration | Reference |
---|---|---|
30 May 2585 BC | 07m17s | [12] |
10 June 2567 BC | 07m21s | [12] |
6 May 2249 BC | 07m20s | [12] |
17 May 2231 BC | 07m21s | [12] |
5 June 762 BC | 07m25s | [13] |
15 June 744 BC | 07m28s | [13] |
26 June 726 BC | 07m18s | [13] |
16 June 345 | 07m17s | [14] |
27 June 363 | 07m24s | [14] |
8 July 381 | 07m22s | [14] |
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 | ||||
20th BC | 239 | 84 | 71 | 62 | 22 | 11m38s | 28 December 1983 BC | March 1958 BC | [15] |
19th BC | 253 | 93 | 80 | 63 | 17 | 08m57s | 28 October 1896 BC | January 1806 BC | [16] |
18th BC | 254 | 95 | 74 | 64 | 21 | 11m10s | 10 November 1710 BC | [17] | |
17th BC | 230 | 75 | 71 | 60 | 24 | 12m07s | 12 December 1656 BC | July 1611 BC | [18] |
16th BC | 225 | 78 | 67 | 59 | 21 | 10m07s | 25 January 1583 BC | June 1535 BC, May 1524 BC | [19] |
15th BC | 226 | 77 | 69 | 62 | 18 | 10m00s | 25 September 1410 BC | April 1448 BC | [20] |
14th BC | 234 | 76 | 84 | 68 | 6 | 11m29s | 18 November 1320 BC | [21] | |
13th BC | 250 | 93 | 86 | 64 | 7 | 11m11s | 9 December 1284 BC | December 1210 BC | [22] |
12th BC | 252 | 93 | 89 | 63 | 7 | 10m27s | 14 December 1108 BC | October 1123 BC, September 1112 BC | [23] |
11th BC | 238 | 79 | 91 | 68 | 0 | 10m34s | 25 December 1090 BC | August 1036 BC, July 1025 BC, June 1014 BC | [24] |
10th BC | 226 | 84 | 75 | 61 | 6 | 09m01s | 24 October 984 BC | [25] | |
9th BC | 225 | 80 | 75 | 66 | 4 | 10m21s | 7 November 817 BC | [26] | |
8th BC | 234 | 79 | 88 | 64 | 3 | 11m29s | 10 December 763 BC | [13] | |
7th BC | 253 | 96 | 87 | 63 | 7 | 10m06s | 22 November 604 BC | December 689 BC, November 678 BC, October 602 BC | [27] |
6th BC | 255 | 96 | 86 | 65 | 8 | 10m50s | 4 January 531 BC | September 591 BC, August 515 BC, July 504 BC | [28] |
5th BC | 241 | 84 | 78 | 62 | 17 | 10m24s | 26 January 495 BC | May 417 BC | [29] |
4th BC | 225 | 83 | 63 | 56 | 23 | 10m16s | 7 December 391 BC | [30] | |
3rd BC | 226 | 83 | 62 | 57 | 24 | 11m47s | 30 November 214 BC | [31] | |
2nd BC | 237 | 80 | 73 | 63 | 21 | 12m08s | 22 December 178 BC | [32] | |
1st BC | 251 | 92 | 77 | 65 | 17 | 08m51s | 14 February 87 BC | [33] | |
1st AD | 248 | 90 | 75 | 58 | 25 | 11m18s | 4 November 96 | August 7, July 18, April 97 | [34] |
2nd AD | 237 | 80 | 77 | 64 | 16 | 12m23s [lower-alpha 3] | 7 December 150 | [36] | |
3rd AD | 227 | 79 | 74 | 69 | 5 | 11m09s | 8 January 205 | [37] | |
4th AD | 222 | 73 | 76 | 66 | 7 | 10m44s | 2 January 363 | [14] |
A total solar eclipse took place on Sunday, November 23, 2003, with a magnitude of 1.0379. 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 corridor in the Antarctic region. A partial eclipse was seen from the much broader path of the Moon's penumbra, including the southern tip of South America and most of Australia.
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season in its new moon phase, when the Moon's orbital plane is closest to the plane of Earth's orbit. In a total eclipse, the disk of the Sun is fully obscured by the Moon. In partial and annular eclipses, only part of the Sun is obscured. Unlike a lunar eclipse, which may be viewed from anywhere on the night side of Earth, a solar eclipse can only be viewed from a relatively small area of the world. As such, although total solar eclipses occur somewhere on Earth every 18 months on average, they recur at any given place only once every 360 to 410 years.
The total solar eclipse of July 11, 2010 occurred over the southern Pacific Ocean. 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 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.
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 Wednesday, January 26, 2028. 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 December 24, 1973. 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 southern Mexico, southwestern Nicaragua, Costa Rica including the capital city San José, Panama, Colombia including the capital city Bogotá, southern Venezuela, Brazil, southern Guyana, southern Dutch Guiana, southern French Guiana, Portuguese Cape Verde including the capital city Praia, Mauritania including the capital city Nouakchott, Spanish Sahara, Mali, and Algeria.
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 23, 1987. 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 in the Soviet Union, China, southwestern Mongolia, Okinawa Islands of Japan except Kume Island and the southwestern tip of Kerama Islands, the Federal States of Micronesia, Papua New Guinea, Solomon Islands, Rotuma Islands of Fiji, Wallis Islands and West Samoa. Occurring only 5 days after apogee, the Moon's apparent diameter was relatively small.
An annular solar eclipse occurred at the Moon's ascending node of the orbit on Wednesday, August 22, 1979. 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 93% of the Sun in a very broad path, 953 km wide at maximum, and lasted 6 minutes and 3 seconds. This was the second solar eclipse in 1979, the first one a total solar eclipse on February 26.
An annular solar eclipse occurred on September 11, 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.
An annular solar eclipse will occur on Monday, November 15, 2077, with a magnitude of 0.9371. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially 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. The path of annularity will cross North America and South America. This will be the 47th solar eclipse of Saros cycle 134. A small annular eclipse will cover only 93.71% of the Sun in a very broad path, 262 km wide at maximum, and will last 7 minutes and 54 seconds. Occurring only 4 days after apogee, the Moon's apparent diameter is smaller.
Saros cycle series 136 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's descending node.
This article contains information and statistics about solar eclipses occurring after the modern era, from the 22nd century to the 30th century.
This article gives statistics for lunar eclipses grouped by century. Detailed information about tetrads, timing, and other facts can be found at the linked references.
{{cite web}}
: CS1 maint: archived copy as title (link){{cite web}}
: CS1 maint: archived copy as title (link)