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 |
During the 22nd century, there will be 235 solar eclipses of which 79 will be partial, 87 will be annular, 65 will be total and 4 will be hybrids between total and annular eclipses. Of these, five annular eclipses will be non-central, [1] in the sense that the very center (axis) of the Moon's shadow will miss the Earth (for more information see gamma). [2] In the 22nd century, the greatest number of eclipses in one year is four, in 11 different years: 2112, 2134, 2141, 2152, 2159, 2170, 2177, 2181, 2188, 2195, and 2199. The predictions given here are by Fred Espenak of NASA's Goddard Space Flight Center. [1]
The longest measured duration in which the Moon completely covered the Sun, known as totality, will be during the solar eclipse of July 16, 2186. This total solar eclipse will have a maximum duration of 7 minutes and 29.22 seconds. This will be the longest total solar eclipse between 4000 BCE and at least CE 6000 (10,000 years). The longest possible duration of a total solar eclipse is 7 minutes and 32 seconds. The longest annular solar eclipse of the 22nd century will take place on January 10, 2168, with a duration of 10 minutes and 55 seconds. The maximum possible duration is 12 minutes and 29 seconds. [a]
The table contains the date and time of the greatest eclipse (in dynamical time), which in this case is the time when the axis of the Moon's shadow cone passes closest to the centre of Earth; this is in (Ephemeris Time). The number of the saros series that the eclipse belongs to is given, followed by the type of the eclipse (either total, annular, partial or hybrid), the gamma of the eclipse (how centrally the shadow of the Moon strikes the Earth), and the magnitude of the eclipse (the fraction of the Sun's diameter obscured by the Moon). For total and annular eclipses, the duration of the eclipse is given, as well as the location of the greatest eclipse (the point of maximum eclipse) and the path width of the total or annular eclipse. The geographical areas from which the eclipse can be seen are listed along with a chart illustrating each eclipse's respective path. [3]
Extrema Type | Date | Duration | Magnitude |
---|---|---|---|
Longest Annular Solar Eclipse | 2168 January 10 | 10m 55s | 0.923 |
Shortest Annular Solar Eclipse | 2191 April 23 | 00m 02.87s | 0.9993 |
Longest Total Solar Eclipse | 2186 July 16 | 07m 29s | - |
Shortest Total Solar Eclipse | 2200 April 14 | 01m 23s | - |
Longest Hybrid Solar Eclipse | 2172 October 17 | 01m 34s | - |
Shortest Hybrid Solar Eclipse | 2164 March 23 | 00m 29s | - |
Largest Partial Solar Eclipse | 2109 August 26 | - | 0.96698 |
Smallest Partial Solar Eclipse | 2112 June 24 | - | 0.02818 |
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.
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.
An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 29, 2014, with a magnitude of 0.9868. 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. The Moon's apparent diameter was near the average diameter because it occurred 6.2 days after perigee and 7.2 days before apogee.
An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, January 15, 2010, with a magnitude of 0.919. 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 1.75 days before apogee, the Moon's apparent diameter was smaller.
A partial solar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, January 4, 2011, with a magnitude of 0.8576. 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.
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.
A total solar eclipse will occur at the Moon's ascending node of orbit on Sunday, July 16, 2186, with a magnitude of 1.0805. 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 only about 3 minutes before perigee, the Moon's apparent diameter will be larger.
A partial solar eclipse occurred at the Moon's ascending node of orbit between Wednesday, December 23 and Thursday, December 24, 1992, with a magnitude of 0.8422. 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.
A partial solar eclipse will occur at the Moon's ascending node of orbit on Sunday, January 14, 2029, with a magnitude of 0.8714. 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.
A partial solar eclipse occurred at the Moon's ascending node of orbit on Friday, December 13, 1974, with a magnitude of 0.8266. 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.
A partial solar eclipse occurred at the Moon's ascending node of orbit on Sunday, December 2, 1956, with a magnitude of 0.8047. 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.
A partial solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, February 16, 2083, with a magnitude of 0.9433. 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.
An annular solar eclipse will occur at the Moon's descending node of orbit between Sunday, November 3 and Monday, November 4, 2097, with a magnitude of 0.9494. 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 5.4 days before apogee, the Moon's apparent diameter will be smaller.
An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, February 7, 2092, with a magnitude of 0.984. 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 6.25 days before perigee, the Moon's apparent diameter will be larger.
A partial solar eclipse occurred at the Moon's ascending node of orbit on Friday, October 31, 1902, with a magnitude of 0.696. 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.
A partial solar eclipse occurred at the Moon's ascending node of orbit between Monday, November 21 and Tuesday, November 22, 1938, with a magnitude of 0.7781. 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.
A partial solar eclipse occurred at the Moon's ascending node of orbit on Wednesday, November 10, 1920, with a magnitude of 0.742. 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 passes above or below the Earth.