An eclipse season is a period, roughly every six months, when eclipses occur. Eclipse seasons are the result of the axial parallelism of the Moon's orbital plane (tilted five degrees to the Earth's orbital plane), just as Earth's weather seasons are the result of the axial parallelism of Earth's tilted axis as it orbits around the Sun. During the season, the "lunar nodes" – the line where the Moon's orbital plane intersects with the Earth's orbital plane – align with the Sun and Earth, such that a solar eclipse is formed during the new moon phase and a lunar eclipse is formed during the full moon phase.
Only two (or occasionally three) eclipse seasons occur during each year, and each season lasts about 35 days and repeats just short of six months (173 days) later, thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. During the eclipse season, the Moon is at a low ecliptic latitude (less than around 1.5° north or south), hence the Sun, Moon, and Earth become aligned straightly enough (in syzygy) for an eclipse to occur. Eclipse seasons should occur 38 times within a saros period (6,585.3 days).
The type of each solar eclipse (whether total or annular, as seen from the sublunar point) depends on the apparent sizes of the Sun and Moon, which are functions of the distances of Earth from the Sun and of the Moon from Earth, respectively, as seen from Earth's surface. These distances vary because both the Earth and the Moon have elliptic orbits.
If both orbits were coplanar (i.e. on the same plane) with each other, then two eclipses would happen every lunar month (29.53 days), assuming the Earth had a perfectly circular orbit centered around the Sun, and the Moon's orbit was also perfectly circular and centered around the Earth. A lunar eclipse would occur at every full moon, a solar eclipse every new moon, and all solar eclipses would be the same type.
An eclipse season is the only time when the Sun (from the perspective of the Earth) is close enough to one of the Moon's nodes to allow an eclipse to occur. During the season, whenever there is a full moon a lunar eclipse may occur and whenever there is a new moon a solar eclipse may occur. If the Sun is close enough to a node, then a "full" eclipse [total or annular solar, or total lunar] will occur. Each season lasts from 31 to 37 days, and seasons recur about every 6 months (173 days). At least two (one solar and one lunar, in any order), and at most three eclipses (solar, lunar, then solar again, or vice versa), will occur during every eclipse season. This is because it is about 15 days (a fortnight) between a full moon and a new moon and vice versa. If there is an eclipse at the very beginning of the season, then there is enough time (30 days) for two more eclipses.
In other words, because the eclipse season (34 days long on average) is longer than the synodic month (one lunation, or the time for the Moon to return to a particular phase and about 29.5 days), the Moon will be new or full at least two, and up to three, times during the season. Eclipse seasons occur slightly shy of six months apart (successively occurring every 173.31 days - half of an eclipse year), the time it takes the Sun to travel from one node to the next along the ecliptic. If the last eclipse of an eclipse season occurs at the very beginning of a calendar year, a total of seven eclipses to occur since there is still time before the end of the calendar year for two full eclipse seasons, each having up to three eclipses. [1] [2] [3]
In each sequence below, each eclipse is separated by a fortnight. The first and last eclipse in each sequence is separated by one synodic month. See also Eclipse cycles .
June 5 Descending node (full moon) | June 21 Ascending node (new moon) | July 5 Descending node (full moon) |
---|---|---|
Penumbral lunar eclipse Lunar saros 111 | Annular solar eclipse Solar saros 137 | Penumbral lunar eclipse Lunar saros 149 |
June 12 Descending node (new moon) | June 26 Ascending node (full moon) | July 11 Descending node (new moon) |
---|---|---|
Partial solar eclipse Solar saros 118 | Total lunar eclipse Lunar saros 130 | Partial solar eclipse Solar saros 156 |
(The two eclipse seasons above share similarities (lunar or solar centrality and gamma of each eclipse in the same column) because they are a half saros apart.) [4]
Date | Type (phase) | Time of season | Saros series | next eclipse will occur... |
---|---|---|---|---|
January 31, 1999 | lunar (full) | beginning | Lunar saros 114 (58 of 71) | next new moon |
February 16, 1999 | solar (new) | end | Solar saros 140 (28 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
July 28, 1999 | lunar (full) | beginning | Lunar saros 119 (60 of 82) | next new moon |
August 11, 1999 | solar (new) | end | Solar saros 145 (21 of 77) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
January 21, 2000 | lunar (full) | beginning | Lunar saros 124 (48 of 73) | next new moon |
February 5, 2000 | solar (new) | end | Solar saros 150 (16 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
July 1, 2000 | solar (new) | beginning | Solar saros 117 (68 of 71) | next full moon |
July 16, 2000 | lunar (full) | middle | Lunar saros 129 (37 of 71) | next new moon |
July 31, 2000 | solar (new) | end | Solar saros 155 (5 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
December 25, 2000 | solar (new) | beginning | Solar saros 122 (57 of 70) | next full moon |
January 9, 2001 | lunar (full) | end | Lunar saros 134 (26 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
June 21, 2001 | solar (new) | beginning | Solar saros 127 (57 of 82) | next full moon |
July 5, 2001 | lunar (full) | end | Lunar saros 139 (20 of 79) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
December 14, 2001 | solar (new) | beginning | Solar saros 132 (45 of 71) | next full moon |
December 30, 2001 | lunar (full) | end | Lunar saros 144 (15 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
May 26, 2002 | lunar (full) | beginning | Lunar saros 111 (66 of 71) | next new moon |
June 10, 2002 | solar (new) | middle | Solar saros 137 (35 of 70) | next full moon |
June 24, 2002 | lunar (full) | end | Lunar saros 149 (2 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
November 20, 2002 | lunar (full) | beginning | Lunar saros 116 (57 of 73) | next new moon |
December 4, 2002 | solar (new) | end | Solar saros 142 (22 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
May 16, 2003 | lunar (full) | beginning | Lunar saros 121 (54 of 82) | next new moon |
May 31, 2003 | solar (new) | end | Solar saros 147 (22 of 80) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
November 9, 2003 | lunar (full) | beginning | Lunar saros 126 (44 of 70) | next new moon |
November 23, 2003 | solar (new) | end | Solar saros 152 (12 of 70) | next eclipse season |
... no eclipses for about 5 months... | ||||
April 19, 2004 | solar (new) | beginning | Solar saros 119 (65 of 71) | next full moon |
May 4, 2004 | lunar (full) | end | Lunar saros 131 (33 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
October 14, 2004 | solar (new) | beginning | Solar saros 124 (54 of 73) | next full moon |
October 28, 2004 | lunar (full) | end | Lunar saros 136 (19 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
April 8, 2005 | solar (new) | beginning | Solar saros 129 (51 of 80) | next full moon |
April 24, 2005 | lunar (full) | end | Lunar saros 141 (23 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
October 3, 2005 | solar (new) | beginning | Solar saros 134 (43 of 71) | next full moon |
October 17, 2005 | lunar (full) | end | Lunar saros 146 (10 of 72) | next eclipse season |
... no eclipses for about 5 months... | ||||
March 14, 2006 | lunar (full) | beginning | Lunar saros 113 (63 of 71) | next new moon |
March 29, 2006 | solar (new) | end | Solar saros 139 (29 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
September 7, 2006 | lunar (full) | beginning | Lunar saros 118 (51 of 73) | next new moon |
September 22, 2006 | solar (new) | end | Solar saros 144 (16 of 70) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
March 3, 2007 | lunar (full) | beginning | Lunar saros 123 (52 of 72) | next new moon |
March 19, 2007 | solar (new) | end | Solar saros 149 (20 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
August 28, 2007 | lunar (full) | beginning | Lunar saros 128 (40 of 71) | next new moon |
September 11, 2007 | solar (new) | end | Solar saros 154 (6 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
February 7, 2008 | solar (new) | beginning | Solar saros 121 (60 of 71) | next full moon |
February 21, 2008 | lunar (full) | end | Lunar saros 133 (26 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
August 1, 2008 | solar (new) | beginning | Solar saros 126 (47 of 72) | next full moon |
August 16, 2008 | lunar (full) | end | Lunar saros 138 (28 of 82) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
January 26, 2009 | solar (new) | beginning | Solar saros 131 (50 of 70) | next full moon |
February 9, 2009 | lunar (full) | end | Lunar saros 143 (17 of 72) | next eclipse season |
... no eclipses for about 5 months... | ||||
July 7, 2009 | lunar (full) | beginning | Lunar saros 110 (71 of 72) | next new moon |
July 22, 2009 | solar (new) | middle | Solar saros 136 (37 of 71) | next full moon |
August 6, 2009 | lunar (full) | end | Lunar saros 148 (3 of 70) | next eclipse season |
... no eclipses for about 5 months... | ||||
December 31, 2009 | lunar (full) | beginning | Lunar saros 115 (57 of 72) | next new moon |
January 15, 2010 | solar (new) | end | Solar saros 141 (23 of 70) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
June 26, 2010 | lunar (full) | beginning | Lunar saros 120 (57 of 83) | next new moon |
July 11, 2010 | solar (new) | end | Solar saros 146 (27 of 76) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
December 21, 2010 | lunar (full) | beginning | Lunar saros 125 (48 of 72) | next new moon |
January 4, 2011 | solar (new) | end | Solar saros 151 (14 of 72) | next eclipse season |
... no eclipses for about 5 months... | ||||
June 1, 2011 | solar (new) | beginning | Solar saros 118 (68 of 72) | next full moon |
June 15, 2011 | lunar (full) | middle | Lunar saros 130 (34 of 71) | next new moon |
July 1, 2011 | solar (new) | end | Solar saros 156 (1 of 69) | next eclipse season |
... no eclipses for about 5 months... | ||||
November 25, 2011 | solar (new) | beginning | Solar saros 123 (53 of 70) | next full moon |
December 10, 2011 | lunar (full) | end | Lunar saros 135 (23 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
May 20, 2012 | solar (new) | beginning | Solar saros 128 (58 of 73) | next full moon |
June 4, 2012 | lunar (full) | end | Lunar saros 140 (24 of 77) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
November 13, 2012 | solar (new) | beginning | Solar saros 133 (45 of 72) | next full moon |
November 28, 2012 | lunar (full) | end | Lunar saros 145 (11 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
April 25, 2013 | lunar (full) | beginning | Lunar saros 112 (65 of 72) | next new moon |
May 10, 2013 | solar (new) | middle | Solar saros 138 (31 of 70) | next full moon |
May 25, 2013 | lunar (full) | end | Lunar saros 150 (1 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
October 18, 2013 | lunar (full) | beginning | Lunar saros 117 (52 of 71) | next new moon |
November 3, 2013 | solar (new) | end | Solar saros 143 (23 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
April 15, 2014 | lunar (full) | beginning | Lunar saros 122 (56 of 74) | next new moon |
April 29, 2014 | solar (new) | end | Solar saros 148 (21 of 75) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
October 8, 2014 | lunar (full) | beginning | Lunar saros 127 (42 of 72) | next new moon |
October 23, 2014 | solar (new) | end | Solar saros 153 (9 of 70) | next eclipse season |
... no eclipses for about 5 months... | ||||
March 20, 2015 | solar (new) | beginning | Solar saros 120 (61 of 71) | next full moon |
April 4, 2015 | lunar (full) | end | Lunar saros 132 (30 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
September 13, 2015 | solar (new) | beginning | Solar saros 125 (54 of 73) | next full moon |
September 28, 2015 | lunar (full) | end | Lunar saros 137 (26 of 78) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
March 9, 2016 | solar (new) | beginning | Solar saros 130 (52 of 73) | next full moon |
March 23, 2016 | lunar (full) | end | Lunar saros 142 (18 of 73) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
September 1, 2016 | solar (new) | beginning | Solar saros 135 (39 of 71) | next full moon |
September 16, 2016 | lunar (full) | end | Lunar saros 147 (8 of 70) | next eclipse season |
... no eclipses for about 5 months... | ||||
February 11, 2017 | lunar (full) | beginning | Lunar saros 114 (59 of 71) | next new moon |
February 26, 2017 | solar (new) | end | Solar saros 140 (29 of 71) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
August 7, 2017 | lunar (full) | beginning | Lunar saros 119 (61 of 82) | next new moon |
August 21, 2017 | solar (new) | end | Solar saros 145 (22 of 77) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
January 31, 2018 | lunar (full) | beginning | Lunar saros 124 (49 of 73) | next new moon |
February 15, 2018 | solar (new) | end | Solar saros 150 (17 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
July 13, 2018 | solar (new) | beginning | Solar saros 117 (69 of 71) | next full moon |
July 27, 2018 | lunar (full) | middle | Lunar saros 129 (38 of 71) | next new moon |
August 11, 2018 | solar (new) | end | Solar saros 155 (6 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
January 6, 2019 | solar (new) | beginning | Solar saros 122 (58 of 70) | next full moon |
January 21, 2019 | lunar (full) | end | Lunar saros 134 (27 of 72) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
July 2, 2019 | solar (new) | beginning | Solar saros 127 (58 of 82) | next full moon |
July 16, 2019 | lunar (full) | end | Lunar saros 139 (21 of 79) | next eclipse season |
... no eclipses for about 5 and a half months... | ||||
December 26, 2019 | solar (new) | beginning | Solar saros 132 (46 of 71) | next full moon |
January 10, 2020 | lunar (full) | end | Lunar saros 144 (16 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
June 5, 2020 | lunar (full) | beginning | Lunar saros 111 (67 of 71) | next new moon |
June 21, 2020 | solar (new) | middle | Solar saros 137 (36 of 70) | next full moon |
July 5, 2020 | lunar (full) | end | Lunar saros 149 (3 of 71) | next eclipse season |
... no eclipses for about 5 months... | ||||
November 30, 2020 | lunar (full) | beginning | Lunar saros 116 (58 of 73) | next new moon |
December 14, 2020 | solar (new) | end | Solar saros 142 (23 of 72) | next eclipse season |
The penumbral lunar eclipse of November 29–30, 2020 was followed by the solar eclipse of December 14, 2020.
In each sequence below, each eclipse is separated by a fortnight. The first and last eclipse in each sequence is separated by one synodic month. See also Eclipse cycles .
July 7th Ascending node (full moon) | July 22nd Descending node (new moon) | August 6th Ascending node (full moon) |
---|---|---|
Penumbral lunar eclipse Lunar saros 110 | Total solar eclipse Solar saros 136 | Penumbral lunar eclipse Lunar saros 148 |
July 13th Ascending node (new moon) | July 27th Descending node (full moon) | August 11th Ascending node (new moon) |
---|---|---|
Partial solar eclipse Solar saros 117 | Total lunar eclipse Lunar saros 129 | Partial solar eclipse Solar saros 155 |
(The two eclipse seasons above share similarities (lunar or solar centrality and gamma of each eclipse in the same column) because they are a half saros apart.) [4]
In each sequence below, each eclipse is separated by a fortnight. The first and last eclipse in each sequence is separated by one synodic month. See also Eclipse cycles .
July 6th Descending node (full moon) | July 20th Ascending node (new moon) | August 4th Descending node (full moon) |
---|---|---|
Penumbral lunar eclipse Lunar saros 109 | Annular solar eclipse Solar saros 135 | Penumbral lunar eclipse Lunar saros 147 |
July 11th Descending node (new moon) | July 26th Ascending node (full moon) | August 9th Descending node (new moon) |
---|---|---|
Partial solar eclipse Solar saros 116 | Total lunar eclipse Lunar saros 128 | Partial solar eclipse Solar saros 154 |
(The two eclipse seasons above share similarities (lunar or solar centrality and gamma of each eclipse in the same column) because they are a half saros apart.) [4]
In each sequence below, each eclipse is separated by a fortnight. The first and last eclipse in each sequence is separated by one synodic month. See also Eclipse cycles .
July 21st Ascending node (new moon) | August 4th Descending node (full moon) | August 20th Ascending node (new moon) |
---|---|---|
Partial solar eclipse Solar saros 115 | Total lunar eclipse Lunar saros 127 | Partial solar eclipse Solar saros 153 |
July 26th Ascending node (full moon) | August 10th Descending node (new moon) | August 24th Ascending node (full moon) |
---|---|---|
Penumbral lunar eclipse Lunar saros 108 | Annular solar eclipse Solar saros 134 | Penumbral lunar eclipse Lunar saros 146 |
(The two eclipse seasons above share similarities (lunar or solar centrality and gamma of each eclipse in the same column) because they are a half saros apart.) [4]
Eclipses may occur repeatedly, separated by certain intervals of time: these intervals are called eclipse cycles. The series of eclipses separated by a repeat of one of these intervals is called an eclipse series.
The saros is a period of exactly 223 synodic months, approximately 6585.321 days, or 18 years plus 10, 11, or 12 days, and 8 hours, that can be used to predict eclipses of the Sun and Moon. One saros period after an eclipse, the Sun, Earth, and Moon return to approximately the same relative geometry, a near straight line, and a nearly identical eclipse will occur, in what is referred to as an eclipse cycle. A sar is one half of a saros.
An exeligmos is a period of 54 years, 33 days that can be used to predict successive eclipses with similar properties and location. For a solar eclipse, after every exeligmos a solar eclipse of similar characteristics will occur in a location close to the eclipse before it. For a lunar eclipse the same part of the earth will view an eclipse that is very similar to the one that occurred one exeligmos before it. The exeligmos is an eclipse cycle that is a triple saros, three saroses long, with the advantage that it has nearly an integer number of days so the next eclipse will be visible at locations and times near the eclipse that occurred one exeligmos earlier. In contrast, each saros, an eclipse occurs about eight hours later in the day or about 120° to the west of the eclipse that occurred one saros earlier.
A total lunar eclipse will take place on May 26, 2040. The northern limb of the Moon will pass through the center of the Earth's shadow. This is the second central lunar eclipse of Saros series 131. This lunar event will occur near perigee, as a result, it will be referred to as a "super flower blood moon" or "super blood moon", though not quite as close to Earth as the eclipse of May 26, 2021.
A total lunar eclipse will take place between Monday and Tuesday, June 25-26, 2029. A central total eclipse lasting 1 hour and 41 minutes 53 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 color at maximum eclipse. It will be able to be seen from most of the Americas, Western Europe and Africa. The partial eclipse will last for 3 hours and 39 minutes 32 seconds in total.
A total lunar eclipse took place on Saturday, April 13, 1968, the first of two total eclipses in 1968, the second being on October 6, 1968.
A total lunar eclipse will take place on June 6, 2058. The Moon will pass through the center of the Earth's shadow.
An annular solar eclipse occurred on Tuesday, April 29, 2014. 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 center of the Moon's shadow missed the Earth's South Pole, but the partial eclipse was visible from parts of Antarctica and Australia, and an annular eclipse was visible from a small part of Antarctica.
A total lunar eclipse took place at the Moon's descending node of the orbit on Tuesday, May 24, 1910 with an umbral eclipse magnitude of 1.09503. A total lunar eclipse takes place when the Earth comes between the Sun and the Moon and its shadow covers the Moon. Eclipse watchers can see the Moon turn red when the eclipse reaches totality. Total eclipses of the Moon happen at Full Moon when the Sun, Earth, and Moon are aligned to form a line. The astronomical term for this type of alignment is syzygy, which comes from the Greek word for being paired together. The Moon does not have its own light but shines because its surface reflects the Sun's rays. During a total lunar eclipse, the Earth comes between the Sun and the Moon and blocks any direct sunlight from reaching the Moon. The Sun casts the Earth's shadow on the Moon's surface. A shallow total eclipse saw the Moon in relative darkness for 49 minutes and 29.5 seconds. The Moon was 9.503% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 35 minutes and 22.9 seconds in total.
A partial solar eclipse occurred on July 31, 2000. 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. It was visible from northern Russia, northeastern Scandinavia, northern Greenland, western Canada, and the northwestern United States.
A total solar eclipse will occur at the Moon's descending node of the orbit on Saturday, March 30, 2052. 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 cross central Mexico and the southeastern states of the United States. Almost all of North America and the northern edge of South America will see a partial eclipse. It will be the 2nd total eclipse visible from the Florida Panhandle and southwest Georgia in 6.6 years. It will be the first total solar eclipse visible from Solar Saros 130 in 223 synodic months. It will be the last total solar eclipse visible in the United States until May 11, 2078.
An annular solar eclipse occurred at the Moon's descending node of the orbit on December 4, 1983. 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 Cape Verde, Annobón Island of Equatorial Guinea, Gabon, the People's Republic of Congo, Zaire, northern Uganda, southern Sudan, northwestern Kenya, Ethiopia and Somalia. The Sun's altitude was 66°. Occurring 6.5 days before apogee, the Moon's apparent diameter was near the average diameter.
A total solar eclipse occurred on Tuesday, June 30, 1992. 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 southeastern Uruguay and southern tip of Rio Grande do Sul, Brazil.
An annular solar eclipse occurred at the Moon's descending node of the orbit on February 4–5, 1981. 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. This annular solar eclipse was large because the Moon covered 99.4% of the Sun, with a path width of only 25 km . It was visible in Australia, crossing over Tasmania and southern Stewart Island of New Zealand near sunrise on February 5 (Thursday), and ended at sunset over western South America on February 4 (Wednesday). Occurring only 4 days before perigee, the moon's apparent diameter was larger.
An annular solar eclipse occurred at the Moon's ascending node of the orbit on August 10, 1980, centred over the 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. 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 Tabuaeran of Kiribati, Peru, Bolivia, northern Paraguay and Brazil. Occurring 5 days before apogee, the Moon's apparent diameter was smaller. At greatest eclipse, the Sun was 79 degrees above horizon.
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 March 18, 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 part of Indonesia, and two atolls in the Trust Territory of the Pacific Islands which belongs to the Federated States of Micronesia now.
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.
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.
An annular solar eclipse will occur on Friday, November 4, 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. 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 Pacific Ocean, South America, and Atlantic Ocean. The tables below contain detailed predictions and additional information on the Annular Solar Eclipse of 4 November 2078.