A total lunar eclipse took place on Sunday, July 26, 1953.
An annular solar eclipse occurred on Wednesday, May 30, 1984. 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 Mexico, the United States, Azores Islands, Morocco and Algeria. It was the first annular solar eclipse visible in the US in 33 years. The Moon's apparent diameter was near the average diameter because it occurred 6.7 days after apogee and 7.8 days before perigee.
An annular solar eclipse occurred on July 31, 1962. 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 only 4.7 days before apogee, the Moon's apparent diameter was larger. This solar eclipse occurred 44 days after the final game of 1962 FIFA World Cup.
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 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.
The Saros cycle series 120 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. 55 of these are umbral eclipses. The series started with a partial solar eclipse on May 27, 933 AD, and transitioned into an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and are total eclipses from June 8, 1564 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 118 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 72 events. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 119 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occur at the Moon's ascending node.
Saros cycle series 133 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 events. All eclipses in this series occur at the Moon's ascending node.
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 occur at the Moon's descending node.
Saros cycle series 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 events. 55 of these are umbral eclipses and other 15 of these are partial solar eclipses. All eclipses in this series occur at the Moon's ascending node.
Saros cycle series 139 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years and 11 days, containing 71 events. It has 16 partial solar eclipses, 12 will be hybrid and 43 will be total. The first total eclipse occurred on December 21, 1843, over southern Asia and lasted 1 minute and 43 seconds. The last total eclipse will occur on March 26, 2601, over Antarctica and the Southern Ocean, lasting 35 seconds.
Saros cycle series 140 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 141 for solar eclipses occurs at the Moon's ascending node, repeats every 18 years, 11 days and contains 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739 through October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. All eclipses in this series occur at the Moon's ascending node.
Saros cycle series 143 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years and 11 days, containing 72 events. It consisted of 10 partial eclipses, 12 total eclipses, 4 hybrid events, 26 annular eclipses, and ends with 20 partial eclipses. The longest total eclipse of the series was in 1887 at 3 minutes and 50 seconds. All eclipses in this series occur at the Moon's ascending node.
Saros cycle series 144 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 events. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 146 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 76 events. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 150 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 155 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days. Saros 155 contains 71 events in which of 15 will be partial solar eclipses and other 56 are umbral. There are 60 solar eclipses before 3000 AD. All eclipses in this series occur at the Moon's ascending node.
