Solar eclipse of February 7, 2073 | |
---|---|
Type of eclipse | |
Nature | Partial |
Gamma | 1.1651 |
Magnitude | 0.6768 |
Maximum eclipse | |
Coordinates | 70°30′N114°54′E / 70.5°N 114.9°E |
Times (UTC) | |
Greatest eclipse | 1:55:59 |
References | |
Saros | 122 (61 of 70) |
Catalog # (SE5000) | 9671 |
A partial solar eclipse will occur at the Moon's descending node of orbit on Tuesday, February 7, 2073, with a magnitude of 0.6768. 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.
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [1]
122 | February 7, 2073 Partial | 127 | August 3, 2073 Total |
132 | January 27, 2074 Annular | 137 | July 24, 2074 Annular |
142 | January 16, 2075 Total | 147 | July 13, 2075 Annular |
152 | January 6, 2076 Total | 157 | July 1, 2076 Partial |
It is a part of Saros cycle 122, repeating every 18 years, 11 days, containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171, hybrid eclipses on August 13, 1189 and August 25, 1207, and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. The longest duration of totality was 1 minute, 25 seconds on July 12, 1135, and the longest duration of annularity was 6 minutes, 28 seconds on October 10, 1874.
Series members 52-68 occur between 1900 and 2200: | ||
---|---|---|
52 | 53 | 54 |
November 2, 1910 | November 12, 1928 | November 23, 1946 |
55 | 56 | 57 |
December 4, 1964 | December 15, 1982 | December 25, 2000 |
58 | 59 | 60 |
January 6, 2019 | January 16, 2037 | January 27, 2055 |
61 | 62 | 63 |
February 7, 2073 | February 18, 2091 | March 1, 2109 |
64 | 65 | 66 |
March 13, 2127 | March 23, 2145 | April 3, 2163 |
67 | 68 | |
April 14, 2181 | April 25, 2199 |
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An annular solar eclipse will occur at the Moon’s ascending node of orbit on Tuesday, February 17, 2026, with a magnitude of 0.963. 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.
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An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 28, 2044, with a magnitude of 0.96. 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 total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, July 24, 2055, with a magnitude of 1.0359. 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.
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An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 17, 2064, with a magnitude of 0.9262. 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.
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