A partial solar eclipse will occur on March 19, 2072. 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.
| Solar eclipse of March 19, 2072 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | -1.1405 |
| Magnitude | 0.7199 |
| Maximum eclipse | |
| Coordinates | 72°12′S 30°24′W / 72.2°S 30.4°W |
| Times (UTC) | |
| Greatest eclipse | 20:10:31 |
| References | |
| Saros | 150 (20 of 71) |
| Catalog # (SE5000) | 9669 |
Related eclipsesEdit
Solar eclipses 2069–2072Edit
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]
| 120 | April 21, 2069 Partial |
125 | October 15, 2069 Partial |
| 130 | April 11, 2070 Total |
135 | October 4, 2070 Annular |
| 140 | March 31, 2071 Annular |
145 | September 23, 2071 Total |
| 150 | March 19, 2072 Partial |
155 | September 12, 2072 Total |
Saros 150Edit
It is a part of Saros cycle 150, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no total eclipses in this series. The series ends at member 71 as a partial eclipse on September 29, 2991. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.
| Series members 11-21 occur between 1901 and 2100: | ||
|---|---|---|
| 11 | 12 | 13 |
 December 12, 1909 |
 December 24, 1927 |
 January 3, 1946 |
| 14 | 15 | 16 |
 January 14, 1964 |
 January 25, 1982 |
 February 5, 2000 |
| 17 | 18 | 19 |
 February 15, 2018 |
 February 27, 2036 |
 March 9, 2054 |
| 20 | 21 | |
| March 19, 2072 |
 March 31, 2090 | |
Metonic seriesEdit
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.
| 21 eclipse events between June 1, 2011 and June 1, 2087 | ||||
|---|---|---|---|---|
| May 31 – June 1 | March 19–20 | January 5–6 | October 24–25 | August 12–13 |
| 118 | 120 | 122 | 124 | 126 |
 June 1, 2011 |
 March 20, 2015 |
 January 6, 2019 |
 October 25, 2022 |
 August 12, 2026 |
| 128 | 130 | 132 | 134 | 136 |
 June 1, 2030 |
 March 20, 2034 |
 January 5, 2038 |
 October 25, 2041 |
 August 12, 2045 |
| 138 | 140 | 142 | 144 | 146 |
 May 31, 2049 |
 March 20, 2053 |
 January 5, 2057 |
 October 24, 2060 |
 August 12, 2064 |
| 148 | 150 | 152 | 154 | 156 |
 May 31, 2068 |
March 19, 2072 |
 January 6, 2076 |
 October 24, 2079 |
 August 13, 2083 |
| 158 | 160 | 162 | 164 | 166 |
 June 1, 2087 |
 October 24, 2098 |
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ReferencesEdit
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
External linksEdit
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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