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Map | |
Type of eclipse | |
Nature | Annular |
Gamma | 0.4091 |
Magnitude | 0.9179 |
Maximum eclipse | |
Duration | 701 s (11 min 41 s) |
Coordinates | 1°00′N 169°42′W / 1°N 169.7°W / 1; -169.7 |
Max. width of band | 340 km (210 mi) |
Times (UTC) | |
Greatest eclipse | 23:05:37 |
References | |
Saros | 141 (22 of 70) |
Catalog # (SE5000) | 9490 |
An annular solar eclipse occurred on January 4-5, 1992. Template:Annular solar eclipse summary
Images
Related eclipses
Solar eclipses of 1990-1992
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.
Solar eclipse series sets from 1990 to 1992 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | January 26, 1990 Annular |
−0.9457 | 126 Partial in Finland |
July 22, 1990 Total |
0.7597 | |
131 | January 15, 1991 Annular |
−0.2727 | 136 Totality in Playas del Coco, Costa Rica |
July 11, 1991 Total |
−0.0041 | |
141 | January 4, 1992 Annular |
0.4091 | 146 | June 30, 1992 Total |
−0.7512 | |
151 | December 24, 1992 Partial |
1.0711 |
Saros 141
This eclipse is a part of Saros series 141, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2640. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on June 13, 2857. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 20 at 12 minutes, 9 seconds on December 14, 1955. All eclipses in this series occur at the Moon’s ascending node of orbit.
Series members 12–33 occur between 1801 and 2200: | ||
---|---|---|
12 | 13 | 14 |
September 17, 1811 |
September 28, 1829 |
October 9, 1847 |
15 | 16 | 17 |
October 19, 1865 |
October 30, 1883 |
November 11, 1901 |
18 | 19 | 20 |
November 22, 1919 |
December 2, 1937 |
December 14, 1955 |
21 | 22 | 23 |
December 24, 1973 |
January 4, 1992 |
January 15, 2010 |
24 | 25 | 26 |
January 26, 2028 |
February 5, 2046 |
February 17, 2064 |
27 | 28 | 29 |
February 27, 2082 |
March 10, 2100 |
March 22, 2118 |
30 | 31 | 32 |
April 1, 2136 |
April 12, 2154 |
April 23, 2172 |
33 | ||
May 4, 2190 |
Metonic series
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 ascending node.
22 eclipse events between January 5, 1935 and August 11, 2018 | ||||
---|---|---|---|---|
January 4–5 | October 23–24 | August 10–12 | May 30–31 | March 18–19 |
111 | 113 | 115 | 117 | 119 |
January 5, 1935 |
August 12, 1942 |
May 30, 1946 |
March 18, 1950 | |
121 | 123 | 125 | 127 | 129 |
January 5, 1954 |
October 23, 1957 |
August 11, 1961 |
May 30, 1965 |
March 18, 1969 |
131 | 133 | 135 | 137 | 139 |
January 4, 1973 |
October 23, 1976 |
August 10, 1980 |
May 30, 1984 |
March 18, 1988 |
141 | 143 | 145 | 147 | 149 |
January 4, 1992 |
October 24, 1995 |
August 11, 1999 |
May 31, 2003 |
March 19, 2007 |
151 | 153 | 155 | ||
January 4, 2011 |
October 23, 2014 |
August 11, 2018 |
References
- 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.
- "NASA - Catalog of Solar Eclipses of Saros 141". eclipse.gsfc.nasa.gov.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
Photos:
- APOD Ring of Fire Revisited, annular eclipse at sunset
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