Solar eclipse of March 30, 2033

Solar eclipse of March 30, 2033
	Map
Type of eclipse
Nature	Total
Gamma	0.9778
Magnitude	1.0462
Maximum eclipse
Duration	157 sec (2 m 37 s)
Coordinates	71.3°N 155.8°W
Max. width of band	781 km (485 mi)
Times (UTC)
Greatest eclipse	18:02:36
References
Saros	120 (62 of 71)
Catalog # (SE5000)	9581

A total solar eclipse will occur on March 30, 2033. 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 will be visible in Nome, Alaska, Utqiagvik, Alaska and Chukchi Peninsula in the mid-morning hours. This is the last of 55 umbral eclipses of Solar Saros 120. The 1st was in 1059. The total duration is 974 years.

Images

Animated path

Related eclipses

Solar eclipses of 2033–2036

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]

Solar eclipse series sets from 2033–2036
Descending node		Ascending node
120	March 30, 2033 Total	125	September 23, 2033 Partial
130	March 20, 2034 Total	135	September 12, 2034 Annular
140	March 9, 2035 Annular	145	September 2, 2035 Total
150	February 27, 2036 Partial	155	August 21, 2036 Partial
A partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.

Saros 120

This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and 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 occurs at the Moon’s descending node.

Series members 55–65 occur between 1901 and 2100
55	56	57
January 14, 1907	January 24, 1925	February 4, 1943
58	59	60
February 15, 1961	February 26, 1979	March 9, 1997
61	62	63
March 20, 2015	March 30, 2033	April 11, 2051
64	65
April 21, 2069	May 2, 2087

Metonic cycle

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).

21 eclipse events between June 12, 2029 and June 12, 2105
June 11–12	March 30–31	January 16	November 4–5	August 23–24
118	120	122	124	126
June 12, 2029	March 30, 2033	January 16, 2037	November 4, 2040	August 23, 2044
128	130	132	134	136
June 11, 2048	March 30, 2052	January 16, 2056	November 5, 2059	August 24, 2063
138	140	142	144	146
June 11, 2067	March 31, 2071	January 16, 2075	November 4, 2078	August 24, 2082
148	150	152	154
June 11, 2086	March 31, 2090	January 16, 2094	November 4, 2097

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.

External links

http://eclipse.gsfc.nasa.gov/SEplot/SEplot2001/SE2033Mar30T.GIF

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[1] 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.