Solar eclipse of March 30, 2052

A total solar eclipse will occur at the Moon's descending node of the orbit on Saturday, March 30, 2052. 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. The path of totality will cross central Mexico and the southeastern states of the United States. Almost all of North America and the northern edge of South America will see a partial eclipse. It will be the 2nd total eclipse visible from the Florida Panhandle and southwest Georgia in 6.6 years. It will be the first total solar eclipse visible from Solar Saros 130 in 223 synodic months. It will be the last total solar eclipse visible in the United States until May 11, 2078.

Solar eclipse of March 30, 2052
Map
Type of eclipse
NatureTotal
Gamma0.3238
Magnitude1.0466
Maximum eclipse
Duration248 s (4 min 8 s)
Coordinates22°24′N 102°30′W / 22.4°N 102.5°W / 22.4; -102.5
Max. width of band164 km (102 mi)
Times (UTC)
Greatest eclipse18:31:53
References
Saros130 (54 of 73)
Catalog # (SE5000)9623

Related eclipses edit

Solar eclipses 2051–2054 edit

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 2051 to 2054
Descending node   Ascending node
Saros Map Saros Map
120 April 11, 2051
 
Partial
125 October 4, 2051
 
Partial
130 March 30, 2052
 
Total
135 September 22, 2052
 
Annular
140 March 20, 2053
 
Annular
145 September 12, 2053
 
Total
150 March 9, 2054
 
Partial
155 September 2, 2054
 
Partial

Saros 130 edit

This eclipse is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular eclipses in the series. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occurs at the Moon’s descending node.[2]

Series members 43–56 between 1853 and 2300
43 44 45
 
November 30, 1853
 
December 12, 1871
 
December 22, 1889
46 47 48
 
January 3, 1908
 
January 14, 1926
 
January 25, 1944
49 50 51
 
February 5, 1962
 
February 16, 1980
 
February 26, 1998
52 53 54
 
March 9, 2016
 
March 20, 2034
 
March 30, 2052
55 56 57
 
April 11, 2070
 
April 21, 2088
 
May 3, 2106
58 59 60
 
May 14, 2124
 
May 25, 2142
 
June 4, 2160
61 62 63
 
June 16, 2178
 
June 26, 2196
 
July 8, 2214
64 65 66
 
July 18, 2232
 
July 30, 2250
 
August 9, 2268
67
 
August 20, 2286

Inex series edit

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Metonic cycle edit

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).

Notes edit

  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.
  2. ^ "Saros Series catalog of solar eclipses". NASA.

References edit