Solar eclipse of January 5, 2038

Solar eclipse of January 5, 2038
Solar eclipse of January 5, 2038
	Map
Type of eclipse
Nature	Annular
Gamma	0.4169
Magnitude	0.9728
Maximum eclipse
Duration	198 s (3 min 18 s)
Coordinates	2°06′N 25°24′W / 2.1°N 25.4°W
Max. width of band	107 km (66 mi)
Times (UTC)
Greatest eclipse	13:47:11
References
Saros	132 (47 of 71)
Catalog # (SE5000)	9592

An annular solar eclipse will occur on January 5, 2038. 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.

Images edit

Animated path

Related eclipses edit

There are 7 eclipses in 2038 (the maximum possible), included four penumbral lunar eclipses: January 21, June 17, July 16, and December 11.

Solar eclipses of 2036–2039 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]

Note: Partial solar eclipses on February 27, 2036 and August 21, 2036 occur on the previod lunar year eclipse set.

Solar eclipse series sets from 2036 to 2039
Ascending node		Descending node
117	July 23, 2036 Partial	122	January 16, 2037 Partial
127	July 13, 2037 Total	132	January 5, 2038 Annular
137	July 2, 2038 Annular	142	December 26, 2038 Total
147	June 21, 2039 Annular	152	December 15, 2039 Total

Saros 132 edit

This eclipse is a part of Saros cycle 132, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on August 13, 1208. It contains annular eclipses from March 17, 1569 through March 12, 2146, hybrid on March 22, 2164 and April 3, 2182 and total eclipses from April 14, 2200 through June 19, 2308. The series ends at member 71 as a partial eclipse on September 25, 2470. The longest duration of annularity was 6 minutes, 56 seconds on May 9, 1641, and totality will be 2 minutes, 14 seconds on June 8, 2290. All eclipses in this series occurs at the Moon’s descending node.

Series members 28–50 occur between 1690 and 2100:
28	29	30
June 11, 1695	June 22, 1713	July 4, 1731
31	32	33
July 14, 1749	July 25, 1767	August 5, 1785
34	35	36
August 17, 1803	August 27, 1821	September 7, 1839
37	38	39
September 18, 1857	September 29, 1875	October 9, 1893
40	41	42
October 22, 1911	November 1, 1929	November 12, 1947
43	44	45
November 23, 1965	December 4, 1983	December 14, 2001
46	47	48
December 26, 2019	January 5, 2038	January 16, 2056
49	50
January 27, 2074	February 7, 2092

Metonic series 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). 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