Solar eclipse of May 30, 1965
Solar eclipse of May 30, 1965 | |
---|---|
Type of eclipse | |
Nature | Total |
Gamma | −0.4225 |
Magnitude | 1.0544 |
Maximum eclipse | |
Duration | 315 s (5 min 15 s) |
Coordinates | 2°30′S 133°48′W / 2.5°S 133.8°W |
Max. width of band | 198 km (123 mi) |
Times (UTC) | |
Greatest eclipse | 21:17:31 |
References | |
Saros | 127 (55 of 82) |
Catalog # (SE5000) | 9432 |
A total solar eclipse occurred on May 30, 1965. Template:Total solar eclipse summary
Related eclipses
Solar eclipses of 1964-1967
This eclipse is a member of a 1964–1967 series at alternating nodes every 6 synodic months.
Note: Partial solar eclipses on January 14, 1964 and July 9, 1964 belong to the previous lunar year set.
Solar eclipse series sets from 1964 to 1967 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
117 | 1964 June 10 Partial |
−1.13926 | 122 | 1964 December 04 Partial |
1.11929 | |
127 | 1965 May 30 Total |
−0.42251 | 132 | 1965 November 23 Annular |
0.39061 | |
137 | 1966 May 20 Annular |
0.34672 | 142 | 1966 November 12 Total |
−0.33001 | |
147 | 1967 May 09 Partial |
1.14218 | 152 | 1967 November 02 Total (non-central) |
−1.00067 |
Saros 127
It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. There are no annular eclipses in this series. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532. All eclipses in this series occurs at the Moon’s ascending node.[1]
Series members 52–68 occur between 1901 and 2200 | ||
---|---|---|
52 | 53 | 54 |
April 28, 1911 |
May 9, 1929 |
May 20, 1947 |
55 | 56 | 57 |
May 30, 1965 |
June 11, 1983 |
June 21, 2001 |
58 | 59 | 60 |
July 2, 2019 |
July 13, 2037 |
July 24, 2055 |
61 | 62 | 63 |
August 3, 2073 |
August 15, 2091 |
August 26, 2109 (Partial) |
64 | 65 | 66 |
September 6, 2127 (Partial | September 16, 2145 (Partial) | September 28, 2163 (Partial) |
67 | 68 | |
October 8, 2181 (Partial) | October 19, 2199 (Partial) |
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
- ^ "Solar Saros series 127". NASA Goddard Space Flight Center. NASA. Retrieved 2 November 2017.
External links
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Russia expedition for solar eclipse of May 30, 1965