Solar eclipse of February 5, 2065
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A partial solar eclipse will occur at the Moon's ascending node of orbit on Thursday, February 5, 2065,[1] with a magnitude of 0.9123. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
| Solar eclipse of February 5, 2065 | |
|---|---|
Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | 1.0336 |
| Magnitude | 0.9123 |
| Maximum eclipse | |
| Coordinates | 62°12′N 21°54′W / 62.2°N 21.9°W |
| Times (UTC) | |
| Greatest eclipse | 9:52:26 |
| References | |
| Saros | 151 (17 of 72) |
| Catalog # (SE5000) | 9652 |
This will be the first of four partial solar eclipses in 2065, with the others occurring on July 3, August 2, and December 27.
The partial solar eclipse will be visible for parts of North Africa, West Africa, Europe, and Central Asia.
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[2]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2065 February 05 at 07:40:45.3 UTC |
| Greatest Eclipse | 2065 February 05 at 09:52:25.5 UTC |
| Ecliptic Conjunction | 2065 February 05 at 10:03:58.8 UTC |
| Equatorial Conjunction | 2065 February 05 at 10:42:35.2 UTC |
| Last Penumbral External Contact | 2065 February 05 at 12:03:51.2 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.91233 |
| Eclipse Obscuration | 0.86757 |
| Gamma | 1.03356 |
| Sun Right Ascension | 21h18m22.7s |
| Sun Declination | -15°41'30.6" |
| Sun Semi-Diameter | 16'13.3" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 21h16m47.2s |
| Moon Declination | -14°47'52.5" |
| Moon Semi-Diameter | 15'25.7" |
| Moon Equatorial Horizontal Parallax | 0°56'37.5" |
| ΔT | 93.9 s |
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
| January 22 Descending node (full moon) |
February 5 Ascending node (new moon) |
|---|---|
| Total lunar eclipse Lunar Saros 125 |
Partial solar eclipse Solar Saros 151 |
- A total lunar eclipse on January 22.
- A partial solar eclipse on February 5.
- A partial solar eclipse on July 3.
- A total lunar eclipse on July 17.
- A partial solar eclipse on August 2.
- A partial solar eclipse on December 27.
- Preceded by: Solar eclipse of April 20, 2061
- Followed by: Solar eclipse of November 24, 2068
- Preceded by: Solar eclipse of December 26, 2057
- Followed by: Solar eclipse of March 19, 2072
- Preceded by: Lunar eclipse of February 1, 2056
- Followed by: Lunar eclipse of February 11, 2074
- Preceded by: Solar eclipse of March 9, 2054
- Followed by: Solar eclipse of January 6, 2076
- Preceded by: Solar eclipse of January 26, 2047
- Followed by: Solar eclipse of February 16, 2083
- Preceded by: Solar eclipse of February 27, 2036
- Followed by: Solar eclipse of January 16, 2094
- Preceded by: Solar eclipse of April 7, 1978
- Followed by: Solar eclipse of December 8, 2151
Solar eclipses of 2062–2065
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.[3]
The partial solar eclipses on July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2062 to 2065 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 121 | March 11, 2062 Partial |
−1.0238 | 126 | September 3, 2062 Partial |
1.0191 | |
| 131 | February 28, 2063 Annular |
−0.336 | 136 | August 24, 2063 Total |
0.2771 | |
| 141 | February 17, 2064 Annular |
0.3597 | 146 | August 12, 2064 Total |
−0.4652 | |
| 151 | February 5, 2065 Partial |
1.0336 | 156 | August 2, 2065 Partial |
−1.2759 | |
This eclipse is a part of Saros series 151, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on August 14, 1776. It contains annular eclipses from February 28, 2101 through April 23, 2191; a hybrid eclipse on May 5, 2209; and total eclipses from May 16, 2227 through July 6, 2912. The series ends at member 72 as a partial eclipse on October 1, 3056. 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 will be produced by member 19 at 2 minutes, 44 seconds on February 28, 2101, and the longest duration of totality will be produced by member 60 at 5 minutes, 41 seconds on May 22, 2840. All eclipses in this series occur at the Moon’s ascending node of orbit.[4]
| Series members 3–24 occur between 1801 and 2200: | ||
|---|---|---|
| 3 | 4 | 5 |
| September 5, 1812 |
September 17, 1830 |
September 27, 1848 |
| 6 | 7 | 8 |
| October 8, 1866 |
October 19, 1884 |
October 31, 1902 |
| 9 | 10 | 11 |
| November 10, 1920 |
November 21, 1938 |
December 2, 1956 |
| 12 | 13 | 14 |
| December 13, 1974 |
December 24, 1992 |
January 4, 2011 |
| 15 | 16 | 17 |
| January 14, 2029 |
January 26, 2047 |
February 5, 2065 |
| 18 | 19 | 20 |
| February 16, 2083 |
February 28, 2101 |
March 11, 2119 |
| 21 | 22 | 23 |
| March 21, 2137 |
April 2, 2155 |
April 12, 2173 |
| 24 | ||
| April 23, 2191 | ||
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.
| 21 eclipse events between July 1, 2000 and July 1, 2076 | ||||
|---|---|---|---|---|
| July 1–2 | April 19–20 | February 5–7 | November 24–25 | September 12–13 |
| 117 | 119 | 121 | 123 | 125 |
| July 1, 2000 |
April 19, 2004 |
February 7, 2008 |
November 25, 2011 |
September 13, 2015 |
| 127 | 129 | 131 | 133 | 135 |
| July 2, 2019 |
April 20, 2023 |
February 6, 2027 |
November 25, 2030 |
September 12, 2034 |
| 137 | 139 | 141 | 143 | 145 |
| July 2, 2038 |
April 20, 2042 |
February 5, 2046 |
November 25, 2049 |
September 12, 2053 |
| 147 | 149 | 151 | 153 | 155 |
| July 1, 2057 |
April 20, 2061 |
February 5, 2065 |
November 24, 2068 |
September 12, 2072 |
| 157 | ||||
| July 1, 2076 | ||||
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||||
|---|---|---|---|---|
| February 21, 1803 (Saros 127) |
January 21, 1814 (Saros 128) |
December 20, 1824 (Saros 129) |
November 20, 1835 (Saros 130) |
October 20, 1846 (Saros 131) |
| September 18, 1857 (Saros 132) |
August 18, 1868 (Saros 133) |
July 19, 1879 (Saros 134) |
June 17, 1890 (Saros 135) |
May 18, 1901 (Saros 136) |
| April 17, 1912 (Saros 137) |
March 17, 1923 (Saros 138) |
February 14, 1934 (Saros 139) |
January 14, 1945 (Saros 140) |
December 14, 1955 (Saros 141) |
| November 12, 1966 (Saros 142) |
October 12, 1977 (Saros 143) |
September 11, 1988 (Saros 144) |
August 11, 1999 (Saros 145) |
July 11, 2010 (Saros 146) |
| June 10, 2021 (Saros 147) |
May 9, 2032 (Saros 148) |
April 9, 2043 (Saros 149) |
March 9, 2054 (Saros 150) |
February 5, 2065 (Saros 151) |
| January 6, 2076 (Saros 152) |
December 6, 2086 (Saros 153) |
November 4, 2097 (Saros 154) |
October 5, 2108 (Saros 155) |
September 5, 2119 (Saros 156) |
| August 4, 2130 (Saros 157) |
July 3, 2141 (Saros 158) |
June 3, 2152 (Saros 159) |
April 1, 2174 (Saros 161) | |
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.
| Series members between 1801 and 2200 | ||
|---|---|---|
| August 5, 1804 (Saros 142) |
July 17, 1833 (Saros 143) |
June 27, 1862 (Saros 144) |
| June 6, 1891 (Saros 145) |
May 18, 1920 (Saros 146) |
April 28, 1949 (Saros 147) |
| April 7, 1978 (Saros 148) |
March 19, 2007 (Saros 149) |
February 27, 2036 (Saros 150) |
| February 5, 2065 (Saros 151) |
January 16, 2094 (Saros 152) |
December 28, 2122 (Saros 153) |
| December 8, 2151 (Saros 154) |
November 17, 2180 (Saros 155) |
|
- ^ "February 5, 2065 Partial Solar Eclipse". timeanddate. Retrieved 19 August 2024.
- ^ "Partial Solar Eclipse of 2065 Feb 05". EclipseWise.com. Retrieved 19 August 2024.
- ^ 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 151". eclipse.gsfc.nasa.gov.
