Solar eclipse of July 3, 2065
| Partial eclipse | |
 Map | |
| Gamma | 1.4619 |
|---|---|
| Magnitude | 0.1638 |
| Maximum eclipse | |
| Coordinates | Lua error: callParserFunction: function "#coordinates" was not found. |
| Times (UTC) | |
| Greatest eclipse | 17:33:52 |
| References | |
| Saros | 118 (71 of 72) |
| Catalog # (SE5000) | 9654 |
A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, July 3, 2065,[1] with a magnitude of 0.1638. 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.
This will be the second of four partial solar eclipses in 2065, with the others occurring on February 5, August 2, and December 27.
The partial solar eclipse will be visible for parts of Northern Europe and northern Russia.
Eclipse details
[edit | edit source]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 July 3 at 16:32:44.5 UTC |
| Equatorial Conjunction | 2065 July 3 at 17:01:37.1 UTC |
| Ecliptic Conjunction | 2065 July 3 at 17:17:29.5 UTC |
| Greatest Eclipse | 2065 July 3 at 17:33:52.5 UTC |
| Last Penumbral External Contact | 2065 July 3 at 18:35:10.0 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.16388 |
| Eclipse Obscuration | 0.07678 |
| Gamma | 1.46186 |
| Sun Right Ascension | 06h53m43.9s |
| Sun Declination | +22°51'26.7" |
| Sun Semi-Diameter | 15'43.9" |
| Sun Equatorial Horizontal Parallax | 08.6" |
| Moon Right Ascension | 06h54m50.6s |
| Moon Declination | +24°10'43.8" |
| Moon Semi-Diameter | 15'05.3" |
| Moon Equatorial Horizontal Parallax | 0°55'22.6" |
| ΔT | 94.2 s |
Eclipse season
[edit | edit source]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. The first and last eclipse in this sequence is separated by one synodic month.
| July 3 Descending node (new moon) |
July 17 Ascending node (full moon) |
August 2 Descending node (new moon) |
|---|---|---|
| Error creating thumbnail: | File:Lunar eclipse chart close-2065Jul17.png | File:SE2065Aug02P.png |
| Partial solar eclipse Solar Saros 118 |
Total lunar eclipse Lunar Saros 130 |
Partial solar eclipse Solar Saros 156 |
Related eclipses
[edit | edit source]Eclipses in 2065
[edit | edit source]- 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.
Metonic
[edit | edit source]- Followed by: Solar eclipse of April 21, 2069
Tzolkinex
[edit | edit source]- Preceded by: Solar eclipse of May 22, 2058
Half-Saros
[edit | edit source]- Preceded by: Lunar eclipse of June 27, 2056
- Followed by: Lunar eclipse of July 8, 2074
Tritos
[edit | edit source]- Preceded by: Solar eclipse of August 3, 2054
- Followed by: Solar eclipse of June 1, 2076
Solar Saros 118
[edit | edit source]- Preceded by: Solar eclipse of June 23, 2047
- Followed by: Solar eclipse of July 15, 2083
Inex
[edit | edit source]- Preceded by: Solar eclipse of July 23, 2036
- Followed by: Solar eclipse of June 13, 2094
Triad
[edit | edit source]- Followed by: Solar eclipse of May 4, 2152
Solar eclipses of 2065–2069
[edit | edit source]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 February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2065 to 2069 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | July 3, 2065 Error creating thumbnail: Partial |
1.4619 | 123 | December 27, 2065 File:SE2065Dec27P.png Partial |
−1.0688 | |
| 128 | June 22, 2066 File:SE2066Jun22A.png Annular |
0.733 | 133 | December 17, 2066 File:SE2066Dec17T.png Total |
−0.4043 | |
| 138 | June 11, 2067 File:SE2067Jun11A.png Annular |
−0.0387 | 143 | December 6, 2067 File:SE2067Dec06H.png Hybrid |
0.2845 | |
| 148 | May 31, 2068 File:SE2068May31T.png Total |
−0.797 | 153 | November 24, 2068 File:SE2068Nov24P.png Partial |
1.0299 | |
| 158 | May 20, 2069 File:SE2069May20P.png Partial |
−1.4852 | ||||
Saros 118
[edit | edit source]This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 totality was produced by member 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit.[4]
| Series members 57–72 occur between 1801 and 2083: | ||
|---|---|---|
| 57 | 58 | 59 |
| File:SE1813Feb01A.gif February 1, 1813 |
File:SE1831Feb12A.gif February 12, 1831 |
File:SE1849Feb23A.gif February 23, 1849 |
| 60 | 61 | 62 |
| File:SE1867Mar06A.gif March 6, 1867 |
File:SE1885Mar16A.gif March 16, 1885 |
File:SE1903Mar29A.png March 29, 1903 |
| 63 | 64 | 65 |
| File:SE1921Apr08A.png April 8, 1921 |
File:SE1939Apr19A.png April 19, 1939 |
File:SE1957Apr30A.png April 30, 1957 |
| 66 | 67 | 68 |
| File:SE1975May11P.png May 11, 1975 |
File:SE1993May21P.png May 21, 1993 |
File:SE2011Jun01P.png June 1, 2011 |
| 69 | 70 | 71 |
| File:SE2029Jun12P.png June 12, 2029 |
File:SE2047Jun23P.png June 23, 2047 |
Error creating thumbnail: July 3, 2065 |
| 72 | ||
| File:SE2083Jul15P.png July 15, 2083 | ||
Metonic series
[edit | edit source]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.
Tritos series
[edit | edit source]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 2054 and 2200 | ||||
|---|---|---|---|---|
| File:SE2054Aug03P.png August 3, 2054 (Saros 117) |
Error creating thumbnail: July 3, 2065 (Saros 118) |
File:SE2076Jun01P.png June 1, 2076 (Saros 119) |
File:SE2087May02P.png May 2, 2087 (Saros 120) |
File:SE2098Apr01P.png April 1, 2098 (Saros 121) |
| File:SE2109Mar01P.png March 1, 2109 (Saros 122) |
File:Saros123 59van70 SE2120Jan30P.jpg January 30, 2120 (Saros 123) |
File:Saros124 61van73 SE2130Dec30P.jpg December 30, 2130 (Saros 124) |
File:Saros125 61van73 SE2141Nov28P.jpg November 28, 2141 (Saros 125) |
File:Saros126 55van72 SE2152Oct28P.jpg October 28, 2152 (Saros 126) |
| File:Saros127 66van82 SE2163Sep28P.jpg September 28, 2163 (Saros 127) |
File:Saros128 67van73 SE2174Aug27P.jpg August 27, 2174 (Saros 128) |
File:Saros129 61van80 SE2185Jul26T.jpg July 26, 2185 (Saros 129) |
File:SE2196Jun26T.png June 26, 2196 (Saros 130) | |
Inex series
[edit | edit source]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.
The partial solar eclipses on January 1, 1805 (part of Saros 109) and November 21, 1862 (part of Saros 111) are also a part of this series but are not included in the table below.
| Series members between 2036 and 2200 | ||
|---|---|---|
| File:SE2036Jul23P.png July 23, 2036 (Saros 117) |
Error creating thumbnail: July 3, 2065 (Saros 118) |
File:SE2094Jun13P.png June 13, 2094 (Saros 119) |
| File:Saros120 67van71 SE2123May25P.jpg May 25, 2123 (Saros 120) |
File:Saros121 68van71 SE2152May04P.jpg May 4, 2152 (Saros 121) |
File:Saros122 67van70 SE2181Apr14P.jpg April 14, 2181 (Saros 122) |
References
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- ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
External links
[edit | edit source]- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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