| Partial eclipse | |
 Map | |
| Gamma | 1.3766 |
|---|---|
| Magnitude | 0.3129 |
| Maximum eclipse | |
| Coordinates | 65°48′N178°00′W / 65.8°N 178°W /65.8; -178 |
| Times (UTC) | |
| Greatest eclipse | 10:52:31 |
| References | |
| Saros | 118 (70 of 72) |
| Catalog # (SE5000) | 9612 |
A partialsolar eclipse will occur at the Moon'sdescending node of orbit on Sunday, June 23, 2047,[1] with amagnitude of 0.3129. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, 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 2047, with the others occurring onJanuary 26,July 22, andDecember 16.
The partial solar eclipse will be visible for parts of northernCanada, northernAlaska, northernGreenland, andNortheast Asia.
Animated path
| Country or territory | City or place | Start of partial eclipse | Maximum eclipse | End of partial eclipse | Duration of eclipse (hr:min) | Maximum coverage | |||
|---|---|---|---|---|---|---|---|---|---|
 Canada | Coral Harbour | 04:31:49 | 04:49:59 | 05:08:24 | 0:37 | 1.30% | |||
| Canada | Baker Lake | 04:29:51 | 04:55:51 | 05:22:19 | 0:52 | 4.41% | |||
| Canada | Pond Inlet | 05:38:31 | 06:03:41 | 06:29:13 | 0:51 | 3.07% | |||
| Canada | Yellowknife | 03:40:27 (sunrise) | 04:04:23 | 04:35:42 | 0:55 | 8.83% | |||
 Greenland | Pituffik | 06:45:09 | 07:10:26 | 07:36:01 | 0:51 | 2.82% | |||
| Canada | Resolute | 04:39:18 | 05:11:06 | 05:43:21 | 1:04 | 6.99% | |||
| Canada | Grise Fiord | 05:41:58 | 06:11:37 | 06:41:40 | 1:00 | 5.09% | |||
| Greenland | Qaanaaq | 08:45:59 | 09:12:25 | 09:39:09 | 0:53 | 3.23% | |||
| Canada | Eureka | 04:46:53 | 05:18:57 | 05:51:22 | 1:04 | 6.34% | |||
| Canada | Inuvik | 03:44:59 | 04:21:32 | 04:58:25 | 1:13 | 14.87% | |||
| Canada | Alert | 05:53:48 | 06:23:15 | 06:52:57 | 0:59 | 4.31% | |||
 United States | Nuiqsut | 01:54:22 | 02:32:56 | 03:11:37 | 1:17 | 17.61% | |||
| United States | Point Hope | 02:03:42 | 02:42:50 | 03:21:52 | 1:18 | 19.30% | |||
 Russia | Anadyr | 22:16:05 | 22:46:44 | 23:02:52 (sunset) | 0:47 | 18.18% | |||
| Russia | Pevek | 22:16:39 | 22:56:34 | 23:36:07 | 1:19 | 19.02% | |||
| United States | Fairbanks | 02:59:00 (sunrise) | 03:02:53 | 03:06:33 | 0:08 | 1.19% | |||
| Russia | Srednekolymsk | 21:28:53 | 22:08:12 | 22:46:52 | 1:18 | 17.52% | |||
| Russia | Magadan | 21:41:24 | 22:12:51 | 22:19:50 (sunset) | 0:38 | 15.34% | |||
| Russia | Tiksi | 19:35:35 | 20:13:42 | 20:51:04 | 1:15 | 12.49% | |||
| Russia | Verkhoyansk | 20:40:33 | 21:18:26 | 21:55:30 | 1:15 | 13.49% | |||
| Russia | Khatanga | 17:45:51 | 18:18:39 | 18:50:45 | 1:05 | 6.22% | |||
| Russia | Norilsk | 18:00:23 | 18:24:33 | 18:48:16 | 0:48 | 2.13% | |||
| Russia | Yakutsk | 19:52:47 | 20:28:20 | 21:03:00 | 1:10 | 11.57% | |||
 China | Qiqihar | 19:29:15 | 19:40:50 | 19:44:41 (sunset) | 0:15 | 2.05% | |||
| China | Mohe | 19:17:19 | 19:45:15 | 20:12:30 | 0:55 | 5.70% | |||
| Russia | Chita | 20:29:29 | 20:51:50 | 21:13:40 | 0:44 | 2.61% | |||
| China | Hulunbuir | 19:29:35 | 19:52:07 | 20:10:15 (sunset) | 0:41 | 2.99% | |||
| Russia | Irkutsk | 19:42:16 | 19:55:49 | 20:09:08 | 0:27 | 0.51% | |||
 Mongolia | Choibalsan | 19:40:07 | 19:56:58 | 20:13:32 | 0:33 | 1.18% | |||
| References:[1] | |||||||||
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 | 2047 June 23 at 09:29:32.0 UTC |
| Equatorial Conjunction | 2047 June 23 at 10:34:45.0 UTC |
| Ecliptic Conjunction | 2047 June 23 at 10:37:04.7 UTC |
| Greatest Eclipse | 2047 June 23 at 10:52:30.6 UTC |
| Last Penumbral External Contact | 2047 June 23 at 12:15:32.3 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.31293 |
| Eclipse Obscuration | 0.19776 |
| Gamma | 1.37663 |
| Sun Right Ascension | 06h08m27.7s |
| Sun Declination | +23°25'10.2" |
| Sun Semi-Diameter | 15'44.2" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 06h09m05.2s |
| Moon Declination | +24°40'56.6" |
| Moon Semi-Diameter | 15'07.9" |
| Moon Equatorial Horizontal Parallax | 0°55'32.1" |
| ΔT | 82.6 s |
This eclipse is part of aneclipse 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 afortnight. The first and last eclipse in this sequence is separated by onesynodic month.
| June 23 Descending node (new moon) | July 7 Ascending node (full moon) | July 22 Descending node (new moon) |
|---|---|---|
|  |  |
| Partial solar eclipse Solar Saros 118 | Total lunar eclipse Lunar Saros 130 | Partial solar eclipse Solar Saros 156 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[3]
The partial solar eclipses onJanuary 26, 2047 andJuly 22, 2047 occur in the previous lunar year eclipse set.
| Solar eclipse series sets from 2047 to 2050 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 118 | June 23, 2047 Partial | 1.3766 | 123 | December 16, 2047 Partial | −1.0661 | |
| 128 | June 11, 2048 Annular | 0.6468 | 133 | December 5, 2048 Total | −0.3973 | |
| 138 | May 31, 2049 Annular | −0.1187 | 143 | November 25, 2049 Hybrid | 0.2943 | |
| 148 | May 20, 2050 Hybrid | −0.8688 | 153 | November 14, 2050 Partial | 1.0447 | |
This eclipse is a part ofSaros 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 throughApril 30, 1957. The series ends at member 72 as a partial eclipse onJuly 15, 2083. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos 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’sdescending node of orbit.[4]
| Series members 57–72 occur between 1801 and 2083: | ||
|---|---|---|
| 57 | 58 | 59 |
 February 1, 1813 |  February 12, 1831 |  February 23, 1849 |
| 60 | 61 | 62 |
 March 6, 1867 |  March 16, 1885 |  March 29, 1903 |
| 63 | 64 | 65 |
 April 8, 1921 |  April 19, 1939 |  April 30, 1957 |
| 66 | 67 | 68 |
 May 11, 1975 |  May 21, 1993 |  June 1, 2011 |
| 69 | 70 | 71 |
 June 12, 2029 | June 23, 2047 |  July 3, 2065 |
| 72 | ||
 July 15, 2083 | ||
Themetonic 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.
| 22 eclipse events between June 23, 2047 and November 16, 2134 | ||||
|---|---|---|---|---|
| June 22–23 | April 10–11 | January 27–29 | November 15–16 | September 3–5 |
| 118 | 120 | 122 | 124 | 126 |
June 23, 2047 |  April 11, 2051 |  January 27, 2055 |  November 16, 2058 |  September 3, 2062 |
| 128 | 130 | 132 | 134 | 136 |
 June 22, 2066 |  April 11, 2070 |  January 27, 2074 |  November 15, 2077 |  September 3, 2081 |
| 138 | 140 | 142 | 144 | 146 |
 June 22, 2085 |  April 10, 2089 |  January 27, 2093 |  November 15, 2096 |  September 4, 2100 |
| 148 | 150 | 152 | 154 | 156 |
 June 22, 2104 |  April 11, 2108 |  January 29, 2112 |  November 16, 2115 |  September 5, 2119 |
| 158 | 160 | 162 | 164 | |
 June 23, 2123 |  November 16, 2134 | |||
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 2036 and 2200 | ||||
|---|---|---|---|---|
 July 23, 2036 (Saros 117) | June 23, 2047 (Saros 118) |  May 22, 2058 (Saros 119) |  April 21, 2069 (Saros 120) |  March 21, 2080 (Saros 121) |
 February 18, 2091 (Saros 122) |  January 19, 2102 (Saros 123) |  December 19, 2112 (Saros 124) |  November 18, 2123 (Saros 125) |  October 17, 2134 (Saros 126) |
 September 16, 2145 (Saros 127) |  August 16, 2156 (Saros 128) |  July 16, 2167 (Saros 129) |  June 16, 2178 (Saros 130) |  May 15, 2189 (Saros 131) |
 April 14, 2200 (Saros 132) | ||||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 1844 and 2200 | ||
|---|---|---|
 November 10, 1844 (Saros 111) | ||
 September 12, 1931 (Saros 114) | ||
 July 13, 2018 (Saros 117) | June 23, 2047 (Saros 118) |  June 1, 2076 (Saros 119) |
 May 14, 2105 (Saros 120) |  April 24, 2134 (Saros 121) |  April 3, 2163 (Saros 122) |
 March 13, 2192 (Saros 123) | ||
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