Solar eclipse of October 25, 2041
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's descending node of orbit between Thursday, October 24 and Friday, October 25, 2041,[1] with a magnitude of 0.9467. 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. Occurring about 4.3 days after apogee (on October 20, 2041, at 17:10 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts of Mongolia, northeastern China, North Korea, Japan, the Marshall Islands, and Kiribati. A partial solar eclipse will be visible for parts of East Asia, Southeast Asia, northeastern Australia, Oceania, and Hawaii.
Images
File:SE2041Oct25A.gif
Animated path
Eclipse details
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.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2041 October 24 at 22:41:02.8 UTC |
| First Umbral External Contact | 2041 October 24 at 23:48:18.5 UTC |
| First Central Line | 2041 October 24 at 23:50:49.8 UTC |
| First Umbral Internal Contact | 2041 October 24 at 23:53:21.7 UTC |
| Equatorial Conjunction | 2041 October 25 at 01:13:01.1 UTC |
| First Penumbral Internal Contact | 2041 October 25 at 01:22:11.2 UTC |
| Ecliptic Conjunction | 2041 October 25 at 01:31:31.7 UTC |
| Greatest Eclipse | 2041 October 25 at 01:36:21.7 UTC |
| Last Penumbral Internal Contact | 2041 October 25 at 01:51:07.0 UTC |
| Greatest Duration | 2041 October 25 at 01:51:55.5 UTC |
| Last Umbral Internal Contact | 2041 October 25 at 03:19:38.3 UTC |
| Last Central Line | 2041 October 25 at 03:22:07.7 UTC |
| Last Umbral External Contact | 2041 October 25 at 03:24:36.3 UTC |
| Last Penumbral External Contact | 2041 October 25 at 04:31:44.8 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.94666 |
| Eclipse Obscuration | 0.89617 |
| Gamma | 0.41332 |
| Sun Right Ascension | 13h59m22.0s |
| Sun Declination | -12°10'20.1" |
| Sun Semi-Diameter | 16'04.9" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 14h00m02.5s |
| Moon Declination | -11°49'54.3" |
| Moon Semi-Diameter | 15'00.8" |
| Moon Equatorial Horizontal Parallax | 0°55'06.0" |
| ΔT | 79.5 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| October 25 Descending node (new moon) |
November 8 Ascending node (full moon) |
|---|---|
| File:SE2041Oct25A.png | File:Lunar eclipse chart close-2041Nov08.png |
| Annular solar eclipse Solar Saros 134 |
Partial lunar eclipse Lunar Saros 146 |
Related eclipses
Eclipses in 2041
- A total solar eclipse on April 30.
- A partial lunar eclipse on May 16.
- An annular solar eclipse on October 25.
- A partial lunar eclipse on November 8.
Metonic
- Preceded by: Solar eclipse of January 5, 2038
- Followed by: Solar eclipse of August 12, 2045
Tzolkinex
- Preceded by: Solar eclipse of September 12, 2034
- Followed by: Solar eclipse of December 5, 2048
Half-Saros
- Preceded by: Lunar eclipse of October 18, 2032
- Followed by: Lunar eclipse of October 30, 2050
Tritos
- Preceded by: Solar eclipse of November 25, 2030
- Followed by: Solar eclipse of September 22, 2052
Solar Saros 134
- Preceded by: Solar eclipse of October 14, 2023
- Followed by: Solar eclipse of November 5, 2059
Inex
- Preceded by: Solar eclipse of November 13, 2012
- Followed by: Solar eclipse of October 4, 2070
Triad
- Preceded by: Solar eclipse of December 25, 1954
- Followed by: Solar eclipse of August 25, 2128
Solar eclipses of 2040–2043
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.[4]
| Solar eclipse series sets from 2040 to 2043 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | May 11, 2040 File:SE2040May11P.png Partial |
−1.2529 | 124 | November 4, 2040 File:SE2040Nov04P.png Partial |
1.0993 | |
| 129 | April 30, 2041 File:SE2041Apr30T.png Total |
−0.4492 | 134 | October 25, 2041 File:SE2041Oct25A.png Annular |
0.4133 | |
| 139 | April 20, 2042 File:SE2042Apr20T.png Total |
0.2956 | 144 | October 14, 2042 File:SE2042Oct14A.png Annular |
−0.303 | |
| 149 | April 9, 2043 File:SE2043Apr09T.png Total (non-central) |
1.0031 | 154 | October 3, 2043 File:SE2043Oct03A.png Annular (non-central) |
1.0102 | |
Saros 134
This eclipse is a part of Saros series 134, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554; hybrid eclipses from January 3, 1573 through June 27, 1843; and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 72 as a partial eclipse on August 6, 2510. 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 11 at 1 minutes, 30 seconds on October 9, 1428, and the longest duration of annularity will be produced by member 52 at 10 minutes, 55 seconds on January 10, 2168. All eclipses in this series occur at the Moon’s descending node of orbit.[5]
| Series members 32–53 occur between 1801 and 2200: | ||
|---|---|---|
| 32 | 33 | 34 |
| File:SE1807Jun06H.png June 6, 1807 |
File:SE1825Jun16H.png June 16, 1825 |
File:SE1843Jun27H.png June 27, 1843 |
| 35 | 36 | 37 |
| File:SE1861Jul08A.png July 8, 1861 |
File:SE1879Jul19A.png July 19, 1879 |
File:SE1897Jul29A.png July 29, 1897 |
| 38 | 39 | 40 |
| File:SE1915Aug10A.png August 10, 1915 |
File:SE1933Aug21A.png August 21, 1933 |
File:SE1951Sep01A.png September 1, 1951 |
| 41 | 42 | 43 |
| File:SE1969Sep11A.png September 11, 1969 |
File:SE1987Sep23A.png September 23, 1987 |
File:SE2005Oct03A.png October 3, 2005 |
| 44 | 45 | 46 |
| File:SE2023Oct14A.png October 14, 2023 |
File:SE2041Oct25A.png October 25, 2041 |
File:SE2059Nov05A.png November 5, 2059 |
| 47 | 48 | 49 |
| File:SE2077Nov15A.png November 15, 2077 |
File:SE2095Nov27A.png November 27, 2095 |
File:SE2113Dec08A.png December 8, 2113 |
| 50 | 51 | 52 |
| File:SE2131Dec19A.png December 19, 2131 |
File:SE2149Dec30A.png December 30, 2149 |
File:SE2168Jan10A.png January 10, 2168 |
| 53 | ||
| File:SE2186Jan20A.png January 20, 2186 | ||
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 descending node.
Tritos series
Template:Solar Tritos series 2009 January 26
Inex series
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 | ||
|---|---|---|
| File:SE1810Apr04A.gif April 4, 1810 (Saros 126) |
File:SE1839Mar15T.gif March 15, 1839 (Saros 127) |
File:SE1868Feb23A.gif February 23, 1868 (Saros 128) |
| File:SE1897Feb01A.gif February 1, 1897 (Saros 129) |
File:SE1926Jan14T.png January 14, 1926 (Saros 130) |
File:SE1954Dec25A.png December 25, 1954 (Saros 131) |
| File:SE1983Dec04A.png December 4, 1983 (Saros 132) |
File:SE2012Nov13T.png November 13, 2012 (Saros 133) |
File:SE2041Oct25A.png October 25, 2041 (Saros 134) |
| File:SE2070Oct04A.png October 4, 2070 (Saros 135) |
File:SE2099Sep14T.png September 14, 2099 (Saros 136) |
File:SE2128Aug25A.png August 25, 2128 (Saros 137) |
| File:SE2157Aug05A.png August 5, 2157 (Saros 138) |
File:SE2186Jul16T.png July 16, 2186 (Saros 139) |
|
References
<templatestyles src="Reflist/styles.css" />
Script error: No such module "Check for unknown parameters".
External links
Script error: No such module "Navbox".