Solar eclipse of June 11, 2048
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, June 11, 2048,[1] with a magnitude of 0.9441. 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 15.5 hours after apogee (on June 10, 2048, at 21:20 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts of Colorado, Kansas, the Oklahoma panhandle, Nebraska, northwestern Missouri, Iowa, southeastern Minnesota, northwestern Illinois, Wisconsin, and Michigan in the United States, eastern Canada, southern Greenland, Iceland, the Faroe Islands, Norway, Sweden, Estonia, Latvia, Lithuania, Belarus, western Russia, eastern Ukraine, southwestern Kazakhstan, southern Uzbekistan, Turkmenistan, southwestern Tajikistan, Afghanistan, and northern Pakistan. A partial solar eclipse will also be visible for parts of North America, Central America, the Caribbean, Europe, North Africa, the Middle East, and Central Asia.
Images
File:SE2048Jun11A.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 | 2048 June 11 at 10:09:44.8 UTC |
| First Umbral External Contact | 2048 June 11 at 11:25:33.1 UTC |
| First Central Line | 2048 June 11 at 11:28:35.8 UTC |
| First Umbral Internal Contact | 2048 June 11 at 11:31:41.1 UTC |
| Ecliptic Conjunction | 2048 June 11 at 12:51:11.2 UTC |
| Equatorial Conjunction | 2048 June 11 at 12:56:14.7 UTC |
| Greatest Duration | 2048 June 11 at 12:57:27.0 UTC |
| Greatest Eclipse | 2048 June 11 at 12:58:52.8 UTC |
| Last Umbral Internal Contact | 2048 June 11 at 14:26:06.6 UTC |
| Last Central Line | 2048 June 11 at 14:29:11.5 UTC |
| Last Umbral External Contact | 2048 June 11 at 14:32:13.6 UTC |
| Last Penumbral External Contact | 2048 June 11 at 15:48:00.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.94415 |
| Eclipse Obscuration | 0.89141 |
| Gamma | 0.64685 |
| Sun Right Ascension | 05h22m03.9s |
| Sun Declination | +23°08'47.0" |
| Sun Semi-Diameter | 15'45.1" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 05h22m09.1s |
| Moon Declination | +23°43'34.6" |
| Moon Semi-Diameter | 14'42.3" |
| Moon Equatorial Horizontal Parallax | 0°53'58.0" |
| ΔT | 83.2 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.
| June 11 Descending node (new moon) |
June 26 Ascending node (full moon) |
|---|---|
| File:SE2048Jun11A.png | File:Lunar eclipse chart close-2048Jun26.png |
| Annular solar eclipse Solar Saros 128 |
Partial lunar eclipse Lunar Saros 140 |
Related eclipses
Eclipses in 2048
- A total lunar eclipse on January 1.
- An annular solar eclipse on June 11.
- A partial lunar eclipse on June 26.
- A total solar eclipse on December 5.
- A penumbral lunar eclipse on December 20.
Metonic
- Preceded by: Solar eclipse of August 23, 2044
- Followed by: Solar eclipse of March 30, 2052
Tzolkinex
- Preceded by: Solar eclipse of April 30, 2041
- Followed by: Solar eclipse of July 24, 2055
Half-Saros
- Preceded by: Lunar eclipse of June 6, 2039
- Followed by: Lunar eclipse of June 17, 2057
Tritos
- Preceded by: Solar eclipse of July 13, 2037
- Followed by: Solar eclipse of May 11, 2059
Solar Saros 128
- Preceded by: Solar eclipse of June 1, 2030
- Followed by: Solar eclipse of June 22, 2066
Inex
- Preceded by: Solar eclipse of July 2, 2019
- Followed by: Solar eclipse of May 22, 2077
Triad
- Preceded by: Solar eclipse of August 11, 1961
- Followed by: Solar eclipse of April 13, 2135
Solar eclipses of 2047–2050
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]
The partial solar eclipses on January 26, 2047 and July 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 File:SE2047Jun23P.png Partial |
1.3766 | 123 | December 16, 2047 File:SE2047Dec16P.png Partial |
−1.0661 | |
| 128 | June 11, 2048 File:SE2048Jun11A.png Annular |
0.6468 | 133 | December 5, 2048 File:SE2048Dec05T.png Total |
−0.3973 | |
| 138 | May 31, 2049 File:SE2049May31A.png Annular |
−0.1187 | 143 | November 25, 2049 File:SE2049Nov25H.png Hybrid |
0.2943 | |
| 148 | May 20, 2050 File:SE2050May20H.png Hybrid |
−0.8688 | 153 | November 14, 2050 File:SE2050Nov14P.png Partial |
1.0447 | |
Saros 128
This eclipse is a part of Saros series 128, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471; hybrid eclipses from June 28, 1489 through July 31, 1543; and annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. 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 27 at 1 minutes, 45 seconds on June 7, 1453, and the longest duration of annularity was produced by member 48 at 8 minutes, 35 seconds on February 1, 1832. All eclipses in this series occur at the Moon’s descending node of orbit.[5]
| Series members 47–68 occur between 1801 and 2200: | ||
|---|---|---|
| 47 | 48 | 49 |
| File:SE1814Jan21A.gif January 21, 1814 |
File:SE1832Feb01A.gif February 1, 1832 |
File:SE1850Feb12A.gif February 12, 1850 |
| 50 | 51 | 52 |
| File:SE1868Feb23A.gif February 23, 1868 |
File:SE1886Mar05A.gif March 5, 1886 |
File:SE1904Mar17A.png March 17, 1904 |
| 53 | 54 | 55 |
| File:SE1922Mar28A.png March 28, 1922 |
File:SE1940Apr07A.png April 7, 1940 |
File:SE1958Apr19A.png April 19, 1958 |
| 56 | 57 | 58 |
| File:SE1976Apr29A.png April 29, 1976 |
File:SE1994May10A.png May 10, 1994 |
File:SE2012May20A.png May 20, 2012 |
| 59 | 60 | 61 |
| File:SE2030Jun01A.png June 1, 2030 |
File:SE2048Jun11A.png June 11, 2048 |
File:SE2066Jun22A.png June 22, 2066 |
| 62 | 63 | 64 |
| File:SE2084Jul03A.png July 3, 2084 |
File:SE2102Jul15A.png July 15, 2102 |
File:SE2120Jul25A.png July 25, 2120 |
| 65 | 66 | 67 |
| File:Saros128 65van73 SE2138Aug05P.jpg August 5, 2138 |
File:Saros128 66van73 SE2156Aug16P.jpg August 16, 2156 |
File:Saros128 67van73 SE2174Aug27P.jpg August 27, 2174 |
| 68 | ||
| File:Saros128 68van73 SE2192Sep06P.jpg September 6, 2192 | ||
Metonic series
Template:Solar Metonic series 2029–2116
Tritos series
Template:Solar Tritos series 2004 October 14
Inex series
Template:Solar Inex series 2019 July 2
References
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External links
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