June 2094 lunar eclipse
Total eclipse | |||||||||||||||||
Date | June 28, 2094 | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gamma | 0.0288 | ||||||||||||||||
Magnitude | 1.8249 | ||||||||||||||||
Saros cycle | 131 (38 of 72) | ||||||||||||||||
Totality | 100 minutes, 36 seconds | ||||||||||||||||
Partiality | 235 minutes, 42 seconds | ||||||||||||||||
Penumbral | 326 minutes, 27 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse will occur at the Moon’s descending node of orbit on Monday, June 28, 2094,[1] with an umbral magnitude of 1.8249. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.9 days before perigee (on June 30, 2094, at 7:50 UTC), the Moon's apparent diameter will be larger.[2]
The Moon will pass through the center of the Earth's shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red color at maximum eclipse. With a gamma value of only 0.0288 and an umbral eclipse magnitude of 1.8249, this is the greatest eclipse in Lunar Saros 131 as well as the second largest and darkest lunar eclipse of the 21st century.
Visibility
[edit]The eclipse will be completely visible over eastern Australia, Antarctica, and the central and eastern Pacific Ocean, seen rising over east Asia and western Australia and setting over North and South America.[3]
Eclipse details
[edit]Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
Parameter | Value |
---|---|
Penumbral Magnitude | 2.78793 |
Umbral Magnitude | 1.82485 |
Gamma | 0.02882 |
Sun Right Ascension | 06h31m43.3s |
Sun Declination | +23°13'34.7" |
Sun Semi-Diameter | 15'44.1" |
Sun Equatorial Horizontal Parallax | 08.7" |
Moon Right Ascension | 18h31m43.6s |
Moon Declination | -23°11'51.1" |
Moon Semi-Diameter | 16'20.2" |
Moon Equatorial Horizontal Parallax | 0°59'57.5" |
ΔT | 121.4 s |
Eclipse season
[edit]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.
June 13 Ascending node (new moon) |
June 28 Descending node (full moon) |
July 12 Ascending node (new moon) |
---|---|---|
Partial solar eclipse Solar Saros 119 |
Total lunar eclipse Lunar Saros 131 |
Partial solar eclipse Solar Saros 157 |
Related eclipses
[edit]Eclipses in 2094
[edit]- A partial lunar eclipse on January 1.
- A total solar eclipse on January 16.
- A partial solar eclipse on June 13.
- A total lunar eclipse on June 28.
- A partial solar eclipse on July 12.
- A partial solar eclipse on December 7.
- A total lunar eclipse on December 21.
Metonic
[edit]- Preceded by: Lunar eclipse of September 8, 2090
- Followed by: Lunar eclipse of April 15, 2098
Tzolkinex
[edit]- Preceded by: Lunar eclipse of May 17, 2087
- Followed by: Lunar eclipse of August 9, 2101
Half-Saros
[edit]- Preceded by: Solar eclipse of June 22, 2085
- Followed by: Solar eclipse of July 4, 2103
Tritos
[edit]- Preceded by: Lunar eclipse of July 29, 2083
- Followed by: Lunar eclipse of May 28, 2105
Lunar Saros 131
[edit]- Preceded by: Lunar eclipse of June 17, 2076
- Followed by: Lunar eclipse of July 9, 2112
Inex
[edit]- Preceded by: Lunar eclipse of July 17, 2065
- Followed by: Lunar eclipse of June 9, 2123
Triad
[edit]- Preceded by: Lunar eclipse of August 28, 2007
- Followed by: Lunar eclipse of April 29, 2181
Lunar eclipses of 2092–2096
[edit]This section is empty. You can help by adding to it. (December 2024) |
Saros 131
[edit]Lunar Saros series 131, has 72 lunar eclipses. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
This eclipse series began in AD 1427 with a partial eclipse at the southern edge of the Earth's shadow when the Moon was close to its descending node. Each successive Saros cycle, the Moon's orbital path is shifted northward with respect to the Earth's shadow, with the first total eclipse occurring in 1950. For the following 252 years, total eclipses occur, with the central eclipse being predicted to occur in 2078. The first partial eclipse after this is predicted to occur in the year 2220, and the final partial eclipse of the series will occur in 2707. The total lifetime of the lunar Saros series 131 is 1280 years. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Because of the ⅓ fraction of days in a Saros cycle, the visibility of each eclipse will differ for an observer at a given fixed locale. For the lunar Saros series 131, the first total eclipse of 1950 had its best visibility for viewers in Eastern Europe and the Middle East because mid-eclipse was at 20:44 UT. The following eclipse in the series occurred approximately 8 hours later in the day with mid-eclipse at 4:47 UT, and was best seen from North America and South America. The third total eclipse occurred approximately 8 hours later in the day than the second eclipse with mid-eclipse at 12:43 UT, and had its best visibility for viewers in the Western Pacific, East Asia, Australia and New Zealand. This cycle of visibility repeats from the initiation to termination of the series, with minor variations. Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Lunar Saros series 131, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 57 umbral lunar eclipses (42 partial lunar eclipses and 15 total lunar eclipses). Solar Saros 138 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Greatest | First | |||
---|---|---|---|---|
The greatest eclipse of the series will occur on 2094 Jun 28, lasting 102 minutes.[5] |
Penumbral | Partial | Total | Central |
1427 May 10 | 1553 July 25 | 1950 Apr 2 | 2022 May 16 | |
Last | ||||
Central | Total | Partial | Penumbral | |
2148 Jul 31 | 2202 Sep 3 | 2563 Apr 9 | 2707 Jul 7 |
1914 Mar 12 | 1932 Mar 22 | 1950 Apr 2 | |||
1968 Apr 13 | 1986 Apr 24 | 2004 May 4 | |||
2022 May 16 | 2040 May 26 | 2058 Jun 6 | |||
2076 Jun 17 | 2094 Jun 28 | ||||
Half-Saros cycle
[edit]A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two annular solar eclipses of Solar Saros 138.
June 22, 2085 | July 4, 2103 |
---|---|
See also
[edit]Notes
[edit]- ^ "June 27–28, 2094 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 14 December 2024.
- ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 December 2024.
- ^ "Total Lunar Eclipse of 2094 Jun 28" (PDF). NASA. Retrieved 14 December 2024.
- ^ "Total Lunar Eclipse of 2094 Jun 28". EclipseWise.com. Retrieved 14 December 2024.
- ^ Listing of Eclipses of cycle 131
- ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
External links
[edit]- 2094 Jun 28 chart Eclipse Predictions by Fred Espenak, NASA/GSFC