October 2050 lunar eclipse
Total eclipse | |||||||||||||||||
Date | October 30, 2050 | ||||||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gamma | 0.4435 | ||||||||||||||||
Magnitude | 1.0549 | ||||||||||||||||
Saros cycle | 127 (44 of 72) | ||||||||||||||||
Totality | 34 minutes, 30 seconds | ||||||||||||||||
Partiality | 192 minutes, 51 seconds | ||||||||||||||||
Penumbral | 313 minutes, 8 seconds | ||||||||||||||||
| |||||||||||||||||
A total lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, October 30, 2050,[1] with an umbral magnitude of 1.0549. 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 after perigee (on October 28, 2050, at 5:10 UTC), the Moon's apparent diameter will be larger.[2]
This lunar eclipse is the second of a tetrad, with four total lunar eclipses in series, the others being on May 6, 2050; April 26, 2051; and October 19, 2051.
Visibility
The eclipse will be completely visible over North and South America, west Africa, and western Europe, seen rising over the central and eastern Pacific Ocean and setting over central and east Africa, eastern Europe, and west, central, and south Asia.[3]
Eclipse details
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 | 2.03564 |
Umbral Magnitude | 1.05490 |
Gamma | 0.44351 |
Sun Right Ascension | 14h18m15.4s |
Sun Declination | -13°48'46.9" |
Sun Semi-Diameter | 16'06.2" |
Sun Equatorial Horizontal Parallax | 08.9" |
Moon Right Ascension | 02h17m49.7s |
Moon Declination | +14°14'46.2" |
Moon Semi-Diameter | 16'25.2" |
Moon Equatorial Horizontal Parallax | 1°00'15.6" |
ΔT | 85.6 s |
Eclipse season
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 30 Descending node (full moon) |
November 14 Ascending node (new moon) |
---|---|
Total lunar eclipse Lunar Saros 127 |
Partial solar eclipse Solar Saros 153 |
Related eclipses
Eclipses in 2050
- A total lunar eclipse on May 6.
- A hybrid solar eclipse on May 20.
- A total lunar eclipse on October 30.
- A partial solar eclipse on November 14.
Metonic
- Preceded by: Lunar eclipse of January 12, 2047
- Followed by: Lunar eclipse of August 18, 2054
Tzolkinex
- Preceded by: Lunar eclipse of September 19, 2043
- Followed by: Lunar eclipse of December 11, 2057
Half-Saros
- Preceded by: Solar eclipse of October 25, 2041
- Followed by: Solar eclipse of November 5, 2059
Tritos
- Preceded by: Lunar eclipse of November 30, 2039
- Followed by: Lunar eclipse of September 29, 2061
Lunar Saros 127
- Preceded by: Lunar eclipse of October 18, 2032
- Followed by: Lunar eclipse of November 9, 2068
Inex
- Preceded by: Lunar eclipse of November 19, 2021
- Followed by: Lunar eclipse of October 10, 2079
Triad
- Preceded by: Lunar eclipse of December 30, 1963
- Followed by: Lunar eclipse of August 30, 2137
Lunar eclipses of 2049–2052
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Date Viewing |
Type Chart |
Saros | Date Viewing |
Type Chart | |
112 | 2049 May 17 |
Penumbral |
117 | 2049 Nov 09 |
Penumbral | |
122 | 2050 May 06 |
Total |
127 | 2050 Oct 30 |
Total | |
132 | 2051 Apr 26 |
Total |
137 | 2051 Oct 19 |
Total | |
142 | 2052 Apr 14 |
Penumbral |
147 | 2052 Oct 08 |
Partial | |
Last set | 2049 Jun 15 | Last set | 2048 Dec 20 | |||
Next set | 2053 Mar 04 | Next set | 2053 Aug 29 |
Saros 127
Lunar saros series 127, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 54 umbral lunar eclipses (38 partial lunar eclipses and 16 total lunar eclipses). Solar Saros 134 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 occurred on 1888 Jul 23, lasting 102 minutes. |
Penumbral | Partial | Total | Central |
1275 Jul 09 | 1473 Nov 04 | 1798 May 29 | 1834 Jun 21 | |
Last | ||||
Central | Total | Partial | Penumbral | |
1960 Sep 05 |
2068 Nov 09 | 2429 Jun 17 | 2555 Sep 02 |
1906 Aug 04 | 1924 Aug 14 | 1942 Aug 26 | |||
1960 Sep 05 | 1978 Sep 16 | 1996 Sep 27 | |||
2014 Oct 08 | 2032 Oct 18 | 2050 Oct 30 | |||
2068 Nov 09 | |||||
Half-Saros cycle
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two annular solar eclipses of Solar Saros 134.
October 25, 2041 | November 5, 2059 |
---|---|
See also
Notes
- ^ "October 29–30, 2050 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 12 December 2024.
- ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 12 December 2024.
- ^ "Total Lunar Eclipse of 2050 Oct 30" (PDF). NASA. Retrieved 12 December 2024.
- ^ "Total Lunar Eclipse of 2050 Oct 30". EclipseWise.com. Retrieved 12 December 2024.
- ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
External links
- 2050 Oct 30 chart: Eclipse Predictions by Fred Espenak, NASA/GSFC