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Astronomical event From Wikipedia, the free encyclopedia
A partial lunar eclipse will occur at the Moon’s ascending node of orbit on Friday, June 26, 2048,[1] with an umbral magnitude of 0.6404. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. 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. Occurring only about 21 hours after perigee (on June 25, 2048, at 5:50 UTC), the Moon's apparent diameter will be larger.[2]
Partial eclipse | |||||||||||||
![]() The Moon's hourly motion shown right to left | |||||||||||||
Date | June 26, 2048 | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gamma | 0.6796 | ||||||||||||
Magnitude | 0.6404 | ||||||||||||
Saros cycle | 140 (26 of 77) | ||||||||||||
Partiality | 159 minutes, 10 seconds | ||||||||||||
Penumbral | 285 minutes, 44 seconds | ||||||||||||
| |||||||||||||
The eclipse will be completely visible over South America, west and southern Africa, and Antarctica, seen rising over much of North America and setting over Europe, east Africa, and west, central, and south Asia.[3]
![]() ![]() |
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 | 1.58412 |
Umbral Magnitude | 0.64039 |
Gamma | 0.67965 |
Sun Right Ascension | 06h22m31.9s |
Sun Declination | +23°19'54.0" |
Sun Semi-Diameter | 15'44.1" |
Sun Equatorial Horizontal Parallax | 08.7" |
Moon Right Ascension | 18h22m07.4s |
Moon Declination | -22°38'42.2" |
Moon Semi-Diameter | 16'40.4" |
Moon Equatorial Horizontal Parallax | 1°01'11.5" |
ΔT | 84.1 s |
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) |
---|---|
![]() | ![]() |
Annular solar eclipse Solar Saros 128 | Partial lunar eclipse Lunar Saros 140 |
Descending node | Ascending node | |||||
---|---|---|---|---|---|---|
Saros | Date Viewing |
Type Chart |
Saros | Date Viewing |
Type Chart | |
115 | 2046 Jan 22![]() |
Partial![]() |
120 | 2046 Jul 18![]() |
Partial![]() | |
125 | 2047 Jan 12![]() |
Total![]() |
130 | 2047 Jul 07![]() |
Total![]() | |
135 | 2048 Jan 01![]() |
Total![]() |
140 | 2048 Jun 26![]() |
Partial![]() | |
145 | 2048 Dec 20![]() |
Penumbral![]() |
150 | 2049 Jun 15![]() |
Penumbral![]() | |
Last set | 2045 Aug 27 | Last set | 2045 Mar 03 | |||
Next set | 2049 Nov 09 | Next set | 2049 May 17 |
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 147.
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