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Partial eclipse | |||||||||||||
Date | November 8, 2041 | ||||||||||||
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Gamma | 0.9212 | ||||||||||||
Magnitude | 0.1714 | ||||||||||||
Saros cycle | 146 (12 of 72) | ||||||||||||
Partiality | 90 minutes, 21 seconds | ||||||||||||
Penumbral | 268 minutes, 0 seconds | ||||||||||||
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A partial lunar eclipse will occur at the Moon’s ascending node of orbit on Friday, November 8, 2041,[1] with an umbral magnitude of 0.1714. 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 about 2.7 days after perigee (on November 5, 2041, at 10:50 UTC), the Moon's apparent diameter will be larger.[2]
The eclipse will be completely visible over North and South America, western Europe, and west Africa, seen rising over the central Pacific Ocean and setting over much of Africa, eastern Europe, the Middle East, and central 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 | 1.16747 |
Umbral Magnitude | 0.17144 |
Gamma | 0.92123 |
Sun Right Ascension | 14h54m42.6s |
Sun Declination | -16°39'56.0" |
Sun Semi-Diameter | 16'08.5" |
Sun Equatorial Horizontal Parallax | 08.9" |
Moon Right Ascension | 02h53m15.3s |
Moon Declination | +17°30'36.2" |
Moon Semi-Diameter | 16'12.4" |
Moon Equatorial Horizontal Parallax | 0°59'28.8" |
ΔT | 80.2 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.
October 25 Descending node (new moon) |
November 8 Ascending node (full moon) |
---|---|
Annular solar eclipse Solar Saros 134 |
Partial lunar eclipse Lunar Saros 146 |
This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[5]
The penumbral lunar eclipses on January 21, 2038 and July 16, 2038 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 5, 2042 and September 29, 2042 occur in the next lunar year eclipse set.
Lunar eclipse series sets from 2038 to 2042 | ||||||||
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Descending node | Ascending node | |||||||
Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
111 | 2038 Jun 17 |
Penumbral |
1.3082 | 116 | 2038 Dec 11 |
Penumbral |
−1.1448 | |
121 | 2039 Jun 06 |
Partial |
0.5460 | 126 | 2039 Nov 30 |
Partial |
−0.4721 | |
131 | 2040 May 26 |
Total |
−0.1872 | 136 | 2040 Nov 18 |
Total |
0.2361 | |
141 | 2041 May 16 |
Partial |
−0.9746 | 146 | 2041 Nov 08 |
Partial |
0.9212 | |
156 | 2042 Oct 28 |
Penumbral |
− |
This eclipse is the fourth of five Metonic cycle lunar eclipses on the same date, November 8–9, each separated by 19 years.
The Metonic cycle repeats nearly exactly every 19 years and represents a Saros cycle plus one lunar year. Because it occurs on the same calendar date, the Earth's shadow will be in nearly the same location relative to the background stars.
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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 153.
November 3, 2032 | November 14, 2050 |
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