Total eclipse | |||||||||||||||||
Date | January 9, 2001 | ||||||||||||||||
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Gamma | 0.3720 | ||||||||||||||||
Magnitude | 1.1902 | ||||||||||||||||
Saros cycle | 134 (26 of 73) | ||||||||||||||||
Totality | 61 minutes, 2 seconds | ||||||||||||||||
Partiality | 196 minutes, 19 seconds | ||||||||||||||||
Penumbral | 311 minutes, 2 seconds | ||||||||||||||||
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A total lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, January 9, 2001,[1] with an umbral magnitude of 1.1902. 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 only about 8 hours before perigee (on January 10, 2001, at 4:00 UTC), the Moon's apparent diameter was larger.[2]
The eclipse was completely visible over Africa, Europe, and Asia, seen rising over eastern and northern North America and eastern South America and setting over Australia and the western Pacific Ocean.[3]
Hourly motion shown right to left | |
The Moon passed straight through the center of the Earth's shadow at the descending node in Gemini. |
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 | 2.16314 |
Umbral Magnitude | 1.19022 |
Gamma | 0.37198 |
Sun Right Ascension | 19h25m03.5s |
Sun Declination | -21°59'58.3" |
Sun Semi-Diameter | 16'15.9" |
Sun Equatorial Horizontal Parallax | 08.9" |
Moon Right Ascension | 07h25m08.0s |
Moon Declination | +22°22'46.0" |
Moon Semi-Diameter | 16'43.0" |
Moon Equatorial Horizontal Parallax | 1°01'21.1" |
ΔT | 64.1 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.
December 25 Descending node (new moon) |
January 9 Ascending node (full moon) |
---|---|
Partial solar eclipse Solar Saros 122 |
Total lunar eclipse Lunar Saros 134 |
Lunar eclipse series sets from 1998–2002 | ||||||||
---|---|---|---|---|---|---|---|---|
Descending node | Ascending node | |||||||
Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
109 | 1998 Aug 08 |
penumbral |
1.4876 | 114 | 1999 Jan 31 |
penumbral |
−1.0190 | |
119 | 1999 Jul 28 |
partial |
0.7863 | 124 |
2000 Jan 21 |
total |
−0.2957 | |
129 | 2000 Jul 16 |
total |
0.0302 | 134 |
2001 Jan 09 |
total |
0.3720 | |
139 | 2001 Jul 05 |
partial |
−0.7287 | 144 | 2001 Dec 30 |
penumbral |
1.0732 | |
149 | 2002 Jun 24 |
penumbral |
−1.4440 | |||||
Last set | 1998 Sep 06 | Last set | 1998 Mar 13 | |||||
Next set | 2002 May 26 | Next set | 2002 Nov 20 |
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 141.
January 4, 1992 | January 15, 2010 |
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