January 2000 lunar eclipse

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, January 21, 2000,[1] with an umbral magnitude of 1.3246. 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 1.5 days after perigee (on January 19, 2000, at 17:50 UTC), the Moon's apparent diameter was larger.[2]

January 2000 lunar eclipse
Total eclipse
Partial from Buenos Aires, 3:20 UTC
DateJanuary 21, 2000
Gamma−0.2957
Magnitude1.3246
Saros cycle124 (48 of 74)
Totality76 minutes, 59 seconds
Partiality203 minutes, 19 seconds
Penumbral318 minutes, 12 seconds
Contacts (UTC)
P102:04:26
U103:01:50
U204:05:01
Greatest04:43:31
U305:22:00
U406:25:09
P407:22:38

Visibility

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The eclipse was completely visible over most of North America, South America, and western Europe, seen rising over the Pacific Ocean and setting over Africa, Europe, and west Asia.[3]

   
Hourly motion shown right to left

Eclipse details

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Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

January 21, 2000 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.30601
Umbral Magnitude 1.32459
Gamma −0.29571
Sun Right Ascension 20h10m32.9s
Sun Declination -20°03'20.2"
Sun Semi-Diameter 16'15.2"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 08h10m24.0s
Moon Declination +19°45'29.3"
Moon Semi-Diameter 16'33.7"
Moon Equatorial Horizontal Parallax 1°00'46.8"
ΔT 63.8 s

Eclipse season

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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.

Eclipse season of January–February 2000
January 21
Ascending node (full moon)
February 5
Descending node (new moon)
   
Total lunar eclipse
Lunar Saros 124
Partial solar eclipse
Solar Saros 150
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Eclipses in 2000

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 124

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Inex

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Triad

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Lunar eclipses of 1998–2002

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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

Tritos series

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The tritos series repeats 31 days short of 11 years at alternating nodes. Sequential events have incremental Saros cycle indices.

This series produces 20 total eclipses between April 24, 1967 and August 11, 2185, only being partial on November 19, 2021.

Tritos eclipse series (subset 1901–2087)
Descending node   Ascending node
Saros Date
Viewing
Type
chart
Saros Date
Viewing
Type
chart
115 1901 Oct 27
 
Partial
 
116 1912 Sep 26
 
Partial
 
117 1923 Aug 26
 
Partial
 
118 1934 Jul 26
 
Partial
 
119 1945 Jun 25
 
Partial
 
120 1956 May 24
 
Partial
 
121 1967 Apr 24
 
Total
 
122 1978 Mar 24
 
Total
 
123 1989 Feb 20
 
Total
 
124 2000 Jan 21
 
Total
 
125 2010 Dec 21
 
Total
 
126 2021 Nov 19
 
Partial
 
127 2032 Oct 18
 
Total
 
128 2043 Sep 19
 
Total
 
129 2054 Aug 18
 
Total
 
130 2065 Jul 17
 
Total
 
131 2076 Jun 17
 
Total
 
132 2087 May 17
 
Total
 
133 2098 Apr 15
 
Total
 

Half-Saros cycle

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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).[5] This lunar eclipse is related to two annular solar eclipses of Solar Saros 131.

January 15, 1991 January 26, 2009
   

See also

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References

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  1. ^ "January 20–21, 2000 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 12 November 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 12 November 2024.
  3. ^ "Total Lunar Eclipse of 2000 Jan 21" (PDF). NASA. Retrieved 12 November 2024.
  4. ^ "Total Lunar Eclipse of 2000 Jan 21". EclipseWise.com. Retrieved 12 November 2024.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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