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February 1990 lunar eclipse

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February 1990 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateFebruary 9, 1990
Gamma−0.4148
Magnitude1.0750
Saros cycle133 (25 of 71)
Totality42 minutes, 19 seconds
Partiality204 minutes, 17 seconds
Penumbral339 minutes, 35 seconds
Contacts (UTC)
P116:21:21
U117:28:55
U218:49:55
Greatest19:11:06
U319:32:13
U420:53:12
P422:00:56

A total lunar eclipse occurred at the Moon’s descending node of orbit on Friday, February 9, 1990,[1] with an umbral magnitude of 1.0750. 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. The Moon's apparent diameter will be near the average diameter because it will occur 7.7 days after perigee (on February 2, 1990, at 2:40 UTC) and 6.75 days before apogee (on February 16, 1990, at 13:05 UTC).[2]

Visibility

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The eclipse was completely visible over east Africa, eastern Europe, and Asia, seen rising over northeastern North America, eastern South America, western Europe and west and central Africa and setting over Australia, northwestern North America, and the western and central Pacific Ocean.[3]

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]

February 9, 1990 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.11912
Umbral Magnitude 1.07499
Gamma −0.41481
Sun Right Ascension 21h32m41.8s
Sun Declination -14°34'08.6"
Sun Semi-Diameter 16'12.6"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 09h32m01.7s
Moon Declination +14°12'35.9"
Moon Semi-Diameter 15'31.5"
Moon Equatorial Horizontal Parallax 0°56'58.5"
ΔT 56.9 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 1990
January 26
Ascending node (new moon)
February 9
Descending node (full moon)
Annular solar eclipse
Solar Saros 121
Total lunar eclipse
Lunar Saros 133
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Eclipses in 1990

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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 133

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Inex

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Triad

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Lunar eclipses of 1988–1991

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Lunar eclipse series sets from 1988–1991
Descending node   Ascending node
Saros Date
viewing
Type
chart
Gamma Saros Date
viewing
Type
chart
Gamma
113 1988 Mar 03
Penumbral
0.98855 118 1988 Aug 27
Partial
−0.86816
123 1989 Feb 20
Total
0.29347 128 1989 Aug 17
Total
−0.14905
133 1990 Feb 09
Total
−0.41481 138 1990 Aug 06
Partial
0.63741
143 1991 Jan 30
Penumbral
−1.07522 148 1991 Jul 26
Penumbral
1.43698
Last set 1987 Apr 14 Last set 1987 Oct 07
Next set 1991 Dec 21 Next set 1991 Jun 27

Saros 133

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This lunar eclipse is part of series 133 of the Saros cycle, which repeats every 18 years and 11 days. Series 133 runs from the year 1557 until 2819. The previous eclipse of this series occurred on January 30, 1972 and the next will occur on February 21, 2008.

It is the 5th of 21 total lunar eclipses in series 133. The first was on December 28, 1917. The last (21st) will be on August 3, 2278. The longest two occurrences of this series (14th and 15th) will last for a total of 1 hour and 42 minutes on May 18, 2152 and May 30, 2170. Solar saros 140 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.

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 140.

February 4, 1981 February 16, 1999

See also

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Notes

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  1. ^ "February 9–10, 1990 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 7 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 7 January 2025.
  3. ^ "Total Lunar Eclipse of 1990 Feb 09" (PDF). NASA. Retrieved 7 January 2025.
  4. ^ "Total Lunar Eclipse of 1990 Feb 09". EclipseWise.com. Retrieved 7 January 2025.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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