February 1990 lunar eclipse

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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See also: Eclipse cycle

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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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 lunar eclipses on June 27, 1991 (penumbral) and December 21, 1991 (partial) occur in the next lunar year eclipse set.

Lunar eclipse series sets from 1988 to 1991
Descending node   Ascending node
Saros Date
Viewing 		Type
Chart 		Gamma Saros Date
Viewing 		Type
Chart 		Gamma
113 1988 Mar 03
 Penumbral
 0.9886 118 1988 Aug 27
 Partial
 −0.8682
123 1989 Feb 20
 Total
0.2935 128 1989 Aug 17
 Total
 −0.1491
133 1990 Feb 09
 Total
 −0.4148 138 1990 Aug 06
 Partial
 0.6374
143 1991 Jan 30
 Penumbral
 −1.0752 148 1991 Jul 26
 Penumbral
 1.4370

Saros 133

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This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 71 events. The series started with a penumbral lunar eclipse on May 13, 1557. It contains partial eclipses from August 7, 1683 through December 17, 1899; total eclipses from December 28, 1917 through August 3, 2278; and a second set of partial eclipses from August 14, 2296 through March 11, 2639. The series ends at member 71 as a penumbral eclipse on June 29, 2819.

The longest duration of totality will be produced by member 35 at 101 minutes, 41 seconds on May 30, 2170. All eclipses in this series occur at the Moon’s descending node of orbit.[6]

Greatest First
The greatest eclipse of the series will occur on 2170 May 30, lasting 101 minutes, 41 seconds.[7] Penumbral Partial Total Central
1557 May 13
 1683 Aug 07
 1917 Dec 28
 2098 Apr 15
Last
Central Total Partial Penumbral
2224 Jul 01
 2278 Aug 03
 2639 Mar 11
 2819 Jun 29

Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
1804 Jul 22
(Saros 116) 		1815 Jun 21
(Saros 117) 		1826 May 21
(Saros 118) 		1837 Apr 20
(Saros 119) 		1848 Mar 19
(Saros 120)
1859 Feb 17
(Saros 121) 		1870 Jan 17
(Saros 122) 		1880 Dec 16
(Saros 123) 		1891 Nov 16
(Saros 124) 		1902 Oct 17
(Saros 125)
1913 Sep 15
(Saros 126) 		1924 Aug 14
(Saros 127) 		1935 Jul 16
(Saros 128) 		1946 Jun 14
(Saros 129) 		1957 May 13
(Saros 130)
1968 Apr 13
(Saros 131) 		1979 Mar 13
(Saros 132) 		1990 Feb 09
(Saros 133) 		2001 Jan 09
(Saros 134) 		2011 Dec 10
(Saros 135)
2022 Nov 08
(Saros 136) 		2033 Oct 08
(Saros 137) 		2044 Sep 07
(Saros 138) 		2055 Aug 07
(Saros 139) 		2066 Jul 07
(Saros 140)
2077 Jun 06
(Saros 141) 		2088 May 05
(Saros 142) 		2099 Apr 05
(Saros 143) 		2110 Mar 06
(Saros 144) 		2121 Feb 02
(Saros 145)
2132 Jan 02
(Saros 146) 		2142 Dec 03
(Saros 147) 		2153 Nov 01
(Saros 148) 		2164 Sep 30
(Saros 149) 		2175 Aug 31
(Saros 150)
2186 Jul 31
(Saros 151) 		2197 Jun 29
(Saros 152)

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).[8] 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. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  6. ^ "NASA - Catalog of Lunar Eclipses of Saros 133". eclipse.gsfc.nasa.gov.
  7. ^ Listing of Eclipses of series 133
  8. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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