Jump to content

May 2069 lunar eclipse

From Wikipedia, the free encyclopedia
May 2069 lunar eclipse
Total eclipse
The Moon's hourly motion shown right to left
DateMay 6, 2069
Gamma0.2717
Magnitude1.3242
Saros cycle132 (33 of 71)
Totality84 minutes, 16 seconds
Partiality226 minutes, 11 seconds
Penumbral368 minutes, 7 seconds
Contacts (UTC)
P16:03:38
U17:14:38
U28:25:35
Greatest9:07:43
U39:49:42
U411:00:49
P412:11:45
October 2069 →

A total lunar eclipse will occur at the Moon’s ascending node of orbit on Monday, May 6, 2069,[1] with an umbral magnitude of 1.3242. 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 2.3 days after apogee (on May 4, 2069, at 1:40 UTC), the Moon's apparent diameter will be smaller.[2]

This lunar eclipse will be the third of an almost tetrad, with the others being on May 17, 2068 (partial); November 9, 2068 (total); and October 30, 2069 (total).

With the southern tip of the Moon passing through the center of the Earth's shadow, this is the first central eclipse of Lunar Saros 132.

The Moon will also occult the bright star Alpha Librae as seen from the southern hemisphere a few hours before greatest eclipse.[3]

Visibility

[edit]

The eclipse will be completely visible over western North America, Antarctica, and the eastern Pacific Ocean, seen rising over east Asia and Australia and setting over central and eastern North America and South America.[4]


The moon's hourly motion across the Earth's shadow in the constellation of Libra.

Eclipse details

[edit]

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]

May 6, 2069 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 2.39773
Umbral Magnitude 1.32418
Gamma 0.27172
Sun Right Ascension 02h55m56.2s
Sun Declination +16°44'53.2"
Sun Semi-Diameter 15'51.4"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 14h56m07.8s
Moon Declination -16°30'25.4"
Moon Semi-Diameter 14'46.2"
Moon Equatorial Horizontal Parallax 0°54'12.3"
ΔT 99.0 s

Eclipse season

[edit]

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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of April–May 2069
April 21
Descending node (new moon)
May 6
Ascending node (full moon)
May 20
Descending node (new moon)
Partial solar eclipse
Solar Saros 120
Total lunar eclipse
Lunar Saros 132
Partial solar eclipse
Solar Saros 158
[edit]

Eclipses in 2069

[edit]

Metonic

[edit]

Tzolkinex

[edit]

Half-Saros

[edit]

Tritos

[edit]

Lunar Saros 132

[edit]

Inex

[edit]

Triad

[edit]

Lunar eclipses of 2067–2070

[edit]
Lunar eclipse series sets from 2067-2070
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Saros Date
Viewing
Type
Chart
112 2067 May 28
Penumbral
117 2067 Nov 21
Penumbral
122 2068 May 17
Partial
127 2068 Nov 09
Total
132 2069 May 06
Total
137 2069 Oct 30
Total
142 2070 Apr 25
Penumbral
147 2070 Oct 19
Partial

Metonic series

[edit]

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 in nearly the same location relative to the background stars.

This series has 9 events centered on May 6th and October 30th: (saros number)

Ascending node Descending node
  1. 2031 May 07.160 - penumbral (112)
  2. 2050 May 06.937 - total (122)
  3. 2069 May 06.380 - total (132)
  4. 2088 May 05.677 - partial (142)
  5. 2107 May 07.186 - penumbral (152)
  1. 2031 Oct 30.323 - penumbral (117)
  2. 2050 Oct 30.139 - total (127)
  3. 2069 Oct 30.148 - total (137)
  4. 2088 Oct 30.125 - partial (147)

Saros 132

[edit]

Lunar saros series 132, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 44 umbral lunar eclipses (32 partial lunar eclipses and 12 total lunar eclipses).

Greatest First

The greatest eclipse of the series will occur on 2123 Jun 9, lasting 106 minutes.[6]
Penumbral Partial Total Central
1492 May 12
1636 Aug 16
2015 Apr 4
2069 May 6
Last
Central Total Partial Penumbral
2177 Jul 11
2213 Aug 2
2429 Dec 11
2754 Jun 26

There are 11 series events between 1901 and 2100, grouped into threes (called an exeligmos), each column with approximately the same viewing longitude on earth.

1901–2100
1907 Jan 29 1925 Feb 8 1943 Feb 20
1961 Mar 2 1979 Mar 13 1997 Mar 24
2015 Apr 4 2033 Apr 14 2051 Apr 26
2069 May 6 2087 May 17

Tritos series

[edit]

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

Inex series

[edit]

The inex series repeats eclipses 20 days short of 29 years, repeating on average every 10571.95 days. This period is equal to 358 lunations (synodic months) and 388.5 draconic months. Saros series increment by one on successive Inex events and repeat at alternate ascending and descending lunar nodes.

This period is 383.6734 anomalistic months (the period of the Moon's elliptical orbital precession). Despite the average 0.05 time-of-day shift between subsequent events, the variation of the Moon in its elliptical orbit at each event causes the actual eclipse time to vary significantly. It is a part of Lunar Inex series 39.

All events in this series listed below and more are total lunar eclipses.

Inex series from 1000 to 2500 AD
Ascending node Descending node Ascending node Descending node
Saros Date Saros Date Saros Date Saros Date
96 1027 Apr 23 97 1056 Apr 2 98 1085 Mar 14 99 1114 Feb 21
100 1143 Feb 1 101 1172 Jan 13 102 1200 Dec 22 103 1229 Dec 2
104 1258 Nov 12 105 1287 Oct 22 106 1316 Oct 2 107 1345 Sep 12
108 1374 Aug 22 109 1403 Aug 2 110 1432 Jul 13 111 1461 Jun 22
112 1490 Jun 2 113 1519 May 14 114 1548 Apr 22 115 1577 Apr 2
116 1606 Mar 24 117 1635 Mar 3 118 1664 Feb 11 119 1693 Jan 22
120 1722 Jan 2 121 1750 Dec 13 122 1779 Nov 23 123 1808 Nov 3
124 1837 Oct 13 125 1866 Sep 24 126 1895 Sep 4 127 1924 Aug 14
128 1953 Jul 26
129 1982 Jul 6
130 2011 Jun 15
131 2040 May 26
132 2069 May 6
133 2098 Apr 15
134 2127 Mar 28 135 2156 Mar 7
136 2185 Feb 14 137 2214 Jan 27 138 2243 Jan 7 139 2271 Dec 17
140 2300 Nov 27 141 2329 Nov 7 142 2358 Oct 18 143 2387 Sep 28
144 2416 Sep 7 145 2445 Aug 17 146 2474 Jul 29

Half-Saros cycle

[edit]

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[7] This lunar eclipse is related to two total solar eclipses of Solar Saros 139.

April 30, 2060 May 11, 2078

See also

[edit]

Notes

[edit]
  1. ^ "May 5–6, 2069 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 13 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 13 December 2024.
  3. ^ Jean Meeus, G. P. Konnen, "Occultations of Bright Stars by the Eclipsed Moon", Journal of the British Astronomical Association, Vol. 85, No. 1, pp. 17-24 (1974).
  4. ^ "Total Lunar Eclipse of 2069 May 06" (PDF). NASA. Retrieved 13 December 2024.
  5. ^ "Total Lunar Eclipse of 2069 May 06". EclipseWise.com. Retrieved 13 December 2024.
  6. ^ Listing of Eclipses of series 132
  7. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
[edit]

References

[edit]
  • Bao-Lin Liu, Canon of Lunar Eclipses 1500 B.C.-A.D. 3000, 1992