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April 2034 lunar eclipse

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Astronomical event
April 2034 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateApril 3, 2034
Gamma1.1144
Magnitude−0.2263
Saros cycle142 (19 of 74)
Penumbral265 minutes, 25 seconds
Contacts (UTC)
P116:52:54
Greatest19:06:59
P421:18:19
← October 2033September 2034 →

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Monday, April 3, 2034, with an umbral magnitude of −0.2263. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into the Earth's penumbra. 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. Occurring about 2.2 days before apogee (on April 5, 2034, at 23:45 UTC), the Moon's apparent diameter will be smaller.

Visibility

The eclipse will be completely visible over east Africa, eastern Europe, Asia, and western Australia, seen rising over west Africa, western Europe, and eastern South America and setting over eastern Australia and northeast Asia.

Eclipse details

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

April 3, 2034 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.85566
Umbral Magnitude −0.22631
Gamma 1.11441
Sun Right Ascension 00h51m54.0s
Sun Declination +05°33'29.1"
Sun Semi-Diameter 15'59.8"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 12h53m05.6s
Moon Declination -04°35'42.2"
Moon Semi-Diameter 14'47.1"
Moon Equatorial Horizontal Parallax 0°54'15.6"
ΔT 76.0 s

Eclipse season

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 March–April 2034
March 20
Descending node (new moon)
April 3
Ascending node (full moon)
Total solar eclipse
Solar Saros 130
Penumbral lunar eclipse
Lunar Saros 142

Related eclipses

Eclipses in 2034

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 142

Inex

Triad

Lunar eclipses of 2031–2034

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.

The penumbral lunar eclipse on June 5, 2031 occurs in the previous lunar year eclipse set.

Lunar eclipse series sets from 2031 to 2034
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
112 2031 May 07
Penumbral
−1.0694 117 2031 Oct 30
Penumbral
1.1774
122 2032 Apr 25
Total
−0.3558 127 2032 Oct 18
Total
0.4169
132 2033 Apr 14
Total
0.3954 137 2033 Oct 08
Total
−0.2889
142 2034 Apr 03
Penumbral
1.1144 147 2034 Sep 28
Partial
−1.0110

Saros 142

This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 73 events. The series started with a penumbral lunar eclipse on September 19, 1709. It contains partial eclipses from May 5, 2088 through July 10, 2196; total eclipses from July 22, 2214 through April 21, 2665; and a second set of partial eclipses from May 3, 2683 through July 29, 2827. The series ends at member 73 as a penumbral eclipse on November 17, 3007.

The longest duration of totality will be produced by member 34 at 103 minutes, 54 seconds on September 15, 2304. All eclipses in this series occur at the Moon’s ascending node of orbit.

Greatest First
The greatest eclipse of the series will occur on 2304 Sep 15, lasting 103 minutes, 54 seconds. Penumbral Partial Total Central
1709 Sep 19
2088 May 05
2214 Jul 22
2250 Aug 13
Last
Central Total Partial Penumbral
2448 Dec 10
2665 Apr 21
2827 Jul 29
3007 Nov 17

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.

Series members 7–28 occur between 1801 and 2200:
7 8 9
1817 Nov 23 1835 Dec 05 1853 Dec 15
10 11 12
1871 Dec 26 1890 Jan 06 1908 Jan 18
13 14 15
1926 Jan 28 1944 Feb 09 1962 Feb 19
16 17 18
1980 Mar 01 1998 Mar 13 2016 Mar 23
19 20 21
2034 Apr 03 2052 Apr 14 2070 Apr 25
22 23 24
2088 May 05 2106 May 17 2124 May 28
25 26 27
2142 Jun 08 2160 Jun 18 2178 Jun 30
28
2196 Jul 10

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 149.

March 29, 2025 April 9, 2043

See also

Notes

  1. "April 3–4, 2034 Penumbral Lunar Eclipse". timeanddate. Retrieved 23 November 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 23 November 2024.
  3. "Penumbral Lunar Eclipse of 2034 Apr 03" (PDF). NASA. Retrieved 23 November 2024.
  4. "Penumbral Lunar Eclipse of 2034 Apr 03". EclipseWise.com. Retrieved 23 November 2024.
  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 142". eclipse.gsfc.nasa.gov.
  7. Listing of Eclipses of series 142
  8. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

External links

Lunar eclipses
Lists of lunar eclipses
Lunar eclipses
by era
Lunar eclipses
by saros series
August 2017 lunar eclipse
Partial eclipses
May 2022 lunar eclipse
Total eclipses
February 2017 lunar eclipse
Penumbral eclipses
Partial
Total
Related
  • Category
  • symbol denotes next eclipse in series


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