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April 2099 lunar eclipse

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Astronomical event

April 2099 lunar eclipse
Partial eclipse
The Moon's hourly motion shown right to left
DateApril 5, 2099
Gamma−0.9304
Magnitude0.1680
Saros cycle143 (23 of 73)
Partiality88 minutes, 4 seconds
Penumbral257 minutes, 43 seconds
Contacts (UTC)
P16:18:44
U17:43:31
Greatest8:27:36
U49:11:35
P410:36:27
← October 2098September 2099 →

A partial lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, April 5, 2099, with an umbral magnitude of 0.1680. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in 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 1.4 days after perigee (on April 3, 2099, at 23:30 UTC), the Moon's apparent diameter will be larger.

Visibility

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

Eclipse details

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

April 5, 2099 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.13534
Umbral Magnitude 0.16996
Gamma −0.93038
Sun Right Ascension 00h58m32.6s
Sun Declination +06°14'54.6"
Sun Semi-Diameter 15'59.6"
Sun Equatorial Horizontal Parallax 08.8"
Moon Right Ascension 12h56m44.9s
Moon Declination -07°04'45.1"
Moon Semi-Diameter 16'34.0"
Moon Equatorial Horizontal Parallax 1°00'48.0"
ΔT 126.2 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 2099
March 21
Ascending node (new moon)
April 5
Descending node (full moon)
Annular solar eclipse
Solar Saros 131
Partial lunar eclipse
Lunar Saros 143

Related eclipses

Eclipses in 2099

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 143

Inex

Triad

Lunar eclipses of 2096–2099

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 eclipses on June 6, 2096 and November 29, 2096 occur in the previous lunar year eclipse set.

Lunar eclipse series sets from 2096 to 2099
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
113 2096 May 07
Penumbral
1.2896 118 2096 Oct 31
Penumbral
−1.1307
123 2097 Apr 26
Partial
0.5377 128 2097 Oct 21
Total
−0.4608
133 2098 Apr 15
Total
−0.2272 138 2098 Oct 10
Total
0.2749
143 2099 Apr 05
Partial
−0.9304 148 2099 Sep 29
Penumbral
1.0174

Saros 143

This eclipse is a part of Saros series 143, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on August 18, 1720. It contains partial eclipses from March 14, 2063 through June 21, 2225; total eclipses from July 2, 2243 through April 13, 2712; and a second set of partial eclipses from April 25, 2730 through July 9, 2856. The series ends at member 72 as a penumbral eclipse on October 5, 3000.

The longest duration of totality will be produced by member 36 at 99 minutes, 9 seconds on September 6, 2351. All eclipses in this series occur at the Moon’s descending node of orbit.

Greatest First
The greatest eclipse of the series will occur on 2351 Sep 06, lasting 99 minutes, 9 seconds. Penumbral Partial Total Central
1720 Aug 18
2063 Mar 14
2243 Jul 02
2297 Aug 03
Last
Central Total Partial Penumbral
2495 Dec 02
2712 Apr 13
2856 Jul 09
3000 Oct 05

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 6–27 occur between 1801 and 2200:
6 7 8
1810 Oct 12 1828 Oct 23 1846 Nov 03
9 10 11
1864 Nov 13 1882 Nov 25 1900 Dec 06
12 13 14
1918 Dec 17 1936 Dec 28 1955 Jan 08
15 16 17
1973 Jan 18 1991 Jan 30 2009 Feb 09
18 19 20
2027 Feb 20 2045 Mar 03 2063 Mar 14
21 22 23
2081 Mar 25 2099 Apr 05 2117 Apr 16
24 25 26
2135 Apr 28 2153 May 08 2171 May 19
27
2189 May 29

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 partial solar eclipses of Solar Saros 150.

March 31, 2090 April 11, 2108

See also

Notes

  1. "April 4–5, 2099 Partial Lunar Eclipse". timeanddate. Retrieved 14 December 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 December 2024.
  3. "Partial Lunar Eclipse of 2099 Apr 05" (PDF). NASA. Retrieved 14 December 2024.
  4. "Partial Lunar Eclipse of 2099 Apr 05". EclipseWise.com. Retrieved 14 December 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 143". eclipse.gsfc.nasa.gov.
  7. Listing of Eclipses of series 143
  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
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