Partial eclipse | |||||||||||||
The Moon's hourly motion shown right to left | |||||||||||||
Date | April 5, 2099 | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gamma | −0.9304 | ||||||||||||
Magnitude | 0.1680 | ||||||||||||
Saros cycle | 143 (23 of 73) | ||||||||||||
Partiality | 88 minutes, 4 seconds | ||||||||||||
Penumbral | 257 minutes, 43 seconds | ||||||||||||
| |||||||||||||
← 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.
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 cycleThis 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.
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
- An annular solar eclipse on March 21.
- A partial lunar eclipse on April 5.
- A total solar eclipse on September 14.
- A penumbral lunar eclipse on September 29.
Metonic
- Preceded by: Lunar eclipse of June 17, 2095
- Followed by: Lunar eclipse of January 23, 2103
Tzolkinex
- Preceded by: Lunar eclipse of February 23, 2092
- Followed by: Lunar eclipse of May 17, 2106
Half-Saros
- Preceded by: Solar eclipse of March 31, 2090
- Followed by: Solar eclipse of April 11, 2108
Tritos
- Preceded by: Lunar eclipse of May 5, 2088
- Followed by: Lunar eclipse of March 6, 2110
Lunar Saros 143
- Preceded by: Lunar eclipse of March 25, 2081
- Followed by: Lunar eclipse of April 16, 2117
Inex
- Preceded by: Lunar eclipse of April 25, 2070
- Followed by: Lunar eclipse of March 16, 2128
Triad
- Preceded by: Lunar eclipse of June 4, 2012
- Followed by: Lunar eclipse of February 4, 2186
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
- "April 4–5, 2099 Partial Lunar Eclipse". timeanddate. Retrieved 14 December 2024.
- "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 14 December 2024.
- "Partial Lunar Eclipse of 2099 Apr 05" (PDF). NASA. Retrieved 14 December 2024.
- "Partial Lunar Eclipse of 2099 Apr 05". EclipseWise.com. Retrieved 14 December 2024.
- 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.
- "NASA - Catalog of Lunar Eclipses of Saros 143". eclipse.gsfc.nasa.gov.
- Listing of Eclipses of series 143
- Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
External links
- 2099 Apr 05 chart Eclipse Predictions by Fred Espenak, NASA/GSFC