June 2058 lunar eclipse
Template:Short description Template:Infobox lunar eclipse A total lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, June 6, 2058,[1] with an umbral magnitude of 1.6628. It will be a central lunar eclipse, in which part of the Moon will pass through the center of the Earth's shadow. 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 1.6 days before perigee (on June 8, 2058, at 9:30 UTC), the Moon's apparent diameter will be larger.[2]
During the eclipse, IC 4634 will be occulted by the Moon over Antarctica. Deep-sky objects are rarely occulted during a total eclipse from any given spot on Earth.[3]Template:Rp
Visibility
The eclipse will be completely visible over east Africa, Antarctica, west, central, and south Asia, and western Australia, seen rising over west Africa, Europe, and eastern South America and setting over east Asia and eastern Australia.[4]
| File:Lunar eclipse from moon-2058Jun06.png File:Lunar eclipse chart close-2058Jun06.png |
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[5]
| Parameter | Value |
|---|---|
| Penumbral Magnitude | 2.62261 |
| Umbral Magnitude | 1.66277 |
| Gamma | −0.11810 |
| Sun Right Ascension | 05h00m41.7s |
| Sun Declination | +22°43'57.0" |
| Sun Semi-Diameter | 15'45.8" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 17h00m35.5s |
| Moon Declination | -22°50'55.4" |
| Moon Semi-Diameter | 16'25.3" |
| Moon Equatorial Horizontal Parallax | 1°00'16.2" |
| ΔT | 90.8 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| May 22 Ascending node (new moon) |
June 6 Descending node (full moon) |
June 21 Ascending node (new moon) |
|---|---|---|
| File:SE2058May22P.png | File:Lunar eclipse chart close-2058Jun06.png | File:SE2058Jun21P.png |
| Partial solar eclipse Solar Saros 119 |
Total lunar eclipse Lunar Saros 131 |
Partial solar eclipse Solar Saros 157 |
Related eclipses
Eclipses in 2058
- A partial solar eclipse on May 22.
- A total lunar eclipse on June 6.
- A partial solar eclipse on June 21.
- A partial solar eclipse on November 16.
- A total lunar eclipse on November 30.
Metonic
- Preceded by: Lunar eclipse of August 18, 2054
- Followed by: Lunar eclipse of March 25, 2062
Tzolkinex
- Preceded by: Lunar eclipse of April 26, 2051
- Followed by: Lunar eclipse of July 17, 2065
Half-Saros
- Preceded by: Solar eclipse of May 31, 2049
- Followed by: Solar eclipse of June 11, 2067
Tritos
- Preceded by: Lunar eclipse of July 7, 2047
- Followed by: Lunar eclipse of May 6, 2069
Lunar Saros 131
- Preceded by: Lunar eclipse of May 26, 2040
- Followed by: Lunar eclipse of June 17, 2076
Inex
- Preceded by: Lunar eclipse of June 26, 2029
- Followed by: Lunar eclipse of May 17, 2087
Triad
- Preceded by: Lunar eclipse of August 6, 1971
- Followed by: Lunar eclipse of April 7, 2145
Lunar eclipses of 2056–2060
Template:Lunar eclipse set 2056-2060
Saros 131
This eclipse is a part of Saros series 131, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on May 10, 1427. It contains partial eclipses from July 25, 1553 through March 22, 1932; total eclipses from April 2, 1950 through September 3, 2202; and a second set of partial eclipses from September 13, 2220 through April 9, 2563. The series ends at member 72 as a penumbral eclipse on July 7, 2707.
The longest duration of totality will be produced by member 38 at 100 minutes, 36 seconds on June 28, 2094. All eclipses in this series occur at the Moon’s descending node of orbit.[6]
| Greatest | First | |||
|---|---|---|---|---|
| File:Lunar eclipse chart close-2094Jun28.png The greatest eclipse of the series will occur on 2094 Jun 28, lasting 100 minutes, 36 seconds.[7] |
Penumbral | Partial | Total | Central |
| 1427 May 10 |
1553 Jul 25 |
1950 Apr 02 File:Lunar eclipse chart close-1950Apr02.png |
2022 May 16 File:Lunar eclipse chart close-2022may16.png | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 2148 Jul 31 |
2202 Sep 03 |
2563 Apr 09 |
2707 Jul 07 | |
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
Template:Lunar Tritos series November 2003
Inex series
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | |||||
|---|---|---|---|---|---|
| 1826 Nov 14 (Saros 123) |
1855 Oct 25 (Saros 124) |
1884 Oct 04 (Saros 125) | |||
| 1913 Sep 15 (Saros 126) |
1942 Aug 26 (Saros 127) |
1971 Aug 06 (Saros 128) | |||
| File:Lunar eclipse chart close-1913Sep15.png | File:Lunar eclipse from moon-1913Sep15.png | File:Lunar eclipse chart close-1942Aug26.png | File:Lunar eclipse from moon-1942Aug26.png | File:Lunar eclipse chart close-1971Aug06.png | File:Lunar eclipse from moon-1971Aug06.png |
| 2000 Jul 16 (Saros 129) |
2029 Jun 26 (Saros 130) |
2058 Jun 06 (Saros 131) | |||
| File:Lunar eclipse chart close-2000jul16.png | File:Lunar eclipse from moon-2000Jul16.png | File:Lunar eclipse chart close-29jun26.png | File:Lunar eclipse from moon-2029Jun26.png | File:Lunar eclipse chart close-2058Jun06.png | File:Lunar eclipse from moon-2058Jun06.png |
| 2087 May 17 (Saros 132) |
2116 Apr 27 (Saros 133) |
2145 Apr 07 (Saros 134) | |||
| File:Lunar eclipse chart close-2087May17.png | File:Lunar eclipse from moon-2087May17.png | ||||
| 2174 Mar 18 (Saros 135) | |||||
Half-Saros cycle
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 138.
| May 31, 2049 | June 11, 2067 |
|---|---|
| File:SE2049May31A.png | File:SE2067Jun11A.png |
See also
Notes
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- ↑ Listing of Eclipses of series 131
- ↑ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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External links
- 2058 Jun 06 chart Eclipse Predictions by Fred Espenak, NASA/GSFC
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