July 2047 lunar eclipse
{{Short description|Central lunar eclipse}}
{{Infobox lunar eclipse
| type = total
| image = Lunar eclipse chart close-2047Jul07.png
| caption = The Moon's hourly motion shown right to left
| date = July 7, 2047
| gamma = −0.0636
| magnitude = 1.7529
| saros_ser = 130
| saros_no = 36 of 72
| totality = 100 minutes, 49 seconds
| partiality = 218 minutes, 31 seconds
| penumbral = 333 minutes, 27 seconds
| p1 = 7:37:44
| u1 = 8:44:58
| u2 = 9:43:49
| greatest = 10:34:15
| u3 = 11:24:39
| u4 = 12:23:29
| p4 = 13:21:01
| previous = January 2047
| next = January 2048
}}
A total lunar eclipse will occur at the Moon’s ascending node of orbit on Sunday, July 7, 2047,{{cite web|title=July 6–7, 2047 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2047-july-7|publisher=timeanddate|access-date=11 December 2024}} with an umbral magnitude of 1.7529. 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 3.4 days after perigee (on July 4, 2047, at 0:55 UTC), the Moon's apparent diameter will be larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2047&n=136|publisher=timeanddate|access-date=11 December 2024}}
Totality will last 100 minutes 49 seconds, the second longest for this Saros series.
Visibility
The eclipse will be completely visible over eastern Australia, Antarctica, and the central and eastern Pacific Ocean, seen rising over east Asia and western Australia and setting over North and South America.{{cite web|title=Total Lunar Eclipse of 2047 Jul 07|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot2001/LE2047Jul07T.pdf|publisher=NASA|access-date=11 December 2024}}
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Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Total Lunar Eclipse of 2047 Jul 07|url=https://eclipsewise.com/lunar/LEprime/2001-2100/LE2047Jul07Tprime.html|publisher=EclipseWise.com|access-date=11 December 2024}}
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|+July 7, 2047 Lunar Eclipse Parameters ! Parameter ! Value |
Penumbral Magnitude
| 2.73257 |
Umbral Magnitude
| 1.75293 |
Gamma
| −0.06362 |
Sun Right Ascension
| 07h06m19.6s |
Sun Declination
| +22°33'30.9" |
Sun Semi-Diameter
| 15'43.9" |
Sun Equatorial Horizontal Parallax
| 08.7" |
Moon Right Ascension
| 19h06m23.0s |
Moon Declination
| -22°37'10.8" |
Moon Semi-Diameter
| 16'03.5" |
Moon Equatorial Horizontal Parallax
| 0°58'56.1" |
ΔT
| 83.5 s |
{{clear}}
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. The first and last eclipse in this sequence is separated by one synodic month.
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|+ Eclipse season of June–July 2047 ! June 23 | ||
200px | 200px | 200px |
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| Partial solar eclipse | Total lunar eclipse Lunar Saros 130 | Partial solar eclipse Solar Saros 156 |
Related eclipses
= Eclipses in 2047 =
= Metonic =
- Preceded by: Lunar eclipse of September 19, 2043
- Followed by: Lunar eclipse of April 26, 2051
= Tzolkinex =
- Preceded by: Lunar eclipse of May 26, 2040
- Followed by: Lunar eclipse of August 18, 2054
= Half-Saros =
- Preceded by: Solar eclipse of July 2, 2038
- Followed by: Solar eclipse of July 12, 2056
= Tritos =
- Preceded by: Lunar eclipse of August 7, 2036
- Followed by: Lunar eclipse of June 6, 2058
= Lunar Saros 130 =
- Preceded by: Lunar eclipse of June 26, 2029
- Followed by: Lunar eclipse of July 17, 2065
= Inex =
- Preceded by: Lunar eclipse of July 27, 2018
- Followed by: Lunar eclipse of June 17, 2076
= Triad =
- Preceded by: Lunar eclipse of September 5, 1960
- Followed by: Lunar eclipse of May 8, 2134
= Lunar eclipses of 2046–2049 =
{{Lunar eclipse set 2046-2049}}
= Saros 130 =
{{Lunar Saros series 130}}
= Tritos series =
{{Lunar Tritos series November 2003}}
= Inex series =
{{Lunar Inex series July 2018}}
= Half-Saros cycle =
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros This lunar eclipse is related to two annular solar eclipses of Solar Saros 137.
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See also
Notes
{{reflist}}
External links
- {{LEplot2001 link|2047|Jul|07|T}}
{{Lunar eclipses}}
{{DEFAULTSORT:Lunar eclipse 2047-07}}