Solar eclipse of April 10, 2089
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse will occur at the Moon's descending node of orbit between Sunday, April 10 and Monday, April 11, 2089,[1] with a magnitude of 0.9919. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The Moon's apparent diameter will be near the average diameter because it will occur 7 days after apogee (on April 3, 2089, at 23:20 UTC) and 6.8 days before perigee (on April 17, 2089, at 17:00 UTC).[2]
The path of annularity will be visible from parts of southeastern Australia, Tonga, and Niue. A partial solar eclipse will also be visible for parts of Australia, Oceania, Antarctica, Mexico, and Central America.
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 2089 April 10 at 19:56:15.6 UTC |
| First Umbral External Contact | 2089 April 10 at 20:59:15.4 UTC |
| First Central Line | 2089 April 10 at 21:00:03.3 UTC |
| Greatest Duration | 2089 April 10 at 21:00:03.3 UTC |
| First Umbral Internal Contact | 2089 April 10 at 21:00:51.4 UTC |
| First Penumbral Internal Contact | 2089 April 10 at 22:11:51.4 UTC |
| Equatorial Conjunction | 2089 April 10 at 22:33:57.5 UTC |
| Greatest Eclipse | 2089 April 10 at 22:44:41.5 UTC |
| Ecliptic Conjunction | 2089 April 10 at 22:48:21.4 UTC |
| Last Penumbral Internal Contact | 2089 April 10 at 23:17:50.5 UTC |
| Last Umbral Internal Contact | 2089 April 11 at 00:28:41.8 UTC |
| Last Central Line | 2089 April 11 at 00:29:26.8 UTC |
| Last Umbral External Contact | 2089 April 11 at 00:30:11.6 UTC |
| Last Penumbral External Contact | 2089 April 11 at 01:33:05.8 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.99192 |
| Eclipse Obscuration | 0.98391 |
| Gamma | −0.33186 |
| Sun Right Ascension | 01h20m36.9s |
| Sun Declination | +08°29'24.5" |
| Sun Semi-Diameter | 15'57.8" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 01h20m58.3s |
| Moon Declination | +08°11'12.9" |
| Moon Semi-Diameter | 15'35.9" |
| Moon Equatorial Horizontal Parallax | 0°57'14.7" |
| ΔT | 113.5 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.
| March 26 Ascending node (full moon) |
April 10 Descending node (new moon) |
|---|---|
| File:SE2089Apr10A.png | |
| Penumbral lunar eclipse Lunar Saros 114 |
Annular solar eclipse Solar Saros 140 |
Related eclipses
Eclipses in 2089
- A penumbral lunar eclipse on March 26.
- An annular solar eclipse on April 10.
- A penumbral lunar eclipse on September 19.
- A total solar eclipse on October 4.
Metonic
- Preceded by: Solar eclipse of June 22, 2085
- Followed by: Solar eclipse of January 27, 2093
Tzolkinex
- Preceded by: Solar eclipse of February 27, 2082
- Followed by: Solar eclipse of May 22, 2096
Half-Saros
- Preceded by: Lunar eclipse of April 4, 2080
- Followed by: Lunar eclipse of April 15, 2098
Tritos
- Preceded by: Solar eclipse of May 11, 2078
- Followed by: Solar eclipse of March 10, 2100
Solar Saros 140
- Preceded by: Solar eclipse of March 31, 2071
- Followed by: Solar eclipse of April 23, 2107
Inex
- Preceded by: Solar eclipse of April 30, 2060
- Followed by: Solar eclipse of March 22, 2118
Triad
- Preceded by: Solar eclipse of June 10, 2002
- Followed by: Solar eclipse of February 10, 2176
Solar eclipses of 2087–2090
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[4]
The partial solar eclipse on June 1, 2087 occurs in the previous lunar year eclipse set.
| Solar eclipse series sets from 2087 to 2090 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 120 | May 2, 2087 File:SE2087May02P.png Partial |
1.1139 | 125 | October 26, 2087 File:SE2087Oct26P.png Partial |
−1.2882 | |
| 130 | April 21, 2088 File:SE2088Apr21T.png Total |
0.4135 | 135 | October 14, 2088 File:SE2088Oct14A.png Annular |
−0.5349 | |
| 140 | April 10, 2089 File:SE2089Apr10A.png Annular |
−0.3319 | 145 | October 4, 2089 File:SE2089Oct04T.png Total |
0.2167 | |
| 150 | March 31, 2090 File:SE2090Mar31P.png Partial |
−1.1028 | 155 | September 23, 2090 File:SE2090Sep23T.png Total |
0.9157 | |
Saros 140
Template:Solar Saros series 140
Metonic series
Template:Solar Metonic series 2047–2134
Tritos series
Template:Solar Tritos series 2001 December 14
Inex series
Template:Solar Inex series 2002 June 10
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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