Solar eclipse of November 4, 2097
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, November 3 and Monday, November 4, 2097,[1] with a magnitude of 0.9494. 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. Occurring about 5.4 days before apogee (on November 9, 2097, at 12:15 UTC), the Moon's apparent diameter will be smaller.[2]
The path of annularity will be visible from parts of Antarctica. A partial solar eclipse will also be visible for parts of southwestern Australia and Antarctica. This annular eclipse is notable in that the path of annularity passes over the South Pole.
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 | 2097 November 3 at 23:34:35.1 UTC |
| First Umbral External Contact | 2097 November 4 at 01:06:01.0 UTC |
| First Central Line | 2097 November 4 at 01:10:07.9 UTC |
| First Umbral Internal Contact | 2097 November 4 at 01:14:32.3 UTC |
| Greatest Eclipse | 2097 November 4 at 02:01:25.2 UTC |
| Greatest Duration | 2097 November 4 at 02:10:27.8 UTC |
| Ecliptic Conjunction | 2097 November 4 at 02:11:36.5 UTC |
| Equatorial Conjunction | 2097 November 4 at 02:45:40.7 UTC |
| Last Umbral Internal Contact | 2097 November 4 at 02:47:47.0 UTC |
| Last Central Line | 2097 November 4 at 02:52:14.7 UTC |
| Last Umbral External Contact | 2097 November 4 at 02:56:25.0 UTC |
| Last Penumbral External Contact | 2097 November 4 at 04:28:03.3 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.94941 |
| Eclipse Obscuration | 0.90138 |
| Gamma | −0.89264 |
| Sun Right Ascension | 14h40m01.3s |
| Sun Declination | -15°33'59.2" |
| Sun Semi-Diameter | 16'07.3" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 14h38m39.0s |
| Moon Declination | -16°19'33.5" |
| Moon Semi-Diameter | 15'12.3" |
| Moon Equatorial Horizontal Parallax | 0°55'48.3" |
| ΔT | 121.5 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.
| October 21 Ascending node (full moon) |
November 4 Descending node (new moon) |
|---|---|
| File:Lunar eclipse chart close-2097Oct21.png | File:SE2097Nov04A.png |
| Total lunar eclipse Lunar Saros 128 |
Annular solar eclipse Solar Saros 154 |
Related eclipses
Eclipses in 2097
- A partial lunar eclipse on April 26.
- A total solar eclipse on May 11.
- A total lunar eclipse on October 21.
- An annular solar eclipse on November 4.
Metonic
- Preceded by: Solar eclipse of January 16, 2094
- Followed by: Solar eclipse of August 24, 2101
Tzolkinex
- Preceded by: Solar eclipse of September 23, 2090
- Followed by: Solar eclipse of December 17, 2104
Half-Saros
- Preceded by: Lunar eclipse of October 30, 2088
- Followed by: Lunar eclipse of November 11, 2106
Tritos
- Preceded by: Solar eclipse of December 6, 2086
- Followed by: Solar eclipse of October 4, 2108
Solar Saros 154
- Preceded by: Solar eclipse of October 24, 2079
- Followed by: Solar eclipse of November 16, 2115
Inex
- Preceded by: Solar eclipse of November 24, 2068
- Followed by: Solar eclipse of October 16, 2126
Triad
- Preceded by: Solar eclipse of January 4, 2011
- Followed by: Solar eclipse of September 4, 2184
Solar eclipses of 2094–2098
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 solar eclipses on January 16, 2094 (total) and July 12, 2094 (partial) occur in the previous lunar year eclipse set, and the partial solar eclipses on April 1, 2098 and September 25, 2098 occur in the next lunar year eclipse set.
| Solar eclipse series sets from 2094 to 2098 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 119 | June 13, 2094 File:SE2094Jun13P.png Partial |
−1.4613 | 124 | December 7, 2094 File:SE2094Dec07P.png Partial |
1.1547 | |
| 129 | June 2, 2095 File:SE2095Jun02T.png Total |
−0.6396 | 134 | November 27, 2095 File:SE2095Nov27A.png Annular |
0.4903 | |
| 139 | May 22, 2096 File:SE2096May22T.png Total |
0.1196 | 144 | November 15, 2096 File:SE2096Nov15A.png Annular |
−0.20 | |
| 149 | May 11, 2097 File:SE2097May11T.png Total |
0.8516 | 154 | November 4, 2097 File:SE2097Nov04A.png Annular |
−0.8926 | |
| 159 | May 1, 2098 | 164 | October 24, 2098 File:SE2098Oct24P.png Partial |
−1.5407 | ||
Saros 154
Template:Solar Saros series 154
Metonic series
Template:Solar Metonic series 2029–2116
Tritos series
Template:Solar Tritos series 2010 July 11
Inex series
Template:Solar Inex series 2011 January 4
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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