Solar eclipse of November 4, 2078
| Solar eclipse of November 4, 2078 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Annular |
| Gamma | -0.2285 |
| Magnitude | 0.9255 |
| Maximum eclipse | |
| Duration | 509 sec (8 m 29 s) |
| Coordinates | 27°48′S 83°18′W / 27.8°S 83.3°W |
| Max. width of band | 287 km (178 mi) |
| Times (UTC) | |
| Greatest eclipse | 16:55:44 |
| References | |
| Saros | 144 (20 of 70) |
| Catalog # (SE5000) | 9684 |
An annular solar eclipse will occur on Friday, November 4, 2078. 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 path of annularity will cross Pacific Ocean, South America, and Atlantic Ocean. The tables below contain detailed predictions and additional information on the Annular Solar Eclipse of 4 November 2078.
Eclipse Magnitude = 0.92551
Eclipse Obscuration = 0.85657
Gamma = -0.22852
Greatest Eclipse = 04 Nov 2078 16:53:57.5 UTC (16:55:44.4 TD)
Delta T = 1 minute, 46.9 seconds
Annularity Duration at Greatest Eclipse = 8 minutes, 29 seconds, 80 milliseconds
Annularity Duration at Greatest Duration = 8 minutes, 31 seconds, 940 milliseconds
Path Width at Greatest Eclipse = 287.5 km (178.6 mi)
Path Width at Greatest Duration = 286.0 km (177.7 mi)
Moon diameter = 1764.8 arcseconds
Sun diameter = 1935.0 arcseconds
Moon declination = 15 degrees, 49 minutes, 24.5 seconds south of the Celestial equator
Sun declination = 15 degrees, 38 minutes, 7.6 seconds south of the Celestial equator
Moon right ascension = 14 hours, 40 minutes, 33.5 seconds
Sun right ascension = 14 hours, 40 minutes, 53.9 seconds
Eclipse season[]
This is the second eclipse this season.
First eclipse this season:
Third eclipse this season:
Related eclipses[]
Solar eclipses 2076–2079[]
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.[1]
| Solar eclipse series sets from 2076–2079 | ||||
|---|---|---|---|---|
| Ascending node | Descending node | |||
| Saros | Map | Saros | Map | |
| 119 | June 1, 2076 Partial |
124 | November 26, 2076 Partial | |
| 129 | May 22, 2077 Total |
134 | November 15, 2077 Annular | |
| 139 | May 11, 2078 Total |
144 | November 4, 2078 Annular | |
| 149 | May 1, 2079 Total |
154 | October 24, 2079 Annular | |
Saros 144[]
It is a part of Saros cycle 144, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no total eclipses in the series. The series ends at member 70 as a partial eclipse on May 5, 2980. The longest duration of annularity will be 9 minutes, 52 seconds on December 29, 2168.
| Series members 11–21 occur between 1901 and 2100: | ||
|---|---|---|
| 11 | 12 | 13 |
 Jul 30, 1916 |
 Aug 10, 1934 |
 Aug 20, 1952 |
| 14 | 15 | 16 |
 Aug 31, 1970 |
 Sep 11, 1988 |
 Sep 22, 2006 |
| 17 | 18 | 19 |
 Oct 2, 2024 |
 Oct 14, 2042 |
 Oct 24, 2060 |
| 20 | 21 | |
Nov 4, 2078 |
 Nov 15, 2096 | |
Tritos series[]
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2100 | |||
|---|---|---|---|
 December 21, 1805 (Saros 119) |
 November 19, 1816 (Saros 120) |
 October 20, 1827 (Saros 121) | |
 September 18, 1838 (Saros 122) |
 August 18, 1849 (Saros 123) |
 July 18, 1860 (Saros 124) | |
 June 18, 1871 (Saros 125) |
 May 17, 1882 (Saros 126) |
 April 16, 1893 (Saros 127) | |
 March 17, 1904 (Saros 128) |
 February 14, 1915 (Saros 129) |
 January 14, 1926 (Saros 130) | |
 December 13, 1936 (Saros 131) |
 November 12, 1947 (Saros 132) |
 October 12, 1958 (Saros 133) | |
 September 11, 1969 (Saros 134) |
 August 10, 1980 (Saros 135) |
 July 11, 1991 (Saros 136) | |
 June 10, 2002 (Saros 137) |
 May 10, 2013 (Saros 138) |
 April 8, 2024 (Saros 139) | |
 March 9, 2035 (Saros 140) |
 February 5, 2046 (Saros 141) |
 January 5, 2057 (Saros 142) | |
 December 6, 2067 (Saros 143) |
November 4, 2078 (Saros 144) |
 October 4, 2089 (Saros 145) | |
 September 4, 2100 (Saros 146) |
|||
In the 22nd century:
- Solar saros 147: annular solar eclipse of August 4, 2111
- Solar saros 148: total solar eclipse of July 4, 2122
- Solar saros 149: total solar eclipse of June 3, 2133
- Solar saros 150: annular solar eclipse of May 3, 2144
- Solar saros 151: annular solar eclipse of April 2, 2155
- Solar saros 152: total solar eclipse of March 2, 2166
- Solar saros 153: annular solar eclipse of January 29, 2177
- Solar saros 154: annular solar eclipse of December 29, 2187
- Solar saros 155: total solar eclipse of November 28, 2198
In the 23rd century:
- Solar saros 156: annular solar eclipse of October 29, 2209
- Solar saros 157: annular solar eclipse of September 27, 2220
- Solar saros 158: total solar eclipse of August 28, 2231
- Solar saros 159: partial solar eclipse of July 28, 2242
- Solar saros 160: partial solar eclipse of June 26, 2253
- Solar saros 161: partial solar eclipse of May 26, 2264
- Solar saros 162: partial solar eclipse of April 26, 2275
- Solar saros 163: partial solar eclipse of March 25, 2286
- Solar saros 164: partial solar eclipse of February 22, 2297
Metonic cycle[]
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days).
| 21 eclipse events between June 12, 2029 and June 12, 2105 | ||||
|---|---|---|---|---|
| June 11–12 | March 30–31 | January 16 | November 4–5 | August 23–24 |
| 118 | 120 | 122 | 124 | 126 |
 June 12, 2029 |
 March 30, 2033 |
 January 16, 2037 |
 November 4, 2040 |
 August 23, 2044 |
| 128 | 130 | 132 | 134 | 136 |
 June 11, 2048 |
 March 30, 2052 |
 January 16, 2056 |
 November 5, 2059 |
 August 24, 2063 |
| 138 | 140 | 142 | 144 | 146 |
 June 11, 2067 |
 March 31, 2071 |
 January 16, 2075 |
November 4, 2078 |
 August 24, 2082 |
| 148 | 150 | 152 | 154 | |
 June 11, 2086 |
 March 31, 2090 |
 January 16, 2094 |
 November 4, 2097 | |
References[]
- ^ 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.
External links[]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
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