Solar eclipse of September 25, 2098
| Solar eclipse of September 25, 2098 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Partial |
| Gamma | 1.14 |
| Magnitude | 0.7871 |
| Maximum eclipse | |
| Coordinates | 61°06′N 101°00′W / 61.1°N 101°W |
| Times (UTC) | |
| Greatest eclipse | 0:31:16 |
| References | |
| Saros | 126 (52 of 72) |
| Catalog # (SE5000) | 9729 |
A partial solar eclipse will occur on September 25, 2098. 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. A partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
Related eclipses
Solar eclipses 2098–2100
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]
The partial solar eclipse on October 24, 2098 occurs in the previous lunar year eclipse set.
| Solar eclipse series sets from 2098 to 2101 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 121 | April 1, 2098 Partial |
−1.1005 | 126 | September 25, 2098 Partial |
1.14 | |
| 131 | March 21, 2099 Annular |
−0.4016 | 136 | September 14, 2099 Total |
0.3942 | |
| 141 | March 10, 2100 Annular |
0.3077 | 146 | September 4, 2100 Total |
−0.3384 | |
| 151 | February 28, 2101 Annular |
0.9964 | 156 | August 24, 2101 Partial |
−1.1392 | |
Saros 126
This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. Its 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.
The longest duration of annularity was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit.[2]
| Series members 36–57 occur between 1801 and 2200: | ||
|---|---|---|
| 36 | 37 | 38 |
 April 4, 1810 |
 April 14, 1828 |
 April 25, 1846 |
| 39 | 40 | 41 |
 May 6, 1864 |
 May 17, 1882 |
 May 28, 1900 |
| 42 | 43 | 44 |
 June 8, 1918 |
 June 19, 1936 |
 June 30, 1954 |
| 45 | 46 | 47 |
 July 10, 1972 |
 July 22, 1990 |
 August 1, 2008 |
| 48 | 49 | 50 |
 August 12, 2026 |
 August 23, 2044 |
 September 3, 2062 |
| 51 | 52 | 53 |
 September 13, 2080 |
September 25, 2098 |
 October 6, 2116 |
| 54 | 55 | 56 |
 October 17, 2134 |
 October 28, 2152 |
 November 8, 2170 |
| 57 | ||
 November 18, 2188 | ||
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.
- ^ "NASA - Catalog of Solar Eclipses of Saros 126". eclipse.gsfc.nasa.gov.
External links
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