Solar eclipse of March 10, 2081
Solar eclipse of March 10, 2081 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | −0.3653 |
Magnitude | 0.9304 |
Maximum eclipse | |
Duration | 456 s (7 min 36 s) |
Coordinates | 22°24′S 36°42′W / 22.4°S 36.7°W |
Max. width of band | 277 km (172 mi) |
Times (UTC) | |
Greatest eclipse | 15:23:31 |
References | |
Saros | 131 (54 of 70) |
Catalog # (SE5000) | 9689 |
An annular solar eclipse will occur at the Moon's ascending node of orbit on Monday, March 10, 2081, with a magnitude of 0.9304. 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.
Related eclipses[edit]
Eclipses in 2081[edit]
- An annular solar eclipse on March 10, 2081.
- A partial lunar eclipse on March 25, 2081.
- A total solar eclipse on September 3, 2081.
- A penumbral lunar eclipse on September 18, 2081.
Metonic[edit]
- Preceded by: Solar eclipse of May 22, 2077
- Followed by: Solar eclipse of December 27, 2084
Tzolkinex[edit]
- Preceded by: Solar eclipse of January 27, 2074
- Followed by: Solar eclipse of April 21, 2088
Half-Saros[edit]
- Preceded by: Lunar eclipse of March 4, 2072
- Followed by: Lunar eclipse of March 15, 2090
Tritos[edit]
- Preceded by: Solar eclipse of April 11, 2070
- Followed by: Solar eclipse of February 7, 2092
Solar Saros 131[edit]
- Preceded by: Solar eclipse of February 28, 2063
- Followed by: Solar eclipse of March 21, 2099
Inex[edit]
- Preceded by: Solar eclipse of March 30, 2052
- Followed by: Solar eclipse of February 18, 2110
Triad[edit]
- Preceded by: Solar eclipse of May 10, 1994
- Followed by: Solar eclipse of January 10, 2168
Solar eclipses of 2080–2083[edit]
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 July 15, 2083 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 2080 to 2083 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | March 21, 2080![]() Partial |
−1.0578 | 126 | September 13, 2080![]() Partial |
1.0723 | |
131 | March 10, 2081![]() Annular |
−0.3653 | 136 | September 3, 2081![]() Total |
0.3378 | |
141 | February 27, 2082![]() Annular |
0.3361 | 146 | August 24, 2082![]() Total |
−0.4004 | |
151 | February 16, 2083![]() Partial |
1.017 | 156 | August 13, 2083![]() Partial |
−1.2064 |
Saros 131[edit]
This eclipse is a part of Saros series 131, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on August 1, 1125. It contains total eclipses from March 27, 1522 through May 30, 1612; hybrid eclipses from June 10, 1630 through July 24, 1702; and annular eclipses from August 4, 1720 through June 18, 2243. The series ends at member 70 as a partial eclipse on September 2, 2369. 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 totality was produced by member 28 at 58 seconds on May 30, 1612, and the longest duration of annularity was produced by member 50 at 7 minutes, 54 seconds on January 26, 2009. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]
Series members 39–60 occur between 1801 and 2200: | ||
---|---|---|
39 | 40 | 41 |
![]() September 28, 1810 |
![]() October 9, 1828 |
![]() October 20, 1846 |
42 | 43 | 44 |
![]() October 30, 1864 |
![]() November 10, 1882 |
![]() November 22, 1900 |
45 | 46 | 47 |
![]() December 3, 1918 |
![]() December 13, 1936 |
![]() December 25, 1954 |
48 | 49 | 50 |
![]() January 4, 1973 |
![]() January 15, 1991 |
![]() January 26, 2009 |
51 | 52 | 53 |
![]() February 6, 2027 |
![]() February 16, 2045 |
![]() February 28, 2063 |
54 | 55 | 56 |
![]() March 10, 2081 |
![]() March 21, 2099 |
![]() April 2, 2117 |
57 | 58 | 59 |
![]() April 13, 2135 |
![]() April 23, 2153 |
![]() May 5, 2171 |
60 | ||
![]() May 15, 2189 |
Inex series[edit]
This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
Inex series members between 1901 and 2100: | ||
---|---|---|
![]() July 10, 1907 (Saros 125) |
![]() June 19, 1936 (Saros 126) |
![]() May 30, 1965 (Saros 127) |
![]() May 10, 1994 (Saros 128) |
![]() April 20, 2023 (Saros 129) |
![]() March 30, 2052 (Saros 130) |
![]() March 10, 2081 (Saros 131) |
References[edit]
- ^ 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 131". eclipse.gsfc.nasa.gov.
External links[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC