Solar eclipse of March 10, 2100
Solar eclipse of March 10, 2100 | |
---|---|
Type of eclipse | |
Nature | Annular |
Gamma | 0.3077 |
Magnitude | 0.9338 |
Maximum eclipse | |
Duration | 449 s (7 min 29 s) |
Coordinates | 12°00′N 162°24′W / 12°N 162.4°W |
Max. width of band | 257 km (160 mi) |
Times (UTC) | |
Greatest eclipse | 22:28:11 |
References | |
Saros | 141 (28 of 70) |
Catalog # (SE5000) | 9733 |
An annular solar eclipse will occur at the Moon's ascending node of orbit between Wednesday, March 10 and Thursday, March 11, 2100, with a magnitude of 0.9338. 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 kilometers wide. The path of annularity will move from Indonesia at sunrise, over the islands of Hawaii and Maui around noon, and through the northwestern United States at sunset.
The eclipse will be visible over Indonesia and Pacific Ocean west of the International Date Line, on the morning of Thursday, March 11, 2100, and the Pacific Ocean east of International Date Line and North America on the afternoon of Wednesday, March 10, 2100. The path of annularity will be visible in those locations.
Related eclipses[edit]
Eclipses in 2100[edit]
- A penumbral lunar eclipse on February 24, 2100.
- An annular solar eclipse on March 10, 2100.
- A penumbral lunar eclipse on August 19, 2100.
- A total solar eclipse on September 4, 2100.
Metonic[edit]
- Preceded by: Solar eclipse of May 22, 2096
- Followed by: Solar eclipse of December 29, 2103
Tzolkinex[edit]
- Preceded by: Solar eclipse of January 27, 2093
- Followed by: Solar eclipse of April 23, 2107
Half-Saros[edit]
- Preceded by: Lunar eclipse of March 5, 2091
- Followed by: Lunar eclipse of March 17, 2109
Tritos[edit]
- Preceded by: Solar eclipse of April 10, 2089
- Followed by: Solar eclipse of February 8, 2111
Solar Saros 141[edit]
- Preceded by: Solar eclipse of February 27, 2082
- Followed by: Solar eclipse of March 22, 2118
Inex[edit]
- Preceded by: Solar eclipse of March 31, 2071
- Followed by: Solar eclipse of February 18, 2129
Triad[edit]
- Preceded by: Solar eclipse of May 10, 2013
- Followed by: Solar eclipse of January 9, 2187
Solar eclipses of 2098–2101[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 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 141[edit]
This eclipse is a part of Saros series 141, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2640. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on June 13, 2857. 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 20 at 12 minutes, 9 seconds on December 14, 1955. All eclipses in this series occur at the Moon’s ascending node of orbit.[2]
Series members 12–33 occur between 1801 and 2200: | ||
---|---|---|
12 | 13 | 14 |
![]() September 17, 1811 |
![]() September 28, 1829 |
![]() October 9, 1847 |
15 | 16 | 17 |
![]() October 19, 1865 |
![]() October 30, 1883 |
![]() November 11, 1901 |
18 | 19 | 20 |
![]() November 22, 1919 |
![]() December 2, 1937 |
![]() December 14, 1955 |
21 | 22 | 23 |
![]() December 24, 1973 |
![]() January 4, 1992 |
![]() January 15, 2010 |
24 | 25 | 26 |
![]() January 26, 2028 |
![]() February 5, 2046 |
![]() February 17, 2064 |
27 | 28 | 29 |
![]() February 27, 2082 |
![]() March 10, 2100 |
![]() March 22, 2118 |
30 | 31 | 32 |
![]() April 1, 2136 |
![]() April 12, 2154 |
![]() April 23, 2172 |
33 | ||
![]() May 4, 2190 |
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 9, 1926 (Saros 135) |
![]() June 20, 1955 (Saros 136) |
![]() May 30, 1984 (Saros 137) |
![]() May 10, 2013 (Saros 138) |
![]() April 20, 2042 (Saros 139) |
![]() March 31, 2071 (Saros 140) |
![]() March 10, 2100 (Saros 141) |
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 141". eclipse.gsfc.nasa.gov.
External links[edit]
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC