Solar eclipse of March 10, 2100

Future annular solar eclipse
12°00′N 162°24′W / 12°N 162.4°W / 12; -162.4Max. width of band257 km (160 mi)Times (UTC)Greatest eclipse22:28:11ReferencesSaros141 (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

Eclipses in 2100

Metonic

Tzolkinex

Half-Saros

  • Preceded by: Lunar eclipse of March 5, 2091
  • Followed by: Lunar eclipse of March 17, 2109

Tritos

Solar Saros 141

Inex

Triad

Solar eclipses of 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]

Solar eclipses 2098–2100
121 April 1, 2098

Partial
126 September 25, 2098

Partial
131 March 21, 2099

Annular
136 September 14, 2099

Total
141 March 10, 2100

Annular
146 September 4, 2100

Total

Saros 141

Solar saros 141, repeating every about 18 years, 11 days, and 8 hours, contains 70 events. The series started with partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739, to October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. The longest annular eclipse occurred on December 14, 1955, with maximum duration of annularity at 12 minutes and 9 seconds. All eclipses in this series occur at the Moon’s ascending node.[2]

Series members 17–36 occur between 1901 and 2259
17 18 19

November 11, 1901

November 22, 1919

December 2, 1937
20 21 22

December 14, 1955

December 24, 1973

January 4, 1992
23 24 25

January 15, 2010

January 26, 2028

February 5, 2046
26 27 28

February 17, 2064

February 27, 2082

March 10, 2100
29 30 31

March 22, 2118

April 1, 2136

April 12, 2154
32 33 34

April 23, 2172

May 4, 2190

May 15, 2208
35 36

May 27, 2226

June 6, 2244

Inex series

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

  1. ^ 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.
  2. ^ Saros Series Catalog of Solar Eclipses NASA Eclipse Web Site.

External links

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements
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