Trichome

Solar eclipse of March 29, 1903
Map
Type of eclipse
NatureAnnular
Gamma0.8413
Magnitude0.9767
Maximum eclipse
Duration113 s (1 min 53 s)
Coordinates56°12′N 130°18′E / 56.2°N 130.3°E / 56.2; 130.3
Max. width of band153 km (95 mi)
Times (UTC)
Greatest eclipse1:35:23
References
Saros118 (62 of 72)
Catalog # (SE5000)9288

An annular solar eclipse occurred at the Moon's descending node of orbit on Sunday, March 29, 1903,[1][2] with a magnitude of 0.9767. 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. Annularity was visible from China (now northwestern China, Mongolia and northeastern China), Russia on March 29 (Sunday), and Northern Canada on March 28 (Saturday).

Related eclipses[edit]

Eclipses in 1903[edit]

Metonic[edit]

Tzolkinex[edit]

Half-Saros[edit]

Tritos[edit]

Solar Saros 118[edit]

Inex[edit]

Triad[edit]

Solar eclipses of 1902–1906[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.[3]

The partial solar eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1902 to 1906
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
108 April 8, 1902

Partial
1.5024 113 October 1, 1902
118 March 29, 1903

Annular
0.8413 123 September 21, 1903

Total
−0.8967
128 March 17, 1904

Annular
0.1299 133 September 9, 1904

Total
−0.1625
138 March 6, 1905

Annular
−0.5768 143
August 30, 1905

Total
0.5708
148 February 23, 1906

Partial
−1.2479 153 August 20, 1906

Partial
1.3731

Saros 118[edit]

This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit.[4]

Tritos series[edit]

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.

Notes[edit]

  1. ^ "Eclipse of the sun yesterday". Daily Leader. Davenport, Iowa. 1903-03-29. p. 5. Retrieved 2023-10-27 – via Newspapers.com.
  2. ^ "Annular Solar Eclipse". The Washington Times. Washington, District of Columbia. 1903-03-29. p. 4. Retrieved 2023-10-27 – via Newspapers.com.
  3. ^ 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.
  4. ^ "NASA - Catalog of Solar Eclipses of Saros 118". eclipse.gsfc.nasa.gov.

References[edit]


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