Solar eclipse of September 12, 1950

A total solar eclipse occurred on September 12, 1950. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible from eastern Soviet Union (today's Russia) and the whole Semichi Islands in Alaska.

Solar eclipse of September 12, 1950
Map
Type of eclipse
NatureTotal
Gamma0.8903
Magnitude1.0182
Maximum eclipse
Duration74 sec (1 m 14 s)
Coordinates54.8°N 172.3°E / 54.8; 172.3
Max. width of band134 km (83 mi)
Times (UTC)
Greatest eclipse3:38:47
References
Saros124 (51 of 73)
Catalog # (SE5000)9399

Solar eclipses of 1950–1953

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]

Saros 124

Solar saros 124, repeating every about 18 years and 11 days, contains 73 events. The series started with partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211, to September 22, 1968, and a hybrid solar eclipse on October 3, 1986. The series ends at member 73 as a partial eclipse on May 11, 2347. The longest total eclipse occurred on May 3, 1734, at 5 minutes and 46 seconds.[2]

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

Notes

  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.
gollark: https://media.discordapp.net/attachments/629419596428083210/777242606102380574/unknown.png?width=427&height=422
gollark: You'd have to keep decreasing it for every repost though.
gollark: I didn't. Depending on how it gets split into blocks or something it might work.
gollark: Based on something or other it runs on perceptual hashes which use a discrete cosine transform thingy, so it might be easiest to DCT the image data, fiddle with the parameters a bit, and convert it back.
gollark: I should really work on trying to evade meme repost detection again. I think I determined that rotation past about 15 degrees got around it but was very obvious, and adding small amounts of noise didn't.

References

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.