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Saros cycle 140 - Information and visualization
{{Solar eclipses Solar saros series
Saros cycle
The saros () is a period of exactly 223 synodic months, approximately 6585.3211 days, or 18 years, 10, 11, or 12 days (depending on the number of leap years), and 8 hours, that can be used to predict eclipses of the Sun and Moon. One saros period ...
series 141 for solar eclipse
A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of the Earth, totally or partially. Such an alignment occurs during an eclipse season, approximately every six month ...
s occurs at the Moon's ascending node, repeats every 18 years, 11 days and contains 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739 through 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. All eclipses in this series occurs at the Moon's ascending node.
Longest Annular Solar Eclipse: Annular Solar Eclipse on Wednesday, December 14, 1955 - 12 minutes, 9 seconds
Smallest Annular Solar Eclipse: Annular Solar Eclipse on Monday, December 24, 1973 - Magnitude: 0.9174
This solar saros is linked to Lunar Saros 134
Saros cycle series 134 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events.
This lunar saros is linked to Solar Saros 141.
See also
* List of lunar eclipses
** List of Saros series for lunar ...
.
Umbral eclipses
Umbral eclipses can be classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 141 appears in the following table.Events
Notes
References
* http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros141.htmlExternal links
Saros cycle 140 - Information and visualization
{{Solar eclipses Solar saros series