Template:Solar eclipse set 2011–2014
Appearance
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 eclipses on January 4, 2011 and July 1, 2011 occur in the previous lunar year eclipse set.
Solar eclipse series sets from 2011 to 2014 | ||||||
---|---|---|---|---|---|---|
Descending node | Ascending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
118![]() Partial in Tromsø, Norway |
June 1, 2011![]() Partial |
1.21300 | 123![]() Hinode XRT footage |
November 25, 2011![]() Partial |
−1.05359 | |
128![]() Annularity in Red Bluff, CA, USA |
May 20, 2012![]() Annular |
0.48279 | 133![]() Totality in Mount Carbine, Queensland, Australia |
November 13, 2012![]() Total |
−0.37189 | |
138 Annularity in Churchills Head, Australia |
May 10, 2013![]() Annular |
−0.26937 | 143 Partial in Libreville, Gabon |
November 3, 2013![]() Hybrid |
0.32715 | |
148![]() Partial in Adelaide, Australia |
April 29, 2014![]() Annular (non-central) |
−0.99996 | 153![]() Partial in Minneapolis, MN, USA |
October 23, 2014![]() Partial |
1.09078 |
- ^ 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.