Template:Solar eclipse set 2008–2011
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 June 1, 2011 and November 25, 2011 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2008 to 2011 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
121![]() Partial in Christchurch, New Zealand |
February 7, 2008![]() Annular |
−0.95701 | 126![]() Totality in Kumul, Xinjiang, China |
August 1, 2008![]() Total |
0.83070 | |
131![]() Annularity in Palangka Raya, Indonesia |
January 26, 2009![]() Annular |
−0.28197 | 136![]() Totality in Kurigram District, Bangladesh |
July 22, 2009![]() Total |
0.06977 | |
141![]() Annularity in Jinan, Shandong, China |
January 15, 2010![]() Annular |
0.40016 | 146 Totality in Hao, French Polynesia |
July 11, 2010![]() Total |
−0.67877 | |
151![]() Partial in Poland |
January 4, 2011![]() Partial |
1.06265 | 156 | July 1, 2001![]() Partial |
−1.49171 |
- ^ 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.