Solar eclipse of January 15, 2010 | |
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Annularity from Bangui, Central African Republic |
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![]() Map
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Type of eclipse | |
Nature | Annular |
Gamma | 0.4002 |
Magnitude | 0.919 |
Maximum eclipse | |
Duration | 11m 8s |
Coordinates | 1.6N 69.3E |
Max. width of band | 333 km |
Times (UTC) | |
(P1) Partial begin | 4:05:28 |
(U1) Total begin | 5:13:55 |
Greatest eclipse | 7:07:39 |
(U4) Total end | 8:59:04 |
(P4) Partial end | 10:07:35 |
References | |
Saros | 141 (23 of 70) |
Catalog # (SE5000) | 9529 |
The solar eclipse of January 15, 2010 was an annular eclipse of the Sun with a magnitude of 0.9190. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially obscuring Earth's view of the Sun. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun, causing the sun to look like an annulus (ring), blocking most of the Sun's light. An annular eclipse appears as a partial eclipse over a region thousands of kilometres wide.
It was the longest annular solar eclipse of the millennium,[1] and the longest until December 23, 3043, with a maximum length of 11 mins and 7.8 seconds. (The solar eclipse of January 4, 1992, was longer, at 11 minutes, 41 seconds, occurring in the middle of the Pacific Ocean.)[2]
The eclipse was visible as only a partial eclipse in much of Africa, Eastern Europe, the Middle East and Asia. It was seen as an annular eclipse within a narrow stretch of 300 km (190 mi) width across Central Africa, Maldives, South Kerala (India), South Tamil Nadu (India), Sri Lanka and parts of Bangladesh, Burma and China.
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The eclipse started in the Central African Republic, traversed Cameroon, DR Congo and Uganda, passed through Nairobi, Kenya, and passed over the Indian Ocean, where it reached its greatest visibility. It then entered Maldives, where it was the longest on land with 10.8 viewable minutes. The annular eclipse at Malé, the capital city of Maldives, started at 12:20:20 and ended at 12:30:06 Maldives local time (UTC+5). This was also the longest duration of any eclipse with an international airport in its track.[3]
At approximately 13:20 IST, the annular solar eclipse entered India at Thiruvananthapuram (Trivandrum), Kerala and exited India at Rameswaram, Tamil Nadu.
The eclipse was viewable for 10.4 minutes in India. After Rameswaram, it entered Sri Lanka at Delft Island, exited at Jaffna in Sri Lanka, crossed the Bay of Bengal and re-entered India in Mizoram.
Thiruvananthapuram, which was the entry point of the eclipse in India, was equipped with telescopes and announced facilities for the public to view the eclipse.[4] Vikram Sarabhai Space Centre, situated in Trivandrum, analysed the atmospheric-ionospheric parameters during the eclipse.[5] Many scientists camped in the city to witness and study the eclipse.[6]
At Rameswaram, the sunrise was not visible due to thick clouds, but it started getting clear at around 9 AM local time and became almost totally clear by the time the eclipse began. The sky had a thin layer of cirrus clouds till 2:30PM. Among the eclipse-watchers was Sky Watchers' Association of North Bengal (SWAN) from Siliguri at the foothills of West Bengal and Tamilnadu Astronomical Association.
Dhanushkodi, which falls on the central line of the eclipse, was a good place to view the eclipse. The northernmost limit of shadow in India was Cuddalore, Neyveli, Erode, Kodaikanal, and Madurai. Other prime viewing locations in Tamil Nadu include Thoothukudi and Cape Comorin, 22 km north of the center line. The exact location of the line is between the NH end and the Dhanushkodi ruins. Dhanushkodi is about 2 km east of the central line. The degree difference is about 0.2 between the central line – with Kodandaramar Temple and Dhanushkodi ruins vice versa. Dhanushkodi is about 5 km from the Kodandaramar Temple.
After South Asia, annularity passed Myanmar and China before leaving the Earth.
![]() Eclipse taken at Jaffna Hindu College, Jaffna District, Sri Lanka. |
![]() Eclipse taken against the Jaffna Public Library, Jaffna District, Sri Lanka. |
![]() Eclipse taken against the Nallur Kandaswamy temple, Jaffna District, Sri Lanka. |
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![]() Animation of path |
![]() Stages of solar eclipse in Thiruvananthapuram (Trivandrum), India. |
![]() Photograph of the eclipse seen from India |
The eclipse from Degania A, Israel, 05:41 UT |
![]() Montage of the eclipse from Degania A, Israel, from 05:03 UT to 07:05 UT |
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![]() Photograph of the ending stages of the eclipse as seen from Chennai |
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![]() Photograph of Partial Stage from Pallipalayam, Tamilnadu, India. |
![]() Reflection of Solar Eclipse on floor due to holes at roof in palliapalayam, Tamilnadu, India. |
![]() Satellite image of the Moon's shadow falling on India and the Bay of Bengal. |
This set of solar eclipses repeat approximately every 177 days and 4 hours at alternating nodes of the moon's orbit.
Ascending node | Descending node | |||||
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Saros | Map | Saros | Map | |||
121![]() Partial from New Zealand |
2008 February 7![]() Annular |
126![]() Total from Russia |
2008 August 1![]() Total |
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131![]() Bandar Lampung, Indonesia |
2009 January 26![]() Annular |
136![]() Total from Bangladesh |
2009 July 22![]() Total |
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141 Bangui, Central African Republic |
2010 January 15![]() Annular |
146 Total from Easter Island |
2010 July 11![]() Total |
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151 | 2011 January 4![]() Partial (north) |
156 | 2011 July 1![]() Partial (south) |
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Partial solar eclipses on June 1, 2011 and November 25, 2011 occur on the next lunar year eclipse set. |
Solar Saros 141 repeats every 18 years, 11 days and contains 70 events. The series started with partial solar eclipse on May 19, 1613. It contains 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. [7]
Series members 17-28 occur between 1901 and 2100:
17 | 18 | 19 |
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![]() November 11, 1901 |
![]() November 22, 1919 |
![]() December 2, 1937 |
20 | 21 | 22 |
![]() December 14, 1955 |
![]() December 24, 1973 |
![]() January 4, 1992 |
23 | 24 | 25 |
![]() January 15, 2010 |
![]() January 26, 2028 |
![]() February 5, 2046 |
26 | 27 | 28 |
![]() February 17, 2064 |
![]() February 27, 2082 |
![]() March 10, 2100 |
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).
This series has 20 eclipse events between June 10, 1964 and August 21, 2036.
June 10-11 | March 27-29 | January 15-16 | November 3 | August 21-22 |
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117 | 119 | 121 | 123 | 125 |
![]() June 10, 1964 |
![]() March 28, 1968 |
![]() January 16, 1972 |
![]() November 3, 1975 |
![]() August 22, 1979 |
127 | 129 | 131 | 133 | 135 |
![]() June 11, 1983 |
![]() March 29, 1987 |
![]() January 15, 1991 |
![]() November 3, 1994 |
![]() August 22, 1998 |
137 | 139 | 141 | 143 | 145 |
![]() June 10, 2002 |
![]() March 29, 2006 |
![]() January 15, 2010 |
![]() November 3, 2013 |
![]() August 21, 2017 |
147 | 149 | 151 | 153 | 155 |
![]() June 10, 2021 |
![]() March 29, 2025 |
![]() January 14, 2029 |
![]() November 3, 2032 |
![]() August 21, 2036 |
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