An annular solar eclipse occurred at the Moon's ascending node of the orbit on January 15, 2010,^[1][2] with a magnitude of 0.91903. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. It was the longest annular solar eclipse of the millennium,^[3] and the longest until December 23, 3043, with the length of maximum eclipse of 11 minutes, 7.8 seconds, and the longest duration of 11 minutes, 10.7 seconds.^[4] This is about 4 minutes longer than total solar eclipses could ever get. (The solar eclipse of January 4, 1992, was longer, at 11 minutes, 40.9 seconds, occurring in the middle of the Pacific Ocean.)^[5]

Lasting 11 minutes and 7.8 seconds, and eclipse magnitude of only 0.91903, this was the longest and smallest annular solar eclipse of the 21st century. It was an annular solar eclipse on January 15, 2010.

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.

Eclipse Magnitude: 0.91903

Eclipse Obscuration: 0.84462

Gamma: 0.40016

Saros Series: 141st (23 of 70)

Sun Right Ascension: 19.8

Moon Right Ascension: 19.79

Sun Declination: -21.1

Moon Declination: -20.8

Sun Diameter: 1951.0 arcseconds

Moon Diameter: 1768.6 arcseconds

Radius of the Penumbral Shadow: 7,322.7 km (4,550.1 mi)

Radius of the Antumbral Shadow: 361.7 km (224.8 mi)

Path Width: 333.1 km (207 mi)

Greatest Eclipse: 2010 January 15 at 07:06:33.2 UTC

Apogee at 2010 January 17 at 01:41 UTC (406,433 km (252,546 mi))

The eclipse started in the Central African Republic near the border with Chad, traversed DR Congo, Uganda, Kenya, passed through the northern tip of Tanzania, southwestern Somalia and three islands of Seychelles (Bird, Denis and Aride), before it entered the Indian Ocean, where it reached its greatest visibility. It then passed through Maldives. The annular eclipse at Malé, the capital city of the country, started at 12:20:17 and ended at 12:31:02 local time (UTC+5), lasting for 10 minutes and 45 seconds (645 seconds). This was also the longest duration of any eclipse with an international airport in its track.^[6]

At approximately 13:20 IST, the annular solar eclipse entered India at Thiruvananthapuram (Trivandrum), the capital of Kerala and exited India at Rameswaram, Tamil Nadu.

The eclipse was viewable for 10 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.^[7] Vikram Sarabhai Space Centre, situated in Trivandrum, analysed the atmospheric-ionospheric parameters during the eclipse.^[8] Many scientists camped in the city to witness and study the eclipse.^[9]

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 2:30 pm. Among the eclipse-watchers was Sky Watchers' Association of North Bengal (SWAN) from Siliguri at the foothills of West Bengal and Tamil Nadu 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, the antumbra passed through the southern tip of Bangladesh, Myanmar and China before leaving the Earth.

• Photographic equipment may allow the planet Venus to be shown about 1.5 degrees west and south of the annular ring of the sun.
• Animation of path
• Satellite image showing the moon's antumbra falling over India and the Bay of Bengal
• Degania A, Israel, 5:41 UTC
• Bangalore, India, 7:20 UTC
• Jaffna, Sri Lanka, 7:56 UTC
• Sanda, Hyogo, 7:59 UTC
• Bandar Pusat Jengka, Malaysia, 8:05 UTC
• Akashi, Hyogo, 8:05 UTC
• Chennai, India, 8:10 UTC
• Reflection of the eclipse from Pallipalayam, India
• Stages of annular eclipse from Thiruvananthapuram, India
• Batticaloa, Sri Lanka, 8:28 UTC
• Hanoi, Vietnam, 8:36 UTC
• Central, Hong Kong, 8:40 UTC
• Bangui, Central African Republic
• Taichung, Taiwan, 9:19 UTC