Solar eclipse of January 15, 2010
An annular solar eclipse occurred on January 15, 2010 with a magnitude of 0.9190. 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. 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, 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. This is about 4 minutes longer than total solar eclipses could ever get.
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 width across Central Africa, Maldives, South Kerala, South Tamil Nadu, Sri Lanka and parts of Bangladesh, Burma and China.
The tables below contain detailed predictions and additional information on the Annular Solar Eclipse of January 15, 2010
Eclipse Magnitude: 0.91903Eclipse Obscuration: 0.84462
Gamma: 0.40016
Saros Series: 141st
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
Radius of the Antumbral Shadow: 361.7 km
Path Width: 333.1 km
Greatest Eclipse: 2010 January 15 at 07:06:33.2 UTC
Apogee at 2010 January 17 at 01:41 UTC
Event | UTC time |
First Penumbral External Contact | 2010 Jan 15 at 04:05:27.6 UTC |
First Umbral External Contact | 2010 Jan 15 at 05:13:55.0 UTC |
First Central Line | 2010 Jan 15 at 05:17:34.8 UTC |
First Umbral Internal Contact | 2010 Jan 15 at 05:21:15.9 UTC |
First Penumbral Internal Contact | 2010 Jan 15 at 06:50:06.9 UTC |
Greatest Eclipse | 2010 Jan 15 at 07:06:33.2 UTC |
Last Penumbral Internal Contact | 2010 Jan 15 at 07:22:37.8 UTC |
Last Umbral Internal Contact | 2010 Jan 15 at 08:51:40.5 UTC |
Last Central Line | 2010 Jan 15 at 08:55:22.8 UTC |
Last Umbral External Contact | 2010 Jan 15 at 08:59:03.9 UTC |
Last Penumbral External Contact | 2010 Jan 15 at 10:07:35.3 UTC |
Visibility of the eclipse
The eclipse started in the Central African Republic near the border with Chad, traversed DR Congo and Uganda, passed through Nairobi, Kenya, the northern tip of Tanzania, southwestern Somalia and three islands of Seychelles, 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. This was also the longest duration of any eclipse with an international airport in its track.At approximately 13:20 IST, the annular solar eclipse entered India at Thiruvananthapuram, the capital of 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.
, India where the eclipse was 94%
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. Vikram Sarabhai Space Centre, situated in Trivandrum, analysed the atmospheric-ionospheric parameters during the eclipse. Many scientists camped in the city to witness and study the eclipse.
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 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, annularity passed Myanmar and China before leaving the Earth.
Gallery
Related eclipses
Eclipses of 2010
- An annular solar eclipse on January 15.
- A partial lunar eclipse on June 26.
- A total solar eclipse on July 11.
- A total lunar eclipse on December 21.
Tzolkinex
- Preceded: Solar eclipse of December 4, 2002
- Followed: Solar eclipse of February 26, 2017
Half-Saros cycle
- Preceded: Lunar eclipse of January 9, 2001
- Followed: Lunar eclipse of January 21, 2019
Tritos
- Preceded: Solar eclipse of February 16, 1999
- Followed: Solar eclipse of December 14, 2020
Solar Saros 141
- Preceded: Solar eclipse of January 4, 1992
- Followed: Solar eclipse of January 26, 2028
Inex
- Preceded: Solar eclipse of February 4, 1981
- Followed: Solar eclipse of December 26, 2038
Triad
- Preceded: Solar eclipse of March 17, 1923
- Followed: Solar eclipse of November 15, 2096
Solar eclipses 2008–2011