Astro Payyanur

The longest solar eclipse was watched by hundreds of people including school students at ASTRO observatory Payyanur. Even though clouds cast shadows over crowd gathered here till 6.45 am. Then the sun came out of clouds to show the cosmic drama of eclipse. ASTRO coordinator K Gangadharan Master gave class and instructions for the people gathered

For the second time in a year, a total eclipse of the Sun is about to cross China. But unlike the Moon's hard-to-reach shadow path last August, the celestial spectacle on July 22, 2009, will darken major cities, densely populated countryside, and a vast expanse of tropical ocean. And the eclipse itself will be a monster, with totality lasting more than 6.6 minutes at maximum. That makes this the longest totality until 2132.

A total solar eclipse occurs once every year or two on average, but each is visible only from a narrow track covering less than 1% of Earth’s surface. The eclipse of August 1, 2008, was visible only from parts of the Arctic, Siberia, and central Asia. Nevertheless, thousands of enthusiasts traveled by land, air, and polar icebreaker for the chance to bask briefly in the silvery twilight glow of the Sun’s corona.

The main reason why this year's totality lasts so long is because the eclipse starts just a few hours after the Moon reaches perigee. At such a close distance, the Moon appears fully 8% larger than the Sun and casts a broader than usual shadow. At the point of greatest eclipse in the western Pacific, the path of totality is 258 km (161 miles) wide.

The umbra (dark central portion) of the lunar shadow first touches Earth at sunrise at 00:53 Universal Time in the Gulf of Khambhat off western India. The shadow takes just 8 minutes to cross India before spilling into northern Bangladesh and easternmost Nepal. A minute later the umbra engulfs most of Bhutan, while the eclipse duration on the central line crosses the 4-minute mark. The Sun’s altitude is 21°.

The shadow then crosses northern Burma, a corner of Tibet, and China’s Yunnan province. Passing through the middle of Sichuan province, the eclipse track darkens the capital city of Chengdu (2 million inhabitants, 3.3 minutes of totality), Chongqing (4.1 million, 4 minutes), and Wuhan (9.7 million, 5.5 minutes). Traveling nearly due east, the shadow track encompasses the meandering course of the Yangtze River.

Near the Pacific coast, Hangzhou's 4 million citizens experience a total eclipse lasting 5.3 minutes. The Sun’s altitude is now 55°. A minute later Shanghai, China’s largest city with 20 million people, plunges into totality for 5 minutes, though it is well north of the central line. This may be the most people that have ever been in the Moon’s shadow at once.

As it moves out over the East China Sea, the umbra sweeps over Japan’s Ryukyu Islands, then Iwo Jima and Kitaio Jima, before curving southeast across the Pacific. The instant of greatest eclipse occurs at 2:35:19 UT, when totality lasts longest: 6 minutes 39 seconds. This happens over open ocean with no land in sight.

The second half of the eclipse path crosses nothing but ocean and a few tiny islands and coral atolls among the Marshall Islands and Kiribati. The total eclipse finally ends at 4:18 UT, at sunset about 1,000 km northwest of Tahiti. The Moon’s shadow lifts off Earth and returns to space, after covering 0.7% of Earth’s surface in 3.4 hours.

Future Total Eclipses

On July 11, 2010, this part of the world will be favored with its third total solar eclipse in as many years. The track is almost entirely over the South Pacific. Easter Island and southern Chile (at sunset) offer the only landfalls. And the South Pacific also hosts the next one, on November 13, 2012.

A total solar eclipse won’t cross the Americas until August 21, 2017, when the Moon’s umbra will sweep from Oregon to South Carolina.

Annular Solar Eclipse of January 26

The first solar eclipse of 2009 occurs at the Moon's ascending node in western Capricornus. An annular eclipse will be visible from a wide track that traverses the Indian Ocean and western Indonesia. A partial eclipse will be seen within the much larger path of the Moon's penumbral shadow, which includes the southern third of Africa, Madagascar, Australia except Tasmania, southeast India, Southeast Asia and Indonesia. (Figure 1).

The annular path begins in the South Atlantic at 06:06 UT when the Moon's antumbral shadow meets Earth and forms a 363 kilometre wide corridor. Traveling eastward, the shadow quickly sweeps south of the African continent, missing it by approximately 900 kilometres. Slowly curving to the northeast the path crosses the southern Indian Ocean. Greatest eclipse[1] takes place at 07:58:39 UT when the eclipse magnitude[2] will reach 0.9282. At this instant, the annular duration is 7 minutes 54 seconds, the path width is 280 kilometres and the Sun is 73° above the flat horizon formed by the open ocean. The central track continues northeast where it finally encounters land in the form of the Cocos Islands and onward to southern Sumatra and western Java (Figure 2). At 09:40 UT, the central line duration is 6 minutes 18 seconds and the Sun's altitude at 25°. In its final minutes, the antumbral shadow cuts across central Borneo and clips the northwestern edge of Celebes before ending just short of Mindanao, Philippines at 09:52 UT. During a 3 hour 46 minute trajectory across our planet, the Moon's antumbra travels approximately 14,500 kilometres and covers 0.9% of Earth's surface area. Path coordinates and central line circumstances are presented in Table 1.

Partial phases of the eclipse are visible primarily from southern Africa, Australia, Southeast Asia and Indonesia. Local circumstances for a number of cities are listed in Table 2. All times are given in Universal Time. The Sun's altitude and azimuth, the eclipse magnitude and obscuration[3] are all given at the instant of maximum eclipse.

This is the 50th eclipse of Saros 131. The family began with an unusually long series of 22 partial eclipses starting on 1125 Aug 01. The first central eclipse was total in the Northern Hemisphere on 1522 Mar 27. It was followed by 5 more total eclipses before the series produce 5 hybrid eclipses from 1630 to 1702. The first annular eclipse of Saros 131 occurred on 1720 Aug 04. The series will produce 29 more annular eclipses the last of which is 2243 Jun 18. Saros 131 terminates on 2369 Sep 02 after a string of 7 partial eclipses. Complete details for 70 eclipses in the series may be found at: