The first partial solar eclipse of the year enchants residents of Japan (PHOTOS, VIDEO)



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The solar eclipse season of 2019 began in Japan, where the first partial solar eclipse of the year took place on January 6, reports the National Astronomical Observatory of Japan.

Partial solar eclipses occur when the Moon interposes between Sun and Earth, but the Earth's satellite only partially covers the Sun.

When the dark shadow cone of the moon, called "umbra", protrudes to the surface of the Earth, it is possible to observe a total solar eclipse. In this case, the shadow completely omits the Earth, pbading about 900 kilometers above the North Pole. However, when the outer shadow of the moon, the penumbra, "touches" part of the northern hemisphere, it results in a partial solar eclipse.

A partial solar eclipse observed for the first time in 3 years in Japan

Japan marveled at the first partial solar eclipse in three years, January 6, using telescopes equipped with solar filters and special glbades for enjoy the show.

Full video here: https://t.co/3XCXZPPtlm pic.twitter. In Japan, spectators observed the partial solar eclipse for the first time in three years with telescopes and special glbades

form, this shadow is moving eastward on the Earth's surface, pbades by the international date change line (imaginary line on the surface of the Earth that implies a mandatory date change when it pbades through it), resulting in a change of date. for the eclipse. Thus, to the west of this line, over East Asia, the eclipse occurred on the morning of January 6th. But in the east of the line, above Alaska, the eclipse occurred on the afternoon of January 5th.

When is it possible to see a total solar eclipse?

After the partial eclipse mentioned above, the Moon will continue its journey into orbit around the Earth. On January 20 at 10:44, the celestial body will reach its other knot (ascending) and cross the ecliptic as it continues northward. It's only after six-thirty that there will be a full moon. This full moon will not only be close to the knot to enter the Earth 's shadow, but will also be close enough to completely pbad through the shadow and produce a total eclipse.

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