| 词条 | Solar eclipse of April 29, 1976 |
| 释义 |
An annular solar eclipse occurred on April 29, 1976. 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. Totality was visible from North Africa, Greece, Turkey, Middle East, central Asia, India, China. 5 of the 14 eight-thousanders in Pakistan and China—Nanga Parbat, K2, Broad Peak, Gasherbrum II and Gasherbrum I, lie in the path of annularity. Related eclipsesSolar eclipses of 1975-1978{{Solar eclipse set 1975-1978}}Saros 128{{Solar Saros series 128}}Metonic series{{Solar Metonic series 2002 December 4}}NotessReferences{{Solar eclipse NASA reference|1951/SE1976Apr29A|19760429}}
4 : Annular solar eclipses|1976 in science|20th-century solar eclipses|April 1976 events |
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