Solar eclipse of April 29, 1976
Introduction An annular solar eclipse occurred at the Moon's descending node of the orbit on Thursday, 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.Annularity 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.
Observation The Institute of Physics and Institute of Mathematics of the Chinese Academy of Sciences and the Xinjiang Earthquake Team conducted observations of gravitational effects using gravimeters, inclinometers, pendulum clocks and seismometers in southwestern Hotan County, Hotan Prefecture, Xinjiang near the Karakoram Pass at an altitude of . Results showed that the gravitational acceleration had no obvious effect within the accuracy of the instruments. No inclination was recorded on the photosensitive paper of the inclinometer due to the width of its lines. Three inclinations were pen-recorded, whose time and direction were clearly related to that of the eclipse. Due to the difficult conditions with the high altitude, the observation team was unable to obtain more comparative data.
Related eclipses === Eclipses in 1976 ===* An annular solar eclipse on Thursday, 29 April 1976. * A partial lunar eclipse on Thursday, 13 May 1976. * A total solar eclipse on Saturday, 23 October 1976. * A penumbral lunar eclipse on Saturday, 6 November 1976.=== Solar eclipses of 1975–1978 ====== Saros 128 ====== Metonic series===
Notes
References *  Solar eclipse of April 29, 1976 in Russia