Eclipses

Overview

An eclipse is when one celestial object casts a shadow on another. They occur during the alignment of three bodies in space, known as a syzygy, in which one body blocks light from a second body from reaching the third. On Earth, this is most commonly associated with the moon blocking the sun—a solar eclipse—and the Earth blocking sunlight from reaching the moon—a lunar eclipse.

Once considered a bad omen linked to a displeased sun god or to the attempted destruction of the sun, the term "eclipse" derives from a Greek word meaning "to forsake." By the fifth century BCE, patterns in the frequency of eclipses and the motions of the sun and moon allowed ancient astronomers to predict future occurrences. These events were used to demonstrate that the Earth was round and to determine the size of and distance to the moon more than two millennia ago.

Since then, eclipses have led to improved understanding of the sun's corona, or outer atmosphere, the discovery of helium, and the validation of general relativity. Analyses of blocked starlight from beyond the solar system have contributed to the discovery of binary star systems—pairs of orbiting stars—and almost three-quarters of known exoplanets.

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