SCIENCE DAILY
An artist’s concept depicts a dense, dead star called a white dwarf crossing in front of a small, red star. The white dwarf’s gravity is so great that it bends and magnifies light from the red star, causing it to appear bigger than it really is. CREDIT/NASA/JPL-Caltech)
NASA’s Kepler space telescope, in concert with Cornell-led measurements of stars’ ultraviolet activity, has observed the effects of a dead star bending the light of its companion red star.
The findings are among the first detections of this effect — a result predicted by Einstein’s theory of general relativity — in binary, or double, star systems.
The dead star, also called a white dwarf, is the burnt-out core of what used to be a star like our sun. It is locked in an orbiting dance with its partner, a small “red dwarf” star. While the tiny white dwarf is physically smaller than the red dwarf, it is more massive. When the white dwarf passed in front of its star, its gravity caused the starlight to observably bend and brighten.
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