Variable Stars

A variable star is a star whose brightness as seen from Earth changes with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are classified as either: • Intrinsic variables, whose luminosity actually changes; for example, because the star periodically swells and shrinks. • Extrinsic variables, whose apparent changes in brightness are due to changes in the amount of their light that can reach Earth; for example, because the star has an orbiting companion that sometimes eclipses it. Many, possibly most, stars have at least some variation in luminosity: the energy output of the Sun, for example, varies by about 0.1% over an 11-year solar cycle.

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Three new RR Lyrae variable stars discovered

Dozens of variable stars detected in the open cluster NGC 6611

Beautiful New Hubble Photo Shows Hot, Young Variable Stars in the Orion Nebula