Cepheid variable
A Cepheid variable or Cepheid is a member of a particular class of variable stars, notable for a fairly tight correlation between their period of variability and absolute luminosity. The namesake and prototype of these variables is the star Delta Cephei, discovered to be variable by John Goodricke in 1784.
Related Topics:
Variable star - Delta Cephei - John Goodricke - 1784
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Because of this correlation (discovered by Henrietta Swan Leavitt in 1912), Cepheid variables can be used as a standard candle to determine the distance to their host clusters or galaxies. Since the period-luminosity relation can be calibrated with great precision using the nearest Cepheid stars, the distances found with this method are among the most accurate available.
Related Topics:
Henrietta Swan Leavitt - 1912 - Standard candle - Cluster - Galaxies
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~ Table of Content ~
| ► | Introduction |
| ► | Description |
| ► | Use as a "standard candle" |
| ► | Notes |
| ► | Examples |
| ► | See also |
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