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Pi
Variable starIts story
Pi Cassiopeiae is a double-lined spectroscopic binary: two stars packed so close that the spectrograph picks out both chemical signatures while they chase each other in a circular two-day orbit. That proximity distorts them: they are no longer spheres but ellipsoids whose apparent brightness shifts slightly as they spin, on a 23.57-hour cycle that is exactly half the orbital period. The pair lies 175 light-years away, on the southern edge of Cassiopeia's W.
- Constellation
- Cassiopeia
- Apparent magnitude
- 4.95
- Distance
- 175.1 light years
- Coordinates (J2000)
- RA 10.867° · Dec 47.025°
- Catalogue
- HIP 3414 · HD 4058
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