Delta Cephei
 |
Delta Cephei. Image: © T. Credner & S. Kohle,
AlltheSky.com |
The second Cepheid variable to
be identified and the prototype for the category known as Type I
Cepheids, or Delta Cephei stars.
With a change in apparent magnitude of 3.5 to 4.4 over a period of 5.366
days, Delta Cep's entire range of variability can be followed with the naked
eye.
At a declination of +58°, Delta makes a perfect target for northern
observers, especially those who see Cepheus
as a circumpolar constellation. Also, it lies conveniently between two bright
stars that shine close to each end of its range of variability: Zeta Cep
(magnitude 3.6) and Epsilon Cep (magnitude 4.2). For those observing with
binoculars or a modest telescope, Delta Cep's companion stars can be discerned.
A seventh magnitude mate is located 41" from the variable itself and is
thought to be physically associated with it. A second nearby star of 13th
magnitude, located 20.9" from Delta, is most likely a line-of-sight object.
| visual magnitude |
4.07 (mean) |
| absolute magnitude |
-3.47 |
| spectral type |
G2Ib |
| temperature |
5,500–6,800 K |
| luminosity |
2,000 Lsun |
| mass |
5 Msun |
| distance |
890 light-years (273 pc) |
| position |
R.A. 22h 29m 12s,
Dec. +58° 25' 08" |
| other designations |
27 Cep, HR 8571, BD +57°2548,
HD 213306, SAO 34508, FK5 847,
AAVSO 2225+57, IRAS 22273+5809,
HIP 110991 |
Related categories
NOTABLE
STARS VARIABLE
STARS
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