11 Camelopardalis

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**11 Camelopardalis**
Observation data Equinox J2000.0
Constellation	Camelopardalis
Right ascension	05^h06^m08.5^s
Declination	+58°58′21″
Apparent magnitude (V)	+5.22
Absolute magnitude (V)	-1.35
Distance	671 ± 104 ly (206 ± 32 pc)
Spectral type	B2.5Ve
Other designations
BV Camelopardalis, HR 1622, HD 32343, BD+58°804, HIP 23734, SAO 25001, GC 6193, BDS 2480, CCDM 05062+5900

11 Camelopardalis is a star system in the constellation Camelopardalis. It forms a double star with 12 Camelopardalis, which is only 3 arcminutes away.

11 Camelopardalis is a blue-white B-type main sequence dwarf with a mean apparent magnitude of +5.22. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies by 0.07 magnitudes with a period of a few hours. It is approximately 671 light years from Earth.

This variable star–related article is a stub. You can help Wikipedia by expanding it.

Retrieved from "http://en.wikipedia.org../../../1/1/_/11_Camelopardalis_459b.html"

Categories: Variable star stubs | Flamsteed objects | Camelopardalis constellation | Blue-white dwarfs | Double stars | Gamma Cassiopeiae variables

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