Epsilon Cephei

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Epsilon Cephei

A visual band light curve for Epsilon Cephei, adapted from Bruntt et al. (2007)[1]
Observation data
ICRS
)
Constellation Cepheus
Right ascension 22h 15m 02.19530s[2]
Declination +57° 02′ 36.8771″[2]
Apparent magnitude (V) 4.15 - 4.21[3]
Characteristics
Spectral type F0 V (Sr II)[4] or F0 IV[5]
U−B color index +0.073[6]
B−V color index +0.277[6]
Variable type δ Sct[3]
Distance
85 ± 2 ly
(26.2 ± 0.7 pc)
Absolute magnitude (MV)+2.13[8]
Details
ε Cep Aa
Gyr
ε Cep Ab
Mass0.57[12] M
HIP 109857, HR 8494, SAO 34227[13]
Database references
SIMBADdata

Epsilon Cephei,

apparent visual magnitude of 4.18.[6]

Properties

Physical Characteristics

This is a yellow-white hued,

AU. This dust has a combined mass equal to 6.6% of the Earth's mass.[10]

Binary

There is a faint companion star at an

AU. The probability of a random star being situated this close to Epsilon Cephei is about one in a million, so it is most likely physically associated. If so, then the debris disk is probably circumbinary. The fact that this companion was not detected during the Hipparcos mission may indicate its orbit has a high eccentricity. The companion star has a K-band magnitude of 7.8 and is probably of class K8–M2.[5]

Naming

In

Chinese name for ε Cephei itself is 螣蛇九 (Téng Shé jiǔ, English: the Ninth Star of Flying Serpent)[14]

References