Kappa1 Apodis

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For other star systems with this Bayer designation, see Kappa Apodis.
Kappa1 Apodis
Diagram showing star positions and boundaries of the Apus constellation and its surroundings
Cercle rouge 100%.svg

Location of κ1 Apodis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Apus
Right ascension 15h 31m 30.82178s[1]
Declination −73° 23′ 22.5291″[1]
Apparent magnitude (V) 5.52[2]
Characteristics
Spectral type B1npe[3]
U−B color index -0.791[2]
B−V color index -0.128[2]
Variable type γ Cas[4]
Astrometry
Radial velocity (Rv) +62[5] km/s
Proper motion (μ) RA: +0.56[1] mas/yr
Dec.: -18.40[1] mas/yr
Parallax (π) 2.63 ± 0.27[1] mas
Distance approx. 1,200 ly
(approx. 380 pc)
Details
Mass 12.0 ± 0.3[6] M
Surface gravity (log g) 3.90[7] cgs
Temperature 21,500[7] K
Age 5.6 ± 1.0[6] Myr
Other designations
CD−72°1139, CPD−72°1802, FK5 567, HD 137387, HIP 76013, HR 5730, SAO 257289.[8]

Kappa1 Apodis is the Bayer designation for a binary star[3] system in the southern circumpolar constellation of Apus. Based upon parallax measurements, it is located roughly 1,200 light-years (370 parsecs) from Earth. The combined apparent visual magnitude of the system is 5.52,[2] indicating that this is a faint, naked eye star that can be viewed in dark suburban skies.

This is a spectroscopic binary system with an orbital period of 0.6 days.[3] The combined spectrum matches a stellar classification of B1npe.[3] The 'e' suffix indicates that this is a Be star with emission lines in the spectrum. An 'n' means that the absorption lines in the spectrum are broadened from the Doppler effect as a result of rapid rotation. Finally, the 'p' shows some peculiarity in the spectrum. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +5.43 to +5.61.

This is a runaway star with a peculiar velocity of 69.8 ± 4.7 km/s.[6] Because it is a binary star system, it was most likely not turned into a runaway system as the result of a supernova explosion.[3] A companion star is a 12th magnitude orange K-type subgiant located at an angular separation of 27 arcseconds.

References

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External links