Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Octans |
Right ascension | 22h 50m 22.8139s[1] |
Declination | −80° 07′ 25.8418″[1] |
Apparent magnitude (V) | 5.32 - 5.36[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | B6 V[4] (B5/7 V)[5] |
U−B color index | −0.48[6][7] |
B−V color index | −0.13[6] |
Variable type | SPB[8] |
Astrometry | |
Radial velocity (Rv) | 22.1±0.5[9] km/s |
Proper motion (μ) | RA: +20.003 mas/yr[1] Dec.: −12.607 mas/yr[1] |
Parallax (π) | 6.35 ± 0.0644 mas[1] |
Distance | 514 ± 5 ly (157 ± 2 pc) |
Absolute magnitude (MV) | −0.57[10] |
Details | |
Mass | 4.02±0.05[3] M☉ |
Radius | 3.0±0.5[11] R☉ |
Luminosity | 360+24 −22[3] L☉ |
Surface gravity (log g) | 4.09[11] cgs |
Temperature | 14,050[12] K |
Metallicity [Fe/H] | −0.1[12] dex |
Rotational velocity (v sin i) | 30[13] km/s |
Age | 46+25 −16[14] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Xi Octantis, Latinized from ξ Octantis, is a solitary[17] variable star in the southern circumpolar constellation Octans. It has an apparent magnitude of about 5.3, allowing it to be faintly seen with the naked eye; however, this varies slightly. Located 514 light years away, the object is receding with a heliocentric radial velocity of 22 km/s.
Xi Octantis has a stellar classification of B6 V,[4] indicating that it is an ordinary B-type main-sequence star. Hintler et al. gives it a luminosity class IV (subgiant)[19] while Houk and Cowley gives a classification intermediate between a B5 and B7 dwarf.[5] Nevertheless, it has 4 times the mass of the Sun[3] and is 3 times larger.[11] It shines with a luminosity of 360 L☉[3] from its photosphere at an effective temperature of 14,050 K,[12] giving it a whitish blue glow. Xi Octantis is 46 million years old[14] – 64.8% through its short main sequence lifetime[12] – and spins modestly with a projected rotational velocity of 30 km/s.[13]
When the Hipparcos catalogue was released in 1997, Xi Octantis was found to vary in magnitude[20] — ranging from 5.32 to 5.36 based on data from the International Variable Star Index.[2] It has since been classified as a Slowly pulsating B-dwarf with a period of 1.78 days.[2]
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