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Alpha Pyxidis

Alpha Pyxidis
Diagram showing star positions and boundaries of the Pyxis constellation and its surroundings
Cercle rouge 100%.svg

Location of α Pyxidis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Pyxis
Right ascension 08h 43m 35.53756s
Declination –33° 11′ 10.9898″
Apparent magnitude (V) 3.67
Characteristics
Spectral type B1.5III
U−B color index –0.84
B−V color index –0.19
Variable type Beta Cephei
Astrometry
Radial velocity (Rv) +15.3 km/s
Proper motion (μ) RA: –14.27 mas/yr
Dec.: +10.43 mas/yr
Parallax (π) 3.71 ± 0.14mas
Distance 880 ± 30 ly
(270 ± 10 pc)
Details
Mass 10.7 M
Radius 6.3 ± 1.0 R
Luminosity 10,000 L
Surface gravity (log g) 3.63 cgs
Temperature 24,300 K
Metallicity [Fe/H] -0.18 dex
Rotational velocity (v sin i) 11 km/s
Other designations
α Pyxidis, CPD−32° 2399, FK5 327, HD 74575, HIP 42828, HR 3468, SAO 199546.
Database references
SIMBAD data

Alpha Pyxidis (Alpha Pyx, α Pyxidis, α Pyx) is a giant star in the constellation Pyxis. It has a stellar classification of B1.5III and is a Beta Cephei variable. This star has more than ten times the mass of the Sun and is more than six times the Sun's radius. The surface temperature is 24,300 K and the star is about 10,000 times as luminous as the Sun. Stars such as this with more than 10 solar masses are expected to end their life by exploding as a supernova.

In Chinese, 天狗 (Tiān Gǒu), meaning Celestial Dog, refers to an asterism consisting of α Pyxidis, e Velorum, f Velorum, β Pyxidis, γ Pyxidis and δ Pyxidis. Consequently, α Pyxidis itself is known as 天狗五 (Tiān Gǒu wǔ, English: the Fifth Star of Celestial Dog.)


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Wikipedia

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