Pi Puppis

For meteor shower appearing in the region of this star, see Pi Puppids.
Pi Puppis
Diagram showing star positions and boundaries of the Puppis constellation and its surroundings
Location of π Puppis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 17m 08.55678s[1]
Declination −37° 05′ 50.8962″[1]
Apparent magnitude (V) 2.733[2]
Characteristics
Spectral type K3 Ib[3]
U−B color index +1.238[2]
B−V color index +1.608[2]
Variable type SRd[4]
Astrometry
Radial velocity (Rv)+15.8[5] km/s
Proper motion (μ) RA: −10.05[1] mas/yr
Dec.: +6.47[1] mas/yr
Parallax (π)4.04 ± 0.33 mas[1]
Distance810 ± 70 ly
(250 ± 20 pc)
Absolute magnitude (MV)−4.5[6]
Details
Mass11.7±0.2[7] M☉
Radius235[8] R☉
Luminosity11,378[8] L☉
Surface gravity (log g)0.13[8] cgs
Temperature3,990–4,055[9] K
Age20.0±3.9[7] Myr
Other designations
π Pup, CPD−36°1211, FK5 278, GC 9706, HD 56855, HIP 35264, HR 2773, SAO 197795, PPM 283747, CCDM J07171-3706A, WDS J07171-3706A[10]
Database references
SIMBADdata

Pi Puppis, Latinized from π Puppis, also named Ahadi,[11][12] is the second-brightest star in the southern constellation of Puppis. It has an apparent visual magnitude of 2.733, so it can be viewed with the naked eye at night. Parallax measurements yield an estimated distance of roughly 810 light-years (250 parsecs) from the Earth. This is a double star with a magnitude 6.86 companion at an angular separation of 0.72 arcsecond and a position angle of 148° from the brighter primary.[13]

A light curve for Pi Puppis, plotted from Hipparcos data,[14] folded with the period derived by Koen and Eyer (2002)[15]

The spectrum of Pi Puppis matches a stellar classification of K3 Ib.[3] The Ib luminosity class indicates this a lower luminosity supergiant star that has consumed the hydrogen fuel at its core, evolved away from the main sequence, and expanded to about 235 times the Sun's radius. The effective temperature of the star's outer envelope is approximately 4,000 K,[9] which gives it the orange hue of a K-type star.[16] With a mass 11.7[7] times that of the Sun, this is a short-lived star with an estimated age of 20 million years.[7]

It is a semiregular variable star[4] that varies in apparent magnitude from a high of 2.70 down to 2.85.[17] Pi Puppis is the brightest star in the open cluster Collinder 135.[18]

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