PU Puppis

PU Puppis
Location of PU Puppis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 38m 18.04541s
Declination −25° 21 53.3017
Apparent magnitude (V) 4.69
Characteristics
Spectral type B8III
U−B color index −0.35
B−V color index −0.11
Variable type β Lyr
Astrometry
Radial velocity (Rv)+41.00 km/s
Proper motion (μ) RA: −3.03 mas/yr
Dec.: −7.42 mas/yr
Parallax (π)5.27±0.26 mas
Distance620 ± 30 ly
(190 ± 9 pc)
Absolute magnitude (MV)−1.80±0.25
(−1.77 + 5.85)
Absolute bolometric
magnitude
 (Mbol)
−2.35 + 5.54
Orbit
Period (P)2.58237±0.00005 d
Semi-major axis (a)13.30 ± 0.40 R
Inclination (i)56.2°
Details
PU Pup A
Mass4.10±0.20 M
Radius6.60±0.30 R
Luminosity695±80 L
Surface gravity (log g)3.40±0.05 cgs
Temperature11,500±500 K
Rotational velocity (v sin i)123 km/s
PU Pup B
Mass0.65±0.05 M
Radius0.90±0.10 R
Luminosity0.50±0.10 L
Surface gravity (log g)4.30±0.10 cgs
Temperature5,000±350 K
Other designations
m Puppis, PU Pup, CD−25°4828, CCDM J07383-2522AB, GC 10266, HIP 37173, HR 2944, HD 61429, SAO 174175, WDS J07383-2522AB
Database references
SIMBADdata

PU Puppis (PU Pup) is a class B8III (blue giant) star in the constellation Puppis. Its apparent magnitude is 4.69 and it is approximately 620 light years away based on parallax.

It is a β Lyrae variable, ranging from 4.75 to 4.69 magnitude with a period of 2.58 days. The secondary is estimated at 5.6 magnitude, although recent observations have failed to confirm it. The primary has a mass of 4.10 solar masses, and is radiating at an effective temperature of 11,500 K. The secondary, with a mass 65% that of the Sun, has a surface temperature of about 5,000 K.