Pi Puppis

for Pi Puppis, plotted from Hipparcos data, folded with the period derived by Koen and Eyer (2002) The spectrum of Pi Puppis matches a stellar classification of K3 Ib. 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 , which gives it the orange hue of a K-type star. With a mass 11.7 times that of the Sun, this is a short-lived star with an estimated age of 20 million years. It is a semiregular variable star that varies in apparent magnitude from a high of 2.70 down to 2.85. Pi Puppis is the brightest star in the open cluster Collinder 135. ==Nomenclature==

This star does not seem to have had a traditional proper name, but some 21st-century sources use the name Ahadi, which is derived from Arabic for "having much promise". This name appears in the SIMBAD database and at least one academic paper. In Chinese, (), meaning Bow and Arrow, refers to an asterism consisting of π Puppis, δ Canis Majoris, η Canis Majoris, HD 63032, HD 65456, ο Puppis, k Puppis, ε Canis Majoris and κ Canis Majoris. Consequently, π Puppis itself is known as (, ). ==Observation==

Pi Puppis is a semiregular variable star with an apparent magnitude of 2.733. It appears slightly orange in color with a B-V color index of +1.608, similar to that of the famous Mira. It is typically the second brightest star in Puppis, only behind the blue supergiant Naos, and the brightest star in the open cluster Collinder 135. About every five years, the Pi Puppids, a meteor shower associated with the comet 26P/Grigg–Skjellerup, appears near the star in late April. The Pi Puppids are a variable meteor shower, with varying maximums each year. ==References==