PU Puppis (PU Pup) is a class B8III (blue giant) star in the constellation Puppis. Its apparent magnitude is about 4.7 and it is approximately 620 light years away based on parallax.
It is a β Lyrae variable, ranging from 4.69 to 4.75 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.
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![PU Puppis: A light curve for PU Puppis, plotted from TESS data[9]](https://upload.wikimedia.org/wikipedia/commons/thumb/e/ed/PUPupLightCurve.png/1280px-PUPupLightCurve.png?utm_source=en.wikipedia.org&utm_campaign=parser&utm_content=thumbnail)
