Zeta Puppis

StarDate: April 3, 2013

You are missing some Flash content that should appear here! Perhaps your browser cannot display it, or maybe it did not initialize correctly.

You are missing some Flash content that should appear here! Perhaps your browser cannot display it, or maybe it did not initialize correctly.



The brightest star of the constellation Puppis, which represents the stern of the ship Argo, is one in a million - or one in several million, to be more precise. It’s a member of the hottest and most massive class of stars, known in astronomical parlance as Class O. These stars are the rarest class of all, with perhaps only a few thousand of them in the entire galaxy.

Zeta Puppis is low in the south as night falls this evening. It’s well to the lower left of Sirius, the brightest star in the night sky.

Zeta Pup looks only a fraction as bright as Sirius, but that’s only because of their distances. Sirius is less than nine light-years away, while Zeta Pup is more than a hundred times farther. If you put the two stars side by side, Zeta Puppis would shine thousands of times brighter than Sirius.

Class O stars are the most massive main-sequence stars in the galaxy - those that are in the prime of life. They’re many times heavier than the Sun. Such stars are squeezed more tightly by gravity, heating their cores to billions of degrees. That also heats their surfaces, making them much hotter and bluer than the Sun.

The heat in an O star’s core cranks up the rate of nuclear reactions. So even though Zeta Pup is more massive than the Sun, it’ll live a much shorter life - tens of millions of years, versus 10 billion years for the Sun. And at the end, it’s likely to blow itself to bits as a supernova - a brilliant demise for a brilliant star.

 

Script by Damond Benningfield, Copyright 2013

For more skywatching tips, astronomy news, and much more, read StarDate magazine.

The one constant in the Universe: StarDate magazine

FacebookTwitterYouTube

©2014 The University of Texas McDonald Observatory