Faint But Steady

StarDate: July 5, 2012

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.



61 Cygni is one of our closest stellar neighbors — just 11 light-years away. And it consists of two stars, not one.

Even so, it’s only barely visible to the unaided eye — a faint dot not far from the graceful outline of Cygnus, the swan. That’s because its two stars are only about half as massive as the Sun. But what the stars lack in flash, they’ll make up for in longevity — both will live much longer lives than the Sun.

In fact, not a single star of that class has had time to die from old age.

A star’s lifespan is determined by its mass. Heavier stars have more hydrogen to power their nuclear reactions, so you might expect them to live longer. But that’s just not the case. A massive star’s gravity is much stronger, so it squeezes the star’s core more tightly, making it much hotter. That revs up its nuclear reactions, so the star burns through its hydrogen fuel in a hurry. In fact, the heaviest stars live only a few million years.

Lightweight stars aren’t squeezed as tightly, so they consume their fuel at a more leisurely pace. A star the mass of the Sun will “burn” its hydrogen for about 10 billion years. And a star that’s less than about three-quarters of the Sun’s mass will live several billion years longer. Since the universe is only 13.7 billion years old, that means that not a single one of these stars has had time to burn out on its own. Only interactions with other stars could snuff out such feeble cosmic lights.

 

Script by Damond Benningfield, Copyright 2012

 

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