A Sparkly Cluster of Stars Is Younger than It First Looks

The entire universe in blog form
Jan. 31 2013 12:26 PM

A Sparkling Imposter

Hubble picture of the star cluster NGC 411
Hubble photo of the odd but beautiful star cluster NGC 411. Click to embiggen.

Image credit: ESA/Hubble & NASA

I love star clusters. They’re crucial to our understanding of the way stars form, live, and die—stars change as they age, making it hard to compare one to another if they are vastly different ages. But the stars in a cluster are all born at the same time, so that makes it a lot easier to understand their behavior. It’s like having them in a lab for study.

Phil Plait Phil Plait

Phil Plait writes Slate’s Bad Astronomy blog and is an astronomer, public speaker, science evangelizer, and author of Death From the Skies!  

There are two kinds of clusters: globular clusters (old, roughly spherical, and densely packed), and open clusters (younger, shapeless, and with stars scattered throughout). I’ve seen both kinds many, many times in photos as well as with my own eyes; they’re a favorite target of mine when I’m using a small telescope.


Which is why this Hubble picture of NGC 411 really threw me for a moment. What kind of cluster is it?

I thought it was a globular for a moment. The shape is about right, if a little diffuse. But then I noticed all the blue stars. This image is a combination of ultraviolet (shown as blue), visible light (green), and infrared (red). All the globular clusters we know are old, as old as the galaxy itself, about 10-12 billion years. Blue stars are hot, massive, and young: They explode as supernovae after only a few million years. Globular clusters had lots of blue stars when they were young, eons ago, but those stars are long gone. All that remains are yellow, orange, and red stars (though there are exceptions).

The globular star cluster 47 Tucanae
The globular cluster 47 Tuc is a fantastic example of these old, dense beehives of stars. Click to apiarenate.

Image credit:ESO/M.-R. Cioni/VISTA Magellanic Cloud survey

NGC 411 has far too many blue stars to be a globular. So it’s an open cluster. In fact, its age can be determined by looking at the colors of the stars in it—bluer stars are more massive and blow up sooner, so by looking at the bluest stars in it, an upper limit to the age can be found. In practice it’s way harder than this, but studies show NGC 411 is about 1.5 billion years old. That’s far too young to be a globular, though fairly old for an open cluster.

Then I got my second surprise: NGC 411 isn’t even in our galaxy. It’s in the Small Magellanic Cloud, a dwarf companion galaxy to the Milky Way. That puts it at a distance of about 200,000 light years, far, far more distant than the clusters I peruse with my own ‘scope.

And there’s one more thing to notice. In the higher-resolution images (here’s the 3700 x 2750 pixel version) you can see several small galaxies dotting the sky in the background. Those galaxies are probably hundreds of millions or even billion of light years distant, thousands of times farther away than NGC 411. So think about that: In this picture you can see right through the cluster of stars, and right through its parent galaxy into truly deep space. You’re seeing those galaxies as they were before dinosaurs walked the Earth, some even before life arose out of our planet’s oceans.

Some objects like NGC 411 might be good at being deceptive about their ages, but whole galaxies? Not so much. The Universe has been around a long, long time. But I have to say: It looks pretty good for its age.



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