Why Galactic Nuclei Erupt

Astronomers know that when galaxies’ nuclei become active–releasing tremendous floods of energy–supermassive black holes are the ultimate culprit.

We also know that supermassive black holes lurk at the hearts of most large galaxies.

But most galaxies are not active; only a small percentage are. Our home galaxy is host to a supermassive black hole, but it’s not active. Neither is the black hole within the nucleus of our nearest galactic neighbor, Andromeda.

So, what makes a supermassive black hole erupt?

Continue reading

Exploring Radio Lobes

Meet galaxy NGC 5128, also known as Centaurus A.

Anyone notice something weird going on here?

If you’ve been following my recent posts on galaxies, you might notice that this does not look like a typical galaxy. It has a clear dust band, so it can’t be an elliptical; elliptical galaxies have no obvious dust or gas. But it doesn’t look much like a spiral, either: it has a bright, spherical cloud of stars you’d more expect from an elliptical!

And it’s definitely not an irregular galaxy. It definitely has a disk shape, and irregulars are not disk galaxies.

So what the heck is going on with this galaxy?

Continue reading