The Anatomy of Galaxies
Following on from my post about the Hubble diagram, I thought I’d mention a bit about the main types of galaxies that are out there. Galaxies come in three basic types: spirals, ellipticals and irregulars. Each of these three broad morphologies of galaxy tells us a little about what is going on inside the galaxy itself. They are all structured differently.
The spiral arms of a galaxy contain most of the interstellar medium – dust and other material between stars – within a galaxy. It is in the spiral arms that new stars are forming, hence their usually bright, blueish or white colour. Spirals are made of about 10-20% dust and gas. This is the source material for the stars that are forming within the spiral arms. It is the dust that obscures background light to create the dark lanes you see in spiral galaxies. You can the arms and the dust lanes very well in this artistic impression of our own galaxy, the Milky Way from Nick Risinger / NASA.
The central bulge of spiral galaxy contains older, redder stars and often also contains a invisible, massive black hole. Some, but by no means all, central bulges have the appearance of a mini elliptical galaxy.
The central bulge and spiral arms vary greatly in appearance from galaxy-to-galaxy. But of course, you know this from working on Galaxy Zoo!
Spiral galaxies are also made up of a third component: the galactic halo. This is an almost spherical fuzz of stars and globular clusters surrounding the galaxy, trapped by gravity. You can see the halo quite well in the above image of the Sombrero Galaxy, which is a spiral seen almost edge-on. This image is from Hubble Heritage
Elliptical galaxies are essentially all bulge and nothing else! In an elliptical galaxy the stars tend to be older and there is less gas and dust around. The stars orbit around the centre of mass of the galaxy in a more random way – their orbits are not constrained to a disk shape. There is very little star formation going on in elliptical galaxies and so they usually appear reddish in colour: dominated by older, cooler stars.
There is obviously little to say about the structure of irregular galaxies because they are irregular. They make up about a quarter of all galaxies. It is thought that many irregulars were once ellipticals or spirals and have been distorted by interactions or collisions with other galaxies. Irregular galaxies can have very high star formation rates and can contain a lot of dust and gas – often more than spiral galaxies.
Galaxy Zoo: Hubble has a whole new branch of questions to try and help classify these clumpy galaxies.
You could add this fourth category to the list of galaxy types. Dwarf galaxies might appear to be just smaller versions of the above types, but they are the most common type of galaxy. There are more dwarfs than any of the others, if you just count them up.
The Large and Small Magellanic Clouds – the LMC and SMC, which are visible in the Southern Hemisphere – are actually two small galaxies, orbiting around our own larger Milky Way. The image below, from Mr. Eclipse, shows both of these objects. The LMC is an irregular galaxy and the SMC is a dwarf.
We’ll continue talking about the different types of galaxies – and how they all fit together – in the next post in this series. In the meantime might I suggest yet another type of galaxy, perhaps with a coffee and a bit of classification?
Thank you very much, Robert for this informative blog. Looking forward to its sequels.
JKHC ( 10/6/10 )
Really interesting and informative. I’m just getting started with Galaxy Zoo and am loving the experience so far. Thanks for the info!
Thanks for this. As a layman in astronomy this has been really informative and has helped me gain a better understanding of what I am looking at when I am classifying galaxies. Looking forward to future articles.
Very good and useful info. I was baffled by those clumpy galaxies that didn’t even look like galaxies, thanks to your article, now I know what they are.
Doesn’t the middle irregular galaxy look kinda like a spiral?
In this article, you talked about dwarf galaxies. It said that they are the most common, just smaller and more like clouds. If they are the most common then why aren’t they on the list of types of galaxies?
I was curious if you could inform me on the formation of the galaxies. What causes the galaxies to form in the shape? What factors contribute to this formation? Why do they form into a spiral, elliptical, or irregular galaxy?
Why does the irrelgular galaxy contain more dust and gas?
This was very insightful and informative, it was awesome especially the part where you talked about the galaxy. what is the estimated length of a spiral arm?
Robert, we are befuddled by these magnificent galaxies. However we have but one inquiry for you, how do you know how old all of these galaxies are?
When you were talking about elliptical galaxy, you said it was essentially all bulge.. What is a bulge??
What determines how much interstellar medium there is in a galaxy?